The Birthplace of Proto-Life: Role of Secondary Minerals in Forming Metallo-Proteins through Water-Rock Interaction of Hadean Rocks.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2018-12-01 Epub Date: 2019-04-03 DOI:10.1007/s11084-019-09571-y
Kazumi Yoshiya, Tomohiko Sato, Soichi Omori, Shigenori Maruyama
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引用次数: 6

Abstract

The surface of Hadean Earth was mainly covered with three types of rocks-komatiite, KREEP basalt and anorthosite-which were remarkably different from those on the modern Earth. The water-rock interaction between these rocks and water provided a highly reducing environment and formed secondary minerals on the surface of the rocks that are important for producing metallo-enzymes for the emergence of primordial life. Previous studies suggested a correlation between the active site of metallo-enzymes and sulfide minerals based on the affinity of their structures, but they did not discuss the origin of metallic elements contained in these minerals which is critical to understanding where life began. We investigated secondary minerals formed through water-rock interactions of komatiite in a subaerial geyser system, then discussed the relationship between the active site of metallo-enzymes and secondary minerals. Instead of komatiite, we used serpentinite collected from the Hakuba Happo area, Nagano Prefecture in central-north Japan, which is thought to be a modern analog for the Hadean environment. We found several minor minerals, such as magnetite, chromite, pyrite and pentlandite in addition to serpentine minerals. Pentlandite has not been mentioned in previous studies as one of the candidates that could supply important metallic elements to build metallo-enzymes. It has been shown to be a catalyst for hydrogen generation possibly, because of structural similarity to the active site of hydrogenases. We consider the possibility that nickel-iron sulfide, pentlandite, could be important minerals for the origin of life. In addition, we estimated what kinds of minor minerals would be obtained from the water-rock interaction of these rocks using thermodynamic calculations. KREEP basalt contains a large amount of iron and it could be useful for producing metallo-enzymes, especially ferredoxins-electron transfer enzymes, which may have assisted in the emergence of life.

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原生命的诞生地:次生矿物在通过哈代岩石的水-岩石相互作用形成金属蛋白中的作用。
哈代地球表面主要覆盖着三种类型的岩石--孔雀石、KREEP 玄武岩和正长岩,它们与现代地球上的岩石有着明显的不同。这些岩石与水的相互作用提供了一个高度还原的环境,并在岩石表面形成了次生矿物,这些次生矿物对于产生原始生命出现所需的金属酶非常重要。以前的研究根据硫化物矿物结构的亲和性,提出了金属酶活性位点与硫化物矿物之间的相关性,但没有讨论这些矿物中所含金属元素的来源,而这对于了解生命的起源至关重要。我们研究了在一个地下间歇泉系统中通过水-岩石相互作用形成的科马蒂石次生矿物,然后讨论了金属酶活性位点与次生矿物之间的关系。我们使用了从日本中北部长野县白马八方地区采集的蛇纹石,而不是光卤石。除了蛇纹石矿物外,我们还发现了一些次要矿物,如磁铁矿、铬铁矿、黄铁矿和戊兰特石。在以前的研究中,我们没有提到过彭脱石是可以提供重要金属元素来构建金属酶的候选矿物之一。它被证明是氢气生成的催化剂,这可能是因为它的结构与氢气酶的活性位点相似。我们认为,硫化镍铁、五菱锡矿可能是生命起源的重要矿物。此外,我们还通过热力学计算估算了这些岩石在水与岩石相互作用过程中会产生哪些次要矿物。KREEP 玄武岩含有大量的铁,它可能有助于产生金属酶,特别是铁氧还蛋白-电子传递酶,这可能有助于生命的出现。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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