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
TRACING OF THE COUPLED SI AND FE CYCLE IN THE ARCHEAN OCEAN
Paper number: T249-12
Program: Technical Sessions
Time: 4:15 PM – 4:30 PM
Authors
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Xin-Yuan Zheng Presenting AuthorUniversity of Wisconsin-Madison; NASA Astrobiology Institute, Madison, WI
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Aaron M. SatkoskiUniversity of Wisconsin-Madison, NASA Astrobiology Institute, Madison, WI
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Brian L. BeardUniversity of Wisconsin-Madison; NASA Astrobiology Institute, Madison, WI
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Thiruchelvi R. ReddyUniversity of Wisconsin-Madison, NASA Astrobiology Institute, Madison, WI
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Nicolas J. BeukesUniversity of Johannesburg, Johannesburg
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Clark M. JohnsonUniversity of Wisconsin-Madison, NASA Astrobiology Institute, Madison, WI
Abstract
Our experiments showed that amorphous Fe-Si gel is a likely precursor of BIFs[1,3], potentially revising estimates of Si and Fe concentrations of Precambrian seawater. Also, our experiments showed that abiologic incorporation of Fe(II) into Fe(III)-Si gel is difficult to reach the Fe(II)-Fe(III) stoichiometry of magnetite, a common mineral found in BIFs. Microbial dissimilatory iron reduction of Fe(III)-Si gel can, however, easily produce a solid with Fe(II)-Fe(III) stoichiometry equal to magnetite, and leaves a unique, negative δ30Si signature that should be preserved in quartz associated with magnetite upon phase transformation of Fe-Si gel.
Here we test experiment predictions through measurement of δ30Si values in ~3.2 Ga Manzimnyama BIF, Barberton, South Africa (BARB 4 drill core). Analysis is focused on quartz that is closely associated with hematite and magnetite. Preliminary δ30Si results from hematite-rich samples show a large spread (-3.2‰ and -0.5‰). δ56Fe results from the same samples were interpreted to reflect the earliest oxygenic photosynthesis[4]. A broad negative correlation between δ30Si and δ56Fe for closely-related quartz and Fe oxide was observed, possibly reflecting a link between the extent of Fe oxidation and production of Fe-Si gel in the ocean. A lower extent of Fe(II) oxidation (higher δ56Fe) presumably led to formation of Fe-Si gel with limited Fe(II) incorporation, which would decrease δ30Si values. It is not yet clear, however, how formation of magnetite may occur through this mechanism. Further analysis of δ30Si and δ56Fe in magnetite-rich samples is underway, and will be used to further elucidate the origin of magnetite and the Si cycle at ~3.2 Ga.
[1] Zheng et al., GCA, 2016; [2] Reddy et al., GCA, 2016; [3] Konhauser et al., Earth-Science Rev, 2017; [4] Satkoski et al., EPSL, 2015
Geological Society of America Abstracts with Programs. Vol. 49, No. 6
doi: 10.1130/abs/2017AM-300243
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