Physics
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phys...39..410r&link_type=abstract
Physica Scripta (ISSN 0031-8949), vol. 39, no. 3, March 1989, p. 410-416. Research supported by the Ib Henriksens Fond; Statens
Physics
13
Cooling, Iron Meteorites, Kamacite, Solar System, Intermetallics, Iron, Nickel, Rates (Per Time), Widmanstatten Structure, Meteorites, Iron Meteorites, Parent Bodies, Cooling Rates, Iiicd Irons, Iab Irons, Ivb Irons, Carlton, Toluca, Odessa, Metallography, Kamacite, Chinga, Taenite, Laboratory Studies, Samples, Meteorite, Experiments, Procedure, Techniques, Comparisons, Nickel, Origin, Source, Diagrams, Core, Size, Regolith, Accretion
Scientific paper
Metallographic cooling rates for the iron meteorites Carlton (IIICD), Toluca (IAB), and Odessa (IAB) are calculated using the central Ni concentration versus taenite width method. For members of group IVB, the ungrouped iron meteorite Chinga, and the high-Ni members of IIICD and IAB, kamacite bandwidth cooling rates are determined. The cooling rates are up to several orders of magnitude faster than those from previous calculations.
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