Series expansions for encounter-type solutions of Hill's problem
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Publication:4720810
DOI10.1007/BF01234287zbMath0613.70004OpenAlexW2066396263MaRDI QIDQ4720810
Publication date: 1986
Published in: Celestial Mechanics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/bf01234287
gravitational interactionimpact parameterHill problemasymptotic motionsSaturn's ringsmutual separations
Related Items (15)
On the Sitnikov problem ⋮ Encounter in the Keplerian field: Analytical treatment ⋮ Secular resonances between bodies on close orbits. II: Prograde and retrograde orbits for irregular satellites ⋮ A Hopf variables view on the libration points dynamics ⋮ Robust control of the Hill's problem with drag ⋮ Generalized Hill's problem: Lagrangian Hill's case ⋮ The circular restricted three-body problem in curvilinear coordinates ⋮ Influence of a hyperbolic flyby of a small mass on the orbital evolution of a massive binary ⋮ Coupling between corotation and Lindblad resonances in the presence of secular precession rates ⋮ Elliptical Hill's problem (large and small impact parameters) ⋮ The generalized Hill problem. Case of an external field of force deriving from a central potential ⋮ Secular resonances between bodies on close orbits: a case study of the Himalia prograde group of Jovian irregular satellites ⋮ Shannon entropy applied to the planar restricted three-body problem ⋮ Formation of the extreme Kuiper-Belt binary \(2001 \text{QW}_{322}\) through adiabatic switching of orbital elements ⋮ The problem of close approach of two small masses in the field of massive oblate primary
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