Sea Star Pisaster Ochraceus Research Articles

Lethal and sublethal implications of low temperature exposure for three intertidal predators

Benthic invertebrate predators play a key role in top-down trophic regulation in intertidal ecosystems. While the physiological and ecological consequences of predator exposure to high temperatures during summer low tides are increasingly well-studied, the effects of cold exposure during winter low tides remain poorly understood. To address this knowledge gap, we measured the supercooling points, survival, and feeding rates of three intertidal predator species in British Columbia, Canada — the sea stars Pisaster ochraceus and Evasterias troschelii and the dogwhelk Nucella lamellosa — in response to exposure to sub-zero air temperatures. Overall, we found that all three predators exhibited evidence of internal freezing at relatively mild sub-zero temperatures, with sea stars exhibiting an average supercooling point of −2.50 °C, and the dogwhelk averaging approximately −3.99 °C. None of the tested species are strongly freeze tolerant, as evidenced by moderate-to-low survival rates after exposure to −8 °C air. All three predators exhibited significantly reduced feeding rates over a two-week period following a single 3-h sublethal (−0.5 °C) exposure event. We also quantified variation in predator body temperature among thermal microhabitats during winter low tides. Predators that were found at the base of large boulders, on the sediment, and within crevices had higher body temperatures during winter low tides, as compared to those situated in other microhabitats. However, we did not find evidence of behavioural thermoregulation via selective microhabitat use during cold weather. Since these intertidal predators are less freeze tolerant than their preferred prey, winter low temperature exposures can have important implications for organism survival and predator-prey dynamics across thermal gradients at both local (habitat-driven) and geographic (climate-driven) scales.

Identifying the core microbiome of the sea star Pisaster ochraceus in the context of sea star wasting disease.

Sea stars are keystone species and their mass die-offs due to sea star wasting disease (SSWD) impact marine communities and have fueled recent interest in the microbiome of sea stars. We assessed the host specificity of the microbiome associated with three body regions of the sea star Pisaster ochraceus using 16S rRNA gene amplicon surveys of the bacterial communities living on and in Pisaster, their environment, and sympatric marine hosts across three populations in British Columbia, Canada. Overall, the bacterial communities on Pisaster are distinct from their environment and differ by both body region and geography. We identified core bacteria specifically associated with Pisaster across populations and nearly absent in other hosts and the environment. We then investigated the distribution of these core bacteria on SSWD-affected Pisaster from one BC site and by reanalyzing a study of SSWD on Pisaster from California. We find no differences in the distribution of core bacteria in early disease at either site and two core taxa differ in relative abundance in advanced disease in California. Using phylogenetic analyses, we find that most core bacteria have close relatives on other sea stars and marine animals, suggesting these clades have evolutionary adaptions to an animal-associated lifestyle.

Variation in the behavioral tolerance of congeneric marine snails to low-pH exposure

The ocean is acidifying, with multiple consequences for coastal organisms. However, species may differ in their sensitivities. Some taxa may find future conditions mildly stressful or even advantageous, while others will persist only through acclimatization or genetic adaptation. An open question is whether such variation in the sensitivity of species to ocean acidification relates to their evolutionary histories of exposure to reduced pH. Here, we explored this unknown through an investigation of differences in pH tolerance of 2 shoreline gastropods, the black turban snail Tegula funebralis and its congener, the brown turban snail T. brunnea. These species occupy distinct vertical distributions on rocky shores, each subject to different extremes in low pH. We assayed the extent to which low pH degrades the flight behavior of each species in response to the predatory sea star Pisaster ochraceus. Across a range of pH, the tidepool-inhabiting T. funebralis exhibited less behavioral disruption than T. brunnea at any given pH value but also experienced impairment at a pH characteristic of the present-day minimum in its habitat (7.1 pH). The latter pattern suggests T. funebralis operates near what may be a fixed tolerance limit to low pH. T. funebralis also exhibited hints of elevated intraspecific variation in its behaviors, which could imply scope for selection to act. Deeper-dwelling T. brunnea, in contrast, showed little sensitivity to present-day pH minima found where it lives (7.6 pH) and displayed less variation upon which selection might operate. These results provide a initial framework for investigations into the capacity of species of differing evolutionary histories to cope with future ocean acidification.

