Abstract
The absence of redbeds, the occurrence of readily oxidizable minerals in placers, and the rarity of sulphate minerals are some features which suggest generally reduced conditions on the Earth's surface during Archaean time1. Supporting this conjecture are δ34S values near 0‰ for sulphides of sedimentary rocks2–4 and massive sulphide deposits5, since isotopic fractionation requires oxidation–reduction reactions. The flux of oxidized species during the Archaean produced by fixation of organic carbon was, however, comparable with modern levels6, but was largely consumed by reactions with a large supply of reduced mantle material4,7. Notable occurrences of Archaean sulphate are ∼3,400-Myr stratiform barites in Australia8,9, South Africa10 and India11, with δ34S ∼+4‰ (refs 8–10) which are believed to have formed by bacterial oxidation of primary (0‰) sulphide10. Consideration of the Archaean sulphur cycle has focused on sulphate of this origin. We draw attention here to sulphate of different isotopic composition, +8 to +14‰, of magmatic origin, that contributed to the total flux of oxidized species during the Archaean.
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Hattori, K., Cameron, E. Archaean magmatic sulphate. Nature 319, 45–47 (1986). https://doi.org/10.1038/319045a0
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DOI: https://doi.org/10.1038/319045a0
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