Celestial mechanics

, Volume 1, Issue 3–4, pp 343–346 | Cite as

On oscillatory motion in the problem of three bodies

  • Donald G. Saari
Article

Abstract

In the case of oscillatory motion in the problem of three bodies it is shown that ast→∞ the mutual distances between particles cannot separate faster thanCt2/3 whereC is some positive constant. As bounding functions of time exist for the other classifications of motion in the three body problem, it follows in general that the mutual distances between particles is 0(t) ast→∞.

Keywords

Positive Constant Body Problem Oscillatory Motion Mutual Distance 
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References

  1. Chazy, J.: 1922,Ann. Sci. École Norm. 39, 1–130.Google Scholar
  2. Pollard, H.: 1966,Mathematical Introduction to Celestial Mechanics, Prentice-Hall, New York.Google Scholar

Copyright information

© D. Reidel Publishing Company 1970

Authors and Affiliations

  • Donald G. Saari
    • 1
  1. 1.Dept. of MathematicsNorthwestern UniversityEvanstonU.S.A.

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