Titlebook: Orbital Dynamics in the Gravitational Field of Small Bodies; Yang Yu Book 2016 Springer-Verlag Berlin Heidelberg 2016 Solar System Small B

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Modelling Orbital Dynamics in the Potential of Small Bodies,rbital equations in the gravitational field of a small body. The basic form of the equation is first presented with the potential described by a homogenous polyhedron, and several transformations are listed to identify the general properties of this kind of systems, which is taken as the beginning t

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Stability of Equilibrium Points and Behaviour of Nearby Trajectories, equilibrium points of the target body, and presents the geometry and topology of the contour surfaces of efficient potential .. Sections?. and . use the linearized theory to determine the stability and type of an equilibrium point, and reveal the orbital motion on local invariant manifolds. Based o

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Topological Classification and Stability of Large-Scale Periodic Orbits,odic orbits around irregular bodies, which is then applied to find out the periodic orbital families of the target small body. Section?. surveys the stabilities of these orbits, and Sect.?. further describes the topologies of different orbital families, based on which a classification method is prop

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Orbital Resonance Near the Equatorial Plane of Small Bodies,hedral gravity model continues to be adopted to approximate the irregular field configuration. Section?. starts with an analysis on the variation of orbital energy, showing the mechanical essence of 1:1 resonance near the small bodies. Section?. surveys the parameter dependence of the resonant orbit

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2190-5053 systems, like asteroid 216 Kleopatra, are explored in great detail, and the results prove to be both revealing and pervasive for a large group of SSSBs.?.978-3-662-57070-8978-3-662-52693-4Series ISSN 2190-5053 Series E-ISSN 2190-5061

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