Deriving the Distribution of Ordinary Chondrite (H, L, LL)-like Materials in Asteroids from Their Visible and Near-Infrared Reflectance Spectroscopy

Details Deriving the Distribution of Ordinary Chondrite (H, L, LL)-like Materials in Asteroids from Their Visible and Near-Infrared Reflectance Spectroscopy Deriving the Distribution of Ordinary Chondrite (H, L, LL)-like Materials in Asteroids from Their Visible and Near-Infrared Reflectance Spectroscopy

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1997h&link_type=abstract

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

Physics

1

Scientific paper

We have attempted to identify asteroid surface materials similar to
ordinary chondrite types by examining reflectance spectra of the S, A,
R, and V asteroids over the 1-µm band range, and derive their
distributions.

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