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Celestial Mechanics and Dynamical Astronomy

, Volume 49, Issue 2, pp 133–144 | Cite as

Encounter in the keplerian field: Analytical treatment

  • V. A. Brumberg
  • T. V. Ivanova
Article

Abstract

In extending the results of Henon and Petit (1986) an algorithm is suggested for constructing the series representing the general encounter-type solution of the spatial eccentric Hill's problem. The series are arranged in powers of the eccentricity E of Hill's problem and two integration constants e and k characterizing eccentricity and inclination of the relative motion. A particular non-periodic solution of Henon and Petit corresponding to E = e = k = 0 is taken as an intermediary. The perturbations to this solution are constructed similar to the lunar theory of Hill and Brown.

Keywords

Relative Motion Integration Constant Analytical Treatment Lunar Theory Keplerian Field 
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References

  1. Brumberg, V. A.: 1961, Astron. J. USSR, 38, 738.Google Scholar
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Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • V. A. Brumberg
    • 1
  • T. V. Ivanova
    • 1
  1. 1.Institute of Applied AstronomyLeningradU.S.S.R.

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