Computer Science
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993metic..28...86t&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 28, no. 1, p. 86-97.
Computer Science
109
Geochemistry, Meteorites, Meteoritic Composition, Nakhlites, Petrology, Electron Microscopy, Igneous Rocks, Mars (Planet), Mineralogy, Weathering, Meteorites, Aqueous Alteration, Lafayette, Snc Meteorites, Nakhlite, Stony Meteorites, Achondrites, Samples, Meteorite, Laboratory Studies, Description, Electron Microscopy, Sem, Tem, Origin, Formation, Mars, Minerals, Smectite, Texture, Composition, Water, Crust, Chemistry, Procedure, Petrography, Mineralogy, Veinlets, Fusion Crust, Oxidation, Transport, Tempera
Scientific paper
The structure and chemical composition of the Lafayette meteorite were examined using several methods. The meteorite contains abundant hydrous post-magnetic alteration material consisting of ferroan smectite clays, magnetite, and ferrihydrite. The textural relations, mineralogy, and composition of these materials were examined and their preterrestrial nature was documented. Olivine, pyroxene, and glass alteration are described and the bulk compositions of the alteration veinlets is discussed. Essential features of the geochemistry of the alteration processes are described. It is suggested that the alteration of the Lafayette meteorite occurred during episodic infiltrations of small volumes of saline water. Constraints placed on water chemistry and water-rock interactions in the Martian crust are outlined.
Barrett Ruth A.
Gooding James L.
Treiman Allan H.
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