Climatic and tectonic drivers of late Oligocene Antarctic ice volume

B. Duncan*, R. McKay, R. Levy, T. Naish, J. G. Prebble, F. Sangiorgi, S. Krishnan, F. Hoem, C. Clowes, T. Dunkley Jones, E. Gasson, C. Kraus, D. K. Kulhanek, S. R. Meyers, H. Moossen, C. Warren, V. Willmott, G. T. Ventura, J. Bendle

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

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Cenozoic evolution of the Antarctic ice sheets is thought to be driven primarily by long-term changes in radiative forcing, but the tectonic evolution of Antarctica may also have played a substantive role. While deep-sea foraminiferal oxygen isotope records provide a combined measure of global continental ice volume and ocean temperature, they do not provide direct insights into non-radiative influences on Antarctic Ice Sheet dynamics. Here we present an Antarctic compilation of Cenozoic upper-ocean temperature for the Ross Sea and offshore Wilkes Land, generated by membrane lipid distributions from archaea. We find trends of ocean temperature, atmospheric carbon dioxide and oxygen isotopes largely co-vary. However, this relationship is less clear for the late Oligocene, when high-latitude cooling occurred despite interpretation of oxygen isotopes suggesting global warming and ice-volume loss. We propose this retreat of the West Antarctic Ice Sheet occurred in response to a tectonically driven marine transgression, with warm surface waters precluding marine-based ice-sheet growth. Marine ice-sheet expansion occurred only when ocean temperatures further cooled during the Oligocene–Miocene transition, with cold orbital conditions and low atmospheric carbon dioxide. Our results support a threshold response to atmospheric carbon dioxide, below which Antarctica’s marine ice sheets grow, and above which ocean warming exacerbates their retreat.
Original languageEnglish
Pages (from-to)819–825
Number of pages7
JournalNature Geoscience
Issue number10
Early online date15 Sept 2022
Publication statusPublished - Oct 2022

Bibliographical note

Funding Information:
The authors are grateful for access to samples from the IODP core repository at Texas A&M University for DSDP Sites 270 and 274 and to the Alfred Wegener Institute for access to samples from the Cape Roberts Project. This study was funded via an Antarctica New Zealand Sir Robin Irvine PhD Scholarship, Scientific Committee of Antarctic Research Fellowship and Rutherford Foundation Postdoctoral Fellowship (RFT-VUW1804-PD) awarded to B.D., with additional funding by the Royal Society Te Apārangi Marsden Fund award MFP-VUW1808 (B.D. and R.M.) and the New Zealand Ministry of Business Innovation and Employment through the Antarctic Science Platform (ANTA1801) and contract C05X1001 (B.D., R.M., R.L., T.N. and J.G.P.). The Natural Environment Research Council funded J.B. (standard grant Ne/I00646X/1). J.B. and T.D.J. also acknowledge support from Natural Environment Research Council grant NE/P013112/1. D.K.K. was supported by US National Science Foundation award OCE-1326927. The authors are grateful for support from IODP and support in kind from the University of Birmingham and Yale University. We thank S. Schouten (NIOZ) for laboratory support and assistance with temperature data and J. Super for assistance with sample analysis while at Yale University.

Publisher Copyright:
© 2022, The Author(s), under exclusive licence to Springer Nature Limited.

ASJC Scopus subject areas

  • General Earth and Planetary Sciences


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