Defensive and Sensory Chemical Ecology of Brown Algae
CHARLES D. AMSLER AND VICTORIA A. FAIRHEAD
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Defensive and Sensory Chemical Ecology of Brown Algae
CHARLES D. AMSLER AND VICTORIA A. FAIRHEAD
Department of Biology, The University of Alabama at Birmingham, Birmingham, Alabama 35294‐1170
I. Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . II. Phlorotannins . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. Chemical Structure and Synthesis . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Comparison of Quantification Methods . . . . . . . . . . . . . . . . . . . . . . . . . . . C. Cellular Roles . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . D. Putative Ecological Roles . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . E. Spatial and Intra/Interspecific Variability . . . . . . . . . . . . . . . . . . . . . . . . . F. Rates and Cost of Production . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . G. Current Uncertainty and Future Directions . . . . . . . . . . . . . . . . . . . . . . . III. Nonphlorotannin Antiherbivore Defences . . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. Dictyotales . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Desmarestiales . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . C. Other Orders . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . D. Activated Defences . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . IV. Testing Chemical Defence Theories with Brown Algae. . . . . . . . . . . . . . . . . A. Optimal Defence Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Induced Defence Model. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . C. Carbon‐Nutrient Balance and Resource Allocation . . . . . . . . . . . . . . . . D. Tests of Multiple and Other Theories . . . . . . . . . . . . . . . . . . . . . . . . . . . . . V. Nonphlorotannin Defences Against Bacteria, Fouling Organisms, and Pathogens. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . VI. Volatile Halogenated Organic Compounds . . . . . . . . . . . . . . . . . . . . . . . . . . . . VII. Sensory Chemical Ecology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. Chemoattraction to Pheromones . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Behaviour and Sensory Capabilities of Spores . . . . . . . . . . . . . . . . . . . . . Advances in Botanical Research, Vol. 43 Incorporating Advances in Plant Pathology Copyright 2006, Elsevier Ltd. All rights reserved.
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0065-2296/06 $35.00 DOI: 10.1016/S0065-2296(05)43001-3
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VIII. Concluding Remarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
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ABSTRACT The ecological interactions of brown algae are important as these macroalgae are common and often keystone members in many benthic marine communities. This review highlights their chemical interactions, particularly with potential herbivores, but also with fouling organisms, with potential pathogens, with each other as gametes, and with their microenvironments when they are spores. Phlorotannins, which are phenolic compounds unique to brown algae, have been studied heavily in many of these respects and are highlighted here. This includes recent controversy about their roles as defences against herbivory, as well as new understanding of their roles in primary cellular functions that may, in many instances, be more important than, and which at least have to be considered in concert with, any possible ecological functions. Brown algae have also been useful models for testing theories about the evolution of and ecological constraints on chemical defence. Furthermore, their microscopic motile gametes and spores have the ability to react to their chemical environments behaviourally.
I. INTRODUCTION Chemical ecology can be described as the study of chemically mediated interactions between organisms or between organisms and their environment, and most such interactions can be grouped into three broad categories. One category is chemical communication between organisms, such as brown algal male gamete attraction to pheromones, which is discussed in Section VII.A. A second is organisms sensing and responding to their chemical environments, and in brown algae this is observed in spores, which are able to sense and respond behaviourally to nutrients as described in Section VII.B. However, most studies of the chemical ecology of brown algae fall into the third category, which is chemical defence. Defences can be mounted against predators, pathogens, biofoulers, or competitors. A majority of the research on chemical defences in brown algae to date, and consequently a majority of this review is focused on defences against predators, but we also discuss defences against pathogens and biofoulers in Sections II. D.3 and V. Outside of speculation about potential allelopathic roles of pheromones, as discussed briefly in Section VII.A, we are aware of little work on brown algae examining chemical interactions between competitors, although the report of Ra˚ berg et al. (2005) is a fascinating recent example. The chemicals mediating defensive interactions are usually secondary metabolites (also called natural products) so termed to distinguish them from
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metabolites with primary metabolic roles within the cells of many taxa. However, as discussed in Section II, brown algal phlorotannins are an important exception to this as they have important primary roles in addition to ‘‘secondary’’ functions as chemical defences. Brown algae have been included in numerous recent reviews that have covered various aspects of algal chemical ecology (Amsler, 2001; Amsler and Iken, 2001; Arnold and Targett, 2002; Cronin, 2001; La Barre et al., 2004; Paul and Puglisi, 2004; Paul et al., 2001; Pohnert, 2004; Pohnert and Boland, 2002; Potin et al., 2002; Steinberg and de Nys, 2002; Steinberg et al., 2001, 2002; Targett and Arnold, 2001; Van Alstyne et al., 2001a). Here we have attempted to take a comprehensive approach in reviewing the current state of brown algal chemical ecology, and we believe that this focus on the group is warranted. Brown algae, which comprise the Class Phaeophyceae, are unique in being very far removed phylogenetically from all other eukaryotic macrophytes (i.e., red macroalgae, green macroalgae, bryophytes, and vascular plants, which clade together in modern phylogenetic trees) with the notable exception of the endosymbiotically derived red lineage chloroplasts of brown algae and their heterokont relatives (Baldauf, 2003; Falkowski et al., 2004; Keeling, 2004). A great deal of the conceptual framework of defensive chemical ecology is based on studies of vascular plants (cf. Section IV), and this phylogenetic distinctiveness of the Phaeophyceae makes them ideal tools to test and extend such ideas in trophically analogous but phylogenetically distinct organisms. Brown algae are also very important members of many marine communities ranging from the tropics to near the poles (Lobban and Harrison, 1994) and often dominate these communities in terms of structure and biomass, particularly in temperate and polar waters (e.g., Dayton, 1985a,b, 1990; Schiel and Foster, 1986; Wiencke and Clayton, 2002). Brown algae do occasionally occur in freshwater (Graham and Wilcox, 2000), but we are aware of no studies of their chemical ecology in freshwater systems. Consequently this review focuses entirely on marine and estuarine environments. With respect to defences against predation, we include only chemical forms of defence even though brown algae can also deter herbivory via morphological or otherwise physical mechanisms (e.g., Lewis et al., 1987; Lowell et al., 1991) or via life history adaptations that expose relatively palatable stages to herbivores over a minimal period of time (Lubchenco and Cubit, 1980). Because of the length of this review, we presume that many readers will consult only some parts at any given time and, consequently, we have chosen to include redundancy in two forms in the text. There are a number of published studies that are referred to, but in diVerent contexts, and often
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with diVerent emphasis, both in Section II on phlorotannins and in Section IV on tests of chemical defence theories. Also, particularly because this review is focused on brown algae as a specific taxonomic group, we feel that it is important throughout to be explicit about the ordinal‐level taxonomic relationships between the species discussed. Both similarities and diVerences in the chemical ecology of diVerent brown algal species, as described later, should be considered within a phylogenetic context. To provide such context, we have attempted to exhaustively identify the ordinal‐level classification of each species every time it is discussed, although sometimes using terms such as ‘‘kelp’’ for members of the Laminariales, ‘‘fucoid’’ for members of the Fucales, or ‘‘dictyotalean’’ for members of the Dictyotales. It is hoped that a reader of the entire review or of multiple parts thereof will understand the reasons for this redundancy.
II. PHLOROTANNINS Phlorotannins are polyphenolic polar metabolites with both primary and secondary roles. They occur only in the Phaeophyceae and account for over 10% dry weight in many species or up to 20% in others (Ragan and Glombitza, 1986). Their roles and functions have been the subject of many studies over the last few decades, particularly those roles that relate to antiherbivory and antifouling. Recent reviews have covered several aspects of our current knowledge in relation to phlorotannins and this work will not specifically focus on these areas, but it will still briefly address important areas such as chemical structure and roles at the cellular level. The comprehensive review by Ragan and Glombitza (1986) covered work up to that time, and recent reviews have concentrated on more specific aspects, such as the mediating role phlorotannins play in the interaction between algae and herbivores (Targett and Arnold, 1998, 2001) and on the putative roles of phlorotannins at the cellular level (Schoenwaelder, 2002). Arnold and Targett (2002) provide an overview of marine tannins in general, reviewing work on both vascular and nonvascular taxa, and Paul and Puglisi (2004) include a discussion of phlorotannins in their wide‐ranging review of chemical interactions between marine organisms. A. CHEMICAL STRUCTURE AND SYNTHESIS
1. Structure Phlorotannins are polymers of phloroglucinol (1,3,5‐trihydroxybenzene; Fig. 1) and are classified into six groups on the basis of the chemical structure of the polymer (fucols, phlorethols, fucophlorethols, fuhalols,
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Fig. 1. Chemical structures of phloroglucinol and subunits of the six diVerent structural classes of phlorotannins.
isofuhalos, and eckols; Fig. 1) (Ragan and Glombitza, 1986). They have several properties in common with some vascular plant tannins, although they remain chemically quite diVerent. Properties in common with the condensed tannins of vascular plants include the ability to bind to metal ions and to precipitate protein and carbohydrate from solution (Ragan and
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Glombitza, 1986). The molecular masses of phlorotannins vary between 126 Da and 650 kDa (Targett and Arnold, 2001), but are found most commonly in the 10 to 100 kDa range (Boettcher and Targett, 1993). 2. Location in the cell: soluble and cell wall bound forms The highest concentration of phlorotannins in the cell is found in physodes, which are membrane‐bound vesicles appearing as light‐refractive bodies in the cytoplasm (for reviews, see Ragan and Glombitza, 1986; Schoenwaelder, 2002). Phlorotannins in this form are soluble (Ragan and Glombitza, 1986). Physodes may occur in most tissues of the thallus but commonly occur in the outermost layers (Ragan and Glombitza, 1986; Tugwell and Branch, 1989). Lu¨ der and Clayton (2004) suggest that as much as 90% of the total phlorotannin content of Ecklonia radiata (Order Laminariales) can be found in the epidermal layer. Shibata et al. (2004) reported that the phlorotannin distribution in tissues of three other Ecklonia spp. is similarly concentrated in epidermal layers. Phlorotannins are also found as a constituent of cell walls (Schoenwaelder and Clayton, 1999a), where they are incorporated after release from the physodes (see Section II.C.1). Physodes are able to move to areas of active cell wall formation via interactions with the cytoskeleton (Schoenwaelder and Clayton, 1999b). The cell wall bound phlorotannins are thought to occur in levels an order of magnitude lower than levels of soluble phlorotannins in the cell (Koivikko et al., 2005). 3. Synthesis and metabolic turnover Phlorotannins are generally thought to be synthesised via the acetate–malonate pathway (Herbert, 1989) in a process that may involve a polyketide synthase (PKS) type enzyme complex (Arnold and Targett, 2002). However, Chen et al. (1997) have proposed an alternative hypothesis that they are produced by the shikimic acid pathway, in a manner analogous to vascular plant tannins. Identification of the phlorotannin synthetic pathway is an important goal for future research. This is particularly so if it leads to methodologies to monitor phlorotannin synthesis at the genetic or enzymatic levels, which could potentially help resolve some of the uncertainties in studies of phlorotannins as described later. Arnold and Targett (1998) developed a method using stable isotope (13C) techniques to determine rates of phlorotannin synthesis. In Lobophora variegata (Order Dictyotales) and in Sargassum pteropleuron and Fucus distichus (Order Fucales), phlorotannin synthesis costs represented 1 % of total assimilated carbon when calculated over a range of carbon assimilation rates. Arnold and Targett (1998) emphasised that these investment rates do not include other costs, such as maintaining the metabolic pathways and
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storage structures, which may diVer between species and for diVerent metabolites. They also investigated polymerisation (‘‘aging’’) in Sargassum pteropleuron, observing that 30 kDa polymers formed rapidly in a 5‐h period following the labelling incubation, and that this size class was gradually replaced with 30 kDa polymers from that time on. In a later study these authors used the same methods in field and laboratory experiments that provided evidence for relatively high rates of metabolic turnover in two tropical species (L. variegata and Sargassum hystrix var buxifolium), although the rate for L. variegata (2 days for complete turnover) was considered to be related to exudation under the stressful experimental conditions (Arnold and Targett, 2000). The turnover rate for S. hystrix var. buxifolium was slower at 17 days for a complete removal of 13C from the measurable phlorotannin pool, which was recorded in field experiments considered to involve very low rates of exudation. B. COMPARISON OF QUANTIFICATION METHODS
Several methods provide measures of phlorotannins, either by quantifying the total level of polyphenolics or by specifically measuring levels of tannins (for reviews, see Ragan and Glombitza, 1986; Targett and Arnold, 1998). The chemical behaviour of phlorotannins (as reactive, large, structurally similar, polar metabolites) has led to colorimetric methods becoming accepted as the preferred technique to eVectively quantify the levels of soluble, physode‐bound phlorotannins (Ragan and Glombitza, 1986; Targett and Arnold, 1998). These colorimetric methods, of which there are several, measure the total level of phenolics in the sample, which does not allow diVerentiation of size classes (Stern et al., 1996b), considered an important factor in determining the bioactivity of phlorotannins (see Section II.D.2). Results gained from each procedure will be variously aVected by the exact chemical structure of the phlorotannins in the sample (including size and bond types) and by the choice of reference compound (Ragan and Glombitza, 1986; Stern et al., 1996b; Van Alstyne, 1995). The proliferation of methods means it is sometimes diYcult to make comparisons between studies, but as each method has its advantages in particular instances, it is hard to advocate a single preferred method, and relative comparisons within studies (when results are gained using the same procedure) are still valid. The strong hydrogen‐bonding capacity of phlorotannins means they can be eVectively removed from a sample by treatment with the resin polyvinylpolypyrrolidone (PVPP) (reviewed by Toth and Pavia, 2001). This allows quantification methods to be assessed (e.g., Targett et al., 1995) or to be modified by including PVPP‐treated samples (e.g., Cronin and Hay, 1996a; Peckol
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et al., 1996; Yates and Peckol, 1993) and is useful for creating appropriate controls in experimental design (e.g., Wilkstro¨ m and Pavia, 2004). Extraction of phlorotannins prior to quantification is problematic no matter what assay is preferred. Polyphenolics are prone to oxidation and thus an inert atmosphere and dark, cold conditions are required for any procedure. The ability to oxidise rapidly, in combination with their tendency to precipitate proteins, is likely to result in underestimates of concentrations unless these factors are controlled for (Ragan and Glombitza, 1986). Extraction of phenolics is normally by aqueous alcohol (usually methanol) or aqueous acetone (Ragan and Glombitza, 1986), which minimises extraction of nonphenolic substances (e.g., proteins) that may be inadvertently measured in the quantification assay (Van Alstyne, 1995). Koivikko et al. (2005) compared the eYciency of various solvents for extracting phlorotannins from Fucus vesiculosus, indicating that 70% aqueous acetone was the most eYcient in that case. 1. Folin–Denis A modification of the Folin–Denis procedure (Folin and Denis, 1915) is perhaps the most widely used method of quantifying phlorotannins. During the Folin–Denis assay, polyphenolics are oxidised in reactions linked to the production of stable blue‐coloured molecules (via the reduction of phosphomolybdic and phosphotungstic acids), which allows measurement through spectrophotometry and quantification using a commercially available standard (Ragan and Glombitza, 1986). Although several compounds are known to interfere with the reactions (Ragan and Glombitza, 1986) and the reagent is also reactive with certain nonpolyphenolic compounds, these factors are not considered to aVect results beyond normal error limits (Targett and Arnold, 1998; Targett et al., 1995; but see Appel et al., 2001). 2. Folin–Ciocalteu The Folin–Ciocalteu assay, using a modified reagent (Folin and Ciocalteu, 1927; Waterman and Mole, 1994), represents an improvement of the Folin– Denis assay by reducing levels of precipitates (Van Alstyne, 1995), which allows use with small sample volumes (Stern et al., 1996b). In common with the Folin–Denis assay, the reagent is reactive with compounds other than phenolics, but this represents only a small percentage of the overall measurement (Van Alstyne, 1995). 3. 2,4‐Dimethyloxybenzaldehyde The DMBA assay, another colorimetric assay, depends on the ability of 2,4‐ dimethyloxybenzaldehyde (DMBA) to react specifically with phlorotannins (1,3‐ and 1,3,5‐substituted phenols), but not other phenolics, producing a
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pink‐coloured chromophore (Stern et al., 1996b). This assay has the disadvantage of requiring a standard to be produced for each species (by purification of phlorotannins from it or a very closely related species) in contrast to those aforementioned assays that utilise commercially available phloroglucinol. This is due to the larger variability in reactivity depending on the specific nature of the phlorotannins (Stern et al., 1996b). However, the DMBA assay is less sensitive to interferences from nonphenolic substances (Stern et al., 1996b), and once a standard has been prepared, the simplicity of the assay procedure allows more easily for a sample design with much larger numbers of samples (as long as the samples come from the same, or closely related, species). 4. Cell wall bound Koivikko et al. (2005) published a method for measuring cell wall bound phlorotannins. The method was adapted from vascular plant studies and involves alkaline degradation of the bonds between phenolics and alginic acid in the cell walls. C. CELLULAR ROLES
1. Cell wall structure Phlorotannins have recently been confirmed as being an important component of the brown algal cell wall (Schoenwaelder and Clayton, 1999a) and as being vital for the process of cytokinesis (for a review, see Schoenwaelder, 2002). In zygotes of Acrocarpia paniculata and Hormosira bankisii (Order Fucales), phlorotannins are secreted into cell walls following the fusion and breakup of physode membranes (Schoenwaelder and Clayton, 1998a,b) where they are then thought to complex with alginic acid (Schoenwaelder and Clayton, 1999a). Investigations in the same species also revealed that prior to cell division the physodes form a distinct line across the centre of cell, which occurs before any other cell wall constituents accumulate (Schoenwaelder and Clayton, 1998b). 2. Adhesion to the substrate A secretion of phenolics coincides with the adhesion of zygotes in Acrocarpia paniculata and Fucus gardneri (Order Fucales) where secretion is localised at the point of adhesion (Schoenwaelder and Clayton, 1998a; Vreeland et al., 1998). Secretion of polyphenolics also occurs after fertilisation in Durvillaea potatorum (Order Durvillales; Clayton and Ashburner, 1994). Adhesion of these newly formed zygotes is thought to be via an extracellular glue composed, in part, by phenolics (Vreeland et al., 1998; reviewed in Schoenwaelder, 2002).
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3. Spermatozoid inhibitors During the period in which newly fertilised zygotes remain unprotected from polyspermy (which is potentially deadly), secreted phlorotannins are thought to protect the zygote by impairing sperm motility (Schoenwaelder and Clayton, 1998a; reviewed in Schoenwaelder, 2002). 4. Wound healing That phlorotannins play a role in wound healing has been recognised for over three decades (Fagerberg and Dawes, 1976; Fulcher and McCully, 1971), and recent work has further clarified this role (Lu¨der and Clayton, 2004). Lu¨ der and Clayton (2004) created small wounds with a cork borer in sections of Ecklonia radiata (Order Laminariales) and then followed the healing process for 9 days using microscopy techniques (light, fluorescence, and transmission electron). They found clear evidence of an accumulation of phlorotannins around wound sites, which was evident 1 day after wounding. This became prominent in the nearby medulla after only 3 days and by 9 days dense accumulations were found throughout the medulla of the entire algal section. They observed that new medullary cells produced at the wound site were structurally diVerent and contained several physodes, which increased in number and size over the next few days. Cortical cells were also observed to accumulate physodes. By day 5 the wound surface was composed entirely of cells dense with physodes, which diVerentiated into epidermal cells that remained rich in physodes. They concluded that phlorotannins function in both wound‐sealing (which is consistent with the clotting proposal of Fagerberg and Dawes, 1976) and structural wound‐healing roles (consistent with their role in cell wall formation; see Section II.C.1). In addition, the general accumulation of phlorotannins throughout the medulla was considered to be an antiherbivore response (see Section II.D.1), which may reduce infection (see Section II.D.3). D. PUTATIVE ECOLOGICAL ROLES
1. Antiherbivory: evidence for and against deterrence A multitude of studies have focused on the role of phlorotannins in herbivore defence. These studies have generally utilised feeding experiments that give herbivores the choice between tissues with diVerent phlorotannin contents and artificial foods containing algal extracts or pure compounds, with only the latter method being a test of phlorotannin bioactivity. The concentration and dose of phlorotannins in the oVered food influence greatly the outcome of the algal–herbivore interaction (Pereira and Yoneshigue‐ Valentin, 1999; Targett and Arnold, 1998; Van Alstyne et al., 1999c), and the
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type and nutritional quality of the bioassay food may also be important (Deal et al., 2003; Kubanek et al., 2004). A positive deterrent eVect has not been found consistently and seems to be highly dependent not only on the selection of algae but also on the herbivore species. Even when the same herbivore species is used, the interactions mediated by phlorotannins do not always yield the same results. The numerous studies conducted using Fucus vesiculosus (Order Fucales) demonstrate these points. The gastropod Littorina littorea preferred to graze on F. vesiculosus with a lower phenolic content when oVered the choice between this and higher phenolic content foods (Geiselman and McConnell, 1981; Yates and Peckol, 1993). In contrast, Jormalainen et al. (2004) found a preference of Idotea baltica for phlorotannin (extracted from F. vesiculosus) containing food, an eVect that increased with higher concentrations (10% compared to 5%), which they suggest to be related to host recognition. Also, Hemmi et al. (2004) established that while the I. baltica preferred damaged F. vesiculosus for at least 10 days after clipping, this was not associated with diVerences in phlorotannin levels, as clipping did not induce the production of phlorotannins. Furthermore, crude polar extracts from F. vesiculosus deterred feeding by sea urchins (Arbacia punctulata), but bioassay‐guided fractionation of this extract revealed that deterrence was not due to phlorotannins (Deal et al., 2003). Feeding assays showed that even at concentrations 400% of the natural level (1% dwt), isolated phlorotannins were not an eVective deterrent to feeding by A. punctulata (Deal et al., 2003). Kubanek et al. (2004) also used bioassay‐guided fractionation techniques and found that the deterrent eVect of crude F. vesiculosus extracts was due to defensive compounds other than phlorotannins, but they were not able to isolate the bioactive compounds and did not detect the galactolipid reported by Deal et al. (2003). They tested the eVect of purified phlorotannins (at 3, 6, and 12 natural yield) on the feeding of amphipods (Ampithoe longimana) and sea urchins (A. punctilata), which normally avoid F. vesiculosus, and found no deterrent eVects. The amphipod Ampithoe valida, which is commonly known to eat F. vesiculosus in the field, was deterred only at the 12 concentration (Kubanek et al., 2004). Investigations of other taxa have also produced mixed results. Within the Fucales, Van Alstyne (1988) found that snails (Littorina sitkana) moved away from areas of wounded Fucus gardneri (as F. distichus), which showed phlorotannin accumulation, and preferred to feed on undamaged algae with lower phlorotannin contents. The isopod Idotea granulosa preferred the high phlorotannin content tissue of Ascophyllum nodosum, which may have been due to the higher nitrogen content of that tissue (Pavia et al., 1997). Feeding by the snail Littorina obtusata on Ascophyllum nodosum tissue with a high
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phlorotannin content was decreased (Pavia and Toth, 2000a; Toth and Pavia, 2000b), but feeding by I. granulosa was not aVected by phlorotannin content (Pavia and Toth, 2000a). In a subsequent study the basal stipes of A. nodosum were found to have the highest phlorotannin contents and were consumed less by L. obtusata than other tissue types (Pavia et al., 2002). Phenolics extracted from Sargassum furcatum were deterrent at 2 and 5% of food content to amphipods (Parhyale hawaiensis), but the natural concentration (0.5%) did not deter feeding, consistent with the observed palatability of this species to P. hawaiensis (Pereira and Yoneshigue‐Valentin, 1999). In contrast (Cronin and Hay, 1996a) reported that feeding by amphipods was not influenced by the phlorotannin concentration of Sargassum filipendula. In members of the Laminariales (kelps), Johnson and Mann (1986) reported that the avoidance of the intercalary meristem region of Laminaria longicruris by grazing snails (Lacuna vincta) correlated with a high phenolic content. Abalone (Haliotis rufescens) preferred to feed on phenolic poor species, and phenolics extracted from Dictyoneurum californicum deterred feeding by 90% (Winter and Estes, 1992). However, Wakefield and Murray (1998) concluded that the feeding preferences of Norrisia norrisi (herbivorous snail) were determined more by factors such as habitat and refuge provision or toughness than by phlorotannin content. Feeding preference assays revealed that the snail consistently preferred the high phlorotannin content kelps over other algal species, although comparisons within the kelps did show the least preferred species (Egregia menziesii) was that with the highest phlorotannin content, but this was also the toughest kelp species. In a study of Zonaria angusta (Order Dictyotales), amphipods (Tethygeneia sp. and Hyale rubra) preferred to consume young tissue with a low density of physodes (Poore, 1994). The amphipods preferentially consumed the area directly behind the apical cell row, which has a low density of physodes, in preference to both the single layer of physode‐dense apical meristematic cells and older tissue with moderate densities of physodes (Figs. 2 and 3). A number of studies comparing palatability across orders have also been reported. Steinberg and van Altena (1992) found that some of the Australasian herbivores they tested were deterred from feeding by extracts from some algal species, but in general they found that Australasian marine herbivores were not deterred by phlorotannins. This contrasts to North American herbivores tested (e.g., Tegula funebralis and Tegula brunnea), which were strongly deterred by the presence of phlorotannins (Steinberg, 1984, 1985, 1988; Steinberg and van Altena, 1992). Steinberg et al. (1991) showed that the concentration of phlorotannins (from tropical and temperate species) in foods could not be related to feeding deterrence of tropical herbivorous fish. Also, the herbivorous fish Cebidichthys violaceus was
DEFENSIVE AND SENSORY CHEMICAL ECOLOGY OF BROWN ALGAE
13
Fig. 2. Apical region of Zonaria angustata branches: intact (left) and displaying damage from amphipod feeding (center and right). On the right is a branch in which the apical cell row has been breached by amphipods with the area behind it having been consumed. The center shows a branch in which the dangling apical cell row has broken away. From Poore (1994).
Fig. 3. Distribution of physodes in a longitudinal section of the apical tissues of Zonaria angustata. Physode distribution was compiled from photomicrographs. Physodes are visible as dark‐staining subcellular bodies with high densities in the apical meristem (left) and old growth (right) and in low densities adjacent to the meristem (center). From Poore (1994).
deterred from feeding by the presence of polar extracts of the fucoid Fucus gardneri in its diet, but not by polar extracts from the kelp Macrocystis integrifolia (Ireland and Horn, 1991). Van Alstyne et al. (2001b) examined the feeding preferences of four herbivores (sea urchins and snails) towards tissue that diVered in phlorotannin concentrations (juvenile and adult tissue from six members of the Laminariales and two members of the Fucales). Although they found much variation amongst species and life stages in terms of deterrence level, phlorotannins were apparently not responsible.
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The lack of a consistent feeding response to phlorotannins has led some authors to question whether they can be considered a defensive metabolite (Jormalainen and Honkanen, 2004; Jormalainen et al., 2003) and also highlights the complex role other metabolites play in defence, a fact that is often overlooked but which can confound experimental designs (Deal et al., 2003; Kubanek et al., 2004). 2. EVects on digestion and reproduction Studies of eVects of phlorotannins on the assimilation eYciencies of herbivores, as with those on feeding deterrence, have produced results that are often ambiguous. The specific structure of the phlorotannins occurring in an algal species, in combination with diVerences in the gut environment of herbivores, is thought to be partly responsible for this confusion (see review in Targett and Arnold, 2001). Several features of the gut are important in determining the activity of ingested phlorotannins (such as morphology, pH, enzyme composition, microbial activity) and these factors diVer widely among diVerent herbivores (Targett and Arnold, 2001). The acidity of the gut may be most important in fish, with basic guts correlated with higher assimilation eYciencies (Targett and Arnold, 2001). The presence of surfactants in herbivore gut fluid has also been shown to be involved in ameliorating the eVects of phlorotannins (Tugwell and Branch, 1992). Nevertheless, phlorotannins are considered to aVect food value via their ability to complex with proteins and other macromolecules in the gut, which can aVect assimilation eYciency (Stern et al., 1996a; see review in Targett and Arnold, 2001). Polar extracts (that should include most phlorotannins) of Fucus gardneri (Order Fucales), but not of Macrocystis integrifolia (Order Laminariales), significantly reduced the ability of the fish Cebidichthys violaceus to digest a palatable green alga (Ulva lobata), in particular reducing the assimilation eYciency of nitrogen (Ireland and Horn, 1991). Shell growth of abalone (Haliotis rufescens) was inhibited by the addition of polyphenolics from Dictyoneurum californicum (Order Laminariales) into its diet (Winter and Estes, 1992). In addition, the total carbon and nitrogen assimilations of the herbivorous isopod Idotea baltica decreased with increasing phlorotannin content in an artificial food diet, although as mentioned earlier this herbivore was not deterred from feeding by higher phlorotannin content (Jormalainen and Honkanen, 2004). However, Hemmi and Jormalainen (2004) reported that the body size of female I. baltica was significantly correlated with the phlorotannin content of Fucus vesiculosus (Order Fucales) in their habitat. Also, Toth et al. (2005) found that an increased level of phlorotannins in the diet of Littorina obtusata (fed on Ascophyllum nodosum, Order Fucales) did
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15
not have an eVect on growth rates, but did reduce significantly the number of viable eggs that the gastropod produced. A high dietary phlorotannin content did not aVect the assimilation eYciencies of three tropical herbivores (fish Sparisoma radians and Sparisoma chrysopterum, which have a basic gut environment, or the crab Mithrax sculptus) (Targett and Arnold, 2001; Targett et al., 1995). Similarly, the growth and conversion eYciencies of the Australasian herbivores Tripneustes gratilla (sea urchin) and Turbo undulata (snail) were not aVected by feeding on a diet high in phlorotannins for several months (Steinberg and van Altena, 1992). Also, a phlorotannin‐rich diet (containing 3 natural concentration of phlorotannins from F. vesiculosus) was correlated with enhanced growth and survivorship of the amphipod Ampithoe valida (Kubanek et al., 2004). In common with vascular plant tannins, molecular size is an important determinant of the eVects of phlorotannins on herbivores. Boettcher and Targett (1993) studied the eVect of diVerent molecular size fractions on the assimilation eYciency of the fish Xiphister mucosus (which has an acidic gut environment; Targett and Arnold, 2001). They utilised force‐feeding bioassays with extracts from various temperate and tropical browns with which X. mucosus cooccurs but is not observed to eat. The high molecular size (>10 kDa) phlorotannins had a significant eVect in reducing the assimilation eYciency (total, organic and protein) of the herbivore. This is the same size class (10–100 kDa) of phlorotannins that was found in the highest concentrations in all but one of the surveyed species. Boettcher and Targett (1993) suggested that diVerences in the molecular size distribution of phlorotannins in diVerent species could be part of the explanation for such wide‐ranging results in deterrence studies. Phlorotannins do, in some cases, aVect the nutritional value of foods, but animals (including marine herbivores) can engage in compensatory feeding to overcome this eVect (Cruz‐Rivera and Hay, 2001). This may mean that some herbivores simply eat more of a particular (phlorotannin containing) species in order to meet nutritional requirements (but see Honkanen et al., 2002). In addition, some herbivores preferred phlorotannin‐containing foods (Jormalainen and Honkanen, 2004; Pavia et al., 1997). These outcomes are not consistent with the fitness benefit that should be associated with a putative defensive metabolite. 3. Antibacterial and antifouling activity The potential antifouling and antibacterial roles of phlorotannins were first proposed in the 1940s and 1960s, respectively, and many subsequent studies have investigated the validity of these roles (reviewed in Ragan and Glombitza, 1986), with results to date also being inconclusive, at least for the
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antifouling role. In addition, note the caveats about the ecological relevance of antifouling or antiepiphytic bacteria bioassays noted in Section V. Fletcher (1975) reported that phlorotannins in the crustose alga Ralfsia spongiocarpa (Order Ectocarpales) were eVective in protecting the thallus from epiphytic fouling. In studies of members of the Fucales, Sieburth and Conover (1965) found that extracts containing Sargassum natans polyphenolics acted as an antibiotic. Phlorotannins extracted from Sargassum tenerrimum inhibit bacterial growth as well as larval settlement of polychaetes (Lau and Qian, 1997) and of barnacles (Lau and Qian, 2000) at ecologically relevant concentrations. Phlorotannins from Fucus spiralis and Ascophyluum nodosum aVected the survival and therefore the habitat choice of the ciliate Voticella marina (Langlois, 1975). A study by Wilkstro¨ m and Pavia (2004) showed that phlorotannins from Fucus vesiculosus inhibit settlement of the fouling barnacle Balanus improvisus at ecologically relevant concentrations (1 mg liter1). The second species they studied was Fucus evanescens, an invasive species, which had quantitatively much lower natural levels of fouling that the native F. vesiculosus. However, in settlement bioassays, Balanus improvisus settled on F. evanescens at higher rates when given a choice between the two species. The authors found that whilst the phlorotannin concentration of the thallus did not diVer between the two species (about 10% dwt in both), the inhibitory eVect of phlorotannins from F. vesiculosus was greater and eVective at lower concentrations than those extracted from F. evanescens. Contradictory results from field experiments (i.e., lower fouling on F. evanescens) and laboratory work (i.e., phlorotannins from F. vesiculosus more eVective antifouling) indicated that the higher eVectiveness of antifouling mechanisms in F. evanescens was not due to settlement inhibition by phlorotannins, but was due to a higher postsettlement mortality (Wilkstro¨ m and Pavia, 2004). The high level of fouling on F. vesiculosus indicates that while phlorotannins from this species can deter larval settlement, other factors are responsible for juvenile mortality. Furthermore, this demonstrates that the settlement inhibition eVect of phlorotannins is not constant even among congeneric species. In another study of F. vesiculosus, Honkanen and Jormalainen (2005) found that the variation in fouling biomass levels, which they observed on diVerent genotypes, was not correlated with tissue phlorotannin content. Lu¨ der and Clayton (2004) suggested that the presence of increased numbers of physodes at wound surfaces in Ecklonia radiata (Order Laminariales) may serve to reduce microbe infection. Molecular size may be an important factor in determining the bioactivity of phlorotannins, including antibiotic roles (Ragan and Glombitza, 1986). By contrast, Jennings and Steinberg (1997) concluded that natural concentrations of phlorotannins at the thallus
DEFENSIVE AND SENSORY CHEMICAL ECOLOGY OF BROWN ALGAE
17
surface of Ecklonia radiata were unlikely to be able to eVectively reduce epiphytism by the green alga Ulva lactuca and found no correlation between epiphyte load and tissue phlorotannin content. Their study of phlorotannin exudation rates in E. radiata found these to be much lower than rates reported in other studies, which mainly utilised stressed algae (Jennings and Steinberg, 1994, 1997). An inhibitory eVect of phlorotannins from E. radiata and Sargassum vestitum (Order Fucales) on the germination of U. lactuca was found, but only at unnaturally high concentrations (>10 mg liter1) (Jennings and Steinberg, 1997). The authors highlighted the importance in these types of studies of measuring or estimating concentrations of phlorotannins where the encounter occurs (i.e. at the boundary layer) and which the larvae or epiphytes are actually likely to encounter so that measuring tissue content is probably not appropriate for studies of epiphytism (Jennings and Steinberg, 1997). 4. Sunscreen Depletion of the ozone layer over the past few decades has led to higher levels of damaging UV‐B radiation reaching shallow water benthic communities (Frederick et al., 1998), which has led to concern over the eVects of UV‐B on benthic organisms (Karentz, 2001; Karentz and Bosch, 2001). Phlorotannins absorb in the UV‐B range of the spectrum (Pavia et al., 1997) and are considered to be one way in which the algal thallus can protect itself from photodestruction caused by UV radiation (reviewed in Schoenwaelder, 2002). A 2‐week exposure to increased UV‐B radiation led to a significant increase in the phlorotannin content of Ascophyllum nodosum (Order Fucales) (Pavia et al., 1997). In a subsequent experiment, Pavia and Brock (2000) found that A. nodosum exposed to ambient UV‐B increase phenolic content after 7 weeks (but not after 2 weeks) in comparison to individuals that had had UV‐B removed from the available spectrum. However, in a field study involving a smaller increase in UV‐B radiation, no increase was found in phlorotannin content in Desmarestia anceps or in Desmarestia menziesii (Order Desmarestiales; V. A. Fairhead, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result). Swanson and Druehl (2002) reported that tissue phlorotannin content increased in Macrocystis integrifolia (Order Laminariales) after exposure to UV‐B radiation (but also UV‐A, which phlorotannins do not absorb well). Phlorotannin exudate from M. integrifolia reduced transmission of UV‐B radiation and also reduced the harmful eVects of UV‐B on developing kelp meiospores (germination rates were higher when water contained exudate) (Swanson and Druehl, 2002). The authors suggested that in regions with high kelp densities the concentration of phlorotannins in the water body
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C. D. AMSLER AND V. A. FAIRHEAD
could alter the spectral characteristics and shield marine organisms from biologically harmful UV‐B (Swanson and Druehl, 2002). However, UV-B did not affect phlorotannins in Fucus gardneri germlings (Order Fucales; Henry and Van Alstyne, 2004). 5. Heavy metal chelation The capacity of phlorotannins to bind to metal ions is well established, which has led to the suggestion that phlorotannins may be able to reduce the toxicity of certain heavy metal pollutants (reviewed in Ragan and Glombitza, 1986; Toth and Pavia, 2000a), but very little work has been done in this area. Ragan et al. (1979) found that phlorotannins are particularly good at chelating divalent metal ions such as copper and lead. The toxicity and anthropogenic release of heavy metals into the oceans means that an ability to detoxify both the cell (e.g., Skipnes et al., 1975; Smith et al., 1986) and the surrounding environment (e.g., Ragan et al., 1980) would be advantageous for the marine system. However, Toth and Pavia (2000a) concluded that probably substances other than phlorotannins (e.g., polysaccharides and/or phytochelatins) are important for the detoxification and resistance to copper accumulation in Ascophyllum nodosum (Order Fucales). Increasing the copper concentration in the surrounding water resulted in accumulation of copper in the algal tissues (without aVecting growth rates), but not in an increase in phlorotannin content. Karez and Periera (1995) reported that a majority of the copper, lead, cadmium, zinc, and chromium in Padina gymnospora (Order Dictyotales) coextracted with phlorotannins and hypothesised that this was because they were chelated by the phenolics. E. SPATIAL AND INTRA/INTERSPECIFIC VARIABILITY
The concentration of phlorotannins has been found to vary from undetectable levels to up to 20% of thallus dry weight, varying within and between species, as well as showing spatial variation on just about every scale (for reviews, see Ragan and Glombitza, 1986; Van Alstyne et al., 2001a). Phlorotannin content has been found to vary within the thallus of an individual (Fairhead et al., 2005a; Pavia et al., 2003; Pfister, 1992; Poore, 1994; Steinberg, 1984; Toth and Pavia, 2002b; Tugwell and Branch, 1989; Tuomi et al., 1989; Van Alstyne et al., 1999a), between individuals in the same population (Fairhead et al., 2005a; Pavia et al., 2003), between diVerent sites ˚ berg, 1996; Pavia et al., 2003; Steinberg, 1989; and populations (Pavia and A Stiger et al., 2004; Targett et al., 1992; Toth and Pavia, 2000a; Van Alstyne et al., 1999a,b), across depths (Connan et al., 2004; Fairhead et al., 2005a; Martinez, 1996), between diVerent species (Fairhead et al., 2005a; Ragan
DEFENSIVE AND SENSORY CHEMICAL ECOLOGY OF BROWN ALGAE
19
and Glombitza, 1986; Steinberg, 1989; Steinberg and van Altena, 1992; Tugwell and Branch, 1989; Van Alstyne et al., 1999a,b; Stiger et al., 2004), between diVerent aged tissue (Pavia et al., 2003; Toth and Pavia, 2002b), across seasons (Connan et al., 2004; Stiger et al., 2004), and across large geographical areas (Steinberg, 1989; Targett et al., 1992; Van Alstyne and Paul, 1990; Van Alstyne et al., 1999b). Because the bioactivity of phlorotannins is often concentration dependant, this high degree of variation in phlorotannin content has important consequences for mediating the interactions between herbivores and brown macroalgae (Targett and Arnold, 2001; Van Alstyne et al., 2001a). Biogeographical patterns in phlorotannin content exist, with Australasian brown algae tending to have, on average, concentrations over five times higher than those from the northeast Pacific (Steinberg, 1989; Steinberg et al., 1995). The ecological and evolutionary consequences of this variation for algal–herbivore interactions are reviewed in Van Alstyne et al. (2001a). There is also evidence for a tropical‐temperate pattern, with tropical brown algae often containing low levels of phlorotannins (<2%) (Pereira and Yoneshigue‐Valentin, 1999; Steinberg, 1986; Van Alstyne and Paul, 1990). This was postulated to be a result of the lack of eVectiveness of phlorotannins against some tropical herbivorous fish (Steinberg, 1986; Steinberg and Paul, 1990). However, not all tropical fish are resistant to phlorotannins (Van Alstyne and Paul, 1990). Also, Pereira and Yoneshigue‐Valentin (1999) demonstrated that although phlorotannins occur in low levels in browns from the tropical south Atlantic (0.5%), sympatric herbivores are deterred by higher concentrations (2–5%), implying that they could be an eVective defence in that system if natural levels were greater. In addition, tropical brown algae do not always have low phlorotannin concentrations. Targett et al. (1992) established that, in contrast to tropical Indo‐Pacific species, many Caribbean species have high phlorotannin levels (e.g., >14%) and that all the species surveyed had concentrations >2% dwt. A later study broadened the geographical range of high phlorotannin concentration phaeophytes to the western tropical Atlantic (Targett et al., 1995). Other studies of members of the Fucales and Laminariales have found within‐species diVerences in the concentration of phenolics across diVerent regions separated by tens to hundreds of kilometres, such as the southern and eastern coasts of Australia and northern New Zealand (Cystophora moniliformis and Ecklonia radiata; Steinberg, 1989), the eastern coast of North America (Fucus vesiculosus; Target et al., 1992) and the western U.S. coastline (a variety of kelps and fucoids, Van Alstyne et al., 1999b). For other species, smaller scales (<1 km) have been more important for detecting patterns of variation than larger geographical scales (Ascophyllum
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C. D. AMSLER AND V. A. FAIRHEAD
˚ berg, 1996). Jormalainen et al. (2003) and Honkanen nodosum; Pavia and A and Jormalainen (2005) both reported a high degree of variation among diVerent populations of F. vesiculosus (which accounted for up to 65% of the total variation). Within‐population and within‐thallus variability of polyphenolic content has also been observed in A. nodosum, as well as interannual variability within populations (Pavia et al., 1999a, 2003). Several instances of interannual variability in phenolic content were also reported by Steinberg (1989) for kelp and fucoid populations. Phenolic content has also been correlated with tissue age and life cycle stages. New tissue in Zonaria angustata (Order Dictyotales) had a significantly lower density of physodes than the older branch tissue (Fig. 3; Poore, 1994). Denton et al. (1990) found that phlorotannin contents diVered between juveniles and adults but that the pattern was species specific for the three species of Fucus (Order Fucales) they investigated. Steinberg (1989) reported that juvenile Ecklonia radiata (Order Laminariales) contained higher levels of phenolics than adult secondary blades. Similarly, Van Alstyne et al. (2001b) examined diVerences in phlorotannin content between juvenile and adult kelps and fucoids and found that juveniles often had higher concentrations, but not always and that in one kelp species the adults displayed higher phenolic levels. By contrast, Pavia et al. (2003) reported that the annual shoots of adult Ascophyllum nodosum (Order Fucales) tend to have a higher phenolic content than juvenile tissue, and Stiger et al. (2004) reported the same pattern in the fucoids Sargassum mangarevense and Turbinaria ornata. The reproductive tissue of the kelps Alaria marginata, Ecklonia maxima, and Macrocystis angustifolia contain higher phenolic contents than vegetative tissue but not those in Alaria nana or Laminaria pallida (Pfister, 1992; Steinberg, 1984; Tugwell and Branch, 1989; Van Alstyne et al., 1999a). By contrast, the phlorotannin concentration in reproductive structures of the fucoids Fucus vesiculosus, Fucus gardneri, and Pelvetia compressea contain lower levels than the vegetative tissue (Tuomi et al., 1989; Van Alstyne et al., 1999a) Variation in phenolic content among meristematic, vegetative, and reproductive tissues was detected in 8 out of 15 kelp species and in 2 of 5 fucoid species surveyed by Van Alstyne et al. (1999a). Meristematic tissue tended to have the highest concentrations (Van Alstyne et al., 1999a). Phlorotannins content also varied significantly throughout the thallus of the kelp Laminaria hyperborean, as well as between individuals and populations (Toth and Pavia, 2002a). The fronds tended to have lower levels than the meristems, and older meristematic tissue tended to have higher concentrations than new meristems, although no consistent diVerences were seen between new and old fronds (Toth and Pavia, 2002a,b). Significant variation in phenolic content was
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21
detected among stipes, holdfasts, meristems, reproductive, and vegetative tissue in the kelps Alaria marginata, Ecklonia maxima, and Macrocystis angustifolia (Tugwell and Branch, 1989). Similarly, the kelp Ecklonia radiata showed significant within‐thallus variation, with higher content (on a dry weight basis) in the primary blade and stipes compared to secondary blades (Jennings and Steinberg, 1997). The basal stipes of the fucoid Ascophyllum nodosum, considered to have the highest fitness value of the species’ diVerent tissues (Pavia et al., 2002), have the highest phlorotannin concentration and are the least preferred by the gastropod Littorina obtusata (Pavia et al., 2002; Toth et al., 2005). We detected significant within‐thallus and between individual variation in the phlorotannin content of Desmarestia anceps and Desmarestia menziesii (Order Desmarestiales) (Fairhead et al., 2005a). Samples were taken from 13 areas of the thallus of multiple individuals (from various sites and depths), and results showed that whilst within‐thallus variation was significant for each individual, the actual pattern in phenolic content was not consistent across individuals of each species, either overall or grouped by collection site or depth. This spatial variability makes it exceptionally challenging to formulate hypotheses regarding the potential influence of various abiotic (e.g., light) or biotic (e.g., herbivory) factors on phlorotannin production. F. RATES AND COST OF PRODUCTION
1. Costs and trade‐oVs? Several studies have reported a correlation between increased levels of phenolics and decreasing growth rates, which has been taken in some cases as evidence for a trade‐oV between growth and a cost for phlorotannin production. However, most studies did not find this relationship consistently. Decreased growth of Ecklonia radiata (Order Laminariales) was correlated with increased phlorotannin content, but only in spring (Steinberg, 1995). Yates and Peckol (1993) found a correlation between decreased growth of Fucus vesiculosus (Order Fucales) and increased phlorotannin concentration at a site with high nitrogen (where phenolic content was lower overall), but this relationship was not found at their low nitrogen sites. Pfister (1992) found a relationship between lower growth rates and increased phlorotannin content in the fronds of Alaria nana (Order Laminariales), but in the sporophylls (which had the higher phlorotannin content) the relationship between phlorotannin concentration and growth was positive. Growth and phlorotannin content were correlated negatively in annual shoots of Ascophyllum nodosum (Order Fucales), a relationship that was consistent across two populations and over two years of data collection (Pavia et al., 1999b).
