Numerical stability analysis around L(4) in the post-Newtonian restricted three-body problem

被引：4

作者：

Rosswog, S

Trautmann, D

机构：

[1] Department of Theoretical Physics, University of Basel, 4056 Basel

来源：

PLANETARY AND SPACE SCIENCE | 1996年 / 44卷 / 04期

关键词：

D O I：

10.1016/0032-0633(95)00125-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The post-Newtonian equation of motion of the restricted, circular three-body problem are integrated numerically. Using this integration the stable region around the triangular libration point L(4) for a relativistic system of mass ration earth-moon is calculated. The set of stable points is compared with the results of McKenzie and Szevehely found for the Newtonian case. The stable region shows a very complex structure which shows similarities to the one found in the Newtonion problem. Copyright (C) 1996 Elsevier Science Ltd.

引用

页码：313 / 316

页数：4

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