Stability of the triangular points under combined effects of radiation and oblateness in the restricted three-body problem

DOI10.1007/S11038-013-9415-5zbMath1329.85002OpenAlexW2152176129MaRDI QIDQ892392

Elbaz I. Abouelmagd

Publication date: 19 November 2015

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s11038-013-9415-5

zbMATH Keywords

stabilityrestricted three-body problemradiation pressuretriangular pointsoblateness

Mathematics Subject Classification ID

Two-body problems (70F05) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Galactic and stellar dynamics (85A05) Equations of motion in general relativity and gravitational theory (83C10) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (7)

Effects of Poynting-Robertson (P-R) drag, radiation, and oblateness on motion around the L_4,5 equilibrium points in the CR3BP ⋮ The effect of photogravitational force and oblateness in the perturbed restricted three-body problem ⋮ On the perturbed restricted three-body problem ⋮ Periodic orbit in the frame work of restricted three bodies under the asteroids belt effect ⋮ Dynamics of a dumbbell satellite under the zonal harmonic effect of an oblate body ⋮ Libration points in the restricted three-body problem: Euler angles, existence and stability ⋮ The perturbed photogravitational restricted three-body problem: analysis of resonant periodic orbits

Cites Work

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• Solar System Dynamics
• The restricted 3-body problem with radiation pressure
• Existence of libration points in the generalised photogravitational restricted problem of three bodies
• 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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