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高氯酸盐耦合一氧化碳(CO)氧化:火星盐水中可能存在微生物介导反应的证据。

Perchlorate-Coupled Carbon Monoxide (CO) Oxidation: Evidence for a Plausible Microbe-Mediated Reaction in Martian Brines.

作者信息

Myers Marisa R, King Gary M

机构信息

Department of Biological Sciences, Louisiana State University, Baton Rouge, LA, United States.

出版信息

Front Microbiol. 2017 Dec 22;8:2571. doi: 10.3389/fmicb.2017.02571. eCollection 2017.

DOI:10.3389/fmicb.2017.02571
PMID:29312249
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5743682/
Abstract

The presence of hydrated salts on Mars indicates that some regions of its surface might be habitable if suitable metabolizable substrates are available. However, several lines of evidence have shown that Mars' regolith contains only trace levels of the organic matter needed to support heterotrophic microbes. Due to the scarcity of organic carbon, carbon monoxide (CO) at a concentration of about 700 parts per million (about 0.4 Pa) might be the single most abundant readily available substrate that could support near-surface bacterial activity. Although a variety of electron acceptors can be coupled to CO oxidation, perchlorate is likely the most abundant potential oxidant in Mars' brines. Whether perchlorate, a potent chaotrope, can support microbial CO oxidation has not been previously documented. We report here the first evidence for perchlorate-coupled CO oxidation based on assays with two distinct euryarchaeal extreme halophiles. CO oxidation occurred readily in 3.8 M NaCl brines with perchlorate concentrations from 0.01 to 1 M. Both isolates were able to couple CO with perchlorate or chlorate under anaerobic conditions with or without nitrate as an inducer for nitrate reductase, which serves as a perchlorate reductase in extreme halophiles. In the presence of perchlorate, CO concentrations were reduced to levels well below those found in Mars' atmosphere. This indicates that CO could contribute to the survival of microbial populations in hydrated salt formations or brines if water activities are suitably permissive.

摘要

火星上存在水合盐表明,如果有合适的可代谢底物,其表面的一些区域可能适合居住。然而,一系列证据表明,火星的风化层仅含有痕量水平的支持异养微生物所需的有机物质。由于有机碳稀缺,浓度约为百万分之700(约0.4帕斯卡)的一氧化碳(CO)可能是能够支持近地表细菌活动的最丰富的现成底物。尽管多种电子受体可以与CO氧化偶联,但高氯酸盐可能是火星盐水中最丰富的潜在氧化剂。高氯酸盐这种强效离液剂是否能够支持微生物的CO氧化,此前尚无文献记载。我们在此报告基于对两种不同的广古菌极端嗜盐菌的检测得出的高氯酸盐偶联CO氧化的首个证据。在高氯酸盐浓度为0.01至1 M的3.8 M NaCl盐水中,CO氧化很容易发生。在有无硝酸盐作为硝酸盐还原酶诱导剂(在极端嗜盐菌中作为高氯酸盐还原酶)的厌氧条件下,两种分离株都能够将CO与高氯酸盐或氯酸盐偶联。在存在高氯酸盐的情况下,CO浓度降低到远低于火星大气中发现的水平。这表明,如果水活度适宜,CO可能有助于水合盐形成物或盐水中微生物种群的存活。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/d26694abaec8/fmicb-08-02571-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/f5b17cd6d900/fmicb-08-02571-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/1dd86305836e/fmicb-08-02571-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/0ac4e0699531/fmicb-08-02571-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/d26694abaec8/fmicb-08-02571-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/f5b17cd6d900/fmicb-08-02571-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/1dd86305836e/fmicb-08-02571-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/0ac4e0699531/fmicb-08-02571-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2e7a/5743682/d26694abaec8/fmicb-08-02571-g004.jpg

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