Terrestrial and extraterrestrial chemical components of early Archean impact spherule layers from Fairview Gold Mine, northern Barberton greenstone belt, South Africa

Author:

Gonçalves de Oliveira* Grace Juliana1,Reimold Wolf Uwe2,Crósta Álvaro Penteado1,Hauser Natalia2,Koeberl Christian3,Mader Dieter3,Schmitt Ralf-Thomas4,Mohr-Westheide Tanja5

Affiliation:

1. Institute of Geosciences, University of Campinas, R. Carlos Gomes 250, 13083-855 Campinas, São Paulo, Brazil

2. Laboratory of Geochronology and Isotope Geochemistry, Institute of Geosciences, University of Brasília, Darcy Ribeiro Campus, Asa Norte, CEP 70190-900, Brasília, Brazil

3. Department of Lithospheric Research, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria

4. Museum für Naturkunde–Leibniz Institute for Evolution and Biodiversity Science, Invalidenstrasse 43, 10115 Berlin, Germany

5. Museum für Naturkunde–Leibniz Institute for Evolution and Biodiversity Science, Invalidenstrasse 43, 10115 Berlin, Germany, and Institut für Geologische Wissenschaften, Freie Universität Berlin, Malteserstrasse 74-100, 12249 Berlin, Germany

Abstract

ABSTRACT Early Archean spherule layers, widely accepted to represent distal ejecta deposits from large-scale impact events onto the early Earth, have been described from several stratigraphic levels of the Barberton greenstone belt in South Africa. Recently, exploration drilling at the Fairview Gold Mine (25°43′53″S, 31°5′59″E) in the northern domain of the belt resulted in the discovery of a new set of spherule layer intersections. The Fairview spherule layers in drill cores BH5901, BH5907, BH5911, and BH5949 were intersected just a few meters apart, at about the same stratigraphic position within the transition from the Onverwacht Group to the Fig Tree Group. The Fairview spherule layers have petrographic and chemical similarities to at least three other well-known Barberton spherule layers (S2–S4), and multiple spherule layer bed intersections in drill cores BARB5 and CT3, all from about the same stratigraphic position. They are not uniform in composition, in particular with respect to abundances of highly siderophile elements. The highest concentrations of moderately (Cr, Co, Ni) and highly siderophile (Ir) elements are within the range of concentrations for chondrites and, thus, reinforce the impact hypothesis for the generation of the Fairview spherule layers. Iridium peak concentrations and Cr/Ir interelement ratios for spherule layer samples from drill cores BH5907, BH5911, and BH5949 suggest admixtures of 50%–60% chondritic material, whereas for the BH5901 spherule layer, only an admixture of 1% chondritic material is indicated. We discuss whether these four Fairview spherule layers represent the same impact event, and whether they can be correlated to any of the S2–S4, CT3, and BARB5 intersections.

Publisher

Geological Society of America

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