Impact of Radiation Pressure on the Out-of-Plane Libration Points in The Restricted Three-Body Problem with Rotating Mass Dipole Effect

dc.contributor.authorChukwueloka, Emeka Henry
dc.contributor.authorVincent, Ekele Aguda
dc.contributor.authorTaura, Joel John
dc.date.accessioned2026-01-28T23:31:48Z
dc.date.issued2025-09
dc.description.abstractThis paper investigates the impact of radiation pressure of the primary body on a third body in the vicinity of the out-of-plane libration points of the restricted problem of three bodies under a rotating mass dipole effect. It studies the impact of radiation factor (q1), force ratio (k) and mass-ratio parameter (𝜇) on the location, zero-velocity curves and instability of the out-of-plane libration points in the framework of the CRTBP. A symmetrical out-of-plane libration points are identified numerically on the xz-plane and the three system’s parameters, that is q1, k and 𝜇, are found to have impact on the positions of these points. In addition, the force ratio and radiation factor have significant effect on the configuration of the zero-velocity contours. The linear stability of the points for a broad scope of the parameters’ combinations was investigated, and it is found that the out-of-plane libration points are generally points of instability.
dc.identifier.urihttps://dx.doi.org/10.4314/ dujopas.v11i3c.28
dc.identifier.urihttps://repository.nmu.edu.ng/handle/123456789/75
dc.language.isoen
dc.publisherDutse Journal of Pure and Applied Sciences (DUJOPAS)
dc.subjectCRTBP
dc.subjectRotating mass dipole
dc.subjectRadiation pressure
dc.subjectOut-of-plane libration points
dc.subjectZero-velocity curves
dc.titleImpact of Radiation Pressure on the Out-of-Plane Libration Points in The Restricted Three-Body Problem with Rotating Mass Dipole Effect
dc.typeArticle

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