PP007-01
Global climate and cryosphere controls on South Atlantic carbonate deposition since the Oligocene (30-0 Ma)

Monday, 7 December 2020: 10:30
Virtual
Anna Joy Drury1,2, Diederik Liebrand1, Thomas Westerhold1, Helen Beddow3, David A Hodell4, Nina Rohlfs1, Roy Wilkens5, Mitchell W Lyle6, Heiko Palike1 and Lucas Joost Lourens3, (1)MARUM - University of Bremen, Bremen, Germany, (2)University College London, Department of Earth Sciences, London, United Kingdom, (3)Department of Earth Sciences, Faculty of Geosciences, Utrecht University, Budapestlaan 4, 3584 CD, Utrecht, Netherlands, (4)University of Cambridge, Godwin Laboratory for Palaeoclimate Research, Cambridge, United Kingdom, (5)University of Hawaii at Manoa, School of Ocean and Earth Science and Technology (SOEST), Honolulu, HI, United States, (6)Oregon State University, College of Earth Ocean and Atmospheric Science, Corvallis, OR, United States
Abstract:
The evolution of the Cenozoic Icehouse from a unipolar to a bipolar world is broadly known; however, the exact development of orbital-scale climate variability is less well understood. High-resolution carbonate (CaCO3) records can provide insight into climate and carbon cycle dynamics, however few suitable Atlantic CaCO3 records exist. Here, we present the first astronomically-tuned South Atlantic CaCO3 record spanning the last 30 Myr, derived from X-ray fluorescence (XRF) ln(Ca/Fe) data collected at Ocean Drilling Program Site 1264. This new CaCO3 record allows us to investigate how changes in global climate and the cryosphere influenced orbital-scale dynamics during the Cenozoic Icehouse. We recognise three phases with distinctly different orbital controls on South Atlantic CaCO3 deposition, driven by major shifts in global climate: 1) strong ~110 kyr eccentricity pacing prevails during Oligo-Miocene global warmth (~30-13 Ma); 2) increased precession pacing appears after the mid Miocene Climate Transition (MMCT) (~14-8 Ma); 3) obliquity pacing appears in the late Miocene (~8 to ~3.3 Ma) following the increasing influence of high-latitude processes. Extensive CaCO3 dissolution occurs between 18.5-14.5 Ma, in response to the widespread early Miocene warmth and preceding Antarctic deglaciation across the Miocene Climate Optimum (~17-14.5 Ma) by 1.5 Myr. The precession-pacing of CaCO3 deposition after ~14 Ma signals a reorganisation of South Atlantic surface and/or deep-water circulation following Antarctic reglaciation at the MMCT. The increased sensitivity to precession at Site 1264 likely reflects increased regional CaCO3 productivity and/or an influx of cooler, less corrosive deep-waters. The highest %CaCO3 and mass accumulation rates indicate the late Miocene Biogenic Bloom (LMBB) occurs between ~7.8-3.3 Ma at Site 1264. The global onset of the LMBB may reflect an increased nutrient flux into the oceans due to enhanced glacial/chemical weathering and/or increased dust input. Regional variability in the timing and amplitude of the LMBB could reflect geographical differences in the degree of cooling, continental aridification and/or changes in oceanic circulation during the latest Miocene.