Infrequent Fluctuations in Temperature and Salinity May Enhance Feeding in Pisaster ochraceus (Asteroidea) but Not in Dendraster excentricus (Echinoidea) Larvae.

AbstractIn recent years, low-salinity events characterized by high temperatures (18-23 °C) and low-salinity waters (20‰-22‰) have increased during late spring and summer, when many marine invertebrate larvae are developing. The present study examines the effects of low-salinity events on particle ingestion for larvae of two echinoderm species, the sea star Pisaster ochraceus and the sand dollar Dendraster excentricus. Larvae were exposed to high temperatures and low salinities for 24 hours, followed by feeding on the alga Isochrysis galbana in high or low salinity for another 10 minutes. Exposing Pisaster larvae to high temperatures and low salinities, followed by feeding in low salinity, did not impair ingestion rates. In fact, these larvae ingested particles at similar and sometimes higher rates than those in the controls. In sharp contrast, a 24-hour exposure to a high temperature and low salinity, followed by continued exposure to low salinity to feed, led to a decrease in the number of particles ingested by 8-arm Dendraster larvae. Larvae of both species captured very few particles when returned to 30‰ after a low-salinity event, indicating that continuous interruption of larval feeding by low-salinity events during development could be deleterious. Sand dollar larvae may have responded negatively to low-salinity events in our experiments because they are found in protected bays, where they may seldom experience these events.

Adaptive and Plastic Responses to Environmental Variation: Introduction to a Virtual Symposium in The Biological Bulletin.

Adaptive and Plastic Responses to Environmental Variation: Introduction to a Virtual Symposium in The Biological Bulletin.

Keystone predation: trait‐based or driven by extrinsic processes? Assessment using a comparative‐experimental approach

AbstractKeystone predation can be a determinant of community structure, including species diversity, but factors underlying “keystoneness” have been minimally explored. Using the system in which the original keystone, the sea star Pisaster ochraceus, was discovered, we focused on two potential (but overlapping) determinants of keystoneness: intrinsic traits or state variables of the species (e.g., size, density), and extrinsic environmental parameters (e.g., prey productivity) that may provide conditions favorable for keystone predator evolution. Using a comparative‐experimental approach, with repeated field experiments at multiple sites across a variable coastal environment, we tested predation rates, or how quickly predators consumed prey, and predation effects, or community response to predator presence or absence. We tested five hypotheses: (H1) predation rates and effects will vary in space but not time; (H2) per population predation rates will vary primarily with individual traits and population variables; (HJHH3) per capita predation rates will vary only with individual traits; (H4) predation effects will vary with traits, variables, and external drivers; and (H5) as predicted by the keystone predation hypothesis, diversity will vary unimodally with predation pressure. As hypothesized, predation rates differed among sites but not over time (H1), and in caging exclusion experiments, predation effect varied with both intrinsic and extrinsic factors (H4). Unexpectedly, predation rates varied with both intrinsic and extrinsic (H2, per population), or only with extrinsic (H3, per capita) factors. Further, in large‐plot exclusion experiments, predation effect was most closely associated with individual traits (contra H4). Finally, taxon diversity varied unimodally with proxies of predation pressure (sessile prey abundance) and was sensitive to extrinsic factors (mussel growth, temperature, and upwelling, H5). Hence, keystoneness depended on predator individual traits, predator population variables, and environmental parameters. However, temporal differences in caging experiments suggested that environmental characteristics underlying prey dynamics may be preeminent. Compared to prior experiments, predation was weaker with low prey input compared to periods with high prey input. Collectively, our results suggest that keystone predator evolution depends on the coalescence of species‐specific characteristics, and environmental parameters favoring high prey productivity. Our approach may be a model for future studies exploring the generality of keystoneness.

Predator identity dominates non-consumptive effects in a disease-impacted rocky shore food web.

