EVOLUTION OF THE DEVONIAN EARTH SYSTEM THROUGH THE LENS OF GEOCHEMISTRY: FROM CARBON CYCLING AND ANOXIA TO PLATE TECTONICS (Invited Presentation)
Traditional geochemical proxies such as carbon (δ13C) and sulfur (δ34S) isotopes have been a workhorse for identifying potential periods of anoxia in deep time. Paired positive δ13C and δ34S excursions recorded in older Cambrian and Ordovician successions are closely linked to biotic turnover and extinction events. However, the Devonian δ34S record has only recently been the focus of similar detailed study. Curiously, no major δ34S excursions occur alongside δ13C excursions during the Devonian mass extinction interval similar to older extinctions, suggesting that either anoxia was not as severe or that the sulfate reservoir was large enough to be buffered from brief anoxic periods. Though evidence for local anoxia exist in the form of changes in ichnofabrics, black shales, and I/Ca ratios of carbonate rocks, it is possible that anoxia was not as severe or global in extent. If weathering rates had increased to bury more organic carbon in nearshore settings, this could mimic the appearance of anoxia via increased δ13C values. Ongoing work using Li and Sr isotopes suggests that the radiation of land plants, and later uplift from orogenesis, occurred during these periods of anoxia. This has created a far more complicated story of the relationship extinction, anoxia, and the Devonian carbon cycle than previously thought.