Abstract
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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Papadakis, K.E. Families of periodic orbits in the photogravitational three-body problem. Astrophys Space Sci 245, 1–13 (1996). https://doi.org/10.1007/BF00637799
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DOI: https://doi.org/10.1007/BF00637799