Computer Science
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985gecoa..49..397n&link_type=abstract
Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 49, Feb. 1985, p. 397-410.
Computer Science
12
Iron Meteorites, Kamacite, Meteoritic Composition, Meteoritic Microstructures, Widmanstatten Structure, Computerized Simulation, Cooling, Nickel Alloys, Phase Diagrams, Precipitates, Meteorites, Iron Meteorites, Cooling, Experiments, Patterns, Kamacite, Thermal Effects, Techniques, Procedure, Electron Microscopy, Simulations, Chemistry, Composition, Taenite, Matrix, Description, Nucleation, Aem, Nickel, Phosphorous, Phases, Kinetics, Parent Bodies, Thermal History, Diffusion, Models
Scientific paper
Intragranular kamacite has been experimentally grown in Fe-Ni-P alloys containing between 5 and 10 percent by weight Ni and between 0 and 1.0 percent by weight P. The nucleation and growth process of these precipitates is studied using analytical electron microscopy techniques. A numerical model is developed to simulate the growth of intragranular kamacite in Fe-Ni-P alloys based on the experimental results, and this model is used to revise the existing cooling rate estimates of iron meteorites from observed Widmanstaetten patterns. It is found that heterogeneous sites like phospides are necessary for the nucleation of intragranular kamacite in the Fe-Ni-P system, and that kamacite size depends largely on the bulk Ni content and the cooling rate and to a lesser extent on the P concentration. The cooling rates predicted by the new model are two orders of magnitude greater than those previously estimated. To accommodate the new rates, meteorite parent bodies need only be a few kilometers in diameter.
Goldstein Joseph I.
Narayan C.
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