Letters to Nature

Nature 421, 245-249 (16 January 2003) | doi:10.1038/nature01290; Received 25 July 2002; Accepted 12 November 2002

Rapid Cenozoic glaciation of Antarctica induced by declining atmospheric CO2

Robert M. DeConto1 & David Pollard2

  1. Department of Geosciences, University of Massachusetts, Amherst, Massachusetts 01003, USA
  2. EMS Environment Institute, The Pennsylvania State University, University Park, Pennsylvania 16802, USA

Correspondence to: Robert M. DeConto1 Correspondence and requests for materials should be addressed to R.D. (e-mail: Email: deconto@geo.umass.edu).

The sudden, widespread glaciation of Antarctica and the associated shift towards colder temperatures at the Eocene/Oligocene boundary (approx34 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 continent5. 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.