Evolution of a "Class Two" Family of Periodic Orbits in the General Planar Problem of Three Bodies

Details Evolution of a "Class Two" Family of Periodic Orbits in the General Planar Problem of Three Bodies Evolution of a "Class Two" Family of Periodic Orbits in the General Planar Problem of Three Bodies

Aug 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973cemec...8...11s&link_type=abstract

Celestial Mechanics, Volume 8, Issue 1, pp.11-23

Physics

7

Scientific paper

The elliptic restricted problem of three bodies with unit eccentricity of the primaries is used to generate a family of periodic orbits in the general problem of three bodies. The parameter of the family is the mass of one of the participating bodies. This varies from zero to a termination value. The mass ratio of the primaries of the unperturbed problem (three to five) is maintained throughout the generation of the family. In this way an asymmetry is introduced generalizing the Copenhagen elliptic problem as the generating model. All members of the family experience a close approach and a collision between the primaries during half of the period of the orbit, therefore, the family is classified as ‘Class Two’.

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