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代谢过程在铁氧化微生物中作为生物特征得以保留:对火星生物特征探测的启示。

Metabolic Processes Preserved as Biosignatures in Iron-Oxidizing Microorganisms: Implications for Biosignature Detection on Mars.

机构信息

1 NASA Goddard Space Flight Center , Greenbelt, Maryland.

2 Department of Physics, Astronomy, and Geosciences, Towson University , Towson, Maryland.

出版信息

Astrobiology. 2019 Jan;19(1):40-52. doi: 10.1089/ast.2017.1745. Epub 2018 Jul 25.

Abstract

Iron-oxidizing bacteria occupy a distinct environmental niche. These chemolithoautotrophic organisms require very little oxygen (when neutrophilic) or outcompete oxygen for access to Fe(II) (when acidophilic). The utilization of Fe(II) as an electron donor makes them strong analog organisms for any potential life that could be found on Mars. Despite their importance to the elucidation of early life on, and potentially beyond, Earth, many details of their metabolism remain unknown. By using on-line thermochemolysis and gas chromatography-mass spectrometry (GC-MS), a distinct signal for a low-molecular-weight molecule was discovered in multiple iron-oxidizing isolates as well as several iron-dominated environmental samples, from freshwater and marine environments and in both modern and older iron rock samples. This GC-MS signal was neither detected in organisms that did not use Fe(II) as an electron donor nor present in iron mats in which organic carbon was destroyed by heating. Mass spectral analysis indicates that the molecule bears the hallmarks of a pterin-bearing molecule. Genomic analysis has previously identified a molybdopterin that could be part of the electron transport chain in a number of lithotrophic iron-oxidizing bacteria, suggesting one possible source for this signal is the pterin component of this protein. The rock samples indicate the possibility that the molecule can be preserved within lithified sedimentary rocks. The specificity of the signal to organisms requiring iron in their metabolism makes this a novel biosignature with which to investigate both the evolution of life on ancient Earth and potential life on Mars.

摘要

铁氧化细菌占据独特的环境生态位。这些化能自养生物对氧气的需求量非常低(当为中性菌时),或者在竞争铁(II)时会优先消耗氧气(当为嗜酸菌时)。利用 Fe(II) 作为电子供体,它们成为了在火星上可能存在的任何潜在生命的有力模拟生物。尽管它们对阐明地球早期生命以及潜在的地球外生命非常重要,但它们的许多代谢细节仍然未知。通过使用在线热化学分解和气相色谱-质谱联用 (GC-MS),在多个铁氧化菌分离物以及来自淡水和海洋环境的多个铁主导环境样本中,都发现了一种低分子量分子的独特信号,这些样本包括现代和古老的铁岩石样本。在不将 Fe(II) 用作电子供体的生物体中,以及在加热破坏有机碳的铁垫中,均未检测到这种 GC-MS 信号。质谱分析表明,该分子具有蝶呤分子的特征。基因组分析先前已经鉴定出一种钼蝶呤,它可能是许多化能自养铁氧化细菌电子传递链的一部分,这表明该信号的一个可能来源是该蛋白质的蝶呤成分。岩石样本表明,该分子有可能在石化的沉积岩中得到保存。该信号对代谢过程中需要铁的生物体具有特异性,这使其成为一种新的生物特征,可以用来研究古代地球上生命的演化以及火星上潜在的生命。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c80/6338579/b2b2dba7b764/fig-1.jpg

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