Stable orbits of planets of a binary star system in the three-dimensional restricted problem

DOI10.1023/A:1013238413100zbMath0997.70010OpenAlexW1644898671MaRDI QIDQ5960088

Roger A. Broucke

Publication date: 11 April 2002

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1013238413100

zbMATH Keywords

three-body problembinary star systemdirect periodic orbitdynamical stabilityretrograde periodic orbitsymmetric orbitsthree-dimensional restricted three-body problem

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15)

Related Items (3)

Determination of the doubly symmetric periodic orbits in the restricted three-body problem and Hill's lunar problem ⋮ On the figure-8 periodic solutions in the three-body problem ⋮ The Restricted Five-Body Problem With Cyclic Kite Configuration

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