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Both Hemmi et al. (2004) and Cronin and Hay (1996a) reported positive relationships between growth and phlorotannin content in Fucus vesiculosus, but Jormalainen et al. (2003) found no evidence of a trade‐oV. In addition, Arnold and Targett (1998) pointed out that the presence of a correlation does not imply causation and that these studies only measured static concentrations, not taking into account the rates of phlorotannin turnover, which have been shown to be relatively high (Arnold and Targett, 2000). Turnover will increase the metabolic cost of maintaining a particular level of defence beyond that accounted for by simply measuring the accumulation of phlorotannins (Arnold and Targett, 2000). Toth et al. (2005) also pointed out that, in addition to which particular algal tissue is under consideration (as these do not all have the same fitness value), cost–benefit relationships must diVer depending on the type and density of the herbivore population. Arnold and Targett (2003) provided a fresh perspective on this issue. They suggested that the cycle of production and the roles of phlorotannins mean that there is in fact no possibility of a trade‐oV between growth and phlorotannin production rates, and they also accounted for the apparent trade‐ oVs reported in previous studies. They proposed a model of production that sees phlorotannins as sequestered in physodes after synthesis (Fig. 4), in which state they are reactive (and therefore measurable) in colorimetric assays. It is in this chemical form that phlorotannins act as secondary metabolites, for example, as a deterrent to herbivores or as antibacterial agents, which is dependant upon their ability to complex with proteins and other macromolecules (see Section II.D.2). These roles are only seen by
Fig. 4. Model proposed by Arnold and Targett (2003) of phlorotannin biosynthesis illustrating the transition of these compounds from reactive chemical defences in physodes to oxidised components of brown algal cell walls (CW). From Arnold and Targett (2003).
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Fig. 5. Diagram explaining the apparent growth defence trade‐oVs in brown algae with variable rates of phlorotannin production as a function of their multiple transitional roles as proposed by Arnold and Targett (2003). (A) In rapidly growing tissues, high rates of physode secretion at cell membranes provide components for cell walls and levels of measurable phlorotannins are low. (B) In slow‐growing tissues, physode decomposition at cell walls slows, production outpaces decomposition, and measured levels of phlorotannins increase. This model predicts a negative correlation between algal growth and phlorotannin content irrespective of any cost for phlorotannin production. From Arnold and Targett (2003).
Arnold and Targett (2003) as transitional, however, and are lost when the phlorotannins are cycled into their primary role of cell wall construction, where they are no longer measurable by colorimetric assays (Fig. 5). The important consequence of this scheme is that it is the requirement for cell wall construction that drives the rates of phlorotannin production and not their secondary role in defence. This means that measurable phlorotannin levels will drop when the requirement for cell wall construction (i.e., growth) is high and will increase in slow‐growing tissue where rates of phlorotannin synthesis outpace rates of decomposition and incorporation into cell walls (Fig. 5). In this way the model allows for apparent trade‐oVs between growth and phlorotannin production without necessarily requiring phlorotannin production to be allocated a cost that competes with growth. If the trade‐ oV with growth processes is eliminated, this requires questions as to the relevance of many ecological defence theories for describing patterns of phlorotannin production (see Section IV). 2. Possible determinants of production or induction Regardless of how well our knowledge of phlorotannin production fits into particular theories concerning the ecology or evolution of chemical defence, there is no doubt that many factors, both biotic and abiotic, can
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be correlated with changes in rates of production. The relative influence of one factor in a particular study may be seen as support for a chosen theory, but overall the picture of phlorotannin production is complex and does not fit easily into any one particular ecological theory (see Section IV). a. Light. Several studies have found correlative evidence for the link between irradiance and phlorotannin production. Current evidence also suggests that UV‐B radiation can induce phlorotannin production, which provides protection for the alga (Pavia and Brock, 2000; Pavia et al., 1997; Swanson and Druehl, 2002; see Section II.D.4). Fucus vesiculosus (Order Fucales) displayed a seasonal pattern in phlorotannin content that was well correlated with irradiance (Peckol et al., 1996). A similar consistent seasonal pattern in phlorotannin concentration has been found in Australian brown algae, with higher concentrations in the spring compared to autumn (Steinberg, 1995; Steinberg and van Altena, 1992). A two‐week reduction in irradiance reduced phlorotannin contents in F. vesiculosus but not in the fucoid Ascophyllum nodosum, and evidence showed that individuals collected from sun‐exposed sites contain higher concentration of phlorotannins than those from more shaded sites (Pavia and Toth, 2000b). We observed that Desmarestia anceps (Order Desmarestiales) had significantly higher phlorotannin concentrations when collected from the upper end of its depth distribution than from the lower part of its distribution, which was not true in Desmarestia menziesii, although that could have been because the depth diVerence was smaller in D. menziesii (Fairhead et al., 2005a). Phlorotannin concentrations in both species increased when they were transplanted from a 15‐m depth to a 5‐m depth regardless of whether they were shielded from UV radiation, suggesting that increased photosynetically active radiation was responsible for the diVerence (V. A. Fairhead, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result). However, neither study was intended to examine the eVects of irradiance alone, so strict irradiance controls were not performed. Consequently, although it is likely that the diVerences observed between phlorotannin levels were because of diVerences in light, this conclusion cannot be definitive. However, other investigations have found no such correlation with irradiance in other species, for example, in the fucoids Sargassum globulariaefolium and Fucus gardneri (as F. distichus) (Steinberg, 1986; Van Alstyne, 1988), or have found the peak concentration to occur in the winter (Ragan and Jensen, 1978). Also, Cronin and Hay (1996a) found no eVect on phlorotannin content of their manipulation of the irradiance environment of the fucoid Sargassum filipendula. If irradiance does play a role in phlorotannin
DEFENSIVE AND SENSORY CHEMICAL ECOLOGY OF BROWN ALGAE
25
production, it is complex and is probably tightly coupled with resource availability and/or growth processes. b. Nutrients. Several studies of Fucus vesiculosus have assessed the impact of nutrients on phlorotannin production, and the results have been inconsistent. Ilvessalo and Tuomi (1989) found an inverse correlation between tissue nitrogen and phlorotannin content in F. vesiculosus (Order Fucales). Yates and Peckol (1993) found that F. vesiculosus collected from low nitrogen sites (with lower tissue‐N content) had higher phenolic content than algae collected from high nitrogen sites (with higher tissue‐N contents) except at certain times of the year when concentrations were low overall. At both sites the phenolic content was inversely correlated to tissue‐N content over the year. However, experimental manipulation of nutrient levels failed to find a consistent reduction in phenolic content in response to nutrient enrichment (which consistently increased tissue‐N). Similarly, Peckol et al. (1996) found inconsistencies between sites (one of which was the same as in the previous study) in their study of the eVects of nitrogen enrichment on the same species. While natural phlorotannin levels were correlated negatively with tissue‐N content, Pavia and Toth (2000b) did not find any eVect of nutrient enrichment on phlorotannin content. Jormalainen et al. (2003) found that nutrient enhancement decreased phlorotannin production in F. vesiculosus, and Hemmi et al. (2004) found a decrease in the phlorotannin content of F. vesiculosus grown in water enriched with N‐P‐K fertiliser, an eVect that became significant between 10 and 38 days after the treatment began (Hemmi and Jormalainen, 2004; Hemmi et al., 2004). Investigations of other species have reported no eVect of nutrient enrichment on phenolic content in the fucoids Sargassum filipendula and Ascophyllum nodosum (Cronin and Hay, 1996a; Pavia and Brock, 2000; Pavia and Toth, 2000b) or the kelp Hedophyllum sessile (Pfister and Van Alstyne, 2003), whereas phlorotannins decreased in embryos of the fucoid Fucus gardneri (Van Alstyne and Pelletreau, 2000) and in the dictyotalean alga Lobophora variegata (Arnold et al., 1995). There was also a negative correlation between phlorotannins and nitrogen levels at their collection sites in the fucoids Turbinaria ornata and Sargassum mangarevense (Stiger et al., 2004). There is probably an influence of nutrients in the phenotypic modification of phlorotannin content, but as with other environmental factors, it is complex and poorly understood. c. Induction by herbivory. Although phlorotannins are probably eVective herbivore deterrents, the eVect is concentration dependant. Low constituent levels may not be enough to deter feeding, but an induction of phlorotannin
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production in response to herbivory will serve to reduce future herbivory, particularly from small, relatively immobile herbivores. Grazing over 2–4 weeks by the snail Littorina obtusata induced the production of phlorotannins in the fucoid Ascophyllum nodosum (Pavia and Brock, 2000; Pavia and Toth, 2000a) and this reduced grazing pressure (i.e., palatability) (Pavia and Toth, 2000a). Pavia and Toth (2000a) also noted that in natural populations of A. nodosum, individuals with more grazing marks had significantly higher phlorotannin levels than individuals with no apparent evidence of grazing. In the same study they demonstrated that the type of herbivore is important because grazing by the isopod Idotea granulosa did not produce an induction response. The authors suggest that these diVerent responses may be due in part to the diVering amounts of damage caused by the two herbivores, as the feeding mechanism of L. obtusata, which is also larger and less motile, may cause greater tissue losses and thus represent a stronger selective pressure. Toth et al. (2005) also reported that the phlorotannin content of A. nodosum increased after 2 weeks of grazing by L. obtusata, more so in the basal shoots than in the apical shoots. In an experiment that utilised snails (Theodoxus fluviatilis) to manipulate levels of fouling organisms on Fucus vesiculosus (Order Fucales), Honkanen and Jormalainen (2005) found that phlorotannin content was higher in algae from a low fouling treatment that included snails. They pointed out that the confounding factor of fouling level makes it diYcult to directly assess the impact of herbivore activity in this case, as a higher fouling level may also aVect phlorotannin production (e.g., by reducing available irradiance); in addition the snails are not known to consume F. vesiculosus and are thought to just feed on the epibiota, removing hyaline hairs (which are involved in nutrient uptake) in the process (Jormalainen et al., 2003). Whether responses to actual herbivory are an adaptive response to grazing or are due to other eVects of grazing (e.g., removal of epibiota or algal biomass, increase in nutrient absorption) that may aVect resource availability remain unclear in many cases (Jormalainen et al., 2003). Jormalainen et al. (2003) addressed this issue in Fucus vesiculosus through manipulations of the epibiota level and of the nutrient environment and also with simulated and actual herbivore presence. Their results suggest that physical contact with the herbivores is important (i.e., mere presence of herbivores but without contact had no eVect), but that this is species specific. Only one of their herbivore species (the snail Theodoxus fluviatilis) induced production of phlorotannins; the presence of another snail (Physa fontinalis) did not result in an increase in phlorotannin content. Neither of these species is thought to actually consume F. vesiculosus and the authors considered the eVect of
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T. fluviatilis to be related to the removal of hyaline hairs, which impacts nutrient assimilation, and not to a defence response. Phlorotannin content in the kelp Laminaria hyperborea decreased in response to grazing by a limpet (Ansates pellucida) and by a gastropod (Lacuna vincta), although this may have been an artefact of the artificial environment (Toth and Pavia, 2002a). In addition, we failed to find any eVect of grazing by two species of amphipods or one species of gastropod on the phlorotannin content of Desmarestia menziesii (Order Desmarestiales; V. A. Fairhead, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result). d. EVect of mechanical wounding. Mechanical wounding has been utilised frequently to test predications about the eVects of natural herbivory. Whilst it would be ideal to closely replicate the actual feeding process (Baldwin, 1990), this is often diYcult in practise and work in this area has been done by clipping, scraping with a blade, or wounding with a hole punch, which should not be assumed to simulate herbivory without testing for its validity (Pavia and Toth, 2000a). Additionally, mechanical wounding does not replicate other parts of the grazing process, such as water‐borne cues (Toth and Pavia, 2000b, see Section II.F.2.e) or, perhaps, specific forms of cell wall degradation (Potin et al., 2002). Nevertheless, several studies utilising diVerent species in both Fucales (Peckol et al., 1996; Van Alstyne, 1988; Yates and Peckol, 1993) and Laminariales (Hammerstrom et al., 1998; Lu¨ der and Clayton, 2004) have found an induction of phlorotannins in response to mechanical wounding within 3 to 5 days after wounding. However, an increase in phlorotannins in response to artificial wounding is not always observed (Hammerstrom et al., 1998; Hemmi et al., 2004; Pavia and Toth, 2000a; Pavia et al., 1997, 2003; Peckol et al., 1996; Steinberg, 1994; Yates and Peckol, 1993). Additionally, in a study of the eVects of mechanical wounding on Desmarestia menziesii, we found no increase in phlorotannin content after mechanical wounding (V. A. Fairhead, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result). Lu¨ der and Clayton (2004) suggested that this discrepancy of results may be partly a consequence of a dilution eVect when the total tissue phlorotannin content is measured, which masks accumulation in the outermost layers of the cell. e. Water‐borne cues. Recent studies have provided evidence for a potential role of water‐borne cues in the induction of phlorotannin production. Ascophyllum nodosum (Order Fucales) significantly increased tissue phlorotannin content when exposed, in a flow‐through system, to water from other aquaria containing snails (Littorina obtusata) grazing on other A. nodosum individuals (Toth and Pavia, 2000b). L. obtusata is a relatively sedentary
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species that feeds slowly so it probably has a restricted feeding range, and feeding on nearby individuals by L. obtusata may provide a reliable cue for upcoming herbivore attacks (Toth and Pavia, 2000b). Water‐borne cues may be particularly useful in an intertidal environment where physical damage is common and as such may not provide an adequate cue for herbivory (Pavia and Toth, 2000a). f. Methyl jasmonate. Arnold et al. (2001) assessed whether the plant growth regulator methyl jasmonate (MeJA), known to be important in vascular plant defence responses, is involved in phlorotannin production. Fucus vesiculosus individuals were incubated with diVering concentrations of airborne MeJA during the low tide period. Phenolic content in samples collected 12 days after incubation showed raised levels in MeJA‐treated individuals at a magnitude similar to that for a simulated grazing (clipping) treatment (Arnold et al., 2001). The authors suggested that further investigations of the role of the octadecanoid pathway are needed, but that MeJA could potentially be used to manipulate phlorotannin levels experimentally (Arnold et al., 2001). G. CURRENT UNCERTAINTY AND FUTURE DIRECTIONS
Perhaps the only conclusive statement one can make regarding phlorotannin distributions is that they are highly variable in space and time. Phenotypic plasticity in response to biotic (e.g., grazing pressure) and abiotic (e.g., nutrient and irradiance levels) factors has been well documented by field surveys and induction experiments, but these responses are by no means consistent, even within one species (e.g., Fucus vesiculosus). In addition, phenotypic responses of brown macroalgae contribute to a large variability of phlorotannin content in response to multiple stimuli, apparently in multiple ways. Genotypic variability may also be contributing to some of the within‐species variability reported (Honkanen and Jormalainen, 2005; Jormalainen and Honkanen, 2004), and the moderate to high rates of phlorotannin turnover within cells that has been reported (Arnold and Targett, 2000) could also influence this variability. This makes attempts to understand the ecological role of phlorotannins (e.g., are they constitutive or induced defences or can they be considered as a group to be herbivore deterrents) very diYcult. Complex interactions between putative production‐controlling factors mean that studies need to incorporate, or at least control for, multiple abiotic and biotic variables in study designs (e.g., Pavia and Brock, 2000; Peckol et al., 1996). Recent advances in our knowledge of physical and biological influences on phlorotannin production should allow
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future work to provide clearer outcomes, and should they be developed, genetic or enzymatic methods to monitor phlorotannin production in response to multiple, interactive stimuli would likely prove invaluable. It is no longer valid to, a priori, equate a feeding deterrent eVect in brown algae with an eVect of phlorotannins or visa versa, even in crude extracts that should be enriched in phlorotannins (e.g., Deal et al., 2003; Hemmi et al., 2004; Kubanek et al., 2004), and we also now know that the type of herbivore (e.g., gut type) influences the outcome of algal–herbivore interactions mediated by phlorotannins (Targett and Arnold, 1998, 2001). Future attempts to understand the ecological roles of phlorotannins need to incorporate these factors. Spatial variability must be studied in combination with assessments of induced defence (e.g., Taylor et al., 2002), as there is good evidence that these responses can aVect concentrations throughout the thallus over time in order to determine intrathallus variation patterns conclusively (Toth et al., 2005). Our current level of knowledge of the influence of environmental factors on the phenotypic variation of phlorotannins is limited, and we are a long way from having the ability to make predictive statements about environmental influences on phenolic content, if indeed these are appropriate. If the primary role of phlorotannins as cell wall constituents is indeed the driving force for phlorotannin production (Arnold and Targett, 2003), then eVorts to understand phlorotannin variability should be focused on the complexities of that process, as the utility for an alga of using phlorotannins as a defensive metabolite would be constrained by it (Pavia et al., 2003). Conversely, there is a large data base from numerous research laboratories correlating phlorotannin levels with defence against herbivores. We would not agree that, based on the few reports where other compounds have been identified as the actual antiherbivore component in crude extracts enriched in phlorotannins, one can assume that phlorotannins are not active as feeding deterrents in other populations or taxa even when past workers did not look for them with exhaustive, organic chemical methodology. However, we also strongly believe that more careful chemical analyses of the bioactive compounds should be performed in the future whenever knowing the specific chemical nature of feeding deterrents is critical in an experimental analysis. Correlations between feeding deterrence and colorimetrically determined phlorotannin levels should be assumed to be nothing more than that, i.e., as correlations, not causes. However, ecologically, such a correlation may be suYcient in many instances. Our own experiences make it clear to us that, although possible, purifying phlorotannins for use in chemical and biological assays without allowing them to become oxidised is far from being a trivial exercise. In addition, the organic chemistry
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technical skills and technology necessary to identify bioactive but nonphlorotannin metabolites within extracts are often not available to many ecologists. So in the end, the specific question being asked should determine the extent to which the involvement of phlorotannins in ecological interactions needs to be correlative vs definitive. The observations that increased levels of phlorotannins often but not always correlate with increased feeding deterrence demonstrate that one cannot assume that there is such a correlation in every species or situation. In our opinion, if the biological relevance of a study involves changes in palatability in addition to phlorotannin levels, one should always couple feeding bioassays on fresh thalli, on ground tissues, and/or on extracts with the phlorotannin content determinations. Unlike the potential technical diYculties presented to ecologists in determining if nonphlorotannin metabolites might be responsible for observed unpalatability, performing feeding bioassays themselves is usually a very practical option. Significantly, in many studies regarding predator–prey interactions in an ecological or evolutionary context, the response of the predator is likely more important than the particular attribute of the prey that caused it.
III. NONPHLOROTANNIN ANTIHERBIVORE DEFENCES A. DICTYOTALES
Dictyotalean algae produce a wide variety of terpenoids, acetogenins, and compounds of mixed biosynthetic origin (terpenoid‐aromatics) that, in contrast to phlorotannins, are commonly bioactive at concentrations of a few percent down to well under 1% algal dw (Hay and Fenical, 1988, 1992; Hay and Steinberg, 1992; Hay et al., 1987b; Paul et al., 2001). The most commonly studied brown algae producing nonphlorotannin secondary metabolites are species in the tropical and warm‐temperate genus Dictyota (Order Dictyotales), with well over 200 known secondary metabolites (Paul et al., 2001). Ecological roles for the bicyclic diterpene alcohol pachydictyol‐A (Fig. 6) have been especially well documented, particularly as antiherbivore defences against fish as well as some sea urchins and amphipods (e.g., Hay and Fenical, 1992; Hay and Steinberg, 1992; Hay et al., 1987a,b, 1988a; Paul, 1992; Pereira et al., 1994), although it is not bioactive against some other herbivores (e.g., Hay and Fenical, 1992; Hay and Steinberg, 1992; Hay et al., 1987a; Paul, 1992; Paul and Van Alstyne, 1988; Pereira et al., 2000a). Dictyota spp. and other members of the Dictyotales also produce a wide
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Fig. 6. Chemical structures of defensive secondary metabolites from Order Dictyotales.
variety of related compounds with known antiherbivore bioactivity such as dictyol B, dictyol B acetate, dictyol E, dictyol H, acutiol A, dolobelladiene 1 (10,18‐diacetoxy‐8‐hydroxy‐2,6‐dolobelladiene), and (6R)‐6‐hydroxydichotoma‐3,14‐diene‐1,17‐dial (Figs. 6 and 7); as with pachydictyol‐A, these have often been shown to be active against some herbivores but not others (e.g., Barbosa et al., 2004; Cronin et al., 1997; Fleury et al., 1994; Hay and Fenical, 1992; Hay et al., 1987a,b, 1988a; Hay and Steinberg, 1992; Pereira
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Fig. 7. Chemical structures of defensive secondary metabolites from Order Dictyotales.
et al., 2000a). Cruz‐Rivera and Hay (2003) demonstrated that at least some of these compounds (a mixture of pachydictyol‐A and dictyol‐E) interact with food quality and were more deterrent to five species of amphipods (but not to one species of isopod) when presented in relatively lower quality
DEFENSIVE AND SENSORY CHEMICAL ECOLOGY OF BROWN ALGAE
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artificial foods. Although not consistently so, this compound mix also decreased amphipod fitness with the negative eVects greater when the animals were maintained on a lower quality diet (Cruz‐Rivera and Hay, 2003). Based on studies utilising crude extracts that should have contained dictyols, these compounds might also play a role in host choice by amphipods (Pereira et al., 2000b). Vallim et al. (2005) reviewed diterpenes in the Ditcyotaceae from a chemotaxonomic perspective focusing on Dictyota and the most closely related genera in the family. While terpenoids, acetogenins, and related mixed biosynthetic compounds continue to be discovered from the Dictyotales (e.g., Ali et al., 2004; Soto et al., 2003), much recent attention has turned to manipulative or otherwise more detailed investigations into their functions as well as to the identification of other types of compounds with roles in antiherbivore defence of dictyotalean algae. With respect to other classes of bioactive compounds, some of the attention has been focused on sulfated and nonsulfated C11 compounds produced by Dictyopteris spp., which appear to have particularly strong eVects on amphipod herbivory (e.g., Hay et al., 1988b). Amphipods and other mesoherbivores are becoming recognised as potentially having very important roles as macroalgal predators in some communities (e.g., Arrontes, 1999; Brawley, 1992; DuVy and Hay, 2000; Peters, 2003) so defences that appear to be specific to mesoherbivores are of particular interest. Schnitzler et al. (1998) demonstrated that the sulfated compounds 3‐hexyl‐[1,2]dithiepan‐5‐one (a cyclic dithiepanone; Fig. 7) and three related, noncyclic metabolites, including thioacetic acid S‐(3‐oxoundecyl)‐ester (Fig. 7), were strong deterrents of feeding by a sympatric, herbivorous amphipod (Ampithoe longimana) but not a herbivorous sea urchin (Arbacia punctulata). Later, this same group compared palatability to Ampithoe longimana of Dictyopteris membranacea, which produces these sulfated C11 compounds, with D. hoytii, a species that does not produce them as well as with a strain of D. membranacea from culture that had lost the ability to synthesise these compounds (Schnitzler et al., 2001). D. hoytii was strongly preferred over D. membranacea when presented as fresh thallus, dried and ground thallus prepared into artificial foods, or as lipophilic or hydrophilic extracts incorporated into artificial foods. The nonsulfated‐C11‐producing strain of D. membranacea was also preferred over the field‐collected algae that produce the C11 compounds when dried and ground thallus was presented in artificial foods. In the same study, the authors showed that a maintenance diet of artificial foods supplemented with 3‐hexyl‐[1,2]dithiepan‐5‐one and 9‐oxo acid (Fig. 7), a nonsulfated compound likely to be a by‐product of sulfated C11 compound synthesis, both strongly decreased survivorship of amphipods (Schnitzler et al., 2001).
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These sulfated C11 compounds are very similar to a group of compounds released as pheromones by female gametes in a wide variety of brown algae (Amsler and Iken, 2001; Pohnert and Boland, 2002; see Section VII.A). Hay et al. (1998) showed that the pheromone produced by Dictyota, dictyotene (Fig. 9), and six of nine degradation products of dictyotene [most found naturally in Dictyopteris spp.; to our knowledge, the pheromone(s) produced by Dictyopteris spp. female gametes has not been reported] inhibited feeding by the Ampithoe longimana but only 2 of these 10 significantly decreased feeding by Arbacia punctulata. As Hay et al. (1998) discussed, the potential for brown algal pheromones and their degradation products to also function as chemical defences against mesoherbivores is intriguing. Very little information is available on biotic interactions of macroalgal germlings (Amsler et al., 1992) but it is very likely that animals such as micro‐ and mesoherbivores that commonly feed on microalgae would be particularly important predators on recently settled macroalgal propagules. Consequently, assuming some cost to their production, it would be of obvious adaptive benefit to the algae if these compounds and their biosynthetic pathways functioned not only in male gamete attraction, but also in protecting the settled female gametes and, potentially, the resulting zygotes and germlings from predation. These C11 metabolites are not just produced by female gametes but also, as in Dictyopteris, by macroscopic stages of the algae as well as by some microalgae and vascular plants (Boland, 1995; Pohnert and Boland, 2002) so there is no reason to suspect that their production need cease after syngamy (even though in many cases production does appear to cease; Maier and Mu¨ ller, 1986) or that they could not be produced by other life history stages. If they are of adaptive value as antiherbivore defences in settled gametes and zygotes, however, one would predict that they would be equally valuable in defending settled meiospores, asexual spores, and their germlings. We are aware of no such reports of such compounds being produced by these other microscopic life history stages, although this could very likely be because no one has looked for them there. However, it is noteworthy that these pheromones can be quite odoriferous and detectable by human olfaction in cultures of sexually reproducing brown algae (Mu¨ller, 1967, 1989). It would be somewhat surprising if they had gone undetected by phycologists in cultures producing meiospores or asexual spores if they are released at comparable levels to the pheromones from cultures where gametes are being produced. Nevertheless, this is an aspect of brown algal chemical ecology that warrants further attention. Another potentially defensive chemical compound that has recently received attention in the Dictyotales is sulfuric acid in high concentrations. As noted later (Section III.B), this had been documented previously in the
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Desmarestiales, where there is evidence that it does serve a defensive role. Sasaki et al. (1999) reported that three Dictyopteris spp. and Spatoglossum crassum concentrated SO42 with cellular pH levels estimated at 0.5 to 0.9. These authors speculated that the acids might function as antiherbivore defences as in the Desmarestiales, but no ecologically relevant assays were conducted. Sasaki et al. (2004) surveyed 61 brown algal species from 10 orders and extended the known, high acid Dictyotales to 7 of a total 27 species surveyed. Two species from other orders also contained high concentrations of SO42 but the ions were balanced by Ca2þ rather than Hþ so the cells were not highly acidic. It would not be at all surprising if the high pH levels found is these dictyotalean algae had ecologically relevant roles similar to those in the Desmarestiales, but this remains to be determined empirically. Likely as a result of their well‐known terpenoid, acetogenin, and mixed biosynthetic defensive chemistry and their widespread geographic occurrence in tropical and warm temperate seas, members of the Dictyotales have been important models in experimental studies of macroalgal chemical ecology. This includes tests of chemical defence theories as detailed in Section IV, but they have also served as models for other important experimental questions. For example, it has long been thought that grazing pressure is higher in the tropics than at temperate latitudes (e.g., Gaines and Lubchenco, 1982; Vermeij, 1978) and that this has resulted in higher levels of chemical defences in tropical macroalgae (e.g., Fenical, 1980; reviewed by Van Alstyne et al., 2001a). However, this has rarely been experimentally tested. Bolser and Hay (1996) compared the palatability to tropical and temperate sea urchins of congeneric tropical (Bahamas) and temperate (North Carolina) macroalgae from four dictyotalean genera (Dictyopteris, Dictyota, Lobophora, and Padina) and Sargassum (Order Fucales) as well as one red and one green algal genus. When presented as dried thallus powders in artificial foods, the temperate species were, in general, preferred significantly by both tropical and temperate sea urchins with the exception of Dictyota. Assuming that these specific Dictyota spp. are an exception and the tropical vs. temperate pattern is indeed generalisable, one would predict that this would select for increased tolerance to defensive metabolites by tropical herbivores because they are confronted with more heavily defended prey. Cronin et al. (1997) tested that prediction using diterpenoid secondary metabolites from the tropical species Dictyota acutiloba and reported that acutilol A (Fig. 6) and two closely related diterpenoids were indeed more strongly deterrent to temperate than tropical macroherbivores (fish and sea urchins). (See also Section II.E for a discussion of hypotheses about latitudinal variations in phlorotannin concentrations and of tests thereof.)
