重力减弱情况下的电解建模:利用月球及月球以外的原地资源生产氧气

Paul A. Burke, Michael Nord, Charles Hibbitts, J. Berdis
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引用次数: 0

摘要

熔融沉积物电解作为一种原地资源利用(ISRU)技术,有可能在月球表面生产氧气和金属合金,为双月和最终的火星空间探索打开新的大门。本研究对电解气泡的形成、增长、脱离和上升的基本物理学原理进行了研究。为此,开发并运行了计算流体动力学(CFD)模型,模拟水电解、熔盐电解(MSE)和熔融月球流石(MRE)在多个重力降低水平上的电解过程。结果表明,重力降低、电极表面粗糙度(可能是由于表面降解造成的)、流体特性和电极方向都会影响电解效率,甚至可能通过延迟气泡脱离而阻碍电解。在设计和运行重力降低的电解系统时,必须考虑到这项研究的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Modeling electrolysis in reduced gravity: producing oxygen from in-situ resources at the moon and beyond
Molten Regolith Electrolysis, as an in situ resource utilization (ISRU) technology, has the potential to enable the production of oxygen and metallic alloys on the Lunar surface; opening new doors in Cis-Lunar, and eventually Martian space exploration. This research studies the fundamental physics which govern the formation, growth, detachment, and rise of electrolytic bubbles. To this end, computational fluid dynamic (CFD) models were developed and run, to simulate water electrolysis, molten salt electrolysis (MSE), and molten Lunar regolith (MRE) electrolysis across multiple reduced gravity levels. The results demonstrate that reduced gravity, electrode surface roughness (possibly due to surface degradation), fluid properties, and electrode orientation can all affect electrolytic efficiency and possibly even stall electrolysis by delaying bubble detachment. The findings of this research must be considered when designing and operating electrolysis systems at reduced gravity levels.
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