On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary

Joint Authors

Singh, Jagadish
Bello, Nakone

Source

Advances in Astronomy

Issue

Vol. 2015, Issue 2015 (31 Dec. 2015), pp.1-12, 12 p.

Publisher

Hindawi Publishing Corporation

Publication Date

2015-08-25

Country of Publication

Egypt

No. of Pages

12

Main Subjects

Astronomy

Abstract EN

We consider a version of the relativistic restricted three-body problem (R3BP) which includes the effects of oblateness of the secondary and radiation of the primary.

We determine the positions and analyze the stability of the triangular points.

We find that these positions are affected by relativistic, oblateness, and radiation factors.

It is also seen that both oblateness of the secondary and radiation of the primary reduce the size of stability region.

Further, a numerical exploration computing the positions of the triangular points and the critical mass ratio of some binaries systems consisting of the Sun and its planets is given in the tables.

American Psychological Association (APA)

Bello, Nakone& Singh, Jagadish. 2015. On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary. Advances in Astronomy،Vol. 2015, no. 2015, pp.1-12.
https://search.emarefa.net/detail/BIM-1051972

Modern Language Association (MLA)

Bello, Nakone& Singh, Jagadish. On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary. Advances in Astronomy No. 2015 (2015), pp.1-12.
https://search.emarefa.net/detail/BIM-1051972

American Medical Association (AMA)

Bello, Nakone& Singh, Jagadish. On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary. Advances in Astronomy. 2015. Vol. 2015, no. 2015, pp.1-12.
https://search.emarefa.net/detail/BIM-1051972

Data Type

Journal Articles

Language

English

Notes

Includes bibliographical references

Record ID

BIM-1051972