Slag chemistry on the Moon

The Australasian Institute of Mining and Metallurgy
S P. Singh G A. Brooks M G. Shaw B Eisenbart A R. Duffy M A. Rhamdhani A K. Shukla
Organization:
The Australasian Institute of Mining and Metallurgy
Pages:
12
File Size:
3743 KB
Publication Date:
Aug 21, 2024

Abstract

The field of astrometallurgy is a growing area of study. Metal production on the Moon is likely to begin in less than a decade as major space agencies such as NASA (National Aeronautics and Space Administration) and CNSA (China National Space Administration) are preparing to construct permanent lunar bases. The utilisation of regolith to generate oxygen and metals is expected to be important in the development of a sustainable lunar habitat. This paper provides an overview of potential metallurgical processing methods for lunar conditions, emphasising the impact of lunar factors on slag chemistry. The interaction between regolith and the extracted metals, as well as their impact on slag composition and refractory performance, are critical considerations in metal production on the lunar surface. The initial research on lunar metallurgical technologies is focused on oxygen extraction and Fe-Si alloys are reported as the by-products of these processes. This paper delves into the fundamental thermodynamics associated with the carbothermic reduction of lunar regolith. Thermodynamic analysis using the FactSage™ ver 8.2 software package indicates that the Fe-Si alloy can be produced as a metallic product from the lunar regolith at temperatures ranging from 1400°C to 1600°C under terrestrial conditions. However, under ultra-high vacuum conditions (3 × 10-15 bar) on the Moon, the required operating temperature for producing ferrosilicon would be significantly reduced. Thermodynamic modelling results indicate that under lunar vacuum conditions, Fe-Si alloys only exist as solid phases at lower temperatures below 650°C. At higher temperatures, both Fe and Si are expected to be present in the gas phase. In this work, the carbothermic reduction of the Lunar Mare Simulant (LMS-1) is conducted under terrestrial conditions. The findings indicate that the process can readily yield Fe-Si alloys with 7–10 wt per cent Si at 1600°C. Additionally, energy dispersive spectroscopy (EDS) analysis of the resulting Fe-Si alloy indicates the presence of phosphorus up to 1 wt per cent.
Citation

APA: S P. Singh G A. Brooks M G. Shaw B Eisenbart A R. Duffy M A. Rhamdhani A K. Shukla  (2024)  Slag chemistry on the Moon

MLA: S P. Singh G A. Brooks M G. Shaw B Eisenbart A R. Duffy M A. Rhamdhani A K. Shukla Slag chemistry on the Moon. The Australasian Institute of Mining and Metallurgy, 2024.

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