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Abstract

An approach to coordinated, spatially resolved, insitu carbon isotope analysis of organic matter and carbonate minerals, and sulfur three- and four-isotope analysis of pyrite with an unprecedented combination of spatial resolution, precision, and accuracy is described. Organic matter and pyrite from eleven rock samples of Neoarchean drill core express nearly the entire range of C-13, S-34, S-33, and S-36 known from the geologic record, commonly in correlation with morphology, mineralogy, and elemental composition. A new analytical approach (including a set of organic calibration standards) to account for a strong correlation between H/C and instrumental bias in SIMS C-13 measurement of organic matter is identified. Small (2-3m) organic domains in carbonate matrices are analyzed with sub-permil accuracy and precision. Separate 20- to 50-m domains of kerogen in a single similar to 0.5cm(3) sample of the similar to 2.7Ga Tumbiana Formation have C-13=-52.3 +/- 0.1 parts per thousand and -34.4 +/- 0.1 parts per thousand, likely preserving distinct signatures of methanotrophy and photoautotrophy. Pyrobitumen in the similar to 2.6Ga Jeerinah Formation and the similar to 2.5Ga Mount McRae Shale is systematically C-13-enriched relative to co-occurring kerogen, and associations with uraniferous mineral grains suggest radiolytic alteration. A large range in sulfur isotopic compositions (including higher S-33 and more extreme spatial gradients in S-33 and S-36 than any previously reported) are observed in correlation with morphology and associated mineralogy. Changing systematics of S-34, S-33, and S-36, previously investigated at the millimeter to centimeter scale using bulk analysis, are shown to occur at the micrometer scale of individual pyrite grains. These results support the emerging view that the dampened signature of mass-independent sulfur isotope fractionation (S-MIF) associated with the Mesoarchean continued into the early Neoarchean, and that the connections between methane and sulfur metabolism affected the production and preservation of S-MIF during the first half of the planet's history.