A PHOTOGRAPHIC SURVEY OF THE EPIBENTHIC MEGAFAUNA OF THE ARCTIC LAPTEV SEA SHELF - DISTRIBUTION, ABUNDANCE, AND ESTIMATES OF BIOMASS AND ORGANIC-CARBON DEMAND
D. Piepenburg et Mk. Schmid, A PHOTOGRAPHIC SURVEY OF THE EPIBENTHIC MEGAFAUNA OF THE ARCTIC LAPTEV SEA SHELF - DISTRIBUTION, ABUNDANCE, AND ESTIMATES OF BIOMASS AND ORGANIC-CARBON DEMAND, Marine ecology. Progress series, 147(1-3), 1997, pp. 63-75
The epibenthic megafauna of the high-Arctic Laptev Sea shelf was inves
tigated in August/September 1993 and October 1995. At 13 stations in w
ater depths of between 14 and 45 m, series of 5 to 29 photographs, eac
h depicting about 1 m(2) of the seabed, were taken to assess epifaunal
distribution patterns and abundances. Furthermore, population biomass
of dominant brittle stars was estimated by combining abundance values
with size-mass relationships and size frequencies established by meas
uring specimens on scaled photographs. A total of 13 epibenthic specie
s were identified. Species numbers per station were low, ranging betwe
en 1 and 6. Total epibenthic abundances, averaging 173.7 ind. m(-2), r
anged considerably between 0.1 and 579.5 ind, m(-2). Except for some s
tations on shallow shelf banks <20 m that were characterized by bottom
-water salinities <30 due to fluvial dilution, the brittle star Ophioc
ten sericeum dominated the megabenthic shelf assemblages. At the flank
s of sunken Pleistocene river valleys in depths >30 m, it reached maxi
mum density and biomass values of 566 ind, m(-2) and 1.5 g ash-free dr
y mass (AFDM) m(-2), respectively. At some sites, the brittle star Oph
iura sarsi occurred in abundances of up to 35 ind. m(-2) and attained
a biomass of 3.8 g AFDM m(-2). Of local importance were the sea cucumb
er Myriotrochus rinckii (up to 70 ind. m(-2)) and the bivalve Arctinul
a greenlandica (up to 33 ind. m(-2)). All other species were recorded
with distinctly lower densities (less than or equal to 1 ind. m(-2)).
Gross estimates of population respiration and production of dominant b
rittle stars suggest that their organic carbon demand may amount to a
pooled average of about 4 mg C m(-2) d(-1) in the Laptev Sea, locally
even to a maximum of >10 mg C m(-2) d(-1). This finding indicates that
a substantial portion of the energy flow in this high-Arctic shelf ec
osystem may be channelled through dense brittle star assemblages.