Rapid marine oxygen variability: Driver of the Late Ordovician mass extinction
Nevin P Kozik1, Seth A Young1, Sean M Newby1
1Department of Earth, Ocean and Atmospheric Science - National High Magnetic Field Laboratory, Florida State University, Tallahassee, FL 32306, USA.
Abstract:
The timing and connections between global cooling, marine redox conditions, and biotic turnover are underconstrained for the Late Ordovician. The second most severe mass extinction occurred at the end of the Ordovician period, resulting in ~85% loss of marine species between two extinction pulses. As the only "Big 5" extinction that occurred during icehouse conditions, this interval is an important modern analog to constrain environmental feedbacks. We present a previously unexplored thallium isotope records from two paleobasins that record global marine redox conditions and document two distinct and rapid excursions suggesting vacillating (de)oxygenation. The strong temporal link between these perturbations and extinctions highlights the possibility that dynamic marine oxygen fluctuations, rather than persistent, stable global anoxia, played a major role in driving the extinction. This evidence for rapid oxygen changes leading to mass extinction has important implications for modern deoxygenation and biodiversity declines.
More Related Videos
10:43Unraveling the Unseen Players in the Ocean - A Field Guide to Water Chemistry and Marine Microbiology
Published on: November 5, 2014
09:45Laboratory Simulation of an IronII-rich Precambrian Marine Upwelling System to Explore the Growth of Photosynthetic Bacteria
Published on: July 24, 2016
Related Concept Videos
Speciation Rates
Diversity of Protists III
Oxygenic Photosynthesis
The Fossil Record
Oxygen Requirements and Growth Patterns
Threats to Biodiversity
