Characteristics exponents of the triangular solution in the elliptical restricted three-body problem under radiating and triaxial primaries
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2017-02-01 
https://doi.org/10.14419/ijaa.v5i1.7114
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ER3BP, Dynamical System Libration Points, Flouqet Theory. -
Abstract
This Paper deals with the effects of the radiation pressure and triaxiality of primaries on the stability of infinitesimal motion about triangular equilibrium points [ , ] in the elliptical restricted three body problem (ER3EB) around binary system. For determining the characteristic exponents of variational equations with periodic coefficient, we have used analytical method, described by Bennet in [3, 4]. This analytical method is based on Floquet’s theory. The stability of equilibrium points has been discussed under the assumption thatboth the primaries are radiating and triaxial. For this we have drawn transition cureves in μ-e plane. And it is seen that system is stable outside the transition curves, while system is Unstable within the transition curves.
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How to Cite
Narayan, A., Pandey, K. K., & Shrivastava, S. K. (2017). Characteristics exponents of the triangular solution in the elliptical restricted three-body problem under radiating and triaxial primaries. International Journal of Advanced Astronomy, 5(1), 12-18. https://doi.org/10.14419/ijaa.v5i1.7114Received date: 2016-12-16
Accepted date: 2017-01-11
Published date: 2017-02-01