Experimental hypervelocity impacts: Implication for the analysis of material retrieved after exposure to space environment Part I. Impacts on aluminium targets

被引:7
|
作者
Mandeville, Jean-Claude [1 ]
Perrin, Jean-Marie [2 ,3 ]
Vidal, Loic [4 ]
机构
[1] MANDESPACE, F-31000 Toulouse, France
[2] Observ Haute Provence, CNRS UMS 3470, St Michel Observ, F-04870 St Michel, France
[3] Observat Spatiales LATMOS UMR 8190, Lab ATmospheres Milieux, F-78280 Guyancourt, France
[4] Inst Sci Mat Mulhouse IS2M, CNRS LRC 7228, F-68057 Mulhouse, France
关键词
Meteoroids; Orbital debris; Hypervelocity impact; EDX; Spacecraft; SOLAR-CELLS;
D O I
10.1016/j.actaastro.2012.08.033
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
During the last three decades a wide variety of surfaces have been brought back to Earth after being exposed to space environment. The impact features found on these surfaces are used to evaluate the damages caused to spacecraft and can give clues to the characteristics of the orbital debris and meteoroids that created them. In order to derive more precisely the particle parameters and to improve the analysis of projectile remnants, we have performed an extensive analysis of craters caused by the impact of high velocity particles on thick ductile targets, using a micro-particle accelerator. We show that from the geometry of the craters and from the analysis of the remnants it is possible to derive the main characteristics of the projectiles. In particular, using up-to-date instrumentation, scanning electron microscope (SEM) and Energy Dispersive X-ray (EDX) spectrometer, we found that even small residues inside craters can be identified. However, this study shows that a velocity resolution better than 1 km/s would be appropriate to obtain a fair calibration of the impact processes on a ductile target. This would allow to decipher with precision impact features on ductile surfaces exposed to space environment. (C) 2012 Elsevier Ltd. All rights reserved.
引用
收藏
页码:532 / 544
页数:13
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