The Effect of Radiation Pressure on the Equilibrium Points in the Generalised Photogravitational Restricted Three Body Problem

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dc.creatorKushvah, Badam Singh
dc.date2008-01-22
dc.date2008-05-16
dc.date.accessioned2026-07-07T12:38:29Z
dc.date.available2026-07-07T12:38:29Z
dc.descriptionThe existence of equilibrium points and the effect of radiation pressure have been discussed numerically. The problem is generalized by considering bigger primary as a source of radiation and small primary as an oblate spheroid. We have also discussed the Poynting-Robertson(P-R) effect which is caused due to radiation pressure. It is found that the collinear points $L_1,L_2,L_3$ deviate from the axis joining the two primaries, while the triangular points $L_4,L_5$ are not symmetrical due to radiation pressure. We have seen that $L_1,L_2,L_3$ are linearly unstable while $L_4,L_5$ are conditionally stable in the sense of Lyapunov when P-R effect is not considered. We have found that the effect of radiation pressure reduces the linear stability zones while P-R effect induces an instability in the sense of Lyapunov.
dc.identifierhttps://arxiv.org/abs/0801.3369
dc.identifierhttp://arxiv.org/abs/0801.3369
dc.identifierAstrophysics and Space Science, Volume 315, Numbers 1-4 / June, 2008
dc.identifierdoi:10.1007/s10509-008-9823-6
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218775
dc.subjectDynamical Systems
dc.subject70F15
dc.titleThe Effect of Radiation Pressure on the Equilibrium Points in the Generalised Photogravitational Restricted Three Body Problem
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