Mutual potential between two rigid bodies with arbitrary shapes and mass distributions

被引:58
|
作者
Hou, Xiyun [1 ]
Scheeres, Daniel J. [2 ]
Xin, Xiaosheng [1 ]
机构
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Jiangsu, Peoples R China
[2] Univ Colorado, Dept Aerosp Engn Sci, Boulder, CO 80309 USA
来源
基金
中国国家自然科学基金;
关键词
Full two rigid body problem; Binary systems; Spin-orbit coupling; Numerical simulations; Stability; BINARY ASTEROID SYSTEMS; FULL 2-BODY PROBLEM; BODY PROBLEM; CELESTIAL MECHANICS; ROTATIONAL FISSION; POWER-SERIES; SOLID BODIES; 1999; KW4; DYNAMICS; SIMULATION;
D O I
10.1007/s10569-016-9731-y
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Formulae to compute the mutual potential, force, and torque between two rigid bodies are given. These formulae are expressed in Cartesian coordinates using inertia integrals. They are valid for rigid bodies with arbitrary shapes and mass distributions. By using recursive relations, these formulae can be easily implemented on computers. Comparisons with previous studies show their superiority in computation speed. Using the algorithm as a tool, the planar problem of two ellipsoids is studied. Generally, potential truncated at the second order is good enough for a qualitative description of the mutual dynamics. However, for ellipsoids with very large non-spherical terms, higher order terms of the potential should be considered, at the cost of a higher computational cost. Explicit formulae of the potential truncated to the fourth order are given.
引用
收藏
页码:369 / 395
页数:27
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