Definition
Cryovolcanism is a volcanic phenomenon that occurs in environments with extremely low temperature. 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 Io, Jupiter’s innermost Galilean satellite, and on Enceladus, one of Saturn’s satellites. Traces of cryovolcanism are also found on Titan and Triton. Apart from Io’s volcanoes from which sulfur dioxide (SO2) is outgassed, cryovolcanism generally erupts water (H2O), methane (CH4), and ammonia (NH3). Cryovolcanism could also be present on other outer satellites and trans-Neptunian objects.
See Also
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2014 Springer-Verlag Berlin Heidelberg
About this entry
Cite this entry
Encrenaz, T. (2014). Cryovolcanism. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_372-2
Download citation
DOI: https://doi.org/10.1007/978-3-642-27833-4_372-2
Received:
Accepted:
Published:
Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics
Publish with us
Chapter history
-
Latest
Cryovolcanism- Published:
- 21 July 2019
DOI: https://doi.org/10.1007/978-3-642-27833-4_372-3
-
Original
Cryovolcanism- Published:
- 30 April 2015
DOI: https://doi.org/10.1007/978-3-642-27833-4_372-2