Polar amplification of orbital-scale climate variability in the early Eocene greenhouse world

Publication date

2024-06-12

Authors

Fokkema, Chris D.ISNI 0000000512527130
Agterhuis, TobiasISNI 0000000506317380
Gerritsma, Danielle
De Goeij, Myrthe
Liu, Xiaoqing
De Regt, Pauline
Rice, Addison HelenORCID 0000-0002-4507-6717ISNI 0000000507301348
Vennema, Laurens
Agnini, Claudia
Bijl, P.K.ORCID 0000-0002-1710-4012ISNI 0000000394379738

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Document Type

Article
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cc_by

Abstract

Climate variability is typically amplified towards polar regions. The underlying causes, notably albedo and humidity changes, are challenging to accurately quantify with observations or models, thus hampering projections of future polar amplification. Polar amplification reconstructions from the ice-free early Eocene (∼56-48 Ma) can exclude ice albedo effects, but the required tropical temperature records for resolving timescales shorter than multi-million years are lacking. Here, we reconstruct early Eocene tropical sea surface temperature variability by presenting an up to ∼4 kyr resolution biomarker-based temperature record from Ocean Drilling Program (ODP) Site 959, located in the tropical Atlantic Ocean. This record shows warming across multiple orbitally paced carbon cycle perturbations, coeval with high-latitude-derived deep-ocean bottom waters, showing that these events represent transient global warming events (hyperthermals). This implies that orbital forcing caused global temperature variability through carbon cycle feedbacks. Importantly, deep-ocean temperature variability was amplified by a factor of 1.7-2.3 compared to the tropical surface ocean, corroborating available long-term estimates. This implies that fast atmospheric feedback processes controlled meridional temperature gradients on multi-million year, as well as orbital, timescales during the early Eocene. Our combined records have several other implications. First, our amplification factor is somewhat larger than the same metric in fully coupled simulations of the early Eocene (1.1-1.3), suggesting that models slightly underestimate the non-ice-related - notably hydrological - feedbacks that cause polar amplification of climate change. Second, even outside the hyperthermals, we find synchronous eccentricity-forced temperature variability in the tropics and deep ocean that represent global mean sea surface temperature variability of up to 0.7 °C, which requires significant variability in atmospheric pCO2. We hypothesize that the responsible carbon cycle feedbacks that are independent of ice, snow, and frost-related processes might play an important role in Phanerozoic orbital-scale climate variability throughout geological time, including Pleistocene glacial-interglacial climate variability.

Keywords

Global and Planetary Change, Stratigraphy, Palaeontology, SDG 13 - Climate Action

Citation

Fokkema, C D, Agterhuis, T, Gerritsma, D, De Goeij, M, Liu, X, De Regt, P, Rice, A, Vennema, L, Agnini, C, Bijl, P K, Frieling, J, Huber, M, Peterse, F & Sluijs, A 2024, 'Polar amplification of orbital-scale climate variability in the early Eocene greenhouse world', Climate of the Past, vol. 20, no. 6, pp. 1303-1325. https://doi.org/10.5194/cp-20-1303-2024