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MULTIPLE-SPACECRAFT TRANSFERS TO SUN-EARTH DISTANT RETROGRADE ORBITS FOR ASTEROID DETECTION MISSIONS

机译:星际探测任务向远地逆行的多重空间转移

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As demonstrated by the meteorite fall in Chelyabinsk, Russia, in February 2013, also asteroids with a diameter smaller than 40 m can enter the Earth's atmosphere and cause a local damage on ground. For such small Potentially Hazardous Asteroids (PHAs) a short warning would be sufficient to have a protection plan in place on ground. However, small asteroids are difficult to be detected from ground, especially if they approach the Earth from the Sun direction, such as the Chelyabinsk object. For this reason, a multi-spacecraft mission was proposed to monitor PHAs from a telescope base orbiting on Distant Retrograde Orbits of the Sun - Earth system. This space-based system would allow increasing the warning time of asteroids incoming from the Sun direction. In this article a trade-off analysis is performed on the DRO and constellation size based on some measures of the detection capabilities. Moreover, the transfer to selected DROs from a Low Earth Orbit is designed to minimise the total Av and time to build the constellation.
机译:正如2013年2月俄罗斯车里雅宾斯克陨石坠落所证明的那样,直径小于40 m的小行星也可以进入地球大气层,并对地面造成局部破坏。对于如此小的潜在危险小行星(PHA),简短警告就足以在地面上制定保护计划。但是,很难从地面检测到小行星,特别是当它们从车里雅宾斯克天体等从太阳方向接近地球时。由于这个原因,提出了一个多航天器飞行任务,以监视从绕太阳-地球系统的远距逆向轨道运行的望远镜基地的PHA。这种基于天基的系统将允许增加从太阳方向入射的小行星的警告时间。在本文中,将基于检测能力的一些度量对DRO和星座图大小进行权衡分析。此外,从低地球轨道转移到选定DRO的目的是最大程度地减少构建星座图的总Av和时间。

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