Earth's First Redox Revolution

Author:

Ostrander Chadlin M.12,Johnson Aleisha C.13,Anbar Ariel D.14

Affiliation:

1. School of Earth and Space Exploration, Arizona State University, Tempe, Arizona 85287, USA

2. Department of Marine Chemistry and Geochemistry, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts 02543, USA;

3. Department of Geophysical Sciences, The University of Chicago, Chicago, Illinois 60637, USA

4. School of Molecular Sciences, Arizona State University, Tempe, Arizona 85287, USA

Abstract

The rise of molecular oxygen (O2) in the atmosphere and oceans was one of the most consequential changes in Earth's history. While most research focuses on the Great Oxidation Event (GOE) near the start of the Proterozoic Eon—after which O2 became irreversibly greater than 0.1% of the atmosphere—many lines of evidence indicate a smaller oxygenation event before this time, at the end of the Archean Eon (2.5 billion years ago). Additional evidence of mild environmental oxidation—probably by O2—is found throughout the Archean. This emerging evidence suggests that the GOE might be best regarded as the climax of a broader First Redox Revolution (FRR) of the Earth system characterized by two or more earlier Archean Oxidation Events (AOEs). Understanding the timing and tempo of this revolution is key to unraveling the drivers of Earth's evolution as an inhabited world—and has implications for the search for life on worlds beyond our own. ▪  Many inorganic geochemical proxies suggest that biological O2 production preceded Earth's GOE by perhaps more than 1 billion years. ▪  Early O2 accumulation may have been dynamic, with at least two AOEs predating the GOE. If so, the GOE was the climax of an extended period of environmental redox instability. ▪  We should broaden our focus to examine and understand the entirety of Earth's FRR.

Publisher

Annual Reviews

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Astronomy and Astrophysics

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