Abstract

Sulfate minerals are rare in the Archean rock record and largely restricted to the occurrence of barite (BaSO4 ). The origin of this barite remains controversially debated. The mass-independent fractionation of sulfur isotopes in these and other Archean sedimentary rocks suggests that photolysis of volcanic aerosols in an oxygen-poor atmosphere played an important role in their formation. Here, we report on the multiple sulfur isotopic composition of sedimentary anhydrite in the ca. 3.22Ga Moodies Group of the Barberton Greenstone Belt, southern Africa. Anhydrite occurs, together with barite and pyrite, in regionally traceable beds that formed in fluvial settings. Variable abundances of barite versus anhydrite reflect changes in sulfate enrichment by evaporitic concentration across orders of magnitude in an arid, nearshore terrestrial environment, periodically replenished by influxes of seawater. The multiple S-isotope compositions of anhydrite and pyrite are consistent with microbial sulfate reduction. S-isotope signatures in barite suggest an additional oxidative sulfate source probably derived from continental weathering of sulfide possibly enhanced by microbial sulfur oxidation. Although depositional environments of Moodies sulfate minerals differ strongly from marine barite deposits, their sulfur isotopic composition is similar and most likely reflects a primary isotopic signature. The data indicate that a constant input of small portions of oxidized sulfur from the continents into the ocean may have contributed to the observed long-term increase in Δ33 Ssulfate values through the Paleoarchean.

Highlights

  • | INTRODUCTIONExamples of preserved Archean sulfate deposits are known from the Indian Dharwar Craton (Hoering, 1989; Muller et al, 2017), the southern African Barberton Greenstone Belt (BGB; Bao, Rumble, & Lowe, 2007; Heinrichs & Reimer, 1977; Muller, Philippot, Rollion-Bard, & Cartigny, 2016; Roerdink, Mason, Farquhar, & Reimer, 2012), and the western Australian Warrawoona Group of the Pilbara Block (Farquhar et al, 2000; Mojzsis et al, 2003; Roerdink et al, 2012; Shen, Farquhar, Masterson, Kaufman, & Buick, 2009; Ueno, Ono, Rumble, & Maruyama, 2008)

  • The abundance of detrital pyrite and uraninite in the Archean sedimentary record has been interpreted to indicate very low atmospheric oxygen levels (Burron et al, 2018; England, Rasmussen, Krapez, & Groves, 2002; Guy et al, 2012; Hofmann, Bekker, Rouxel, Rumble, & Master, 2009; Koglin, Frimmel, Minter, & Brätz, 2010)

  • The mass-independent fractionation of sulfur isotopes in these and other Archean sedimentary rocks suggests that photolysis of volcanic aerosols in an oxygen-poor atmosphere played an important role in their formation

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Summary

| INTRODUCTION

Examples of preserved Archean sulfate deposits are known from the Indian Dharwar Craton (Hoering, 1989; Muller et al, 2017), the southern African Barberton Greenstone Belt (BGB; Bao, Rumble, & Lowe, 2007; Heinrichs & Reimer, 1977; Muller, Philippot, Rollion-Bard, & Cartigny, 2016; Roerdink, Mason, Farquhar, & Reimer, 2012), and the western Australian Warrawoona Group of the Pilbara Block (Farquhar et al, 2000; Mojzsis et al, 2003; Roerdink et al, 2012; Shen, Farquhar, Masterson, Kaufman, & Buick, 2009; Ueno, Ono, Rumble, & Maruyama, 2008). Braided fluvial facies are stacked in wide and shallow channels with

MdQ4 MdS3
| METHODS
| DISCUSSION
| CONCLUSIONS
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