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Deuterium on Venus - Observations from earthAbsorption lines of HDO and H2O have been detected in a 0.23-wave number resolution spectrum of the dark side of Venus in the interval 2.34 to 2.43 microns, where the atmosphere is sounded in the altitude range from 32 to 42 kilometers (8 to 3 bars). The resulting value of the D/H ratio is 120 + or - 40 times the telluric ratio, providing unequivocal confirmation of in situ Pioneer Venus mass spectrometer measurements that were in apparent conflict with an upper limit set from International UIltraviolet Explorer spectra. The 100-fold enrichment of the D/H ratio on Venus compared to earth is thus a fundamental constraint on models for its atmospheric evolution.
Document ID
19910041451
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
De Bergh, Catherine
(Observatoire de Paris-Meudon France)
Bezard, Bruno
(Paris Observatoire, Meudon, France)
Owen, Tobias
(Hawaii, University Honolulu, United States)
Crisp, David
(JPL Pasadena, CA, United States)
Maillard, Jean-Pierre
(CNRS Institut d'Astrophysique, Paris, France)
Date Acquired
August 14, 2013
Publication Date
February 1, 1991
Publication Information
Publication: Science
Volume: 251
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
91A26074
Funding Number(s)
CONTRACT_GRANT: NAGW-1505
CONTRACT_GRANT: NGR-33-015-141
CONTRACT_GRANT: NSF INT-87-15243
Distribution Limits
Public
Copyright
Other

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