关于乌尔蛋白质组的建议

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2018-06-01 Epub Date: 2017-11-10 DOI:10.1007/s11084-017-9553-2
Miryam Palacios-Pérez, Fernando Andrade-Díaz, Marco V José
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引用次数: 2

摘要

在这里,我们通过假设原始的 RNY 遗传密码,勾勒出了一个可信的蛋白质组。我们仅使用 RNA 基因型就揭示了原始表型;这意味着我们恢复了最古老的蛋白质组,主要由 RNY 三联体编码的 8 个氨基酸组成。通过观察这些片段可以发现,它们不是位于催化位点,而是位于辅助因子结合位点。这意味着分子的稳定作用早在其催化活性出现之前就已经出现了,因此乌尔蛋白质组包括一组与辅因子稳定结合位点(CSBSs)相对应的蛋白质模块,我们称之为原始结合组。利用我们的方法,我们仅使用 RMSD 就重建了 Sobolevsky 和 Trifonov(2006 年)发现的 "第一个蛋白质模块 "的结构。我们还研究了可能与它们结合的辅因子。我们结合关于原始生命形式的几种建议,讨论了 CSBSs 作为原生生物中第一个蛋白质模块的概念。
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A Proposal of the Ur-proteome.

Herein we outline a plausible proteome, encoded by assuming a primeval RNY genetic code. We unveil the primeval phenotype by using only the RNA genotype; it means that we recovered the most ancestral proteome, mostly made of the 8 amino acids encoded by RNY triplets. By looking at those fragments, it is noticeable that they are positioned, not at catalytic sites, but in the cofactor binding sites. It implies that the stabilization of a molecule appeared long before its catalytic activity, and therefore the Ur-proteome comprised a set of proteins modules that corresponded to Cofactor Stabilizing Binding Sites (CSBSs), which we call the primitive bindome. With our method, we reconstructed the structures of the "first protein modules" that Sobolevsky and Trifonov (2006) found by using only RMSD. We also examine the probable cofactors that bound to them. We discuss the notion of CSBSs as the first proteins modules in progenotes in the context of several proposals about the primitive forms of life.

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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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