Using Models of Permanent Shadow to Constrain Lunar Polar Water Ice Abundances

Details Using Models of Permanent Shadow to Constrain Lunar Polar Water Ice Abundances Using Models of Permanent Shadow to Constrain Lunar Polar Water Ice Abundances

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2297e&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2297

Physics

1

Scientific paper

We use models of permanent shadow to constrain the locations of enhanced
water- equivalent hydrogen at the Moon's poles, deconvolve Lunar
Prospector neutron data subject to these constraints and find numerous
locations of >1wt% H2O equivalent.

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