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Cryovolcanism

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Encyclopedia of Astrobiology
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Cryovolcanism is a volcanic phenomenon that occurs in environments with extremely low temperatures. There, instead of molten silicates, cryovolcanoes erupt liquid water, methane, ammonia, or sulfur dioxide onto the icy surface of a planet or satellite. It has been observed on several satellites of the outer solar system. In particular, active cryovolcanism has been discovered at the surface of Jupiter’s Galilean satellite Europa and on Saturn’s satellites Enceladus and possibly Titan. Traces of cryovolcanism are also found on Triton and possibly Pluto. The ejection products of cryovolcanism include water (H2O), methane (CH4), ammonia (NH3), and dinitrogen (N2). Cryovolcanism could also be present on other outer satellites and trans-Neptunian objects.

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Correspondence to Therese Encrenaz .

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Encrenaz, T. (2019). Cryovolcanism. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_372-3

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_372-3

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-27833-4

  • Online ISBN: 978-3-642-27833-4

  • eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics

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Chapter history

  1. Latest

    Cryovolcanism
    Published:
    21 July 2019

    DOI: https://doi.org/10.1007/978-3-642-27833-4_372-3

  2. Original

    Cryovolcanism
    Published:
    30 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_372-2