The 3-μm Hydrated Silicate Signature on C Class Asteroids: Implications for Origins of Outer Belt Objects

Details The 3-μm Hydrated Silicate Signature on C Class Asteroids: Implications for Origins of Outer Belt Objects The 3-μm Hydrated Silicate Signature on C Class Asteroids: Implications for Origins of Outer Belt Objects

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988lpi....19..567j&link_type=gif

Abstracts of the Lunar and Planetary Science Conference, volume 19, page 567, (1988)

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