Computer Science
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984lpico.526...20g&link_type=abstract
Press Abstracts from the Fifteenth Lunar and Planetary Science Conference, held March 12 -16, 1984, in Houston, TX. LPI Contribu
Computer Science
Carbonaceous Chondrites, Geochemistry, Inclusions, Meteoritic Composition, Mineralogy, Refractory Materials, Aluminum Oxides, Chemical Analysis, Crystallography, Electron Microscopy, Solar Corona, Spinel
Scientific paper
Inclusions found in type 3 carbonaceous chondrites such as the Allende meteorite are described and compared with those in the Murchison type 2 carbonaceous chondrite. Scanning electron microscope studies of the SH-6 (containing abundant hibonite) and the GR-1 (containing abundant hibonite and corundum) are discussed. Because corundum and hibonite are higher temperature condensates than the melilite and pyroxene found in the Allende meteorite, it is concluded that most refractory inclusions in the Murchison meteorite were isolated from the solar nebular gas at a higher temperature than their counterparts in the Allende meteorite. Whether the inclusion crystallized from a liquid or condensed directly from solar nebular gas is discussed.
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