生命早期的甲烷生成:古老而非原始。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Israel Muñoz-Velasco, Carlos García-Ferris, Ricardo Hernandez-Morales, Antonio Lazcano, Juli Peretó, Arturo Becerra
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引用次数: 13

摘要

在已知的六种自养途径中,伍德-荣格达尔途径(WL)是唯一同时存在于产乙酸的细菌(同源乙酸菌)和产甲烷的古细菌(亲氢甲烷菌)中的途径,有人认为 WL 是最古老的代谢途径之一。然而,只有所谓的羰基分支是古细菌和细菌共有的,而甲基分支则不同,无论是反应的数量还是酶的数量,它们之间都没有同源物。在这项研究中,我们发现,尽管古细菌伍德-荣格达尔途径(MBWL)的进化史无法追溯到最后共同祖先,但细菌和非甲烷古细菌中都有甲基分支的某些部分。我们还分析了甲烷发生的不同变体(富氢途径、乙酰脆化途径和富甲途径),并得出结论:这些途径中的每一种途径,以及每一种不同的酶或亚基(在多聚酶的情况下),都有各自错综复杂的进化历史。我们的研究支持这种观点,即养氢型甲烷发生比其他变体更古老,尽管还没有古老到足以出现在最后的古细菌共同祖先中。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Methanogenesis on Early Stages of Life: Ancient but Not Primordial.

Of the six known autotrophic pathways, the Wood-Ljungdahl pathway (WL) is the only one present in both the acetate producing Bacteria (homoacetogens) and the methane producing Archaea (hydrogenotrophic methanogens), and it has been suggested that WL is one of the oldest metabolic pathways. However, only the so-called carbonyl branch is shared by Archaea and Bacteria, while the methyl branch is different, both in the number of reactions and enzymes, which are not homologous among them. In this work we show that some parts of the methyl branch of archaeal Wood-Ljungdahl pathway (MBWL) are present in bacteria as well as in non-methanogen archaea, although the tangled evolutionary history of MBWL cannot be traced back to the Last Common Ancestor. We have also analyzed the different variants of methanogenesis (hydrogenotrophic, acetoclastic and methylotrophic pathways), and concluded that each of these pathways, and every different enzyme or subunit (in the case of multimeric enzymes), has their own intricate evolutionary history. Our study supports the scenario of hydrogenotrophic methanogenesis being older than the other variants, albeit not old enough to be present in the last archaeal common ancestor.

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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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