在碱性水热喷口环境中甲酸反应的合理性。

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Arthur Omran
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引用次数: 7

摘要

益生元过程需要可靠的自由能来源和可能包括糖的复杂化学混合物。甲糖反应是这些糖的潜在来源。在中等到升高的温度和pH范围内,这些糖会迅速腐烂。研究表明,基于CaCO3的化学花园催化甲糖反应产生葡萄糖、核糖和其他单糖。这些薄无机膜被探索为水热喷口材料的类似物——一个可能的生命起源地,同样暴露在非常陡峭的pH梯度中。在简单反应-扩散模型模拟的支持下,这项研究表明,这种梯度允许糖在薄膜的特定层中动态积累,有效地保护了甲糖的产量。因此,在碱性水热喷口环境中,甲糖反应可能是一种看似合理的益生元反应,可能为RNA世界奠定了基础。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Plausibility of the Formose Reaction in Alkaline Hydrothermal Vent Environments.

Prebiotic processes required a reliable source of free energy and complex chemical mixtures that may have included sugars. The formose reaction is a potential source of those sugars. At moderate to elevated temperature and pH ranges, these sugars rapidly decay. Here it is shown that CaCO3-based chemical gardens catalyze the formose reaction to produce glucose, ribose, and other monosaccharides. These thin inorganic membranes are explored as analogs of hydrothermal vent materials-a possible place for the origin of life-and similarly exposed to very steep pH gradients. Supported by simulations of a simple reaction-diffusion model, this study shows that such gradients allow for the dynamic accumulation of sugars in specific layers of the thin membrane, effectively protecting formose sugar yields. Therefore, the formose reaction may be a plausible prebiotic reaction in alkaline hydrothermal vent environments, possibly setting the stage for an RNA world.

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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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