Spectral Analysis of the Distribution of Impact Melt-Rich Lithologies in Lunar Crater Kepler Using M^3 Data

Details Spectral Analysis of the Distribution of Impact Melt-Rich Lithologies in Lunar Crater Kepler Using M^3 Data Spectral Analysis of the Distribution of Impact Melt-Rich Lithologies in Lunar Crater Kepler Using M^3 Data

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2257o&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2257

Physics

Scientific paper

Moon Mineralogy Mapper data show Kepler impact melt to be gabbroic, and
highlight an uprange splash. A halo of less-crystalline material,
possibly derived from a collapsing impact plume, is shifted ~downrange.
Both surficial features are invisible in visual imagery.

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