T285 Recoveries from Mass Extinction: Patterns, Processes, and Comparisons I
Wednesday, 8 October 2008
8:00 AM - 12:00 PM
Sulfur and Carbon Geochemistry and the End Permian Mass Extinction
Paper number: T285-14
Program: Technical Sessions
Time: 11:15 AM – 11:30 AM
Authors
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Frank CorsettiUniversity of Southern California, Los Angeles, CA
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Sylvain RichozAustrian Academy of Sciences, Graz, N/A
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Aymon BaudGeol Museum, Lausanne
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David BottjerUniversity of Southern California, Los Angeles, CA
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Douglas E. HammondUniv of Southern California, Los Angeles, CA
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Will BerelsonUSCEarth Sciences, Los Angeles, CA
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Alan J. KaufmanUniversity of Maryland, College Park, MD
Abstract
A detailed examination of the boundary interval reveals large negative fluctuations (~10‰) in δ34S before the mass extinction horizon that are coincident with three- to five-fold increases in total sulfur. The pre-extinction negative excursions are interpreted to have resulted from the oxidation of pyrite during the extraction of CAS; this mechanism may explain similar negative excursions in the δ34S of CAS reported from other P-T boundary sections. The increase in total sulfur has been reported from other P-T boundary sections and may indicate episodes of enhanced pyrite formation in shallow water carbonate settings due to the expansion of deep-ocean anoxia, possibly due to the introduction of volcanogenic reductants from the Siberian Traps.
At and above the mass extinction horizon, δ34S increases dramatically, and δ34S and δ13C exhibit negatively correlated fluctuations through a short stratigraphic interval. Here, the negative co-variation between δ34S and δ13C indicates rapidly changing redox conditions in the upper ocean, attributed to multiple upward excursions of the chemocline separating surface oxic from deep anoxic/sulfidic (euxinic) water masses. The direct cause of the mass extinction was likely the change to euxinic conditions in the shallow ocean, which may have introduced toxic levels of CO2 and H2S to the atmosphere.