Subsurface Structure of Mare Serenitatis Observed with Lunar Radar Sounder and Multiband Imager Onboard Kaguya

Details Subsurface Structure of Mare Serenitatis Observed with Lunar Radar Sounder and Multiband Imager Onboard Kaguya Subsurface Structure of Mare Serenitatis Observed with Lunar Radar Sounder and Multiband Imager Onboard Kaguya

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1576o&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1576

Computer Science

Scientific paper

Radar reflectors are detected under a large area of Mare Serenitatis.
Meanwhile, layered structures are discernible on some crater walls in
mineral content maps of the mare. We discuss characteristics of the
subsurface layers by comparing these data.

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