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Stability of the Galilean Satellites in Deep Orbital ResonanceThe Galilean satellites are locked in the Laplace resonance, which is responsible for forcing their significant orbital eccentricites. The eccentricites in turn result in tidal energy dissipation within the satellites that is responsible for the great thermal activity on Io, including both volcanism observed by Voyager and heat flux measured from Earth. The resonance results from the nearly 2:1 commensurability of orbital periods (or equivalently of mean motions) taken by pairs. These geometrical relations enhance the mutual gravitational effects. Yoder pointed out that tides raised on Io tend to drive the system out of resonance (toward greater nu and correspondingly smaller eccentricities) while tides raised on Jupiter tend to drive the system towards deeper resonance (smaller nu and larger forced eccentricities). The possible behavior of the system in deep resonance is investigated.
Document ID
Acquisition Source
Legacy CDMS
Document Type
Contribution to a larger work
Richard Greenburg
(Planetary Science Institute Tucson, Arizona, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Reports of Planetary Geology and Geophysics Program - 1984
Publisher: National Aeronautics and Space Administration
Volume: NASA-TM-87563
Issue Publication Date: January 1, 1985
Subject Category
Lunar And Planetary Exploration
Accession Number
Distribution Limits
Use by or on behalf of the US Gov. Permitted.
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