等离子体
离解(化学)
火星人
远程等离子体
材料科学
火星探测计划
纳米技术
化学
环境科学
天体生物学
化学气相沉积
物理
有机化学
量子力学
作者
Vasco Guerra,Tiago Silva,Nuno R. Pinhão,Olivier Guaitella,Carmen Guerra-Garcia,Floran J. J. Peeters,Mihalis N. Tsampas,M. C. M. van de Sanden
摘要
This work discusses the potential of combining non-thermal plasmas and conducting membranes for in situ resource utilization (ISRU) on Mars. By converting different molecules directly from the Martian atmosphere, plasmas can create the necessary feed-stock and base chemicals for processing fuels, breathing oxygen, building materials, and fertilizers. Different plasma sources operate according to different principles and are associated with distinct dominant physicochemical mechanisms. This diversity allows exploring different energy transfer pathways leading to CO2 dissociation, including direct electron-impact processes, plasma chemistry mediated by vibrationally and electronically excited states, and thermally driven dissociation. The coupling of plasmas with membranes is still a technology under development, but a synergistic effect between plasma decomposition and oxygen permeation across conducting membranes is anticipated. The emerging technology is versatile, scalable, and has the potential to deliver high rates of production of molecules per kilogram of instrumentation sent to space. Therefore, it will likely play a very relevant role in future ISRU strategies.
科研通智能强力驱动
Strongly Powered by AbleSci AI