Abstract
Global stability regions are found for classi orbits of the circular restricted 3-body problem for primary masses equal and Jacobi constantK>15.5. As this constant decreases, the stability, region shrinks extremely rapidly.
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Mullins, L.D., Bartlett, J.H. Global stability and the restricted 3-body problem. Celestial Mechanics 7, 421–437 (1973). https://doi.org/10.1007/BF01227508
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DOI: https://doi.org/10.1007/BF01227508