Analytical computation of bifurcation of orbits near collinear libration point in the restricted three-body problem

Mingpei Lin, Tong Luo, Hayato Chiba
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Abstract

A unified analytical solution is presented for constructing the phase space near collinear libration points in the Circular Restricted Three-body Problem (CRTBP), encompassing Lissajous orbits and quasihalo orbits, their invariant manifolds, as well as transit and non-transit orbits. Traditional methods could only derive separate analytical solutions for the invariant manifolds of Lissajous orbits and halo orbits, falling short for the invariant manifolds of quasihalo orbits. By introducing a coupling coefficient {\eta} and a bifurcation equation, a unified series solution for these orbits is systematically developed using a coupling-induced bifurcation mechanism and Lindstedt-Poincar\'e method. Analyzing the third-order bifurcation equation reveals bifurcation conditions for halo orbits, quasihalo orbits, and their invariant manifolds. Furthermore, new families of periodic orbits similar to halo orbits are discovered, and non-periodic/quasi-periodic orbits, such as transit orbits and non-transit orbits, are found to undergo bifurcations. When {\eta} = 0, the series solution describes Lissajous orbits and their invariant manifolds, transit, and non-transit orbits. As {\eta} varies from zero to non-zero values, the solution seamlessly transitions to describe quasihalo orbits and their invariant manifolds, as well as newly bifurcated transit and non-transit orbits. This unified analytical framework provides a more comprehensive understanding of the complex phase space structures near collinear libration points in the CRTBP.
受限三体问题中碰撞自由点附近轨道分岔的分析计算
本文提出了一种统一的解析解,用于构建环形受限三体问题(CRTBP)中的相空间邻接共线自由点,包括Lissajous轨道和准光环轨道、它们的不变流形以及过境轨道和非过境轨道。传统方法只能分别求出利萨如轨道和光环轨道的不变流形的解析解,而准光环轨道的不变流形的解析解则不尽人意。通过引入耦合系数{\eta}和分岔方程,利用耦合诱导分岔机制和Lindstedt-Poincar\'e方法,系统地建立了这些轨道的统一级数解。分析三阶分岔方程揭示了晕轨道、准晕轨道及其不变流形的分岔条件。此外,还发现了与光环轨道类似的新的周期轨道族,并发现了非周期性/准周期性轨道,如过境轨道和非过境轨道,也会发生分岔。当{\eta}=0时,数列解描述了利萨如轨道及其不变量、过境轨道和非过境轨道。当{eta}从零开始变化时,解无缝过渡到描述准全轨道及其不变流形,以及新分岔的过境轨道和非过境轨道。这种统一的分析框架使我们能够更全面地理解 CRTBP 中共轭天平点附近的复杂相空间结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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