Meteorite-asteroid spectral comparison - The effects of comminution, melting, and recrystallization

Details Meteorite-asteroid spectral comparison - The effects of comminution, melting, and recrystallization Meteorite-asteroid spectral comparison - The effects of comminution, melting, and recrystallization

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar...97..288c&link_type=abstract

Icarus (ISSN 0019-1035), vol. 97, no. 2, June 1992, p. 288-297.

Computer Science

48

Asteroids, Chondrites, Comminution, Melting, Meteoritic Composition, Recrystallization, Spectral Reflectance, Absorption Spectra, Albedo, Lunar Rocks, Meteorites, Regolith

Scientific paper

The present laboratory simulation of possible spectral-alteration effects on the optical surface of ordinary chondrite parent bodies duplicated regolith processes through comminution of the samples to finer rain sizes. After reflectance spectra characterization, the comminuted samples were melted, crystallized, recomminuted, and again characterized. While individual spectral characteristics could be significantly changed by these processes, no combination of the alteration procedures appeared capable of affecting all relevant parameters in a way that improved the match between chondritic meteorites and S-class asteroids.

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