Petrologic study of the Belgica 7904 carbonaceous chondrite - Hydrous alteration, oxygen isotopes, and relationship to CM and CI chondrites

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Carbonaceous Chondrites, Chondrule, Cosmochemistry, Olivine, Petrology, Hydration, Meteoritic Composition, Meteoritic Microstructures, Oxygen Isotopes, Meteorites, Alteration, Parent Bodies, Matrix, Mineralogy, Nebula, Phyllosilicates, Origin, Stony Meteorites, Chondrites, Petrology, Antarctic Meteorites, Belgica Meteorites, Yamato Meteorites, B7904, Y82162, Y86720, C Chondrites, Oxygen, Isotopes, Rims, Comparisons, Samples, Meteorite, Hydration, Chondrules, Composition, Description, Formation, Clasts, Pare

Scientific paper

The genetic relationships between the petrology, hydration reactions, and isotopic oxygen composition in the Belgica 7904 (B7904) carbonaceous chondrite, and the relationship between B7904 and the CM and CI chondrites were investigated by characterizing seven components separated from B7904. The seven specimens included two partially altered chondrules, two phylosilicate clasts, two olivine fragments, and one matrix sample. The results of the analyses and thermodynamic calculations suggest that CI chondrites may have been produced in a two-stage alteration process from materials similar to that of the B7904 matrix, by reactions with liquid water in their parent body. The common CM chondrites may have undergone aqueous alteration in the parent body, in addition to hydration in the nebula, resulting in two-stage alterations; the parent body may have been different from that of B7904.

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