Physics
Scientific paper
Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988sci...240.1767o&link_type=abstract
Science (ISSN 0036-8075), vol. 240, June 24, 1988, p. 1767-1770.
Physics
129
Abundance, Deuterium, Heavy Water, Isotopic Enrichment, Line Spectra, Mars (Planet), Hydrogen, Mars Atmosphere, Mars Surface
Scientific paper
Deuterium on Mars has been detected by the resolution of several Doppler-shifted lines of HDO near 3.7 micrometers in the planet's spectrum. The ratio of deuterium to hydrogen is (9±4)×10-4; the abundance of H2O was derived from lines near 1.1 micrometers. This ratio is enriched on Mars over the telluric value by a factor of 6±3. The enrichment implies that hydrogen escaped more rapidly from Mars in the past than it does now, consistent with a dense and warm ancient atmosphere on the planet.
de Bergh Catherine
Lutz Barry L.
Maillard Jean Pierre
Owen Tobias
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