Multiple Components in Narrow Planetary Rings

dc.creatorBenet, L.
dc.creatorMerlo, O.
dc.date2007-02-19
dc.date2008-01-09
dc.date.accessioned2026-07-07T08:54:04Z
dc.date.available2026-07-07T08:54:04Z
dc.descriptionThe phase-space volume of regions of regular or trapped motion, for bounded or scattering systems with two degrees of freedom respectively, displays universal properties. In particular, drastic reductions in the volume (gaps) are observed at specific values of a control parameter. Using the stability resonances we show that they, and not the mean-motion resonances, account for the position of these gaps. For more degrees of freedom, exciting these resonances divides the regions of trapped motion. For planetary rings, we demonstrate that this mechanism yields rings with multiple components.
dc.description4 pages, 7 figures (some in colors)
dc.identifierhttps://arxiv.org/abs/nlin/0702039
dc.identifierhttp://arxiv.org/abs/nlin/0702039
dc.identifierPhys. Rev. Lett. Vol 100 (2008) 014102
dc.identifierdoi:10.1103/PhysRevLett.100.014102
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/145802
dc.subjectChaotic Dynamics
dc.subjectAstrophysics
dc.titleMultiple Components in Narrow Planetary Rings
dc.typetext

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