Tidal Response of Titan's Interior Models Consistent with Cassini-Derived Constraints

Details Tidal Response of Titan's Interior Models Consistent with Cassini-Derived Constraints Tidal Response of Titan's Interior Models Consistent with Cassini-Derived Constraints

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1707c&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1707

Physics

Scientific paper

The goal of this paper is to identify to what extent tidal Love number
and dissipation factor data can help distinguish between the models
proposed so far to explain Titan's moment of inertia derived from
Cassini Radio Science observations.

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