Physics
Scientific paper
Jul 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..214..351b&link_type=abstract
Icarus, Volume 214, Issue 1, p. 351-355.
Physics
3
Scientific paper
Estimates of the moments of inertia of Titan, as separately deduced from its gravitational field and spin pole orientation, are quite different. This discrepancy can be resolved if Titan is either not precessing as a rigid body (e.g. if the shell is decoupled from the interior by an ocean), or if the spin pole is not fully damped (e.g. due to atmospheric excitation). By the end of the Cassini mission, continued monitoring of the changing spin pole orientation, by Cassini radar observations, will determine which effect dominates.
Bills Bruce G.
Nimmo Francis
No associations
LandOfFree
Rotational dynamics and internal structure of Titan does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Rotational dynamics and internal structure of Titan, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotational dynamics and internal structure of Titan will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-995946