Predicting the effects of predator diversity loss on food webs is challenging, because predators can both consume and induce behavioral responses in their prey (i.e., non-consumptive effects or NCEs). Studies manipulating predator diversity and investigating NCEs are rare, especially in marine systems. Recently, a severe outbreak of sea star wasting syndrome (SSWS) on the west coast of North America resulted in unprecedented declines of the sea star Pisaster ochraceus. We investigated the consequences of Pisaster loss on an abundant grazer, the black turban snail Tegula funebralis, through NCEs. We combined a laboratory experiment and field surveys to examine the importance of identity vs. diversity in a predator assemblage (Pisaster, crabs, and octopuses) on Tegula behavior, feeding, and growth. Laboratory and field results indicated that predator identity, not diversity, drives Tegula behavior and causes NCEs. Mesocosm treatments with Pisaster caused greater NCEs on Tegula than assemblages without Pisaster. Tegula's distribution in the field, which is driven primarily by anti-predator behavior, was strongly associated only with Pisaster abundance, and not with the abundance of crabs, octopuses, and other predatory sea stars (Leptasterias spp.). We conclude that Pisaster primarily drives Tegula vertical distribution and may be having strong NCEs on Tegula on northern California rocky shores. Furthermore, predator diversity in northern California does not provide functional redundancy, in terms of NCEs on Tegula, to buffer the system from Pisaster loss. Thus, predator-induced vertical distributions and grazing suppression may not be maintained in areas where Pisaster populations are reduced or slow to recover from SSWS.

Coelomic Fluid Evaluation in Clinically Normal Ochre Sea Stars Pisaster ochraceus: Cell Counts, Cytology, and Biochemistry Reference Intervals.

Coelomic fluid sampling is a noninvasive technique that is used to access the body fluid of sea stars for diagnostics and research. Given recent mortality events including sea star wasting disease, which has killed millions of sea stars along the Pacific coast since 2013, there is a need for validated diagnostic tests to evaluate sea star health. The objectives of this study were to establish coelomic fluid reference intervals for clinically normal ochre sea stars Pisaster ochraceus in an open system aquarium, to describe the cytologic findings, and to compare the chemistries of coelomic fluid with open system tank water. Coelomic fluid from 26 clinically normal sea stars was sampled for coelomocyte counts, cytologic evaluation, and biochemical analysis including magnesium, sodium, potassium, chloride, calcium, and total protein. The number of coelomocytes and total protein did not fit normal distribution and were excluded from analyses. Reference intervals were established for other chemistry analytes. There was no statistical difference in biochemistries between sea star coelomic fluid and water from five open system tanks, which supports previous evidence that sea stars are osmoconformers. Very low numbers of coelomocytes were observed cytologically. These results provide a useful baseline and diagnostic tool for health assessments of sea stars.

Arms of larval seastars of Pisaster ochraceus provide versatility in muscular and ciliary swimming.

Larval swimming with cilia, unaided by muscles, is the presumed ancestral condition for echinoderms, but use of muscles in swimming has evolved several times. Ciliation and musculature of the arms of brachiolaria-stage larvae in the family Asteriidae provide unusual versatility in the use of muscles in swimming. The muscles affect swimming in two different ways. (1) Contraction of muscles moves the arms, propelling the larva. (2) Contraction of muscles changes orientation of the arms, thereby changing direction of ciliary currents and direction of swimming. New observations of the brachiolaria of the asteriid seastar Pisaster ochraceus demonstrate more versatility in both of these uses of muscles than had been previously described: the posterolateral arms stroke in more ways to propel the larva forward and to change the direction of swimming, and more pairs of the arms point ciliary currents in more directions for changes in direction of swimming. Morphology of brachiolariae suggests that these uses of muscles in swimming evolved before divergence of the families Stichasteridae and Asteriidae within forcipulate asteroids. This versatile use of muscles for swimming, both alone and in combination with ciliary currents, further distinguishes the swimming of these brachiolariae from swimming by larvae of other echinoderms and larvae of acorn worms in the sister phylum Hemichordata.

Lamellose Axial Shell Sculpture Reduces Gastropod Vulnerability to Sea Star Predation.

