Abstract. Antarctic continental ice masses fluctuated considerably
during the Oligocene “coolhouse”, at elevated atmospheric CO2
concentrations of ∼600–800 ppm. To assess the role of the
ocean in the Oligocene ice sheet variability, reconstruction of past ocean
conditions in the proximity of the Antarctic margin is needed. While
relatively warm ocean conditions have been reconstructed for the Oligocene
offshore of Wilkes Land, the geographical extent of that warmth is unknown. In
this study, we reconstruct past surface ocean conditions from glaciomarine
sediments recovered from Deep Sea Drilling Project (DSDP) Site 274 offshore of
the Ross Sea continental margin. This site, located offshore of Cape Adare is
ideally situated to characterise Oligocene regional surface ocean
conditions, as it is situated between the colder, higher-latitude Ross Sea
continental shelf and the warm-temperate Wilkes Land margin in the
Oligocene. We first improve the age model of DSDP Site 274 using integrated
bio- and magnetostratigraphy. Subsequently, we analyse organic walled
dinoflagellate cyst assemblages and lipid biomarkers (TEX86, TetraEther indeX of 86 carbon atoms) to
reconstruct surface palaeoceanographic conditions during the Oligocene
(33.7–24.4 Ma). Both TEX86-based sea surface temperature (SST) and
microplankton results show temperate (10–17 ∘C ± 5.2 ∘C) surface ocean conditions at Site 274 throughout the Oligocene.
Oceanographic conditions between the offshore Wilkes Land margin and Cape Adare
became increasingly similar towards the late Oligocene (26.5–24.4 Ma); this is
inferred to be the consequence of the widening of the Tasmanian Gateway,
which resulted in more interconnected ocean basins and frontal systems.
Maintaining marine terminations of terrestrial ice sheets in a proto-Ross Sea
with offshore SSTs that are as warm as those suggested by our data requires a strong ice flux
fed by intensive precipitation in the Antarctic hinterland during colder
orbital states but with extensive surface melt of terrestrial ice during
warmer orbital states.