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Oxidation of the Ediacaran Ocean

Naturevolume 444pages744747 (2006) | Download Citation

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Abstract

Oxygenation of the Earth’s surface is increasingly thought to have occurred in two steps. The first step, which occurred 2,300 million years (Myr) ago, involved a significant increase in atmospheric oxygen concentrations and oxygenation of the surface ocean1,2. A further increase in atmospheric oxygen appears to have taken place during the late Neoproterozoic period3,4 (800–542 Myr ago). This increase may have stimulated the evolution of macroscopic multicellular animals and the subsequent radiation of calcified invertebrates4,5, and may have led to oxygenation of the deep ocean6. However, the nature and timing of Neoproterozoic oxidation remain uncertain. Here we present high-resolution carbon isotope and sulphur isotope records from the Huqf Supergroup, Sultanate of Oman, that cover most of the Ediacaran period (635 to 548 Myr ago). These records indicate that the ocean became increasingly oxygenated after the end of the Marinoan glaciation, and they allow us to identify three distinct stages of oxidation. When considered in the context of other records from this period7,8,9,10,11,12,13,14,15, our data indicate that certain groups of eukaryotic organisms appeared and diversified during the second and third stages of oxygenation. The second stage corresponds with the Shuram excursion in the carbon isotope record16 and seems to have involved the oxidation of a large reservoir of organic carbon suspended in the deep ocean6, indicating that this event may have had a key role in the evolution of eukaryotic organisms. Our data thus provide new insights into the oxygenation of the Ediacaran ocean and the stepwise restructuring of the carbon6,16,17 and sulphur cycles3,18,19 that occurred during this significant period of Earth’s history.

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Acknowledgements

We thank D. Canfield for use of laboratory facilities and discussions; C. Colonero, J. Fong and S. Studley for laboratory assistance; A. Bradley, D. Finkelstein, G. Love, B. McElroy, A. Maloof and W. Watters for comments; and T. Lyons for suggestions that improved the manuscript. We thank Petroleum Development Oman (PDO) for access to samples and support for this project, and the Oman Ministry of Oil and Gas for permission to publish this paper. Support was provided by PDO and the National Aeronautics and Space Administration. J.P.G. and D.A.F. were supported by the Agouron Institute. L.M.P. was supported by a NASA Astrobiology Institute grant. R.E.S. was supported by an NSF Biocomplexity grant and a NASA Exobiology grant.

Author information

Author notes

    • J. P. Grotzinger

    Present address: Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, 91125, USA

Affiliations

  1. Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Massachusetts, 02139, Cambridge, USA

    • D. A. Fike
    • , J. P. Grotzinger
    •  & R. E. Summons
  2. Department of Geological Sciences, Indiana University, Bloomington, Indiana, 47405, USA

    • L. M. Pratt

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Reprints and permissions information is available at www.nature.com/reprints. The authors declare no competing financial interests.

Corresponding author

Correspondence to D. A. Fike.

Supplementary information

  1. Supplementary Notes

    This file contains Supplementary Figures 1–3 and also a discussion of lithostratigraphy, diagenesis, isotopic trends and Supplementary Methods. (DOC 2778 kb)

  2. Supplementary Table

    This file is excel spreadsheet containing the entire data presented in the paper. (XLS 58 kb)

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https://doi.org/10.1038/nature05345

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