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Within the North Carolina populations studied by Bolser and Hay (1996), Dictyota spp. from the two regions were equivalent in palatability, but oVshore populations, particularly of D. menstrualis, were usually significantly less palatable than inshore populations, which was reflected in comparisons of palatability between North Carolina and Bahamas species. Using the amphipod Ampithoe longimana as the bioassay animal, Taylor et al. (2003) reported that the increased unpalatability of the North Carolina oVshore populations of D. menstrualis was due primarily to the production of 4‐hydroxydictyodial A and 18,O‐diohydro‐4‐hydroxy‐dictyodial A 18‐acetate (Fig. 7) in the oVshore but not inshore populations. The diVerence between populations was not because of diVerences in pactydictyol A or dictyol E, which, as noted earlier, are deterrent to sea urchins and fish but often not to amphipods. Amphipods raised on oVshore populations had decreased growth, reproduction, and survivorship compared to animals raised on inshore algae. These authors also reported that oVshore populations of Sargassum filipendula (Order Fucales) and Spatoglossum schroederi were less palatable to the amphipods than inshore populations. In addition, Pereira et al. (2004) reported that crude extracts of Stypopodium zonale from two widely separated sites in Brazil deterred herbivory by crabs (Pachygrapsus transverses) and sea urchins (Lytechinus variegatus). However, extracts from one site (Bu´ zios) were significantly more deterrent than from the other (Fernando de Noronha), which was correlated with a diVerence in the major defensive metabolites present in the two populations. The major compound produced by the Bu´ zios population was the meroditerpene atomaric acid (Fig. 8), whereas at Fernando de Noronha it was the meroditerpene stypoldione (Fig. 8). Atomaric acid was strongly bioactive against both crabs and sea urchins when presented at the natural concentration found within the Bu´ zios algae, whereas stypoldione was less active as a deterrent for sea urchins and not significantly deterrent to the crabs when presented at the natural concentration from the Fernando de Noronha population. The selective factors that might be responsible for the intraspecific diVerences documented in these studies are unclear, but nevertheless these results are important because they show that there can be marked qualitative diVerences in defensive attributes within individual macroalgal species, even when collected from geographically close but distinct populations. Dictyotalean algae have also been very important models for examination of other aspects of macroalgal–herbivore relationships. For example, although Ampithoe longimana is often used as a bioassay animal for studies of dictyotalean chemical defences along the southeastern United States coast and preferentially feeds on nondefended macroalgae if oVered in the laboratory (e.g., Cruz‐Rivera and Hay, 2003), in nature it actually prefers to live
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Fig. 8. Chemical structures of defensive secondary metabolites from Orders Desmarestiales, Fucales, and Dictyotales.
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and feed on Dictyota menstrualis in this region (DuVy and Hay, 1994). This appears to be an adaptation that reduces predation on the amphipod by omnivorous fish that eat both macroalgae and amphipods but are chemically deterred by D. menstrualis (DuVy and Hay, 1991, 1994). The distribution of A. longimana continues much further north along the U.S. coast than D. menstrualis, and Sotka and Hay (2002) reported that allopatric A. longimana from Connecticut were less resistant to the defensive chemistry from D. menstrualis and also had lower growth rates and fitness than sympatric amphipods when raised on D. menstrualis (and Dictyota ciliolata) in the laboratory. Furthermore, these diVerences were based genetically, as they persisted through two generations in culture. Sotka et al. (2003) expanded upon and collaborated these conclusions by examining this relationship across three sympatric and six allopatric populations of A. longimana. When amphipods from northern and southern populations were crossed experimentally (Sotka, 2003), the hybrid oVspring were intermediate between the parental strains in terms of feeding preference for D. menstrualis, further confirming the genetic basis of resistance to the algal chemical defences. B. DESMARESTIALES
That members of the genus Desmarestia can sequester very high levels of acid within their thalli has been known since at least the 1930s (Kylin, 1931; Miwa, 1931; Wirth and Rigg, 1937), although early workers diVered on the specific acid responsible and it was not until the 1950s that this was resolved to be sulfuric acid across the genus (Eppley and Bovell, 1958; Meuse, 1956). Vacuolar pH within cells is commonly estimated as below 1.0 with H2SO4 comprising 12 to 25% of the thalli by dry weight (Anderson and Velimirov, 1982; Eppley and Bovell, 1958; McClintock et al., 1982; Miwa, 1931; Pelletreau and Muller‐Parker, 2002; Sasaki et al., 1999, 2004). Although previous authors (e.g., Anderson and Velimirov, 1982; Dayton, 1985b) had proposed that the acidity could be a defence against herbivores, it is surprising that an explicit test of this was not published until Pelletreau and Muller‐Parker (2002) demonstrated that sulfuric acid added to artificial foods at levels comparable to those found in Desmarestia munda could explain the unpalatability of thalli of that species to sea urchins. Marine tunicates also sequester sulfuric acid at high concentrations and although its potential defensive role has been somewhat controversial, using techniques similar to Pelletreau and Muller‐Parker (2002), it has been shown that the acid can also serve as an ecologically relevant defence against potential predators of tunicates (McClintock et al., 2004; Pisut and Pawlik, 2002).
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Based on their consensus molecular phylogeny of the Family Desmarestiaceae, Peters et al. (1997) concluded that sequestration of high concentrations of H2SO4 is a derived characteristic in the family and arose only once. However, Desmarestia antarctica, which groups at the base of the family with other southern hemisphere species that are nonacidic, also produces acid (presumably H2SO4), albeit in much lower concentrations than other Desmarestia spp. (pH of cell slurries ¼ 4.5; Moe and Silva, 1989). D. antarctica thalli are very unpalatable to sympatric algal consumers (amphipods, fish, sea stars) and crude extracts (pH neutralised) of D. antarctica are also deterrent to them, but only modestly so (Amsler et al., 2005a). Amsler et al. (2005a) proposed that the strong observed unpalatability of the fresh thalli is likely a combination of deterrent eVects of the modest secondary metabolite deterrence and the weak acidity. Perennial, nonacidic members of the Desmarestiales, particularly Desmarestia anceps, D. menziesii, and Himantothallus grandifolius, dominate shallow water, hard‐bottom communities along the western Antarctic Peninsula, often covering the vast majority of the bottom with biomass levels comparable to temperate kelp forests (Amsler et al., 1995; Brouwer et al., 1995; Neushul, 1965; Wiencke and Clayton, 2002). These nonacidic species are strongly unpalatable as thallus to sympatric sea stars, fish, and amphipods (Amsler et al., 2005a). Although some of this unpalatability could be due to relatively high levels of phlorotannins (Fairhead et al., 2005a), more lipophilic compounds not present in phlorotannin‐enriched extracts were responsible for at least some of the unpalatability in D. menziesii and H. grandifolius as well as in Phaeurus antarcticus (K. Iken, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result; Amsler et al., 2005a). The only specific metabolite identified to date with ecologically relevant bioactivity is menzoquinone (Fig. 8), a hydroquinone with feeding deterrent bioactivity against sea stars (Ankisetty et al., 2004) but not amphipods (C. D. Amsler, unpublished). C. OTHER ORDERS
A majority of chemical defence studies of other brown algae have focused on the potential roles of phlorotannins, as described in Section II.D. Although there are over 280 nonphlorotannin secondary metabolites known from other orders in the Phaeophyceae (Harper et al., 2001), relatively few studies have targeted ecological roles for specific compounds. Deal et al. (2003) reported that the chemical defence of Fucus vesiculosus (Order Fucales) from North Carolina and Maine (USA) against the sea urchin Arbacia punctulata was due to a polar galactolipid (Fig. 8) and one or
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more hydrophilic, nonphenolic compounds rather than to phlorotannins. The latter compound or compounds were unstable and could not be identified. Kubanek et al. (2004) similarly localised the chemically deterrent bioactivity against A. punctulata and two amphipod species in F. vesiculosus from North Carolina and Connecticut to unstable but clearly nonphlorotannin compounds. Sargassum spp. (Order Fucales) are commonly, although not always, unpalatable to sympatric herbivores (e.g., Hay, 1986) and produce significant levels of phlorotannins (e.g., Arnold and Targett, 2000; Stiger et al., 2004), but Cronin and Hay (1996a) reported that the palatability of S. filipendula was not correlated with experimentally manipulated phlorotannin contents. The Antarctic fucoid Cystosphaera jacquinotii is unpalatable to sympatric sea stars, amphipods, and fish (Amsler et al., 2005a) and although phlorotannins could be responsible for all or part of this unpalatability with amphipods and fish, the sea stars were deterred by relatively lipophilic extracts and not by those enriched in phlorotannins (K. Iken, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result; Amsler et al., 2005a). Similarly, Adenocystis utricularis (Order Chordariales) was chemically defended against sympatric Antarctic sea stars and amphipods, but phlorotannin‐enriched extracts were not deterrent (K. Iken, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished result; Amsler et al., 2005a). Although potentially challenging technically if chemical instability proves to be common, understanding the potential roles of nonphlorotannin secondary metabolites in chemical defence of brown algae outside the Dictyotales remains an important area for future studies, particularly in the light of recent work (Deal et al., 2003; Kubanek et al., 2004) highlighting the importance of nonphlorotannin defences even in taxa that elaborate high concentrations of phlorotannins. D. ACTIVATED DEFENCES
Activated chemical defences are those that are produced constitutively but maintained in a biologically inactive form until wounding inflicted by a herbivore or other cause cues an enzymatic conversion of this precursor into a bioactive form. Such defences are fundamentally distinct from the induced defences described in Section IV.B because the alga (or other organism) has already made an investment of resources in the defensive compound(s). However, the defensive compounds are stored in a less biologically active form that presumably is less toxic to the producing alga or otherwise less costly to maintain. Activated defences in algae were first identified in green macroalgae (Paul and Van Alstyne, 1992) and have since been identified in a number of other macroalgae and microalgae
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(e.g., Jung et al., 2002; Pohnert, 2002; Steinke et al., 2002; Van Alstyne and Houser, 2003). However, to our knowledge the only report of an attempt to identify them in brown algae is that of Cetrulo and Hay (2000) who surveyed for induced responses in 42 macroalgal species, including 17 brown algal species (11 from Order Dictyotales, 4 Fucales, 2 Scytosiphonales, and 1 Ectocarpales). They reported that extracts from three Dictyota spp. (Order Dictyotales) and Scytosiphon lomentaria (Order Scytosiphonales) that had been severely wounded before extraction were significantly less palatable than extracts of unwounded thalli to sea urchins, fish, or both. These data suggest that defence activation had occurred due to the wounding, although the possibility that the results were caused by loss of some palatable component from the wounded algae cannot be ruled out completely. To our knowledge, compounds that might have been activated have not been identified from these algae, and identification of specific activated defences would, obviously, discount the possibility that the observed changes in palatability were caused by loss of feeding stimulants.
IV. TESTING CHEMICAL DEFENCE THEORIES WITH BROWN ALGAE Almost all chemical defence theories that have been applied to or tested with macroalgae are derived from the terrestrial plant literature. This should not be surprising considering the much greater overall level of research eVort that has been focused on terrestrial organisms. However, the application of these ideas to algae is certainly appropriate considering that macroalgae are analogous to terrestrial plants in being autotrophic and in being unable to behaviourally fight or flee a predator. Consequently, macroalgae provide analogous but phylogenetically distinct models with which to test these ideas about chemical defence and, potentially, to expand upon them in ways not possible with terrestrial organisms. That is particularly true of brown algae because of the much greater phylogenetic separation between them and terrestrial plants compared to red or green macroalgae (Section I); in fact, a majority of studies concerning chemical defence theory in macroalgae have utilised brown algae as models, particularly with respect to the optimal defence theory (ODT) and the induced defence model (IDM). Many of these studies have focused in whole or in part on phlorotannins, which, as noted earlier (Section II.E) display a wide range of variability on multiple scales. For the purposes of this section, in those cases we will follow the original authors in presuming that phlorotannins were indeed the defensive compounds even though in many cases that may not have been
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demonstrated definitively. It would be wise to consider all such studies carefully in the light of currently evolving ideas about the primary and secondary roles of phlorotannins and their eVectiveness as chemical defences (Sections II.E and III.C), particularly where chemical assays were not coupled with feeding bioassays testing palatability of the algal thallus or extracts thereof or where an energetic trade‐oV between allocations to defence versus growth was assumed. All chemical defence theories assume some cost to the production, maintenance, and/or storage of secondary metabolite defences but also assume that such costs are oVset by benefits to the fitness of an organism. Although accurate measurements of total costs of chemical defences can be diYcult, the biosynthesis of secondary metabolites clearly generates significant costs in terrestrial plants (reviewed by Heil, 2002; Purrington, 2000; Stamp, 2003). In brown algae, several authors have quantified costs of phlorotannin production in situ (see Section II.F.1). However, Arnold and Targett (2003) have argued that conclusions about costs from such studies are flawed because they do not consider the primary roles of phlorotannins [but see Koivikko et al. (2005) for evidence that the proportion of phlorotannins devoted to primary roles may be relatively small compared to secondary roles]. With respect to benefits, utilising terrestrial plant models, Mauricio and Rausher (1997), Agrawal (1998), and Baldwin (1998) directly demonstrated cost–benefit relationships and/or increases in fitness with respect to allocation of resources to chemical defence, and similar results continue to be reported in other terrestrial plants (e.g., Glawe et al., 2003). Corresponding studies of the benefits of defence in brown algae have primarily been correlative in linking investment in chemical defences with decreased consumption by or decreased fecundity in herbivores (e.g., Borell et al., 2004; Fairhead et al., 2005b; Toth et al., 2005). An important goal for future research on brown and other macroalgae is the direct demonstration of a fitness benefit to the algae as a consequence of the production of chemical defences. A. OPTIMAL DEFENCE THEORY
The optimal defence theory (Rhoades, 1979) examines within‐organism variations in defensive chemistry in the context of the competing relationship between growth and the production of chemical defences. ODT was developed in the context of the common and often marked diVerences observed in defensive compound allocations to various organs and tissues in terrestrial plants (Denno and McClure, 1983; McKey, 1974, 1979). Assuming that there is some cost to the production of defensive compounds, ODT predicts
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that defences should be directly correlated with risk of attack and inversely correlated with the cost of a particular defence. Furthermore, the theory predicts that within an organism, defences should be diVerentially allocated to those tissues or structures most valuable in terms of fitness and that there should be a correlation between energetic investment and defence in specific tissues. Most tests of ODT predictions in macroalgae have used brown algae as models and most but not all of these studies have provided support for the theory. In a general sense, the portion of a macroalgal thallus most exposed to herbivore attack is the epidermis (or meristoderm as appropriate), as these outer layers are the first thing the predator would encounter. Tugwell and Branch (1989) tested several predictions of ODT in three species of kelps, including the hypothesis that phlorotannins would be most concentrated in the meristoderm, which was indeed the case. The meristoderm layers in Ecklonia maxima and Laminaria pallida had phlorotannin concentrations manyfold higher than cortical and medullary layers, and the concentrations in Macrocystis angustifolia meristoderm layers made up a majority of the total found in the thalli. However, these authors only looked at the distribution of phlorotannins and did not bioassay the thallus layers or extracts thereof to test the hypothesis that the increased phlorotannin concentrations in fact resulted in greater unpalatability. Nevertheless the observation of higher phlorotannin levels in the meristoderm is very consistent with many studies on a wide variety of brown algae that, while not framed in the context of defence theories, have reported higher densities of physodes in epidermal layers (reviewed by Schoenwaelder, 2002; see Section II.A.2). Reproductive tissues are of apparently obvious importance in terms of fitness and, because of relatively dense cytoplasm, might also be expected to often be relatively high in energetic investment. In both senses, the ODT would predict that they have relatively high levels of defence. Kelps (Order Laminariales) are excellent models for testing predictions about resource allocation to reproductive tissues because they typically produce meiospores in relatively large, discrete sori that are often borne on specialised blades (sporophylls). In a seminal paper, Steinberg (1984) demonstrated that sporophylls in Alaria marginata had much higher phlorotannin levels than vegetative blades and were significantly less palatable to herbivorous snails in both laboratory and field assays. Neither tissue nitrogen nor thallus toughness was correlated with the herbivore preference, strongly supporting the hypothesis that the diVerence in palatability was due to chemical defences and in line with ODT predictions. Tugwell and Branch (1989) also examined phlorotannin concentrations in kelp reproductive tissues and reported higher concentrations in sporophylls of Ecklonia maxima and
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Macrocystis angustifolia compared to vegetative tissues but this pattern did not hold for fertile sori in Laminaria pallida, which had very low phlorotannin concentrations. As noted earlier, however, these authors did not assay the eYcacy of the phlorotannins as antipredator defences. Van Alstyne et al. (1999a) measured phlorotannin contents in Alaria marginata from several diVerent sites and reported higher levels in sporophylls from some but not all when compared to vegetative blades (although not compared to the vegetative meristems) but this was not true in A. nana from two sites where there was no significant diVerence in phlorotannin concentrations between vegetative blades and sporophylls. Pfister (1992), however, did report higher phlorotannin levels in sporophylls than in vegetative blades of A. nana from one of the same sites reported on by Van Alstyne et al. (1999a). In both studies, overall phlorotannin levels were relatively low and the extent to which the reported diVerences could be due to intraannual or seasonal variation is unknown. Van Alstyne et al. (1999a) also compared phlorotannin levels between vegetative blades and reproductive tissues (receptacles) in four members of Order Fucales and reported that, in apparent contrast to ODT predictions, they were significantly lower in the receptacles of Fucus gardneri and Pelvetia compressa and not significantly diVerent between these tissues in Fucus spiralis or Pelvetiopsis limitata. Although palatability was not measured, higher phlorotannin contents had been correlated previously with reduced palatability in F. gardneri as (F. distichus, Van Alstyne, 1988). Similarly, Tumoi et al. (1989) reported that phlorotannin levels were lower in receptacles of Fucus vesiculosus than in vegetative tissues (although the receptacles were physically tougher than vegetative tissues). However, this chemical diVerence is only a contradiction if indeed the reproductive tissues are more important in terms of overall fitness. Although as mentioned earlier that makes a great deal of sense intuitively, it may not always be true. As Pavia et al. (2002) have noted, the life history characteristics of the algae need to be considered since, for example, loss of reproductive tissues may be much more detrimental in a short‐lived annual species compared to a long‐ lived perennial. Using the relatively long‐lived fucoid Ascophyllum nodosum as a model, these authors applied demographic elasticity (proportional sensitivity) analysis of population–projection matrices in an attempt to objectively estimate relative fitness values of diVerent components of the thalli. This analysis predicted that fitness values, and therefore by ODT prediction, defences, should be highest in the stipes, intermediate in the annual shoots (which contain the meristems), and lowest in the receptacles. Indeed, both palatability of fresh tissue to the herbivorous snail Littorina obtusata and phlorotannin contents followed these predictions with stipes
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being significantly less palatable and higher in phlorotannins than annual shoots, which were significantly less palatable and higher in phlorotannins than the receptacles. The pattern of fitness value and defensive levels within the Ascophyllum nodosum (Pavia et al., 2002) does make sense intuitively when one considers not only the life history characteristics but also the morphology of the species. Even though meristems and receptacles are obviously important, in an alga like A. nodosum with a single primary axis, damage to that axis (the stipe) that caused or increased the chance of catastrophic breakage would mean the loss of all thallus components above that point, including multiple apical shoots and receptacles. Although based on a subjective rather than objective analysis of fitness value, we have compared within‐ thallus variation chemical and physical defences in two large, nonacidic, perennial members of the Desmarestiales with similar but not identical levels of morphological complexity as a test of ODT predictions (Fairhead et al., 2005b). In terms of thallus construction, although approximately an order of magnitude larger in overall size, Desmarestia anceps is similar to A. nodosum in typically having a single primary axis (stipe) that supports lateral branches containing most of the photosynthetic and reproductive tissues. We reasoned that because breakage of the stipe would result in loss of a large amount of the lateral tissues, on a per unit volume (or biomass) basis, ODT would predict higher levels of defence in the stipes, which indeed was the case with both chemical and physical defences (chemical defences measured as palatability of crude extracts to the sympatric, herbivorous amphipod Gondogeneia antarctica). In contrast, the sympatric and ecologically similar congener Desmarestia menziesii typically has multiple main axes supporting lateral branches, less morphological distinction between main axes and laterals, and fewer orders of branching overall. In D. menziesii there was no diVerence in palatability of crude extracts of main axes and laterals, although the main axes were physically tougher. We also included holdfasts in our analyses, which also diVered morphologically between the species. In D. anceps, the holdfast is composed of multiple, intertwined haptera that are capable of regrowth. Although damage to a holdfast that resulted in an alga becoming dislodged from the substrate is obviously the most extreme form of damage possible for a large macroalga, we reasoned that mesograzer damage to any individual part of the D. anceps holdfast would be less severe in terms of the chances for catastrophic breakage than damage to the primary stipe. This was both because of the multihaptera construction of the holdfast and because small damage to the main stipe, which must withstand much greater physical bending due to wave surge, is more likely to result in catastrophic breakage (cf. Duggins et al., 2001; Koehl and
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Wainwright, 1977; Utter and Denny, 1996) and, based on that assumption, the observations that the holdfast was less chemically defended (although not significantly diVerent in terms of toughness) compared to the primary stipe was consistent with ODT predictions. Conversely, in D. menziesii the holdfast is a single, small discoid structure rather than a mat of individual haptera. Coupled with the smaller diVerence between primary and lateral axes, we predicted that the holdfast tissue would be at least comparable to the main axes in terms of fitness value and indeed they were both significantly tougher than the lateral branches, although all three components were equivalent in terms of chemical defences. It is also of note that although these ODT‐predictable diVerences were evident in crude extract feeding bioassays utilising an important, sympatric herbivore, they were not explained by the marked but much less consistent intrathallus variation in the levels of phlorotannins (Fairhead et al., 2005a). Also based on a subjective rather than objective analysis of fitness value, Taylor et al. (2002) made a very similar prediction about the relative fitness values of thallus components in Sargassum filipendula, reasoning that lower portions of the thallus were most important because they supported the upper, meristematic, and reproductive branches. They reported that these lower portions of the stipes were most unpalatable to a sympatric herbivorous amphipod but that this unpalatability was the result of physical toughness rather than of chemical defences. Several other studies have compared defensive investment in brown algal vegetative tissues in terms of ODT predictions, particularly with respect to meristematic vs. older or more developed sections of the vegetative thallus. Tugwell and Branch (1989) reported that in three kelps, phlorotannin levels in meristems, holdfasts, and stipes were higher than in the blades. Van Alstyne et al. (1999a) reported higher phlorotannin levels in meristems compared to blades in eight kelp species. An additional seven kelp species and four fucoids did not have significant diVerences in phlorotannin levels between the two tissue types, although in the seven kelps, overall phlorotannin levels were usually much lower than in the species displaying a diVerence (Van Alstyne et al., 1999a). As noted previously, neither of these studies directly examined palatability of the specific tissues to herbivores, but Johnson and Mann (1986) did correlate much higher phlorotannin levels in meristems compared to blades in the kelp Laminaria longicuris with palatability to a herbivorous snail. The stipe, holdfast, and midrib were also relatively unpalatable but this appeared to be correlated with physical toughness rather than chemical defence (Johnson and Mann, 1986). Although the chemical nature of deterrence can only be inferred from the presence and concentration of physodes, Poore (1994) documented a
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visually striking example of diVerential levels of defence among meristems, newly formed cells, and older cells in Zonaria angustata (Order Dictyotales). Z. angustata grows from a row of meristemsatic apical cells that are darkly colored because of a high density of physodes (Figs. 2 and 3). Newly formed cells have few physodes and are very lightly colored, and as cells age (correlated with their distance back from the apical cell row), they accumulate physodes (Fig. 3). Palatability of these cell zones to two species of herbivorous amphipods was strongly negatively correlated with the density of physodes and not related to diVerences in physical toughness (Poore, 1994). It is of note that this species also covers its antheridia (male reproductive cells) with a sterile cell layer rich in physodes, which have been suggested to play a role in herbivore deterrence (Phillips and Clayton, 1991). Although the high level of apparent chemical defence in the apical cell row (and over the antheridia) would seem in line with ODT predictions, the fact that the amphipods could rip through the apical cell row and consume the new, palatable cell zone behind it, thereby leading to the loss of entire apical cell rows (Fig. 2), indicates that defending only the apical cells is ineVective in the larger sense, at least with respect to the two amphipod species used in these experiments. Nevertheless, as Poore (1994) discussed, the very great diVerences in palatability of thallus components separated by only a few cells highlight the fact that particularly with small mesograzers, such as amphipods, chemical ecologists may need to consider the distribution and eYcacy of chemical defences over very fine spatial scales within a macroalgal thallus. Cronin and Hay (1996b) tested the ODT prediction that younger, meristemsatic tissues should be more highly defended than older tissues using another member of the Dictyotales, Dictyota ciliolata, and reported that ODT predictions were not met. The younger blade apices were significantly more palatable and less chemically defended than older portions of the thallus. Although some authors have contrasted this with Poore’s (1994) report on Z. angustata because the latter species had a defended meristem (apical cell row) at the branch tips, such a contrast is misleading as it ignores important morphological diVerences between the genera. Even though both are members of the Family Dictyotaceae, Dictyota spp. grow from a single apical cell at the tip of each branch rather than from an apical cell row. In both D. ciliolata and Z. angustata the young cell zone immediately behind the apical cell(s) was significantly more palatable than older tissues farther down the thallus. Cronin and Hay (1996b) speculated that one reason for the diVerence between this and tests in other orders of brown algae supporting predictions of the ODT is that Dictyota spp. lack a known mechanism to transport materials between cells within the thallus (even though closely
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related Dictyopteris menbranacea does have structures morphologically consistent with transport capacity in their midribs; Katsaros and Galatis, 1988). While a lack of translocation capability remains to be proven as an explanation for the diVerences between defences in meristematic and other nonsupportive vegetative tissues in Dictyota spp. (which do not have midribs), it points to an important feature of brown macroalgae that is sometimes (but not always, e.g., Hemmi et al., 2004; Van Alstyne, 1988) overlooked by chemical ecologists when interpreting within‐thallus patterns of chemical defence or in studies of the induction of chemical defence. Although it is commonly recognised that members of the Laminariales have conductive cells (trumpet hyphae) that allow translocation of photosynthate and other substances within the thallus (Graham and Wilcox, 2000; Lobban and Harrison, 1994), other orders of brown algae are likely to have analogous capabilities (Raven, 2003). Members of the Desmarestiales also contain trumpet hyphae (Fritsch, 1945; Raven, 2003) and although members of the Fucales do not have quite such obvious conductive structures, it has been known for over 120 years that there is analogous cytoplasmic continuity between their medullary cells (Hick, 1885; Moss, 1983) and analogous structures may also be present in the Ascoseriales and Scytosiphonales (Raven, 2003). Members of the Fucales are able to translocate inorganic nutrients and photosynthate via filamentous medullary cells within their thalli, although apparently only from older to younger tissues (Diouris and Floc’h, 1984; Floc’h, 1982). Consequently, there is at least a possibility that they could also transport defensive compounds or, with respect to defence induction (Section IV.B), inductive signal molecules within their thalli (cf. Ryan and Pearce, 1998). These features need to be considered more often when both designing and interpreting the results of chemical defence studies, and the potential for transport of defensive compounds and/or inductive signals should be specifically tested more frequently. B. INDUCED DEFENCE MODEL
The induced defence model (Harvell, 1990; Karban and Meyers, 1989) follows from the ODT prediction that defence production should be directly correlated with risk of attack. Assuming that chemical defences are indeed costly to an organism, if predation pressure is variable in space or time one mechanism by which these costs might be reduced is for the organism to produce defences only when under attack by a consumer. Conversely, ODT and IDM would predict constitutive defence production if predation pressure is consistent and heavy. However, temporal and spatial patterns of predation are critical because limiting the production of chemical defences
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to those times when an organism is under attack by a consumer would only be beneficial if the defences could be produced in time to have a significant impact on consumption by the predator. Hay (1996) proposed that inducible chemical defences in macroalgae and other benthic marine organisms would likely be most eVective if produced in response to mesograzers because they cause only partial damage to their prey, at least over short time intervals, and because they often feed on individual macroalgae for long enough periods for a chemical response to be produced. Nevertheless, the critical features of predation are its spatial and temporal scales if induced responses are to be eVective. Not all mesograzers feed on individual prey for long times or are limited to feeding within small spatial ranges (cf. Paul et al., 2001). Also, larger predators such as Antarctic sea stars sometimes prey on an individual organism for very long periods of time (cf. Amsler, 2001; Dayton et al., 1974). As a result, not all small consumers feed in ways that would be predicted by the IDM to select for induced defences, whereas some larger consumers do feed over temporal and spatial scales that would be predicted to select for induced defences in their prey. Induction of defence or ‘‘resistance’’ in brown algae, particularly with the Fucales, has been a relatively active area of research in the past few years and, until very recently (Ceh et al., 2005; Weidner et al., 2004), browns were the only macroalgal group known to have inducible defences against herbivory. Induced chemical defences in macroalgae were first documented in a landmark study by Van Alstyne (1988), which demonstrated that two weeks after simulated grazing (mechanical clipping) of Fucus gardneri (as F. distichus, Order Fucales), clipped thalli were significantly less palatable than controls to herbivorous snails and had significantly higher phlorotannin concentrations in and adjacent to the damaged areas. Within the Fucales, chemical defence induction, detected at least in part via a change in palatability to herbivores, has also been documented in Fucus vesiculosus (Hemmi et al., 2004; Rohde et al., 2004; Yates and Peckol, 1993), Ascophyllum nodosum (Borell et al., 2004; Pavia and Toth, 2000a; Toth and Pavia, 2000b; Toth et al., 2005), Sargassum filipendula (Sotka et al., 2002; Taylor et al., 2002), and Sargassum asperifolium (Ceh et al., 2005). Induction measured as increases in phlorotannins without concurrent measurements of palatability has also been reported (Pavia and Brock, 2000; Peckol et al., 1996). Very nonpolar extracts of Cystoseira myrica that had been subjected to amphipod grazing were significantly less palatable than extracts from untreated controls; however, although there was a trend for the same pattern in intact thalli, the diVerence was not statistically significant (Ceh et al., 2005). Pavia et al. (1997) were unable to detect decreased palatability or increased phlorotannin levels in Ascophyllum nodosum that was clipped
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mechanically in a design similar to that of Van Alstyne (1988). However, Pavia and Toth (2000a) documented an induction of increased phlorotannin levels and a concomitant decrease in palatability when A. nodosum was fed on by the snail Littorina obtusata but not by the isopod Idotea granulosa or when subjected to two diVerent methods of mechanical wounding even though the snails and amphipods removed equivalent algal biomass. This indicates that for at least some macroalgae, induction is not a general response to wounding but rather is cued specifically by specific herbivores (as is also known in terrestrial plants; cf. Karban and Baldwin, 1997). Potin et al. (2002) have hypothesised that the herbivore‐specific signal could be related to specific oligoalginates released during cell wall decomposition and/ or to alginate‐degrading enzymes of the herbivore (cf. Section V). Toth and Pavia (2000b) showed that the inductive signal was a waterborne compound that could induce defence production in ungrazed thalli receiving water from aquaria containing A. nodosum that were being grazed on by L. obtusata (but not by mechanically wounded A nodosum). This result was particularly exciting in the context of the growing terrestrial plant literature on airborne induction of chemical defences between individuals (e.g., Kessler and Baldwin, 2001). [For a more detailed microreview focused on Pavia and Toth (2000a) and Toth and Pavia (2000b), see Amsler (2001).] Particularly interesting in the context of diVusible chemical cues for defence induction identified by Toth and Pavia (2000b), Arnold et al. (2001) reported that a brief exposure to methyl jasmonate, a volatile compound involved with inter‐plant defence induction in terrestrial plants, could significantly stimulate phlorotannin synthesis in Fucus vesiculosus. Neither this compound nor its precursor is known from brown algae, and because the eVects of the increased phlorotannins on palatability to herbivores were not measured, the direct ecological relevance of this observation cannot be assessed. However, methyl jasmonate has been identified in red macroalgae (Bouarab et al., 2004), and these authors speculate that it may have been acquired from the plastid endosymbiont and, hence, potentially may be found in any photosynthetic eukaryote. Rohde et al. (2004) demonstrated that chemical defences (measured as unpalatability) in F. vesiculosus could be induced by direct grazing of either the snail Littorina littorea or the isopod Idotea baltica. Waterborne cues from I. baltica grazing could induce defences in neighboring F. vesiculosus, but this was not true of grazing by L. littorea. Defence levels returned to preinduction levels within 2 weeks. Similar to the work of Pavia and Toth (2000a) and Toth and Pavia (2000b), this demonstrates defence induction by waterborne cues and that the specific herbivore involved significantly aVects the specific algal response. However, there are important diVerences between results and interpretations in the two sets of
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studies. The two macroalgal species are in the same family (Fucaceae) and the snails and isopods are congeners. However, only the snails induced defences in Ascophyllum nodosum while both herbivores did with F. vesiculosus, and snail grazing resulted in waterborne cues with A. nodosum but not F. vesiculosus, even though isopod grazing did result in waterborne cues from F. vesiculosus. Pavia and Toth (2000a) hypothesised that diVerences between responses to the two herbivores by A. nodosum could be due to the snails being much less motile predators than the isopods. They reasoned that the isopods do not remain on an individual alga long enough for an induced response to be eVective. With respect to the responses of F. vesiculosus, Rohde et al. (2004) noted the same diVerences in relative mobility between the herbivores, but suggested that this reduced selection for a waterborne signal for the snails because a single animal remains on an individual alga for relatively long periods of time. The more mobile isopods, however, move more readily between neighboring algae, making an ability to sense and respond to grazed neighbors more adaptive. These are diVerent species at diVerent geographic locations, and these two sets of interpretations need not be mutually exclusive. However, the somewhat reversed reasoning applied in the two sets of circumstances does highlight the fact that we are far from truly understanding the mechanistic or selective relevance of the herbivore‐specific nature of induced defence responses. Pavia’s research group combined their studies of defence induction in Ascophyllum nodosum with their tests of ODT (Pavia et al., 2002; cf. Section IV.A) to extend ODT predictions on within‐thallus variation in constitutive levels of defensive allocation to within‐thallus variation in defence induction. Toth et al. (2005) reported that even though basal stipes, with a higher assigned fitness value, had significantly higher constitutive levels of phlorotannins than lower fitness value apical shoots, and even though both did significantly induce phlorotannin production when grazed by I. obtusata, phlorotannin induction was significantly greater in the more valuable basal stipes. Although feeding deterrence was not measured in this study to correlate with the phlorotannin levels, snails fed basal stipes had lower fecundity than those fed apical shoots, which was significantly more pronounced in snails fed previously grazed algal thalli, indicating that diVerences in within‐thallus defences and their induction in the macroalgae impacted herbivore fitness. Taylor et al. (2002) also combined tests of the ODT and IDM in a comparison of constitutive and induced responses to amphipod herbivory in the fucoid Sargassum filipendula. As noted earlier, the lower stipes, which were judged highest in fitness value, were constitutively defended via physical toughness rather than chemistry. However, in the intermediate valuable upper stipes, which contained the meristems,
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herbivory did induce chemical defence, whereas both upper and lower blades were defended neither physically nor chemically. The most valuable tissues were defended constitutively, the intermediate valuable tissues only when under herbivore attack, and the more readily replaceable tissues not at all, even though some of them are immediately adjacent to the induced upper stipes in the algal thallus. Sotka et al. (2002) confirmed the tissue‐specific nature of the induced response and showed that waterborne cues from neighboring macroalgae did not induce defences in ungrazed thalli. Hemmi et al. (2004) also employed an experimental design that allowed them to test for the spread of an induced response within macroalgal thalli. Mechanical clipping of the fucoid Fucus vesiculosus induced chemical defences measured as decreased palatability to the isopod Idotea baltica, but the induction was very localised and did not spread either laterally or vertically within individual thalli. In addition, the induced responses were relatively short‐lived, lasting more than 10 but less than 38 days. Hemmi et al. (2004) suggested that such a localised and short‐lived response may have little eVect on overall‐thallus defences but might serve to disperse grazing damage within a thallus, thereby decreasing the likelihood of thallus breakage. In these same experiments, nutrient levels were also manipulated and although they did aVect phlorotannin production (see Sections II.F.2.b and IV.C), the phlorotannin levels were not correlated with palatability to I. baltica. Although the experimental design used by these investigators might not have been able to detect the transport of a chemical inducer from younger to older tissues if such a signal was confined to the thallus side on which the wound occurred, it is significant that the design should have detected transport from older tissues towards the apical meristems, the direction in which translocation of photosynthate and ions have been reported in F. vesiculosus (Diouris and Floc’h, 1984; Floc’h, 1982). Borell et al. (2004) confirmed Pavia and Toth’s (2000a) observations on induction of Ascophyllum nodosum (Order Fucales) defences by Littorina obtusata, although they also observed a significant eVect of mechanical clipping on A. nodosum palatability in one of two experimental trials. They utilised this system as a test of the herbivore motility model proposed previously for interactions of terrestrial plants and their insect herbivores (Coleman et al., 1996; Edwards and Wratten, 1987). Consistent with this model, L. obtusata spent more time grazing on the less defended primary and annual shoots compared to the more defended stipes. Feeding damage on thalli with previously induced defences was more diVuse than in uninduced controls, the feeding scars were smaller in previously induced thalli, and total consumption was lower in previously induced thalli.
