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Letters to Nature
Nature 314, 248 - 250 (21 March 1985); doi:10.1038/314248a0

Martian atmospheric carbon dioxide and weathering products in SNC meteorites

R. H. Carr, M. M. Grady, I. P. Wright & C. T. Pillinger

Planetary Sciences Unit, Department of Earth Sciences, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK

SNC meteorites—four shergottites, three nakhlites and Chassigny—are postulated to have originated on Mars1. Their late crystallization ages (<1,300 Myr compared with 4,600 Myr for other igneous meteorites) and the presence, in shock-produced glass in EETA79001, of noble gas2 and nitrogen3 components resembling the martian atmosphere provide evidence for such a provenance. If this interpretation is correct then carbon dioxide, by far the most abundant constituent of the martian atmosphere4, should also be present. The stepped combustions described here show that most of the carbon present in the samples can be ascribed to terrestrial contamination. EETA79001, however, contains 4.6 p.p.m. of an isotopically distinct component enriched in 13C (delta 13C = +36permil), whereas high-temperature carbon of inferred igneous origin in this meteorite and other SNCs has a delta 13C value of about -30permil. The 12C/13C ratio of the isotopically heavy component is within the error limits of Viking measurements4 in the martian atmosphere and, thus, strengthens the case for a planetary origin. Another carbon-containing species, believed to be carbonate, has been found in Nakhla (delta 13C = between +12 and +24permil) and may be a product of atmospheric weathering on Mars.

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