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A numerical investigation of the one-dimensional Newtonian three-body problem

III. Mass Dependence in the Stability of Motion

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Abstract

The one-dimensional Newtonian three-body problem is known to have stable (quasi-)periodic orbits when the masses are equal. The existence and size of the stable region is discussed here in the case where the three masses are arbitrary. We consider only the stability of the periodic (generalized) Schubart's (1956) orbit. If this orbit is linearly stable it is almost always surrounded by a region of stable quasi-periodic orbits and the size and shape of this stable region depends on the masses. The three-dimensional linear stability of the periodic orbits is also determined. Final results show that the region of stability has a complicated shape and some of the stable regions in the mass-plane are quite narrow. The non-linear three-dimensional stability is studied independently by extensive numerical integrations and the results are found to be in agreement with the linear stability analysis. The boundaries of stable region in the mass-plane are given in terms of polynomial approximations. The results are compared with a similar work by Héenon (1977).

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References

  • Aarseth, S.J. and Zare, K.: 1974, Cel. Mech. 10, 185–205

    Google Scholar 

  • Arnold, V.I.: 1989, Mathematical Methods of Classical Mechanics, second edition, Springer-Verlag, New York

    Google Scholar 

  • Bulirsch, R. and Stoer, J.: 1966, Nun. Math. 8, 1–13

    Google Scholar 

  • Hénon, M.: 1976, Cel. Mech. 13, 267–285

    Google Scholar 

  • Hénon, M.: 1977, Cel. Mech. 15, 243–261

    Google Scholar 

  • Hénon, M.: 1983, in Iooss, G., Helleman, R.H.G. and Stora, R., ed(s)., Chaotic Behaviour of Deterministic Systems, Elsevier, Amsterdam, 53–170

    Google Scholar 

  • Herrick, S.: 1972, Astrodynamics, VoIII, Van Nostrand Reinhold, London, 79–124

    Google Scholar 

  • Marchal, C.: 1988, in M.J. Valtonen, ed(s)., The Few Body Problem, Kluwer, Dordrecht, 5–25

    Google Scholar 

  • McGehee, R.: 1974, Inventiones math. 27, 191–227

    Google Scholar 

  • Mikkola, S. and Hietarinta, J.: 1989, Cel. Mech. 46, 1–18

    Google Scholar 

  • Mikkola, S. and Hietarinta, J.: 1990, Cel. Mech. 47, 321–331

    Google Scholar 

  • Press, W.H., Flannery, B.P., Teukolsky, G.A. and Vetterling, W.T.: 1986, Numerical Recipes, Cambridge University Press, 563–568

  • Schubart, J.: 1956, Astron. Nachr. 283, 17–22

    Google Scholar 

  • Whittaker, E.T.: 1937, Analytical Dynamics of Particles and Rigid Bodies, fourth edition, Cambridge University Press

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Mikkola, S., Hietarinta, J. A numerical investigation of the one-dimensional Newtonian three-body problem. Celestial Mech Dyn Astr 51, 379–394 (1991). https://doi.org/10.1007/BF00052929

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  • DOI: https://doi.org/10.1007/BF00052929

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