The MMCO-EOT conundrum:Same benthic δ 18 O, different CO 2

Knowledge on climate change during the Cenozoic largely stems from benthic δ 18 O records, which document combined effects of deep-sea temperature and ice volume. Information on CO 2 is expanding but remains uncertain and intermittent. Attempts to reconcile δ 18 O, sea level, and CO 2 by studying pr...

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Bibliographic Details
Published in:Paleoceanography
Main Authors: Stap, Lennert B., van de Wal, Roderik S.W., De Boer, Bas, Bintanja, Richard, Lourens, Lucas J.
Format: Article in Journal/Newspaper
Language:English
Published: 2016
Subjects:
Online Access:https://research.vu.nl/en/publications/5c2e6dff-cbbd-4dc4-8c6a-42b458acd544
https://doi.org/10.1002/2016PA002958
https://hdl.handle.net/1871.1/5c2e6dff-cbbd-4dc4-8c6a-42b458acd544
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Summary:Knowledge on climate change during the Cenozoic largely stems from benthic δ 18 O records, which document combined effects of deep-sea temperature and ice volume. Information on CO 2 is expanding but remains uncertain and intermittent. Attempts to reconcile δ 18 O, sea level, and CO 2 by studying proxy data suffer from paucity of data and apparent inconsistencies among different records. One outstanding issue is the difference suggested by proxy CO 2 data between the Eocene-Oligocene boundary (EOT) and the Middle-Miocene Climatic Optimum (MMCO), while similar levels of δ 18 O are shown during these times. This conundrum implies changing relations between δ 18 O, CO 2 , and temperature over time. Here we use a coupled climate-ice sheet model, forced by two different benthic δ 18 O records, to obtain continuous and mutually consistent records of δ 18 O, CO 2 , temperature, and sea level over the period 38 to 10 Myr ago. We show that the different CO 2 levels between the EOT and MMCO can be explained neither by the standard configuration of our model nor by altering the uncertain ablation parametrization on the East Antarctic Ice Sheet. However, we offer an explanation for the MMCO-EOT conundrum by considering erosion and/or tectonic movement of Antarctica, letting the topography evolve over time. A decreasing height of the Antarctic continent leads to higher surface temperatures, reducing the CO 2 needed to maintain the same ice volume. This also leads to an increasing contribution of ice volume to the δ 18 O signal. This result is, however, dependent on how the topographic changes are implemented in our ice sheet model.