Tidal Loading On Titan

Details Tidal Loading On Titan Tidal Loading On Titan

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufm.p53a1449k&link_type=abstract

American Geophysical Union, Fall Meeting 2004, abstract #P53A-1449

Physics

5417 Gravitational Fields (1227), 5430 Interiors (8147), 5450 Orbital And Rotational Dynamics, 6280 Saturnian Satellites

Scientific paper

The tidal response of Titan as a function of interior structure modeling is revised. The Love numbers of the solid body are estimated assuming thermal and mechanical equilibrium. Atmospheric tides are also taken into account. The influence of Saturn's gravitational tide on the atmosphere cause significant surface pressure oscillations as predicted from analytical as well as numerical models. The results are discussed with respect to expected Cassini-Huygens measurements.

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