A Study on Bi-circular R4BP with Dissipative Forces: Motion of a Spacecraft in the Earth-Moon-Focused View

Equilibria, stability and chaos in photogravitational Bi-Circular restricted four-body problem

“… Singh and Omale (2019) further emphasized that in the CR4BP, a combination of Stokes drag force and oblateness of the primaries leads to a decaying effect in the orbital elements. In Singh et al. (2020) , the investigation revealed that circumstellar dust and radiation pressure in CR4BP in Manve's field cause dissipative effect on the motion of a test particle.…”

“… Abouelmagd and Ansari (2019) revealed the motion properties of the infinitesimal body in the framework of Bi-Circular Sun perturbed Earth-Moon System. Singh and Omale (2020) did a study on the Bi-Circular R4BP with dissipative forces and they pointed that the P-R drag exert greater drag effect on the motion of a test particle than the Stokes drag. The Bi-Bircular restricted four body problem (BR4BP) is very useful for analytic and application purpose, for example, The low eccentricity of the Earth's and Moon's orbit and the small inclination of the Moon's orbital plane, make the Bi-Circular R4BP an accurate model to describe the dynamics of a spacecraft in the Sun-Earth-Moon system; see Yagasaki (2004) and Mingotti et al.…”