T249 The Co-Evolution of Life and Its Environment during the Precambrian: The Rise of Oxygenic Photosynthesis and the Great Oxidation Event
Tuesday, 24 October 2017
1:30 PM - 5:30 PM
Skagit 5
CONSTRAINING THE MOLYBDENUM ISOTOPE BUDGET OF 2.63 – 2.50 GA OCEANS
Paper number: T249-15
Program: Technical Sessions
Time: 5:00 PM – 5:15 PM
Authors
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Brian KendallUniversity of Waterloo, Waterloo, ON
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Stephen J. RomanielloArizona State University, Tempe, AZ
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Gwyneth W. GordonArizona State University, Tempe, AZ
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Stephanie OlsonUniversity of California, Riverside, Riverside, CA
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Timothy LyonsUniversity of California, Riverside, CA
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Sune G. NielsenWoods Hole Oceanographic Institution, Woods Hole, MA
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Wang ZhengArizona State University, Tempe, AZ
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Ariel AnbarArizona State University, Tempe, AZ
Abstract
To address this gap, we measured Mo abundances and isotopic compositions for multiple marine shales deposited between 2.63 and 2.50 Ga under both non-euxinic and euxinic conditions, as delineated by correlative iron speciation analyses. The oldest euxinic samples, from the 2.63 Ga Jeerinah Formation (Fm), have δ98Mo as heavy as 1.2‰ (relative to NIST SRM 3134 + 0.25‰) after correction for detrital content. Non-euxinic samples from the 2.60 Ga Wittenoom Fm and 2.58 Ga Nauga Fm yield lower values, likely due to non-euxinic local depositional conditions, and thus do not directly constrain seawater Mo isotope compositions. The youngest euxinic samples, from the 2.50 Ga Klein Naute Fm, have heavier Mo isotope compositions up to 1.5‰, similar to values reported for the roughly coeval Mt. McRae Shale.
Our data from the euxinic Jeerinah Fm provide evidence for a low seawater Mo reservoir and isotope composition, suggesting low environmental O2 levels at 2.63 Ga. In contrast, higher Mo abundances and heavy isotope values in the 2.5 Ga euxinic shales from the Klein Naute Fm and Mt. McRae Shale are most likely a response to a higher seawater Mo reservoir and heavier global Mo isotope signature. Consistent with previous arguments, a “whiff” of atmospheric O2 at this time most likely enhanced delivery of Mo to the ocean and increased the area of oxic seafloor where isotopically light Mo is preferentially buried.
Geological Society of America Abstracts with Programs. Vol. 49, No. 6
doi: 10.1130/abs/2017AM-306885
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