4.7 Article

Significance of 56Fe depletions in late-Archean shales and pyrite

Journal

GEOCHIMICA ET COSMOCHIMICA ACTA
Volume 316, Issue -, Pages 87-104

Publisher

PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.gca.2021.10.013

Keywords

Iron; Isotopes; GOE; Archean; Oxygen

Funding

  1. NSF Frontiers in Earth System Dynamics program award [NSF EAR-1338810]
  2. Woods Hole Oceanographic Institution Postdoctoral Scholarship
  3. NASA Astrobiology Institute through the Science Mission Directorate [NNA15BB03A]
  4. Interdisciplinary Consortia for Astrobiology Research Program
  5. Canada Research Chairs
  6. NSERC [RGPIN-2019-0409]
  7. NSF Graduate Research Fellowship Program [026257-001]

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Research indicates that sedimentary rocks and minerals formed during the late Archean Eon contain lower levels of Fe-56 compared to other periods, possibly due to factors such as very negative seawater delta Fe-56 values, shuttling of light Fe isotopes in redox-stratified environments, and pyrite formation in Fe(II)-rich oceans. These processes, along with evidence of Fe shuttle and pyrite formation, likely played a role in driving strong 56Fe depletions. The connection between severe Fe-56 depletions and distant euxinic settings suggests a persistent presence of a very negative global seawater delta Fe-56 value during the latest Archean, supporting the idea of a prolonged initial oxidation process on Earth.
Sedimentary rocks and minerals formed during the final two-hundred million years of the Archean Eon (2.7 to 2.5 billion years ago, or Ga) are more depleted in Fe-56 than at any other time in Earth's past. Three hypotheses are proposed to explain these Fe-56 depletions: (1) a very negative late-Archean seawater delta Fe-56 value, (2) shuttling of isotopically light Fe across the chemocline in redox-stratified settings, and (3) pyrite formation in an Fe(II)-rich ocean. Each of these scenarios has different implications for the initial oxidation of Earth's surface, the climax of which - the Great Oxidation Event - immediately postdates the appearance of these 56Fe depletions in the rock record. To help inform this debate, we measured the Fe isotope ratios of 120 shale and pyrite samples from Western Australia (Mt. McRae Shale and Jeerinah Formation) and South Africa (Klein Naute Formation) deposited between-2.65 Ga and-2.50 Ga. As in previous studies, we also find very strong sedimentary Fe-56 depletions, to as low as delta Fe-56 =-2.06 +/- 0.08% in bulk shales and delta Fe-56 =-2.31 +/- 0.08% in pyrite. Some, but not all, of the severest (56F)e depletions appear alongside evidence of an Fe shuttle and local pyrite formation. These processes need not be mutually exclusive, and some combination of them likely played a partial, probably faciliatory role in driving some strong 56Fe depletions in our dataset. Most interestingly, and with little exception, the severest Fe-56 depletions appear in samples deposited farther from shore under H2S-rich and anoxic (euxinic) conditions. We find it difficult to explain this connection without invoking the persistent presence of a very negative global seawater delta Fe-56 value during the latest Archean, one that was most consistently captured in sediments formed in distal euxinic settings. In order to impart this isotopic effect on seawater, the global seawater Fe(II) reservoir needed to have been partially oxidized during at least the final few hundreds of millions of years leading up to the Great Oxidation Event. Our new data add support to the idea that Earth's initial oxidation was a long and protracted process rather than a rapid event. (C) 2021 Elsevier Ltd. All rights reserved.

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