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Distant Retrograde Orbits for space-based Near Earth Objects detection

机译:遥测逆行轨道用于天基近地物体探测

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摘要

We analyse a concept for the detection of Potentially Hazardous Asteroids (PHAs) from a space-based network of telescopes on retrograde Distant Periodic Orbits. Planar periodic orbits are designed in the Sun-Earth circular restricted three-body problem, starting from initial conditions in the Hill's problem available from the literature. A family of retrograde orbits centred at the Earth is selected as baseline, based on their maximum distance from Earth, larger than the Earth-L_2 distance. Indeed, spacecraft on such orbits can detect PHAs incoming from the Sun direction, which could not otherwise be monitored from current Earth-based systems. A trade-off on the orbit amplitude, asteroid diameter to be detected, and the constellation size is performed considering current visible sensor telescope technology. The Chelyabinsk meteor scenario is studied and the potential warning time that could be gained with a space-based survey system with respect to an Earth based-survey system is shown.
机译:我们分析了一种从逆向遥远周期性轨道上的天基望远镜网络探测潜在危险小行星(PHA)的概念。平面周期轨道是在太阳地球圆形受限三体问题中设计的,从可从文献中获得的希尔问题的初始条件开始。根据与地球的最大距离(大于Earth-L_2距离),选择一个以地球为中心的逆行轨道系列作为基准。实际上,在此类轨道上的航天器可以检测到从太阳方向入射的PHA,否则无法通过当前的地球系统进行监视。考虑到当前的可见传感器望远镜技术,需要对轨道振幅,要检测的小行星直径和星座大小进行权衡。研究了车里雅宾斯克流星的情景,并显示了相对于基于地球的调查系统,基于天基的调查系统可能获得的潜在预警时间。

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