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

Table 2

Effects of radiation pressure factor, P–R drag, and dynamical flattening parameters on the stability of triangular equilibrium points of the Sun-Earth system.

	Case			Remark
1	Classical	0.004504233279349719	0.999780664387228	Stable
2		0.004504233327067630	0.999780664386725	Stable
3		0.004504233279348517	0.999780664379725	Stable
4		0.004504233327101427	0.999780664379223	Stable