On the stability of the triangular libration points for the photogravitational circular restricted problem of three bodies when both of the attracting bodies are radiating as well
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Publication:5903517
DOI10.1007/BF01230257zbMath0633.70015MaRDI QIDQ5903517
Publication date: 1987
Published in: Celestial Mechanics (Search for Journal in Brave)
photogravitational circular restricted problem of three bodiesstability of the triangular libration points
Three-body problems (70F07) Stability for nonlinear problems in mechanics (70K20) Computational methods for problems pertaining to mechanics of particles and systems (70-08)
Related Items (11)
Nonlinear stability of the libration points in the photogravitational restricted three body problem ⋮ Equilibria and stability of the restricted photogravitational problem of \(2+2\) bodies ⋮ Nonlinear stability of the triangular libration points for the photo gravitational elliptic restricted problem of three bodies ⋮ Stability of the triangular points under combined effects of radiation and oblateness in the restricted three-body problem ⋮ On the triangular libration points in photogravitational restricted three-body problem with variable mass ⋮ Existence of libration points in the restricted problem of three bodies with radiation pressure ⋮ Collinear points in the photogravitational ER3BP with zonal harmonics of the secondary ⋮ About stability of libration points in the restricted photogravitational three body problem ⋮ Non-linear stability of triangular equilibrium points in ER3BP under radiating primaries in presence of resonance ⋮ The libration points of a spherical satellite in the photogravitational restricted problem of three bodies ⋮ Normalization algorithms of Hamiltonian near an equilibrium point
Cites Work
- On the stability of triangular libration points taking into account the light pressure for the circular restricted problem of three bodies
- On the stability of triangular libration points of the photogravitational restricted circular three-body problem
- The restricted 3-body problem with radiation pressure
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