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• W2085689402 abstract "Ariel and Umbriel have passed through the 5:3 mean-motion commensurability if the specific dissipation function (Q) for Uranus is less than about 100,000. There is a significant chaotic zone associated with this resonance. Due to the presence of this chaotic zone, the standard theory describing passage through orbital resonances is not applicable. In particular, there are significant changes in the mechanism for and probability of capture into resonance. Tidal evolution within the chaotic zone may have driven orbital eccentricities to relatively high values, with some probability of escape from resonance remaining. In the planar approximation, eccentricities high enough to have a significant effect on the thermal history of Ariel have not been found." @default.
• W2085689402 created "2016-06-24" @default.
• W2085689402 creator A5017703136 @default.
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• W2085689402 date "1988-05-01" @default.
• W2085689402 modified "2023-09-25" @default.
• W2085689402 title "Tidal evolution of the Uranian satellites" @default.
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• W2085689402 doi "https://doi.org/10.1016/0019-1035(88)90038-3" @default.
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