Trajectory and stability of Lagrangian point \(L_{2}\) in the Sun-Earth system
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Publication:535745
DOI10.1007/S10509-010-0493-9zbMath1213.85020arXiv1009.4008OpenAlexW2109413974MaRDI QIDQ535745
Publication date: 13 May 2011
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1009.4008
Two-body problems (70F05) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10)
Related Items (2)
Existence of equilibrium points and their linear stability in the generalized photogravitational Chermnykh-like problem with power-law profile ⋮ Trajectories of \(L _{4}\) and Lyapunov characteristic exponents in the generalized photogravitational Chermnykh-like problem
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- On the Chermnykh-like problems. I. The mass parameter \(\mu = 0.5\)
- On the Chermnykh-like problems. II. The equilibrium points
- Linear stability of equilibrium points in the generalized photogravitational Chermnykh's problem
- Linearization of the Hamiltonian in the generalized photogravitational Chermnykh's problem
- DYNAMICAL EFFECTS FROM ASTEROID BELTS FOR PLANETARY SYSTEMS
- BURRAU'S PROBLEM OF THREE BODIES
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