Non-symmetric doubly-asymptotic orbits at the outer collinear equilibrium pointL3
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In the framework of the solar system case (with only the larger primary radiating) of the photogravitational restricted three-body problem we compute and present some non-symmetric asymptotic orbits connecting the outer collinear equilibrium pointL3 with the neighbourhood of one of the triangular equilibrium pointsL4, 5. Such orbits have not been found previously in the restricted problem.
KeywordsSolar System Primary Radiate System Case Restricted Problem Asymptotic Orbit
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