Simulating OH/H 2 O formation by solar wind at the lunar surface

Details Simulating OH/H 2 O formation by solar wind at the lunar surface Simulating OH/H 2 O formation by solar wind at the lunar surface

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..215..449m&link_type=abstract

Icarus, Volume 215, Issue 1, p. 449-451.

Physics

1

Scientific paper

OH/H 2 O production from solar wind protons implanted to lunar regolith can be effectively simulated in laboratory with deuterium ions. At deuterium ion irradiation of olivine and SiO 2 powders measured mass spectra clearly show OD/D 2 O signatures. Proton-in-oxide production of OH/H 2 O being ubiquitous may be crucially important for life formation in Universe.

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