International Journal of Bifurcation and Chaos · 2011 · 148 citations · 16 references
Natural SciencesMathematicsDifferential EquationsDynamical SystemsGeometryMulti-body DynamicsMultibody DynamicsRestricted Three-body ProblemRigid Body DynamicsStability TheoryCollinear Equilibrium PointsEquilibriumEquilibrium ConfigurationsEquipotential SurfacesLagrange Equilibrium PointsThree-body DynamicsThree-body ProblemThree-body Problem Stability
We study numerically the problem of four bodies, three of which are finite, moving in circles around their center of mass fixed at the origin of the coordinate system, according to the solution of Lagrange where they are always at the vertices of an equilateral triangle, while the fourth is infinitesimal. The fourth body does not affect the motion of the three bodies (primaries). The allowed regions of motion as determined by the zero-velocity surface and corresponding equipotential curves as well as the positions of the equilibrium points are given. The existence and the number of collinear and noncollinear equilibrium points of the problem depend on the mass parameters of the primaries. For three unequal masses, collinear equilibrium solutions do not exist. Critical masses associated with the existence and the number of equilibrium points, are given. The stability of the relative equilibrium solutions in all cases is also studied. The regions of the basins of attraction for the equilibrium points of the present dynamical model for some values of the mass parameters are illustrated.
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V. Szebehely · NASA Technical Reports Server (NASA) · 1967 · 1.3K citations
Infrared images of the transiting disk in the ε Aurigae system
Brian Kloppenborg, R. E. Stencel, John D. Monnier et al. · Nature · 2010 · 144 citations · Full text
Natural Sciences, Astronomy, Physics +14