Dust Mitigation Strategies Enabling Moon Exploration Missions

Guido Saccone, Nunzia Favaloro
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Abstract

Micrometric dust particles of lunar regolith represent one of the most serious issues of the harsh Moon environment. Indeed, the extremely high vacuum conditions expose the lunar soil minerals to intense ultraviolet and galactic cosmic rays’ bombardment during the Moon’s daylight producing photoionization of the constituent’s atoms and electron release. Moreover, the Moon periodically interacts with the surrounding solar wind which generates a continuous flux of charged particles accompanied by electric fields around the terminator region able to lift off the lunar regolith dust up to ~100 km above the geometrical surface. In this way, micrometric granular matter forms a subtle veil of contaminants. This electrically charged and extremely adhering dust environment not only can cause various critical drawbacks to several robotic parts, e.g., mechanical components, electronic devices, solar panels, thermal radiators, rover seals and bearings, etc. but also can dramatically damage the respiratory systems of humans if accidentally inhaled. For these reasons, lunar dust was recognized, by several agencies including NASA and ESA, as one of the main hazards for the ongoing robotic and manned exploration and colonization of our natural satellite. To overcome or at least mitigate these issues, several technologies were developed and assessed ranging from the active ones requiring a source of energy, e.g., mechanical, fluidal, and, above all, electric devices, to the passive technologies involving suitable material design and development. The work here reported presents several possible active and passive chemical and physical strategies for protecting sensitive surfaces of space systems against granular contamination. This paper is intended as a survey of dust mitigation issues and technical mitigation with the approach pursued by the Italian Aerospace Research Centre (CIRA) related to a hybrid technique with an innovative material. The strategy that is under implementation by CIRA is based on the combination of active and passive techniques and consists of the design and development of innovative high-performance polymers exhibiting simultaneously outstanding thermo-mechanical properties and superior non-sticking capacity, i.e., abhesion.

促进月球探测任务的减尘战略
月球风化层的微尘粒子代表了严酷的月球环境中最严重的问题之一。事实上,在月球的日光下,极高的真空条件使月球土壤矿物质暴露在强烈的紫外线和银河宇宙射线的轰击下,产生了组成原子的光电离和电子释放。此外,月球周期性地与周围的太阳风相互作用,产生带电粒子的连续通量,并伴随着在终端区域周围的电场,能够将月球风化层尘埃提升到几何表面以上约100公里处。通过这种方式,微米颗粒物质形成了污染物的微妙面纱。这种带电且极具粘性的粉尘环境不仅会对机器人的几个部件造成各种严重的缺陷,例如机械部件、电子设备、太阳能电池板、热辐射器、漫游车密封件和轴承等,而且如果不小心吸入,还会严重损害人类的呼吸系统。由于这些原因,包括美国宇航局和欧洲航天局在内的几个机构认为,月球尘埃是正在进行的机器人和载人探索和殖民我们自然卫星的主要危害之一。为了克服或至少减轻这些问题,开发和评估了几种技术,从需要能源的主动技术,例如机械、流体和最重要的电力设备,到涉及合适材料设计和开发的被动技术。这里报告的工作提出了几种可能的主动和被动的化学和物理策略,以保护空间系统的敏感表面免受颗粒污染。本文旨在对意大利航空航天研究中心(CIRA)采用的与创新材料混合技术相关的方法进行粉尘缓解问题和技术缓解的调查。CIRA正在实施的策略是基于主动和被动技术的结合,包括设计和开发创新的高性能聚合物,同时表现出出色的热机械性能和卓越的不粘着能力,即附着力。
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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