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Astrophysics and Space Science

, Volume 201, Issue 2, pp 281–285 | Cite as

Remarks on the photogravitational restricted three-body problem

  • Ioan Todoran
Article

Abstract

The effects of the radiation pressure in the restricted three-body problem are considered and the existence of the “out-of-plane” equilibrium points is analyzed. It is found that within the framework of the stellar stability, the five Lagrangian points are the only equilibrium points, at least as far as the force of the radiation pressure is taken into account.

Keywords

Radiation Equilibrium Point Radiation Pressure Lagrangian Point 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Kopal, Z.: 1978,Dynamics of the Close Binary Systems, D. Reidel Publ. Co., Dordrecht.Google Scholar
  2. Ragos, O. and Zagouras, C.: 1988,Cel. Mechanics 44, 135.Google Scholar

Copyright information

© Kluwer Academic Publishers 1993

Authors and Affiliations

  • Ioan Todoran
    • 1
  1. 1.Astronomical ObservatoryCluj-NapocaRomania

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