Feeding ecology of the subantarctic sea star Anasterias minuta within tide pools in Patagonia, Argentina (original) (raw)

2008, Rev. Biol. Trop

The feeding ecology of the brooding sea star Anasterias minuta within tide pools was examined in Central and South Patagonia. 8 470 observations of sea stars were made. A. minuta does not feed while brooding. It consumes a wide range of prey, including molluscs and crustaceans, and can be regarded as a generalist or opportunistic predator. The purple mussel Perumytilus purpuratus was the most abundant prey item (57.6%). Other important prey were the gastropod Pareuthria plumbea, the isopod Exosphaeroma lanceolatum and the mussels Aulacomya atra atra and Mytilus edulis platensis. The proportion of sea stars feeding on sessile prey increases with sea-star size. A significant positive correlation was found between the size of the sea star and the size of the most frequent prey. The diet was fairly constant throughout the year, but diet composition differed between sites, shore level and sea-star size. The diversity of prey consumed by A. minuta was highest on the semi-exposed coast of Caleta Cordova Norte during the temperate season on the infralittoral fringe. A. minuta does not eat prey in proportion to its abundance beneath rocks within tide pools at the infralittoral fringe. Generally, the sea star consumed P. purpuratus and the gastropod P. plumbea more than other prey, even when they were not the most abundant prey present. At the midlittoral zone of the semi-exposed coast of Caleta Cordova Norte, the sea star feeds on prey species accordingly to their abundance. Larger P. purpuratus and E. lanceolatum were eaten disproportionately more often. A. minuta may have an opportunistic feeding strategy, taking unattached, wave-washed mussels when available rather that attached mussels. Consequently, it may have a variable impact on the community structure.

Selective Feeding by a Predatory Sea Star Across a Depth Gradient in Northern Patagonia, Chile

2021

Sea stars often function as keystone predators in food webs of intertidal and subtidal communities, especially in temperate and sub-polar regions. In South America the sea star Cosmasterias lurida is distributed along both the Atlantic and Pacific coasts of Patagonia and is one of the most conspicuous and abundant benthic predators in the shallow subtidal zone (<25 m). Its feeding strategy and prey selection are, however, still poorly known. This study describes the feeding behavior of C. lurida at a site in the Seno del Reloncaví (Chile), assessing its abundance, size and prey selection in the field relative to observed prey abundance and size along a bathymetric gradient. We hypothesized that C. lurida is a generalist predator, feeding on suitable prey according to their availability. However, we found that this predator only consumed a limited number (7 of 48) of potential prey species, primarily the slipper limpets Crepipatella spp. and the mussels Aulacomya ater and Mytilus ...

Feeding aggregations of sea stars ( Asterias spp. and Henricia sanguinolenta ) associated with sea urchin ( Strongylocentrotus droebachiensis ) grazing fronts in Nova Scotia

Marine Biology, 2007

Migrating feeding aggregations (or fronts) of sea urchins can dramatically alter subtidal seascapes by destructively grazing macrophytes. While direct effects of urchin fronts on macrophytes (particularly kelps) are well documented, indirect effects on associated fauna are largely unknown. Secondary aggregations of predators and scavengers form around fronts of Strongylocentrotus droebachiensis in Nova Scotia. We recorded mean densities of the sea stars Asterias spp. (mainly A. rubens) and Henricia sanguinolenta of up to 11.6 and 1.7 individuals 0.25 m−2 along an urchin front over 1 year. For Asterias, mean density at the front was 7 and 15 times greater than in the kelp bed and adjacent barrens, respectively. There was strong concordance between locations of peak density of urchins and sea stars (Asterias r = 0.98; H. sanguinolenta r = 0.97) along transects across the kelp–barrens interface, indicating that sea star aggregations migrated along with the urchin front at rates of up to 2.5 m per month. Size–frequency distributions suggest that Asterias at the front were drawn from both the barrens (smaller individuals) and the kelp bed (larger individuals). These sea stars fed intensively on mussels on kelp holdfasts and in adjacent patches. Urchin grazing may precipitate aggregations of sea stars and other predators or scavengers by incidentally consuming or damaging mussels and other small invertebrates, and thereby releasing a strong odor cue. Consumption of protective holdfasts and turf algae by urchins could facilitate feeding by these consumers, which may obtain a substantial energy subsidy during destructive grazing events.

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