{"title":"Thermal and electrochemical properties of a mixture of lunar regolith simulant (FJS-1) and CaF2","authors":"Yuta Suzuki , Seiya Tanaka , Takuya Goto","doi":"10.1016/j.pss.2025.106177","DOIUrl":null,"url":null,"abstract":"<div><div>To establish the electrochemical reduction process of lunar regolith as an in-situ resource utilization technology on the Moon, it is crucial to prepare a high-temperature electrolytic melt that has a composition suitable for electrolysis. In this study, we propose a mixed melt consisting of lunar regolith, which comprises metal-oxide compounds, and CaF<sub>2</sub>, which can be collected from fluorapatite on the Moon's surface. To characterize the lunar regolith-CaF<sub>2</sub> system, the thermal and electrochemical properties of a mixture of a lunar mare regolith simulant (FJS-1) and CaF<sub>2</sub> were investigated. The differential thermal analysis curves measured for various compositions of FJS-1 and CaF<sub>2</sub> found that the eutectic temperature was 1275 K at FJS-1:CaF<sub>2</sub> = 90:10 wt%, which is lower than the melting point of FJS-1, 1393 K. By electrochemical impedance spectroscopic technique, the electrical resistance of the melts at 1673 K was found to be 43 Ω for the FJS-1 melt, while the mixed melt of FJS-1 and CaF<sub>2</sub> (80:20 wt%) was found to be 5 Ω. The XRD analysis of the solidified melts revealed that the mixed melts' unique physical properties were due to the formation of chemical bonding of F<sup>−</sup> ions due to CaF<sub>2</sub> and metal ions due to FJS-1. Furthermore, the electrochemical behavior of the mixed melt was investigated, demonstrating the electrodeposition of metals such as Si and Al derived from FJS-1. The reported data will provide new guidelines for designing electrolytic systems on the Moon, expanding the possibilities for controlling the temperature and electrochemical operations.</div></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"266 ","pages":"Article 106177"},"PeriodicalIF":1.8000,"publicationDate":"2025-07-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Planetary and Space Science","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0032063325001448","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
To establish the electrochemical reduction process of lunar regolith as an in-situ resource utilization technology on the Moon, it is crucial to prepare a high-temperature electrolytic melt that has a composition suitable for electrolysis. In this study, we propose a mixed melt consisting of lunar regolith, which comprises metal-oxide compounds, and CaF2, which can be collected from fluorapatite on the Moon's surface. To characterize the lunar regolith-CaF2 system, the thermal and electrochemical properties of a mixture of a lunar mare regolith simulant (FJS-1) and CaF2 were investigated. The differential thermal analysis curves measured for various compositions of FJS-1 and CaF2 found that the eutectic temperature was 1275 K at FJS-1:CaF2 = 90:10 wt%, which is lower than the melting point of FJS-1, 1393 K. By electrochemical impedance spectroscopic technique, the electrical resistance of the melts at 1673 K was found to be 43 Ω for the FJS-1 melt, while the mixed melt of FJS-1 and CaF2 (80:20 wt%) was found to be 5 Ω. The XRD analysis of the solidified melts revealed that the mixed melts' unique physical properties were due to the formation of chemical bonding of F− ions due to CaF2 and metal ions due to FJS-1. Furthermore, the electrochemical behavior of the mixed melt was investigated, demonstrating the electrodeposition of metals such as Si and Al derived from FJS-1. The reported data will provide new guidelines for designing electrolytic systems on the Moon, expanding the possibilities for controlling the temperature and electrochemical operations.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research