Motion and stability of triangular equilibrium points in elliptical restricted three body problem under the radiating primaries

Effects of radiation on stability of triangular equilibrium points in elliptic restricted three body problem

“…Furthermore, the nonlinear stability of the infinitesimal in the orbits or the size of the stable region around L 4 was "studied by Gyorgrey [16]" and the parametric resonance stability around L 4, in elliptical restricted three body problem was "studied by Erdi [18]". The influence of the eccentricity of the orbit of the primary bodies with or without radiation pressure on the existence of the equilibrium points and there stability was "discussed to some extent by Khasan [12], [13], Pinyol [19], Floria [20], Halan and Rana [21], Markeev [22], Selaru and Dumitrescu [14], [15], Nayayan and Ramesh [23], [24]". The stability of triangular points in the elliptical restricted three body problem under radiating and oblate primaries was "studied by Singh and Umar [25], [26]".…”

Characteristics exponents of the triangular solution in the elliptical restricted three-body problem under radiating and triaxial primaries

“…[12], Narayan, A., Kumar, C.R. [13], Narayan, A., Singh, N. [14], Narayan, A., Usha, T. [15] , Singh, J., Aishetu, U. (2012), Singh, J., Aishetu, U.…”

Analysis on nonlinear stability of the triangular libration points for radiating and oblate primaries in ER3BP

“…The ER3BP are studied by [11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26]. The present paper investigates the stability of the infinitesimal mass about the triangular equilibrium points in both resonance and non-resonance case satisfying…”