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Early Archean spherule layers from the Barberton Greenstone Belt, South Africa: Mineralogy and geochemistry of the spherule beds in the CT3 drill core

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Abstract

Little is known about the Hadean and the Archean impact record on Earth. In the CT3 drill core from the Fig Tree Group of the northern Barberton Greenstone Belt, 17 spherule layer intersections occur, which, provide an outstanding new opportunity to gain insights into meteorite bombardment of the early Earth. CT3 spherules, as primary features, mostly exhibit textural patterns similar to those of the other Barberton spherule layers, but locally mineralogical and chemical compositional differences are observed, likely as a result of various degrees of alteration. The observed mineralogy of the spherule layers is of secondary origin and comprises K-feldspar, phyllosilicates, carbonates, sulfides, and oxides, with the exception of secondary Ni-Cr spinel that is of primary origin. Our petrographic investigations suggest alteration by K-metasomatism, sericitization, silicification, and carbonatization. Siderophile element contents of bulk samples show significant enrichments in Ni (up to 2 wt%) and Ir (up to ~3 ppm), similar to previously studied Archean spherule layers. These values are indicative of the presence of a meteoritic component. On the other hand, lithophile and chalcophile element abundances indicate hydrothermal overprint on the CT3 samples; this may also have influenced the redistribution of the meteoritic component(s). Last, we group the CT3 spherule layers, which occur in three intervals (A, B, and C), according to their petrographic and geochemical features, which indicate evidence for at least three distinct impact events before tectonic overprint that affected the original deposits.

Original languageEnglish
Pages (from-to)2586-2631
Number of pages46
JournalMeteoritics and Planetary Science
Volume52
Issue number12
DOIs
Publication statusPublished - Dec 2017

Funding

Thanks to the Council for Geosciences for access to drill core and Axel Hofmann from the University of Johannesburg for providing the samples. We want to acknowledge Lutz Hecht and his colleagues at MfN Berlin and Dan Topa from NHM Vienna for support with the SEM and EPMA investigations. We are grateful to Dieter Mader (Department of Lithospheric Research, University of Vienna) for help with the INAA, and his support during the study. We thank the staff at the Atominstitut, Vienna, for the irradiations. We thank Kathrin Krahn from MFN Berlin for sample preparation for XRF analysis. We are also grateful to Wencke Wegner and Lidia Pittarello (Department of Lithospheric Research, University of Vienna) for detailed comments on the manuscript and help with some figures. Toni Schulz's research was funded by the German Research Foundation (DFG, SCHU 3061/1-1). WUR's research is supported by the Deutsche Forschungsgemeinschaft (DFG) and the Museum fur Naturkunde Berlin. He contributed to this manuscript while on sabbatical at the Geochronology Laboratory of the University of Brasilia (Brazil). We are grateful to reviewers Bruce M. Simonson, Steven Goderis, and A.E. Michael Poelchau for their constructive comments on an earlier version of this manuscript.

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

  1. SDG 15 - Life on Land
    SDG 15 Life on Land

Austrian Fields of Science 2012

  • 105105 Geochemistry

Keywords

  • INNER SOLAR-SYSTEM
  • EARLY EARTH
  • IMPACT SPHERULES
  • MOUNTAIN LAND
  • METEORITE IMPACTS
  • SURFACE PROCESSES
  • ONVERWACHT GROUP
  • ORIGIN
  • EVOLUTION
  • ISOTOPE

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