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Scattering of Trajectories of Hazardous Asteroids

机译:危险小行星轨迹的散射

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Early detection of possible collisions of asteroids with the Earth is necessary to exept the asteroid-comet hazard. Many collisions associate with resonant returns after preceding approaches. The difficulty of collisions prediction is associated with a resonant returns after encounters with the Earth due to loss of precision in these predictions. On the other hand, we can use the fly-by effect to avoid hazardous asteroid from collision. The main research object is the asteroid Apophis (99942), for which we found about 100 orbits of possible impacts with the Earth and more than 10 - with the Moon. It is shown that the early (before 2029) change of the Apophis orbit allows to avoid all main impacts with the Earth in 21 st century, associated with resonant returns, and such a change of the orbit, in principle, is feasible. The scattering of possible trajectories of Apophis after 2029 and after 2051, as well as 2015 RN35 and other dangerous objects, is discussed.
机译:需要提前检测与地球的小行星可能的碰撞是为了弥补小行星彗星危险所必需的。在前面的方法之后,许多碰撞与谐振返回相关联。由于在这些预测中的精度损失,碰撞预测的难度预测与地球遇到后的谐振返回相关联。另一方面,我们可以使用飞行效果来避免碰撞危险的小行星。主要研究对象是小行星己烯(99942),我们发现大约100个可能的可能影响与地球和10多个 - 与月球。结果表明,APOPOH轨道的早期(2029年)的变化允许避免与21世纪的地球中的所有主要影响,与谐振回报相关,以及原则上的轨道的这种变化是可行的。讨论了2029年和2051年之后的Apophis可能的轨迹,以及2015年RN35和其他危险物品。

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