We investigate in the framework of the elliptic restricted three-body problem (ER3BP), the influence of the zonal harmonics (J2 and J4) of the primary and the radiation pressure of the secondary on the positions and stability of the triangular equilibrium points. The triangular points of the problem are affected by the parameters involved in the systems’ dynamics. The positions change with increase in the zonal harmonics, eccentricity and radiation pressure. The triangular points remain stable in the interval 0<μ<μc as shown arbitrarily.
International Frontier Science Letters (Volume 10)
J. Singh et al., "Influence of the Zonal Harmonics of the Primary on L4,5 in the Photogravitational ER3BP", International Frontier Science Letters, Vol. 10, pp. 23-36, 2016