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Abstract
Geological and geochemical evidence indicates that the Antarctic ice sheet formed
during the Eocene-Oligocene transition, 33.5-34.0 million years ago. Modelling studies
suggest that such ice-sheet formation might have been triggered when atmospheric carbon
dioxide levels (pCO2atm) fell below a critical threshold of approximately 750 p.p.m.v.,
but the timing and magnitude of pCO2atm relative to the evolution of the ice sheet
has remained unclear. Here we use the boron isotope pH proxy on exceptionally well-preserved
carbonate microfossils from a recently discovered geological section in Tanzania to
estimate pCO2atm before, during and after the climate transition. Our data suggest
that are reduction in pCO2atm occurred before the main phase of ice growth,followed
by a sharp recovery to pre-transition values and then a more gradual decline. During
maximum ice-sheet growth, pCO2atm was between approximately 450 and approximately
1,500 p.p.m.v., with a central estimate of approximately 760 p.p.m.v. The ice cap
survived the period of pCO2atm recovery,although possibly with some reduction in its
volume, implying (as models predict) a nonlinear response to climate forcing during
melting. Overall, our results confirm the central role of declining pCO2atm in the
development of the Antarctic ice sheet (in broad agreement with carbon cycle modelling)
and help to constrain mechanisms and feedbacks associated with the Earth's biggest
climate switch of the past 65 Myr.
The sudden, widespread glaciation of Antarctica and the associated shift towards colder temperatures at the Eocene/Oligocene boundary (approximately 34 million years ago) (refs 1-4) is one of the most fundamental reorganizations of global climate known in the geologic record. The glaciation of Antarctica has hitherto been thought to result from the tectonic opening of Southern Ocean gateways, which enabled the formation of the Antarctic Circumpolar Current and the subsequent thermal isolation of the Antarctic continent. Here we simulate the glacial inception and early growth of the East Antarctic Ice Sheet using a general circulation model with coupled components for atmosphere, ocean, ice sheet and sediment, and which incorporates palaeogeography, greenhouse gas, changing orbital parameters, and varying ocean heat transport. In our model, declining Cenozoic CO2 first leads to the formation of small, highly dynamic ice caps on high Antarctic plateaux. At a later time, a CO2 threshold is crossed, initiating ice-sheet height/mass-balance feedbacks that cause the ice caps to expand rapidly with large orbital variations, eventually coalescing into a continental-scale East Antarctic Ice Sheet. According to our simulation the opening of Southern Ocean gateways plays a secondary role in this transition, relative to CO2 concentration.
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