Numerical experiments on planetary orbits in double stars

DOI10.1007/BF01235815zbMath0566.70009OpenAlexW4243806069MaRDI QIDQ3681979

No author found.

Publication date: 1984

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01235815

zbMATH Keywords

eccentricitycritical orbitselliptic restricted three-body problemnumerical studyplanets in double stars

Mathematics Subject Classification ID

Three-body problems (70F07) Software, source code, etc. for problems pertaining to mechanics of particles and systems (70-04)

Related Items (7)

Secular dynamics of S-type planetary orbits in binary star systems: applicability domains of first- and second-order theories ⋮ Evolution of the characteristic curves in the restricted three-body problem in terms of the mass parameter ⋮ Secular dynamics of multiplanetary circumbinary systems: stationary solutions and binary-planet secular resonance ⋮ An analytical study of stable planetary orbits in the circular restricted problem ⋮ An approximate integral and solution for eccentric planetary type orbits in the restricted problem of three bodies ⋮ Stability of outer planetary orbits around binary stars: A comparison of Hill's and Laplace's stability criteria ⋮ On the Stability of Extra-Solar Planetary Systems

Cites Work

• Families of periodic planetary-type orbits in the three-body problem and their stability
• Integration of the elliptic restricted three-body problem with Lie series
• Stability of planetary orbits in binary systems
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