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Induction of chemical defences has also been examined in Dictyotales, Laminariales, and Desmarestiales. In an intensive study combining field manipulations of amphipod grazing with chemical determinations and feeding bioassays of macroalgae from sites that naturally diVered in grazing pressure in some years but not others, Cronin and Hay (1996c) documented induction of chemical defences in Dictyota menstrualis (Order Dictyotales). Macroalgae from a site that 1 year had higher densities of amphipods than two other sites were less palatable and had higher levels of the defensive compounds dictyol E, pachyodictyol A (Fig. 6), and dictyodial (Fig. 8; cf. Section III.A). In a second year, the amphipod densities at these three sites did not diVer and neither did the palatability nor defensive compound concentrations of the D. menstrualis from them. In a third year, there were diVerences between sites but they were smaller than the first year and although there were small but significantly higher levels of the compounds at the site with higher amphipod densities, there was no significant diVerence in palatability of the macroalgal thalli. Within the individual sites, thalli that had amphipod grazing scars were less palatable and had higher levels of defensive compounds. The induction of these responses was confirmed with manipulative studies placing algae in cages with or without amphipods in the field. In other dictyotalean algae, Peckol and Yates (1997) documented increases in phlorotannin contents after simulated grazing in Lobophora variegata and Padina sanctae‐crucis, although potential changes in palatability were not assayed. Weidner et al. (2004) reported an induction of chemical defences in L. variegata after amphipod grazing measured as decreased palatability in extracts prepared using only a very nonpolar solvent. However, this unpalatability was not observed in intact thallus, indicating that multiple changes had occurred, which on balance did not decrease thallus palatability. Macaya et al. (2005) reported a similar result with Glossophora kunthii (Order Dictyotales), where artificial foods containing nonpolar extracts of algae previously grazed by amphipods were deterrent compared to foods containing extracts from control algae, but there was no diVerence between the palatability of the corresponding fresh thalli. However, they went on to demonstrate that defences eVective in intact thalli were restricted to the apical (meristematic area) and basal (stipe and holdfast) regions of the thalli and suggested that the lack of an induction response in intact thalli was probably because the amphipods simply shifted feeding from the defended apical and basal regions to the undefended tissues in between (Macaya et al., 2005). In addition, these authors reported that the induction response seen in extract containing artificial foods could be elicited both by the mere presence
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of amphipods in water upstream of the thalli or by the presence of amphipods grazing on conspecific algae upstream of the thalli. This indicates that the presence of waterborne cues is involved in stimulating the induced response and suggests that the cues come from the amphipods alone and not from algae in the process of being grazed. In all cases, the diVerence in palatability between extracts of induced and control algae disappeared within 12 days of removing the amphipod grazers (Macaya et al., 2005). Rotha¨ usler et al. (2005) reported similar results using the same amphipod species, but defences were not induced by another amphipod species or by sea urchins (although the experimental design as described apparently did not include autogenic controls; cf. Peterson and Renaud, 1989). In Laminariales, induction of phlorotannins in response to simulated grazing has been reported in Agarum fimbriatum, Hedophyllum sessile, Laminaria complanata, L. groenlandica, and Pleurophycus gardneri (Hammerstrom et al., 1998) and in Ecklonia radiata (Lu¨ der and Clayton, 2004), although palatability changes were not assayed in either study. Toth and Pavia (2002a) tested for phlorotannin induction in Laminaria hyperborea in response to grazing by limpets and snails and observed a decrease in phlorotannins after grazing, which they suggested could have been due to a loss of physode‐rich epidermal layers or to compensatory thallus growth. Macaya et al. (2005) reported no induction of defences in Macrocystis integrifolia in experiments performed in parallel with those described earlier using Glossophora kunthii. Rotha¨ usler et al. (2005) reported decreased palatability of previously grazed Lessonia nigrescens compared to controls in one amphipod species but not in another amphipod or sea urchin species using bioassays apparently lacking autogenic controls. The only study we are aware of looking for defence induction in the Desmarestiales is our own group’s work. We tested for changes in palatability or phlorotannin concentrations in Desmarestia menziesii after grazing by two species of amphipods, a snail species, and mechanical wounding, and we observed no eVect of any of these treatments (V. A. Fairhead, C. D. Amsler, J. B. McClintock, and B. J. Baker, unpublished results). C. CARBON‐NUTRIENT BALANCE AND RESOURCE ALLOCATION
The carbon‐nutrient balance hypothesis (CNBH) predicts that because they have a relative excess of fixed carbon, nitrogen‐limited plants should produce compounds such as phenolics and terpenes that do not contain nitrogen as defensive secondary metabolites and that they should produce more of these compounds as nitrogen limitation increases relative to light (and, therefore, carbon fixation) availability (Bryant et al., 1983). Conversely, the
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CNBH predicts that light‐limited (i.e., carbon‐limited) plants should utilise nitrogen‐containing defences such as alkaloids and cyclic peptides, which are often eVective at much lower concentrations than phenolics or terpenes. The CNBH addresses intraspecific diVerences in defences on ecological timescales, whereas the closely related resource allocation model (RAM) makes similar predictions about defensive compound variation between species over evolutionary timescales (Coley et al., 1985). RAM also predicts that species that evolved in growth‐limiting environments should produce relatively high levels of defensive metabolites because replacing tissue lost to herbivory should be more costly than in more growth‐permissive habitats. A number of investigations of brown macroalgae have tested predictions of the CNBH but almost no studies have attempted to extend RAM predictions to brown or other macroalgae. The most common aspect of CNBH tested with brown macroalgae has been the prediction that nutrient limitation would increase the concentration of phenolics or terpenes (or, conversely, that nutrient enhancement would result in decreased levels). This has usually proven true with phlorotannins, including in studies of the Fucales (Hemmi et al., 2004; Jormalainen et al., 2003; Pavia and Toth, 2000b; Pavia et al., 1999b; Peckol et al., 1996; Tuomi et al., 1989; Van Alstyne and Pelletreau, 2000; Yates and Peckol, 1993), the Laminariales (Hurd et al., 2000), and the Dictyotales (Arnold et al., 1995). However, this has not always been true for phlorotannins in some species of the Dictyotales (Peckol and Yates, 1997), Laminariales (Pfister and Van Alstyne, 2003), or Fucales (Cronin and Hay, 1996a; Pavia and Brock, 2000; Pavia and Toth, 2000b), although increased irradiance did increase phlorotannin concentrations in Sargassum filipendula (Order Fucales; Cronin and Hay, 1996a). The CNBH prediction of a link between nutrients and defences did not hold for the one study testing it with terpenes in the Dictyotales (Cronin and Hay, 1996a) (it also did not predict terpene concentrations in red macroalgae; Puglisi and Paul, 1997). In a unique study, Jormalainen et al. (2003) attributed phlorotannin increases in Fucus vesiculosus in response to grazing by the snail Theodoxus fluviatilis to the removal of hyaline hairs that are likely involved in nutrient uptake, as these were the only parts of the macroalgal thallus consumed. Most of the studies of CNBH predictions of phlorotannin levels did not also examine the influence of them on palatability, so it is particularly significant that two investigations that did incorporate palatability assays reported that increased phlorotannin levels caused by the manipulation of nutrients or light did not result in decreases in palatability (Cronin and Hay, 1996a; Hemmi et al., 2004). Overall, as Cronin (2001) has discussed, the CNBH predicts responses of macroalgae in some instances but not others. In addition, the CNBH has
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recently come under attack in the terrestrial plant literature. Hamilton et al. (2001) reviewed a large number of terrestrial tests of the CNBH and concluded that although it sometimes correctly predicts plant responses to the environment, it is incorrect so often that in their opinion the CNBH is of no use as a predictive model and should be abandoned. This conclusion has been echoed by Koricheva (2002) and Nitao et al. (2002) but refuted by Lerdau and Coley (2002). The number of reports testing CNBH predictions in macroalgae is too low for such a definitive conclusion. However, the mixed results to date in macroalgae, coupled with the much larger terrestrial data base, suggest that the CNBH should be applied with great caution, if at all, as a predictive model for macroalgal responses to the environment. As Cronin (2001) has discussed, the RAM has rarely if ever been tested explicitly with macroalgae, probably because the conditions necessary to do so are usually lacking in marine communities. Based on gross generalisations of extremes in the variation of algal growth rates across taxa and of defensive metabolites across latitudes, Cronin (2001) concluded that the overall evidence from a combination of previous studies (that did not specifically intend to address RAM) was not consistent with RAM predictions. Although that could serve as a useful starting point for directed investigations, the vast generalisations underlying the conclusion should make it nothing more than a starting point. With respect to one aspect of RAM not addressed by Cronin (2001), our research group has been able to test the prediction that carbon‐limited macroalgae should selectively produce nitrogen‐containing secondary metabolites, which are often bioactive at much lower concentrations than nonnitrogenous compounds and, therefore, require a lower total carbon investment. Macroalgae in general produce relatively few nitrogenous secondary metabolites (e.g., Harper et al., 2001; Paul et al., 2001). Several authors have suggested that this is because nitrogen is so commonly growth limiting for macroalgae in the ocean that there has been little selection across broad spatial or temporal scales for an investment of nitrogen in defences (Cronin, 2001; Hay and Fenical, 1988; Hay and Steinberg, 1992). However, one place in the world where this is not true is in coastal waters of Antarctica, where nitrogen and other nutrients rarely if ever limit macroalgal growth and where most macroalgae have very low C:N ratios (Dunton, 2001; Peters et al., 2005; Weykam et al., 1996). We tested the RAM prediction that Antarctic macroalgae should commonly produce nitrogenous secondary metabolites using an extraction and chemical staining protocol specifically targeting such compounds in 24 macroalgal species, including eight ecologically dominant brown algal species (Amsler et al., 2005). Coupling this with standard extractions and a literature search, we found no evidence at all of nitrogenous compounds (Amsler et al., 2005). Although this does not mean that
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nitrogen‐containing defences do not exist in Antarctic macroalgae, it does indicate that, in contradiction to RAM‐based predictions, they are likely no more common than in macroalgae from lower latitudes. D. TESTS OF MULTIPLE AND OTHER THEORIES
Although we have chosen to categorise tests of chemical defence theories in the preceding sections by individual theory, the selective factors presumably driving them in nature certainly do not work in isolation, and a number of authors have examined some of these ideas in combination. Studies combining tests of IDM and CNBH have been particularly common (Hemmi et al., 2004; Jormalainen et al., 2003; Pavia and Brock, 2000; Peckol and Yates, 1997; Peckol et al., 1996; Weidner et al., 2004; Yates and Peckol, 1993). IDM has also been explored in combination with UV radiation stress (cf. Section II.D.4; Macaya et al., 2005; Pavia and Brock, 2000; Pavia et al., 1997). Two theories that make somewhat conflicting predictions are the ODT and the growth‐diVerentiation balance hypothesis (GDBH). GDBH addresses diVerential allocation of defences during growth and subsequent diVerentiation, with the production of defences viewed as part of the process of diVerentiation (Herms and Mattson, 1992). One prediction of the GDBH is that newly produced cells, such as those at and near meristems, should be less defended than older, more diVerentiated cells further from meristems. This is opposite the predictions of ODT, as noted earlier in Section IV.A. Both Cronin and Hay (1996b) and Van Alstyne et al. (1999a) compared and contrasted these predictions (their results are detailed in Section IV.A) with the results of Van Alstyne et al. (1999a) not supporting GDBH in most respects, but the results of Cronin and Hay (1996b) being a better fit with GDBH than ODT. As also noted in Section IV.A, these latter authors suggested that the diVerence could be because they were working with algae from a genus (Dictyota) lacking a known internal translocation mechanism that might be used to transport defensive compounds into young tissues in other macroalgal taxa. There are several other chemical defence theories (cf. Cronin, 2001; Stamp, 2003), but to our knowledge, most have not been tested explicitly using brown algae. One exception is the prediction that stressed organisms would be able to devote fewer resources to defence and, therefore, be more palatable than unstressed individuals (Rhoades, 1985). Renaud et al. (1990) reported that desiccation resulted in the normally unpalatable alga Padina gymnospora (Order Dictyotales) becoming more palatable to sea urchins, although a normally palatable sympatric red alga examined in the same study became less so. Cronin and Hay (1996d) reported that desiccation of Dictyota ciliolata (Dictyotales) also reduced the levels of specific defensive
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metabolites (pachydictol A, dictyol B acetate, and dictyodiol; Figs. 6 and 8) and reduced feeding deterrence in bioassays using sea urchins and amphipods. In addition, UV stress decreased levels of the defensive metabolites, suggesting that palatability would have decreased too, but palatability assays were not performed on the UV‐treated algae (Cronin and Hay, 1996d). UV stress reportedly had no influence on the palatability of either Glossophora kunthii (Order Dictyotales) or Macrocystis integrifolia (Order Laminariales) (Macaya et al., 2005).
V. NONPHLOROTANNIN DEFENCES AGAINST BACTERIA, FOULING ORGANISMS, AND PATHOGENS There have been far fewer ecologically relevant reports of antiepiphytic‐ bacteria or antifouling chemical defences of brown algae (or of other macroalgae) compared to reports of antiherbivore defences, even though there have been many studies looking at the antibacterial or antifouling bioactivity of algal extracts. The reason for this discrepancy is that it is relatively diYcult to demonstrate that observed bioactivities against epiphytic bacteria or fouling organisms in vitro actually have ecological relevance. Many authors, ourselves included, have performed bioassays on extracts or purified compounds from marine organisms at concentrations somehow equivalent to those present in the intact organism, and some studies (e.g., da Gama et al., 2002; Henrikson and Pawlik, 1995) have outplanted gels containing such extracts into the sea to test their eVectiveness in preventing fouling. Those are valuable and important as first steps, but to make a strong case for ecological relevance one must also show that the compounds are present at the surface of the organism or in the boundary layer overlying that surface at bioactive concentrations (Steinberg and de Nys, 2002; Steinberg et al., 2001). Bhadury and Wright (2004) reviewed studies of in vitro antibacterial and antifouling activity in marine algae, including 25 brown algal species in the orders Ectocarpales, Scytosiphonales, Chordariales, Dictyotales, Fucales, Laminariales, and Desmarestiales. Other than to update this by listing several more recent reports on brown algae not included in that review (Amsler et al., 2005b; Freile‐Pelegrin and Morales, 2004; Hellio et al., 2004; Mare´ chal et al., 2004), with the exception of part of the discussion earlier concerning potential eVects of phlorotannins (Section II.D.3), this review concentrates on the few studies where chemical defences are very well supported in an ecological context. The only very clear case of nonphlorotannin brown algal secondary metabolites acting as antifoulants in nature that we are aware of is in
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Dictyota menstrualis (Order Dictyotales). Schmitt et al. (1995) reported that D. menstrualis was noticeably less fouled in nature than other macroalgae and that bryozoan larvae would not settle on D. menstrualis in laboratory bioassays even though they would contact its surface and would settle on several other species of brown and red macroalgae. Extracts of surface rubbings of the algal thallus contained pachydictyol A and dictyol E (Fig. 6; also know to be antiherbivore defences; Section III.A). These surface‐rubbing extracts could prevent fouling when coated onto a settlement substrate, although the rubbings were too small to allow the levels of the compounds to be quantified accurately. Dictyol E was toxic to the larvae when presented in solution, and although pachydictyol A in solution was not toxic, it caused abnormal and delayed development (Schmitt et al., 1995). Neither of the assays with compounds in solution is directly ecologically relevant, but this was the only way to approach the question experimentally, as the larvae would not contact a surface coated with the compounds. Because the compounds were detected at the thallus surface, the assays do demonstrate that there could be adverse consequences to the larvae if they settled on D. menstrualis. Schmitt et al. (1998) extended the examination of the eVects of metabolites in solution on larval development and survival to dictyol B acetate (Fig. 6) and dictyodiol (Fig. 8) and to the larvae of an additional bryozoan species, as well as a hydroid species. It is easier for in vitro assays of defences against potential pathogens to be made ecologically relevant because pathogens do invade the host tissues and often the host cells, so needing to know the actual surface concentrations of defensive compounds is not an impediment. Kubanek et al. (2003) reported that crude extracts of Lobophora variegata (Order Dictyotales) from the Bahamas have particularly strong antifungal bioactivity and identified the cyclic lactone lobophorolide (Fig. 8) as a defensive compound with significant bioactivity at exceptionally low concentrations against both pathogenic and saprophytic sympatric fungi. Although L. variegata from 46 of 51 samples collected at 10 sites in the Bahamas contained measurable, bioactive concentrations of lobophorolide, it was not present in two collections from the Red Sea even though crude extracts of the Red Sea algae did have antifungal bioactivity. This indicates that although L. variegata from diVerent regions may be chemically defended against pathogens, the same specific compounds may not be involved. Although the vast majority of the investigations into the defensive chemical ecology of macroalgae have focused on roles of secondary metabolites, recent work has demonstrated that both red and brown algae employ oxidative burst defences against pathogens, a defensive mechanism that has been recognised in terrestrial plants for a number of years (reviewed
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by Lamb and Dixon, 1997; Mahalingam and FedoroV, 2003; Wojtaszek, 1997). This was first discovered in red algae, where cell wall degradation products elicit a rapid release of H2O2 that is toxic to epiphytic bacteria (Weinberger et al., 1999, 2000, 2001). Ku¨pper et al. (2001) demonstrated an analogous response in Laminaria digitata (Order Laminariales) that produces a rapid oxidative burst of H2O2 and O2– in response to oligomeric degradation products of alginate (a major cell wall component of L. digitata and other brown algae). Ku¨ pper et al. (2001) also reported that H2O2 concentrations in the range released by the algae were toxic to pathogenic, alginate‐degrading bacteria and, using histological techniques, demonstrated that the response was confined primarily to the meristoderm. These authors also began to dissect the underlying physiological mechanisms and showed that at least some of the mechanisms are likely conserved within the oxidative burst responses of algae, terrestrial plants, and animals. Ku¨pper et al. (2002) surveyed 45 species of brown algae from 11 orders for constitutive vs. induced production of H2O2. They reported that oxidative bursts in response to alginate oligomers were common in sporophytes in Laminariales and Desmarestiales but not in their filamentous gametophyte stages. One species (Pylaiella littoralis) from the Ectocarpales had an oxidative burst response but 10 other ectocarpalean species did not. Members of the Fucales had high constitutive production of H2O2 but most did not produce additional H2O2 in response to alginate oligomers. Ku¨ pper et al. (2002) also reported that axenic sporophytes of Macrocystis pyrifera (Order Laminariales) were infected rapidly by pathogenic bacteria when the oxidative burst response was blocked with an NAD(P)H oxidase inhibitor but not in controls and that when non‐axenic M. pyrifera or L. digitata sporophytes were treated with the inhibitor, they were attacked rapidly by their natural bacterial flora. These authors also demonstrated that the oxidative burst response is important in resistance of both M. pyrifera and L. digitata to the pathogenic brown algal endophytes Laminariocolax tomentosoides and Laminariocolax macrocystis, although the response took 7 days to occur and likely involves elicitation of other structural or chemical defences (Ku¨ pper et al., 2002).
VI. VOLATILE HALOGENATED ORGANIC COMPOUNDS An additional response that might be defensive against pathogens, biofoulers, and/or herbivores is the release of volatile halogenated organic compounds
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(VHOCs), such as bromoform, dibromomethane, dibromochloromethane, bromodichloromethane, and chloroiodomethane. That brown algae release these compounds is clear (e.g., Gschwend et al., 1985; Laturnus, 1996, 2001; Laturnus et al., 1996; Manley et al., 1992), but to our knowledge, with the exception of one report on antiepiphyte activity in a coralline red alga (Ohsawa et al., 2001), there is no published evidence of any ecological role for them even though they have been thought to potentially be defensive (e.g., Borchardt et al., 2001; Fenical, 1975; Laturnus et al., 1996) and they have received significant attention because they impact atmospheric processes (e.g., Broadgate et al., 2004; Carpenter et al., 2000; Steinke et al., 2002). It has been suggested that VHOC production is related to the oxidative burst defence mechanism in algae (Abrahamsson et al., 2003; Potin et al., 1999, 2002), and the enzymes responsible for VHOC production (e.g., bromoperoxidases; cf. Colin et al., 2003, 2005) have been shown to be involved in cross‐linking phlorotannins in cell walls (Berglin et al., 2004), which could certainly be involved in responses to damage by grazers or pathogens. A deeper understanding of the ecological and physiological roles of VHOCs in brown and other macroalgae remains an important goal. Relatively high levels of VHOC release have been reported from brown algae in Antarctica (Laturnus, 1995, 2001; Laturnus et al., 1996, 1997). Our research group performed feeding bioassays with bromoform, the most abundant VHOC identified previously from Antarctic macroalgae (Laturnus, 1995; Laturnus et al., 1996) using a common, herbivorous Antarctic amphipod, Gondogeneia antarctica. We observed statistically significant decreases in feeding when bromoform was added to artificial foods at initial concentrations of 3 ppm and above (final concentrations in the foods were likely to have been lower but these were not measured; C. D. Amsler, B. J. Baker, and J. B. McClintock, unpublished result). This suggests that bromoform or other VHOCs could function as feeding deterrents if they were produced in such concentrations. However, we were unable to identify bromoform or a number of other VHOCs using gas chromatography from water samples taken in situ within dense beds of Antarctic brown algae or within pieces of intact or mechanically diced brown algal thalli (B. J. Baker, C. D. Amsler, and J. B. McClintock, unpublished result). The level of detection was orders of magnitude below the concentrations with bioactivity against amphipods (even accounting for loss during artificial food preparation) so we concluded that it was unlikely that VHOCs play a role as defences against amphipod herbivory in this system.
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VII. SENSORY CHEMICAL ECOLOGY Brown macroalgae reproduce primarily via motile spores and gametes, and the chemosensory abilities of some of these motile cells appear to be very important, even though nonmotile spores and female gametes are produced by some groups (Graham and Wilcox, 2000) and at least several species or populations reproduce and are dispersed via vegetative means (e.g., Amsler, 1984; Keum et al., 2003). Usually these motile cells are heterokont. Heterokont cells are biflagellate, possessing an anterior flagellum that bears mastigonemes (stiV hairs) that enable these forward‐projecting flagella to pull the cells through the water, and they have a trailing, smooth posterior flagellum (Cahill et al., 1996; Geller and Mu¨ller, 1981; Graham and Wilcox, 2000). Although the sensory chemical ecology of brown algae has received less research attention than brown algal chemical defences, recognition that sensory abilities are present in male gametes long predates studies of defensive chemical ecology and, more recently, limited attention has been focused on the chemosensory abilities of brown algal spores. A. CHEMOATTRACTION TO PHEROMONES
Motile brown algal male gametes (termed spermatozoids in oogamous species) from a wide variety of taxa locate female gametes via pheromones secreted by the female gametes. This behavioural response has been known since the independent work of Thuret and Pringsheim on Fucus (Order Fucales) in the 1850s and of Berhold and Oltmanns on Ectocarpus (Order Ectocarpales) and Kuckuck on Cutleria (Order Cutleriales) in the 1890s (reviewed by Fritsch, 1945; Maier, 1995; Maier and Mu¨ ller, 1986), although it was not until the 1960s that the specific chemicals responsible for the observed chemoattraction began to be identified (Mu¨ ller, 1967, 1968). At present, 12 specific pheromones (Fig. 9) are known to be released by eggs or settled, previously motile female gametes from over 60 species in 13 orders, with most species releasing more than one of the pheromones in addition to some of their biosynthetic precursors (Maier, 1995; Pohnert and Boland, 2002). The eVective distance at which male gametes could possibly perceive the pheromone signals has been estimated as between less than half a millimeter and one or a few millimeters (Boland et al., 1982, 1983; Maier and Mu¨ ller, 1986; Mu¨ ller, 1981), although that distance is likely to decrease with increasing water motion (Gordon and Brawley, 2004). A majority of the recent attention in this area has focused on the biosynthetic pathways and other biochemical aspects of pheromone production and reception (reviewed by Boland, 1995; Maier, 1995; Pohnert and Boland, 2002), and a
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Chemical structures of brown algal pheromones.
number of partial and comprehensive reviews are available (in particular, Maier, 1995) that describe the chemosensory behaviours, methodology, and evolutionary relationships in great detail (see also Amsler and Iken, 2001; Maier, 1993; Maier and Mu¨ ller, 1986; Mu¨ ller, 1989). Consequently, here we present only a selective overview of pheromone‐related behaviours. In the Laminariales, Desmarestiales, and Sporochnales, pheromones act not only as chemoattractants, but also stimulate the release of male gametes from antheridia (Mu¨ ller et al., 1979, 1982, 1988). In Laminaria digitata (Order Laminariales), the threshold concentration of the pheromone lamoxirene
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Fig. 10. A dark‐field, microflash photomicrography sequence showing mass release and chemotaxis of Laminaria digitata spermatozoa in response to the pheromone lamoxirene. Lamoxirine adsorbed onto a porous glass (Spherosil) particle (*) was placed near a fertile clump of filamentous male gametophytes ( ) at time 0, and the response of spermatozoa at 5, 60, 120, and 180 s thereafter is shown. Small white dots are the dark‐field images of spermatozoa. From Maier (1982).
(Fig. 9), necessary to induce spermatozoid release, is below 1010 M (Maier et al., 1988). Spermatozoid release in response to the pheromone is very rapid (Fig. 10; Maier, 1982) and the gametes swim directly towards the pheromone source (Fig. 10; Maier, 1982; Maier and Mu¨ller, 1990). Because the cells orient their swimming such that they move directly towards the source, this is a true chemotactic behaviour (cf. Amsler and Iken, 2001). In addition to the direct chemotaxis, the spermatozoids exhibit a phobic, near – 1808 turn when the concentration of the lamoxirene is decreasing, resulting in a turn back to the general direction of the source (Maier and Mu¨ ller, 1990).
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In Fucus spiralis (Order Fucales), the spermatozoids appear to rely only on a near 1808 turn, phobic responses to decreasing concentrations of the pheromone, fucoserratene (Fig. 9), in order to remain in the vicinity of a released female gamete (Maier and Mu¨ller, 1986). Spermatozoids of the Australasian fucoid Hormosira banksii also display a phobic response to decreasing concentrations of the pheromone homosirene (Fig. 9), but in addition decrease their frequency of turning as homosirene concentration increases (at high concentrations their swimming pattern is superficially, but not mechanistically, similar to those of the damaged spores illustrated in Fig. 11E) (Maier et al., 1992). Chemoattractive responses such as these that rely on modulation of turning frequency and/or swimming speed are properly referred to as chemokinetic rather than chemotactic responses, with the latter being reserved for behaviours that involve movement directly towards or away from a stimulant source (Amsler and Iken, 2001; Dusenbery, 1992; Fraenkel and Gunn, 1961).
Fig. 11. Swimming patterns of Hincksia irregularis spores tracked by computer‐ assisted motion analysis: (A) straight path type characteristic of a majority of spores within 10–20 minutes after release; (B) search circle path type found in 30–40% of spores during the first 50 min after release; (C) orientation behaviour found in approximately 30% of spores between 40 and 60 min after release; (D) gyration behaviour that precedes settlement, first appearing after approximately 40 min and observed in 34% of spores by 60 min after release; and (E) wobbling behaviour observed occasionally (0–6%) in cells of any age and apparently caused by cell damage. From Iken et al. (2001).
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Perhaps the most thoroughly studied chemoattractive behaviour of brown algal gametes is the chemokinetic attraction of Ectocarpus siliculosus (Order Ectocarpales) to the pheromones ectocarpene (Fig. 9) and, as has been discovered recently (Pohnert and Boland, 2002), preectocarpene (Fig. 9). E. siliculosus is morphologically isogamous but functionally oogamous, as the female gamete settles and begins to secrete pheromones within 30 min of release from the gametangia (Mu¨ ller, 1989). Male gametes respond in four ways (Maier, 1995; Maier and Calenberg, 1994; Mu¨ ller, 1989). They already display a preference to remain close to solid surfaces (a thigmotactic response), which increases in the presence of pheromones. They also decrease their swimming speed (an orthokinetic response) and increase their rate of turning (a klinokinetic response) as pheromone concentrations increase. Mu¨ ller (1978) termed this behaviour ‘‘chemo‐thigmo‐klinokinesis.’’ In addition, the gametes exhibit a phobic response to decreasing pheromone concentrations similar to those described earlier in Laminaria and Fucus (Maier and Calenberg, 1994). The turns made by E. siliculosus gametes are initiated by sharp, sideways beats of their short, rudder‐like posterior flagella (Geller and Mu¨ ller, 1981). The posterior flagella probably play a similar role in other taxa, although they are often longer and probably also have a direct role in locomotion (Maier, 1995). However, a posterior flagellum is not absolutely required in male gametes, as demonstrated by members of the Dictyotales, which are able to respond to the pheromones dictyotene or multifidene (Fig. 9), but which produce only a single anterior, mastagoneme‐bearing flagellum (e.g., Phillips et al., 1990a,b). The observations that female gametes of most species produce multiple pheromones (even though their male gametes may not respond to all of them) and that adult, vegetative tissues sometimes produce pheromones have led to speculation that these pheromones could potentially have allelopathic roles. Mu¨ ller (1981) suggested that pheromones could potentially be used to ‘‘misguide’’ male gametes of a competitor, thereby preventing them from reaching conspecific female gametes and producing viable zygotes. Amsler et al. (1992) noted that observations of diVerential patterns of kelp recruitment following simultaneous spore settlement in nature (Reed, 1990) would, hypothetically at least, be consistent with a hypothesis that early maturing Pterygophora californica female gametophytes stimulate premature release of spermatozoa from Macrocystis pyrifera, thereby limiting the supply of M. pyrifera spermatozoa when M. pyrifera female gametophytes become mature. Boland et al. (1983) suggested six hypothetical scenarios by which a brown algal species might interfere with the pheromone‐mediated communication of a competitor. Their data on pheromone production and relative sensitivity in Ectocarpus siliculosus (Order Ectocarpales) and
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Cutleria multifida (Order Cutleriales) suggested that E. siliculosus should have a competitive advantage in nature. This surprised the authors (Boland et al., 1983), as it has long been presumed that the morphologically simple members of the Ectocarpales represent the most primitive members of the Phaeophyceae and they would have predicted that the more ‘‘advanced’’ species would have the competitive advantage. However, recent evidence has indicated that the Ectocarpales may in fact be among the most derived brown algae (Cho et al., 2004; Draisma et al., 2001) regardless of their simple morphology. Boland et al. (1983) also speculated that pheromones produced by vegetative tissues in Dictyopteris spp. (Order Dictyotales; cf. Section III.A) might interfere with reproduction in competitors or epiphytes, an idea echoed by Maier and Mu¨ ller (1986). B. BEHAVIOUR AND SENSORY CAPABILITIES OF SPORES
Considering the range of chemokinetic and chemotactic responses that brown algal gametes can exhibit in response to pheromones, it should not be surprising that other motile life history phases of brown algae can also sense and respond behaviourally to their chemical microenvironments. However, there has been much less attention focused on the behaviours of these other stages, which include both asexual spores produced by mitosis and spores produced by meiosis as part of a sexual life history (meiospores). Either class of spores can, when motile, be referred to as zoospores. To our knowledge, the only reports of chemosensory behaviours in brown algal zoospores are in members of the Laminariales and Ectocarpales. Chemosensory behaviours have been reported in meiospores from three species of kelps (Order Laminariales): Macrocystis pyrifera and Pterygophora californica from California (Amsler and Neushul, 1989, 1990) and Laminaria japonica from Japan (Fukuhara et al., 2002). Spores of all three species are attracted by nitrate, although M. pyrifera and P. californica are more sensitive to it as they were attracted by 10 M nitrate (Amsler and Neushul, 1989), whereas L. japonica spores did not respond to 11 M nitrate (but did to 200 M, the next highest concentration tested; Fukuhara et al., 2002). Based on manual video observations of P. californica swimming in a nitrate gradient (Amsler and Neushul, 1989), the chemoattractive behaviour in these species has been described as a true chemotactic response. However, a more detailed, quantitative behavioural analysis, such as those conducted by Amsler et al. (1999) and Iken et al. (2001), is needed to confirm this. M. pyrifera spores were not attracted by phosphate, but both P. californica and L. japonica spores were (Amsler and Neushul, 1989; Fukuhara et al., 2002). Again though, the L. japonica spores were much less sensitive than
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P. californica. L. japonica was attracted by 100 M phosphate but not by concentrations of 9.7 M and below, whereas P. californica was significantly attracted by 2 M phosphate (Amsler and Neushul, 1989; Fukuhara et al., 2002). In addition, both M. pyrifera and P. californica were attracted by ammonia (low concentrations) and boron while neither species responded to zinc. Manganese attracted M. pyrifera spores but repelled P. californica spores at the same concentration (18 M). Cobalt attracted M. pyrifera spores but had no aVect with those of P. californica. Glycine, aspartate, and iodine all significantly attracted M. pyrifera but were not tested with P. californica (Amsler and Neushul, 1989). Perhaps the most interesting responses were those of M. pyrifera spores to various concentrations of ammonia and ferrous iron. The spores were attracted by ammonia concentrations at and below 90 M and by 1 M Fe2þ but were repelled by 1000 M ammonia and by 45 M Fe2þ (Amsler and Neushul, 1989). The concentrations of ammonia that attracted the spores are likely to be stimulatory for growth and 1 M Fe2þ is stimulatory for reproduction in the gametophyte generation into which the spores germinate. Conversely, the higher concentrations are likely to be inhibitory for growth and reproduction, respectively (references in Amsler and Neushul, 1989). The gametophyte generation that the spores develop into is an obligate stage of the kelp life history (Graham and Wilcox, 2000). It is also microscopic and so must be able to grow to reproductive maturity in the microenvironment that the spore settles in. Although spores themselves presumably have no need for nutrients (because they do not grow or reproduce until they have germinated), chemotaxis towards nutrients when present in beneficial concentrations and away from them at detrimental concentrations is probably adaptive by increasing the chances that the gametophyte will develop in a permissive microenvironment for growth and gametogenesis. Kelp spores can also respond to nutrients by increasing their rate of settlement. Macrocystis pyrifera spore settlement rates are increased significantly by at least some concentrations of ammonia, nitrate, glycine, phosphate, manganese, boron, and both ferrous and ferric iron (Amsler and Neushul, 1990). Although the responses of Pterygophora californica spores to specific nutrients were not examined, their settlement was increased by a macro‐ and micronutrient mixture (Amsler and Neushul, 1990). Nutrient stimulation of spore settlement is probably like spore chemotaxis to nutrients in making it more likely that a spore will settle in a microenvironment conducive to gametophytic growth and reproduction. However, they appear to be mechanistically distinct. The settlement stimulation response is not present for at least several hours after spores are released even though newly released spores are chemotactic. There are also diVerences in the responses
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of M. pyrifera spores to specific nutrients, for example, to phosphate, which does not attract spores but does increase their settlement rates (Amsler and Neushul, 1989, 1990). Fukuhara et al. (2002) examined the eVects of various nitrate and phosphate concentrations on the number of swimming Laminaria japonica spores as a function of time. This could be, but is not necessarily, an indication of settlement rates. Although sample size, sample variance, or statistical analyses were not indicated in the paper for these data, there was a trend for fewer swimming spores over time in three phosphate concentrations between 3.0 and 9.7 M compared to three concentrations between 0.0 and 1.7 M, suggesting that phosphate may stimulate settlement (Fukuhara et al., 2002). There was no convincing concentration‐dependent pattern for spores swimming in various concentrations of nitrate. In the Ectocarpales, the behaviours of asexually produced spores from Ectocarpus siliculosus and Hincksia irregularis have been examined. E. siliculosus spores diVer from those of kelps in not being attracted to nutrients (either chemotactically or chemokinetically) and in not being stimulated to settle by nutrients (Amsler et al., 1999). However, it was only practical to work with E. siliculosus spores soon after release so the potential for them to develop a settlement stimulation response some hours after release, as is observed in kelp spores, could not be tested. E. siliculosus spores did settle diVerentially to substrates of diVerent surface energy (hydrophobicity or wetabiltiy) with fourfold higher rates of settlement on hydrophobic surfaces compared to either positively or negatively charged hydrophilic surfaces (Amsler et al., 1999). H. irregularis also settles at faster rates on hydrophobic surfaces (Greer and Amsler, 2002, 2004; Greer et al., 2003), as do spores of ulvoid green algae (e.g., Callow and Callow, 1998a,b, 2000; Ista et al., 2004). Hincksia irregularis and other members of the Ectocarpales are morphologically simple as adult thalli, but in contrast to long‐held assumptions, that does not necessarily mean that they are evolutionarily primitive compared to other brown algae with greater morphological complexity (Cho et al., 2004; Draisma et al., 2001). Regardless, studies have shown that the zoospores of H. irregularis are behaviourally complex and capable of integrating multiple chemical and other environmental stimuli in determining when or where to settle and germinate. Iken et al. (2001) documented both quantitative and qualitative changes in spore behaviour over time (Fig. 11) that are consistent with a hypothetical, developmental progression of sensory modes. The ‘‘gyration’’ behaviour (Fig. 11D) that often occurs immediately before final settlement and attachment has been reported previously in macroalgal spores (Fletcher and Callow, 1992), but the preceding progression of behaviours (Fig. 11A–C) and the relative synchrony of their development under tightly controlled laboratory conditions surprised even the study’s authors.
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Quantitative measures of the appearance of an apparently abnormal behaviour (Fig. 11E) have proven useful in identifying secondary metabolites from marine invertebrates with potential antifoulant capabilities against the spores (Greer, 2003; Iken et al., 2003). Furthermore, H. irregularis spores are capable of integrating their sensory responses to soluble chemicals and surface hydrophobicity (Greer et al., 2003), as well as their responses to surface hydrophobicity and gradients of light (Greer and Amsler, 2002, 2004). These are clearly not ‘‘simple’’ propagules of simple algae and, as with kelp spores, one should not be surprised if natural selection has shaped their behaviours. This is an area of brown algal sensory chemical ecology ripe for investigation in the near term, and recent progress on the biochemical interactions and sensory biology of green algal zoospores (e.g., Callow et al., 2002; Ista et al., 2004; Joint et al., 2002; Patel et al., 2003) points to progress that might be expected if the quantitative measures of the responses to chemical and other environmental stimuli that have been used with brown algal spores were integrated with other methodologies that have been pioneered with spores of green algae.
VIII. CONCLUDING REMARKS Although there are several ordinal‐level classification schemes for the Phaeophyceae, a widely used current text (Graham and Wilcox, 2000) includes 14 orders. In preparing this review, one thing that struck us is how often we have discussed members of the Fucales, Laminariales, and Dictyotales and how few times we have mentioned many of the others, particularly in the sections on defensive chemical ecology. In some cases this is because the other orders include relatively few species and/or species that are not particularly common, but in some that is not true (e.g., the Ectocarpales, which is widespread throughout the world’s oceans). What is true of most of the other groups (particularly the Ectocarpales) is that those that are widespread are usually not particularly large, and it should not be surprising that the larger and most common macroalgae in communities have received the most attention. Nevertheless, smaller does not mean less interesting or less important, as illustrated by the increased recent attention on mesoherbivores. Poore’s (1994) report illustrated that the distribution of chemical defences can vary within a distance of one to a few cells within an individual macroalga, and studies of chemical defences in some single‐celled microalgae (e.g., Pohnert et al., 2002; Steinke et al., 2002; Strom et al., 2003; Wichard et al., 2005) show that small algae can elaborate eVective chemical defences. Might it not be possible that diVerences in defensive investment analogous to that
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discussed in Sections II.E or IV.A could also occur in smaller macroalgae such as ectocarpoids? Also, if one scales down the idea of mesoherbivores being important in influencing defensive patterns in some larger macroalgae, might micrograzers be selecting analogous and, perhaps, novel or otherwise unexpected patterns of defence in small macroalgae? Less likely, perhaps, but until someone looks, these are open questions. Regardless, algal– herbivore interactions between filamentous or other small macroalgae and herbivores such as mesograzers could still be important in terms of macroalgal community structure, as Peters (2003) has hypothesised for communities along the western Antarctic Peninsula. The smaller brown algae have proven to be valuable models in studies of sensory chemical ecology, and although their size may impose technical limitations, they deserve experimental attention in studies of defensive chemical ecology. It is hoped that this review has been useful as a summary of how much important work has been done in the subdisciplines comprising brown algal chemical ecology as a whole. We have tried throughout to highlight some of the areas that we feel deserve attention in the coming years. However, those are, of course, only a small subset of the important questions yet to be asked.
