Outgassing/Regolith Interactions and Lunar Hydration

Details Outgassing/Regolith Interactions and Lunar Hydration Outgassing/Regolith Interactions and Lunar Hydration

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2079c&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2079

Physics

Scientific paper

A model of lunar interior outgassing successfully predicted that
hydrated regolith would be found in a patchy distribution concentrated
within ~20° of the poles, as detected by the Chandrayaan-1 M3 and in
hydrogen by epithermal neutron absorption.

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