The Effects of Grain Size, <45-1000 μm, on the Reflectance Spectrum of Planetary Analogs from 0.35-2.5 μm

Details The Effects of Grain Size, <45-1000 μm, on the Reflectance Spectrum of Planetary Analogs from 0.35-2.5 μm The Effects of Grain Size, <45-1000 μm, on the Reflectance Spectrum of Planetary Analogs from 0.35-2.5 μm

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1356c&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

2

Scientific paper

The spectral reflectance properties of three common planetary materials
are presented here (basalt, olivine, orthopyroxene). Five different
grain sizes have each been spectrally characterized from 0.35-2.5 μm.

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