Photogravitationally Restricted Three-Body Problem and Coplanar Libration Point
ZHENG Xuetang, YU Lizhong
Department of Applied Physics, East China Institute of Technology, Nanjing 210014
Photogravitationally Restricted Three-Body Problem and Coplanar Libration Point
ZHENG Xuetang;YU Lizhong
Department of Applied Physics, East China Institute of Technology, Nanjing 210014
关键词 ：
96.50.Gn ,
97.80.-d
Abstract ： The photogravitationally restricted three-body problem in which the mass reduction factors of two primaries q1 , q2 ∈ (-∞,1] is studied and the calculating formula of the location of coplanar libration points is given in this paper. As an application, the motion of cometary dust in the solar system and dust grain in binary AR Cas is also discussed.
Key words ：
96.50.Gn
97.80.-d
出版日期: 1993-01-01
引用本文:
ZHENG Xuetang;YU Lizhong. Photogravitationally Restricted Three-Body Problem and Coplanar Libration Point[J]. 中国物理快报, 1993, 10(1): 61-64.
链接本文:
https://cpl.iphy.ac.cn/CN/
或
https://cpl.iphy.ac.cn/CN/Y1993/V10/I1/61
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[2]
SHI Zhi-dong;LI Zhong-yuan;CHEN Yao. Disruption of Charged Dust Grains in Cometary Plasma Environments
[3]
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[4]
QIN Bo;WU Xiang-ping;ZOU Zhen-long. Self-Microlensing in Compact Binary Systems
[5]
YU Li-zhong;ZHENG Xue-tang. Influence of Mass-Loss on the Orbit of Comet Shoemaker-Levy 9
1993, Vol. 10 
