Computer Science
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989metic..24....1g&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 24, March 1989, p. 1-7. Research supported by SERC.
Computer Science
9
Carbonates, Chondrites, Isotopic Enrichment, Meteoritic Composition, Weathering, Antarctic Regions, Carbon, Oxygen, Petrography, Meteorites, Weathering, Lew 85320, Ordinary Chondrites, Lew Meteorites, Carbon, Oxygen, Isotopes, Composition, Carbonates, Snc Meteorites, Water, Samples, Meteorite, Laboratory Studies, Eeta 79001, Nakhla, Eet Meteorites, Nesquehonite, Formation, Origin, Silicates, Antarctic Meteorites
Scientific paper
Isotopic analysis of nesquehonite recovered from the surface of the LEW 85320 H5 ordinary chondrite shows that the delta C-13 and delta O-18 values of the two generations of bicarbonate (Antarctic and Texas) are different: delta C-13 = + 7.9 per mil and + 4.2 per mil; delta O-18 = + 17.9 per mil and + 12.1 per mil, respectively. Carbon isotopic compositions are consistent with equilibrium formation from atmospheric carbon dioxide at - 2 + or - 4 C (Antarctic) and + 16 + or - 4 C (Texas). Oxygen isotopic data imply that the water required for nesquehonite precipitation was derived from atmospheric water vapor or glacial meltwater which had locally exchanged with silicates, either in the meteorite or in underlying bedrock. Although carbonates with similar delta C-13 values have been identified in the SNC meteorites EETA 79001 and Nakhla, petrographic and temperature constraints argue against their simply being terrestrial weathering products.
Gibson Everett K. Jr.
Grady Michael
Pillinger Colin T.
Wright Ian P.
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