Isotope composition and volume of Earth´s early oceans

Emily Catherine Pope, Dennis K. Bird, Minik Thorleif Rosing

    81 Citationer (Scopus)

    Abstract

    Oxygen and hydrogen isotope compositions of Earth´s seawater are controlled by volatile fluxes among mantle, lithospheric (oceanic and continental crust), and atmospheric reservoirs. Throughout geologic time the oxygen mass budget was likely conserved within these Earth system reservoirs, but hydrogen´s was not, as it can escape to space. Isotopic properties of serpentine from the approximately 3.8 Ga Isua Supracrustal Belt in West Greenland are used to characterize hydrogen and oxygen isotope compositions of ancient seawater. Archaean oceans were depleted in deuterium [expressed as δD relative to Vienna standard mean ocean water (VSMOW)] by at most 25± 5‰, but oxygen isotope ratios were comparable to modern oceans. Mass balance of the global hydrogen budget constrains the contribution of continental growth and planetary hydrogen loss to the secular evolution of hydrogen isotope ratios in Earth´s oceans. Our calculations predict that the oceans of early Earth were up to 26% more voluminous, and atmospheric CH4 and CO2 concentrations determined from limits on hydrogen escape to space are consistent with clement conditions on Archaean Earth.
    OriginalsprogEngelsk
    TidsskriftProceedings of the National Academy of Science of the United States of America
    Vol/bind109
    Udgave nummer12
    Sider (fra-til)4371-4376
    Antal sider6
    ISSN0027-8424
    DOI
    StatusUdgivet - 20 mar. 2012

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