- Supplementary Content
- 10.21203/rs.3.rs-8878619/v1
Impacts of Varying Zonal Harmonics Upto J4 on Dynamics of a Satellite Around Out-of-plane Points of Restricted Three-Body Problem with Variable masses
- Feb 19, 2026
- Research Square
- Joel John Taura + 2 more +2
<title>Abstract</title> This paper investigates the impacts of varying zonal harmonics up to J4 on dynamics of a satellite around out-of-plane equilibrium points of the restricted three-body problem with variable masses. The motion and mass variations of the primaries are described by the Gylden-Mestschersky problem (GMP) and the unified Mestschersky law (UML), respectively.The non-autonomous differential dynamical equations of the satellite are obtained and transformed to an autonomized system, with the help of the Mestschersky transformation, the UML, the particular integral and solutions of the GMP. Four out-of-plane equilibrium points (OEPs) denoted by and are obtained. Further, the OEPs are seen to be unstable and a numerical application is rendered for a satellite placed in the neighborhood of PQ Pegasi. It is observed that Increasing values of zonal harmonics results in the satellites position at the OEPs drifting towards the binary while the satellite is forced away from the PQ Pegasi at the points. A contrary observation occurs when the mass variation is large. Also, the zero velocity curves (ZVCs) are explored and it is seen that increasing the mass variation parameter increases the forbidden region in the presence or absence of zonal harmonic terms. Also, it is seen that, the zonal harmonic J4 term increases the region where motion is permissible, while the J2 term decreases it. Furthermore, it was seen that the orbits of the satellite around the OEPs could be quasi-periodic, divergent straight line or a chaotic. The study is applicable in space missions and astronomy.
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