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Mining moon & mars with microbes: Biological approaches to extract iron from Lunar and Martian regolith

机译:利用微生物开采月球和火星:从月球和火星长石中提取铁的生物方法

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摘要

The logistical supply of terrestrial materials to space is costly and puts limitations on exploration mission scenarios. In-situ resource utilization (ISRU) can alleviate logistical requirements and thus enables sustainable exploration of space. In this paper, a novel approach to ISRU, utilizing microorganisms to extract iron from Lunar or Martian regolith, is presented. Process yields, and kinetics are used to verify the theoretical feasibility of applying four different microorganisms. Based on yields alone, three of the four organisms were not investigated further for use in biological ISRU. For the remaining organism, Shewanella oneidensis, the survivability impact of Martian regolith simulant JSC-MARS1 and Mars-abundant magnesium perchlorate were studied and found to be minimal. The payback time of the infrastructure installation needed for the process with S. oneidensis on Mars was analyzed and the sensitivity to various parameters was investigated. Water recycling efficiency and initial regolith concentration were found to be key to process performance. With a water recycling efficiency of 99.99% and initial regolith concentration of 300 g/L, leading to an iron concentration of approximately 44.7 g/L, a payback time of 3.3 years was found.
机译:向太空物流的后勤供应成本高昂,并限制了探索任务的情景。原地资源利用(ISRU)可以减轻后勤需求,从而实现空间的可持续探索。在本文中,提出了一种利用微生物从月球或火星长石中提取铁的ISRU新方法。使用过程收率和动力学来验证应用四种不同微生物的理论可行性。仅基于产量,没有进一步研究四种生物中的三种用于生物ISRU。对于剩下的生物希瓦氏菌,研究了火星重塑石模拟物JSC-MARS1和火星丰富的高氯酸镁对生存能力的影响,并发现影响很小。分析了火星沙门氏菌在火星上进行过程所需的基础设施安装的投资回收时间,并研究了对各种参数的敏感性。发现水的循环效率和初始碎屑浓度是工艺性能的关键。水的回收效率为99.99%,初始粉煤灰浓度为300 g / L,导致铁浓度约为44.7 g / L,回收期为3.3年。

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  • 来源
    《Planetary and space science》 |2020年第5期|104850.1-104850.9|共9页
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  • 作者单位

    TU Delff Dept Bionanosci Van der Maasweg 9 NL-2629 HZ Delft Netherlands;

    KTH Royal Inst Technol Dept Aeronaut & Vehicle Engn S-10044 Stockholm Sweden;

    NASA Ames Res Ctr Moffett Field CA 94035 USA;

    ESA EAC D-51147 Cologne Germany;

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