Skip to main content

Rhea

  • Living reference work entry
  • First Online:
Encyclopedia of Astrobiology
  • 200 Accesses

Definition

Rhea, discovered by Giovanni Domenico Cassini in 1672, is the largest of the midsized icy satellites of Saturn. Its distance to Saturn is 527,000 km (or 8.7 Saturnian radii). Its diameter is 1,528 km and its density is 1.24 g/cm3, typical of a water-ice body. Rhea was first observed by Voyager 1 in 1980 and then more extensively explored since 2005 by the Cassini orbiter. The surface of Rhea is heavily cratered with little differentiation, with the exception of Izanagi crater, which is 250 km in diameter. Rhea has no orbital resonance with any other satellite, which accounts for the lack of tidal heating and hence of geological activity.

See Also

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Institutional subscriptions

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Therese Encrenaz .

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 2014 Springer-Verlag Berlin Heidelberg

About this entry

Cite this entry

Encrenaz, T. (2014). Rhea. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1369-3

Download citation

  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1369-3

  • 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

Policies and ethics