Asymptotic orbits at the triangular equilibria in the photogravitational restricted three-body problem
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Publication:863217
DOI10.1007/s10509-006-9043-xzbMath1110.85001OpenAlexW2030746995MaRDI QIDQ863217
Publication date: 25 January 2007
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-006-9043-x
periodic orbitheteroclinic orbithomoclinic orbitphotogravitational restricted three-body problemtriangular pointsphotogravitational problemsurface of sectionasymptotic orbitcut of Poincaré
Related Items (4)
Asymmetric periodic solutions in the restricted problem of three bodies ⋮ On some new aspects of the photo-gravitational Copenhagen problem ⋮ Effect of oblateness and radiation pressure on angular frequencies at collinear points ⋮ BIFURCATIONS IN THE TOPOLOGY OF ZERO-VELOCITY SURFACES IN THE PHOTO-GRAVITATIONAL COPENHAGEN PROBLEM
Cites Work
- Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem. I
- Families of periodic orbits in the photogravitational three-body problem
- Families of periodic orbits emanating from homoclinic orbits in the restricted problem of three bodies
- The web of periodic orbits at \(L_4\)
- Homoclinic and heteroclinic solutions in the restricted three-body problem
- The equilibrium state in the Magnetic-Binary problem when the more massive primary is an oblate spheroid
- Connecting orbits and invariant manifolds in the spatial restricted three-body problem
- The restricted 3-body problem with radiation pressure
- [https://portal.mardi4nfdi.de/wiki/Publication:5675367 Proof of a conjecture of E. Str�mgren]
- The nonlinear stability of \(L_4\) in the restricted three-body problem when the bigger primary is a triaxial rigid body
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