Physics
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985lpsc...15..689k&link_type=abstract
(Lunar and Planetary Institute, NASA, American Geophysical Union, et al., Lunar and Planetary Science Conference, 15th, Houston,
Physics
6
Iron Meteorites, Meteoritic Composition, Planetary Evolution, Protoplanets, Barometers, Chemical Evolution, Chronometers, Feldspars, Melting, Silicates, Meteorites, Iron Meteorites, Evolution, Differentiation, Planetesimals, Iab Irons, Iiicd Irons, Parent Bodies, Compositon, Models, Heating, Thermal Effects, Formation, Sulfur, Silicate, Cores, Mantles, Sulfide, Melts, Fractional Crystallization, Rare Gases, Brecciation, Depth, Ages, Stony Meteorites, Comparisons, Winonaites, Samples, Meteorite, Barometry, P
Scientific paper
Some of the properties of IAB and IIICD iron meteorites thought to be derived from partially differentiated planetesimals are summarized, and the physical aspects that may have controlled parent body differentiation and affected the composition of the sulfide melt are outlined. The chemical evolution of the parent body is then discussed, and observations supporting the partial differentiation model are examined. Finally, an attempt is made to reinterpret barometric and chronometric data in light of the partial differentiation model, and tentative conclusions are presented.
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