Stability of the Triangular Libration Points of the Circular Restricted Problem in the Presence of Resonances

Details Stability of the Triangular Libration Points of the Circular Restricted Problem in the Presence of Resonances Stability of the Triangular Libration Points of the Circular Restricted Problem in the Presence of Resonances

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cemda..66..191t&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, Volume 66, Issue 2, pp.191-202

Astronomy and Astrophysics

Astronomy

2

Resonance, Restricted Problem, Stability

Scientific paper

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.

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