Analysis on the stability of triangular points in the perturbed photogravitational restricted three-body problem with variable masses
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Publication:989703
DOI10.1007/s10509-010-0339-5zbMath1195.85008OpenAlexW2091814585MaRDI QIDQ989703
Jagadish Singh, Umar Aishetu, Oni Leke
Publication date: 23 August 2010
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10509-010-0339-5
Related Items (5)
Effects of Poynting-Robertson (P-R) drag, radiation, and oblateness on motion around the L4,5 equilibrium points in the CR3BP ⋮ Effect of oblateness, perturbations, radiation and varying masses on the stability of equilibrium points in the restricted three-body problem ⋮ The effect of photogravitational force and oblateness in the perturbed restricted three-body problem ⋮ On the triangular libration points in photogravitational restricted three-body problem with variable mass ⋮ Equilibrium points and stability in the restricted three-body problem with oblateness and variable masses
Cites Work
- Effect of perturbations on the non linear stability of triangular points in the restricted three-body problem with variable mass
- Stability of the photogravitational restricted three-body problem with variable masses
- Existence of particular solutions in the generalised restricted problem of three bodies with variable masses
- Effect of perturbations on the stability of triangular points. In the restricted problem of three bodies with variable mass
- Effect of peturbations on the location of equilibrium points in the restricted problem of three bodies with variable mass
- Effect of perturbations in Coriolis and centrifugal forces on the stability of libration points in the restricted problem
- BURRAU'S PROBLEM OF THREE BODIES
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