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Mount McRae Shale

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The Mount McRae Shale is a 2.5-Ga-old unit of mudstone, siltstone, chert, iron formation, and dolomite in the Hamersley basin of the Pilbara craton, Western Australia. It is characterized by a high concentration of organic carbon (∼2–8 wt%), abundant disseminated pyrite (∼1 to ∼10 wt% S in the bulk rocks), and pyrite nodules (∼1–10 cm radius). Analysis of S and Fe isotopic compositions of carbonaceous pyritic shale recovered in the NASA-sponsored Astrobiology Drilling Program revealed variations in isotopic compositions that have been linked to changes in the composition of the ocean and the atmosphere and to fluctuations and a temporary rises of atmospheric oxygen that preceded the Great Oxygenation Event (GOE) at 2.32 Ga.

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Correspondence to Nicholas Arndt .

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© 2014 Springer-Verlag Berlin Heidelberg

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Arndt, N. (2014). Mount McRae Shale. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1029-3

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1029-3

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  • Online ISBN: 978-3-642-27833-4

  • eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics

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  1. Latest

    Mount McRae Shale
    Published:
    11 March 2021

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1029-4

  2. Original

    Mount McRae Shale
    Published:
    29 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1029-3