The reproductive biology of the deep-sea asteroids Benthopecten simplex (Perrier), Pectinaster filholi Perrier, and Pontaster tenuispinus Düben & Koren (phanerozonia : benthopectinidae) from the rockall trough

Abstract

Samples of three species of benthopectinid starfish were collected in a time-series from stations in the northern Rockall Trough. A detailed study was made of the reproductive biology of Benthopecten simplex (Perrier) from a fixed station at 2200 m. Studies of the gametogenic cycles of Pectinaster fllholi Perrier and Pontaster tenuispinus Düben & Koren from less regular and more scattered samplings are also presented. The oogenic cycles of the three species are similar. Growing oocytes line the ovary wall and come to lie in the lumen only when well developed. Accessory cells surrounding young oocytes become more numerous as the oocytes develop. Vitellogenesis begins when oocyte diameter reaches ≈ 250–300 μm and oocytes attain a maximum diameter of 950 μm in Benthopecten simplex, 850 μm in Pectinaster filholi, and 800 μm in Pontaster tenuispinus. Unspent oocytes are broken down by phagocytes and degenerate ovaries become filled with the breakdown products. Internal degeneration of large oocytes is not common. Size frequency data show a dominance of previtellogenic oocytes and a pattern of continuous growth of vitellogenic oocytes. There is no evidence of synchrony of growth between individuals and no suggestion of seasonal reproduction is evident from summated sample data. Spermatogenesis follows the pattern previously established for deep-sea asteroids. A mature male remains in a state of constant ripeness, ready to shed sperm at any chance encounter with a female releasing ripe eggs. There is no evidence of brooding in any of the species and from the large size and yolk content of the egg, we can infer direct lecithotrophic development demersally.