Computational Study of the Stability of Natural Amino Acid isomers.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY Origins of Life and Evolution of Biospheres Pub Date : 2021-12-01 Epub Date: 2021-11-05 DOI:10.1007/s11084-021-09615-2
Stefano Crespi, Dhanalakshmi Vadivel, Alfredo Bellisario, Daniele Dondi
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引用次数: 2

Abstract

The secular debate on the origin of life on our planet represents one of the open challenges for the scientific community. In this endeavour, chemistry has a pivotal role in disclosing novel scenarios that allow us to understand how the formation of simple organic molecules would be possible in the early primitive geological ages of Earth. Amino acids play a crucial role in biological processes. They are known to be formed in experiments simulating primitive conditions and were found in meteoric samples retrieved throughout the years. Understanding their formation is a key step for prebiotic chemistry. Following this reasoning, we performed a computational investigation over 100'000 structural isomers of natural amino acids. The results we have found suggest that natural amino acids are among the most thermodynamically stable structures and, therefore, one of the most probable ones to be synthesised among their possible isomers.

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天然氨基酸异构体稳定性的计算研究。
关于地球上生命起源的世俗辩论是科学界面临的公开挑战之一。在这一努力中,化学在揭示新的场景方面发挥着关键作用,这些场景使我们能够理解在地球早期原始地质时代,简单有机分子是如何形成的。氨基酸在生物过程中起着至关重要的作用。众所周知,它们是在模拟原始条件的实验中形成的,并且是在多年来收集的大气样本中发现的。了解它们的形成是研究益生元化学的关键一步。根据这一推理,我们对天然氨基酸的10万个结构异构体进行了计算研究。我们发现的结果表明,天然氨基酸是热力学最稳定的结构之一,因此,在它们可能的异构体中,它是最可能被合成的结构之一。
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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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