在合理的前生物条件下葡萄糖的低聚物化

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
Zhao Li, Li Li, Kristin R McKenna, Merranda Schmidt, Pamela Pollet, Leslie Gelbaum, Facundo M Fernández, Ramanarayanan Krishnamurthy, Charles L Liotta
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引用次数: 4

摘要

多糖是现存生物学中质量最大的一类生物高聚物,但很少有人通过实验研究多糖的前生物起源。在此,我们报告了在可信的前生物条件下,采用湿-干(夜-日)方案,在 50 °C 下用 0.01 M HCl 酸催化缩合模型单糖葡萄糖水溶液的情况。通过高分辨率质谱鉴定,该方案可形成含有多达八个单体单元的低聚糖。通过结合 1H、13C 和二维核磁共振光谱,阐明了低聚物缩醛连接的区域和立体化学,以及葡萄糖转化的定量分析。在 11 种可能的缩醛连接中,已确定了 10 种,包括 α- 和 β- 异构体,其中 α- 和 β- 1,6-acetals 是观察到的主要连接。此外,还介绍了几种葡萄糖二糖(如纤维二糖、麦芽糖和龙胆二糖)在酸催化下的低聚作用,并与葡萄糖的相应低聚作用进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
The Oligomerization of Glucose Under Plausible Prebiotic Conditions.

The prebiotic origin of polysaccharides, the largest class of biopolymers by mass in extant biology, has seldom been investigated experimentally. Herein, we report on the acid-catalyzed condensation of aqueous solutions of glucose, a model monosaccharide, under plausible prebiotic conditions employing a wet-dry (night-day) protocol with 0.01 M HCl at 50 °C. This protocol leads to the formation of oligosaccharides containing up to eight monomeric units identified by high resolution mass spectrometry. The regio- and stereochemistry of the oligomeric acetal linkages, as well as the quantitative analysis of glucose conversion, are elucidated by combining 1H, 13C and 2D NMR spectroscopy. Ten out of eleven possible acetal linkages, including α- and β- anomers, have been identified with the α- and β- 1,6-acetals being the dominant linkages observed. In addition, the acid-catalyzed oligomerization of several glucose disaccharides such as cellobiose, maltose, and gentiobiose are presented along with an accompanying comparison with the corresponding oligomerization of glucose.

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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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