Numerical simulation of high-velocity impact ejecta following falls of comets and asteroids onto the Moon

被引:40
|
作者
Artemieva, N. A. [1 ]
Shuvalov, V. V. [1 ]
机构
[1] Russian Acad Sci, Inst Geospheres Dynam, Moscow 119334, Russia
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1134/S0038094608040059
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High-velocity comet and asteroid impacts onto the Moon are considered and the material masses ejected after such impacts at velocities above the second-cosmic velocity for the Moon (2.4 km/s) are calculated. Although the results depend on a projectile type and the velocity and angle of an impact, it has been demonstrated that, on average, the lunar mass decreases with time. The Moon has lost about 5 x 10(18) kg, that is, about one-hundredth of a percent of its mass, over the last 3.8-3.9 billion years. The ejection of lunar meteorites and lunar dust, rich in He-3, is considered as well. The results of the study are compared to the results of earlier computations and data on lunar meteorites.
引用
收藏
页码:329 / 334
页数:6
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