T76 Co-Evolution of Earth’s Surface Environment and Eukaryotic Life from the Mid-Proterozoic to Early Paleozoic
Tuesday, 27 October 2020
1:30 PM - 5:30 PM
Meeting Rooms
WAS ANOXIA THE MAIN DRIVER OF THE LATE DEVONIAN MASS EXTINCTION? NEW INSIGHTS USING PAIRED STABLE CARBON AND SULFUR ISOTOPES
Paper number: T76-15
Program: Technical Sessions
Time: 4:25 PM – 4:40 PM
Authors
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Cole EdwardsAppalachian State University, Boone, NC
Abstract
This study reports new δ13C and δ34S trends measured from carbonate rocks (as carbonate-associated sulfate; CAS) and pyrite from three Late Devonian carbonate successions in the Great Basin region. In this study we test whether evidence for anoxia occurs before or at the FFB in the form of paired δ13C and δ34S excursions. Two of the measured sections contain a positive δ13C carbonate excursion above the FFB that co-occurs with CAS and pyrite δ34S excursions. The magnitude of these excursions varies between sections for CAS (δ34SCAS: 2–8‰) and pyrite (δ34SPY: 15–35‰), but both excursions postdate the main Frasnian extinction pulse. Petrographic study of these rocks shows that facies throughout the isotopic excursions exhibit near primary textures and early marine cements using cathodoluminescence microscopy. Because paired δ13C and δ34S excursions are found above the FFB from these sections and postdate the FFB, this suggests that anoxia was not the main cause for the extinction and other driver(s) may have contributed to extinctions than previously thought.
Geological Society of America Abstracts with Programs. Vol. 52, No. 6
doi: 10.1130/abs/2020AM-357493
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