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 ω_{1} = 2ω_{2} and ω_{1} = 3ω_{2}. The motion is unstable for all the values of parameters q and A when ω_{1} = 2ω_{2} and the motion is unstable and stable depending upon the values of the parameters q and A when ω_{1} = 3ω_{2}. 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