Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission

Details Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010icar..208..395t&link_type=abstract

Icarus, Volume 208, Issue 1, p. 395-401.

Physics

17

Scientific paper

The Cassini spacecraft has provided data on over twenty satellites orbiting Saturn. In this study we update the shape measurements derived from imaging data of nearly all the observed regular satellites (those with low eccentricities and inclinations) and briefly discuss some of the implications of their properties. In particular, the improved data show that Rhea’s shape is hydrostatic.

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