Estimates of the Lunar Surface Composition with Clementine Images and LSCC Data

Details Estimates of the Lunar Surface Composition with Clementine Images and LSCC Data Estimates of the Lunar Surface Composition with Clementine Images and LSCC Data

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1258s&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1258

Computer Science

4

Scientific paper

A new approach based on analysis of spectral and compositional data for
lunar samples by the LSCC and using the UVVIS Clementine data with 1 km
resolution is proposed to estimate and map the abundance of TiO2, SiO2,
and FeO, pyroxene and plagioclase content, and maturity degree (Is/FeO).

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