ACKNOWLEDGMENTS We are grateful to numerous colleagues who provided preprints or other literature and to those who allowed us to use illustrations from their work. We are particularly grateful to Alistair Poore for sending scans of original illustrations. The manuscript benefited greatly from the comments of Margaret Amsler, James McClintock, and Robert Thacker. We also thank Majdouline LeRoy for preparing chemical structure figures. Manuscript preparation was supported in part by Grants OPP‐0125181 and OPP‐0442769 from the National Science Foundation.
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Steinberg, P. D. (1985). Feeding preferences of Tegula funebralis and chemical defenses of marine brown algae. Ecological Monographs 55, 333–349. Steinberg, P. D. (1986). Chemical defences and the susceptibility of tropical marine brown algae to herbivores. Oecologia 69, 628–630. Steinberg, P. D. (1988). EVects of quantitative and qualitative variation in phenolic compounds on feeding in three species of marine invertebrate herbivores. Journal of Experimental Marine Biology and Ecology 120, 221–237. Steinberg, P. D. (1989). Biogeographical variation in brown algal polyphenolics and other secondary metabolites: Comparison between temperate Australasia and North America. Oecologia 78, 373–382. Steinberg, P. D. (1994). Lack of short‐term induction of phlorotannins in the Australasian brown algae Ecklonia radiata and Sargassum vestitum. Marine Ecology Progress Series 112, 129–133. Steinberg, P. D. (1995). Seasonal variation in the relationship between growth and phlorotannin production in the kelp Ecklonia radiata. Oecologia 102, 169–173. Steinberg, P. D. and de Nys, R. (2002). Chemical mediation of colonisation of seaweed surfaces. Journal of Phycology 38, 621–629. Steinberg, P. D., de Nys, R. and Kjelleberg, S. (2001). Chemical mediation of surface colonisation. In ‘‘Marine Chemical Ecology’’ (J. B. McClintock and B. J. Baker, eds.), pp. 355–387. CRC Press, Boca Raton, FL. Steinberg, P. D., de Nys, R. and Kjelleberg, S. (2002). Chemical cues for surface colonisation. Journal of Chemical Ecology 28, 1935–1951. Steinberg, P. D., Edyvane, K., de Nys, R., Birdsey, R. and van Altena, I. (1991). Lack of avoidance of phenolic‐rich brown algae by tropical herbivorous fish. Marine Biology 109, 335–343. Steinberg, P. D., Estes, J. A. and Winter, F. C. (1995). Evolutionary consequences of food‐chain length in kelp forest communities. Proceedings of the National Academy of Sciences of the United States of America 92, 8145–8148. Steinberg, P. D. and Paul, V. (1990). Fish feeding and chemical defense of tropical brown algae in Western Australia. Marine Ecology Progress Series 58, 253–259. Steinberg, P. D. and van Altena, I. (1992). Tolerance of marine invertebrate herbivores to brown algal phlorotannins in temperate Australasia. Ecological Monographs 62, 189–222. Steinke, M., Malin, G. and Liss, P. S. (2002). Trophic interactions in the sea: An ecological role for climate relevant volatiles? Journal of Phycology 38, 630–638. Stern, J. L., Hagerman, A. E., Steinberg, P. D. and Mason, P. K. (1996a). Phlorotannin‐protein interactions. Journal of Chemical Ecology 22, 1877–1899. Stern, J. L., Hagerman, A. E., Steinberg, P. D., Winter, F. C. and Estes, J. A. (1996b). A new assay for quantifying brown algal phlorotannins and comparisons to previous methods. Journal of Chemical Ecology 22, 1273–1293. Stiger, V., Deslandes, E. and Payri, C. E. (2004). Phenolic contents of two brown algae, Turbinaria omata and Sargassum mangarevense on Tahiti (French Polynesia): Interspecific, ontogenic and spatio‐temporal variations. Botanica Marina 47, 402–409. Strom, S., Wolfe, G., Holmes, J., Stecher, H., Shimeneck, C., Lambert, S. and Moreno, E. (2003). Chemical defense in the microplankton. I. Feeding and growth rates of heterotrophic protists on the DMS‐producing phytoplankter Emiliania huxleyi. Limnology and Oceanography 48, 217–229. Swanson, A. K. and Druehl, L. D. (2002). Induction, exudation and the UV protective role of kelp phlorotannins. Aquatic Botany 73, 241–253.
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Targett, N. M. and Arnold, T. M. (1998). Predicting the eVects of brown algal phlorotannins on marine herbivores in tropical and temperate oceans. Journal of Phycology 34, 195–205. Targett, N. M. and Arnold, T. M. (2001). EVects of secondary metabolites on digestion in marine herbivores. In ‘‘Marine Chemical Ecology’’ (J. B. McClintock and B. J. Baker, eds.), pp. 391–411. CRC Press, Boca Raton, FL. Targett, N. M., Boettcher, A. A., Targett, T. E. and Vrolijk, N. H. (1995). Tropical marine herbivore assimilation of phenolic‐rich plants. Oecologia 103, 170–179. Targett, N. M., Coen, L. D., Boettcher, A. A. and Tanner, C. E. (1992). Biogeographic comparisons of marine algal polyphenolics: Evidence against a latitudinal trend. Oecologia 89, 464–470. Taylor, R. B., Lindquist, N., Kubanek, J. and Hay, M. E. (2003). Intraspecific variation in palatability and defensive chemistry of brown seaweeds: EVects on herbivore fitness. Oecologia 136, 412–423. Taylor, R. B., Sotka, E. and Hay, M. E. (2002). Tissue‐specific induction of herbivore resistance: Seaweed response to amphipod grazing. Oecologia 132, 68–76. Toth, G. B., Langhamer, O. and Pavia, H. (2005). Inducible and constitutive defenses of valuable seaweed tissues: Consequences for herbivore fitness. Ecology 86, 612–618. Toth, G. and Pavia, H. (2000a). Lack of phlorotannin induction in the brown seaweed Ascophyllum nodosum in response to increased copper concentrations. Marine Ecology Progress Series 192, 119–126. Toth, G. B. and Pavia, H. (2000b). Water‐borne cues induce chemical defense in a marine alga (Ascophyllum nodosum). Proceedings of the National Academy of Sciences of the United States of America 97, 14418–14420. Toth, G. B. and Pavia, H. (2001). Removal of dissolved brown algal phlorotannins using insoluble polyvinylpolypyrrolidone (PVPP). Journal of Chemical Ecology 27, 1899–1910. Toth, G. B. and Pavia, H. (2002a). Lack of phlorotannin induction in the kelp Laminaria hyperborea in response to grazing by two gastropod herbivores. Marine Biology 140, 403–409. Toth, G. B. and Pavia, H. (2002b). Intraplant habitat and feeding preference of two gastropod herbivores inhabiting the kelp Laminaria hyperborea. Journal of the Marine Biological Association of the United Kingdom 82, 243–247. Tugwell, S. and Branch, G. M. (1989). DiVerential polyphenolic distribution amoung tissues in the kelps Ecklonia maxima, Laminaria pallida and Macrocystis angustifolia in relation to plant‐defence theory. Journal of Experimental Marine Biology and Ecology 129, 219–230. Tugwell, S. and Branch, G. M. (1992). EVects of herbivore gut surfactants on kelp polyphenol defenses. Ecology 73, 205–215. Tuomi, J., Ilvessalo, H., Sire´ n, S. and Jormalainen, V. (1989). Within‐plant variation in phenolic content and toughness of the brown alga Fucus vesiculosus L. Botanica Marina 32, 505–509. Utter, B. D. and Denny, M. W. (1996). Wave‐induced forces on the giant kelp Macrocystis pyrifera (Agardh): Field test of a computational model. Journal of Experimental Biology 199, 2645–2654. Vallim, M. A., De Paula, J. C., Pereira, R. C. and Teixeira, V. L. (2005). The diterpenes from dictyotacean marine brown algae in the tropical Atlantic American region. Biochemical Systematics and Ecology 33, 1–16.
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toward Gracilaria conferta (Rhodophyta). Journal of Phycology 37, 418–426. Weykam, G., Go´ mez, I., Wiencke, C., Iken, K. and Klo¨ ser, H. (1996). Photosynthetic characteristics and C:N ratios of macroalgae from King Gorge Island (Antarctica). Journal of Experimental Marine Biology and Ecology 204, 1–22. Wichard, T., Poulet, S. A., Halsband‐Lenk, C., Albaina, A., Harris, R., Liu, D. and Pohnert, G. (2005). Survey of the chemical defence potential of diatoms: Screening of fifty species for ‐unsaturated aldehydes. Journal of Chemical Ecology 31, 949–958. Wiencke, C. and Clayton, M. (2002). ‘‘Antarctic Seaweeds.’’ ARG Gantner Verlag, KG Ruggell. Wilkstro¨ m, S. A. and Pavia, H. (2004). Chemical settlement inhibition versus post‐ settlement mortality as an explanation for diVerential fouling of two congeneric seaweeds. Oecologia 138, 223–230. Winter, F. C. and Estes, J. A. (1992). Experimental evidence for the eVects of polyphenolic compunds from Dictyoneurum californicum Ruprecht (Phaeophyta:Laminariales) on feeding rate and growth in the red abalone Haliotus rufescens Swainson. Journal of Experimental Marine Biology and Ecology 155, 263–277. Wirth, H. E. and Rigg, G. B. (1937). The acidity of the juice of Desmarestia. American Journal of Botany 24, 68–70. Wojtaszek, P. (1997). Oxidative burst: An early plant response to pathogen infection. Biochemical Journal 322, 681–692. Yates, J. L. and Peckol, P. (1993). EVects of nutrient availability and herbivory on polyphenolics in the seaweed Fucus vesiculosus. Ecology 74, 1757–1766.
FURTHER READING Dethier, M. N., Williams, S. L. and Freeman, A. (2005). Seaweeds under stress: Manipulated stress and herbivory affect critical life-history functions. Ecological Monographs 75, 403–418. Molis, M., Ko¨ ner J., Ko, Y. W., Kim, J.H., and Wahl, M. (in press). Inducible responses in the brown seaweed Ecklonia cave: The role of grazer identity and season. Journal of Ecology.
Regulation of Carbon and Amino Acid Metabolism: Roles of Sucrose Nonfermenting‐1‐Related Protein Kinase‐1 and General Control Nonderepressible‐2‐Related Protein Kinase
NIGEL G. HALFORD
Crop Performance and Improvement, Rothamsted Research Harpenden, Hertfordshire AL5 2JQ, United Kingdom
I. Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . II. Amino Acid Signalling. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. General Amino Acid Control in Yeast . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Plant General Control Nonderepressible‐2 and Evidence of Conservation of Elements of General Amino Acid Control . . . . . . . . III. Carbon Metabolite Sensing and Signalling . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. AMP‐activated Protein Kinase, the Fuel Gauge of Animal Cells . . . B. Regulation of Carbon Metabolism in Yeast . . . . . . . . . . . . . . . . . . . . . . . C. Carbon Metabolite Sensing and Signalling in Plants . . . . . . . . . . . . . . . IV. The Link Between Sugar and Abscisic Acid/Stress Signalling Pathways . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . V. Prospects. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Acknowledgment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
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ABSTRACT The sensing and signalling mechanisms through which plant cells respond to levels of carbon metabolites and amino acids are reviewed, focusing on the roles of sucrose nonfermenting‐1‐related protein kinase (SnRK1) and general control nonderepressible‐2‐related protein kinase, drawing comparisons with homologous and analogous systems in animals and fungi. Amino acid signalling and general amino acid control Advances in Botanical Research, Vol. 43 Incorporating Advances in Plant Pathology Copyright 2006, Elsevier Ltd. All rights reserved.
0065-2296/06 $35.00 DOI: 10.1016/S0065-2296(05)43002-5
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in yeast are described, and evidence for the presence of a similar system in plants is discussed. Carbon metabolite signalling in animal, fungal, and plant systems is described. The roles of SnRK1 in sugar sensing and the regulation of carbohydrate metabolism, starch accumulation, sterol biosynthesis, the cell cycle, and development are described. The link between sugar and abscisic acid signalling is discussed.
I. INTRODUCTION A few hours after we eat a meal we start to feel hungry and the gap between eating and wanting to eat again will shorten if we use up energy by exercising or if our bodies have a high demand for nutrients for growth. We regard this as a whole organism eVect, but nutrient availability also has profound eVects at the cellular level. Cells sense and respond to the availability of nutrients, in other words their metabolic status, in several ways. They modify their processes for nutrient uptake, they mobilise or build up intracellular reserves, and they regulate the demand imposed by biosynthetic pathways. One of the great fascinations of this subject is that the regulatory mechanisms that maintain and respond to cellular metabolic status are ancient and must have emerged in primitive eukaryotes before the divergence of plants, animals, and fungi. While these mechanisms have continued to evolve in all three kingdoms, they have been conserved suYciently to be instantly recognisable from higher plants to fungi and humans. Hence, the regulatory pathway that is activated in human skeletal muscle cells to enable them to meet the energy demands of exercise has the same central players as that which enables yeast cells to start making the enzymes required to use alternative carbon sources in the absence of glucose and that which enables the cells in a growing potato tuber to make the enzymes required for the breakdown of sucrose arriving from the leaves. These regulatory processes begin with the sensing of metabolite levels. Indeed, the interest of plant scientists in this field stemmed from the realisation that metabolites themselves initiate signals that have profound eVects on enzyme activity and gene expression, thereby influencing the flux of compounds through metabolic pathways. In this way, metabolite sensing and signalling aVects and is aVected by processes such as photosynthesis, the cell cycle, biotic and abiotic stresses from the environment, nutrient availability, and the partitioning of resources within the plant (Fig. 1). It is, therefore, a crucial factor in determining the survival and productivity of plants and their adaptation to extreme environments. The rapid advances in genomics, transcriptomics, proteomics, and metabolomics mean that there is now a great opportunity to make progress in the elucidation of the sensing and signalling mechanisms that maintain the
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Fig. 1. Schematic showing how metabolic status aVects and is aVected by a range of cellular processes.
Fig. 2. The partitioning of assimilated carbon and nitrogen arriving at a sink organ such as a seed or tuber. The partitioning of assimilate is an important determinant of both yield and quality.
metabolic status of plant cells and regulate and integrate metabolic pathways. This is essential for the development of rational strategies for the modification of metabolism and resource partitioning (Fig. 2). However, the target of a
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broad understanding of these mechanisms remains a considerable way oV. They include the activation and deactivation of enzymes by phosphorylation, the thioredoxin system, the control of transcription, translation, post‐ translational modification and protein turnover, as well as the interactions shown in Fig. 1. This review deals with the sensing and signalling mechanisms through which plant cells respond to levels of carbon metabolites and amino acids, focussing in particular on the roles of sucrose nonfermenting‐1 (SNF1)‐ related protein kinase (SnRK1) and general control nonderepressible‐2 (GCN2)‐related protein kinase. It covers the metabolites that are sensed and what is known about the genes, transporters, metabolic enzymes, transcription factors, and hormones that are involved. Throughout, comparisons are drawn with homologous and analogous systems in animals and fungi.
II. AMINO ACID SIGNALLING A. GENERAL AMINO ACID CONTROL IN YEAST
Amino acid synthesis and protein production in budding yeast (Saccharomyces cerevisiae) are regulated in a wonderfully elegant manner in response to amino acid levels. Amino acid starvation causes a general reduction in protein synthesis and initiates changes in expression of a huge number of genes in a process known as general amino acid control (Hinnebusch, 1992). Fundamental to general amino acid control is the protein kinase GCN2 (Wek et al., 1989). The substrate for GCN2 is the subunit of eukaryotic translation initiation factor‐2 (eIF‐2), which is phosphorylated by GCN2 at serine‐51 (Samuel, 1993) (Fig. 3). eIF‐2 is a trimeric factor (subunits , , and ) that can bind either GDP or GTP. However, only when bound to GTP is it able to carry out its physiological function of binding Met‐tRNA to the ribosome and transferring it to the 40S ribosomal subunit. Following attachment of the [eIF‐2.GTP.Met‐tRNA] complex to the 40S subunit, the GTP is hydrolyzed to GDP and Pi and eIF‐2 is released as an inactive [eIF‐2. GDP] complex. Phosphorylation of eIF‐2 inhibits the recycling of bound GDP to GTP, decreasing the rate of protein synthesis. GCN2‐mediated phosphorylation of eIF‐2 under conditions of amino acid deprivation increases the expression of amino acid biosynthesis genes through the action of a transcriptional activator, GCN4 (Hinnebusch, 1997) (Fig. 4). Upregulation of GCN4 occurs at the translational level, with translation initiating from a downstream initiation codon that is not used
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Fig. 3. The mechanism by which GCN2 inhibits protein synthesis in yeast. GCN2 is activated in response to low amino acid levels and phosphorylates the subunit of eIF‐2. Phosphorylation of eIF‐2 inhibits the recycling of eIF2‐bound GDP to GTP, preventing eIF2 from binding Met‐tRNAi (a special tRNA used for initiation) to the ribosome and transferring it to the 40S ribosomal subunit, thereby decreasing the rate of protein synthesis. Figure kindly provided by Yuhua Zhang.
Fig. 4. A decrease in the binding of Met‐tRNAi to eIF2 causes an increase in the translation of the transcription factor, GCN4, which activates the expression of a large number of genes, including many that encode enzymes involved in amino acid biosynthesis. The free amino acid pool is therefore replenished.
under normal conditions (Hinnebusch, 1992, 1994). Microarray analysis identified 539 yeast genes that are induced by amino acid starvation through the action of GCN4 (Natarajan, 2001). These included genes in
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every amino acid biosynthetic pathway except cysteine, as well as genes encoding amino acid precursors, vitamin biosynthetic enzymes, peroxisomal components, mitochondrial carrier proteins, autophagy proteins, and many genes encoding protein kinases and transcription factors. GCN2 is believed to be activated through interaction with uncharged tRNA (Wek et al., 1989). The region of the protein responsible for this is a domain of approximately 400 amino acid residues that shows significant sequence similarity with histidyl‐tRNA synthetases (Wek et al., 1989). The presence of adjacent kinase catalytic and His‐tRNA synthetase‐like domains is indicative of a GCN2‐type protein kinase. Note that a second mechanism that is distinct from this amino acid response but acts through GCN2 to induce the synthesis of GCN4 is initiated by glucose limitation (Yang et al., 2000). Induction of GCN4 during carbon starvation is believed to enhance the storage of amino acids in the vacuoles, thereby facilitating re‐entry into exponential growth when glucose becomes available. Homologues of GCN2 have been identified in Drosophila melanogaster (Santoyo et al., 1997) and Neurospora crassa (Sattlegger et al., 1998), and there are two other eIF‐2 kinases that have similar catalytic domains to GCN2 but do not contain a histidyl‐tRNA synthetase‐like domain and respond to diVerent stimuli. These are the heme‐regulated inhibitor (HRI), which has been cloned from rabbit and rat (Chen et al., 1991; Mellor et al., 1994a), and the double‐stranded RNA‐dependent kinase (PKR), which has been cloned from human (Meurs et al., 1990). HRI is activated in response to heme deficiency (Chen et al., 1991; Mellor et al., 1994a) and PKR to the presence of double‐stranded RNAs after virus infection (Icely et al., 1991; Mellor et al., 1994b; Meurs et al., 1990). B. PLANT GENERAL CONTROL NONDEREPRESSIBLE‐2 AND EVIDENCE OF CONSERVATION OF ELEMENTS OF GENERAL AMINO ACID CONTROL
The phosphorylation site at serine‐51 is conserved in eIF‐2 homologues from a wide range of eukaryotes, including wheat, and yeast GCN2 will phosphorylate wheat eIF‐2 at this position (Chang et al., 1999, 2000). Furthermore, a GCN2 homologue from Arabidopsis was identified in 2003 (Zhang et al., 2003). This gene, AtGCN2, which is present as a single copy on chromosome 3, encodes a protein of 140 kDa showing approximately 30% identity overall with yeast GCN2, rising to 44% in the catalytic domain. Expression of AtGCN2 in yeast gcn2 mutants complements the mutation, enabling growth in the presence of sulfometuron methyl, an inhibitor of branched chain amino acid biosynthesis, and 3‐aminotriazole, an inhibitor of histidine biosynthesis. Screening of EST and genomic databases with the
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AtGCN2 sequence reveals the presence of similar genes and transcripts in rice, wheat, barley, potato, soybean, sugar beet, sugarcane, Medicago, cotton, poplar, onion, lotus, and Zinnia. However, perhaps surprisingly, there is no obvious candidate for a GCN4 homologue in Arabidopsis that is identifiable on the basis of sequence similarity with yeast GCN4. There is a database entry for a ‘‘GCN4‐complementing’’ gene called GCP1 (accession AJ130878), but this entry dates to the late 1990s and to the author’s knowledge data supporting the claim have never been published. The link between amino acid signalling, nitrogen use eYciency, crop yield, and quality makes the elucidation of amino acid signalling pathways an important target for plant scientists. There is evidence of co‐ordinated regulation of genes encoding enzymes of amino acid biosynthesis in plants. For example, blocking histidine biosynthesis in Arabidopsis with a specific inhibitor, IRL 1803, has been shown to increase the expression of eight genes involved in the synthesis of aromatic amino acids, histidine, lysine, and purines (Guyer et al., 1995). Genes encoding tryptophan biosynthesis pathway enzymes have also been shown to be induced by amino acid starvation (caused by, for example, glyphosate treatment) in Arabidopsis (Zhao et al., 1998). The identification of AtGCN2 supports the hypothesis that at least some elements of general amino acid control are present in plants, but clearly much has to be done to elucidate the whole signalling pathway. It will also be important to determine how amino acid signalling links with the broader signalling network that responds to nitrate availability. Amino acid signalling has the potential to aVect many metabolic and developmental processes. Just one possible example is the regulation of storage protein (prolamin) gene expression in cereal seeds (reviewed by Shewry et al., 2003). The expression of prolamin genes responds sensitively to the availability of nitrogen in the grain (DuVus and Cochrane, 1992; Giese and Hopp, 1984) and many contain a conserved sequence, approximately 30 bp long and positioned around 300 bp upstream of the transcription start site (Forde et al. 1985) (Fig. 5). This sequence contains two conserved motifs, TGTAAAGT and G(A/G)TGAGTCAT; the former has been called the endosperm motif (Hammond‐Kosack et al., 1993) (E motif in Fig. 5) and the latter the GCN4‐like motif (GLM), nitrogen element, or N motif (Hammond‐Kosack et al., 1993; Mu¨ ller and Knudsen, 1993). The central part of the N motif is similar to the binding site of GCN4, the sequence of which is TGACTC, and this element acts as a negative element at low nitrogen levels and a positive element when nitrogen levels are adequate (Mu¨ller and Knudsen, 1993). Two transcription factors, ESBF‐II (Hammond‐Kosack et al., 1993) and SPA (Albani et al., 1997), have been shown to bind this
Fig. 5. Schematic showing the regulatory elements in the promoters of families of wheat storage protein genes. The N motif is similar to the binding site of the yeast transcription factor, GCN4.
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motif, although neither is closely related to GCN4 in terms of amino acid sequence.
III. CARBON METABOLITE SENSING AND SIGNALLING A. AMP‐ACTIVATED PROTEIN KINASE, THE FUEL GAUGE OF ANIMAL CELLS
AMP‐activated protein kinase (AMPK) was one of the first protein kinases to be studied biochemically. It was purified originally as separate activities that caused time‐ and ATP‐dependent inactivations of HMG‐CoA reductase (Beg et al., 1973) or acetyl‐CoA carboxylase (Carlson and Kim, 1973). Later it became clear that these activities were functions of the same protein kinase. The primary function of AMPK is the conservation of ATP and it achieves this function through the phosphorylation and inactivation of regulatory enzymes of ATP‐consuming pathways, such as acetyl‐CoA carboxylase (fatty acid synthesis) (Davies et al., 1990, 1992) and HMG‐CoA reductase (sterol/isoprenoid synthesis) (Clarke and Hardie, 1990; Gillespie and Hardie, 1992). It also regulates gene expression, inhibiting the glucose activation of genes involved in glucose and lipid metabolism in liver cells, including genes encoding pyruvate kinase and fatty acid synthase (Leclerc et al., 1998; Woods et al., 2000). Activation of AMPK has been demonstrated in response to a variety of stresses in mammalian cells, including exercise in skeletal muscle (Winder and Hardie, 1996), interruption of the blood supply in heart muscle (Kudo et al., 1995), treatment of cells with deoxyglucose or high levels of fructose (Moore et al., 1991; Sato et al., 1993), heat shock (Corton et al., 1994), arsenate, and other inhibitors of oxidative metabolism (Corton et al., 1994; Witters et al., 1991). AMPK is attracting increasing interest because it has been implicated in insulin regulation, type 2 diabetes mellitus, and obesity. Mutations in AMPK are associated with a severe heart defect (hypertrophy and arrhythmia). As its name suggests, AMPK is activated allosterically by 50 ‐adenosine monophosphate (AMP) (Carling et al., 1987, 1989). It is also activated by phosphorylation by an upstream protein kinase that itself is activated by AMP (Hawley et al., 1996). AMP binding acts in two other ways to increase AMPK activity: it makes AMP a better substrate for the upstream protein kinase and a worse substrate for protein phosphatase‐2C (Carling et al., 1989; Corton et al., 1995; Davies et al., 1995; Hawley et al., 1995). Activation of AMPK by AMP is antagonised by high concentrations of ATP.
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Fig. 6. Pathways for activation of AMP‐activated protein kinase (AMPK), the ‘‘fuel gauge’’ of mammalian cells, and its targets.
This means that AMPK can act as a fuel gauge for animal cells (Hardie and Carling, 1997) (Fig. 6). Levels of ATP, AMP, and ADP are held in equilibrium by the enzyme adenylate kinase, which catalyses the interconversion of ATP and AMP to two molecules of ADP. Continuous production of ATP when a cell is well nourished leads to a high ATP:ADP ratio, pushing this reaction in the direction of ADP and depleting the pool of AMP. Conversely, when ATP is not being supplied in suYcient amounts by glycolysis, the TCA cycle, and respiration, the ATP:ADP ratio falls and AMP levels rise. AMPK comprises three subunits, a catalytic subunit and accessory and subunits, in a heterotrimeric complex (Davies et al., 1994; Mitchelhill et al., 1994) (Fig. 7). Amino acid and DNA sequencing of the three subunits (Carling et al., 1994; Gao et al., 1995, 1996; Mitchelhill et al., 1994; Woods et al., 1996) revealed that AMPK was the animal homologue of sucrose nonfermenting‐1 (SNF1) of budding yeast (Saccharomyces cerevisiae) and SNF1‐related protein kinase‐1 (SnRK1) of plants. More recently, a protein kinase upstream of AMPK has been identified as LKB1, a tumour repressor that had not been linked previously to metabolic regulation (Woods et al., 2003). In humans, mutations in LKB1 cause Peutz–Jeghers syndrome, suVerers of which are prone to develop rare
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Fig. 7. Components of SnRK1 (plants), AMPK (mammals), and SNF1 (yeast). Plant subunits are labelled in black, animal subunits in mid‐grey, and yeast subunits in light grey. Note that plants have several proteins with some similarity with the AMPK and SNF4 subunits; this subunit dissociates from the catalytic subunit when glucose availability is adequate, allowing the regulatory domain of the catalytic subunit to fold over the catalytic domain, causing inactivation.
cancers. This discovery caused great excitement because it suggested a link between cancer and diabetes, and might explain why exercise provides some protection against both. AMPK phosphorylates a synthetic peptide (His Met Arg Ser Ala Met Ser Gly Leu His Leu Val Lys Arg Arg) known as the SAMS peptide based on the sequence around the primary phosphorylation site for AMPK on rat acetyl‐CoA carboxylase. This has enabled a relatively simple assay for AMPK activity to be developed that measures the rate of phosphorylation of the SAMS peptide using radiolabelled ATP as a phosphate donor (Davies et al., 1989). B. REGULATION OF CARBON METABOLISM IN YEAST
1. SNF1 and glucose repression In yeast, the expression of genes and processes involved in aerobic metabolism or the metabolism of carbon sources other than glucose is prevented if glucose is present above a concentration of about 0.2% (w/v) (Dickinson,
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1999). This process of glucose repression is the over‐riding mechanism for regulating carbon metabolism. It aVects the utilisation of alternative carbon sources, gluconeogenesis, the synthesis of dozens of enzymes, respiration, and the biogenesis of mitochondria and peroxisomes even if other carbon sources are provided. It ensures that glucose is always consumed first, regardless of what other carbon sources are available, and that the glucose is consumed entirely by fermentation to ethanol. Aerobic metabolism commences only when glucose levels are low. A critical component of this fundamental signalling mechanism in budding yeast is a protein kinase called sucrose nonfermenting‐1 (SNF1) (Fig. 8). SNF1, a 72‐kDa protein with an N‐terminal protein serine/threonine kinase domain followed by a C‐terminal regulatory domain (Celenza and Carlson, 1986), was given its name because a snf1 mutant was first identified in a screen for mutants that were unable to switch on the invertase gene SUC2 in response to glucose deprivation. It is now known to be required for growth on other fermentable carbon sources such as galactose and maltose and on nonfermentable carbon sources such as glycerol and ethanol (reviewed by Dickinson, 1999). As well as being required for the derepression of essentially all glucose‐repressed genes, SNF1 aVects sporulation, cell cycle control, glycogen accumulation, peroxisome biogenesis, and regulation of enzyme activity. A transcription factor that is almost certainly a substrate for SNF1 is the transcriptional repressor MIG1. MIG1 contains several potential SNF1 phosphorylation sites, and mutation of these results in ¨ stling and Ronne, 1998). The constitutive repression of transcription (O cellular location of MIG1 is determined by glucose: the addition of glucose causes it to move to the nucleus and the removal of glucose causes it to return to the cytosol (DeVit et al., 1997). Like AMPK, to which it is now known to be homologous, the SNF1 protein kinase actually comprises three subunits (Fig. 7), of which the catalytic subunit is encoded by the SNF1 gene (Celenza and Carlson, 1986). The second subunit in the complex is a protein called SNF4, a regulatory subunit that is required for full activity (Celenza et al., 1989) and which is homologous to the subunit of AMPK. The interaction between SNF1 and SNF4 appears to be regulated by glucose, and in conditions of glucose deprivation, SNF4 counteracts autoinhibition by SNF1 (Jiang and Carlson, 1996). The third subunit, homologous to the subunit of AMPK, is one from a class of proteins that comprises SIP1, SIP2, and GAL83, three related proteins that are interchangeable and may target the complex to diVerent substrates (Yang et al., 1994). SIP1, SIP2, and GAL83 contain two conserved domains: the ASC domain (association with SNF1 complex) (Jiang and Carlson, 1997; Yang et al., 1994) and the KIS domain
Fig. 8. Possible pathways for activation of sucrose nonfermenting‐1 (SNF1) of yeast, and its targets. Carbon ‘‘flow’’ from glucose to ethanol or CO2 is indicated with black arrows; signalling interactions are shown with grey arrows; and dotted lines are used where the mechanism for an interaction is not known.
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(kinase interacting sequence) (Jiang and Carlson, 1997). They appear to form ‘‘scaVold’’ subunits on which the SNF1 and SNF4 proteins assemble (Jiang and Carlson, 1997). Direct interaction between SNF1 and SNF4 proteins only occurs under derepressing (low glucose) conditions (Jiang and Carlson, 1996) (Fig. 7), and this interaction is necessary for the protein kinase activity of SNF1 to be expressed (Celenza and Carlson, 1989; Woods et al., 1994). Using the SAMS peptide as a substrate, activity of the SNF1 complex has been shown to increase dramatically within 5 min of glucose removal (Wilson et al., 1996; Woods et al., 1994). As with the activation of AMPK, this is due to phosphorylation. However, even now, the intracellular signal(s) responsible for triggering this activation remains unknown. Under conditions where SNF1 is activated there are large increases in AMP and decreases in ATP (Wilson et al., 1996) and, by analogy with mammalian AMPK, these nucleotides would be good candidates to be the signals. However, unlike AMPK, no direct eVects of AMP or ATP have been demonstrated on SNF1 in vitro. Three protein kinases that lie upstream of SNF1 (ELM1, PAK1, and TOS3) have now been identified (Hong et al., 2003; Sutherland et al., 2003). It has been proposed that glucose is sensed in yeast by the enzyme hexokinase (Fig. 8). This enzyme has a metabolic function in catalysing the conversion of glucose to glucose‐6‐phosphate (the first stage in glycolysis), but it is found not only in the cytosol where it performs its catalytic function, but also in the nucleus (Herrero et al., 1998; Randez‐Gil et al., 1998). Furthermore, mutations in HXK2, which encodes the major hexokinase PII isoform in S. cerevisiae, cause partially constitutive expression of glucose‐repressed genes (Entian, 1980). However, further work has shown a good correlation between the overall residual hexokinase catalytic activity of diVerent mutants and their ability to exhibit glucose repression (Ma et al., 1989; Rose et al., 1991). This suggests that hexokinase PII has a role in producing the signal molecule, but does not sense or initiate a signal. Despite this, hexokinase is now widely regarded as a ubiquitous glucose sensor in eukaryotes (Rolland et al., 2001). The catalytic activity of hexokinase has been shown to be aVected by components of the trehalose biosynthetic pathway. This pathway involves two enzymes, trehalose phosphate synthase (TPS), which catalyses the formation of trehalose‐6‐phosphate (T6P) from glucose‐6‐phosphate and UDP‐glucose, and trehalose phosphate phosphatase (TPP), which catalyses the dephosphorylation of T6P to trehalose; trehalose is cleaved by another enzyme, trehalase. Both TPS and T6P have an inhibitory eVect on hexokinase, thereby regulating the flux of carbon into glycolysis (Thevelein
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and Hohmann, 1995). This is crucial because it ensures that cellular ATP levels are not depleted through the buildup of glycolytic intermediates (Bonini et al., 2000; Noubhani et al., 2000). This finding has stimulated great interest in the role of T6P as a sensed metabolite in both yeast and plant systems. 2. Glucose induction Whatever the role of glucose in the repression/derepression signalling pathway, it is definitely sensed to initiate a signal in a diVerent pathway, that of glucose induction (Fig. 9). S. cerevisiae has 17 hexose transporters encoded by HXT genes that are expressed diVerentially, depending on the concentration of glucose that is available; high‐aYnity, low‐capacity transporters are expressed when the glucose concentration is low, whereas low‐aYnity,
Fig. 9. Glucose induction in yeast. Glucose is sensed by low‐ and high‐aYnity glucose sensors, SNF3 and RGT2, located in the membrane, and a signal is generated that results in the inactivation of RGT1, a transcriptional repressor of low‐ and high‐ aYnity glucose transporter (HXT) gene promoters. High‐aYnity glucose transporter gene promoters also bind the repressor MIG1, which is active only at high glucose concentrations. When no glucose is present, RGT1 represses all of the HXT genes and none are expressed; when glucose is present at low concentrations, neither RGT1 nor MIG1 is active so all of the HXT genes are expressed; when glucose is present at high concentrations, MIG1 represses the genes encoding high‐aYnity transporters and only the low‐aYnity transporters are expressed.
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high‐capacity transporters are expressed when the glucose concentration is high (Boles and Hollenberg, 1997; Kruckeberg, 1996; Reifenberger et al., 1997). This process ensures that the cell possesses an optimal complement of glucose transporters whatever the medium glucose concentration. Low‐ and high‐aYnity glucose sensors, SNF3 and RGT2, are located in the membrane. Binding of glucose to the sensors causes a signal to be generated that results in inactivation of a protein called RGT1, a transcriptional repressor of HXT gene promoters. The promoters of genes of high‐aYnity glucose transporters also bind the repressor MIG1, which is active at high glucose concentrations (Ozcan and Johnston, 1996). When no glucose is present, none of the HXT genes is expressed because of the action of RGT1. At low concentrations, neither RGT1 nor MIG1 is active so HXT genes are expressed, whereas at high concentrations, only low‐aYnity transporters are expressed because of the action of MIG1. C. CARBON METABOLITE SENSING AND SIGNALLING IN PLANTS
1. SnRK1 A plant homologue of SNF1 and, as was discovered later, of AMPK was first described in 1991 (Alderson et al., 1991). It encodes a 58‐kDa protein showing 48% amino acid sequence identity with SNF1 and AMPK, rising to 62–64% amino acid sequence identity in the kinase catalytic domain. Homologous genes have since been identified and characterised in many plant species and given the name SNF1‐related protein kinase‐1 (SnRK1) (Halford and Hardie, 1998). They are present in small‐ to medium‐sized gene families, comprising, for example, three members in Arabidopsis and 10–20 in barley. The SnRK1 gene family of cereals can be subdivided further into two groups, SnRK1a and SnRK1b, on the basis of amino acid sequence similarity and expression patterns (Halford and Hardie, 1998; Hannappel et al., 1995). A SNF4/AMPK homologue called AtSNF4 has been cloned from Arabidopsis by partial complementation of a snf4 mutant (Kleinow et al., 2000), whereas genes related to the SIP1/SIP2/GAL83/AMPK family have been cloned from Arabidopsis (AKIN 1 and AKIN 2) and potato (StubGAL83) (Bouly et al., 1999; Lakatos et al., 1999). AKIN 1 and AKIN 2 interact with SnRK1 in the two‐hybrid system but also with the yeast SNF1 and SNF4 proteins (Bouly et al., 1999). Potato StubGAL83 was isolated by screening a yeast two‐hybrid cDNA library with a potato SnRK1 cDNA (Lakatos et al., 1999). A maize homologue of AtSNF4 was given the name AKIN because it was found to contain an N‐terminal KIS domain fused with a C‐terminal domain similar to SNF4, AMPK , and AtSNF4 (Lumbreras et al., 2001).
