首页> 外文会议>56th International Astronautical Congress 2005 vol.4 >CHARACTERIZING FRAGMENTS FROM IMPACT ON A MICRO SATELLITE
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CHARACTERIZING FRAGMENTS FROM IMPACT ON A MICRO SATELLITE

机译:通过撞击微卫星来表征片段

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This paper characterizes the properties of fragments from impact on a micro satellite. We have found out that the NASA standard breakup model can be applied to low-velocity non-catastrophic collisions with some simple modifications. However, we are not sure if it can also be applied to low-velocity catastrophic collisions, wherein both projectile and target are totally fragmented. The difference between a catastrophic and a non-catastrophic collision would be determined by the ratio of kinetic energy at impact to target mass. The NASA standard breakup model has defined if the ratio is equal to or greater than 40 J/g, then the collision is catastrophic. Therefore, we hit a micro satellite of a mass of 681.5 g by a solid aluminum alloy sphere of a mass of 38.9 g at a speed of 1.35 km/s. This impact carried out above is catastrophic in modeling. Then, we compares fragments properties with those generated by the NASA standard breakup model 2000 revision to show that size distribution model in the standard breakup model can be applied to a catastrophic low-velocity collision with some simple modifications and size-to-area conversion model in the standard breakup model can be applied to a catastrophic low-velocity collision.
机译:本文描述了碎片撞击微卫星的性质。我们发现,只需进行一些简单的修改,即可将NASA标准分解模型应用于低速非灾难性碰撞。但是,我们不确定是否也可以将其应用于弹丸和目标都完全破碎的低速灾难性碰撞。灾难性碰撞与非灾难性碰撞之间的差异将由撞击时的动能与目标质量之比确定。 NASA标准解体模型已定义,如果该比率等于或大于40 J / g,则碰撞是灾难性的。因此,我们用质量为38.9 g的固态铝合金球以1.35 km / s的速度撞击了质量为681.5 g的微型卫星。上面执行的这种影响在建模中是灾难性的。然后,我们将碎片属性与由NASA标准分解模型2000修订版生成的碎片属性进行比较,以表明标准分解模型中的尺寸分布模型可以通过一些简单的修改和尺寸-面积转换模型应用于灾难性的低速碰撞中在标准解体模型中可以应用灾难性的低速碰撞。

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