Internal Structure of Enceladus and Dione from Orbital Constraints

Details Internal Structure of Enceladus and Dione from Orbital Constraints Internal Structure of Enceladus and Dione from Orbital Constraints

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2199z&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

Based on orbital constraints, we find that Enceladus is likely to have a
liquid ocean beneath its conductive ice shell. Dione probably has a
similar internal structure.

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