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Astrophysics and Space Science

, Volume 194, Issue 2, pp 207–213 | Cite as

Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem, I

  • V. V. Markellos
  • E. Perdios
  • P. Labropoulou
Article

Abstract

The linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem is examined and the stability regions are determined in the space of the parameters of mass, eccentricity, and radiation pressure. It is found that radiation pressure of the larger body for solar system cases exerts only a small quantitative influence on the stability regions.

Keywords

Radiation Equilibrium Point Solar System Large Body Stability Region 
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. Bennett, A.: 1965,Icarus 4, 177.Google Scholar
  2. Danby, J. M. A.: 1964,Astron. J. 69, 165.Google Scholar
  3. Kumar, V. and Choudhry, R. K.: 1989,Celes. Mech. 46, 59.Google Scholar
  4. Meire, R.: 1981,Celes. Mech. 23, 89.Google Scholar
  5. Simmons, J. F. L., McDonald, A. J. C., and Brown, J. C.: 1985,Celes. Mech. 35, 145.Google Scholar
  6. Tschauner, J.: 1971,Celes. Mech. 3, 189.Google Scholar

Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • V. V. Markellos
    • 1
  • E. Perdios
    • 1
  • P. Labropoulou
    • 1
  1. 1.Department of Engineering Science, Division of Applied Mathematics and MechanicsUniversity of PatrasGreece

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