Alice Dottori , Ivan Troisi , Michèle Roberta Lavagna
{"title":"Demonstration of the low-temperature carbothermal process for producing oxygen from lunar regolith: Terrestrial test campaign","authors":"Alice Dottori , Ivan Troisi , Michèle Roberta Lavagna","doi":"10.1016/j.pss.2025.106154","DOIUrl":null,"url":null,"abstract":"<div><div>The solid-gas carbothermal reduction is one of the processes available for extracting oxygen from the lunar regolith, a crucial capability for supporting lunar exploration and establishing a sustainable human presence on the Moon’s surface. This article presents the findings of the experimental campaign conducted at the Politecnico di Milano, which confirmed the feasibility of the process. Water is extracted from dry regolith, and the production of carbon oxides is monitored to gather data on the process. The campaign studied the influence of various parameters to enhance water and oxygen production, including reaction temperatures, regolith granularity and mass, solid-to-gas ratio, processing duration, and others. The extracted water is collected in a condensation stage, while the evolution of the gaseous mixture is monitored using gas chromatography, and the exhaust batch of simulant is analysed through SEM and XRD. These analyses provided qualitative and quantitative assessments of the reaction’s effectiveness, yielding important information about the impact of changing parameters. The study concludes by proposing a set of process parameters to serve as a baseline for future implementation of the low-temperature carbothermal process on the lunar surface.</div></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"266 ","pages":"Article 106154"},"PeriodicalIF":1.8000,"publicationDate":"2025-06-30","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/S0032063325001217","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
The solid-gas carbothermal reduction is one of the processes available for extracting oxygen from the lunar regolith, a crucial capability for supporting lunar exploration and establishing a sustainable human presence on the Moon’s surface. This article presents the findings of the experimental campaign conducted at the Politecnico di Milano, which confirmed the feasibility of the process. Water is extracted from dry regolith, and the production of carbon oxides is monitored to gather data on the process. The campaign studied the influence of various parameters to enhance water and oxygen production, including reaction temperatures, regolith granularity and mass, solid-to-gas ratio, processing duration, and others. The extracted water is collected in a condensation stage, while the evolution of the gaseous mixture is monitored using gas chromatography, and the exhaust batch of simulant is analysed through SEM and XRD. These analyses provided qualitative and quantitative assessments of the reaction’s effectiveness, yielding important information about the impact of changing parameters. The study concludes by proposing a set of process parameters to serve as a baseline for future implementation of the low-temperature carbothermal process on the lunar surface.
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