The Generation of O2 and CO by CO2 Glow Discharge for In-Situ Martian Atmospheric Utilization

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
Maocheng Qian, Fabao Yan, Pengyan Zhang, Bo Li, Zhongchen Wu
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Abstract

Mars has nearly ideal conditions for CO2 dissociation by glow discharge plasmas. The directly generation of O2 and CO on Mars was considered to be feasible and practical for in situ resource utilization of Martian atmosphere to get respirable O2 and fuel. In this paper, we conduct several experiments under simulated Martian conditions to investigate the process and how the key parameters effect the generation of O2 and CO in CO2 glow discharge reactions. The yields of new products (i.e., O2 and CO) under various gas discharge work parameters (i.e., discharge power, frequency, voltage, gap between the discharge plane electrodes and gas pressure) were systematically investigated. The reaction mechanism and reaction path of CO2 glow discharge has been discussed. In our study the max yield of O2 by CO2 discharge dissociation was got about 21.8 g/h at 168 W which is very close to that of NASA MOXIE (Mars Oxygen In-Situ Resource Utilization Experiment) at the same power. Our results showed the great potentiality of glow discharge for the practicable technology of O2 and CO generation for in-situ resource utilization on Mars.

Abstract Image

利用二氧化碳辉光放电生成 O2 和 CO 以在火星大气中就地利用
摘要 火星具有近乎理想的辉光放电等离子体解离二氧化碳的条件。在火星上直接生成 O2 和 CO 被认为是对火星大气进行就地资源利用以获得可吸入 O2 和燃料的可行方法。在本文中,我们在模拟火星条件下进行了多项实验,研究二氧化碳辉光放电反应中生成 O2 和 CO 的过程以及关键参数对其的影响。系统研究了不同气体放电工作参数(即放电功率、频率、电压、放电面电极间隙和气体压力)下新产物(即 O2 和 CO)的产量。讨论了 CO2 辉光放电的反应机理和反应路径。在我们的研究中,二氧化碳放电解离产生的 O2 在 168 W 时的最大产量约为 21.8 g/h,与美国宇航局 MOXIE(火星氧原地资源利用实验)在相同功率下的产量非常接近。我们的研究结果表明,辉光放电在火星原地资源利用的氧气和一氧化碳生成实用技术方面具有巨大潜力。
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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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