Lunar simulant behaviour variability and implications on terrestrial based lunar testing

IF 2.5 2区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
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Abstract

The detrimental effects and challenges of Lunar dust for Lunar exploitation were first identified during the Apollo missions. During the extra vehicle activities (EVAs) undertaken by astronauts, the dust clogged mechanisms, disrupted sensors, and caused several health issues for the astronauts. Despite numerous studies, there is no definite understanding as to why different Apollo missions experienced varying levels of dust disruptions. The variations in dust behaviour could be attributed to the amount of radiation the Lunar soil is exposed to, as well as mineralogy and particle sizes. To enhance our understanding of Lunar dust behaviour this study investigated Space Recourse Technologies, formally known as Exolith, simulant at different mineral compositions, and their surface detachment characteristics were measured. Experiments measuring the individual minerals and their mixed simulant-like counterparts were conducted using electrostatic fields. Inclusive to this, non-dried and dried samples were compared by measuring adhesion to target plates when subject to electrostatic forces. The results found that Highlands simulant exhibited a higher buildup on a target plate than its Mare counterpart by an average of 33% under the same conditions, likely due to particle size differences. In addition to these findings, evidence of particle reactivity decay was observed under repeated tests with up to 60% less Mare simulant and 36% Highlands deposition being measured compared to the first set of experiments. A possible explanation may be particle reactivity. Microscope images identified that particles are transported in groups as opposed to individual grains. These results will help researchers in tailoring dust mitigation solutions based on different regions on the Lunar surface and influence mission planning from the perspective of dust mitigation and contamination.

月球模拟物的行为变化及其对陆基月球测试的影响
月球尘埃对月球开发的不利影响和挑战是在阿波罗任务期间首次发现的。在宇航员进行飞行器外活动(EVA)期间,尘埃堵塞了机械装置,干扰了传感器,并给宇航员造成了一些健康问题。尽管进行了大量研究,但对于为什么不同的阿波罗任务会出现不同程度的灰尘干扰,目前还没有明确的认识。尘埃行为的变化可归因于月球土壤受到的辐射量以及矿物学和颗粒大小。为了加深我们对月球尘埃行为的了解,这项研究调查了不同矿物成分的太空追索技术模拟物(正式名称为外层岩石),并测量了它们的表面脱离特性。使用静电场对单个矿物及其混合模拟物进行了测量。此外,还通过测量样品在静电力作用下与目标板的附着力,对未干燥样品和干燥样品进行了比较。结果发现,在相同条件下,高地模拟物在靶板上的附着力比其马雷对应物平均高出 33%,这可能是由于颗粒大小不同造成的。除了这些发现之外,在重复测试中还观察到了颗粒反应性衰减的证据,与第一组实验相比,马雷模拟物的沉积量减少了 60%,高原模拟物的沉积量减少了 36%。可能的解释是颗粒的反应性。显微镜图像显示,与单个颗粒相比,颗粒是成组运输的。这些结果将有助于研究人员根据月球表面的不同区域定制尘埃减缓解决方案,并从尘埃减缓和污染的角度影响任务规划。
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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来源期刊
Icarus
Icarus 地学天文-天文与天体物理
CiteScore
6.30
自引率
18.80%
发文量
356
审稿时长
2-4 weeks
期刊介绍: Icarus is devoted to the publication of original contributions in the field of Solar System studies. Manuscripts reporting the results of new research - observational, experimental, or theoretical - concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our Solar System or extrasolar systems are welcome. The journal generally does not publish papers devoted exclusively to the Sun, the Earth, celestial mechanics, meteoritics, or astrophysics. Icarus does not publish papers that provide "improved" versions of Bode''s law, or other numerical relations, without a sound physical basis. Icarus does not publish meeting announcements or general notices. Reviews, historical papers, and manuscripts describing spacecraft instrumentation may be considered, but only with prior approval of the editor. An entire issue of the journal is occasionally devoted to a single subject, usually arising from a conference on the same topic. The language of publication is English. American or British usage is accepted, but not a mixture of these.
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