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Titlebook: Generating Families in the Restricted Three-Body Problem; Michel Hénon Book 1997 Springer-Verlag Berlin Heidelberg 1997 astronomy.bifurcat

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发表于 2025-3-21 18:49:54 | 显示全部楼层 |阅读模式
书目名称Generating Families in the Restricted Three-Body Problem
编辑Michel Hénon
视频video
概述The first classification of the orbit structure of a seemingly non-integrable system in every detail
丛书名称Lecture Notes in Physics Monographs
图书封面Titlebook: Generating Families in the Restricted Three-Body Problem;  Michel Hénon Book 1997 Springer-Verlag Berlin Heidelberg 1997 astronomy.bifurcat
描述The classical restricted problem of three bodies is of fundamental importance for its applications to astronomy and space navigation, and also as a simple model of a non-integrable Hamiltonian dynamical system. A central role is played by periodic orbits, of which a large number have been computed numerically. In this book an attempt is made to explain and organize this material through a systematic study of generating families, which are the limits of families of periodic orbits when the mass ratio of the two main bodies becomes vanishingly small. The most critical part is the study of bifurcations, where several families come together and it is necessary to determine how individual branches are joined. Many different cases must be distinguished and studied separately. Detailed recipes are given. Their use is illustrated by determining a number of generating families, associated with natural families of the restricted problem, and comparing them with numerical computations in the Earth-Moon and Sun-Jupiter case.
出版日期Book 1997
关键词astronomy; bifurcation; dynamical systems; three-body problem
版次1
doihttps://doi.org/10.1007/3-540-69650-4
isbn_softcover978-3-662-14156-4
isbn_ebook978-3-540-69650-6Series ISSN 0940-7677
issn_series 0940-7677
copyrightSpringer-Verlag Berlin Heidelberg 1997
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Administration of Contrast Media,t is periodic, it has an infinity of collisions. (Note that there can be more than one collision per period.) The collisions separate the orbit into pieces, which we call .. Two consecutive arcs join at a collision; their tangents at the collision form an angle, generally different from zero. This angle, measured in rotating axes, will be called .
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Generating Orbits of the Second Species,t is periodic, it has an infinity of collisions. (Note that there can be more than one collision per period.) The collisions separate the orbit into pieces, which we call .. Two consecutive arcs join at a collision; their tangents at the collision form an angle, generally different from zero. This angle, measured in rotating axes, will be called .
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https://doi.org/10.1007/3-540-69650-4astronomy; bifurcation; dynamical systems; three-body problem
发表于 2025-3-22 14:06:55 | 显示全部楼层
Michel HénonThe first classification of the orbit structure of a seemingly non-integrable system in every detail
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Further Development of Contrast Media,We use the following more or less standard notations for some special functions:
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Contrast-Enhanced Digital Mammography (CEDM)We have now finished the inventory of generating orbits. Our next task is to find the ., which will play a fundamental role as explained in the Introduction.
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