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Carbon, oxygen and nitrogen isotopic compositions of possible martian weathering products in EETA 79001

Journal Article · · Geochimica et Cosmochimica Acta; (USA)
Carbon and oxygen isotopic analyses of carbonate-rich white-druse material isolated from a contact between lithologies A and C of the EETA 79001 shergottite indicate that this component is probably extraterrestrial in origin, and not simply an Antarctic weathering product. The {delta}{sup 13}C(+6.8{per thousand}) and {delta}{sup 18}O (+21.1{per thousand}) values of the calcium carbonate (predominantly calcite) are unlike {delta}{sup 13}C/{delta}{sup 18}O combinations of most common terrestrial carbonates (whether biogenic or abiogenic). However, {delta}{sup 13}C and {delta}{sup 18}O of the carbonates in EETA 79001 are very similar to the corresponding values for carbonates analyzed from Nakhla (a meteorite closely allied to shergottites). It seems apparent that the carbonate minerals in these SNC meteorites were formed on the meteorites' parent body (Mars ). Isotopic analysis of nitrogen liberated during combustion of a carbonate-rich fraction of EETA 79001 does not give any clear evidence for the {sup 15}N-enriched component isolated from EETA 79001 lithology C glass and postulated as trapped martian atmosphere. However, substantial amounts of nitrogen were present; the origin of these components is unclear but the low temperature of release poses some constraints.
OSTI ID:
5181138
Journal Information:
Geochimica et Cosmochimica Acta; (USA), Journal Name: Geochimica et Cosmochimica Acta; (USA) Vol. 52:4; ISSN GCACA; ISSN 0016-7037
Country of Publication:
United States
Language:
English