Changes in the biochemical composition of the pyloric caeca of female seastars,Asterias rubens, during their annual reproductive cycle

Abstract

The biochemical composition of the pyloric caeca of female seastars (Asterias rubens) was studied throughout the annual reproductive cycle. The pyloric caeca index is high during the pseudo-rest stage of the ovaries and decreases gradually during ovarian growth. The pyloric caeca dry weight varies between 20 and 38% of the fresh weight. Lipids, and less prominently carbohydrates (both glycogen and other reducing sugars), seem to constitute the primary nutrient reserves for gonad growth. Proteins are also available to meet ovarian requirements during vitellogenesis. Glycogen levels are high in late autumn and winter and low at spawning time and in summer, whereas levels of the other reducing sugars are high in post-spawning months and subsequently gradually decrease during gonad development. The total lipid level is extremely variable (averaging 75 mg g-1 organ fresh weight), peak levels of over 200 mg g-1 being found in some individuals in summer and at spawning time. The free amino acid level is constant at about 20 mg g-1. The protein level is rather high throughout the annual cycle, and displays only minor changes. The observed patterns of decrease in major constituents suggest a rapid release of nutrient reserves from the pyloric caeca (deposited during the summer) at the onset of vitellogenesis. Moreover, the needs of the ovaries during further development seem to be so tremendous that during the winter months the digested food may be transported to the ovaries without prior deposition in the pyloric caeca. The changes observed in the pyloric caeca are discussed and compared with those occurring simultaneously in the ovaries.