The eleventh motion constant of the two-body problem

被引:0
|
作者
Andrew J. Sinclair
John E. Hurtado
机构
[1] Auburn University,Aerospace Engineering Department
[2] Texas A&M University,Aerospace Engineering Department
来源
Celestial Mechanics and Dynamical Astronomy | 2011年 / 110卷
关键词
Two-body problem; Motion constants; Boundary-value problems;
D O I
暂无
中图分类号
学科分类号
摘要
The two-body problem is a twelfth-order time-invariant dynamic system, and therefore has eleven mutually-independent time-independent integrals, here referred to as motion constants. Some of these motion constants are related to the ten mutually-independent algebraic integrals of the n-body problem, whereas some are particular to the two-body problem. The problem can be decomposed into mass-center and relative-motion subsystems, each being sixth-order and each having five mutually-independent motion constants. This paper presents solutions for the eleventh motion constant, which relates the behavior of the two subsystems. The complete set of mutually-independent motion constants describes the shape of the state-space trajectories. The use of the eleventh motion constant is demonstrated in computing a solution to a two-point boundary-value problem.
引用
收藏
页码:189 / 198
页数:9
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