The Effects of Grain Size, <10 µm - 4.75 mm, on the Reflectance Spectrum of Planetary Analogs from 0.35-2.5 µm

Details The Effects of Grain Size, <10 µm - 4.75 mm, on the Reflectance Spectrum of Planetary Analogs from 0.35-2.5 µm The Effects of Grain Size, <10 µm - 4.75 mm, on the Reflectance Spectrum of Planetary Analogs from 0.35-2.5 µm

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2082c&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

A basalt and a pyroxene in 29 grain size splits have been added to our
present study. Our hope is that this study will aid identification of
materials in planetary/asteroidal spectra and aid in discerning the
nature of the surface under investigation.

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