Literature DB >> 31709275

Venus Atmospheric Composition in situ Data: A Compilation.

Natasha M Johnson1, Marta R R de Oliveira2.   

Abstract

The Venus atmosphere is of significant interest yet only rudimentary solid data has been gathered about its composition and chemistry. These measurements are scattered through time and place and are limited by parameters such as resolution and error margins as well as reinterpretations. This paper presents an extensive compilation of published in situ data for the atmospheric composition of Venus. It also includes remotely gathered measurements and some extrapolated and modeled data for the lower atmosphere. The composition tables are divided in four categories: noble gases, reactive gases, noble and non-noble isotopes. These tables were first presented in 2016 within the scientific heritage appendix of the Deep Atmosphere Venus Investigation of Noble gases, Chemistry, and Imaging (DAVINCI) mission proposal. These tables provide respective measurements, error margins, techniques, altitudes, instruments, mission and references. The objective of this paper is to provide a simple, comprehensive list of available measurements to date; in particular, the in situ data, to serve as a quick overall Venus atmosphere data reference.

Keywords:  Venus; atmosphere; in situ data; isotopes; noble gases; reactive gases

Year:  2019        PMID: 31709275      PMCID: PMC6839549          DOI: 10.1029/2018EA000536

Source DB:  PubMed          Journal:  Earth Space Sci        ISSN: 2333-5084            Impact factor:   2.900


  4 in total

1.  A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO.

Authors:  Jean-Loup Bertaux; Ann-Carine Vandaele; Oleg Korablev; E Villard; A Fedorova; D Fussen; E Quémerais; D Belyaev; A Mahieux; F Montmessin; C Muller; E Neefs; D Nevejans; V Wilquet; J P Dubois; A Hauchecorne; A Stepanov; I Vinogradov; A Rodin; Jean-Loup Bertaux; D Nevejans; Oleg Korablev; F Montmessin; Ann-Carine Vandaele; A Fedorova; M Cabane; E Chassefière; J Y Chaufray; E Dimarellis; J P Dubois; A Hauchecorne; F Leblanc; F Lefèvre; P Rannou; E Quémerais; E Villard; D Fussen; C Muller; E Neefs; E Van Ransbeeck; V Wilquet; A Rodin; A Stepanov; I Vinogradov; L Zasova; F Forget; S Lebonnois; D Titov; S Rafkin; G Durry; J C Gérard; B Sandel
Journal:  Nature       Date:  2007-11-29       Impact factor: 49.962

2.  Venus was wet: a measurement of the ratio of deuterium to hydrogen.

Authors:  T M Donahue; J H Hoffman; R R Hodges; A J Watson
Journal:  Science       Date:  1982-05-07       Impact factor: 47.728

3.  Deuterium on Venus: observations from Earth.

Authors:  C de Bergh; B Bézard; T Owen; D Crisp; B L Lutz
Journal:  Science       Date:  1991-02-01       Impact factor: 47.728

4.  Composition and structure of the venus atmosphere: results from pioneer venus.

Authors:  J H Hoffman; R R Hodges; M B McElroy; T M Donahue; M Kolpin
Journal:  Science       Date:  1979-07-06       Impact factor: 47.728

  4 in total
  3 in total

1.  Production of ammonia makes Venusian clouds habitable and explains observed cloud-level chemical anomalies.

Authors:  William Bains; Janusz J Petkowski; Paul B Rimmer; Sara Seager
Journal:  Proc Natl Acad Sci U S A       Date:  2021-12-28       Impact factor: 11.205

2.  Venus' Mass Spectra Show Signs of Disequilibria in the Middle Clouds.

Authors:  Rakesh Mogul; Sanjay S Limaye; M J Way; Jaime A Cordova
Journal:  Geophys Res Lett       Date:  2021-04-14       Impact factor: 4.720

3.  The Case (or Not) for Life in the Venusian Clouds.

Authors:  Dirk Schulze-Makuch
Journal:  Life (Basel)       Date:  2021-03-20
  3 in total

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