Earth System Processes 2 (8–11 August 2005)

Paper No. 4
Presentation Time: 10:40 AM

THE ABSENCE OF MASS INDEPENDENT SULFUR ISOTOPE FRACTIONATION IN ARCHEAN SEDIMENTARY ROCKS: EVIDENCE FOR AN OXIC ATMOSPHERE?


WATANABE, Yumiko, Astrobiology Research Center & Dept. of Geosciences, The Pennsylvania State Univ, 434 Deike Bldg, University Park, PA 16802, KLARKE, Alice I., Astrobiology Research Center & Dept. of Geosciences, The Pennsylvania State University, 434 Deike Blgd, University Park, PA 16802, POULSON, Simon, Geological Sciences, Univ of Nevada-Reno, 1664 N. Virginia St, Reno, NV 89557-0138 and OHMOTO, Hiroshi, Astrobiology Research Center & Dept. of Geosciences, The Pennsylvania State University, 435 Deike Building, University Park, PA 16802, yumiko@geosc.psu.edu

The current popular model for the Archean S-cycle (e.g., Farquhar, 2001; Kasting, 2001) predicts the signals of mass independent fractionation of sulfur isotopes (MIF-S: D33S = d33S -- 0.515d34S >[0±0.3 permil]) are in all sulfide and sulfate minerals that precipitated from surface waters (oceans and lakes) prior to 2.32 Ga ago. To test this prediction, we have determined the d34S, d33S, and D33S values of >70 bulk-rock samples from four Archean sedimentary formations recovered by the NASA Astrobiology Biosphere Drilling Project from the Pilbara district, Western Australia. These samples represent a ~150 m section of a lacustrine sandstone/shale unit (the 2.76 Ga Hardey Formation), a ~180 m section of a marine shale/sandstone unit (the 2.92 Ga Mosquito Creek Formation), and a ~100 m thick jasper/black-chert unit and an underlying ~30 m thick black-shale unit (the 3.46 Ga Towers Formation). Small MIF-S values (D33S = ~0.5 permil) were observed on samples from the black shale unit of the Towers Formation. However, samples from the other three formations exhibit no MIF-S (D33S = -0.3 to +0.3 permil), although their d34S values vary from -3 to +8 permil.

The mineralogical and chemical characteristics of the studied samples (e.g., morphology, grain size, and distribution of pyrite crystals relative to clays and quartz; C/S ratio; trace element content) indicate that essentially all the sulfur resides in pyrite crystals, which are not detrital in origin. The pyrite crystals with some MIF-S (DD33S = ~0.5 permil) appear to have formed by hydrothermal fluids during and/or after sediment diagenesis. However, those with no MIF-S formed within the host sediments during the early diagenetic stage (i.e., diagenetic pyrite) and/or in the overlying water bodies (i.e., syngenetic pyrite) by sulfate-reducing bacteria.

Possible interpretations of our data include, but are not restricted to, the following: (1) the Archean atmosphere fluctuated between oxic and anoxic, if atmospheric photochemical reactions are the only causes for MIF-S; or (2) large MIF-S values in some geologic samples were caused by mechanisms other than atmospheric photochemical reactions. Interpretation (2) implies that the presence or absence of MIF-S in geologic samples is not a measure of atmospheric pO2 level.