Stability of triangular libration points in the photogravitational three-body problem

Details Stability of triangular libration points in the photogravitational three-body problem Stability of triangular libration points in the photogravitational three-body problem

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..338p&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-010 8), vol. 13, April 1987, p. 338-344. In Russian. In Russian.

Statistics

Computation

1

Dynamic Stability, Gravitational Effects, Libration, Nonlinear Systems, Stellar Luminosity, Three Body Problem, Binary Stars, Computational Astrophysics, Molecular Clouds

Scientific paper

The stability of a three-parametric family of the relative equilibrium positions (the triangular libration points) of a gas-dust cloud particle in the field of a double star is investigated. The photogravitational restricted circular three-body problem is considered as a dynamical model in which unlike in the classical one both main bodies are luminous. It is shown that stability exists for the majority of the initial conditions and formal stability of the triangular libration points exists practically in the whole area of stability to a first approximation. The resonances of the third and the fourth order, that can disturb formal stability, are considered.

Affiliated with

Also associated with

No associations

Rating

Stability of triangular libration points in the photogravitational three-body problem does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Stability of triangular libration points in the photogravitational three-body problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of triangular libration points in the photogravitational three-body problem will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1349569