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The Allende Meteorite and the Primordial Solar Nebula
アエンデ隕石と原始太陽系
1983
Journal of the Mineralogical Society of Japan
アエンデ隕石と原始太陽系
The constituent units of the Allende meteorite are briefly summarized and their possible origins are presented. Among coarse-grained CAI's, type-B2 CAI's are the most primitive, and type-A CAI's (compact type) are considered to have been formed from the type-B2 via type-B1 by gas reactions in the primordial solar nebula. Fine-grained CAI's or amoeboid olivine inclusions may be primarily aggregates consisting mainly of fassaite with small amounts of spinel and melilite or olivine with variable
doi:10.2465/gkk1952.16.91
fatcat:rbe2e4aktjgvxpxjhthop74n3u