The atmospheres of Jupiter, Saturn, Neptune and Uranus, and Titan are characterized chemically in a review of recent observational and theoretical investigations. Compositions are indicated in tables, and special emphasis is given to the formation of HCN on Jupiter, the differentiation of polar and equatorial zones in the Jovian atmosphere, the mechanisms responsible for the color of the Great Red Spot, and the possible origin of the N2-dominated atmosphere of Titan.


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    Titel :

    Chemical evolution on the giant planets and Titan


    Beteiligte:
    Caldwell, J. (Autor:in) / Owen, T. (Autor:in)

    Erschienen in:

    Erscheinungsdatum :

    01.01.1984



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


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    Formation of Gas Giant Planets

    Lissauer, Jack / D'Angelo, Gennaro | AIAA | 2006


    The Evolution of the Titan Rocket-Titan I to Titan II

    Adams, L. J. / International Astronautical Federation / International Academy of Astronautics | British Library Conference Proceedings | 1997