评价矿物晶格作为金属蛋白进化的进化代理。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Kenneth N McGuinness, Gunnar W Klau, Shaunna M Morrison, Elisha K Moore, Jan Seipp, Paul G Falkowski, Vikas Nanda
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引用次数: 1

摘要

蛋白质协调的铁硫簇驱动整个生命之树的生物体代谢途径中的电子流。目前尚不清楚铁硫团簇最初是如何结合到蛋白质中的。与早期地球上存在的硫化铁矿物的结构相似,表明蛋白质和矿物质的进化之间存在联系。大量蛋白质和矿物晶体结构数据集的可用性,为利用信息学方法大规模探索蛋白质和矿物的共同进化提供了机会。然而,与蛋白质中的金属团簇大小有限相比,矿物晶格的无限重复性质使定量比较变得混乱。我们使用Niggli还原来解决这个问题,将矿物晶格转换为有限的,独特的结构,当翻译时再现晶格。蛋白质和还原矿物结构用商图表示,边和节点分别对应键和原子。提出了一种基于图论的矿物商图与蛋白质商图之间最大共连通边子图(MCCES)的计算方法。MCCES可以适应结构体积的差异,并且在计算相似性时很容易考虑额外的化学标准。为了解释图形大小的差异,我们使用Tversky相似指数。使用一致的标准,我们发现在假定的古代铁硫蛋白簇和铁硫矿物晶格之间几乎没有相似性,这表明这些金属位点并不像以前认为的那样在进化上相互联系。为了更好地理解地圈和生物圈的共同进化,我们讨论了这些发现可能的进化意义,并提出了另一种替代方法——矿物表面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Evaluating Mineral Lattices as Evolutionary Proxies for Metalloprotein Evolution.

Protein coordinated iron-sulfur clusters drive electron flow within metabolic pathways for organisms throughout the tree of life. It is not known how iron-sulfur clusters were first incorporated into proteins. Structural analogies to iron-sulfide minerals present on early Earth, suggest a connection in the evolution of both proteins and minerals. The availability of large protein and mineral crystallographic structure data sets, provides an opportunity to explore co-evolution of proteins and minerals on a large-scale using informatics approaches. However, quantitative comparisons are confounded by the infinite, repeating nature of the mineral lattice, in contrast to metal clusters in proteins, which are finite in size. We address this problem using the Niggli reduction to transform a mineral lattice to a finite, unique structure that when translated reproduces the crystal lattice. Protein and reduced mineral structures were represented as quotient graphs with the edges and nodes corresponding to bonds and atoms, respectively. We developed a graph theory-based method to calculate the maximum common connected edge subgraph (MCCES) between mineral and protein quotient graphs. MCCES can accommodate differences in structural volumes and easily allows additional chemical criteria to be considered when calculating similarity. To account for graph size differences, we use the Tversky similarity index. Using consistent criteria, we found little similarity between putative ancient iron-sulfur protein clusters and iron-sulfur mineral lattices, suggesting these metal sites are not as evolutionarily connected as once thought. We discuss possible evolutionary implications of these findings in addition to suggesting an alternative proxy, mineral surfaces, for better understanding the coevolution of the geosphere and biosphere.

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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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