Caustics of the restricted three-body problem

被引：0

作者：

Santos, DE

Martins, RV

Winter, OC

Cordeiro, RR

机构：

[1] Observ Nacl, BR-20921400 Rio De Janeiro, Brazil

[2] UNESP, Grp Dinam Orbital & Planetol, BR-12500000 Sao Paulo, Brazil

[3] Univ Fed Vicosa, Dept Fis, BR-3657100 Vicosa, MG, Brazil

来源：

ASTRONOMY & ASTROPHYSICS | 1998年 / 331卷 / 03期

关键词：

celestial mechanics; stellar dynamics; chaos;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Trajectories of the planar, circular, restricted three-body problem are given in the configuration space through the caustics associated to the invariant tori of quasi-periodic orbits. It is shown that the caustics of trajectories librating in any particular resonance display some features associated to that resonance. This method can be considered complementary to the Poincare surface of section method, because it provides information not accessible by the other method.

引用

页码：1108 / 1112

页数：5

共 10 条

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