Physics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982georl...9..412k&link_type=abstract
Geophysical Research Letters, vol. 9, Apr. 1982, p. 412-415.
Physics
19
Crystallization, Iron Meteorites, Melts (Crystal Growth), Meteoritic Composition, Abundance, Iron, Nickel, Silicates, Sulfur, Trace Elements, Meteorites, Iron Meteorites, Origin, Crystallization, Saturation, Data, Iron, Nickel, Melt, Iab Meteorites, Iiicd Meteorites, Trace Elements, Partitioning, Parent Bodies, Sulfur, Patterns, Siderophiles, Genesis, Composition, Thermal History, Models, Evolution, Hypotheses, Heating, Comparisons
Scientific paper
It is suggested in light of trace element partitioning data in the Fe-Ni-S-P system that IAB and IIICD group iron meteorites come from one or more S-rich parent bodies. IAB and IIICD may be complementary fractional crystallization/partial melting suites from the same parent body, and their trace element patterns are consistent with CI sulfur and siderophile abundances of a parent body which would have been compositionally intermediate between ordinary and E4 chondrites. Since the model also explains several unusual irons, it becomes possible not only to understand th genesis of all irons, but to link them to the major groups of primitive and differentiated meteorites.
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