posted on 2025-02-07, 15:34authored byTim E van Peer, Diederik Liebrand, Victoria E Taylor, Swaantje Brzelinski, Iris Wolf, André Bornemann, Oliver Friedrich, Steven M Bohaty, Chuang Xuan, Peter C Lippert, Paul A Wilson
<p dir="ltr">Earth’s obliquity and eccentricity cycles are strongly imprinted on Earth’s climate and widely used to measure geological time. However, the record of these imprints on the oxygen isotope record in deep-sea benthic foraminifera (δ18Ob) shows contradictory signals that violate isotopic principles and cause controversy over climate-ice sheet interactions. Here, we present a δ18Ob record of high fidelity from International Ocean Drilling Program (IODP) Site U1406 in the northwest Atlantic Ocean. We compare our record to other records for the time interval between 28 and 20 million years ago, when Earth was warmer than today, and only Antarctic ice sheets existed. The imprint of eccentricity on δ18Ob is remarkably consistent globally whereas the obliquity signal is inconsistent between sites, indicating that eccentricity was the primary pacemaker of land ice volume. The larger eccentricity-paced early Antarctic ice ages were vulnerable to rapid termination. These findings imply that the self-stabilizing hysteresis effects of large land-based early Antarctic ice sheets were strong enough to maintain ice growth despite consecutive insolation-induced polar warming episodes. However, rapid ice age terminations indicate that resistance to melting was weaker than simulated by numerical models and regularly overpowered, sometimes abruptly.</p>
Funding
This research was supported by NERC grants NE/K006800/1 (to P.A.W.), NE/K014137/1 (to P.A.W., C.X., and D.L.), NE/R018235/1 (to C.X. and T.E.v.P.), NE/T012285/1 including UCL’s CoA funding (to T.E.v.P. in a Co-I role), and NE/M021254/1 (to S.M.B. and P.A.W.), a Royal Society Wolfson Research Merit Award (to P.A.W.), and a studentship from the Graduate School of the National Oceanography Centre Southampton to T.E.v.P. T.E.v.P. was also supported as a Research Fellow, funded by the University of Leicester. Further funding for this study was provided by the German Research Foundation (DFG) grants FR2544/7, FR2544/12, and FR2544/17 (all to O.F.) and grant BO2505/9 (to A.B.).
History
Author affiliation
College of Science & Engineering
Geography, Geology & Environment
Source data are provided with this paper. The δ18Ob data and coulometric CaCO3 content generated in this study and the depth-age tie points used in the astronomical tuning have also been archived in the Pangaea database (https://doi.org/10.1594/PANGAEA.958176).