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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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发表于 2025-3-21 18:45:41 | 显示全部楼层 |阅读模式
书目名称Orbital Dynamics in the Gravitational Field of Small Bodies
编辑Yang Yu
视频video
概述Nominated as an outstanding PhD thesis by the Tsinghua University in 2014.Introduces qualitative methods of nonlinear dynamics into the study of orbits around solar system small bodies (SSSBs) with hi
丛书名称Springer Theses
图书封面Titlebook: Orbital Dynamics in the Gravitational Field of Small Bodies;  Yang Yu Book 2016 Springer-Verlag Berlin Heidelberg 2016 Solar System Small B
描述.This prizewinning PhD thesis presents a general discussion of the orbital motion close to solar system small bodies (SSSBs), which induce non-central asymmetric gravitational fields in their neighborhoods. It introduces the methods of qualitative theory in nonlinear dynamics to the study of local/global behaviors around SSSBs. Detailed mechanical models are employed throughout this dissertation, and specific numeric techniques are developed to compensate for the difficulties of directly analyzing. Applying this method, several target 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. .
出版日期Book 2016
关键词Solar System Small Bodies; Orbital Motion around Asteroids; Orbital Stability and Dynamical behavior; E
版次1
doihttps://doi.org/10.1007/978-3-662-52693-4
isbn_softcover978-3-662-57070-8
isbn_ebook978-3-662-52693-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer-Verlag Berlin Heidelberg 2016
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发表于 2025-3-21 21:54:23 | 显示全部楼层
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
发表于 2025-3-22 06:43:32 | 显示全部楼层
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
发表于 2025-3-22 11:41:08 | 显示全部楼层
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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