How Does Titan Retain a Finite Orbital Eccentricity?

Details How Does Titan Retain a Finite Orbital Eccentricity? How Does Titan Retain a Finite Orbital Eccentricity?

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1341b&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1341

Physics

Scientific paper

The present orbital eccentricity of Titan places an upper bound on tidal
dissipation within a hydrocarbon ocean, unless an appropriate excitation
mechanism is identified. Orbital perturbations from a Jupiter-Saturn
near resonance appear adequate.

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