The dynamics of the 1:2 resonant motion with Neptune in the 3D elliptic restricted three-body problem
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20040213/pdf
Reference52 articles.
1. Asymmetric librations in exterior resonances
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3. Extrasolar Planets in Mean‐Motion Resonance: Apses Alignment and Asymmetric Stationary Solutions
4. Broucke, R. A. 1968, Periodic Orbits in the Elliptic Restricted Three Body problem, JPL Technical Report, 32
5. Stability of periodic orbits in the elliptic, restricted three-body problem.
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1. Secular structure of 1:2 and 1:3 mean motion resonances with Neptune;Astronomy & Astrophysics;2024-07
2. Universal method for designing periodic orbits by homotopy classes in the elliptic restricted three-body problem;Astrodynamics;2024-02-08
3. The phase space structure of retrograde mean motion resonances with Neptune: the 4/5, 7/9, 5/8 and 8/13 cases;Celestial Mechanics and Dynamical Astronomy;2022-11-10
4. Review Article: Resonant Families of Periodic Orbits in the Restricted Three-body Problem*;Research in Astronomy and Astrophysics;2022-06-17
5. Retrograde periodic orbits in 1/2, 2/3 and 3/4 mean motion resonances with Neptune;Celestial Mechanics and Dynamical Astronomy;2020-06
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