Synthesizing lunar regolith-geopolymer emulating lunar positive temperature regime

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Planetary and Space Science Pub Date : 2024-03-16 DOI:10.1016/j.pss.2024.105890
Usman Javed , Faiz Uddin Ahmed Shaikh , A.K.M. Samsur Rahman
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Abstract

The development of lunar habitat using lunar regolith is a captivating research area for constructing lunar bases, especially after the discovery of polar ice, and molecular water on the lunar south pole. The aim of this research is to synthesize a robust lunar regolith geopolymer by fine-tuning the concentration and ratios of alkaline activators while implementing curing under lunar positive thermal regime. The geopolymer was synthesized containing lunar highlands simulant (LHS-1) and mare regolith simulant (LMS-1) at the lowest water content using sodium (Na) and potassium (K) based alkaline activators emulating positive temperature regime collected by Diviner Lunar Radiometer Experiment (DLRE). The maximum compressive strength of 41.23 MPa was achieved for highlands regolith simulant-based geopolymer containing a Na-activator with the lowest water-to-precursor ratio of 0.23. The surplus alkali cations in the geopolymer paste matrix resulted in the formation of carbonation products after reacting with atmospheric carbon dioxide. K-activator geopolymer resulted in Kalicinite which has lower thermal stability and dissolution in water, whereas sodium carbonate formed in Na-activator-based geopolymer engrained and embedded precursor particles alongside sodium-calcium aluminosilicate hydrate (N-(C)-A-S-H) gel forming more densified microstructure. Conclusively, lunar regolith geopolymer has the potential for the construction of lunar habitat. However, this study recommends synthesizing geopolymer in vacuum conditions, emulating freeze-thaw cycles for a more precise estimation of microstructural developments and evaluating other critical properties.

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合成模拟月球正温度机制的月球碎屑-地聚合物
特别是在月球南极发现极地冰和分子水之后,利用月球残积岩开发月球栖息地是建设月球基地的一个令人瞩目的研究领域。本研究的目的是通过微调碱性活化剂的浓度和比例,合成一种坚固的月球残积岩土工聚合物,同时在月球正热环境下进行固化。研究人员使用钠(Na)和钾(K)碱性活化剂,模拟 "占卜者月球辐射计实验"(DLRE)收集到的正温度机制,合成了含水量最低的月球高地模拟物(LHS-1)和马雷雷砾岩模拟物(LMS-1)的土工聚合物。高原碎屑模拟岩基土工聚合物的抗压强度最大,达到 41.23 兆帕,其中含有最低水-前体比为 0.23 的钠基活化剂。土工聚合物浆料基质中过剩的碱阳离子与大气中的二氧化碳反应后形成了碳化产物。K-activator 土工聚合物形成了热稳定性较低且易溶于水的加里硅质(Kalicinite),而 Na-activator 土工聚合物中形成的碳酸钠与钠钙铝硅酸盐水合物(N-(C)-A-S-H)凝胶一起啮合并嵌入前体颗粒,形成了更致密的微观结构。最后,月球碎屑土工聚合物具有建造月球栖息地的潜力。不过,本研究建议在真空条件下合成土工聚合物,模拟冻融循环以更精确地估计微观结构的发展,并评估其他关键性能。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
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
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