Marine gastropods exhibit a stunning diversity of shell sculpture, but the functional significance of many sculpture types remains unknown. Unfortunately, experimental tests of the functional significance of differences between species are complicated by other morphological differences, such as shell microstructure, aperture shape, and shell thickness, that may confound interpretation. The most robust experimental tests are therefore performed using different shell forms within a species. We took advantage of the extensive intraspecific shell variation in the common intertidal gastropod Nucella lamellosa to test the adaptive significance of axial lamellae, a type of shell sculpture found in numerous marine gastropod subfamilies. We offered three forms of N. lamellosa (lamellose, artificially smooth, and naturally smooth) to the predatory sea star Pisaster ochraceus under controlled laboratory conditions. Pisaster ochraceus consumed significantly fewer lamellose snails than either artificially or naturally smooth snails. We suggest that shell lamellae deter sea star predation by impairing their ability to capture or manipulate snail prey or by increasing prey effective size. These results suggest a credible hypothesis for the adaptive significance of lamellar sculpture in marine gastropods and provide a valuable missing piece to the story about adaptive phenotypic plasticity in N. lamellosa shell form.

RNA expression and disease tolerance are associated with a "keystone mutation" in the ochre sea star Pisaster ochraceus.

An overdominant mutation in an intron of the elongation factor 1-α (EF1A) gene in the sea star Pisaster ochraceus has shown itself to mediate tolerance to “sea star wasting disease”, a pandemic that has significantly reduced sea star populations on the Pacific coast of North America. Here we use RNA sequencing of healthy individuals to identify differences in constitutive expression of gene regions that may help explain this tolerance phenotype. Our results show that individuals carrying this mutation have lower expression at a large contingent of gene regions. Individuals without this mutation also appear to have a greater cellular response to temperature stress, which has been implicated in the outbreak of sea star wasting disease. Given the ecological significance of P. ochraceus, these results may be useful in predicting the evolutionary and demographic future for Pacific intertidal communities.

Incorporating Context Dependency of Species Interactions in Species Distribution Models

Species distribution models typically use correlative approaches that characterize the species-environment relationship using occurrence or abundance data for a single species. However, species distributions are determined by both abiotic conditions and biotic interactions with other species in the community. Therefore, climate change is expected to impact species through direct effects on their physiology and indirect effects propagated through their resources, predators, competitors, or mutualists. Furthermore, the sign and strength of species interactions can change according to abiotic conditions, resulting in context-dependent species interactions that may change across space or with climate change. Here, we incorporated the context dependency of species interactions into a dynamic species distribution model. We developed a multi-species model that uses a time-series of observational survey data to evaluate how abiotic conditions and species interactions affect the dynamics of three rocky intertidal species. The model further distinguishes between the direct effects of abiotic conditions on abundance and the indirect effects propagated through interactions with other species. We apply the model to keystone predation by the sea star Pisaster ochraceus on the mussel Mytilus californianus and the barnacle Balanus glandula in the rocky intertidal zone of the Pacific coast, USA. Our method indicated that biotic interactions between P. ochraceus and B. glandula affected B. glandula dynamics across >1000 km of coastline. Consistent with patterns from keystone predation, the growth rate of B. glandula varied according to the abundance of P. ochraceus in the previous year. The data and the model did not indicate that the strength of keystone predation by P. ochraceus varied with a mean annual upwelling index. Balanus glandula cover increased following years with high phytoplankton abundance measured as mean annual chlorophyll-a. M. californianus exhibited the same pattern to a lesser degree, although this pattern was not significant. This work bridges the disciplines of biogeography and community ecology to develop tools to better understand the direct and indirect effects of abiotic conditions on ecological communities.

KEYSTONEin: A glycoprotein cue drives predation on mussels and structures rocky intertidal communities

Foundation species provide critical resources to ecological community members and are major determinants of biodiversity. One such species, the California mussel Mytilus californianus, is a superior competitor and dominates space on rocky, wave-swept shores (northeast Pacific Ocean). Live mussels secrete a 29.6 kDa glycoprotein (named 'KEYSTONEin'), with expression localized in epidermis, extrapallial fluid, and periostracum (organic shell coating). Hence, KEY-STONEin is available for contact recognition as predators crawl on rocky surfaces. Purple sea stars Pisaster ochraceus, whelks (Nucella emarginata and Acanthinucella spirata), and lined-shore crabs Pachygrapsus crassipes are common intertidal carnivores. Spanning 3 phyla and differing substantially in sensory mechanisms and hunting techniques, all are major mussel consumers. Here, we constructed faux prey to mimic both physical and chemical properties of mussels. Purified KEYSTONEin was presented at a typical mussel concentration. All 4 predatory species attacked, and ate, KEYSTONEin-infused faux prey as opposed to the organic enrichment or seawater controls. Sea stars, whelks (both species), and crabs also did not distinguish between KEY-STONEin-laced mimics and their live, intact counterparts. Mechanisms of chemical recognition thus have converged across phylogenetically diverse taxa to promote the exploitation of a valuable, shared, prey resource. By providing critical sensory information, KEYSTONEin drives mussel predation and initiates trophic cascades that shape community structure and function. KEY-STONEin is necessary and sufficient as a predatory cue of considerable ecological consequence.

