Abstract
The photogravitational oblate restricted three-body problem is carried out within the post-Newtonian framework. The primaries are assumed to be oblate as well as radiant sources. The perturbed location of the collinear point \( L_{3}\) is computed. A series form of \( L_{3}\) location is obtained as a new analytical results. In order to introduce a semi-analytical view, a Mathematica program is constructed so as to draw the locations of collinear point \( L_{3}\)versus the mass ratio \( \mu\in (0, 0.5)\) taking into account one or more of the considered perturbations. All the obtained figures are analyzed.
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