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Tides in TitanTides 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.
Document ID
20060035105
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
hdl:2014/21964
Authors
Rappaport, Nicole J.
Date Acquired
August 23, 2013
Publication Date
April 21, 1997
Distribution Limits
Public
Copyright
Other
Keywords
Tides Titan CASSINI Saturnian System

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