Definition
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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© 2019 Springer-Verlag GmbH Germany, part of Springer Nature
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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
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Online ISBN: 978-3-642-27833-4
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Cryovolcanism- Published:
- 21 July 2019
DOI: https://doi.org/10.1007/978-3-642-27833-4_372-3
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Cryovolcanism- Published:
- 30 April 2015
DOI: https://doi.org/10.1007/978-3-642-27833-4_372-2