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Re‐analysis of the Arabidopsis AtSNF4 gene shows that it too encodes a protein with this N‐terminal KIS domain. The reason for this domain fusion is not clear. Two other families of plant proteins show similarity with SNF4. These are the PV42 family, which includes PV42 from bean (Phaseolus vulgaris) and AKIN from Arabidopsis (Abe et al., 1995; Bouly et al., 1999), and the SnIP1 family (Slocombe et al., 2002). These show 20–25% amino acid sequence identity with SNF4 and interact with SnRK1 in two‐hybrid assays and in vitro. However, they do not complement the snf4 mutation in yeast and are unique to plants. Both PV42 and SnIP1 will align with SNF4 and AMPK , but show little sequence similarity with each other apart from a short, hydrophobic motif called the SnIP motif (Slocombe et al., 2002). The PV42 and SnIP1 families are unique to plants. 2. SnRK2 and SnRK3 The situation in plants is complicated further by the presence of two other subfamilies of protein kinases, SnRK2 and SnRK3, which contain catalytic domains with sequences that place them clearly within the SNF1 family. The relationship of these protein kinases with other members of the SNF1 family and other protein kinase families is represented in the dendrograms in Figs. 10 and 11A. SnRK2 and SnRK3 have 42–45% amino acid sequence identity with SnRK1, SNF1, and AMPK in the catalytic domain, but no similarity in the regulatory domain (Fig. 11B) and they are unique to plants.
Fig. 10. Dendrogram showing the relationships of subfamilies within the SNF1 family and between the SNF1 family and other families of protein kinases. The SNF1 family includes not only SNF1 (yeast) itself, SnRK1 (plants), and AMPK (mammals), but also two other subfamilies of protein kinases that are unique to plants, SnRK2 and SnRK3, and the cell cycle control proteins, NIM1 (fission yeast) and NIK1 (budding yeast).
Fig. 11. (A) Dendrogram showing the divergence of SNF1‐related protein kinases in plants into three subfamilies: SnRK1, SnRK2, and SnRK3. (B) Schematic showing the structures of SnRK1, SnRK2, and SnRK3 compared with SNF1 and AMPK. Note that there is considerable variation in size within the SnRK3 family. Figures within the diagrams give the amino acid sequence identity with SnRK1 in the catalytic and (where significant) regulatory domains.
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The SnRK2 subfamily includes PKABA1 from wheat, which is involved in mediating ABA‐induced changes in gene expression (Anderberg and Walker‐ Simmons, 1992; Go´ mez‐Cadenas et al., 1999), while the SnRK3 family includes SOS2, an Arabidopsis protein kinase involved in conferring salt tolerance (Halfter et al., 2000; Liu et al., 2000). Importantly, there is no evidence of functional redundancy between these subfamilies of protein kinases. There is some evidence that SnRK3 activity is calcium dependent, unlike that of SnRK1 and SnRK2, although it is not clear how important this regulation is (reviewed by Harper et al., 2004). The completion of the Arabidopsis genome sequencing project means that the full complement of the Arabidopsis SnRK gene family can now be identified. It comprises three SnRK1 genes, two of which (referred to previously as AKIN10 and AKIN11) are active while one (previously known as AKIN30) is silent (Deveraj Jhurreea, unpublished data), nine SnRK2 genes, and 29 SnRK3 genes (Halford et al., 2003a; Hrabak et al., 2003). It is an interesting evolutionary question as to why these subfamilies of SNF1‐ related protein kinase genes are absent from animals and fungi. One interpretation of the dendrogram shown in Fig. 10 is that these gene families were present in primitive eukaryotes, diverging from what would become SNF1, AMPK, and SnRK1 before the separation of plants, animals, and fungi. They were then lost in animals and fungi. However, I propose that SnRK2 and SnRK3 arose from duplication of the SnRK1 gene during plant evolution. The duplication event resulted in accelerated evolution and divergence of the SnRK2 and SnRK3 gene families, explaining their position on the dendrogram. Given the little that we do know about the function of SnRK2s and SnRK3s, one can hypothesise that their emergence allowed plants to develop networks that link environmental stress and metabolite signalling. Exactly when the SnRK2 and SnRK3 gene families diverged from SnRK1 is not yet clear. Two SnRK1 homologues have been identified in the moss, Physcomitrella (Thelander et al., 2004). As yet there is no report of the presence of SnRK2 or SnRK3 genes in this species, but a Chlamydomonas protein kinase called Sac3 involved in the response to sulphur limitation is a member of the SnRK2 family (Davies et al., 1999). 3. Substrates of SnRK1 a. Peptides. Once SnRK1 had been shown to be homologous to AMPK, it was possible to confirm that SnRK1 and a plant protein kinase related to AMPK that had been studied at the biochemical level in Grahame Hardie’s laboratory in Dundee were one and the same (Ball et al., 1995; Barker et al., 1996). Like AMPK, this protein kinase, which had hitherto been known as HMG‐CoA reductase kinase, had been shown to phosphorylate the SAMS
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peptide (MacKintosh et al., 1992). What is more, a purification procedure had already been developed, using cauliflower florets as a source (Ball et al., 1994). A recognition motif for SnRK1 has been established using variant peptide substrates (Weekes et al., 1993). It comprises the phosphorylated serine (SnRK1 will phosphorylate threonine but phosphorylates serine much more eYciently), hydrophobic residues at positions 5 and þ4 relative to the serine, and at least one basic residue, preferably at 3 but tolerated at 4 (Fig. 12). The AMARA peptide (Fig. 12) in which the minimal recognition motif is retained but other residues are alanine apart from the basic C terminus, which is not essential for phosphorylation, appears to be a better substrate than the SAMS peptide (Dale et al., 1995). More recently, basic residues at positions 6 and þ5 have been shown to enhance activity, and a proline residue at position 4 has been found to favour phosphorylation by SnRK1 relative to CDPKs (Huang and Huber, 2001). It is notable that whenever SAMS or AMARA peptide kinase activity has been purified, SnRK1 has accounted for most of it. A minor SAMS peptide kinase activity has been tentatively assigned to SnRK2 but has not been characterised in detail (Ball et al., 1994; Barker et al., 1996; Crawford et al., 2001; Sugden et al., 1999b). Plants expressing antisense SnRK1 sequences retain some AMARA and SAMS peptide kinase activities (Purcell et al., 1998), but it is not clear whether this is residual SnRK1 activity, the activity of SnRK2 and/or SnRK3, or nonspecific background. Mutants of Physcomitrella that lack SnRK1 have almost no AMARA peptide kinase activity at all (Thelander et al., 2004). Intriguingly, the SnIP motif found in PV42 and SnIP1 contains the sequence Hyd‐Xxx‐Bas‐Xxx‐Xxx‐Xxx‐Xxx‐Xxx‐Xxx‐Hyd, where Hyd represents a hydrophobic residue and Bas a basic residue. This resembles the SnRK1 recognition sequence without the target serine residue; such sites act as pseudo‐substrates in the regulatory subunits of the cAMP‐dependent kinase PKA of mammals (Taylor et al., 1990).
Fig. 12. Consensus sequence for phosphorylation by SnRK1 (top row). Required residues are shown in bold. ‘‘Bas’’ indicates a basic residue and ‘‘Hyd’’ a hydrophobic residue. Residues shown in brackets are not required but may enhance phosphorylation. SnRK1 will tolerate the basic residue being at 4 with respect to the serine instead of 3. The middle and bottom rows give the sequences of the AMARA and SAMS peptides, both of which are good substrates for SnRK1.
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b. HMG‐CoA reductase. The demonstration that HMG‐CoA reductase kinase and SnRK1 were one and the same established HMG‐CoA reductase as a substrate for SnRK1. The protein kinase had been shown to phosphorylate and inactivate a bacterially‐expressed Arabidopsis HMG‐CoA reductase in vitro (Ball et al., 1994); the phosphorylation site is Ser‐577. HMG‐CoA reductase catalyses the NADH‐dependent reduction of 3‐ hydroxy‐3‐methylglutaryl‐coenzyme A (HMG‐CoA) to mevalonic acid. In animals and yeast, this is the first committed step in the only pathway for the production of isopentenyl diphosphate, a five‐carbon unit from which all isoprenoids are made. Indeed, it is the overall rate‐limiting step for the isoprenoid biosynthetic pathway. Mevalonate synthesis via HMG‐CoA reductase is also a key step in isoprenoid biosynthesis in plants, although plants possess a second, plastidic pathway for IPP synthesis (Eisenreich et al., 1996). In particular, the HMG‐CoA reductase pathway appears to be the route through which phytosterols are synthesised. Plants contain multiple HMG‐CoA reductases; Arabidopsis, for example, has two: HMG1 and HMG2 (Enjuto et al., 1994). Both HMG1 and HMG2 contain a SnRK1 target site, indeed the site (Met Lys Tyr Asn Arg Ser Ser Arg Asp Ile) is conserved in all of the plant HMG‐CoA reductases characterised so far, with the first of the serine residues being the target for phosphorylation (Halford and Hardie, 1998). Note that it is a suboptimal site in that the basic residue is at 4 with respect to the target serine rather than at 3. The regulation of sterol biosynthesis in plants is of interest to biotechnologists because of the eYcacy of dietary phytosterols in reducing blood cholesterol in humans; with optimised dietary intake they can lower human serum total‐ and low‐density lipoprotein (LDL) or ‘‘bad’’ cholesterol by 10% (Katan et al., 2003). The predominant naturally‐occurring phytosterols, which include ‐sitosterol, campesterol, and stigmasterol, are related structurally to cholesterol (Fig. 13). It has been suggested that they competitively inhibit the uptake of cholesterol from the small intestine (Westrate and Meijer, 1998). Alternatively, they may lead to an increase in the expression of the sterol transporter (Ostlund, 2004; Plat and Mensink, 2002), leading to increased excretion of sterols, including cholesterol, back to the gut lumen. The significance of HMG‐CoA reductase regulation by SnRK1 in the control of phytosterol biosynthesis has been demonstrated by producing transgenic tobacco plants expressing modified HMG‐CoA reductases lacking a SnRK1 target site (Hey et al., in press). Levels of seed sterols were up to 2.5‐fold higher in plants expressing the transgene than in wild type. However, other regulatory mechanisms aVect the activity of HMG‐CoA reductase in plants. One of these must involve the N‐terminal,
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Fig. 13. Diagram showing similarity in the structure of cholesterol and the predominant, naturally‐occurring phytosterols.
membrane‐spanning domain because seed phytosterol levels in tobacco plants expressing an N‐terminally truncated HMG‐CoA reductase lacking this domain were enhanced by up to 3.2‐fold (Harker et al., 2003). c. Sucrose phosphate synthase and nitrate reductase. Two other important enzymes, sucrose phosphate synthase (SPS) and nitrate reductase (NR), have been shown to be substrates for SnRK1. SPS is phosphorylated
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at Ser‐158 and NR at Ser‐543 (Bachmann et al., 1996b; Douglas et al., 1995; Su et al., 1996). In both cases phosphorylation results in inactivation of the enzyme, although the inactivation of NR also requires the binding of a 14‐3‐3 protein to the phosphorylation site (Bachmann et al., 1996a; Moorhead et al., 1996). SPS catalyzes the first step in the synthesis of sucrose, and the fact that SnRK1 potentially regulates SPS activity makes SnRK1 a possible key regulator of source to sink carbon flux and acclimation to carbon supply. Increased leaf SPS activity, for example, would result in more sucrose synthesis, and more sucrose would be available for export to sinks such as seeds and tubers. SnRK1 could be involved in the inactivation of SPS to reduce the export of sucrose from the leaf in response to environmental conditions that limit carbon supply. Phosphorylation at Ser‐158 causes an inactivation at subsaturating concentrations of the substrate, glucose‐6‐phosphate, and high concentrations of the inhibitor, phosphate (McMichael et al., 1993). Nitrate reductase catalyses the first step in the assimilation of nitrogen from nitrate into organic compounds such as amino acids. Although SnRK1 is only one of several protein kinases that phosphorylate nitrate reductase, this potential regulatory mechanism is particularly important because it could be a link between carbon and nitrogen signalling. d. Small heat shock protein (HSP). SnRK1 has been shown to interact with and phosphorylate a small heat shock protein from barley (Slocombe et al., 2004). Although the small HSP is a less eVective substrate than HMG‐ CoA reductase, it is phosphorylated at a specific phosphorylation site towards the N‐terminal end. This site does not conform to the consensus sequence for a SnRK1 target site, which probably explains why the small HSP is a relatively poor substrate. Some other small heat shock proteins are known to be phosphorylated. For example, mammalian small HSPs are substrates for MAPK‐activated protein kinase‐2 (Freshney et al., 1994; Rouse et al., 1994) and maize mitochondrial small heat shock protein HSP22 is phosphorylated significantly at the N terminus in vivo, although the protein kinase responsible has not been identified (Lund et al., 2001). At present, it is not known if N‐terminal phosphorylation of small HSPs by SnRKI leads to a change in function. 4. Redox regulation of ADP‐glucose pyrophosphorylase (AGPase) ADP‐glucose pyrophosphorylase is a plastidic enzyme that catalyses a key step in starch biosynthesis, the conversion of glucose‐1‐phosphate to ADP‐ glucose. Its activity is regulated to a great extent by post‐translational redox modulation; AGPase is a heterotetramer of two small and two large
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subunits, and the regulatory mechanism involves formation of a cysteine bridge between the two small subunits (Fu et al., 1998). Redox regulation of AGPase plays an important role in the control of starch synthesis in response to carbon supply in potato tubers (Tiessen et al., 2002). In tuber discs cut from plants and incubated in the absence of sugars, redox activation of AGPase decreases, but this can be prevented by feeding with either sucrose or glucose (Tiessen et al., 2003). Fascinatingly, palatinose, a nonmetabolisable analogue of sucrose, mimics the sucrose eVect, indicating that sucrose does not have to be metabolised to initiate a signal. Furthermore, sucrose‐ induced redox activation of AGPase does not occur in discs cut from tubers with reduced SnRK1 activity, whereas glucose‐induced activation does. This shows that sucrose‐ and glucose‐induced redox activation of AGPase involve diVerent signalling pathways and puts SnRK1 clearly in the sucrose sensing and signalling pathway but not, in this case, in the glucose sensing and signalling pathway. It also begs the question of how the signal is passed from the cytosol to the plastid, as there is no evidence of SnRK1 being present in plastids. 5. Involvement of SnRK1 in the regulation of gene expression The regulation of gene expression in response to sugars was first demonstrated by Jen Sheen in 1990. She used photosynthetic gene promoter/reporter gene fusions to show that seven maize photosynthetic genes were repressed by glucose or sucrose in a maize protoplast system. The expression of the ribulose 1,5‐bisphosphate carboxylase/oxygenase small subunit (RbcS) gene was shown to be reduced by glucose in cell suspensions of Chenopodium rubrum (Krapp et al., 1993); in the same system, chlorophyll a/b binding protein (Cab) and thylakoid ATPase delta subunit gene expression was reduced by glucose, whereas Cab gene expression was shown to be reduced by sucrose in oilseed rape cell cultures (Harter et al., 1993; Krapp et al., 1993). The demonstration that expression of photosynthetic genes is under feedback regulation by sugars was a landmark discovery (reviewed by Sheen, 1994). The list goes on: genes encoding isocitrate lyase and malate synthase, the two key enzymes involved in the glyoxylate cycle, were shown to be repressed by glucose (Graham et al., 1994). Similarly, the expression of genes encoding ‐amylase was shown to be induced by sugar starvation in rice suspension cultures and repressed by feeding with sucrose, fructose, or glucose (Yu et al., 1991). Conversely, the expression of a gene encoding ‐ amylase was found to be induced by sugars in rosette leaves of Arabidopsis (Mita et al., 1995). Nowadays, of course, broad pictures of eVects on gene expression can be gained by performing microarray experiments, and in 2004 Price and
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co‐workers showed that 444 Arabidopsis genes are upregulated by glucose, including those involved in biotic and abiotic responses, carbohydrate metabolism, N metabolism, lipid metabolism, inositol metabolism, secondary metabolism, nucleic acid related activities, protein synthesis and degradation, transport, signal transduction (e.g., protein kinases and phosphatases, and transcription factors), hormone synthesis, and cell growth or structure. A similar number (534) are downregulated. Section III.C.4 described the eVects of sucrose and glucose feeding on AGPase activity, noting that sucrose and glucose signalling involves diVerent signalling pathways. Experiments on the eVects of these two sugars on gene expression had already indicated that this was the case. For example, sucrose synthase activity increases in response to sucrose but is not aVected by glucose (Salanoubat and Belliard, 1989; Sowokinos and Varns, 1992). Fu and Park (1995) showed that this eVect is mediated at the level of gene expression; they described two diVerentially‐expressed potato sucrose synthase genes, one of which (SUS4) is expressed only in tubers under normal conditions but can be induced in detached leaves in response to incubation with high concentrations of sucrose. The other (SUS3) is expressed predominantly in stems and roots and is not induced by sucrose treatment. Neither gene responds to glucose. Sucrose synthase activity and the onset of starch biosynthesis have also been shown to coincide with an increase in sucrose levels and a decrease in hexose levels in the developing cotyledons of Vicia faba (Weber et al., 1996). Because sucrose synthase catalyses the reversible conversion of sucrose and UDP to UDP‐glucose and fructose, this finding is perhaps not surprising. Nevertheless, the discovery that sucrose can be sensed independently of glucose is an important one. It should be remembered when considering this that the eVects of sucrose and glucose depend in part on the presence in the tissue that is being studied of enzymes such as invertase, sucrose synthase, and sucrose phosphate synthase that interconvert them. If sucrose is cleaved to hexoses prior to entry into a cell, then it is unlikely to initiate a diVerent signal to glucose. Other examples of specifically sucrose‐ induced gene expression include a patatin gene in potato (Grierson et al., 1994) (patatin is the major storage protein in potato tubers) and a nitrate reductase gene in Arabidopsis (Cheng et al., 1992). So what role does SnRK1 play in sucrose or glucose regulation of gene expression? Such a role is suggested strongly by the ability of SnRK1 to complement mutations in SNF1 in yeast. One of the functions of SNF1 is the transcriptional regulation of genes encoding enzymes of carbohydrate metabolism. SnRK1 will perform this role in yeast snf1 mutants to the extent that the yeast can utilise sucrose and nonfermentable carbon sources such as
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ethanol and glycerol (Alderson et al., 1991; Muranaka et al., 1994). It should be emphasised that this results from the derepression of gene expression, not some other function of SNF1. Confirmation of a role for SnRK1 in regulating gene expression in plants was obtained in 1998 using potato plants expressing an antisense SnRK1 gene specifically in the tubers or leaves (Purcell et al., 1998). The expression of sucrose synthase was much lower in tubers expressing the antisense SnRK1 gene than in wild‐type and could not be induced by incubation of excised leaves expressing the antisense SnRK1 gene, again in contrast to wild‐type. Further investigations have shown that the expression of genes encoding ADP‐glucose pyrophosphorylase, ‐amylase, and sucrose phosphate synthase decrease as a result of antisense inhibition of SnRK1 gene expression in potato tubers, whereas both sucrose synthase and ADP‐ glucose pyrophosphorylase gene expression increases if SnRK1 is overexpressed (McKibbin et al., unpublished data). An ‐amylase gene promoter has also been shown to be repressed by antisense SnRK1 in wheat embryos (Laurie et al., 2003). SnRK1 therefore has the potential to control starch biosynthesis and mobilisation at multiple control points, at the levels of both gene expression and post‐translational modulation of enzyme activity, and in response to the levels of sucrose (sucrose synthase, AGPase) or glucose (‐amylase) (Fig. 14). Clearly, subtle regulation of SnRK1 itself and its downstream targets must determine whether starch is accumulated or mobilised. For example, antisense inhibition of SnRK1 may indicate that SnRK1 is required for the expression of a particular gene, but the presence or absence of transcription factors will determine whether SnRK1 regulates the expression of that gene in a specific tissue, cell type, or developmental phase. 6. SnRK1 is implicated in cell cycle control Antisense inhibition of SnRK1 induces a large mitotic cell size in potato cell cultures (Francis and Halford, unpublished data), suggesting that SnRK1 could cross‐talk with components of cell cycle signalling. In yeast cells, however, overexpression of SnRK1 causes a reduction in cell volume to one‐third of normal (Dickinson et al., 1999). There has been evidence of a link between metabolite signalling and the cell cycle in yeast for some time: snf1 mutants fail to arrest in the G1 phase of the cell cycle under conditions of nutrient deprivation (Thompson‐Jaeger et al., 1991) and have a shorter G1 period than the wild‐type (Aon and Cortassa, 1999). Furthermore, SNF1 is related to NIK1 of Saccharomyces cerevisiae and its homologue, NIM1, in Saccharomyces pombe (Fig. 10). NIK1 interacts with the CDC28 complex and is a negative regulator of
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Fig. 14. Points of influence and modes of action for SnRK1 in the starch biosynthetic pathway. Carbon ‘‘flow’’ through the pathway is shown with black arrows; signalling interactions are indicated with grey arrows.
SWE1, a protein kinase involved in the calcium‐dependent control of mitosis (Tanaka and Nojima, 1996). ELM1, one of the protein kinases upstream of SNF1, has also been implicated in the regulation of SWE1. ELM1 mutants have a prolonged mitotic delay, fail to regulate polar bud growth during mitosis, and are defective in cytokinesis (Sreenivasan and Kellogg, 1999). A role for SnRK1 in meristems was suggested by Pien et al. (2001) based on the finding that genes encoding SnRK1, sucrose synthase, and AGPase showed an asymmetric pattern of expression within tomato leaf meristems. A possible role for SnRK1 in meristems could be to link metabolic status to cell cycle control. 7. Phenotypic eVects of manipulating SnRK1 activity Manipulation of SnRK1 activity can have dramatic eVects on plant development, the most extreme of which is to prevent plant growth altogether. For example, eVorts to produce transgenic potato plants expressing antisense SnRK1 under the control of a constitutive promoter (CaMV35S) failed (Purcell et al., 1998). This was despite multiple attempts being made and the fact that successful transformation experiments were being performed alongside using the same antisense sequence but tissue‐specific promoters, suggesting that the failure resulted from a lethal eVect of the transgene during tissue culture.
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Transgenic Arabidopsis plants have now been produced expressing antisense and RNAi SnRK1 sequences under the control of a CaMV35S promoter (unpublished data). These were produced by the floral dip method so no tissue culture was involved, perhaps explaining why these transformation experiments were successful while those with potato were not. A ‘‘lethal’’ eVect has also been observed with expression of an antisense SnRK1 sequence in barley pollen (Zhang et al., 2001). Analysis of pollen grains carrying an antisense SnRK1 transgene showed that they had arrested at the binucleate stage of development, were small, pear shaped, contained little or no starch, and were nonfunctional. Carbohydrate metabolism plays an important role in pollen grain development, and pollen infertility is often associated with a lack of starch accumulation, brought about by mutation (Joppa et al., 1966) or physiological stress (Graham, 1975; Ito, 1978; Saini et al., 1984). Starch acts as a major energy source for development, germination, and tube growth (Baker and Baker, 1979; Clement et al., 1994; Franchi et al., 1996; Pacini and Franchi, 1988). It is possible that inhibition of starch accumulation caused the arrest in pollen development. A less severe phenotype, delayed sprouting, has been observed in potato cv. Desiree tubers expressing an antisense SnRK1 sequence (Halford et al., 2003b). The transgenic tubers do not sprout at all if kept at 4 8C, even after long‐term storage (Fig. 15), although they will sprout when potted up and transferred to a glasshouse. However, recent experiments with cv. Prairie tubers expressing an antisense SnRK1 sequence have failed to replicate this result (unpublished data), indicating that the genetic background plays an important role in the appearance of this phenotype. SnRK1 activity has also been manipulated in the moss, Physcomitrella patens (Thelander et al., 2004). The advantage of using this species is that
Fig. 15. Tubers from wild‐type potato cv. Desiree and transgenic potato cv. Desiree expressing an antisense SnRK1 gene.
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knockout mutants can be produced. Physcomitrella patens contains two SnRK1 genes, and the double knockout mutant shows a complex phenotype of abnormal development, premature senescence, hypersensitivity to auxin, hyposensitivity to cytokinin, and a requirement for continuous light. The requirement for continuous light may again indicate a perturbation in starch accumulation and breakdown, as this has been shown to be required for Arabidopsis to grow normally in a day/night cycle (Caspar et al., 1985, 1991; Lin et al., 1988). 8. Summary of ‘‘downstream’’ eVects of SnRK1 Like its fungal and animal counterparts, SNF1 and AMPK, SnRK1 can control aspects of carbon metabolism at multiple points, potentially aVecting sterol biosynthesis, the accumulation and breakdown of sucrose and starch (with implications for sucrose transport, storage organ development, and carbon partitioning), and the assimilation of nitrogen into organic compounds. It is also implicated in cross talk with cell cycle control mechanisms and in the control of development. Its ‘‘downstream’’ eVects are summarised in Fig. 16. 9. Upstream factors: activation of SnRK1 It has been something of a frustration that the metabolite that is sensed at the ‘‘top’’ of the SnRK1 signal transduction pathway has remained elusive. Feeding experiments with diVerent sugars and plant tissues have failed to give convincing, repeatable results, although glucose‐6‐phosphate has been shown to inhibit SnRK1 in vitro (Toroser et al., 2000). However, it is beginning to be teased out, and the candidates 50 ‐AMP and trehalose‐6‐ phosphate are stimulating considerable interest. Section III.A described the role of 50 ‐AMP as a signalling molecule in animal cells. This metabolite, which accumulates in animal cells as a result of nutrient and other stresses, activates AMPK allosterically. No such activation occurs with SnRK1 (or SNF1), but 50 ‐AMP does modulate the phosphorylation state of SnRK1 and therefore its activity. SnRK1 is regulated in vitro by phosphorylation on a threonine residue within the so‐called T‐loop (Sugden et al., 1999a); dephosphorylation and inactivation have been found to be inhibited by low concentrations of 50 ‐AMP (Sugden et al., 1999a). The implication of this is that 50 ‐AMP could activate the protein kinase upstream of SnRK1 (Fig. 17). Attempts to identify and purify this protein kinase in order to test this hypothesis have proved unsuccessful. However, this work has been given a new impetus by the identification of analogous protein kinases in humans (LKB1) and yeast (ELM1, PAK1, and TOS3). Although a clear homologue
Fig. 16. Targets and modes of action for SnRK1.
Fig. 17. Possible pathways for activation of SNF1‐related protein kinase‐1 (SnRK1). Carbon ‘‘flow’’ from glucose to CO2 is indicated with black arrows; signalling interactions are shown with grey arrows; and dotted lines are used where the mechanism for an interaction is not known.
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of these protein kinases does not exist in plants, there are a number of hitherto uncharacterised candidates from Arabidopsis (unpublished data). There is no doubt that post‐translational modulation of SnRK1 activity is important; experiments in potato have shown that, for example, activity in minitubers is over 40 times higher than in mature tubers while the levels of transcript do not diVer (Man et al., 1997). As described in Section III.B. T6P has an inhibitory eVect on hexokinase in yeast, thereby regulating flux into glycolysis. While it may not perform this exact function in plants, evidence has shown it to be an essential component of metabolic signalling (Eastmond et al., 2002; Pellny et al., 2004; Schluepman et al., 2003, 2004). Furthermore, increasing evidence shows that SnRK1 interacts with and possibly regulates the trehalose biosynthetic pathway. For example, several Arabidopsis trehalose phosphate synthases contain a SnRK1 target site, and expression of one of the two SnRK1 genes in Arabidopsis correlates with T6P content (Schleupmann et al., 2004). Trehalose feeding has been shown to induce the expression of AGPase and starch synthesis in Arabidopsis (Wingler et al., 2000), further evidence of a possible link between trehalose metabolism and SnRK1. Glucose itself is attractive as a signalling molecule because it is universal to all organisms as a source of energy and carbon skeletons. Yeast does sense glucose levels through the membrane‐located sensors SNF3 and RGT2 (Section III.B, Fig. 9), but these initiate signals only through the glucose induction pathway. The metabolite that is sensed to initiate a signal through SNF1 and the more important glucose repression pathway remains elusive. If glucose is a signalling molecule, then one possible mechanism through which it could be sensed is its interaction with hexokinase. In plants, hexokinase has been associated particularly with photosynthetic metabolism as a mechanism that links the carbohydrate status of leaves to photosynthetic gene expression as a means of feedback control (Jang et al., 1997; reviewed by Jang and Sheen, 1997). Proving that hexokinase is a glucose sensor and signalling molecule is diYcult because of its important metabolic role (Halford et al., 1999). Any attempt to alter hexokinase activity in transgenic or mutant plants or with inhibitors may cause changes in other potentially important signalling molecules downstream of hexokinase, such as glucose‐6‐phosphate and 50 ‐AMP. However, Moore and co‐workers (2003) used targeted mutagenesis of one of the Arabidopsis hexokinase genes, HXK1, to produce enzymes that were catalytically inactive; glucose binding still occurred but glucose‐6‐ phosphate was not formed. In transgenic plants the two catalytically inactive hexokinases mediated glucose‐dependent developmental arrest and repression of chlorophyll accumulation without altering catalytic activity
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or glucose‐6‐phosphate and fructose‐6‐phosphate content. This separation of catalytic and signalling functions is good evidence of a signalling role for hexokinase. Nevertheless, frustratingly given that the hexokinase signalling hypothesis was proposed in the mid‐1990s, there is still no convincing hypothesis of how hexokinase generates a signal or what signalling pathway transduces that signal. Hexokinase signalling appears to aVect gene expression, cell proliferation, root and inflorescence growth, leaf expansion, and senescence. Some of these eVects may be mediated through cross‐talk with light and hormone signalling. For example, there is good evidence for interaction and antagonism between hexokinase signalling, light, and cytokinin in the regulation of leaf senescence (Hwang and Sheen, 2001; Wingler et al., 1998). Evidence also shows that glucose signalling interacts with auxin signalling to promote or inhibit growth, depending on tissue or glucose concentration (Moore et al., 2003). Thus, many of the growth‐promoting and hormonal‐like properties of sugars may be explained in part through interactions between hexokinase and hormone signalling pathways. Hexokinase sensing and signalling cannot be the whole story as far as glucose sensing goes in plants is concerned because hexose levels in the vacuole or apoplast of tobacco plants have been shown to be sensed (Heineke et al., 1994; Herbers et al., 1996) and hexokinase is a cytosolic enzyme. It is also notable that the pathway for hexose phosphate production from sucrose via sucrose synthase (the predominant pathway in storage organs) does not involve hexokinase or the production of glucose at all (Fig. 17). Other candidates for glucose sensors are sugar transport proteins (STPs) (Fig. 17). Arabidopsis has 14 STP genes (reviewed by Sherson et al., 2003), the best characterised of which, AtSTP1, encodes a protein that transports galactose, xylose, and mannose, as well as glucose, and responds sensitively to extracellular sugar availability. The glucose to be transported is produced by the hydrolysis of incoming sucrose to glucose and fructose by cell wall invertases, of which Arabidopsis has six. The expression of diVerent invertases and STPs may enable the plant to change its hexose utilisation in response to diVerent environmental conditions; it has also been suggested that STPs have a role in hexose sensing and signal initiation (Sherson et al., 2003). Note that in some tissues and cell types sucrose is imported into the cell (Fig. 17), and the mechanism for fructose import into the cell is still unknown. Whether SnRK1 is involved in hexose sensing and signalling is not clear. Its involvement in regulating ‐amylase (‐AMY2) gene expression in cultured wheat endosperms (Laurie et al., 2003) suggests that it is. The ‐AMY2 gene is glucose‐repressible and starvation‐inducible, making it similar to glucose‐repressed, SNF1‐controlled genes in yeast. SNF1 activity
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does respond rapidly and sensitively to glucose levels (Wilson et al., 1996), although the sensing mechanism is not known. However, this has never been demonstrated unambiguously for SnRK1. SnRK1 certainly appears to be required for the transduction of signals that are initiated by sucrose. The evidence for this was described earlier; the involvement of SnRK1 in regulating sucrose synthase gene expression and AGPase activity in response to sucrose is quite clear. The fact that independent sensing of sucrose has evolved in plants is not surprising, as sucrose is found in all plants, is the end product of photosynthesis, the major transported sugar and the starting point for energy metabolism, and the synthesis of structural components of cells. Nevertheless, the involvement of SnRK1 is interesting because it does not perform a similar function in animals or fungi. It is not known what lies upstream of SnRK1 in the sucrose signalling pathway. However, sucrose transport in plants is mediated by proton‐ coupled sucrose transporters (SUT) (Lalonde et al., 1999, 2003). These SUT proteins are related structurally to the HXT transporters and related glucose sensors of yeast (Section III.B). The SUT transporters have diVerent aYnities for sucrose, with SUT1 being the high‐aYnity transporter and SUT4 the low‐aYnity transporter, while SUT2 appears to be a combined transporter and sensor (Barker et al., 2000; Weise et al., 2000). All three proteins have been localised in sieve elements (Reinders et al., 2002).
IV. THE LINK BETWEEN SUGAR AND ABSCISIC ACID/STRESS SIGNALLING PATHWAYS In the last few years there has been a burgeoning interest in understanding the genetics of cross‐talk between hormone and metabolic pathways, particularly ABA and sugar signalling (Brocard‐GiVord et al., 2003). This was stimulated in part by the results of screens carried out to identify Arabidopsis mutants that are impaired in their response to sugar (sugar response mutants). Several of the mutants identified in these screens turned out to be ABA related, leading to the hypotheses that sugar signalling is mediated directly by ABA (Arenas‐Huertero et al., 2000; Smeekens, 2000), that ABA modulates sugar signalling by priming tissues to respond to sugars (Rook et al., 2001), or that although essentially separate, ABA and sugar signalling converge and cross‐talk through specific factors (Halford and Paul, 2003). Such factors would be expected to be involved in the control of developmental events such as germination and seedling establishment that are sensitive to both ABA and sugars. One of the ABA‐related mutants implicated in sugar signalling is abi5 (ABA‐insensitive 5). Like all of the abi mutants, abi5 was isolated because of the ability of mutant seeds to germinate in the presence of normally
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inhibitory concentrations of ABA (Finkelstein, 1994). The ABI5 gene was found to encode a basic leucine zipper (bZIP) transcription factor that regulates expression of a subset of late embryogenesis‐abundant (LEA) genes (Finkelstein and Lynch, 2000; Lopez‐Molina and Chua, 2000). These LEA genes include AtEM1 and AtEM6. ABI5 is expressed most strongly in seeds but also in vegetative and floral tissues, where it is induced by ABA and stress treatments (Brocard et al., 2002). The ABI5 protein interacts with another transcription factor, ABI3, in two‐hybrid experiments (Nakamura et al., 2001). The two transcription factors have also been shown to act synergistically with one another in the activation of AtEM6, phaseolin, and barley HVA1 and HVA22 gene promoters in rice protoplast transient expression experiments (Gampala et al., 2002). Significantly, their action in these experiments was inhibited by overexpression of aba1–1, a dominant‐negative allele of protein phosphatase ABI1, suggesting that phosphorylation plays a part in their regulation. ABI3 encodes a B3‐binding domain transcription factor and is homologous to the maize gene VP1. Both ABI3 and VP1 have attracted interest because of the significance of VP1/ABI3 in controlling the transition between seed development and germination (Kurup et al., 2000; McKibbin et al., 2002). The product of another ABI gene, ABI4, is believed to be involved with ABI3 and ABI5 in a regulatory network (Brocard et al., 2002), although the nature of the interaction is not known. ABI4 encodes an Apetela2‐type transcription factor (Finkelstein et al., 1998). Overexpression of ABI3, 4, and 5 causes hypersensitivity to sugar as well as ABA, as measured by the ability to germinate in the presence of sugar/ ABA (Brocard et al., 2002). Mutations in ABI4 have been identified in a number of sugar response mutants: impaired sucrose induction‐3 (isi3), sucrose uncoupled‐6 (sun6), sucrose insensitive‐5 (sis5), and glucose insensitive‐6 (gin6). The abi5 mutant is also glucose and mannose insensitive (Arenas‐Huertero et al., 2000; Laby et al., 2000).
V. PROSPECTS Protein phosphorylation is one of the major mechanisms by which cells react to extracellular signals, regulate cellular processes, and respond to nutritional and environmental stimuli. The characterisation and functional analysis of protein kinases therefore represents an important target for plant scientists. SnRK1 and the genes that encode it have been characterised from the molecular level through to the identification of substrates and
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downstream eVects on sucrose synthase, ‐amylase, sucrose phosphate synthase, and ADP‐glucose pyrophosphorylase gene expression. These studies have placed SnRK1 firmly in the sugar sensing signal transduction pathway and at the heart of the control of carbon partitioning. Somewhat disappointingly, SnRK1 remains one of only a few plant protein kinases to have been characterised at the molecular and biochemical level. While less mature, studies on GCN2 in plants suggest that it plays a role in controlling amino acid biosynthesis in response to amino acid availability. A key question is to what extent is a general amino acid control system like that of yeast operating in plant cells. A great opportunity and challenge of the coming years is to exploit the rapidly expanding genomic data and the new ‘‘omics’’ technologies and bioinformatics to increase the pace of discovery in the elucidation of the signalling networks in which SnRK1 and GCN2 operate. The establishment of a consensus sequence for the target phosphorylation site in SnRK1 substrates makes the use of bioinformatics particularly appealing. However, the degeneracy within the target site and the tolerance of apparently any residue at some positions adjacent to the target serine (Fig. 12) make searches for proteins containing the site less than trivial, and specific search tools will have to be developed. Proteomic/phosphoproteomic analyses are based on the identification of proteins that become more or less abundant or are phosphorylated to a greater or lesser degree in response to a particular treatment. The proteins are identified by matrix assisted laser desorption ionisation time of flight (MALDI‐ToF) mass spectrometry (MS) and/or liquid chromatography‐ MS/MS. It should enable components of protein kinase cascades and their target enzymes and transcription factors to be identified much more rapidly than has been possible before. It may even be possible to identify the conduits between pathways that link them into networks. The feasibility of such an approach has been demonstrated in an analysis of the Arabidopsis plasma membrane (Nu¨ hse et al., 2004). This identified receptor‐like and other protein kinases, putative signalling proteins, transporters, ATPases, nuclear proteins, proteins involved in lipid metabolism, traYcking and cellolose synthesis, and others that are phosphorylated.
