Identifying Asteroidal Ordinary Chondrite Assemblages and Petrographic Types from VNIR Spectra

Details Identifying Asteroidal Ordinary Chondrite Assemblages and Petrographic Types from VNIR Spectra Identifying Asteroidal Ordinary Chondrite Assemblages and Petrographic Types from VNIR Spectra

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1412g&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

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Scientific paper

Existing spectral calibrations are sufficient to identify asteroidal
ordinary chondrite assemblages from VNIR (~0.7-2.5 µm) spectra,
but have limitations due to systematic mineralogical variations between
and within the H-, L-, and LL-types.

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