标准基因代码可以从双字母 GC 代码演变而来,而不会造成信息丢失或代价高昂的重新分配。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Alejandro Frank, Tom Froese
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引用次数: 11

摘要

人们普遍认为,在标准遗传密码之前,一定有一个编码较少氨基酸的更简单的密码。由于对代码的大多数改动都代价高昂,因此人们对这种更简单的代码如何扩展成标准遗传代码还不甚了解。我们从最近合成的六字母密码中得到启发,提出了一个新的假设:最初的遗传密码仅由两个字母 G 和 C 组成,然后通过引入另外一对字母 A 和 U 增加了可用密码子的数量。各种证据表明,最初的两个核苷酸确实是 G 和 C。这个密码扩展过程可能从第三个碱基开始,到第二个碱基,最后在第一个碱基中引入第二对字母时,形成了标准遗传密码。所提出的过程与现有的经验证据是一致的,而且它独特地避免了代价高昂的代码变更问题,而是假设代码是通过创建带有额外字母的新密码子来扩大其容量的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Standard Genetic Code can Evolve from a Two-Letter GC Code Without Information Loss or Costly Reassignments.

It is widely agreed that the standard genetic code must have been preceded by a simpler code that encoded fewer amino acids. How this simpler code could have expanded into the standard genetic code is not well understood because most changes to the code are costly. Taking inspiration from the recently synthesized six-letter code, we propose a novel hypothesis: the initial genetic code consisted of only two letters, G and C, and then expanded the number of available codons via the introduction of an additional pair of letters, A and U. Various lines of evidence, including the relative prebiotic abundance of the earliest assigned amino acids, the balance of their hydrophobicity, and the higher GC content in genome coding regions, indicate that the original two nucleotides were indeed G and C. This process of code expansion probably started with the third base, continued with the second base, and ended up as the standard genetic code when the second pair of letters was introduced into the first base. The proposed process is consistent with the available empirical evidence, and it uniquely avoids the problem of costly code changes by positing instead that the code expanded its capacity via the creation of new codons with extra letters.

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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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