Research Article

Impacts of Poynting–Robertson Drag and Dynamical Flattening Parameters on Motion around the Triangular Equilibrium Points of the Photogravitational ER3BP

Figure 1

Effects of radiation pressure factor, P–R drag, and dynamical flattening parameters on the locations of triangular equilibrium points of the Sun-Earth system. (a) Blue triangle is for the classical case. (b) Purple triangle is for case. (c) Brown triangle is for case. (d) Turquoise triangle is for case.
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