Families of Periodic Orbits in the Photogravitational Three-Body Problem

Details Families of Periodic Orbits in the Photogravitational Three-Body Problem Families of Periodic Orbits in the Photogravitational Three-Body Problem

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.245....1p&link_type=abstract

Astrophysics and Space Science, Volume 245, Issue 1, pp.1-13

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

All the families of planar symmetric simple-periodic orbits of the photogravitational restricted plane circular three-body problem, are determined numerically in the case when the primaries are of equal mass and radiate with equal radiation factors (q 1=q2=q). We obtain a global view of the possible patterns of periodic three-body motion while the full range of values of the common radiation factor is explored, from the gravitational case (q=1) down to near the critical value at which the triangular equilibria disappear by coalescing with the inner equilibrium pointL 1 on the rotating axis of the primaries. It is found that for large deviations of its value from the gravitational case the radiation factorq can have a strong effect on the structure of the families.

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