Earthshine at the Lunar Poles and Volatile Stability

Details Earthshine at the Lunar Poles and Volatile Stability Earthshine at the Lunar Poles and Volatile Stability

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1886h&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1886

Physics

Scientific paper

Earthshine is too weak to devolatilize lunar regolith in permanently
shadowed craters. Therefore ice validation missions may be landed in
areas with direct line-of-sight to Earth, eliminating the need for and
cost of a dedicated relay satellite.

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