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A model of the internal structure of Titan: first results

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 determinded, but they will ultimately become verifiable only by data from the Cassini misision.

preprint2005arXivOpen access

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