Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..314p&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 6, May 1980, p. 314-317.) Soviet Astronomy Letters, vol. 6, May-June 1980, p. 173-175.
Astronomy and Astrophysics
Astronomy
Dynamic Stability, Lagrangian Equilibrium Points, Radiation Pressure, Three Body Problem, Gravitational Effects, Hamiltonian Functions, Orbit Perturbation, Perturbation Theory, Solar System
Scientific paper
In the case where the mass of the radiating body (such as the sun) is much smaller than the mass of the other main gravitating body (such as the galactic nucleus), the triangular libration points in the plane photogravitational restricted circular three-body problem will be Liapunov-stable almost everywhere within the region in which the necessary stability conditions are satisfied. Instability will, however, occur on the curves corresponding to the inner third- and fourth-order resonances.
No associations
LandOfFree
Stability of the triangular libration points in the photogravitational restricted circular 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 the triangular libration points in the photogravitational restricted circular three-body problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability of the triangular libration points in the photogravitational restricted circular three-body problem will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1218081