On the stability of the triangular libration points for the photogravitational circular restricted problem of three bodies when both of the attracting bodies are radiating as well

Details On the stability of the triangular libration points for the photogravitational circular restricted problem of three bodies when both of the attracting bodies are radiating as well On the stability of the triangular libration points for the photogravitational circular restricted problem of three bodies when both of the attracting bodies are radiating as well

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cemec..40..155k&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 40, no. 2, 1987, p. 155-170.

Physics

14

Dynamic Stability, Gravitational Effects, Libration, Orbit Perturbation, Three Body Problem, Equations Of Motion, Lagrangian Equilibrium Points, Numerical Stability, Orbital Resonances (Celestial Mechanics)

Scientific paper

The stability of triangular libration points when both the attracting
bodies are radiating as well has been investigated under the
non-resonance cases. It is found that except for some cases for all
values of the radiation reduction factors and for all values of μ
< 0.0285954..., the motion will be stable.

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