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Composition and structure of the atmosphere of Venus

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Abstract

Although in recent years much has been learned about the atmospheric composition and structure of Venus, there are many key questions which remain unanswered. The Pioneer Venus set of experiments is designed to provide information both individually and collectively to help understand and explain first of all the present state of the atmosphere (the composition and distribution in both the lower and upper parts, the state property profiles, the cloud compositions, the role of phase in the thermal structure, the planet's surface and interior composition, the high surface temperature, the stability of CO2, the ionosphere — its chemistry and thermal structure, the existence of superrotation, the response of the upper atmosphere to changes in solar EUV and the solar wind) and secondly the origin and evolution of the atmosphere. This paper discusses these questions and the degree to which the Pioneer Venus instruments will respond to them.

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Authors and Affiliations

  1. The University of Texas at Dallas, 75080, Richardson, Tex., USA

    J. H. Hoffman

  2. NASA Langley Research Center, 23665, Va., Hampton, USA

    G. M. Keating

  3. NASA Goddard Space Flight Center, 20771, Greenbelt, Md., USA

    H. Niemann

  4. NASA Ames Research Center, 94035, Mountain View, Calif., USA

    V. Oyama

  5. NASA Ames Research Center, 94035, Mountain View, Calif., USA

    J. Pollack

  6. NASA Ames Research Center, 94035, Mountain View, Calif., USA

    A. Seiff

  7. The University of Colorado, 80302, Boulder, Co., USA

    A. I. Stewart

  8. The University of Bonn, 5300, Bonn, Germany (FRG)

    U. Von Zahn

Authors
  1. J. H. Hoffman
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  2. G. M. Keating
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  3. H. Niemann
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  4. V. Oyama
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  5. J. Pollack
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  6. A. Seiff
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  7. A. I. Stewart
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  8. U. Von Zahn
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Hoffman, J.H., Keating, G.M., Niemann, H. et al. Composition and structure of the atmosphere of Venus. Space Sci Rev 20, 307–327 (1977). https://doi.org/10.1007/BF02186468

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