Capture in the circular and elliptic restricted three-body problem

被引：31
|
作者：
Makó, Z [1 ]
Szenkovits, F [1 ]
机构：
[1] Univ Babes Bolyai, Fac Math & Informat, R-3400 Cluj Napoca, Romania
来源：
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY | 2004年 / 90卷 / 1-2期
关键词：
asteroid; capture; elliptic restricted three-body problem; Hill-region;
D O I：
10.1007/s10569-004-5899-7
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper the authors provide a study of the phenomenon of the gravitational capture by using the models of the circular and elliptic restricted three-body problem. In the first part the inadequacy of the circular restricted three-body problem in the study of the phenomenon of the capture in the case of NEAs is shown. In the model of the spatial elliptic restricted three-body problem criteria of the capture are deduced by using the pulsating Hill-regions.
引用
收藏
页码：51 / 58
页数：8
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