Outer Main Belt Asteroids: Identification and Distribution of Four Spectral Groups

Details Outer Main Belt Asteroids: Identification and Distribution of Four Spectral Groups Outer Main Belt Asteroids: Identification and Distribution of Four Spectral Groups

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1182t&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1182

Physics

Scientific paper

VNIR spectra of outer main belt asteroids have revealed an interesting
trend spanning the 2.5 < a < 4.6 AU region. Four spectral groups
were identified: the Ceres-like group, the sharp OH group, the rounded
H2O group, and the featureless group.

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