The Relative Effects of Surface and Subsurface Morphology on the Deflection Efficiency of Kinetic Impactors: Implications for the DART Mission

M. DeCoster, R. Luther, Gareth S. Collins, Kaiyi Dai, T. Davison, D. Graninger, Felix Kaufmann, E. Rainey, A. Stickle
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Abstract

The Double Asteroid Redirection Test (DART) mission impacted Dimorphos, the moonlet of the binary asteroid 65803 Didymos, on 2022 September 26 and successfully tested a kinetic impactor as an asteroid deflection technique. The success of the deflection was partly due to the momentum of the excavated ejecta material, which provided an extra push to change Dimorphos’s orbital period. Preimpact images provided constraints on the surface but not the subsurface morphology of Dimorphos. DART observations indicated that Dimorphos contained a boulder-strewn surface, with an impact site located between a cluster of large surface boulders. In order to better understand the momentum enhancement factor (β) resulting from the impact, we performed impact simulations into two types of targets: idealized homogeneous targets with a single boulder of varying size and buried depth at the impact site and an assembly of boulders at the impact site with subsurface layers. We investigated the relative effects of surface morphology to subsurface morphology to put constraints on the modeling phase space for DART following impact. We found that surface features created a 30%–96% armoring effect on β, with large surface boulders measuring on the order of the spacecraft bus creating the largest effect. Subsurface effects were more subtle (3%–23%) and resulted in an antiarmoring effect on β, even when layers/boulders were close to the surface. We also compared our 2D axisymmetric models to a 3D rectilinear model to understand the effects of grid geometry and dimension on deflection efficiency computational results.
表面和次表面形态对动能撞击器偏转效率的相对影响:对 DART 任务的影响
双小行星改向试验(DART)任务于2022年9月26日撞击了双小行星65803 Didymos的小卫星Dimorphos,并成功测试了作为小行星偏转技术的动能撞击器。偏转的成功部分归功于挖掘出的喷出物质的动量,它提供了额外的推动力,改变了迪莫非斯的轨道周期。撞击前的图像提供了迪莫弗斯表面的制约因素,但没有提供其地下形态的制约因素。DART 观测结果表明,Dimorphos 包含一个巨石遍布的表面,撞击点位于表面大石块群之间。为了更好地了解撞击产生的动量增强因子(β),我们对两种类型的目标进行了撞击模拟:一种是理想化的均质目标,在撞击点有大小和埋藏深度不同的单块巨石;另一种是在撞击点的巨石集合体,带有地表下层。我们研究了表面形态与地下形态的相对影响,以对撞击后的 DART 建模阶段空间施加限制。我们发现,地表特征对 β 产生了 30%-96% 的铠装效应,与航天器总线大小相当的大型地表巨石产生的效应最大。地表下的影响更为微妙(3%-23%),即使地层/巨石靠近地表,也会对β产生反铠装效应。我们还将二维轴对称模型与三维直线模型进行了比较,以了解网格几何形状和尺寸对变形效率计算结果的影响。
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