Existence and stability of libration points in the restricted three-body problem when the smaller primary is a triaxial rigid body and the bigger one an oblate spheroid
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Publication:1296551
zbMath0931.70011MaRDI QIDQ1296551
Publication date: 8 March 2000
Published in: Indian Journal of Pure \& Applied Mathematics (Search for Journal in Brave)
stationary solutionselliptic orbitsaxis of symmetrycollinear pointscritical mass parametertriangular pointsmass parameter
Related Items (8)
Periodic orbits generated by Lagrangian solutions of the restricted three body problem when one of the primaries is an oblate body ⋮ 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 ⋮ The effect of photogravitational force and oblateness in the perturbed restricted three-body problem ⋮ The effect of oblateness in the perturbed restricted three-body problem ⋮ Periodic orbits in the restricted problem of three bodies in a three-dimensional coordinate system when the smaller primary is a triaxial rigid body ⋮ Effect of oblateness of an artificial satellite on the orbits around the triangular points of the Earth-Moon system in the axisymmetric ER3BP ⋮ The effect of perturbations on the circular restricted four-body problem with variable masses
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