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Laser melting manufacturing of large elements of lunar regolith simulant for paving on the Moon

风化土 月球土壤 天体生物学 月母马 环境科学 材料科学 地质学 撞击坑 物理
作者
Juan-Carlos Ginés-Palomares,Miranda Fateri,Eckehard Kalhöfer,Tim Schubert,Lena Meyer,Nico Kolsch,Monika Brandić Lipińska,R. John Davenport,Barbara Imhof,René Waclavicek,Matthias Sperl,Advenit Makaya,Jens Günster
出处
期刊:Scientific Reports [Nature Portfolio]
卷期号:13 (1): 15593-15593 被引量:59
标识
DOI:10.1038/s41598-023-42008-1
摘要

Abstract The next steps for the expansion of the human presence in the solar system will be taken on the Moon. However, due to the low lunar gravity, the suspended dust generated when lunar rovers move across the lunar soil is a significant risk for lunar missions as it can affect the systems of the exploration vehicles. One solution to mitigate this problem is the construction of roads and landing pads on the Moon. In addition, to increase the sustainability of future lunar missions, in-situ resource utilization (ISRU) techniques must be developed. In this paper, the use of concentrated light for paving on the Moon by melting the lunar regolith is investigated. As a substitute of the concentrated sunlight, a high-power CO 2 laser is used in the experiments. With this set-up, a maximum laser spot diameter of 100 mm can be achieved, which translates in high thicknesses of the consolidated layers. Furthermore, the lunar regolith simulant EAC-1A is used as a substitute of the actual lunar soil. At the end of the study, large samples (approximately 250 × 250 mm) with interlocking capabilities were fabricated by melting the lunar simulant with the laser directly on the powder bed. Large areas of lunar soil can be covered with these samples and serve as roads and landing pads, decreasing the propagation of lunar dust. These manufactured samples were analysed regarding their mineralogical composition, internal structure and mechanical properties.
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