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

Table 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.

	Case
1	Classical	0.4999969965000000	0.866025403784439
2		0.4999969964999347	0.866025403784474
3		0.4999969965015000	0.866025403782418
4		0.4999969965014348	0.866025403782454