Spectral Features in C and C-like Asteroids and the Possible Presence of Phyllosilicates

Details Spectral Features in C and C-like Asteroids and the Possible Presence of Phyllosilicates Spectral Features in C and C-like Asteroids and the Possible Presence of Phyllosilicates

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1061o&link_type=abstract

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

Computer Science

1

Scientific paper

The composition of C and C-like asteroids can be determined from
reflectivity spectra, which closely resemble that of CI and CM
chondrites that are known to consist of phyllosilicates. The amount and
distribution of water may explain the difference.

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