Limits on the use of nuclear explosives for asteroid deflection

被引:26
作者
Syal, Megan Bruck [1 ]
Dearborn, David S. P. [2 ]
Schultz, Peter H. [1 ]
机构
[1] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[2] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA
关键词
Asteroid deflection; NEO mitigation; Planetary defense; Standoff nuclear explosion;
D O I
10.1016/j.actaastro.2012.10.025
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Recent studies by the US National Research Council identify nuclear explosives as the only current technology able to deflect large asteroids (those exceeding 500 m in diameter) or to mitigate impacts of smaller bodies when the warning time is short. Previous work predicts that either a standoff burst or a very low-yield surface burst is easily capable of deflecting a large (1 km) asteroid without fragmentation. Alternatively, large near-surface or just sub-surface bursts can sufficiently disrupt and disperse smaller bodies (300 m) to ensure that large fractions (in excess of 99.99%) miss the Earth entirely. Even for very short warning times (less than a month), more than 99.5% of a body's mass can be deflected off of an Earth-bound trajectory. However, successfully deflecting a small body, while avoiding fragmentation, becomes a challenging problem when the required kinetic energy increment is a substantial fraction of the body's potential. This paper addresses the challenge of preventing the production of substantial low-speed debris while deflecting small bodies with an impulsive method. (C) 2012 IAA. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:103 / 111
页数:9
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