A model of the internal structure of Titan: first results

Details A model of the internal structure of Titan: first results A model of the internal structure of Titan: first results

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..731..288p&link_type=abstract

EQUATION-OF-STATE AND PHASE-TRANSITION ISSUES IN MODELS OF ORDINARY ASTROPHYSICAL MATTER. AIP Conference Proceedings, Volume 73

Astronomy and Astrophysics

Astrophysics

Saturn

Scientific paper

The aim of this short contribution is to report some preliminary results on a theoretical model of the internal structure of Titan, the satellite of Saturn. All the calculations were performed within the SK theory of dense matter. The central pressure and temperature, as well as a possible chemical composition of this satellite have been determined, but they will ultimately become verifiable only by data from the Cassini mission.

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