T241 The Cretaceous–Paleogene Boundary: From Impact Cratering Processes to Mass Extinction Mechanisms
Wednesday, 13 October 2021
1:30 PM - 5:30 PM
D139/D140
INSIGHTS INTO K-PG EXTINCTION MECHANISMS USING AN EARTH SYSTEM MODEL
Paper number: T241-15
Program: Technical Sessions
Time: 5:00 PM – 5:15 PM
Authors
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Siddhartha MitraGreenville, NC
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Julio SepúlvedaUniversity of Colorado Boulder, Boulder, CO
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Charles BardeenNational Center for Atmospheric Research, Boulder, CO
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Jousha CoupeRutgers University, New Brunswick, NJ
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Victoria GarzaUniversity of Texas Rio Grande Valley, Edinburg, TX
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Cheryl HarrisonLouisiana State University, Baton Rouge, TX
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Kristen KrumhardtNational Center for Atmospheric Research, Boulder, CO
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Michael LevyNational Center for Atmospheric Research, Boulder, CO
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Nicole LovenduskiUniversity of Colorado, Boulder, CO
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Kenneth G. MacLeodUniversity of Missouri-Columbia, Columbia, MO
Abstract
A reason for the ongoing discussion about extinction mechanism comes from our poor understanding of Earth system responses to extreme perturbations. Accurate simulation of the Chicxulub impact is a major challenge because it requires altering an Earth system model for both deep time climate and extreme perturbations. Here, we adapt an Earth system model, which includes an explicit aerosol resolving scheme and an ocean biogeochemistry module, to simulate many of the responses across the K-Pg boundary. These simulations will allow for direct comparison with sedimentological, paleontological, geochemical, and climatological records, providing new insight into the mechanisms responsible for the K-Pg extinction. In this presentation, we will use a series of Earth system model sensitivity tests to explore what aspects of the asteroid impact were most devastating to life.
Geological Society of America Abstracts with Programs. Vol. 53, No. 6
doi: 10.1130/abs/2021AM-371061
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