Publication Date:
2019-06-28
Description:
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.
Keywords:
LUNAR AND PLANETARY EXPLORATION
Type:
Earth and Planetary Science Letters (ISSN 0012-821X); 65; 2
Format:
text