20 Undergraduate and Graduate Geoscience Student Showcase (Posters)
Friday, 17 March 2023
1:30 PM - 5:30 PM
Grand Ballroom A–D
MIDDLE MIOCENE QUALITATIVE RECONSTRUCTION OF THE OLIGOTROPHIC SOUTH ATLANTIC GYRE, IODP EXPEDITIONS 390/393
Paper number: 20-26
Program: Theme Sessions
Time: 1:30 PM – 5:30 PM
Authors
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Emily Racz EstesTexas A&M University, College Station, TX
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Adriane LamBinghamton University, Binghamton, NY
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Gilles GuerinColumbia University, Palisades, NY
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Jesse YeonTexas A&M University, College Station, TX
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Damon TeagleUniversity of Southampton, Southampton
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Julia S. ReeceTexas A&M University, College Station, TX
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Rosalind M. CoggonUniversity of Southampton, Southampton
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Jason SylvanTexas A&M University, College Station, TX
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Trevor WilliamsTexas A&M University, College Station, TX
Abstract
We carried out analysis of shipboard Natural Gamma Radiation (NGR) and X-ray fluorescence (XRF, collected at 2cm intervals at 10, 30, 50 kV) data from sediments of holes U1583C (30°43′S, 20°26′W, water depth 4214.6 m, 30Ma crust) and U1560A (30°24′S, 16°55′W, water depth 3724.4 mbsl, 15Ma crust). In Hole U1583C across the Middle Miocene, the K, Th and U signals become elevated near the onset of the MCO and remain so throughout the study interval. All three elements strongly correlate with one another in Hole U1583C. These findings suggest increased windiness and deposition of terrigenous sediments over the site in response to increased warming. However, this is not the case with NGR data from Hole U1560A. Here, K, Th and U values are lower through the Middle Miocene, and elements do not strongly correlate with one another. XRF data will help resolve differences between NGR signals at Sites U1583 and U1560. Future work will include conducting additional sediment and geochemical analyses to further characterize surface ocean changes in an oligotrophic gyre in response to the MCO and MMCT.
Geological Society of America Abstracts with Programs. Vol. 55, No. 2
doi: 10.1130/abs/2023SE-386040
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