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Nanoindenting the Chelyabinsk meteorite to learn about impact deflection effects in asteroids

机译:对车里雅宾斯克陨石进行纳米压痕以了解小行星的撞击偏转效应

摘要

The Chelyabinsk meteorite is a highly shocked, low porosity, ordinary chondrite, probably similar to S- or Q-type asteroids. Therefore, nanoindentation experiments on this meteorite allow us to obtain key data to understand the physical properties of near-Earth asteroids (NEAs). Tests at different length scales provide information about the local mechanical properties of the minerals forming this meteorite: reduced Young’s modulus, hardness, elastic recovery, and fracture toughness. Those tests are also useful to understand the potential to deflect threatening asteroids using a kinetic projectile. We found that the differences in mechanical properties between regions of the meteorite, which increase or reduce the efficiency of impacts, are not a result of compositional differences. A low mean particle size, attributed to repetitive shock, can increase hardness, while low porosity promotes a higher momentum multiplication. Momentum multiplication is the ratio between the change in momentum of a target due to an impact, and the momentum of the projectile, and therefore higher values imply more efficient impacts. In the Chelyabinsk meteorite the properties of the light-colored lithology materials facilitate obtaining higher momentum multiplication values, compared to the other regions described for this meteorite. Also, we found a low value of fracture toughness in the shock-melt veins of Chelyabinsk, which would promote the ejection of material after an impact and therefore increase the momentum multiplication. These results are relevant in the context of a future mission to test asteroid deflection, currently being studied by ESA and NASA: the Asteroid Impact and Deflection Assessment (AIDA) mission.
机译:车里雅宾斯克陨石是高度震动,低孔隙率的普通球粒陨石,可能类似于S型或Q型小行星。因此,在该陨石上进行的纳米压痕实验使我们能够获得关键数据,以了解近地小行星(NEA)的物理性质。在不同的长度尺度上进行的测试可提供有关形成这种陨石的矿物的局部机械性能的信息:降低的杨氏模量,硬度,弹性恢复和断裂韧性。这些测试对于了解使用动能射弹偏转威胁小行星的潜力也很有用。我们发现,陨石区域之间机械性能的差异(增加或降低撞击效率)不是组成差异的结果。较低的平均粒径(由于重复的冲击)可增加硬度,而较低的孔隙度则可促进较高的动量倍增。动量倍增是目标由于撞击而产生的动量变化与射弹的动量之间的比率,因此,较高的值表示更有效的撞击。与针对该陨石描述的其他区域相比,在车里雅宾斯克陨石中,浅色岩性材料的特性有助于获得更高的动量倍增值。此外,我们在车里雅宾斯克的冲击熔炼静脉中发现了较低的断裂韧性值,这会促进撞击后物料的弹出,从而增加动量倍增。这些结果与未来测试小行星挠度的任务相关,ESA和NASA目前正在研究该任务:小行星撞击和挠度评估(AIDA)任务。

著录项

  • 作者

    Moyano-Cambero Carles E.;

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  • 年度 2017
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  • 原文格式 PDF
  • 正文语种 eng
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