Phycology for the ecologist.

Fifty years ago, Robert Treat Paine published his seminal paper on food web complexity and biodiversity (Paine 1966). In this work, Paine used sea stars to illustrate how relationships among species were key determinants of emergent ecological patterns, and in so doing he injected a healthy dose of testable mechanism into a field that was largely phenomenological at the time. The example of the sea star Pisaster ochraceus as a keystone predator (Paine 1966, 1969) remains a standard example in Ecology textbooks, and undergraduates who take ecology courses today are likely to associate the name Paine with starfish. This article is protected by copyright. All rights reserved.

Sea Star Wasting Disease in the Keystone Predator Pisaster ochraceus in Oregon: Insights into Differential Population Impacts, Recovery, Predation Rate, and Temperature Effects from Long-Term Research.

Sea star wasting disease (SSWD) first appeared in Oregon in April 2014, and by June had spread to most of the coast. Although delayed compared to areas to the north and south, SSWD was initially most intense in north and central Oregon and spread southward. Up to 90% of individuals showed signs of disease from June-August 2014. In rocky intertidal habitats, populations of the dominant sea star Pisaster ochraceus were rapidly depleted, with magnitudes of decline in density among sites ranging from -2x to -9x (59 to 84%) and of biomass from -2.6x to -15.8x (60 to 90%) by September 2014. The frequency of symptomatic individuals declined over winter and persisted at a low rate through the spring and summer 2015 (~5–15%, at most sites) and into fall 2015. Disease expression included six symptoms: initially with twisting arms, then deflation and/or lesions, lost arms, losing grip on substrate, and final disintegration. SSWD was disproportionally higher in orange individuals, and higher in tidepools. Although historically P. ochraceus recruitment has been low, from fall 2014 to spring 2015 an unprecedented surge of sea star recruitment occurred at all sites, ranging from ~7x to 300x greater than in 2014. The loss of adult and juvenile individuals in 2014 led to a dramatic decline in predation rate on mussels compared to the previous two decades. A proximate cause of wasting was likely the “Sea Star associated Densovirus” (SSaDV), but the ultimate factors triggering the epidemic, if any, remain unclear. Although warm temperature has been proposed as a possible trigger, SSWD in Oregon populations increased with cool temperatures. Since P. ochraceus is a keystone predator that can strongly influence the biodiversity and community structure of the intertidal community, major community-level responses to the disease are expected. However, predicting the specific impacts and time course of change across west coast meta-communities is difficult, suggesting the need for detailed coast-wide investigation of the effects of this outbreak.

Prior exposure to low salinity affects the vertical distribution of Pisaster ochraceus (Echinodermata: Asteroidea) larvae in haloclines

