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- W2007120132 abstract "Incomplete arc rings orbiting Neptune have been discovered from the ground, and have been recently observed by the Voyager spacecraft. We first review the possible models accounting for the stability of the three dense arc structures embedded in the faint 63,000 km ring (or “63K ring”). These different models are discussed both from a purely theoretical point of view, and in relation to observations of Neptune's ring system. Subsequently, we analyze other dynamical aspects of the Neptune ring system, including timescales for dynamical repulsion of the rings in the radial direction by nearby shepherding moons and the energy liberated by this process. We then attempt to assess what may be special about the dynamical environment of Neptune's 63K ring and how such an environment may be responsible for the unusual azimuthal structure observed in this ring." @default.
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- W2007120132 date "1992-11-01" @default.
- W2007120132 modified "2023-10-17" @default.
- W2007120132 title "Dynamical models of the arcs in Neptune's 63K ring (1989N1R)" @default.
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- W2007120132 doi "https://doi.org/10.1016/0273-1177(92)90425-w" @default.
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