Stability of triangular points in the relativistic R3BP when the bigger primary is an oblate spheroid

Nakone Bello, J. Singh
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Abstract

Abstract In this paper, we study the effect of oblateness of the more massive primary in the relativistic R3BP. We observe that the locations of the triangular points and their stability are affected by the relativistic and oblateness factors. It is also noticed that the oblateness factor possesses destabilizing behavior. Therefore, the size of the region of stability decreases with increase in the value of the oblateness factor. Further, a numerical study on the locations of the triangular points and the critical mass for the Earth-Moon , Jupiter and its Moons, Saturn and its Moons systems is given.
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相对论性R3BP中较大初心为扁球体时三角形点的稳定性
摘要本文研究了相对论性R3BP中大质量原星系扁率的影响。我们观察到三角形点的位置及其稳定性受到相对论性和扁率因素的影响。还注意到扁率因子具有不稳定行为。因此,稳定区域的大小随着扁率系数的增大而减小。此外,还对地月、木星及其卫星、土星及其卫星系统的三角点位置和临界质量进行了数值研究。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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