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Deuterium on Mars - The abundance of HDO and the value of D/HDeuterium 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 + or - 4) x 10 to the -4th; 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 + or - 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.
Document ID
19880056948
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Owen, Tobias
(New York, State University Stony Brook, United States)
Maillard, Jean Pierre
(CNRS Institut d'Astrophysique, Paris, France)
De Bergh, Catherine
(Paris Observatoire, Meudon, France)
Lutz, Barry L.
(Lowell Observatory Flagstaff, AZ, United States)
Date Acquired
August 13, 2013
Publication Date
June 24, 1988
Publication Information
Publication: Science
Volume: 240
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
88A44175
Funding Number(s)
CONTRACT_GRANT: NSG-7499
CONTRACT_GRANT: NGR-33-015-141
Distribution Limits
Public
Copyright
Other

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