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Journal of Dynamical Systems and Geometric Theories

(Since 2002)
Open Access ·Peer-reviewed·ISSN (Online): 2169-0057·ISSN (Print): 1726-037X

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Journal of Dynamical Systems and Geometric Theories
Open Access Article

Effects of Poynting-Robertson (P-R) drag, radiation, and oblateness on motion around the L4,5 equilibrium points in the CR3BP

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pp. 177–200Vol. 15Issue 2July 2017DOI: 10.1080/1726037X.2017.1411043XML
Received:
30 Sep 2017
Accepted:
14 Nov 2017
Published Online:
06 Dec 2017
Article type:
Article
Language:
EN
Article no.:
1726037X.2017.1411043
Pages:
177–200

Abstract

The research paper under consideration investigates the motion in the vicinity of triangular equilibrium points of the circular restricted three-body problem of a passively gravitating dust particle in the gravitational field for the binaries system (Kruger 60 and Achird). The two bodies of the binary are both oblate radiating stars possessing P-R drag. The position of triangular equilibrium points of the particle is seen to be affected by oblateness, radiation and P-R drag. In our numerical exploration of the binary system Kruger 60 and Achird, we computed the radiation factors q (i= 1,2) and the velocity of light c which is a component of the P-R drag. The points are unstable due to the presence of a positive real part of the complex roots.

Keywords

Celestial MechanicsOblatenessP-R dragR3BP

Subject Classifications

70F15

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