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Astrophysics and Space Science

, Volume 199, Issue 2, pp 185–188 | Cite as

Non-symmetric doubly-asymptotic orbits at the outer collinear equilibrium pointL3

  • E. Perdios
Article

Abstract

In the framework of the solar system case (with only the larger primary radiating) of the photogravitational restricted three-body problem we compute and present some non-symmetric asymptotic orbits connecting the outer collinear equilibrium pointL3 with the neighbourhood of one of the triangular equilibrium pointsL4, 5. Such orbits have not been found previously in the restricted problem.

Keywords

Solar System Primary Radiate System Case Restricted Problem Asymptotic Orbit 
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References

  1. Deprit, A. and Henrard, J.: 1965,Astron. J. 70, 271.Google Scholar
  2. Markellos, V. V.: 1992, in A. E. Roy (ed.),Predictability, Stability and Chaos in N-Body Dynamical Systems, Plenum Publ. Co., New York, p. 413.Google Scholar
  3. Perdios, E. and Markellos, V. V.: 1990,Astrophys. Space Sci. 166, 129.Google Scholar

Copyright information

© Kluwer Academic Publishers 1993

Authors and Affiliations

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

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