NASA NTRS · 20060035105
Tides in Titan
Abstract
Tides raised in Titan by Saturn give rise to a static and a periodic deformation; both will be measured with Doppler tracking during the CASSINI Tour of the Saturnian System. The latter deformation is due to the significant eccentricity of Titan's orbit and has a frequency equal to the orbital angular velocity of Titan.
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Rappaport, Nicole J.. 1997-04-21. Tides in Titan. https://ntrs.nasa.gov/citations/20060035105
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