Secular Resonances in Nonrestricted Hierarchical Triple Systems

被引:6
|
作者
Tan, Pan [1 ,3 ,4 ]
Hou, Xiyun [1 ,3 ,4 ]
Liao, Xinhao [2 ,3 ]
Wang, Wenlei [2 ]
Tang, Jingshi [1 ,3 ,4 ]
机构
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
[2] Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
[3] Nanjing Univ, Inst Space Environm & Astrodynam, Nanjing 210023, Peoples R China
[4] Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210023, Peoples R China
来源
ASTRONOMICAL JOURNAL | 2020年 / 160卷 / 03期
基金
中国国家自然科学基金;
关键词
Orbital resonances; Three-body problem; Exoplanet dynamics; Celestial mechanics; EVOLUTION; PERTURBATIONS; REDUCTIONS; SATELLITES; PLANETS; ORBITS;
D O I
10.3847/1538-3881/aba89c
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, the averaged Hamiltonian of a nonrestricted hierarchical triple system truncated at the third order is investigated. First, each secular resonant term is studied. For the well-studied secular quadrupole theory, it is analytically reformulated in a different manner in our work. The resonance width is numerically determined and displayed on the root 1 - e(1)(2) - root 1 - e(2)(2) plane (also denoted as the (e) over tilde (1) - (e) over tilde (2) plane). In terms of the octupole terms, we show that for a near-planar configuration of the system, considerable variations of both the eccentricities of the inner and outer orbits can be generated by a single resonant term. The resonance width for every secular resonant angle from the octupole terms is also numerically determined and displayed on the (e) over tilde (1) - (e) over tilde (2) plane. The results show that an orbit flip with a near-perpendicular initial mutual inclination is possible for each secular resonance. By displaying the resonance widths of different resonant terms on the same (e) over tilde (1) - (e) over tilde (2) plane, we intuitively show the overlap of different secular resonances. Then, the full averaged Hamiltonian with both quadrupole and octupole terms is investigated using the Poincare surface of section, with a special focus on the orbit flip. For the cases we exploited, we find that the near-planar flip of the inner orbit can be either regular or chaotic while the outer orbit flip is generally chaotic.
引用
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页数:21
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