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Analysis of Effect of Solar Radiation Pressure of Bigger Primary on the Evolution of Periodic Orbits

机译:大一次太阳辐射压力对周期轨道演化的影响分析

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Evolution of periodic orbits in Sun-Mars and Sun-Earth systems are analyzed using?Poincare surface of section technique and the effects of solar radiation pressure of?bigger primary and actual oblateness?of smaller primary on these orbits areconsidered.?It is observed that solar radiation pressure?of bigger primary has substantial effect on period, orbit’s shape, size and their position in the phase space. Since these orbits can be used for the design of low energy transfer trajectories, so perturbations?due to solar radiation pressure has to be understood and should be taken care of?during trajectory design. It is also verified that stability of such orbits are negligible?so they can be used as transfer orbit. For each pair of solar radiation pressure?q?and Jacobi constant?C?we get two separatrices where stability of island becomes zero. In this paper,?detailed stability analysis of periodic orbit having two loops is given when?q?= 0.9845.
机译:利用“庞加莱断面技术”分析了太阳-火星和太阳-地球系统中周期轨道的演化,并考虑了“较大的初生和实际扁率”的太阳辐射压力对这些轨道的影响。较大初级辐射的太阳辐射压力对周期,轨道的形状,大小及其在相空间中的位置有很大影响。由于这些轨道可用于低能量传递轨迹的设计,因此必须了解由于太阳辐射压力引起的扰动,并且在设计轨迹时应加以注意。还证实了这种轨道的稳定性可以忽略不计,因此它们可以用作传递轨道。对于每一对太阳辐射压力Qq和Jacobi常数C,我们得到两个分离,其中岛的稳定性变为零。本文给出了当qq = 0.9845时具有两个环的周期轨道的详细稳定性分析。

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