ACKNOWLEDGMENT Rothamsted Research receives grant‐aided support from the Biotechnology and Biological Sciences Research Council (BBSRC) of the United Kingdom.
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Opportunities for the Control of Brassicaceous Weeds of Cropping Systems Using Mycoherbicides
AARON MAXWELL AND JOHN K. SCOTT
Cooperative Research Centre for Australian Weed Management and The Commonwealth Scientific and Industrial Research Organisation (CSIRO) Entomology, PO Wembley, WA 6913, Australia
I. Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . II. Pathogens of Wild Radish . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. Biotrophic Pathogens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Necrotrophic Pathogens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . C. Host Specificity. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . III. Strategies to Increase Virulence or Specificity . . . . . . . . . . . . . . . . . . . . . . . . . A. Multiple Pathogens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Chemical Synergists . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . C. Phytotoxic Metabolites . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . D. Gene Manipulation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . IV. Epidemiology with Respect to Cropping Conditions . . . . . . . . . . . . . . . . . . . V. Inoculum Production and Formulation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . A. Industrial Scale Inoculum Production. . . . . . . . . . . . . . . . . . . . . . . . . . . . . B. Formulation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . VI. Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Acknowledgments . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
Advances in Botanical Research, Vol. 43 Incorporating Advances in Plant Pathology Copyright 2006, Elsevier Ltd. All rights reserved.
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0065-2296/06 $35.00 DOI: 10.1016/S0065-2296(05)43003-7
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ABSTRACT Mycoherbicides oVer another option in controlling weeds, especially in light of increasing problems with herbicide resistance. Wild radish is a weed of cropping systems for which pathogens found in Australia include a suite of species with diVering host range that could be developed into mycoherbicides useful against weed species from the Brassicaceae. Potentially useful fungal pathogens found in Australia are Alternaria alternata, A. brassicae, A. brassicicola, A. japonica, Fusarium oxysporum, and Hyaloperonospora parasitica. Mycoherbicide candidates are considered in terms of their host specificity, virulence, epidemiological properties, industrial scale inoculum production, and suitability for liquid or solid formulation. Another critical issue is how to avoid nontarget damage in crops of the Brassicaceae such as canola. Hyaloperonospora parasitica has potentially the most specific pathovars for the control of wild radish, but is not well suited for mycoherbicide production. Whereas Alternaria japonica is less host specific than H. parasitica, it is probably the most suited for development as a mycoherbicide. This review identifies opportunities to overcome some of the limitations associated with delivering reliable bioherbicide technology through improved identification of pathogens associated with Brassicaceae, a better understanding of their epidemiology, and possible modifications to improve their mycoherbicide potential.
I. INTRODUCTION The number and extent of herbicide‐resistant weeds are increasing worldwide, with populations of some weeds resistant to several diVerent herbicide groups. One approach to this problem is to develop plant pathogens into mycoherbicides against either a narrow or a broad spectrum of weed species. Although mycoherbicides have been used successfully in horticultural and aquatic situations where moisture is not limiting, their development has largely failed in cropping situations where moisture levels are low or unpredictable. Recent advances in biotechnology and plant pathology oVer ways to overcome some of the problems that have plagued the commercialisation of mycoherbicide candidates. This review explores how the some of these advances could be applied to select, develop, and improve mycoherbicide candidates. We use as a model the wild radish (Raphanus raphanistrum), which is one of Australia’s and the world’s most problematic herbicide‐resistant weeds. Weeds from the family Brassicaceae are a major problem in cropping and horticultural situations worldwide. In southern Australian cropping regions, important brassicaceous weeds include Brassica tournefortii Gouan, Capsella bursapastoris (L.) Medikus, Diplotaxis tenuifolia (L.) DC, Raphanus raphanistrum L., Rapistrum rugosum (L.) All., Sinapis arvensis L., Sisymbrium oYcinale (L.) Scop., Sisymbrium orientale L., and Sisymbrium thellungii O.Schulz (Heap, 2005; Jones et al., 2000; Lemerle et al., 2001). Weeds of cropping systems, of which brassicaceous weeds are an important component, are estimated to cost Australian agriculture at least $1.4 billion annually (Sinden et al., 2004).
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Raphanus raphanistrum is the most important brassicaceous weed species in Australia because of the cost of control and the development of multiple herbicide‐resistant populations. Some populations in southern Australia are resistant across four diVerent modes of action (Walsh et al., 2004): Photosystem II inhibitors such as atrazine; acetolactate synthase (ALS) inhibitors such as chlorsulfuron; auxin analogues such as 2,4‐D; and phyotoene desaturase (PDS) inhibitors such as diflufenican. One response to this problem is to use biological control, either the classical approach of introducing exotic biological control agents or the development of biopesticides from pathogens already present in Australia. At the species level, all known pathogens considered for classical biological control of R. raphanistrum are already recorded on brassicaceous crop or weed species in Australia (Scott and Jourdan, unpublished; Scott et al., 2002). However, recent developments in molecular taxonomic studies have detected cryptic pathogens of the Brassicaceae (Mendes‐Pereira et al., 2003), and it is likely more cryptic or otherwise unknown host‐specific pathogens will emerge, possibly in the Mediterranean regions that are the origins of wild radish. At present the classical biological control option does not seem feasible for wild radish in Australia. The other main biological control method is the use of bioherbicides, for which indigenous or locally established pathogens can be used. It appears that there are no mycoherbicides being developed for weeds in this family, although a diverse range of at least 18 non‐brassicaceous species is being targeted worldwide (Charudattan and Dinoor, 2000). This review focuses on the potential of developing pathogens found in Australia as mycoherbicides against wild radish.
II. PATHOGENS OF WILD RADISH According to published and unpublished herbarium records, 96 fungal species are recorded on brassicaceous hosts in Australia. Table I shows the 26 species found on Raphanus in Australia, recorded elsewhere on radish species (Williams, 1993) and present on other brassicaceous plants in Australia (consequently are potentially found on wild radish), and those species also associated with the crop canola. Although bacterial (Imaizumi et al., 1997) and viral (Charudattan et al., 2003) pathogens have been tested for the biological control of weeds, these are not considered in this review. In the following sections on biotrophic and necrotrophic pathogens, the species in Table I are considered and reduced to a short list (Table II) for further analysis on the priority for further research.
TABLE I A Comparison of Known Fungal Pathogens of Raphanus Recorded on Raphanus spp. and Brassica napus in Southern Australia Based on Cook and Dube´ (1989), Khangura et al. (1999), Kharbanda et al. (2001), Sampson and Walker (1982), Shivas (1989), Simmonds (1966) and Unpublished Herbarium Records from the Qld Herbarium, NSW Herbarium, Australian Pest and Disease Database (APDD) and the Western Australian Department of Agriculture Records (DAR) Host rangeb
Radish hostc
Canola hostc
Other hostsc
NA Oidium sp. NA NA
PV W PV N
þ þ þ
þ þ þ þ
þ þ þ þ
NA NA NA
N W W
þ
þ þ
þ þ
Sclerotium rolfsii Sacc. Alternaria alternata (Fr.) Keissler Alternaria brassicae (Berk.) Sacc. Alternaria brassicicola (Schw.) Wiltshire Alternaria japonica Yoshii Alternaria longissima Deighton and MacGarvie Botryotrichum piluliferum Saccardo and Marchal
W PV N N N N
þ
þ þ þ þ
þ þ þ þ þ
U
þ
þ
Pathogen (teleomorph)a Obligate biotrophs Albugo candida (Pers. ex. Chev.) Kuntze Erysiphe polygoni DC. Hyaloperonospora parasitica (Pers. ex Fr.) Fr. Plasmodiophora brassicae Wor. Facultative biotrophs Aphanomyces raphani Kendrick Phytophthora megasperma Drechsler Pythium acanthicum Drechsler Necrotrophs and hemibiotrophs Athelia rolfsii (Curzi) Tu and Kimbrough Unknown Unknown Unknown Unknown Unknown Chaetomium piluliferum J. Daniels
Pathogen (anamorph)
Unknown Glomerella cingulata (Stonem.) Spauld. and Schrenk Unknown Unknown Leptosphaeria maculans (Desmaz.) Ces. and De Not. Macrophomina phaeseolina (Tassi) Goid. Mycosphaerella brassicicola (Duby) Lindau in Engl. and Prantl Mycosphaerella capsellae Inman and Sivansen Unknown Unknown Thanatephorus cucumeris (A.B. Frank) Donk Unknown a
Colletotrichum coccodes (Wallr.) Hughes Colletotrichum gloeosporoides (Penz.) Penz. and Sacc Fusarium avenaceum (Corda: Fr.) Sacc. Fusarium oxysporum Schlecht. Emend Snyder and Hansen Plenodomus lingam (Tode ex Fr.) Ho¨ nel, formerly Phoma lingam (Tode: Fr.) Desmaz. Rhizoctonia bataticola (Tassi) E.J. Butler NA Pseudocercosporella capsellae (Ellis and Everh.) Deighton Sclerotinia minor Jagger Sclerotinia sclerotiorum (Lib.) de Bary Rhizoctonia solani Ku¨ hn (esp. zymogram group 5) Verticillium dahliae Kleb.
W W
þ
þ
W PV
þ
þ
N
þ
þ
þ
U N
þ
þ þ
N
þ
þ
þ
W W W
þ
þ þ þ
þ þ þ
W
þ
þ
Ninety‐six fungi are recorded from other brassicaceous hosts in Australia. Pathovar (PV) indicates that this species contains pathovars that may be specific to Raphanus, narrow host range (N) indicates that this species is recorded only on the Brassicaceae and may be specialised on hosts within this family, wide host range (W) indicates that this species is recorded across many genera, including those outside the Brassicaceae, uncertain host range (U) indicates that the host range is unclear from the published literature. c þ, recorded on this host. Other hosts refer to other Brassicaceae. b
TABLE II Matrix Indicating Criteria for Mycoherbicide Suitability Against Fungal Pathogens of Raphanus
Pathogen
Likely virulencea
Alternaria alternata Alternaria brassicae Alternaria brassicicola Alternaria japonica Fusarium oxysporum Leptosphaeria maculans Mycosphaerella capsellae
L‐H M M H M M M
Industrial inoculum production in similar taxa Solid Solid Solid Solid
and biphasic and biphasic and biphasic and biphasic Liquid Nil Nil
Formulation suitabilityb
Epidemiological traits suited to Australian cropping systems
Priority for future research
WOW WOW WOW WOW Solid; alginate U U
Yes Mediteranean and temperate Warmer northern zone Yes U Yes U
Low High High High High Low Low
a Virulence is based on the proportion of articles published since 1994 referring to pathogenicity on Raphanus species and from reports on the impact of each pathogen species on R. raphanistrum or where unavailable on R. sativus; Low (L), Moderate (M), High (H). b WOW, water, oil water; U, unknown.
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A. BIOTROPHIC PATHOGENS
Obligate biotrophic pathogens such as the four listed in Table I are usually not appropriate for development as mycoherbicides because they cannot be cultured artificially. It may be possible to grow Hyaloperonospora parasitica (¼Peronospora parasitica) or another of the obligate biotrophic species on a brassicaceous hosts and then distribute infected straw on farms in an augmentative control strategy, for example, to speed up the reinfection process where there is low survival of a useful pathogen over summer. H. parasitica is the most frequently recorded biotrophic disease on Raphanus and it has host‐specific races (Dickinson and Greenhalgh, 1977; Greenhalgh and Dickinson, 1975; Satou and Fukumoto, 1996; Silue´ et al., 1996) and possibly distinct species specialising on Raphanus (Choi et al., 2003). Therefore, H. parasitica is the most promising candidate for the biological control of wild radish using this strategy. Facultative biotrophs such as Aphanomyces raphani can be grown on artificial media, but their requirements for sporulation may be more stringent than for necrotrophic fungi (Singh and Pavgi, 1977). The mycoherbicide DeVine is a formulation of the facultative biotroph Phytophthora palmivora for the control of strangler vine in citrus orchards and hence this group of pathogens shows potential for mycoherbicide development. Of the three facultative biotroph species considered in Table I, A. raphani is the only one that may be suYciently host specific to consider for mycoherbicide development. This pathogen infects plant roots primarily via the production of motile zoospores that require free soil moisture. Therefore the biology of this species may not be ideal for mycoherbicide development against wild radish in Australia where the cropping areas have highly seasonal rainfall and free soil moisture is short‐lived. It may be possible to overcome this limitation through appropriate formulation and targeting the timing of application to coincide with predicted rainfall events early in the season when radish seedlings are emerging.
B. NECROTROPHIC PATHOGENS
The necrotrophic and hemibiotrophic pathogens recorded on brassicaceous hosts (Table I) are generally more suited than biotrophic species for development as mycoherbicides because they can be mass produced more readily. Seven promising candidates were identified from Table I on the basis of evidence of host specialisation within the Brassicaceae and then compared against their fit to criteria desirable in a mycoherbicide (Table II). Although not all of these species are recorded on wild radish in Australia, they are
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recorded from cultivated radish or wild radish elsewhere. All of these fungal species are present in Australia, and isolates obtained could be screened for their eYcacy in causing disease on the desired host weed. Colletotrichum higginsianum is an additional species of interest that has not been recorded in Australia. However, it is possible that the recording of Colletotrichum gloeosporoides is actually C. higginsianum because the former is morphologically plastic and has been confused with C. higginsianum (Sutton, 1980). This is likely because C. higginsianum is a species that specialises on brassicaceous hosts. If further research clarifies this situation, then C. higginsianum would be added to the list of species in Table II. In order to develop one of these necrotrophic or hemibiotrophic pathogens into a mycoherbicide, the following principles need to be addressed. First, the pathogen needs to be suitably host specific and virulent on the target weed; second, it must be suitable for industrial scale inoculum production; third, the conditions that are required to produce a disease epidemic need to be well understood; and finally, the formulation of the product needs to be optimised to maximise disease development, be robust in transport and long‐term storage conditions, and be compatible with spray technology on the farm. The pathogens identified as potential candidates for mycoherbicide development against brassicaceous weeds are considered in light of these requirements. C. HOST SPECIFICITY
Based on molecular and hybridisation evidence, wild radish is very closely related to cultivated radish (Snow et al., 2001) and is closely related to brassica crops. Raphanus is estimated to have diverged from the B. rapa/B. oleracea lineage more recently than B. nigra diverged from the B. rapa/B. oleracea lineage (Yang et al., 2002) (Fig. 1). Thus host specificity is the most important element to consider when selecting pathogens for further study. Significantly, although Raphanus is a monophyletic genus, Brassica is polyphyletic and some species such as B. oxyrhina are more closely related to Raphanus than to most other Brassica species (Warwick and Sauder, 2005). Therefore, host range testing needs to be based on the recent molecular phylogeny of the Brassicaceae rather than relying on current taxonomic generic placement of taxa. Fusarium oxysporum has a broad host range and attacks both monocot and dicot hosts. However, within this species there are host‐specific pathovars. In some cases these pathovars may have diVerent chromosome numbers, be phylogenetically distinct, and could represent actual species, for example, F. oxysporum f. sp conglutinans VCG 0101 and F. oxysporum
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Fig. 1. Phylogenetic tree for Brassica rapa (Br), Brassica oleracea (Bo), Brassica nigra (Bn), Raphanus sativus (Rs) and Lepidium virginicum (Lv) reconstructed from nucleotide substitution (k) data of four intergenic spacers in the trnT–trnF and trnD– trnT fragments. When more than one sequence is available for a particular OTU, the values of K are the mean of all possible pairwise comparisons, as described in Wolfe et al. (1987). Reprinted from Yang et al. (2002) with permission from Elsevier.
f. sp. raphani VCG 0102 (Momol and Kistler, 1992). There are three forma speciales associated with Brassicaceae hosts, and Fusarium oxysporum f. sp. raphani is the most specialised to attack Raphanus (Bosland and Williams, 1987). This pathovar has been characterised by nuclear DNA markers that correspond to virulence on Raphanus hosts (Momol and Kistler, 1992). In a molecular study, Baayen et al. (2000) determined that both monophyletic and non‐monophyletic forma speciales occur in F. oxysporum and speculated that this pattern could be explained by the horizontal gene transfer amongst or between Fusarium species, conferring virulence on a particular host. Alternatively, the pattern of phylogenetically unrelated forma speciales of the same host could be due to the independent evolution of pathogenicity genes against a given host in diVerent lineages of F. oxysporum. Although there is some evidence for the monophyletic origins for three forma speciales of F. oxysporum specialising on diVerent Brassicaceae hosts (Kistler et al., 1987; Kistler et al., 1991; Momol and Kistler, 1992), the molecular phylogeny of these taxa remains unresolved and they may represent distinct species. Although F. oxysporum is recorded on Brassicaceae hosts in Australia, F. oxysporum f. sp. raphani, which attacks Raphanus, has not and its presence would need to be ascertained before this pathogen could be considered for local development as a bioherbicide. Leptosphaeria maculans is pathogenic on wild radish and other brassicaceous species. There is evidence of some degree of host specialisation within the L. maculans species complex (Chen and Seguin‐Swartz, 1999; Johnson and Lewis, 1994), and recent phylogenetic evidence suggests that there are at
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least two species within this complex, which includes the recently described L. biglobosa (Mendes‐Pereira et al., 2003). Chen and Seguin‐Swartz (1999) found variability amongst R. raphanistrum individuals in terms of their susceptibility to L. maculans, which suggests that selection for resistance to this pathogen could develop across wild radish populations following repeated exposure to the proposed mycoherbicide. In addition to this limitation, mycoherbicides based on the sexual (Leptosphaeria) or asexual (Plenodomus/Phoma) stages of this genus have not been developed and therefore industrial scale production of propagules may not be cost eVective. Finally, L. maculans is a major pathogen of canola (Howlett, 2004; Williams, 1992) and any mycoherbicide based on this pathogen will need to be of significant benefit to oVset any risks to farming activities. Rhizoctonia solani is pathogenic on a broad range of hosts, but zymogram groups within this species complex are diVerentially pathogenic according to host. In a study of R. solani from crops and weeds in Australia, isolates from ZG5 (AG2‐1) resulted in 100% inhibition of R. raphanistrum seedling emergence compared to 72 and 64% inhibition of B. napus and Triticum aestivum seedling emergence, respectively (Khangura et al., 1999). Therefore, although this pathovar shows some degree of specialisation, it still causes considerable damage to two of the most important crops in southern Australia. The R. solani groups are therefore unlikely to be of any value as a potential mycoherbicide against wild radish. Furthermore, Rhizoctonia does not produce spores in culture and industrial scale propagule production of this pathogen is likely to be diYcult. There are four species of Alternaria that show some degree of host specialisation on brassicaceous species: A. alternata, A. brassicae, A. brassicicola, and A. japonica. The first of these, A. alternata, forms a complex that contains many host‐specific pathovars on non‐brassicaceous taxa, many of which appear to be determined by the production of host‐specific toxins (HSTs) (Hatta et al., 2002; Kusaba and Tsuke, 1994). However, there is no published information on the existence of isolates uniquely pathogenic on Raphanus or that produce HSTs specific for either Brassica or Raphanus species. Of the three remaining Alternaria species; A. japonica is the most frequently cited on Raphanus and is reported as being most specialised for that genus (Rotem, 1994), A. brassicicola appears to be most common on B. oleraceae, and A. brassicae is associated most frequently with oilseed rape B. campestris (Humpherson‐Jones, 1992; Humpherson‐Jones and Phelps, 1989; Sharma and Kolte, 1994). According to a study of pre‐ and post‐ penetration events across eight brassicaceous hosts (not including Raphanus species), A. brassicicola was the least specialised, A. brassicae was most
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specialised for infection of B. nigra, and A. japonica was most specialised for infection of Sinapis alba. In another study, the species most susceptible to A. brassicae was B. nigra followed in order of least to greatest resistance by B. juncea, B. campestris, B. napus, B. oleracea, and B. carinata (Bansal et al., 1990). None of the necrotrophic species discussed, with the possible exception of F. oxysporum f. sp. raphani, are uniquely pathogenic on Raphanus and hence all pose a risk to canola in terms of mycoherbicide development. Of the necrotophic genera discussed, Alternaria and Fusarium are the most promising for mycoherbicide development in terms of their potential for industrial scale inoculum production. For this reason the following discussion on virulence, inoculum production formulation, and epidemiology focuses on these two genera.
III. STRATEGIES TO INCREASE VIRULENCE OR SPECIFICITY A. MULTIPLE PATHOGENS
Plant disease may be more destructive when combinations of pathogens are involved (Jeger, 2001). Synergistic interactions between pathogens used in weed biological control have been recorded for Cirsium arvense (Guske et al., 2004) in Germany and Xanthium occidentale in Australia (Morin et al., 1993a,b). The potential for synergistic pathogen interactions is an area that requires more exploration and in particular the possibility of applying biotrophic and necrotrophic pathogens simultaneously. Plant defense response to these types of pathogens is upregulated according to two diVerent biochemical pathways: salicylic acid (SA) and jasmonic acid/ethylene (JA), respectively (Tierens et al., 2002). Therefore, a simultaneous assault by the two types of pathogen may render the host more susceptible to disease. Pathogen combinations that could be considered for wild radish include A. japonica and H. parasitica or A. japonica and Aphanomyces raphani. Unless advances in tissue culture or biotechnology enable H. parasitica to be grown in vitro, this pathogen would need to be applied as an infected radish straw‐based formulation. The Alternaria could be sprayed as a foliar mycoherbicide after the radish has emerged early in the cropping phase, but it would be more cost eVective if it were applied as a solid formulation along with radish straw. Similarly, Alternaria and Aphanomyces would be applied simultaneously in a solid formulation such as ‘‘stabileze’’ (Quimby et al., 1999) early in the cropping season to target emerging wild radish seedlings.
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Some chemical herbicides make plants more susceptible to disease either via interference with the physical barriers of the plant to attack or to the biochemical defense pathways of the host. The coupling of chemical growth regulators or herbicides with pathogens has resulted in synergistically higher rates of weed control in many situations (Grant et al., 1990; Hoagland, 1996, 2001; Schnick and Boland, 2004; Tierens et al., 2002). A number of chemical compounds and fungal taxa have been tested that may also be suitable for use against brassica weeds. Probably the earliest recorded herbicide–pathogen interaction against host plants include glyphosate with the pathogens Phytophthora megasperma and Alternaria cassiae against soybean (Keen et al., 1982) and Senna obtusifolia (Cassia obtusifolia) (Sharon et al., 1992), respectively. The application of glyphosate inhibits the enzyme 5‐enolpyruvylshikimate 3‐phosphate synthase, which is involved in the production of plant defense compounds such as phytoalexins. The application of sublethal doses of glyphosate to S. obtusifolia suppressed the accumulation of phytoalexins in response to Alternaria cassiae inoculation and led to a fivefold reduction in the amount of conidia required to kill the plants (Sharon et al., 1992). At the same time there was no increase in susceptibility of the closely related non‐target crop plant Glycine max. A similar interaction with glyphosate has been recorded for the fungal taxa Colletotrichum (Le´ ger et al., 2001) and Fusarium avenaceum (Oleskevich et al., 1998). This suggests that pathovars of Alternaria alternata, A. brassicae, A. brassicicola, A. japonica, and Fusarium oxysporum could be tested for synergistic interactions with glyphosate in controlling brassicaceous weeds such as R. raphanistrum. Watson and Ahn (2001) also noted that chemicals such as thidiazuron (a plant growth regulator) and basagram (a herbicide) have been applied with Colletotrichum coccodes to control Abutilon theophrastii. These chemicals may decrease the capacity of the plant to outgrow the disease. Bromoximal þ MCPA, Metribuzin, Diclofop, Imazethapyr, and Sethoxydim have been used in combination with Colletotrichum gloeosporioides f. sp. malvae to control Malva pusilla (Grant et al., 1990). Some of these chemicals inhibited spore germination and the chemical and biological agents had to be applied separately in order to generate a positive interaction for weed control. Hoagland (2001) lists several other herbicides for which synergistic interactions with four pathogens have been patented and all of these pathogens belong in the genera Alternaria, Colletotrichum, and Fusarium. Significantly, none of these interactions led to an increase in the host range of the pathogens tested (Hoagland, 1996).
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C. PHYTOTOXIC METABOLITES
There is a long list of phytotoxic metabolites that are derived from fungal pathogens such as brefeldin A (Vurro et al., 1998), cercosporin (Assante et al., 1977), colletotrichin (Duke et al., 1992), destruxins (Buchwaldt and Jenson, 1991), fumonisins, and AAL toxin (Abbas et al., 1995; Gelderblom et al., 1988). These could potentially be developed into chemical herbicides or applied in conjunction with a pathogen of wild radish in order to increase disease expression synergistically. Vurro et al. (1998) found that some of these phytotoxic compounds, such as brefeldin A from Alternaria, suppress plant defense enzymes at very low concentrations, even below those required for phytotoxic symptoms such as tissue necrosis. Most of these phytotoxic compounds have a broader host range than the pathogen from which they are derived (Hoagland, 2001) and therefore the use of these metabolites would need to be accompanied by the breeding of resistance in crop plants. For example, destruxins, which are produced by Alternaria brassicae (Buchwaldt and Jenson, 1991), cause necrosis to a much greater range of plants than A. brassicae from which it was isolated. There are at least 36 of these compounds that are diVerentially toxic to various plant and insect species (Pedras et al., 2002). Destruxin B is most phytotoxic to Brassica species and its toxicity decreases according to increasing phylogenetic distance from this genus (Buchwaldt and Green, 1992). There may be other destruxins in this class of compounds that are more toxic to Raphanus and the identification of such compounds could be achieved by screening isolates of A. brassicae and A. japonica from radish hosts. Some of the other pathogens listed in Table I, such as Alternaria japonica, could be tested for the production of phytotoxic compounds against brassica weeds. These metabolites could be developed into chemical herbicides, for example, as occurred with glufosinate and bialaphos, which were developed from a herbicidal strain of a streptomycete. Bialophos is unique in terms of herbicides in that it is produced via a fermentation process. Glufosinate is the synthetic ammonium salt of phosphinothricin (PPT), and resistance to this herbicide has been conferred on over 20 crop plants (Hoagland, 2001), including Brassica napus (Stringam et al., 2003), via the insertion of either bar or pat genes from Streptomyces hygroscopicus or S. viridochromosgenes, respectively. The identification of new compounds from fungal pathogens could lead to similar developments for controlling brassica weeds in a broad range of crops, including those in the Brassicaceae. Another possibility is to introduce genes for phytotoxic compounds into a minor pathogen to create hypervirulence.
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Amsellem et al. (2002) and Gressel (2001) have proposed coupling virulence genes with fail‐safe mechanisms to prevent spread and transgene introgression into crop pathogens in order to improve a mycoherbicide (Fig. 2). Strategies to prevent hypervirulent pathogen spread include creating asporogenous mutants that require an exogenous chemical or defined media to sporulate or that are only capable of infecting via artificial spores. Introgression of transgenes to other fungi would be restricted by flanking the virulence genes with mitigator genes such as antisporulation or antimelanin genes that would reduce the fitness of a fungus that received the gene. Amsellem et al. (2002) demonstrated that adding Fusarium virulence genes to the fungus Colletotrichum coccodes increased its pathogenicity to the weed Abutilon theophrasti without changing the pathogen host range. Genes coding for plant toxins could also be introduced into host‐specific pathovars of brassicaceous weeds. Pathogens (hypervirulent or otherwise) could also be
Fig. 2. Fail‐safe mechanisms for hypervirulent biocontrol agents. Dual fail‐safe mechanisms to prevent (step 1) spread of biocontrol agents and (step 2) their introgression into other organisms. a, chlamydospores; b, microconidia; c, macroconidia; d, ascus with ascospores; e, sclerotia; f, asporogenic mycelia. Reprinted from Gressel (2001) with permission from Elsevier.
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modified genetically to reduce their persistence and dissemination by knocking out genes associated with sporulation or modifying with mating type genes. These traits are especially important for targeting brassicaceous weeds in order to reduce the impact on closely related, nontarget brassicaceous crops such as canola. Ideally, the candidate gene product should be specifically phytotoxic for wild radish and be under the control of one or a few closely linked genes. Destruxins are one group of phytotoxic metabolites that may have this potential. Because a destruxin gene has been cloned from M. anisopliae (Bailey et al., 1996), it should be possible to clone destruxin B and other destruxin genes phytotoxic to Raphanus hosts. This will facilitate the genetic transformation of a candidate mycoherbicide or at least the selection of virulent isolates. Genes from A. brassicae coding for destruxins could be inserted into another host‐specific pathogen such as F. oxysporum f. sp. raphani or a weak pathogen such as Colletotrichum higginsianum. The gene would be introduced under the control of a promoter that is induced during infection or under the control of a chemically induced promoter such as the ethanol‐ induced alcA gene promoter. In the latter scenario, the mycoherbicide and ethanol could be applied together to induce the gene. This would limit the virulence of this pathogen to the initial infection of the weed and reduce the risk to subsequent crops of a related species such as canola to which the organism may also be a weak pathogen. The alcA gene from Aspergillus could be suited to this role because it is a widely used system for the induction of heterologous genes in a range of organisms, including other fungi as well as plants and animals. Nikolaev et al. (2002) have successfully transferred a heterologous gene construct under the control of the alc promoter into a fungal species that lacks the inducible alcA gene. They transferred the inducible and strongly expressed alcA gene encoding alcohol dehydrogenase I from Aspergillus nidulans together with the activator gene alcR in the industrial fungus Aspergillus niger. Induced expression of the alcA gene was similar in the transformed A. niger to the donor A. nidulans, as monitored by alcA transcription, alcohol dehydrogenase activity, and heterologous expression of the reporter enzyme, ‐glucuronidase (Fig. 3). It has also been shown that the expression of genes under the control of the alcA promoter is dose dependent and reversible. Using alcR alcA:Gus reporter constructs, Roslan et al. (2001) found that transgene expression in Arabidopsis reached a peak five days after ethanol induction and by 11 days after induction expression had fallen to levels only marginally above the noninduced state. Therefore the production of a phytotoxin under the control of this inducible promoter
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Fig. 3. ‐Glucuronidase (GUS) activity of A. niger and A. nidulans transformants containing gpd:alcR and palcA:uidA constructs. (A) Kinetics of GUS activity of A. niger transformant containing gpd:alcR and palcA:uidA genes grown under various growth conditions: noninduced conditions (NI, ); induced by 50 mM EMK ( ); induced by 1% ethanol (Et, ); and repressed by 1% glucose in the presence of 1% ethanol (EtG, ). GUS activity was followed up to 12 h and expressed in units per milligram as described in Section II. (B) Kinetics of ‐glucuronidase activity in A. niger and A. nidulans transformants containing gpd:alcR and alcA:uidA genes grown in the presence of 0.1% yeast extract and induced with 1% ethanol up to 12 h. Transformants in A. niger ( ) and A. nidulans ( ) are shown. GUS activity was expressed in units per milligram as described in Section II. (Reprinted from Nikolaev et al., 2002 with permission from Elsevier.)
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could be limited to the time of application after which the production of the phytotoxin would fall and the organism would remain relatively benign to subsequent brassica crop plants. Ideally, a mycoherbicide based on high expression of a phytotoxic metabolite should be developed in conjunction with crop plants that are resistant to the phytotoxin either through host selection or the introduction of genes
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for disabling the phytotoxin. A potential source of resistance to destruxin B is Sinapis alba, which is resistant to A. brassicae partly because it detoxifies destruxin B rapidly via sequential hydroxylation and glucosylation processes (Pedras et al., 2000, 2001). The breakdown product of this process, hydroxydestruxin B, also induced defense‐related phytoalexins in the resistant species S. alba but not in the susceptible species B. napus. Sharma et al. (2002) evaluated 38 Brassicaceae species for resistance to A. brassicae and identified 8 highly resistant species that could prove useful sources of resistance for introgression to crop species. Resistance genes against Alternaria pathogens have been introduced into Brassica crop plants from diverse sources, including fungi (Mora and Earle, 2001) and unrelated plant species (Kanrar et al., 2002). Potentially F. oxysporum is a good candidate pathogen for gene manipulation because protocols for genetic transformation have been developed for this species (Momol and Kistler, 1992). However, the fact that this species is also a pathogen that kills immune compromised mammals, including humans (Ortoneda et al., 2004), may make it an especially contentious pathogen to modify genetically. The safest strategy would be to utilise knowledge gained via techniques such as targeted gene knockout and genomics research (Gold et al., 2001) to further understand pathogenesis and then select or modify virulent isolates of A. brassicae or A. japonica in conjunction with breeding resistance in susceptible crop species such as canola. Other fungal metabolites with phytotoxic activity include cercosporin, fumonisins, and the related AAL toxins. However, these are also mammalian toxins and therefore not likely to be developed into herbicides in their own right. It may be possible to insert genes for these compounds into host‐specific pathogens of brassicaceous weeds in a similar way to that suggested for destruxins. Mycotoxins are thought to be short‐lived in the environment (Hoagland, 2001) and some, such as fumonisin B, are excreted rapidly when ingested by non‐human primates (Shephard and Snijman, 1999). Mycotoxins have been associated with an increasing number of human health problems (Hoagland, 2001). Therefore the potential detrimental aVects of using a mycotoxin‐producing bioherbicide would need to be studied carefully in order to identify risks to human health and to determine the safety of their use. The risks associated with genetically manipulated organisms are managed through the appropriate legislation, and the requirements may change from one nation to another. In Australia, these risks are managed through the regulatory framework of the Gene Technology Act 2000 and the Gene Technology Regulations that came into eVect on June 21, 2001. Any genetically modified mycoherbicides against brassicaceous weeds would be subject to this process.
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IV. EPIDEMIOLOGY WITH RESPECT TO CROPPING CONDITIONS Mycoherbicide applications aim to maximise initial infection rates and rely on disease development to kill plants at the early seedling stage. The initial establishment of disease is critical and for this reason formulations are designed to increase infection rates by maintaining moisture levels at the infection surface. However, the success of a mycoherbicide may also depend on subsequent polycyclic disease dynamics, which include variables identified by Van der Plank (1963, 1984), such as the length of the latent period, the number of infection cycles in a season, host resistance, and external (environmental) factors. If the plant is able to outgrow the initial infection, then the continuous production of spores and the reinfection of growing points on the plant are likely to be important in the eventual success of the disease epidemic. All three Alternaria species specialising on Brassicaceae will infect the host at all developmental stages and may cause seedling stunting or death (Valkonen and Koponen, 1990). Disease development associated with A. brassicae and A. brassicicola increases with host age and can impact severely on pod development, leading to reduced seed set and seed viability (Humpherson‐ Jones, 1992). Sporulation in all three Alternaria species is rapid (12–48 h in vitro) (Humpherson‐Jones and Phelps, 1989), and the latent phase of infection is brief (Verma and Saharan, 1994). Because these species cause disease on all host stages and result in polycyclic epidemics, they are good candidates for mycoherbicide development against brassicaceous weeds. There is an interaction between temperature and humidity for the induction of sporulation in all three species. At 208C a minimum of 87 and 83% relative humidity is required for sporulation of A. brassicae and A. brassicicola, respectively (Humpherson‐Jones and Phelps, 1989). In vivo, the optimal sporulation temperature for A. brassicae is lower (18–248C) than for A. brassicicola (20–308C) (Humpherson‐Jones and Phelps, 1989). Although all three species are able to germinate and infect their hosts relatively quickly, provided that free moisture is available, A. brassicae is most rapid and infection occurs within 6 h at optimal temperatures compared to 18 h for A. brassicicola (Humpherson‐Jones, 1992). Free moisture as rain, dew, or 100% humidity for a minimum of 9–18 h at optimal temperatures between about 20 and 308C is required for infection by all three species. Alternaria brassicae has the lowest optimal temperature range for germination (21–288C) and infection (19–218C) of the three species (Degenhardt et al., 1982). The optimal temperature for germination is 28–318C in A. brassicicola and 23–318C for A. japonica, and the optimal
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temperature for infection is 25–278C for A. brassicicola and 17–298C for A. japonica (Degenhardt et al., 1982). The temperature requirements of A. brassicae and A. japonica are within the range typical of the early part of the cropping season in temperate or Mediterranean climates. In Australia, temperatures in the Western Australian cropping region (April–May) are likely to range from 8 to 278C (Anonymous, 2005a). Cropping regions of southwest Australia are characterised by a Mediterranean type of climate with cool wet winters and hot dry summers (Love, 2005). The cropping zone of south‐eastern Australia is characterised by a temperate climate, with spring rainfall and temperatures within the range required for Alternaria infection during the early part of autumn (Anonymous, 2005b). Cropping is usually restricted to winter unless irrigation is used. The temperature requirements for A. brassicicola are higher and therefore a mycoherbicide based on this species is likely to suit a warmer subtropical climate. The cropping zone of northern New South Wales and southern Queensland is characterised by a tropical to subtropical climate. Alternaria japonica is less well studied, but appears to have a greater range of climatic suitability, is more specialised on Raphanus, and therefore appears to be the best candidate overall. An advantage in the suitability of an organism for mycoherbicide development would be a capacity to germinate under conditions of repeated short moisture periods. This is because extended periods of wetness in Australian cropping areas are not reliable. However, Bailey (2004) found that A. cirsinoxia was able to infect and cause disease on Canada thistle (Cirsium arvense) under intermittent leaf wetness and drying, although viability and disease expression was less than that recorded for continuous wetness of 24–48 h, and a similar pattern may be true for Alternaria species attacking Raphanus. Another epidemiological trait of Alternaria species is their capacity to survive in plant debris or soil to provide inoculum for disease outbreaks in subsequent seasons (Rotem, 1994). Alternaria brassicae and A. brassicicola remain viable for a long period of time as spores on seed coat or as mycelium in seed as well as in infected plant debris for up to 12 weeks or more (Humpherson‐Jones, 1989). This could present problems if these pathogens were developed as a mycoherbicide because they may cause disease in susceptible brassica crops planted in subsequent seasons. This could be managed through selecting strains that are non‐pathogenic to canola, developing non‐sporulating mutants, breeding resistant canola varieties, and by leaving a break period between the use of the mycoherbicide and the
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planting of canola. A break period has been identified as the solution to this type of issue for the biological control fungus Sclerotinium sclerotorium in pastures (Bourdoˆ t et al., 2000; De Jong et al., 2002).
