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小行星颗粒的高迁移率由陨石碎片的实测内聚力揭示。

High mobility of asteroid particles revealed by measured cohesive force of meteorite fragments.

机构信息

Department of Planetology, Kobe University, 1-1 Rokkodaicho, Nada-ku, Kobe 657-8501, Japan.

出版信息

Sci Adv. 2023 Mar 15;9(11):eadd3530. doi: 10.1126/sciadv.add3530. Epub 2023 Mar 17.

Abstract

The cohesive force of asteroid particles is a crucial parameter in microgravity. The cohesive force was evaluated under the assumptions of lunar regolith and proportionality to particle size; however, it is sensitive to particle shape. In this study, cohesive-force measurements of meteorite fragments and aggregates consisting of silica microspheres revealed that the cohesive force is independent of the sizes of the fragments and aggregates as well as of the fragment preparation methods. The cohesive forces of the asteroid particles were found to be orders of magnitude smaller than previously predicted, explaining the high mobility of asteroid surface particles identified by space exploration.

摘要

小行星颗粒的内聚力是微重力中的一个关键参数。在假设月壤和与颗粒尺寸成比例的情况下,对其进行了评估;然而,它对颗粒形状很敏感。在这项研究中,对由二氧化硅微球组成的陨石碎片和聚集体的内聚力测量表明,内聚力与碎片和聚集体的尺寸以及碎片的制备方法无关。发现小行星颗粒的内聚力小了几个数量级,这解释了太空探索中发现的小行星表面颗粒的高迁移率。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7380/10022890/af96c71d002f/sciadv.add3530-f1.jpg

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