GSA Connects 2021 in Portland, Oregon

Paper No. 8-8
Presentation Time: 9:55 AM

A PERSISTENTLY LOW LEVEL OF ATMOSPHERIC OXYGEN IN EARTH’S MIDDLE AGE (Invited Presentation)


LIU, Xiao-Ming, Department of Earth, Marine and Environmental Sciences, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3315, KAH, Linda, Earth and Planetary Sciences, University of Tennessee, Knoxville, TN 37996, KNOLL, Andrew H., Department of Organismic and Evolutionary Biology, Harvard University, Cambridge, NC 02138, CUI, Huan, Ph.D., Stable Isotope Laboratory, Department of Earth Sciences, University of Toronto, Toronto, ON ON M5S, Canada; Equipe Géomicrobiologie, Institut de Physique du Globe de Paris (IPGP), Université de Paris, Paris, 75005, FRANCE, WANG, Chao, 104 South RD., 213 Mitchell Hall, Chapel Hill, NC 27599; Department of Earth, Marine and Environmental Sciences, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599-3315, BEKKER, Andrey, Dept. of Earth and Planetary Sciences, Univ. of California, Riverside, 900 University Avenue, Riverside, CA 92521 and HAZEN, Robert M., Earth and Planets Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, DC 20015

Resolving how Earth’s surface redox conditions evolved through the Proterozoic Eon is fundamental to understanding how biogeochemical cycles have changed through time. Previous studies mostly focused on individual stratigraphic units and do not provide long term estimates of atmospheric oxygen level through time. Moreover, carbonate rocks offer a better time-averaged view of the upper oceans and even the atmosphere. The redox sensitivity of cerium relative to other rare earth elements and its uptake in carbonate minerals make the Ce anomaly (Ce/Ce*) a particularly useful proxy for capturing redox conditions in the local marine environment. Here, we report Ce/Ce* data in marine carbonate rocks through 3.5 billion years (Ga) of Earth’s history, particularly focusing on the mid-Proterozoic (i.e., 1.8 – 0.8 Ga). To better understand the role of atmospheric oxygenation, we use Ce/Ce* data to estimate the partial pressure of atmospheric oxygen (pO2) through this time. Our thermodynamics-based modeling supports a major rise in atmospheric oxygen level in the aftermath of the Great Oxidation Event (~2.4 Ga), followed by relatively invariant pO2 of about 1% of present atmospheric level through most of the Proterozoic Eon (2.4 to 0.65 Ga).