Oxygen isotope relationships in iron meteorites

Details Oxygen isotope relationships in iron meteorites Oxygen isotope relationships in iron meteorites

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983e%26psl..65..229c&link_type=abstract

Earth and Planetary Science Letters (ISSN 0012-821X), vol. 65, no. 2, Nov. 1983, p. 229-232.

Computer Science

42

Iron Meteorites, Meteoritic Composition, Oxygen Isotopes, Abundance, Chondrites, Phosphates, Silicates, Trace Elements

Scientific paper

Iron meteorites with oxygen-bearing phases can be classified in terms of their oxygen isotopic abundances. These iron meteorite classes are isotopically similar to various stony meteorite classes, which may indicate a common origin. The group IAB and IIICD irons may be related to the winonaites; group IIE irons may be related to H chondrites; group IVA irons may be related to L or LL chondrites.

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