用颗粒穿透仪测量小体风化层的机械性能

IF 2.7 1区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Bin Cheng, Erik Asphaug, Yang Yu, Hexi Baoyin
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引用次数: 3

摘要

众所周知,太阳系中的小天体被一层松散的未固结土壤覆盖,这些土壤由沙粒和崎岖的巨石组成。自这些风化层形成以来,各种地球物理过程对其进行了改造。因此,风化层覆盖表面上的地貌为重建发生在小体上的地质过程提供了重要线索。然而,小体风化层的机械强度仍不清楚,这是了解其动态演化的重要参数。此外,风化层的力学特性是设计和操作与小物体表面相互作用的空间任务的关键因素。颗粒穿透仪是一种便于对表面/地下材料进行原位力学表征的仪器,引起了人们的极大关注。然而,我们仍然没有完全了解与颗粒风化层相关的穿透动力学,部分原因是在微重力下测量粒度响应的实验困难,特别是在小体动力学的较长时间尺度上。在这项研究中,我们通过基于软球离散元模型的大规模数值模拟分析了移动机器人对颗粒物质的缓慢侵入。我们证明了无黏性风化层的阻力在接触后随着渗透深度的增加而突然增加,然后过渡到线性状态。稳态分量的比例因子大致与颗粒材料的内摩擦成正比,这使得我们可以通过测量它们的力-深度关系来推断行星土的抗剪强度。当考虑内聚时,由于内聚材料的脆性行为,阻力分布在大侵彻深度处表现为稳态。代表颗粒材料破坏阈值的饱和阻力随风化层内聚强度的增大而增大。这种正相关性为测量小体着陆任务中颗粒风化层的抗拉强度提供了可靠的工具。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Measuring the mechanical properties of small body regolith layers using a granular penetrometer

Small bodies in the solar system are known to be covered by a layer of loose unconsolidated soil composed of grains ranging from dusty sands to rugged boulders. Various geophysical processes have modified these regolith layers since their origin. Therefore, the landforms on regolith-blanketed surfaces hold vital clues for reconstructing the geological processes occurring on small bodies. However, the mechanical strength of small body regolith remains unclear, which is an important parameter for understanding its dynamic evolution. Furthermore, regolith mechanical properties are key factors for the design and operation of space missions that interact with small body surfaces. The granular penetrometer, which is an instrument that facilitates in situ mechanical characterization of surface/subsurface materials, has attracted significant attention. However, we still do not fully understand the penetration dynamics related to granular regolith, partially because of the experimental difficulties in measuring grain-scale responses under microgravity, particularly on the longer timescales of small body dynamics. In this study, we analyzed the slow intrusion of a locomotor into granular matter through large-scale numerical simulations based on a soft sphere discrete element model. We demonstrated that the resistance force of cohesionless regolith increases abruptly with penetration depth after contact and then transitions to a linear regime. The scale factor of the steady-state component is roughly proportional to the internal friction of the granular materials, which allows us to deduce the shear strength of planetary soils by measuring their force-depth relationships. When cohesion is included, due to the brittle behavior of cohesive materials, the resistance profile is characterized by a stationary state at a large penetration depth. The saturation resistance, which represents the failure threshold of granular materials, increases with the cohesion strength of the regolith. This positive correlation provides a reliable tool for measuring the tensile strength of granular regolith in small body touchdown missions.

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来源期刊
Astrodynamics
Astrodynamics Engineering-Aerospace Engineering
CiteScore
6.90
自引率
34.40%
发文量
32
期刊介绍: Astrodynamics is a peer-reviewed international journal that is co-published by Tsinghua University Press and Springer. The high-quality peer-reviewed articles of original research, comprehensive review, mission accomplishments, and technical comments in all fields of astrodynamics will be given priorities for publication. In addition, related research in astronomy and astrophysics that takes advantages of the analytical and computational methods of astrodynamics is also welcome. Astrodynamics would like to invite all of the astrodynamics specialists to submit their research articles to this new journal. Currently, the scope of the journal includes, but is not limited to:Fundamental orbital dynamicsSpacecraft trajectory optimization and space mission designOrbit determination and prediction, autonomous orbital navigationSpacecraft attitude determination, control, and dynamicsGuidance and control of spacecraft and space robotsSpacecraft constellation design and formation flyingModelling, analysis, and optimization of innovative space systemsNovel concepts for space engineering and interdisciplinary applicationsThe effort of the Editorial Board will be ensuring the journal to publish novel researches that advance the field, and will provide authors with a productive, fair, and timely review experience. It is our sincere hope that all researchers in the field of astrodynamics will eagerly access this journal, Astrodynamics, as either authors or readers, making it an illustrious journal that will shape our future space explorations and discoveries.
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