The Continuing Puzzle of the Great Oxidation Event
Abstract
The rise of atmospheric O_2 was a milestone in the history of life. Although O_2 itself is not a climate-active gas, its appearance would have removed a methane greenhouse present on the early Earth and potentially led to dramatic cooling. Moreover, by fundamentally altering the biogeochemical cycles of C, N, S and Fe, its rise first in the atmosphere and later in the oceans would also have had important indirect effects on Earth's climate. Here, we summarize major lines of evidence from the geological literature that pertain to when and how O_2 first appeared in significant amounts in the atmosphere. On the early Earth, atmospheric O_2 would initially have been very low, probably <10^(−5) of the present atmospheric level. Around 2.45 billion years ago, atmospheric O_2 rose suddenly in what is now termed the Great Oxidation Event. While the rise of oxygen has been the subject of considerable attention by Earth scientists, several important aspects of this problem remain unresolved. Our goal in this review is to provide a short summary of the current state of the field, and make the case that future progress towards solving the riddle of oxygen will benefit greatly from the involvement of molecular biologists.
Additional Information
© 2009 Elsevier. Available online 27 July 2009. We thank the Howard Hughes Medical Institute (D.K.N.), the NASA Astrobiology and Exobiology programs (A.L.S., D.K.N. and R.E.S.) and NSF (P.V.W., R.E.S.) for supporting our work.Additional details
- Eprint ID
- 15122
- DOI
- 10.1016/j.cub.2009.05.054
- Resolver ID
- CaltechAUTHORS:20090817-144818780
- Howard Hughes Medical Institute (HHMI)
- NASA
- Created
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2009-09-08Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)