Explosive evolution of small bodies in planetary atmospheres

被引:0
作者
Ibadov, Subhon [1 ,2 ]
Ibodov, Firuz S. [1 ]
机构
[1] Lomonosov Moscow State Univ, SAI, Moscow, Russia
[2] TAS, Inst Astrophys, Dushanbe, Tajikistan
来源
COMPLEX PLANETARY SYSTEMS | 2014年 / 9卷 / 310期
关键词
planets: atmospheres; comets: general; minor planets; asteroids; aerodynamic crushing; hot plasma;
D O I
10.1017/S1743921314008126
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The entry of small celestial bodies such as cometary nuclei, asteroids and their large fragments, into a planetary atmosphere is accompanied by an "explosion", i.e., sudden rise in brightness and the generation of a "blast" shock wave, like the 2013 Chelyabinsk event. Fully analytic approach to the phenomenon is developed taking into account aerodynamic crushing of the body and transversal expansion of the crushed mass, that leads to impulse generation of hot plasma and a "blast" shock wave in the thin "exploding" layer.
引用
收藏
页码:162 / 163
页数:2
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