Abundance, spatial distribution, and size structure of populations of Oreaster reticulatus (Echinodermata: Asteroidea) on sand bottoms

Three populations of Oreaster reticulatus (Linnaeus, 1758) inhabiting shallow-water (<4 m) seagrass habitats in the Grenadines (West Indies, Caribbean Sea) were associated predominantly with beds of Halodule wrightii. Occupation of fringing inshore areas of bare sand was inversely related to wave action; even where sandy patches occurred offshore, the preferred substratum was H. wrightii. The association of O. reticulatus with H. wrightii is related to the asteroid's microphagous feeding habit and the availability of food resources associated with the seagrass. O. reticulatus rarely occurred on dense beds of Thalassia testudinum, but was moderately abundant in areas of sparse cover. Differences in the occurrence of O. reticulatus among seagrass types may be related to factors afdecting foraging effort, such as the tractability of the substratum and mobility upon it. Populations of O. reticulatus exhibited an aggregated dispersion within beds of H. wrightii, possibly attributable to local substratum heterogeneity and/or reproductive behavior. Increased turbulence induced migration to deeper water and markedly increased aggregation along offshore boundaries. The populations were primarily adults, with some late juvenile stages. The paucity of juveniles and their cryptic behavior and coloration suggest that settlement and early postmetamorphic development occurs in alternate habitats, such as dense beds of T. testudinum. Interpopulation differences in size structure may be associated with differences in the quality and availability of food sources.