Critical point families at the 3:1 resonance

DOI10.1007/BF00049517zbMath0925.70129OpenAlexW1978825996MaRDI QIDQ1898003

Miquel Grau-Sánchez

Publication date: 25 October 1995

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

Full work available at URL: https://doi.org/10.1007/bf00049517

Mathematics Subject Classification ID

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

Related Items (1)

Critical point families at the 3:1 resonance

Cites Work

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• Chaotic behaviour of trajectories for the asteroidal resonances
• Resonant motion in the restricted three-body problem
• The elliptic restricted problem at the 3:1 resonance
• Collective resonant phenomena on small bodies in the solar system
• Critical point families at the 3:1 resonance
• A second fundamental model for resonance
• Formation of the Kirkwood gaps in the asteroid belt
• High-order resonances in the restricted three-body problem
• Periodic orbits of the planetary type and their stability
• Stability of periodic orbits in the elliptic, restricted three-body problem.

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