Other
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988metic..23...13r&link_type=abstract
Meteoritics (ISSN 0026-1114), vol. 23, March 1988, p. 13-23.
Other
31
Abundance, Carbonaceous Chondrites, Meteoritic Composition, Petrology, Fine Structure, Grain Size, Olivine, Meteorites, Ningqiang, Classification, Petrology, Laboratory Studies, Cv3 Chondrites, Stony Meteorites, Samples, Meteorites, Description, Inaa, Composition, Procedure, Neutron Activation Analysis, Chondrules, Oxides, C Chondrites, Photomicrographs, Silicates, Inclusions, Refractory Material, Mafic Material, Olivine, Aggregates, Abundance, Petrogenesis, Opacity
Scientific paper
Ningqiang is an anomalous CV chondrite (oxidized subgroup) containing a high abundance of aggregational inclusions (13.7 vol pct) and low abundances of refractory inclusions (1.0 + 1.0 or - 0.5 vol pct) and bulk refractory lithophiles (about 0.82 x CV). Ningqiang may have agglomerated after most refractory inclusions at the nebular midplane had already been incorporated into other objects. Coarse-grained rims surround only about 5 percent of Ningqiang chondrules, compared to about 50 percent in normal CV chondrites. Aggregational inclusions appear to have formed by incipient melting of fine-grained aggregates at relatively low temperatures in the solar nebula, possibly by the mechanism responsible for chondrule formation.
Kallemeyn Gregory W.
Rubin Alan E.
Wang Dongming
Wasson John T.
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