Stability of planetary orbits in binary systems

Details Stability of planetary orbits in binary systems Stability of planetary orbits in binary systems

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cemec..22....7s&link_type=abstract

(Symposium on Star Catalogues, Positional Astronomy and Celestial Mechanics, Washington, D.C., Nov. 30, 1978.) Celestial Mechani

Astronomy and Astrophysics

Astronomy

38

Hill Method, Motion Stability, Planetary Orbits, Satellite Perturbation, Three Body Problem, Celestial Mechanics, Circular Orbits, Orbital Mechanics

Scientific paper

The possible existence of stable orbits is investigated in binary
systems using Hill's method. Analytical stability conditions are
established for satellites, for inner planets and for outer planets,
allowing arbitrary values for the mass-ratio of the binary.

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