Dynamics in the center manifold around \(L_2\) in the quasi-bicircular problem

DOI10.1023/A:1019979414586zbMath1027.70016OpenAlexW2130757444MaRDI QIDQ1870186

Miquel A. Andreu

Publication date: 11 May 2003

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

Full work available at URL: https://doi.org/10.1023/a:1019979414586

zbMATH Keywords

center manifoldinvariant toriEarth-Moon-Sun systemfour body problemquasi-bicircular problem

Mathematics Subject Classification ID

Celestial mechanics (70F15) Dynamical systems in classical and celestial mechanics (37N05) (n)-body problems (70F10)

Related Items (10)

Extension of fast periodic transfer orbits from the Earth-Moon RTBP to the Sun-Earth-Moon quasi-bicircular problem ⋮ Invariant manifolds of a non-autonomous quasi-bicircular problem computed via the parameterization method ⋮ The vicinity of Earth-Moon \(L_1\) and \(L_2\) in the Hill restricted 4-body problem ⋮ Invariant manifolds near \(L_1\) and \(L_2\) in the quasi-bicircular problem ⋮ Regions of prevalence in the coupled restricted three-body problems approximation ⋮ Dynamical aspects of an equilateral restricted four-body problem ⋮ The vicinity of the Earth-Moon \(L_1\) point in the bicircular problem ⋮ Families of Halo-like invariant tori around \(L_2\) in the Earth-Moon bicircular problem ⋮ Using invariant manifolds to capture an asteroid near the \(L_3\) point of the Earth-Moon bicircular model ⋮ Fast periodic transfer orbits in the Sun-Earth-Moon quasi-bicircular problem

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