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LOW ENERGY TRAJECTORY OPTMIZATION FOR CE-2'S EXTENDED MISSION AFTER 2012

机译:2012年后低能耗轨迹优化部队2的扩展任务

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CE-2, the second lunar satellite of China, has been the first satellite in the world to transfer from lunar polar orbitto the Sun-Earth L2 libration point. CE-2 will remain in the L2 Lissajous trajectory until the end of 2012, when about120 m/s delta-v will be left. This paper studies trajectory optimization for CE-2's extended mission after 2012. Theprimary goal of this work is to design a suitable trajectory that maximizes science data return in different regions ofthe Sun-Earth-Moon system. The mission design should encompass as many regions as possible. Both the invariantmanifolds of libration point and lunar gravity assist are used to design the low energy trajectories. A multiple regionsexploration scenario including four main phases is proposed. First, the satellite follows the unstable manifolds toleave the Sun-Earth L2 Lissajous trajectory. After the first lunar flyby, the satellite enters into an Earth high ellipticorbit, from which geomagnetic tail and space environment could be studied. With another one or two lunar flyby,the spacecraft follows the stable manifolds to the Sun-Earth L1 Halo orbit, from which solar physics could be studied.Finally, the spacecraft follows the unstable manifolds to leave the Sun-Earth L1 Halo orbit, and fly towards the Sun-Earth L4 libration point. The spacecraft encounters an asteroid on the way to the L4 point. This paper also discussesthe trajectory optimization for Chang'e 2's practical flight to the Toutatis asteroid, about 22 m/s delta-V is savedcompared to the baseline trajectory. Hence the saved delta-V could be used for trajectory correction maneuvers toinsure the probability of the successful asteroid flyby. This work demonstrates practical applications of advancedastrodynamic concepts in the Sun-Earth-Moon system, including chaotic three-body orbits, periodic three-bodyorbits, gravity assist, and the conic patched method. The result is a practical mission design of a grand tour for theSun-Earth-Moon system using limited fuel resources.
机译:CE-2是中国的第二颗月球卫星,已成为世界上第一颗从月球极轨转移的卫星 到太阳地球L2解放点。 CE-2将保持在L2里萨茹斯(Lissajous)的轨道中,直到2012年底, 剩下120 m / s delta-v。本文研究了CE-2在2012年之后的扩展任务的轨迹优化。 这项工作的主要目标是设计一条合适的轨迹,以最大化科学数据在不同地区的返回。 太阳地球月亮系统。任务设计应涵盖尽可能多的区域。两者不变 释放点和月球重力辅助的歧管用于设计低能轨迹。多个地区 提出了包括四个主要阶段的勘探方案。首先,卫星跟随不稳定的流形进入 离开太阳地球L2 Lissajous轨迹。在第一次月球飞越之后,卫星进入地球的高椭圆形 轨道,从中可以研究地磁尾部和空间环境。随着另外一两个月球飞越, 该航天器沿着稳定的歧管到达太阳地球L1晕圈轨道,从中可以研究太阳物理学。 最后,航天器跟随不稳定的歧管离开太阳地球L1晕轨道,然后飞向太阳- 地球L4解放点。航天器在到达L4点的途中遇到一颗小行星。本文还讨论了 Chang娥二号实际飞行到Toutatis小行星的轨迹优化,节省了约22 m / s的增量V 与基线轨迹相比。因此,保存的delta-V可以用于轨迹修正操作,以 确保小行星飞越成功的可能性。这项工作演示了高级的实际应用 太阳-地球-月亮系统中的空间动力学概念,包括混沌三体轨道,周期性三体 轨道,重力辅助和圆锥形修补方法。结果是为巡回演出进行了实用的任务设计 日月系统使用有限的燃料资源。

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