MEPS Marine Ecology Progress Series Contact the journal Facebook Twitter RSS Mailing List Subscribe to our mailing list via Mailchimp HomeLatest VolumeAbout the JournalEditorsTheme Sections MEPS 542:123-140 (2016) - DOI: https://doi.org/10.3354/meps11563 Prior exposure to low salinity affects the vertical distribution of Pisaster ochraceus (Echinodermata: Asteroidea) larvae in haloclines Samuel M. Bashevkin1,5, Daniel Lee2, Paul Driver2, Emily Carrington3,4, Sophie B. George2,* 1Tufts University, Medford, Massachusetts 02155, USA 2Biology Department, Georgia Southern University, Statesboro, Georgia 30458, USA 3Department of Biology, University of Washington, Seattle, Washington 98105, USA 4Friday Harbor Laboratories, University of Washington, Friday Harbor, Washington 98250, USA 5Present address: Bodega Marine Laboratory, University of California, Davis, Bodega Bay, California 94923, USA *Corresponding author: georges@georgiasouthern.edu ABSTRACT: Increased freshwater discharge during spring/summer from the Fraser River into Puget Sound makes this region ideal to study the effects of low salinity (~20‰) on the vertical distribution of marine invertebrate larvae. We investigated whether exposing early developmental stages of the sea star Pisaster ochraceus to low salinity for 3, 7, and >25 d affects larval morphology and the ability of later developmental stages (brachiolariae) to swim to the surface in the presence or absence of haloclines. We also determined the effect of food patches at the halocline on swimming behavior. Larvae reared in low salinity throughout development had 55-95% shorter posterolateral arms than those in other treatments. In the absence of a halocline, exposure to low salinity for 7 or >25 d reduced the percentage of brachiolariae that swam to the surface (3 and 30%, respectively) compared to brachiolariae held for 0 or 3 d at low salinity (64 and 84%, respectively). Brachiolariae with no exposure to low salinity remained around the halocline in the presence of food, while those reared in continuous low salinity swam directly to the surface. Brachiolariae acclimated to low salinities and then transferred to a stratified water column avoided the halocline even in the presence of food. We conclude that exposure of early developmental stages to low salinity affects the swimming ability of brachiolariae. Our results suggest that sea star populations in the Pacific Northwest could be threatened if the influence of the Fraser River during the spring/summer continues to intensify in the southern Puget Sound region. KEY WORDS: Sea stars · Bipinnariae · Brachiolariae · Morphology · Posterolateral arm length · Vertical distribution · Halocline · Salinity Full text in pdf format Supplementary material PreviousNextCite this article as: Bashevkin SM, Lee D, Driver P, Carrington E, George SB (2016) Prior exposure to low salinity affects the vertical distribution of Pisaster ochraceus (Echinodermata: Asteroidea) larvae in haloclines. Mar Ecol Prog Ser 542:123-140. https://doi.org/10.3354/meps11563 Export citation RSS - Facebook - Tweet - linkedIn Cited by Published in MEPS Vol. 542. Online publication date: January 19, 2016 Print ISSN: 0171-8630; Online ISSN: 1616-1599 Copyright © 2016 Inter-Research.

Shore-level size gradients and thermal refuge use in the predatory sea star Pisaster ochraceus: the role of environmental stressors

The body size of a mobile intertidal invertebrate can determine its access to different microhabitats, and thus alter its exposure to environmental stressors. We surveyed a rocky inter- tidal keystone predator, the sea star Pisaster ochraceus, and characterized size-dependent distribution, defined by individuals' shore level and refuge use. At 2 field sites (in California and Oregon, USA) we examined temporal and geographical variability in habitat selection. We evalu- ated the hypothesis that environmental drivers measured on-site and body temperatures meas- ured using biomimetic sensors (i.e. 'robo-sea stars'), explained the observed distribution patterns, including shore-level size gradients, with larger animals lower on the shore. We tested the effect of size on animals' thermo- and desiccation-tolerance. Using robo-sea star data, thermal perform- ance curves and critical temperatures of different size classes, we investigated potential physio- logical and survival consequences of microhabitat use (shaded vs. sun-exposed). Pisaster is mostly found in thermal refugia during low tide even when the risk of thermal stress in sun-exposed areas is low, suggesting a risk-avoidance strategy. In sheltered microhabitats, Pisaster exhibited shore-level size gradients; in sun-exposed microhabitats, this pattern disappeared. The proportion of individuals found in shaded microhabitats increased with air temperature, solar radiation, and body temperature. Size-dependent sensitivity to stressful temperatures and wind speed did not explain the observed distribution patterns, suggesting that in the field, size constraints prevent larger animals from occupying refuges that small individuals can use. Our data reveal that, despite generally mild conditions, Pisaster risk-avoidance strategy buffers against rare but poten- tially highly stressful events.

Molecular phylogeny of four homeobox genes from the purple sea star Pisaster ochraceus.

