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Research Article

Selenium isotopes record extensive marine suboxia during the Great Oxidation Event

Michael A. Kipp, Eva E. Stüeken, Andrey Bekker, and Roger Buick
PNAS first published January 17, 2017; https://doi.org/10.1073/pnas.1615867114
Michael A. Kipp
aDepartment of Earth & Space Sciences and Astrobiology Program, University of Washington, Seattle, WA 98195-1310;
bVirtual Planetary Laboratory, NASA Astrobiology Institute, Seattle, WA 98195-1310;
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  • For correspondence: kipp@uw.edu
Eva E. Stüeken
aDepartment of Earth & Space Sciences and Astrobiology Program, University of Washington, Seattle, WA 98195-1310;
bVirtual Planetary Laboratory, NASA Astrobiology Institute, Seattle, WA 98195-1310;
cDepartment of Earth Sciences, University of California, Riverside, CA 92521;
dDepartment of Earth & Environmental Sciences, University of St. Andrews, St. Andrews, KY16 9AL, Scotland, United Kingdom
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Andrey Bekker
cDepartment of Earth Sciences, University of California, Riverside, CA 92521;
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Roger Buick
aDepartment of Earth & Space Sciences and Astrobiology Program, University of Washington, Seattle, WA 98195-1310;
bVirtual Planetary Laboratory, NASA Astrobiology Institute, Seattle, WA 98195-1310;
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  1. Edited by Mark H. Thiemens, University of California, San Diego, La Jolla, CA, and approved December 13, 2016 (received for review September 24, 2016)

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Significance

Oxygen is essential for eukaryotic life. The geologic record of early Earth contains abundant evidence of low oxygen levels, and accordingly, a lack of eukaryote fossils. The rise of oxygen to near-modern levels at the end of the Proterozoic Era is thus often cited as the trigger for the evolutionary radiation of complex life forms at this same time. Here we present selenium geochemical data that indicate an expansion of suboxic (>0.4 μM O2) habitats in the shallow oceans between 2.32 and 2.1 Ga––more than one billion years before eukaryotes become abundant in the fossil record. These environments could have harbored the earliest stages of eukaryotic evolution, but may have been too transient for substantial diversification to occur.

Abstract

It has been proposed that an “oxygen overshoot” occurred during the early Paleoproterozoic Great Oxidation Event (GOE) in association with the extreme positive carbon isotopic excursion known as the Lomagundi Event. Moreover, it has also been suggested that environmental oxygen levels then crashed to very low levels during the subsequent extremely negative Shunga–Francevillian carbon isotopic anomaly. These redox fluctuations could have profoundly influenced the course of eukaryotic evolution, as eukaryotes have several metabolic processes that are obligately aerobic. Here we investigate the magnitude of these proposed oxygen perturbations using selenium (Se) geochemistry, which is sensitive to redox transitions across suboxic conditions. We find that δ82/78Se values in offshore shales show a positive excursion from 2.32 Ga until 2.1 Ga (mean +1.03 ± 0.67‰). Selenium abundances and Se/TOC (total organic carbon) ratios similarly show a peak during this interval. Together these data suggest that during the GOE there was pervasive suboxia in near-shore environments, allowing nonquantitative Se reduction to drive the residual Se oxyanions isotopically heavy. This implies O2 levels of >0.4 μM in these settings. Unlike in the late Neoproterozoic and Phanerozoic, when negative δ82/78Se values are observed in offshore environments, only a single formation, evidently the shallowest, shows evidence of negative δ82/78Se. This suggests that there was no upwelling of Se oxyanions from an oxic deep-ocean reservoir, which is consistent with previous estimates that the deep ocean remained anoxic throughout the GOE. The abrupt decline in δ82/78Se and Se/TOC values during the subsequent Shunga–Francevillian anomaly indicates a widespread decrease in surface oxygenation.

  • Paleoproterozoic
  • trace metals
  • oxygen
  • eukaryote evolution

Footnotes

  • ↵1To whom correspondence should be addressed. Email: kipp{at}uw.edu.
  • Author contributions: M.A.K., E.E.S., A.B., and R.B. designed research; M.A.K. and E.E.S. performed research; M.A.K. and E.E.S. analyzed data; and M.A.K., E.E.S., A.B., and R.B. wrote the paper.

  • The authors declare no conflict of interest.

  • This article is a PNAS Direct Submission.

  • This article contains supporting information online at www.pnas.org/lookup/suppl/doi:10.1073/pnas.1615867114/-/DCSupplemental.

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Selenium record of the Great Oxidation Event
Michael A. Kipp, Eva E. Stüeken, Andrey Bekker, Roger Buick
Proceedings of the National Academy of Sciences Jan 2017, 201615867; DOI: 10.1073/pnas.1615867114

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Selenium record of the Great Oxidation Event
Michael A. Kipp, Eva E. Stüeken, Andrey Bekker, Roger Buick
Proceedings of the National Academy of Sciences Jan 2017, 201615867; DOI: 10.1073/pnas.1615867114
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