手性驱动扭转作为二元混合物原始折叠的驱动力。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Dmitry V Zlenko, Aleksey A Skoblin, Alexander S Vedenkin, Mariya G Mikhaleva, Anatoly M Zanin, Vsevolod A Tverdislov, Sergey V Stovbun
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引用次数: 2

摘要

n -三氟乙酰化α-氨基醇(TFAAAs)在手性纯时能够形成准一维超分子纤维(弦),并在外消旋体中形成等距沉淀。弦的形成导致溶液的可逆凝胶化。新鲜凝胶占据所有可用的体积,但在孵育期间,它们收缩并集中在管的中心区域。显微镜观察显示,在小时的时间尺度上,在孵育过程中,弦的直径和旋转的增长。旋转使发夹形成,作为旋转管柱上的挂钩,从而使管柱盘绕,观察到凝胶收缩。扭曲的弦的形态类似于在现代蛋白质中观察到的结构,这允许在生物聚合物的折叠和弦的形成之间进行类比。此外,在TFAAA凝胶中发现的旋转是一个简单系统将分子间凝集的能量转化为旋转运动的例子,因此它们可以被认为是分子马达。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Chirality Driven Twisting as a Driving Force of Primitive Folding in Binary Mixtures.

The N-trifluoroacetylated α-aminoalcohols (TFAAAs) are able to form quasi-one-dimensional supramolecular fibers (strings) when chirally pure, and isometric precipitates in the racemate. The strings' formation leads to the reversible gelation of the solution. The fresh gels occupy all the available volume, however during the incubation, they contract and concentrate in the central region of the tube. The microscopic observations revealed the growth of the strings' diameter and their rotation in the course of the incubation at the hour time-scale. The rotation provides for the hairpins forming that serve as hooks on the rotating string, which provides for coiling of the strings, which was observed as gel contraction. The morphology of the twisted strings resembles the structures observed in modern proteins, which allows drawing an analogy between the folding of biopolymers and the formation of the clew of strings. In addition, the rotation found in the TFAAA gels is an example of a simple system converting the energy of intermolecular agglutination to the rotational movement, so they could be considered as molecular motors.

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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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