Origin and continuation of \(3/2, 5/2, 3/1, 4/1\) and \(5/1\) resonant periodic orbits in the circular and elliptic restricted three-body problem
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Publication:1785903
DOI10.1007/s10569-018-9834-8zbMath1447.70005arXiv1805.00288OpenAlexW2798518141MaRDI QIDQ1785903
Kyriaki I. Antoniadou, Anne-Sophie Libert
Publication date: 2 October 2018
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1805.00288
periodic orbitsthree-body problemorbital stabilitymean-motion resonancehigh eccentricitycircular family
Related Items (2)
On the Stability of the Triangular Equilibrium Points in the Elliptic Restricted Three-Body Problem with Radiation and Oblateness ⋮ Generalized periodic orbits in some restricted three-body problems
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