Mineral chemistry of the shergottites, nakhlites, Chassigny, Brachina, pallasites and ureilites.

Details Mineral chemistry of the shergottites, nakhlites, Chassigny, Brachina, pallasites and ureilites. Mineral chemistry of the shergottites, nakhlites, Chassigny, Brachina, pallasites and ureilites.

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jgr....88..229s&link_type=abstract

Journal of Geophysical Research, Vol. 88, Suppl., p. B229 - B236

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16

Achondrites:Chemistry, Achondrites:Mineralogy

Scientific paper

The authors present minor-element analyses for olivine and pyroxene from the Shergottite-Nakhlite-Chassignite (SNC) group of meteorites that were attributed to Mars on the basis of a young crystallization age as well as other properties. They also include the olivine-rich Brachina meteorite, whose oxygen isotopic ratios rule out membership of the SNC group, in order to determine whether the minor elements are distinctly different. Also, the authors include pallasites and ureilites, which crystallized under reducing conditions, in order to provide a comparison with the more oxidized SNC meteorites.

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