Stability of the Triangular Libration Points of the Circular Restricted Problem in the Presence of Resonances
Abstract
The stability of triangular libration points, when the bigger primary is a source of radiation and the smaller primary is an oblate spheroid. has been investigated in the resonance cases ω1 = 2ω2 and ω1 = 3ω2. The motion is unstable for all the values of parameters q and A when ω1 = 2ω2 and the motion is unstable and stable depending upon the values of the parameters q and A when ω1 = 3ω2. Here q is the radiation parameter and A is the oblateness parameter.
- Publication:
-
Celestial Mechanics and Dynamical Astronomy
- Pub Date:
- June 1996
- DOI:
- 10.1007/BF00054964
- Bibcode:
- 1996CeMDA..66..191T
- Keywords:
-
- resonance;
- restricted problem;
- stability