Other
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983metic..18..113r&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 18, June 30, 1983, p. 113-121.
Other
15
Breccia, Chondrites, Enstatite, Meteoritic Composition, Abundance, Chemical Composition, Mineralogy, Petrography, Solar Corona, Meteorites, Enstatites, Chondrites, Breccias, Atlanta, Clasts, Formation, Solar Nebula, Source, Features, Models, Comparisons, Anlaysis, Procedures
Scientific paper
Atlanta is the fifth known brecciated enstatite chondrite. It contains a centimeter-sized troilite-rich clast, similar to those that occur in Blithfield. All of these clasts probably formed in the solar nebula under high pS2/pO2 conditions in a gas of non-cosmic composition. The absence of ordinary or carbonaceous chondrite clasts in any of the enstatite chondrite breccias and absence of enstatite chondrite clasts or materials formed at high pS2/pO2 ratios in ordinary and carbonaceous chondrite breccias support the model that enstatite chondrites were formed at a location distant from those of the other chondritic groups.
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