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• W3114288450 abstract "In a synodic-pulsating dimensionless coordinate, with a luminous primary and an oblate secondary, we examine the effects of radiation pressure, oblateness (quadruple and octupolar i.e. ) and eccentricity of the orbits of the primaries on the triangular points in the ER3BP. have been shown to disturb the motion of an infinitesimal body and particularly has significant effects on a satellite’s secular perturbation and orbital precessions. The influence of these parameters on the triangular points of Zeta Cygni, 54 Piscium and Procyon A/B are highlighted in this study. Triangular points are stable in the range and their stability is affected by said parameters." @default.
• W3114288450 created "2021-01-05" @default.
• W3114288450 creator A5000026387 @default.
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• W3114288450 date "2020-12-01" @default.
• W3114288450 modified "2023-09-23" @default.
• W3114288450 title "Effect of Oblateness of the Secondary up to <i>J₄ </i>on <i>L_4,5</i> in the Photogravitaional ER3BP" @default.
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• W3114288450 doi "https://doi.org/10.18052/www.scipress.com/ijarm.13.1" @default.
• W3114288450 hasPublicationYear "2020" @default.
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