Homeobox genes cloned from the purple sea star Pisaster ochraceus (Phylum Echinodermata/Class Asteroidea) were used along with related sequences available from members of other representative animal phyla to generate molecular phylogenies for Distal-less/Dlx, Hox5, Hox7, and Hox9/10 homeobox genes. Phylogenetic relationships were inferred based on the predicted 60 amino acid homeodomain, using amino acid (AA) and nucleotide (NT) models as well as the recently developed codon substitution models of sequence evolution. The resulting phylogenetic trees were mostly congruent with the consensus species-tree, grouping these newly identified genes with those isolated from other Asteroidea. This analysis also allowed a preliminary comparison of the performance of codon models with that of NT and AA evolutionary models in the inference of homeobox phylogeny. We found that, overall, the NT models displayed low reliability in recovering major clades at the Superphylum/Phylum level, and that codon models were slightly more dependable than AA models. Remarkably, in the majority of cases, codon substitution models seemed to outperform both AA and NT models at both the Class level and homeobox paralogy-group level of classification.

Quantifying the Effects of Predator and Prey Body Size on Sea Star Feeding Behaviors.

Body size plays a crucial role in determining the strength of species interactions, population dynamics, and community structure. We measured how changes in body size affect the trophic relationship between the sea star Pisaster ochraceus and its prey, the mussel Mytilus trossulus. We tested the effects of a wide range of predator and prey sizes on sea stars' prey-size preference, feeding rate, and prey tissue consumption. We found that preferred prey size increased with sea star size. Pisaster consumption rate (mussels consumed per day) and tissue intake rate (grams of tissue consumed per day) also increased with sea star size. Pisaster consumption rate, but not tissue intake rate, decreased with increasing mussel size. Juvenile sea stars preferred the most profitable prey sizes-that is, those that maximized tissue consumed per unit handling time. When adult sea stars were offered larger, more profitable mussels, tissue intake rates (grams per day) tended to increase, although this relationship was not statistically significant. Our results indicate that the Pisaster-Mytilus interaction depends on the sizes of both predator and prey, that predation rates are sensitive to even small changes in body size, and that shifts in size distributions may affect predator energetics and prey numbers differently depending on the factors that limit tissue consumption rates.

About the Cover.

Next article FreeAbout the CoverPDFPDF PLUSFull Text Add to favoritesDownload CitationTrack CitationsPermissionsReprints Share onFacebookTwitterLinked InRedditEmailQR Code SectionsMoreCoverThe sea star Pisaster ochraceus is a dominant rocky intertidal predator that lives along the west coast of North America. It plays a large role in determining local patterns of biodiversity via its interactions with mussels in the genus Mytilus. The cover image depicts juvenile P. ochraceus (the maroon, purple, and ochre sea stars) foraging among Mytilus trossulus (the bluish-black mussels) on a floating dock at the Hakai Beach Institute on Calvert Island, British Columbia. Several empty mussel shells are evidence of recent sea star predation events. The Pisaster-Mytilus interaction is famous for providing the inspiration for the “keystone predator” concept, and is now widely featured in textbooks.As a well-studied predator-prey pair, Pisaster and Mytilus make an ideal model system for addressing ecological and behavioral theory relating to the effects of body size. Body size of both predator and prey are key attributes of trophic interactions, as differences in body size can determine ease of prey capture, time required to handle and consume the prey, and number of prey required to meet energetic demands. On pages 192–200 of this issue, Gooding and Harley explore the ways in which variation in body size can affect the relationship between the predator P. ochraceus and its preferred prey in wave-protected waters, Mytilus trossulus.Gooding and Harley found that predation rates, expressed as mussels consumed per unit time, increased with increasing sea star size and decreased with increasing mussel size. Larger sea stars preferred to consume larger mussels. For juvenile sea stars, in which size relationships could be worked out in the greatest detail, prey-size preference corresponded with mussel size classes that allowed Pisaster to consume the most tissue in the least amount of time. Overall, the study found that even small changes in predator or prey body size could play a large role in predator energetics (tissue consumed per unit time) and prey population dynamics (individuals consumed per unit time). Because sea star and mussel growth rates and body size frequency distributions are affected by temperature and ocean acidification, changes in body size and the accompanying shifts in predation rates may be one important pathway through which global change alters community structure.Credits: Photo, Christopher D.G. Harley, University of British Columbia; cover design, Beth Liles, Marine Biological Laboratory. Next article DetailsFiguresReferencesCited by The Biological Bulletin Volume 228, Number 3June 2015 Published in association with the Marine Biological Laboratory Article DOIhttps://doi.org/10.1086/BBLv228n3cover © 2015 by Marine Biological Laboratory. All rights reserved.PDF download Crossref reports no articles citing this article.