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Extraction of Water from the Martian Atmosphere

机译:从火星大气中提取水

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We report on experiments to validate a concept for extracting water vapor from the Martian atmosphere byrnadsorption. The adsorber investigated is zeolite 3A, a synthetic molecular sieve that has a cage-like microstructurernwith an effective aperture of 3A. This micropore size allows water molecules to enter but excludes carbon dioxidernmolecules, which comprise 95% of the Martian atmosphere. Although the literature on zeolites is extensive, there isrnlittle information available on type 3A zeolite at Mars ambient conditions, i.e., temperatures of ~ 150-250 K and waterrnvapor pressures ranging from ~10~3 Pa to ~1 Pa. To obtain the desired adsorption data we developed a continuous flowrnMars environmental simulation facility capable of precisely generating and controlling for long durations the desiredrnpressures, temperatures, and humidities. The experiments conducted to date have produced measurements of thernmagnitudes and trends of the uptake kinetics and equilibrium capacity of a small-scale packed bed of zeolite 3A atrnconditions approaching those on Mars. Although the data obtained to date are preliminary, they show that zeolite 3A isrncapable of capturing significant quantities of water vapor at these conditions.
机译:我们报告实验以验证通过吸附从火星大气中提取水蒸气的概念。研究的吸附剂是3A沸石,这是一种合成分子筛,具有笼状微结构,有效孔径为3A。该微孔尺寸允许水分子进入,但不包括占火星大气95%的二氧化碳分子。尽管关于沸石的文献广泛,但在火星环境条件下,即3A型沸石的温度(150〜250 K,水蒸气压力范围从〜10〜3 Pa至〜1 Pa)的信息很少。要获得所需的吸附根据数据,我们开发了一个连续的FlowMars火星环境模拟设施,该设施能够长时间精确地生成和控制所需的压力,温度和湿度。迄今为止进行的实验已经测量了在接近火星条件下的小型3A沸石填充床的吸收动力学和平衡能力的幅值和趋势。尽管迄今为止获得的数据是初步的,但它们表明,在这些条件下,沸石3A不能捕获大量的水蒸气。

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