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


Abstract

The Late Devonian mass extinction is one of the “big five” mass extinctions of the Phanerozoic where ~40% of marine genera went extinct by the end of the Frasnian. The cause of this extinction is thought to be due to global anoxia based on the co-occurrence of positive carbon isotopic (δ13C) excursions and extinction pulses (known as the Kellwasser Event). It is thought that anoxic bottom waters increased organic burial rates and resulted in a positive δ13C excursion. Positive δ13C excursions, however, can be created via other processes, such as changes in weathering sources or alteration. Thus, if anoxia was the primary cause of the Devonian mass extinction (at the Frasnian-Famennian boundary; FFB), other proxy evidence for anoxia should also be preserved during this time in Earth history. Sulfur isotopes (δ34S) are one such proxy where anoxia will cause pyrite burial rates to increase and produce a positive δ34S excursion via the biologic fractionation effect associated with sulfate reduction and pyrite formation. Thus, if anoxia existed, both δ13C and δ34S should increase together.

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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