Regolith Cohesion Measurement via Induced Electrostatic Lofting

Charles Pett, Thomas J.G. Leps, C. Hartzell
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Abstract

Electrostatic dust lofting has been hypothesized to occur on airless bodies such as the Moon and asteroids, but in-situ evidence of this phenomenon has yet to be observed. Nonetheless, experiments and numerical models have provided insight into the fundamental physics of electrostatic dust mobilization. Prior to lofting, grains are bound tightly to the surface by cohesion, the dominant force for sub-mm particles. However, the magnitude of cohesion in regolith remains poorly constrained. We introduce the design of the Electrostatic Sample Collection and Cohesion Quantification (E-SACCQ) system, a technology that induces electrostatic dust lofting to measure regolith cohesion. E-SACCQ induces electrostatic lofting of charged regolith grains via a biased attractor plate and simultaneously images their size and trajectory. Since the local gravity is known and the electrostatic force on the regolith grains is controlled by the attractor plate potential, it is possible to solve for the cohesive force on the grains. Furthermore, the ability to induce electrostatic lofting may also provide a new method of dust removal from spacecraft surfaces and for sample collection on rubble pile asteroids, which may not have suitable, powdery surfaces for conventional scoop style collection methods. In this work, we discuss the preliminary design of the instrument. The feedback between the E-SACCQ electrode and the near-surface plasma environment is numerically modeled. Our models predict that solar wind bombardment will be a significant perturbation to the electric field between the surface and the electrode. The system's sensitivity to key design parameters such as attractor plate potential, size, and operating distance above the surface are also assessed. With respect to grain characterization and position tracking, stereo vision is selected as the preferred solution. Additional plasma simulation modeling and experimental demonstration is required to mature this technology.
感生静电放样法测定风化层内聚力
静电扬尘被假设发生在月球和小行星等无空气的天体上,但这种现象的现场证据尚未观察到。尽管如此,实验和数值模型已经提供了洞察静电粉尘动员的基本物理。在放样之前,颗粒通过内聚力与表面紧密结合,这是亚毫米颗粒的主要力量。然而,风化层内聚力的大小仍然没有得到很好的限制。本文介绍了静电取样和粘聚量化(E-SACCQ)系统的设计,该系统是一种利用静电粉尘放样来测量土壤粘聚力的技术。E-SACCQ通过偏压吸引板诱导带电风化粒的静电放样,同时对其大小和轨迹进行成像。由于局部重力已知,风化层颗粒上的静电力由吸引板电位控制,因此可以求解颗粒上的内聚力。此外,诱导静电放样的能力也可能提供一种从航天器表面除尘的新方法,以及在碎石堆小行星上收集样本的新方法,这些小行星可能没有适合传统勺式收集方法的粉状表面。在这项工作中,我们讨论了仪器的初步设计。对E-SACCQ电极与近表面等离子体环境之间的反馈进行了数值模拟。我们的模型预测太阳风轰击将对表面和电极之间的电场产生显著的扰动。系统对关键设计参数的敏感性,如吸引板电位、尺寸和离地面的操作距离也进行了评估。在颗粒表征和位置跟踪方面,选择立体视觉作为首选方案。进一步的等离子体模拟建模和实验证明需要成熟的技术。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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