POPULATION-STRUCTURE, GROWTH AND RECRUITMENT OF THE EURYALINID BRITTLE-STAR ASTROBRACHION-CONSTRICTUM (ECHINODERMATA, OPHIUROIDEA) IN DOUBTFUL SOUND, FJORDLAND, NEW-ZEALAND
Bg. Stewart et Pv. Mladenov, POPULATION-STRUCTURE, GROWTH AND RECRUITMENT OF THE EURYALINID BRITTLE-STAR ASTROBRACHION-CONSTRICTUM (ECHINODERMATA, OPHIUROIDEA) IN DOUBTFUL SOUND, FJORDLAND, NEW-ZEALAND, Marine Biology, 127(4), 1997, pp. 687-697
The euryalinid brittle-star (snake star) Astrobrachion constrictum (Fa
rquhar) lives coiled around the branches of black coral (Antipathes fi
ordensis) colonies. Twenty-two vertical transects, 10 m wide by 30 m d
eep, were swum in Doubtful Sound over a 2.5 yr period from 1993 to 199
5. Numbers, disc diameters and colour morphotypes of brittle-stars inh
abiting coral colonies were recorded. 36.3% of the coral colonies >200
mm tall (n = 292) hosted greater than or equal to 1 Astrobrachion con
strictum (range 0 to 12). Overall, the population was patchily distrib
uted on the available coral habitat. The dark red colour morphotype of
A. constrictum was most common (87%, n = 279) followed by the yellow,
striped, and then spotted varieties. The population was comprised mai
nly of large (greater than or equal to 10 mm disc diam) individuals, a
nd juveniles were rarely encounter-ed, indicating low rates of recruit
ment or a high mortality of recruits. Disc-diameter data gathered from
this and previous studies indicated that growth in A. constrictum is
initially rapid, with individuals reaching a disc diameter of 15 mm in
similar or equal to 2.5 yr; growth decreases with age, as in other de
ep-sea ophiuroids. Growth rate within years, however, was not constant
, with faster growth in the spring/summer. Maximum size for A. constri
ctum is reached in similar or equal to 8 yr at similar to 23 mm disc d
iam. Anecdotal evidence indicates that A, constrictum may not be confi
ned solely to black coral colonies.