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首页> 外文期刊>Advances in Astronomy >Nonlinear Stability of the Triangular Libration Points for Radiating and Oblate Primaries in CR3BP in Nonresonance Condition
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Nonlinear Stability of the Triangular Libration Points for Radiating and Oblate Primaries in CR3BP in Nonresonance Condition

机译:非共振条件下CR3BP中辐射和扁形基体的三角振动点的非线性稳定性

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摘要

This paper investigates the existence of resonance and nonlinear stability of the triangular equilibrium points when both oblate primaries are luminous. The study is carried out near the resonance frequency, satisfying the conditionsω1=ω2,  ω1=2ω2, andω1=3ω2in circular cases by the application of Kolmogorov-Arnold-Moser (KAM) theory. The study is carried out for the various values of radiation pressure and oblateness parameters in general. It is noticed that the system experiences resonance atω1=2ω2,  ω1=3ω2for different values of radiation pressures and oblateness parameter. The caseω1=ω2corresponds to the boundary region of the stability for the system. It is found that, except for some values of the radiation pressure, and oblateness parameters and forμ≤μc=0.0385209, the triangular equilibrium points are stable.
机译:本文研究了两个扁圆形原色发光时三角平衡点的共振和非线性稳定性的存在。利用Kolmogorov-Arnold-Moser(KAM)理论在圆形情况下满足共振频率ω1=ω2,ω1=2ω2和ω1=3ω2的条件下进行了研究。通常对辐射压力和扁率参数的各种值进行研究。注意到对于不同的辐射压力值和扁率参数,系统在ω1=2ω2,ω1=3ω2处发生共振。 ω1=ω2对应于系统稳定性的边界区域。发现除了辐射压的一些值和扁度参数以及对于μ≤μc= 0.0385209而言,三角形平衡点是稳定的。

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