Literature DB >> 11538265

Deuterium on Venus: observations from Earth.

C de Bergh1, B Bézard, T Owen, D Crisp, B L Lutz.   

Abstract

Absorption 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 micrometers, where the atmosphere is sounded in the altitude range from 32 to 42 kilometers (8 to 3 bars). The resulting value of the deuterium-to-hydrogen ratio (D/H) is 120 +/- 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 Ultraviolet 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.

Entities:  

Keywords:  NASA Discipline Exobiology; NASA Discipline Number 52-10; NASA Program Exobiology; Non-NASA Center

Mesh:

Substances:

Year:  1991        PMID: 11538265     DOI: 10.1126/science.251.4993.547

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  6 in total

1.  The D/H ratio and the evolution of water in the terrestrial planets.

Authors:  C de Bergh
Journal:  Orig Life Evol Biosph       Date:  1993-02       Impact factor: 1.950

2.  Reflections on O2 as a Biosignature in Exoplanetary Atmospheres.

Authors:  Victoria S Meadows
Journal:  Astrobiology       Date:  2017-04-26       Impact factor: 4.335

3.  The Habitability of Proxima Centauri b: Environmental States and Observational Discriminants.

Authors:  Victoria S Meadows; Giada N Arney; Edward W Schwieterman; Jacob Lustig-Yaeger; Andrew P Lincowski; Tyler Robinson; Shawn D Domagal-Goldman; Russell Deitrick; Rory K Barnes; David P Fleming; Rodrigo Luger; Peter E Driscoll; Thomas R Quinn; David Crisp
Journal:  Astrobiology       Date:  2018-02-12       Impact factor: 4.335

4.  Venus Atmospheric Composition in situ Data: A Compilation.

Authors:  Natasha M Johnson; Marta R R de Oliveira
Journal:  Earth Space Sci       Date:  2019-06-25       Impact factor: 2.900

5.  Proposed energy-metabolisms cannot explain the atmospheric chemistry of Venus.

Authors:  Sean Jordan; Oliver Shorttle; Paul B Rimmer
Journal:  Nat Commun       Date:  2022-06-14       Impact factor: 17.694

Review 6.  Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment.

Authors:  Victoria S Meadows; Christopher T Reinhard; Giada N Arney; Mary N Parenteau; Edward W Schwieterman; Shawn D Domagal-Goldman; Andrew P Lincowski; Karl R Stapelfeldt; Heike Rauer; Shiladitya DasSarma; Siddharth Hegde; Norio Narita; Russell Deitrick; Jacob Lustig-Yaeger; Timothy W Lyons; Nicholas Siegler; J Lee Grenfell
Journal:  Astrobiology       Date:  2018-05-10       Impact factor: 4.335

  6 in total

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