The equilibrium points in the perturbed R3BP with triaxial and luminous primaries
From MaRDI portal
Publication:383525
DOI10.1007/s10509-013-1420-7zbMath1276.70009OpenAlexW2009272974MaRDI QIDQ383525
Publication date: 5 December 2013
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-013-1420-7
Three-body problems (70F07) Celestial mechanics (70F15) Stability problems for finite-dimensional Hamiltonian and Lagrangian systems (37J25) Stability of manifolds of solutions to ordinary differential equations (34D35) Stationary solutions of functional-differential equations (34K21)
Related Items (5)
On the stability of the triangular points in the relativistic R3BP with a bigger triaxial primary ⋮ Triangular libration points in the CR3BP with radiation, triaxiality and potential from a belt ⋮ Unnamed Item ⋮ On the stability of \(L_{4,5} \) in the photogravitational relativistic R3BP ⋮ On the stability of the triangular equilibrium points in the photogravitational R3BP with an oblate infinitesimal and triaxial primaries for the binary lalande 21258 system
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Combined effects of perturbations, radiation, and oblateness on the nonlinear stability of triangular points in the restricted three-body problem
- Stability of equilibrium points in the generalized perturbed restricted three-body problem
- On the stability of triangular points in the elliptic R3BP under radiating and oblate primaries
- Effect of perturbations in Coriolis and centrifugal forces on the stability of libration points in the restricted problem
- Locating and Computing All the Simple Roots and Extrema of a Function
- ON MOULTON'S ORBITS IN THE RESTRICTED PROBLEM OF THREE BODIES
- Existence and stability of libration points in the restricted three-body problem when the primaries are triaxial rigid bodies
- Existence and stability of libration points in the restricted three-body problem when the primaries are triaxial rigid bodies and source of radiations
- Computing with certainty individual members of families of periodic orbits of a given period.
This page was built for publication: The equilibrium points in the perturbed R3BP with triaxial and luminous primaries