Unveiling Perturbing Effects of P-R Drag on Motion around Triangular Lagrangian Points of the Photogravitational Restricted Problem of Three Oblate Bodies

The perturbing effects of the Poynting-Robertson drag on motion an infinitesimal mass around triangular Lagrangian points circular restricted three-body problem under small perturbations in Coriolis and centrifugal forces when three bodies are oblate spheroids primaries emitters radiation pressure, is focus this paper. equations governing dynamical system have been derived locations determined. It seen that influenced by perturbation oblateness, pressure and, P-R primaries. Using software Mathematica, numerical analysis carried out to demonstrate how elements: ratio, influence positions equilibrium points, zero velocity surfaces stability. Our investigation reveals that, though oblateness decrease region stability stable, however, they not influential instability but drag. In stable inclusion bigger primary even almost negligible value 1.04548*10-9 overrides other effect changes instability. Hence, we conclude a strong force which remain unstable presence