Characterization of unusual CI/CM/CR meteorites from reflectance spectroscopy

Details Characterization of unusual CI/CM/CR meteorites from reflectance spectroscopy Characterization of unusual CI/CM/CR meteorites from reflectance spectroscopy

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..577h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 577.

Physics

5

Meteorites, Spectral Reflectance, Carbonaceous Meteorites, Wavelengths, Antarctic Regions

Scientific paper

Certain reflectance spectra of CM2 and C2 meteorite powders have been identified as possible candidates for thermally metamorphosed CI/CM/CR meteorites, based on the absence of the 0.7-micron band and the 3-micron band shape and strength. The trends presently established indicate that thermally metamorphosed meteorites exhibit weaker 3-micron absorption bands centered at longer wavelengths than unheated ones.

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