V. INOCULUM PRODUCTION AND FORMULATION A. INDUSTRIAL SCALE INOCULUM PRODUCTION
Because inoculum is of fundamental importance in disease initiation and development, maximising inoculum production through industrial scale fermentation techniques and through appropriate formulation is of prime consideration in developing a mycoherbicide. Propagule production may be achieved in either a liquid or solid‐state fermentation process. Liquid fermentation is preferred because it is the most cost‐eVective technology for growing fungi, but solid state fermentation is often more conducive to fungal spore production (Lomer et al., 2001). Purifying spore preparations from submerged fermentation systems involves centrifugation or filtration techniques that are considered easier and result in a less bulky formulation than techniques for recovering spores from solid‐state or biphasic systems (Auld and Morin, 1995). However, a cyclone air stream technology for the separation of conidia from solid‐state systems has been developed that is viable commercially (Lomer et al., 2001). Of the species listed in Table II, industrial scale inoculum production has previously only been considered for Alternaria and Fusarium genera. In general, Alternaria has been considered as a bioherbicide in other systems (Bailey, 2004; Green and Bailey, 2000; Green et al., 2001; Walker and Boyette, 1986). This genus usually does not produce conidia in liquid culture but will do so in solid‐state fermentation (Daigle et al., 1998; Masangkay et al., 2000). In contrast, Fusarium conidia can be produced in liquid culture (Amsellem, 1999; Quimby et al., 2001). The method of conidia production may aVect the characteristics of the conidia produced with respect to long‐ term viability and spore surface characteristics such as hydrophobicity, as discussed later. For some biopesticide fungi, certain spore types will be produced in liquid and others only on a solid substrate at the interface between substrate and air (Lomer et al., 2001). These various types of conidia are characterised by diVerent cell surface properties, which have implications for infection and for mycoherbicide formulation. Many Ascomycete and Basidiomycete fungal conidia attach to hydrophobic leaf surfaces by virtue of conidia wall
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proteins known as hydrophobins (Wo¨ sten, 2001). Hydrophobin membranes enable spores to attach rapidly and strongly to hydrophobic leaf surfaces and anchor appressoria that penetrate the leaf surface. In other fungal species, spore attachment is facilitated by the production of mucilage, the composition of which may include glycoproteins, lipids, and polysaccharides (Hamer et al., 1988; Sugui et al., 1998; Tucker and Talbot, 2001). This mucilage may be water soluble and assist in the dispersal of spores in rain splash. Spore surface properties may determine the type of mycoherbicide formulation that is most suitable. Hydrophobic conidia are suited to an oil‐based formulation or they can be applied in a water‐based formulation if an emulsifying agent is added (Feng et al., 1994). Fungi such as Colletotrichum, which form hydrophilic mucilaginous matrices around their spores, may be suited to a water‐based formulation without the need to add emulsifying agents. This may in part explain why Auld et al. (1990) were able to obtain successful infection of Xanthium spinosum in field inoculations with a simple liquid formulation of Colletotrichum orbiculare. Extremely hydrophobic spores are likely to clump in water‐based formulation and hence result in uneven dispersal on the target plant and variable levels of infection. B. FORMULATION
A range of solid formulations have been developed, which have been reviewed comprehensively by Auld et al. (2003). Fusarium species have been deployed successfully as mycoherbicides in solid formulations. These include the use of F. oxysporum in a Pesta formulation for the control of sunflower broomrape (Figs. 4 and 5) (Shabanna et al., 2003) and the ‘‘stabileze’’ process of Quimby et al. (1999). Shabanna et al. (2003) compared 19 Pesta formulations, using two types of fungal spores and eight adjuvants, in terms of their shelf‐life and for eYcacy under greenhouse conditions. Amending Pesta with yeast extract reduced the loss of viability of microconidia and chlamydospores during production of the formulations. Viability was greatest when granules were stored at 38C (Figs. 4 and 5). The five most eVective formulations of Pesta caused reduction in Orobanche biomass by 67–80%. For the control of wild radish, one of these formulations could be adopted for the soil‐borne pathogens F. oxysporum f. sp. raphanus or Aphanomyces raphani. This approach would be suitable because Fusarium species have already been applied in these formulations to target other weeds (Amsellem et al., 1999; Shabanna et al., 2003) and because F. oxysporum f. sp. raphanus
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Fig. 4. Shelf life (viable colony‐forming units, cfu) of Fusarium oxysporum f. sp. orthocerus–Pesta microconidia (PM) 1, 5 and 7 at various storage conditions (water activities, aw and temperature levels). Data points are means with standard error bars. Reprinted from Shabana et al. (2003) with permission from Elsevier.
is primarily a root pathogen able to germinate and infect the plant under moist soil conditions (Toyota and Kimura, 1992). Liquid formulations are likely to be better than solid formulations against wild radish or other weeds in dry cropping situations because the
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Fig. 5. Shelf life (viable colony forming units, cfu) of Fusarium oxysporum f. sp. orthocerus –Pesta chlamydospores (PC) 14, 15 and 18 at various storage conditions (water activities, aw and temperature levels). Data points are means with standard error bars. Reprinted from Shabana et al. (2003) with permission from Elsevier.
former are more likely to work under low or unpredictable rainfall events. Mycoherbicides in liquid form are applied as a spray in a similar manner to conventional herbicides and are formulated in order to reduce dew dependency for germination and infection of plant shoots (Auld et al., 2003).
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Of the pathogens listed, the most suited to this approach are the Alternaria species because they are foliar pathogens and are resistant to ultraviolet and other harsh conditions (Rotem, 1994). Auld et al. (2003) reviewed bioherbicide formulations and indicated that water‐in‐oil‐in‐water (WOW) emulsions were better than many other liquid formulations for reducing dew dependence in the field. In the past Alternaria conidia have been produced in solid or biphasic systems (Babu et al., 2004; ´ vila et al., 2000; Masangkay et al., 2000), but not in Daigle et al., 1998; De A submerged fermentation, indicating that their conidia probably only form at the interface between the substrate and the air. Therefore Alternaria spores are probably hydrophobic and would suit a simple, invert, or WOW emulsion, which, as well as facilitating an even distribution of spores, will also reduce dew dependence. Alternaria species have been applied as spores in oil emulsions (Babu et al., 2003; Connick et al., 1991; Shabana et al., 1997) and as spores or mycelia in an alginate gel formulated in either an aqueous or an oil‐based emulsion (Shabana et al., 1995, 1997).
VI. CONCLUSION In terms of host specificity, the biotrophic pathogens A. candida, A. raphani, and H. parasitica f. sp. raphani show the most promise to selectively control wild radish in canola cropping areas (Table II). However, these species are limited by the likely diYculty and cost of producing inoculum on an industrial scale. It may be possible to overcome these diYculties through innovative culture, tissue culture, or biotechnological solutions. First, the ideal candidate species from amongst these would need to be identified by investigating their molecular taxonomy, species boundaries, and host range on Brassica species. Second, the capacity for each of these species to infect under low moisture cropping climates would need to be investigated in terms of dew and temperature requirements and other epidemiological features. If a candidate was identified that could create the disease epidemic required without impacting on canola, then the challenge of developing cost‐ eVective industrial scale inoculum production could be investigated, possibly through tissue culture techniques or gene manipulation of the pathogen to grow on artificial media. Alternaria brassicae, A. brassicicola, A. japonica, and Fusarium oxysporum are the necrotrophic pathogens with the most potential for mycoherbicide development (Table II). The greatest diYculty with these taxa is their potential to attack canola. This could be overcome by identifying whether the pathogenicity of these organisms was due to the production of phytotoxic
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metabolites and then breeding (either by conventional or molecular techniques) host crops that are able to detoxify the compound. The first priority in the necrotroph‐based strategy would be to determine whether there are highly virulent strains of any of these pathogens on wild radish in Australia. Second, the basis of that virulence would need to be determined, and if it were largely due to the production of host‐specific toxins, then such compounds would need to be characterised. Concurrently the virulence of these isolates on canola should be assessed and if they are not pathogenic on canola then further host range testing could be pursued with the view to developing the mycoherbicide along conventional lines. If the HST is responsible for pathogenicity, then canola hosts could be screened for resistance and genes responsible for their detoxification identified (either from canola or from the pathogen). These genes could then be selected for or inserted into canola hosts to enhance resistance. The possibility of synthesising or otherwise fermenting and isolating the phytotoxic compound along the lines of bialophos/glufosinate could be researched. The final product could be a pure mycoherbicide, a combination of the phytotoxic compound and some host‐specific pathogen, or the phytotoxic compound applied alone.
ACKNOWLEDGMENTS We thank the CRC for Australian Weed Management and CSIRO Entomology for their support during this work. Nuccia Eyres from the Agriculture Department of Western Australia assisted by searching the APDD and CCDB databases for pathogen records, and Louise Morin also provided a list of pathogen records from NSW and Qld herbaria. We thank Gavin Ash, Bruce Auld, and Bernie Dell for their comments on drafts of the manuscript.
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Stress Resistance and Disease Resistance in Seaweeds: The Role of Reactive Oxygen Metabolism
MATTHEW J. DRING
Queen’s University Marine Laboratory, Portaferry, Co. Down, BT22 1PF Northern Ireland, United Kingdom
I. II. III. IV.
Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Environmental Stress on Seaweeds . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . Reactive Oxygen Metabolism (ROM) in Vascular Plants and Seaweeds . . .. . Interactions Between ROM and Environmental Stress Factors . . . . . . . . . A. Freezing, Desiccation and Osmotic Stress . . . . . . . . . . . . . . . . . . . . . . . . . B. High Light and Ultraviolet Stress . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . C. Heavy Metal Stress . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . D. Mechanical Stress . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . V. Responses of Seaweeds to Infection: Interaction with ROM. . . . . . . . . . . . VI. Summary and Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . References . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .
176 177 179 183 185 188 190 192 193 197 201
ABSTRACT It has become clear over the last 15–20 years that the immediate eVect of a wide range of environmental stresses, and of infection, on vascular plants is to increase the formation of reactive oxygen species (ROS) and to impose oxidative stress on the cells. Since 1994, suYcient examples of similar responses in a broad range of marine macroalgae have been described to show that reactive oxygen metabolism also underlies the mechanisms by which seaweeds respond (and become resistant) to stress and infection. Desiccation, freezing, low temperatures, high light, ultraviolet radiation, and heavy metals all tend to result in a gradual and continued buildup of ROS because photosynthesis is inhibited and excess energy results in the formation of singlet oxygen. The response to other stresses (infection or oligosaccharides which Advances in Botanical Research, Vol. 43 Incorporating Advances in Plant Pathology Copyright 2006, Elsevier Ltd. All rights reserved.
0065-2296/06 $35.00 DOI: 10.1016/S0065-2296(05)43004-9
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signal that infection is occurring, mechanical stress, hyperosmotic shock) is quite diVerent—a more rapid and intense, but short‐lived production of ROS, described as an ‘‘oxidative burst’’—which is attributed to activation of NADPH oxidases in the plasma membrane. Seaweed species that are able to survive such stresses or resist infection have the capacity to remove the ROS through a high cellular content of antioxidant compounds, or a high activity of antioxidant enzymes.
I. INTRODUCTION Seaweeds that grow in the subtidal zone live in relatively constant and stress‐ free environments, subjected to only small, slow changes in temperature, salinity, and supply of oxygen, inorganic carbon, and other nutrients. The most obvious stress occurs towards the bottom of the photic zone, where irradiance is limiting, or in regions of low nutrient availability, but changes occur slowly so that physiological processes have time to adjust. In the intertidal zone, however, the situation is very diVerent. The disadvantages of terrestrial habitats (unreliable water supply, variable temperatures, exposure to ultraviolet radiation) are combined with the disadvantages of aquatic habitats (variable irradiance and nutrient supply) and, to these, are added the mechanical stresses imposed by the waves. To survive in some intertidal sites, therefore, seaweeds may need to be able to tolerate rapid and frequent changes in temperature and desiccation stress and in salinity and irradiance (both photosynthetically active and ultra‐violet radiation), as well as the abrasion, pressure, and drag associated with wave action. Most work on environmental stresses in seaweeds has described the responses of physiological processes to stress and little attention has been paid to the cellular mechanisms by which plants limit the damage that has been (or may be) caused by stress. This is unfortunate because such approaches are more likely to indicate how the stress is detected, the mechanism of the response, and the way in which plants may become tolerant to a stress (cf. Davison and Pearson, 1996). Consequently, it has been diYcult to generalise about typical responses to a wide range of stresses or to identify the signals by which stresses are perceived. As Davison and Pearson (1996) pointed out, however, there were signs in the mid‐1990s that the production of reactive oxygen species (ROS) was associated with more than one type of stress and that reactive oxygen metabolism (ROM) could play a central role. These signs have strengthened in the last 10 years, and more evidence has accumulated, but the techniques that are needed for exploring ROM have been restricted to relatively few laboratories and there has been no review since 1996 that has highlighted the potential importance of ROM in seaweed ecophysiology. In this period, however, a new field of seaweed research has
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arisen, stimulated by the growing importance of the aquaculture of seaweeds for commercial applications—the study of the susceptibility of seaweeds to disease (‘‘phycopathology’’; Bouarab et al., 2001a,b; Potin et al., 1999)—and this has revealed that ROM is also involved in the responses of several seaweeds to infection by potentially pathogenic organisms and in the ability of such species to resist infection. This work has indicated the parallels between resistance to environmental stress and resistance to disease and has strengthened the importance of ROM to the ecology and exploitation of seaweeds. The aims of this review are as follows. 1. To assemble evidence for a central and integrating role of ROM in the responses of seaweeds to a range of apparently discrete environmental stresses and in the ability of seaweed species to resist and survive such stresses. 2. To demonstrate the similarities and parallels between the responses of seaweeds to environmental stresses and those to infection by potential pathogens (or to chemicals that appear to act as signals of such infection), and in their resistance to both types of stress. The treatment will concentrate on physiological responses and physiological evidence (including some of the basic methods for detecting ROS) rather than on the detailed biochemistry of ROM and on the ecological and aquacultural implications of ROM for seaweeds in order to encourage seaweed physiologists and ecologists to become more familiar with the basic concepts of ROM and to seek further evidence of its importance from a wider range of species.
II. ENVIRONMENTAL STRESS ON SEAWEEDS This section summarises the range of environmental stresses that act upon seaweeds in their natural habitats and discusses recent examples of work exploring the physiological responses to such stresses. It remains true that, as Davison and Pearson (1996) pointed out, most current research into environmental stresses in seaweeds describes the responses of individual physiological processes to stress and fails to investigate the cellular mechanisms by which seaweeds detect diVerent stresses and limit the damage that they cause. The stress that has received most attention in recent years, for obvious reasons, is ultra‐violet (UV) radiation, but it is diYcult to distinguish between the eVects of UV and the eVects of high irradiances of photosynthetically
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active radiation (PAR) with which it is always associated in natural environments (Dring et al., 2001). Nevertheless, it is clear that both UV and high light result in damage to the photosynthetic apparatus, although this has been deduced most frequently in recent years by measuring chlorophyll fluorescence using pulse amplitude moderated (PAM) fluorometers instead of measuring oxygen or carbon exchange. The immediate damage caused by both types of radiation has been linked to D1 protein (e.g., Bouchard et al., 2005) and cyclobutane pyrimidine dimers (van de Poll et al., 2002), whereas the longer term response leading to resistance is associated with the production of mycosporine amino acids (MAAs; Franklin et al., 1999; Krabs et al., 2004). There is increasing recent evidence (reviewed later) that the immediate responses of seaweeds to high irradiances of PAR and/or UV radiation are associated with some aspect of ROM. Such stresses are experienced by seaweed species at the upper limits of their depth distribution in upper sublittoral or intertidal zones, but the lower depth limit for the distribution of many species may be determined by low irradiance, which can be regarded as a distinct type of stress. This is not an acute stress and does not cause direct damage, except through long‐term reduction of energy and carbon supply. The typical responses, either acclimative or adaptive (a distinction that is not explored here), involve changes in the concentration and/or composition of photosynthetic pigments (Raven et al., 2000). Similarly, the low availability of CO2 may impose a stress that is chronic rather than acute, although such stress is rarely encountered in the sea because of the high concentration of bicarbonate, and seaweeds display a range of CO2‐ concentrating mechanisms that enable them to maintain adequate supplies of inorganic carbon (Giordano et al., 2005). The main stresses experienced by intertidal seaweeds are, of course, those associated with emersion, which include desiccation, high temperature, low temperature (especially freezing), and either increased (through evaporation) or decreased (through freshwater runoV) salinity. The impact of all of these stresses tends to be similar because they all result, directly or indirectly, in osmotic challenges to the cells of seaweeds (Pearson and Davison, 1994), and the responses or adaptations may involve the production of osmolytes (Edwards et al., 1988; Kirst, 1990). However, the first indications that ROM might be involved in the environmental responses of seaweeds came from studies of the responses of Fucus spp. to desiccation, freezing, and low temperatures (see later). High temperatures may exert an eVect on metabolic activity that is independent of their contribution towards osmotic stress, and responses have been observed involving the formation of heat stress proteins (Lewis et al., 2001; Li and Brawley, 2004). These responses do not appear to involve ROM.
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Deficiencies in the supply of essential nutrients (especially N, P) are rarely encountered in seaweeds in their natural habitats, although evidence shows that species growing higher on the shore have stronger nutrient uptake mechanisms than species lower on the shore or in the sublittoral, and this is thought to be a response to the limited time available for nutrient uptake because of the longer periods of tidal emersion (Hurd and Dring, 1990; Phillips and Hurd, 2004). However, the damaging eVects of emersion are exerted more rapidly on the process of photosynthesis than on nutrient uptake so that seaweeds are unlikely to respond acutely or specifically to nutrient stress in the sea. Heavy metals, however, are known to exert a damaging eVect on several aspects of seaweed development (Nielsen et al., 2003) and may cause a rapid inhibition of photosynthesis. Again, ROM appears to be involved (see later). Wave action imposes a severe mechanical stress on seaweeds, particularly in the intertidal zone, and several examples of apparent morphological responses to the severity of wave action (or the degree of shelter) have been described. Although wave action is an acute stress, no acute response is possible—apart from breakage of the frond and loss of photosynthetic tissue. Nevertheless, in transplant experiments, individual plants can be seen to have acclimated to a changed wave environment (e.g., Alaria; Sundene, 1962), which suggests that plants can detect and respond to signals indicating the severity of wave action, which probably involves some form of mechanical stress. It is of interest, therefore, that ROM has been implicated in the responses of two quite diVerent seaweeds to mechanical damage (Eucheuma, Collen and Pedersen, 1994; Dasycladus, Ross et al., 2005).
III. REACTIVE OXYGEN METABOLISM (ROM) IN VASCULAR PLANTS AND SEAWEEDS The term ‘‘reactive oxygen metabolism’’ is used in this review to refer to the full range of biochemical reactions involving what are commonly called ‘‘reactive oxygen species.’’ ROS are forms of oxygen, sometimes combined with hydrogen, which, as the name suggests, are more reactive than the relatively stable molecule O2, which is common in the atmosphere. In fact, this stable form of oxygen is strictly a ‘‘triplet oxygen’’ molecule [3O2], in which the two unpaired electrons have the same spin quantum number, and this imposes a restriction on the rate at which the molecule reacts with the many oxidisable substrates in natural environments on Earth. In photosynthetic organisms under light‐saturated conditions, triplet oxygen may be
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photosensitised by an excited triplet chlorophyll molecule to generate ‘‘singlet oxygen’’ [1O2], a form of the dioxygen molecule in which the spin restriction is removed and, consequently, reactivity is increased greatly. Singlet oxygen can react with pigments, proteins, and lipids and is regarded as the main cause of photoinhibition of photosynthesis in plants, including the degradation of D1 protein (Krieger‐Liszkay, 2005). Another of the reactive oxygen species is the so‐called ‘‘superoxide radical’’ [O2], whose extra reactivity is due to the fact that it is both a radical (i.e., has unpaired electrons in its outermost shell) and an anion. Superoxide can be formed directly from singlet oxygen or by reduction of triplet oxygen (Fig. 1), usually as a result of leakage of electrons from respiratory or photosynthetic electron transport pathways (Alscher et al., 1997). At physiological pH, the superoxide radical does not react rapidly with cellular components (Wojtaszek, 1999) and ‘‘disproportionates’’ in solution into another ROS (hydrogen peroxide, H2O2) and triplet oxygen: 3 2 O 2 þ 2H ! H2 O2 þ O2
ð1Þ
This reaction may occur spontaneously, but is enhanced greatly by the activity of superoxide dismutase (SOD), which is found in many compartments of the cell, including the cytosol, chloroplasts, and mitochondria, as well as extracellularly. Several distinct forms of SOD have been found in photosynthetic organisms, incorporating diVerent metals as cofactors (Alscher et al., 2002; Asada, 1999). The thylakoid membranes and cytosol of vascular plants and some algae contain a CuZnSOD, whereas the forms of SOD found in the stroma of the chloroplasts contain iron and those in the mitochondria and peroxisomes contain manganese (Fig. 2). It is the activity of these various forms of SODs in plants that is thought to provide the major protection against the damaging eVects of superoxide (Pinto et al., 2003). Scavenging of superoxide by SODs results in the production of H2O2, which, although less damaging than the superoxide radical, is far from
Fig. 1. Formation of diVerent reactive oxygen species (ROS) from molecular (triplet) oxygen (adapted from Wojtaszek, 1999).
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Fig. 2. Localisation of diVerent forms of superoxide dismutase (SODs) in plant cells (redrawn from Alscher et al., 2002).
harmless. Partly because H2O2 is less reactive and more stable than other ROS, it may diVuse away from its site of formation, into other cells or, especially for aquatic plants, into the outside environment. Significant concentrations can build up in the medium surrounding cultures of both microalgae (e.g., up to 0.9 M by the raphidophyte, Heterosigma akashiwo; Twiner et al., 2001) and macroalgae (e.g., up to 4.0 M by the green seaweed Ulva rigida; Collen and Pedersen, 1996). H2O2 may also participate in a number of enzymatic reactions within plant and algal cells, which are described later. However, reaction between the superoxide radical and H2O2 (the Haber–Weiss reaction) results in the most reactive of the ROS, the hydroxyl radical [OH]: 3 O 2 þ H2 O2 ! OH þ OH þ O2
ð2Þ
This reaction is not thought normally to generate significant quantities of OH in plant cells, but the presence of transition metals, such as Fe3þ or Cu2þ, enhances the rate substantially (Pinto et al., 2003). Another mechanism by which transition metals may promote the formation of OH is the Fenton reaction, in which reduced forms of metal ions (e.g., of Fe, Cu, or Cr)
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are first oxidised by H2O2 and subsequently reduced by reaction with superoxide (Pinto et al., 2003; Wojtaszek, 1999): H2 O2 þ Fe2þ ðor Cuþ Þ ! OH þ OH þ Fe3þ ðor Cu2þ Þ
ð3Þ
2þ þ 3þ 2þ 3 O 2 þ Fe ðor Cu Þ ! Fe ðor Cu Þ þ O2
ð4Þ
Because of its relative stability, hydrogen peroxide is the most readily detected ROS in and around plants and algae, and there is an extensive literature on its reactions and interactions with a variety of biochemicals. The primary reaction of H2O2 is its breakdown into water and triplet oxygen. This may occur spontaneously but, in most cells, is catalysed by catalase: H2 O2 þ H2 O2 ! 2H2 O þ 3 O2
ð5Þ
Another mechanism by which H2O2 can be detoxified is through its reaction with ascorbate, which is mediated by ascorbate peroxidase (APX; see Alscher et al., 1997). This results in the oxidation of ascorbate in the cell or organelle, but ascorbate is regenerated by the oxidation of glutathione (GSH – a tripeptide: glutamate þ cysteine þ glycine), which is regenerated in turn by glutathione reductase (GR) using reduced NADP (Fig. 3). Catalase, the various forms of SOD, and the enzymes involved in this ascorbate/glutathione pathway (APX, DHAR, GR) are referred to frequently as ‘‘antioxidant enzymes,’’ as they are collectively involved in the removal of ROS from various compartments of plant cells and in the reduction of oxidative stress. The activity of such enzymes has been detected in a wide range of seaweed species, including Fucus spp. (Collen and Davison, 1999b, 2001), the green algae Ulva rigida (Collen and Pedersen, 1996), Acrosiphonia penicilliformis, Monostroma arcticum, Chaetomorpha linum, Chaetomorpha melagonium (Aguilera et al., 2002b), and the red algae Devaleraea ramentacea,
Fig. 3. Reactions of the ascorbate‐glutathione pathway (also known as Halliwell–Asada pathway; adapted from Wojtaszek, 1999).
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Palmaria palmata (Aguilera et al., 2002b), Polysiphonia arctica (Dummermuth et al., 2003), Kappaphycus alvarezii (Barros et al., 2003), Chondrus crispus, and Mastocarpus stellatus (Collen and Davison, 1999c; Lohrmann et al., 2004). Although the strategy of most plants seems to be to rid themselves of H2O2 as quickly as possible, H2O2 appears to have a beneficial role in some plants and algae through its interaction with various peroxidase enzymes to produce secondary metabolites of considerable importance. These include lignin in woody plants (Wojtaszek, 1999) and a range of halocarbons in algae. Haloperoxidases have been detected in representatives of all three major groups of seaweeds (Table I), in which they catalyse the production of mainly bromocarbons and iodocarbons from H2O2, bromide, or iodide and an organic substrate. Many of the products are volatile and may escape into the atmosphere (Carpenter et al., 2000) so that there is considerable current interest in establishing the relative contributions that seaweeds and human activities may make towards ozone depletion through brominated hydrocarbons in the atmosphere (Carpenter and Liss, 2000; Goodwin et al., 1997). The products of haloperoxidase activity in seaweeds may also be part of defence mechanisms against microorganisms (McConnell and Fenical, 1977), herbivores (Gschwend et al., 1985), or larval settlement (Ohsawa et al., 2001; Ohshiro et al., 1999) and are thought to assist in the uptake of bromide and iodide in Laminaria spp. (Ku¨ pper et al., 1998). However, it is diYcult to establish a function for all of the many and varied halocarbons produced by seaweeds, and several investigators of these haloperoxidases have concluded that their main function is to detoxify H2O2 (Collen et al., 1994; Manley and Barbero, 2001; Pedersen et al., 1996). Indeed, Manley and Barbero (2001) considered that the internal bromoperoxidase of Ulva lactuca may be the major H2O2‐removing enzyme because of its relatively low Km for H2O2. Peroxidases seem, therefore, to play an important role in the ROM of seaweeds.
IV. INTERACTIONS BETWEEN ROM AND ENVIRONMENTAL STRESS FACTORS The relationship between ROM and environmental stress in vascular plants was first established in the late 1980s (Foyer et al., 1997), and attempts to look for similar relationships in the algae were made soon afterwards, in the mid‐ to late 1990s—first for the freshwater dinoflagellate Peridinium gatunense (Butow et al., 1994, 1997) and then for the first seaweeds—in the response of the cultivated seaweed Eucheuma playcladum to mechanical
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TABLE I Haloperoxidase Enzymes and Their Products in Seaweeds Species Chlorophyta Ulva lactuca U. rigida U. lens Cladophora glomerata Enteromorpha spp. Phaeophyceae Macrocystis pyrifera Laminaria digitata L. digitata Laminaria spp. Ascophyllum nodosum A. nodosum Fucus vesiculosus
Enzymesa
Reference
BrPO
CHBr3
BrPO BrPO
CHBr3 CH2Br2, CHBr3 CHCl3, CHBr3, CH2I2 CHCl3, CHBr3, CH2I2
Manley and Barbero, 2001 Pedersen et al., 1996 Ohshiro et al., 1999 Abrahamsson et al., 2003 Abrahamsson et al., 2003
CH2Br2, CHBr3
Goodwin et al., 1997
I‐uptake
Ku¨ pper et al., 1998
HPO IPO, BrPO IPO, BrPO HPO
Colin et al., 2003 Almeida et al., 2001 Vilter et al., 1983
V‐HPO CHCl3, CHBr3, CH2I2
Ecklonia stolonifera
V‐BPO
Saccorhiza polyschides
V‐IPO
Rhodophyta Meristiella gelidium Laurencia sp. Eucheuma denticulatum E. denticulatum Corallina pilulifera
V‐BPO
C. C. C. C.
V‐BPO V‐BPO V‐BPO V‐BPO
pilulifera pilulifera oYcinalis oYcinalis
Products
Weyand et al., 1999 Abrahamsson et al., 2003 Hara and Sakurai, 1998 Almeida et al., 1998
Various I, Br, and Cl hydrocarbons CHBr3
Collen et al., 1994 Pedersen et al., 1996 Pedersen et al., 1996 Sundstrom et al., 1996
Various I, Br, and Cl hydrocarbons
Mtolera et al., 1996
CHBr3
Shimonishi et al., 1998 Ohsawa et al., 2001 Ohshiro et al., 2002 Carter et al., 2002 Isupov et al., 2000
a
BrPO, bromoperoxidase; HPO, haloperoxidase; IPO, iodoperoxidase; V‐BPO, vanadium peroxidases.
stress (Collen and Pedersen, 1994) and in the resistance of diVerent species of Fucus to the stresses of the intertidal environment (Collen and Davison, 1999a,b).
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STRESS AND DISEASE RESISTANCE IN SEAWEEDS A. FREEZING, DESICCATION AND OSMOTIC STRESS
The first study of ROM in seaweeds of the intertidal zone (Collen and Davison, 1999a,b) examined the responses of Fucus spiralis, F. evanescens, and F. distichus, which are typically found in this sequence from the top to the bottom of the intertidal on rocky shores of the northwest Atlantic to single exposures to either freezing (6 h in darkness at 16 to 18 8C) or desiccation (6 h in darkness at 4 8C after drying in low humidity air to 40% of fresh weight) treatments. The physiological responses of the fronds exposed to these treatments were measured by PAM fluorometry (Fv:Fm) and the production of reactive oxygen was estimated by following the oxidation of an intracellular dye, 20 ,70 ‐dichlorohydrofluorescein diacetate (DCFH‐DA) to the fluorescent 20 ,70 ‐dichlorofluorescein (DCF; Collen and Davison, 1997) and also by measuring the release of H2O2 into the medium. The Fv:Fm values obtained immediately after the freezing treatment indicated that only F. distichus had been aVected adversely by the treatment, and the production of DCF was also increased by freezing only in F. distichus (Collen and Davison, 1999a). However, freezing resulted in a significant increase in H2O2 production only in F. spiralis. The desiccation treatment produced a better diVerentiation among the three species in terms of DCF formation, as it increased sevenfold in F. distichus and threefold in F. evanscens, but was not aVected significantly in F. spiralis (Table II). These indications that freezing and desiccation treatments caused the production of ROS in the thalli of low‐shore species but not in high‐shore species suggested that resistance to such stresses might be associated with the ability of species to reduce the oxidative stress produced by the treatments. This could be achieved by possessing relatively high concentrations of antioxidant compounds (tocopherol, ‐carotene, ascorbate, glutathione) or high activities of the antioxidant enzymes (catalase, SOD, APX, GR) described in
TABLE II Production of Reactive Oxygen (Measured Using Dichlorohydrofluorescein, DCF) by Three Species of Fucus after Desiccation Treatment (6 h in Darkness at 40% Water Content) and 2 h Recovery in Seawater (Collen and Davison, 1999a)a Rate of DCF production (nmol g FW1 h1) Species Fucus spiralis F. evanescens F. distichus
Control 0.094a 0.115a 0.157ab
Values with diVerent subscript letters are significantly diVerent at p ¼ 0.05.
a
Desiccated 0.157ab 0.384b 1.11c
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the previous section, and these concentrations and activities were measured in thalli of the same three Fucus species by Collen and Davison (1999b). The concentrations of the antioxidant compounds did not correlate clearly with the positions of the three species on the shore (or with their response to the stress treatments), but F. distichus exhibited lower activities of catalase, SOD, and APX than the other two species. There were fewer diVerences in antioxidants or enzymes to account for the diVerent responses of F. spiralis and F. evanescens to stress, but the activities of APX and SOD in F. spiralis were considerably higher on a chlorophyll basis, and Collen and Davison (1999b) suggested that this may indicate higher concentrations in the chloroplasts and, therefore, more eYcient scavenging of ROS produced in the light when photosynthesis is inhibited by the stresses imposed. Similar indications of diVerences in antioxidant metabolism with vertical position on the shore, but this time within a single species, have been obtained for the New Zealand red alga Stictosiphonia arbuscula (Burritt et al., 2002). Thalli of this species from the top and bottom of its zone on the shore were maintained at diVerent relative humidities for 12, 24, or 48 h, and their antioxidant metabolism and the leakage of amino acids through their membranes were examined after rehydration. Specimens from low on the shore lost more amino acids through the plasma membrane and produced more H2O2 than high‐shore specimens; these diVerences seemed to be related to the greater activity of APX and GR in thalli from the high shore rather than to higher concentrations of antioxidants. These results support the conclusions of Collen and Davison (1999a,b) about the importance of ROM in enabling seaweeds to survive desiccation stress and are particularly valuable in that they show that intraspecific diVerences occur in a red alga from the southern hemisphere, in addition to interspecific diVerences among brown algae from the northern hemisphere. Studies of three other intertidal species (two red and one brown) from the northwest Atlantic have provided further evidence for the connection between antioxidants and the positions that species occupy in the intertidal zonation and have shown that there may be seasonal variations in the concentrations of antioxidants and the activities of antioxidant enzymes. The morphologically similar pair of red algae, Chondrus crispus and Mastocarpus stellatus, occur together throughout much of their tidal range, but M. stellatus can reach greater tidal heights and was assumed, therefore, to be more tolerant of environmental stress. Although the response of these species to stress treatments was not tested, the rate at which M. stellatus scavenged H2O2 (i.e., reduced the concentration of added H2O2 in seawater) and the resistance of its photosynthetic apparatus (measured as Fv:Fm) to the addition of H2O2 or Rose Bengal (a stain that increases the formation of
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singlet oxygen; Foote, 1967) was greater than for C. crispus (Collen and Davison, 1999c). The concentration of ascorbate and the activity of catalase were also higher in M. stellatus, but C. crispus had more glutathione, and the diVerences in other antioxidants and enzyme activities were less clear cut. A more recent study of the same two species (Lohrmann et al., 2004) showed that there are substantial seasonal variations in the antioxidant concentrations and enzyme activities—both tend to be higher in the winter months than in the summer—which may explain some of the inconsistencies in the earlier data. The most interesting point to emerge from these two studies is that both species appear to acclimate to low temperatures in the winter by increasing their capacity for scavenging ROS, which is thought to be because photosynthesis is more likely to be light saturated at low temperatures so that ROS production will be higher. The activities of catalase, SOD, and APX also declined between February and August in Fucus vesiculosus from the same region (Collen and Davison, 2001). Unfortunately, this study was continued only to the following October and, by this time, recovery was apparent only in APX. The activity of GR did not change over this period, and neither did the concentration of glutathione, whereas ascorbate was three times higher in August and October than in February. After 2 weeks of growth at 0 8C, with or without a daily freezing treatment, or at 20 8C, the content of ascorbate and glutathione had also not changed in F. vesiculosus, but the activity of SOD had increased markedly in the freezing treatment, and that of both APX and GR had decreased in the 20 8C treatment (Collen and Davison, 2001). There is good evidence, therefore, for phenotypic acclimation of the antioxidant enzymes in brown and red algae in response to low temperature and/or freezing treatments, which are consistent with the hypothesis that thalli develop cellular mechanisms to reduce oxidative stress under conditions that are likely to increase such stresses. However, the detailed responses of individual species show considerable variation, and no one antioxidant or enzyme can be used as a marker of the degree of stress being experienced by seaweeds or of the degree of resistance of thalli to intertidal stresses. The physiological responses of the photosynthetic apparatus of Fucus distichus to freezing stress were found to be very similar to those resulting from osmotic dehydration (Pearson and Davison, 1994) and also to the eVects of desiccation stress during emersion on the shore. This suggests that another form of environmental stress that seaweeds may experience—hyperosmotic stress as a result of evaporation of seawater during emersion—will give rise to similar physiological responses. There has been evidence for some time that the ability of vascular plants to tolerate high salinity is associated with ROM (e.g., Gossett et al., 1994; Herna´ ndez et al., 1995; Kalir and
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PoljakoV‐Mayber, 1981) but, although antioxidant responses to hypersaline stress have been recorded in Dunaliella (Jahnke and White, 2003), none of the many studies of the eVects of salinity changes on seaweeds have considered how ROM might be aVected. A recent and welcome exception to this, which (because of its technical sophistication) has much broader implications than simply confirming that seaweeds respond to increased salinity by generating ROS, is a study of Fucus embryos by Coelho et al. (2002). Two‐celled embryos of Fucus serratus were incubated for 20 min in chloromethyl‐20 ,70 ‐dichlorohydrofluorescein diacetate (CM‐DCFH‐DA) and then subjected to a hyperosmotic shock by transferring them to seawater containing 2 M sorbitol. The fluorescence that developed as the CM‐DCFH‐DA was oxidised to DCF by superoxide or H2O2 was monitored by confocal laser microscopy (as described by Rijstenbil et al., 2000) and was detectable in the plasma membrane of the rhizoid apex within 12 s of the start of the osmotic shock treatment. It then spread to the subapical regions within 40–120 s, where it continued to increase for up to 20 min. Simultaneous monitoring of the concentration and distribution of calcium ions within the embryos showed a sharp transient increase in Ca2þ within 10–12 s in the same location as the initial ROS production, which was then propagated as a wave from the apex through the rest of the cell. The production of ROS in the subapical regions was shown to be located exclusively in the mitochondria and was considered to be a separate and secondary response to the osmotic shock, which was initiated as the Ca2þ wave spread through the cell (Fig. 4). This exciting and far‐reaching study suggests that the primary response to osmotic shock (perhaps initiated by the withdrawal of the plasma membrane from the cell wall as a result of dehydration) is the production of ROS outside the plasma membrane, which provides the signal for an inc