Non-symmetric doubly-asymptotic orbits at the outer collinear equilibrium point L3

Details Non-symmetric doubly-asymptotic orbits at the outer collinear equilibrium point L3 Non-symmetric doubly-asymptotic orbits at the outer collinear equilibrium point L3

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.199..185p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 199, no. 2, p. 185-188.

Astronomy and Astrophysics

Astrophysics

4

Asymptotic Properties, Lagrangian Equilibrium Points, Orbital Mechanics, Solar System, Three Body Problem, Equations Of Motion, Gravitational Effects

Scientific paper

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 nonsymmetric asymptotic orbits connecting the outer collinear equilibrium point L3 with the neighborhood of one of the triangular equilibrium points L4.5. Such orbits have not been found previously in the restricted problem.

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