Computation of halo orbits in the photogravitational Sun-Earth system with oblateness

被引：19

作者：

Tiwary, Rishikesh Dutta ^{[1
]}

Kushvah, Badam Singh ^{[1
]}

机构：

[1] Indian Sch Mines, Dept Appl Math, Dhanbad 826004, Bihar, India

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2015年 / 357卷 / 01期

关键词：

Restricted three body problem; Photogravitational; Oblateness; Lissajous orbits; Halo orbits; RESTRICTED 3-BODY PROBLEM; PERIODIC-ORBITS; INVARIANT-MANIFOLDS; EQUILIBRIUM POINTS; CONNECTING ORBITS; DESIGN; STABILITY;

D O I：

10.1007/s10509-015-2243-5

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

In this paper, we extend an existing approach to find the Lissajous and halo orbits around Lagrangian points L-1 and L-2 in the restricted three body problem with the Sun as a radiating source and the Earth as an oblate spheroid. We analyze the effects of radiation pressure and oblateness on the orbits around Libration points L-1 and L-2. A first guess of halo orbits is computed using Lindstedt-Poincare method upto fourth order approximation. Due to the effect of radiation pressure and oblateness the time period increases around L-1 and decreases around L-2.

引用

页码：1 / 16

页数：16

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