T37 Sulfur Cycling in Precambrian to Recent Ocean-Atmosphere Systems: A Session Honoring the Career of William T. Holser
Monday, 5 November 2001
1:30 PM - 5:30 PM
SULFUR ISOTOPE EVIDENCE FOR ATMOSPHERIC BUT NOT BACTERIAL PROCESSES IN FORMATION OF EARLY ARCHEAN SEDIMENTARY SULFIDES AND SULFATES
Paper number: T37-11
Program: Technical Sessions
Time: 1:30 PM – 5:30 PM
Authors
-
Christopher D. CoathUniv. California, Los Angeles, CA
-
Stephen J. MojzsisUniv. Colorado, Boulder, CO
-
James FarquharUniv of Maryland, College Park, MD
-
James R. LyonsUniv. California, Los Angeles, CA
-
Kevin D. McKeeganUniv. California, Los Angeles, CA
-
T. Mark HarrisonUniv. California, Los Angeles, CA
Abstract
We measured sulfur isotope (32S, 33S, 34S) compositions of (1) sedimentary and vein barites; (2) pyrite intimately associated with barite; and (3) pyrite disseminated in black cherts, all from the 3.5 Ga-old Dresser Formation, North Pole area, Western Australia, using multi-collector ion microprobe as well as more conventional methods. Microscopic pyrites from growth laminae within vein barite have the same mass-independent isotopic depletion as the barite (D33S=–1‰) but are about 15‰ lighter in d34S compared to sulfates. This suggests in situ secondary mass-fractionation by hydrothermal processes. Disseminated pyrites in black cherts, on the other hand, commonly exhibit large positive mass-independent effects (D33S ~ +4‰) and very little depletion in 34S. These results support the suggestion that the oxidized and reduced sulfur cycles were decoupled during the Archean (Farquhar et al., Science, August 4, 2000). They also argue against the notion that disseminated pyrite in Archean black shales resulted from the bacterial reduction of seawater sulfate. Instead, the pyrite seems to have been derived from the reduction of elemental sulfur formed, at least in part, by photochemical processes in the anoxic Archean atmosphere.