Mineralogy and cooling history of magnesian lunar granulite 67415

Details Mineralogy and cooling history of magnesian lunar granulite 67415 Mineralogy and cooling history of magnesian lunar granulite 67415

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24.1391t&link_type=abstract

In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z p 1391-1392 (SEE N94-20636 05-91

Mathematics

Logic

3

Computerized Simulation, Cooling, Lunar Composition, Lunar Geology, Mineral Deposits, Mineralogy, Annealing, Breccia, Diffusion, Metamorphism (Geology), Olivine

Scientific paper

Apollo granulite 67415 was investigated by mineralogical techniques to gain better understanding of cooling histories of lunar granulities. Cooling rates were estimated from chemical zoning of olivines in magnesian granulitic clasts by computer simulation of diffusion processes. The cooling rate of 10 deg C/yr obtained is compatible with a model of the granulite formation, in which the impact deposit was cooled from high temperature or annealed, at the depth of about 25 m beneath the surface.

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