Mathematics – Logic
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988metic..23...35f&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 23, March 1988, p. 35-44.
Mathematics
Logic
66
Carbonaceous Chondrites, Grain Size, Meteoritic Composition, Solar Flares, Solar System, Calcium Carbonates, Chemical Composition, Size Distribution, Meteorites, Carbonates, Sulfates, Ci Chondrites, Stony Meteorites, Tonk, Formation, Parent Bodies, Samples, Meteorite, Composition, Electron Probe, Morphology, Mineralogy, Hypotheses, Laboratory Studies, Procedure, Alais, Experiments, Orgueil, Breunnerites, Photomicrographs, Dolomites, Ivuna, Matrix, Dating Methods, Microprobe Methods
Scientific paper
Compositions and morphologies of dolomites, breunnerites, Ca-carbonates, Ca-sulfates and Mg, Ni, Na-sulfates, and their petrologic interrelations, in four CI chondrites are consistent with their having been formed by aqueous activity on the CI parent body. Radiochronometric data indicate that this activity took place very early in solar-system history. No evidence for original ('primitive') condensates seems to be present. However, alteration apparently took place without change in bulk meteorite composition.
Fredriksson Kimmo
Kerridge John F.
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