2006 Philadelphia Annual Meeting (22–25 October 2006)

Paper No. 3
Presentation Time: 2:10 PM

ABRUPT RISE IN PALEOPROTEROZOIC O2 AND GLOBAL MICROBIAL SULFATE REDUCTION


WING, Boswell A., ESSIC and Dept. of Geology/Dept. of Earth and Planetary Sciences, University of Maryland/McGill University, Montreal, QC H2S 2C3, Canada, BAKER, Margaret A., Department of Geology, University of Maryland, College Park, MD 20742, BEKKER, Andrey, Geophysical Laboratory, Carnegie Institution of Washington, 5251 Broad Branch Rd., N.W, Washington, DC 20015-1305, KAUFMAN, Alan J., Geology Department, University of Maryland, College Park, MD 20742 and FARQUHAR, James, Earth System Science Interdisciplinary Center and Department of Geology, University of Maryland, College Park, MD 20742, wing@eps.mcgill.ca

  The inhibition, rise, and maintenance of atmospheric O2 each represent a distinct mode of the evolving relationship between geological processes and microbial activity on Earth.  This presentation will focus on sulfur isotopic evidence from Paleoproterozoic sedimentary rocks for the rise of O2. A first-order similarity exists between S isotopic anomalies preserved in some Archean rocks and those associated with short-wavelength UV photochemistry of SO2 (Farquhar et al., 2001). The Archean environment, therefore, likely permitted production and preservation of the isotopic signatures of UV-driven SO2 photochemistry.  In particular, photochemical models indicate that only O2 levels below 10-5 PAL allow preservation of S isotopic anomalies (Pavlov and Kasting, 2002).  This implies that sulfur isotopic anomalies are a low resolution but high sensitivity proxy for O2. In the Transvaal Supergroup, South Africa, S isotopic anomalies are found in the ~2.46 Ga Kuruman Iron Fm. (33S anomalies from -2 to +2 per mil off of predictions from a reference mass-dependent fractionation relationship), while the ~2.32 Rooihoogte and Timeball Hill Fms. preserve 33S abundances within -0.1 to 0.3 per mil of mass dependence (Bekker et al., 2004).  A significant threshold in O2 abundance must have been crossed sometime between ~2.45 and ~2.32 Ga.  In the Transvaal Basin, this interval encompasses the Duitschland Fm., and we measured S isotopic compositions of carbonate-associated sulfate (CAS) and acid-volatile S (AVS) from this formation in order to more precisely define the nature of the Paleoproterozoic rise in O2 The lower Duitschland Fm. preserves significant 33S isotopic anomalies in both CAS (up to 0.8 ä) and AVS (up to 1.4 ä).  In contrast, CAS from the upper Duitschland Fm. has 33S abundances within 0.0 and 0.2 per mil of mass dependence.  This shift mimics the gross S isotopic transition that has been identified in Paleoproterozoic rocks (Farquhar et al, 2001; Bekker et al., 2004; Papineau et al., 2005) but occurs here over ~200 m of section.  Importantly, 34S abundances in CAS jump by up to ~30 per mil when sizable 33S anomalies disappear.  This dichotomy suggests that an abrupt re-organization of the S cycle accompanied the rise of O2, and may imply an extreme sensitivity of the Paleoproterozoic atmosphere to microbial and geologic forcings.