A Unifying Theory for H-Bearing Volatiles on the Moon

Details A Unifying Theory for H-Bearing Volatiles on the Moon A Unifying Theory for H-Bearing Volatiles on the Moon

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2751s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2751

Physics

Scientific paper

The low oxygen fugacity of the Moon requires that H_2 gas is the
dominant phase in the O-H system. H_2 is easily lost to space, so that
the low H content of most basalts, high D/H ratios, presence of Fe(o)
and high Cl-isotope ratios are all explained.

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