干燥、模拟火星紫外线辐射和真空条件下嗜盐古细菌黄体的存活与萎缩芽孢杆菌的比较。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2020-12-01 Epub Date: 2020-07-02 DOI:10.1007/s11084-020-09597-7
Niloofar Feshangsaz, Farid Semsarha, Saeed Hesami Tackallou, Kamran Nazmi, Euan P Monaghan, Andreas Riedo, Jack J W A van Loon
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引用次数: 6

摘要

地外环境通过各种因素影响生物体的生物化学,包括高水平的辐射和真空、极端温度以及缺乏水和营养物质。各种各样的陆地微生物,包括那些被认为是地球上最古老的居民之一,可以应对高盐度、极端温度、干燥和高辐射。其中的关键是盐古菌,由于它们能够在高盐环境中茁壮成长,因此被认为与天体生物学研究特别相关。在这项研究中,分离自伊朗Urmia盐湖的一种新型盐古菌,Halovarius luteus菌株DA50T,暴露于不同水平的模拟地外环境中,并与萎缩芽孢杆菌进行比较。选择萎缩芽孢杆菌进行比较,是因为它对极端条件具有良好的抵抗力,并且能够产生强大的孢子结构。在没有细胞多层保护作用的情况下,制备薄膜以考察其活力。Hvr的指数后期培养。黄体和萎缩芽孢杆菌分别置于盐水和磷酸盐缓冲盐水培养基中。溶液蒸发后,将细胞包封,暴露于辐射、干燥和真空条件下,用最可能数法研究细胞暴露后的生存能力。利用高效液相色谱法和基质辅助激光解吸/电离台式反射器对真空和紫外辐射暴露后的蛋白质谱进行了研究。结果表明,Hvr对芽孢形成菌萎缩芽孢杆菌活力的影响较小。黄体在不同条件下表现出一定的生存能力。氮流下辐射通量峰值为105 J/m2时,干燥2周后,Hvr。黄体的生存能力下降最大。本研究进一步拓展了我们对恶劣空间环境中天体生物学相关生物边界条件的认识。
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Survival of the Halophilic Archaeon Halovarius luteus after Desiccation, Simulated Martian UV Radiation and Vacuum in Comparison to Bacillus atrophaeus.

Extraterrestrial environments influence the biochemistry of organisms through a variety of factors, including high levels of radiation and vacuum, temperature extremes and a lack of water and nutrients. A wide variety of terrestrial microorganisms, including those counted amongst the most ancient inhabitants of Earth, can cope with high levels of salinity, extreme temperatures, desiccation and high levels of radiation. Key among these are the haloarchaea, considered particularly relevant for astrobiological studies due to their ability to thrive in hypersaline environments. In this study, a novel haloarchaea isolated from Urmia Salt Lake, Iran, Halovarius luteus strain DA50T, was exposed to varying levels of simulated extraterrestrial conditions and compared to that of the bacteria Bacillus atrophaeus. Bacillus atrophaeus was selected for comparison due to its well-described resistance to extreme conditions and its ability to produce strong spore structures. Thin films were produced to investigate viability without the protective influence of cell multi-layers. Late exponential phase cultures of Hvr. luteus and B. atrophaeus were placed in brine and phosphate buffered saline media, respectively. The solutions were allowed to evaporate and cells were encapsulated and exposed to radiation, desiccation and vacuum conditions, and their post-exposure viability was studied by the Most Probable Number method. The protein profile using High Performance Liquid Chromatography and Matrix Assisted Laser Desorption/Ionization bench top reflector time-of-flight are explored after vacuum and UV-radiation exposure. Results showed that the change in viability of the spore-forming bacteria B. atrophaeus was only minor whereas Hvr. luteus demonstrated a range of viability under different conditions. At the peak radiation flux of 105 J/m2 under nitrogen flow and after two weeks of desiccation, Hvr. luteus demonstrated the greatest decrease in viability. This study further expands our understanding of the boundary conditions of astrobiologically relevant organisms in the harsh space environment.

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来源期刊
CiteScore
3.20
自引率
15.00%
发文量
12
审稿时长
>12 weeks
期刊介绍: The subject of the origin and early evolution of life is an inseparable part of the general discipline of Astrobiology. The journal Origins of Life and Evolution of Biospheres places special importance on the interconnection as well as the interdisciplinary nature of these fields, as is reflected in its subject coverage. While any scientific study which contributes to our understanding of the origins, evolution and distribution of life in the Universe is suitable for inclusion in the journal, some examples of important areas of interest are: prebiotic chemistry and the nature of Earth''s early environment, self-replicating and self-organizing systems, the theory of the RNA world and of other possible precursor systems, and the problem of the origin of the genetic code. Early evolution of life - as revealed by such techniques as the elucidation of biochemical pathways, molecular phylogeny, the study of Precambrian sediments and fossils and of major innovations in microbial evolution - forms a second focus. As a larger and more general context for these areas, Astrobiology refers to the origin and evolution of life in a cosmic setting, and includes interstellar chemistry, planetary atmospheres and habitable zones, the organic chemistry of comets, meteorites, asteroids and other small bodies, biological adaptation to extreme environments, life detection and related areas. Experimental papers, theoretical articles and authorative literature reviews are all appropriate forms for submission to the journal. In the coming years, Astrobiology will play an even greater role in defining the journal''s coverage and keeping Origins of Life and Evolution of Biospheres well-placed in this growing interdisciplinary field.
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