The Effect of Goethites on the Polymerization of Glycine and Alanine Under Prebiotic Chemistry Conditions.

IF 1.9 4区 物理与天体物理 Q2 BIOLOGY
João Paulo T Baú, Cristine E A Carneiro, Antônio Carlos S da Costa, Daniel F Valezi, Eduardo di Mauro, Eduardo Pilau, Dimas A M Zaia
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引用次数: 3

Abstract

After pre concentration of monomers, polymerization is the second most important step for molecular evolution. The formation of peptides is an important issue for prebiotic chemistry and consequently for the origin of life. In this work, goethite was synthesized by two different routes, named goethite-I and goethite-II. Although both samples are goethite, Far-FT-IR spectroscopy and EPR spectroscopy showed differences between them, and these differences had an effect on the polymerization of glycine and alanine. For the amino acid polymerization, three protocols were used, that resembled prebiotic Earth conditions: a) amino acid plus goethite were mixed and heated at 90 °C for 10 days in solid state, b) a wet impregnation of the amino acid in the goethite, with subsequent heating at 90 °C for 10 days in solid state, and c) 10 wet/dry cycles each one for 24 h at 90 °C. Experiments with glycine plus goethite-II, using protocols B and C, produced only Gly-Gly. In addition, for the C protocol the amount of Gly-Gly synthesized was 3 times higher than the amount of Ala-Ala. Goethite-I presented a decrease in the EPR signal, when it was submitted to the protocols with and without amino acids. It is probable the decrease in the intensity of the EPR signal was due to a decrease in the imperfections of the mineral. For all protocols the mixture of alanine plus goethite-I or goethite-II produced c(Ala-Ala). However, for wet/dry cycles, protocol C presented higher yields (p < 0.05). In addition, Ala-Ala was produced using protocols A and C. The c(Ala-Ala) formation fitted a zero-order kinetic equation model. The surface areas of goethite-I and goethite-II were 35 m2 g-1 and 37 m2 g-1, respectively. Thermal analysis indicated that the mineral changes the thermal behavior of the amino acids. The main reactions for the thermal decomposition of glycine were deamination and dehydration and for alanine was deamination.

益生元化学条件下针铁矿对甘氨酸和丙氨酸聚合的影响。
在单体预浓缩之后,聚合是分子进化的第二重要步骤。多肽的形成是益生元化学的一个重要问题,因此也是生命起源的一个重要问题。本文通过两种不同的路线合成针铁矿,分别命名为针铁矿i和针铁矿ii。虽然两种样品都是针铁矿,但远红外光谱和EPR光谱显示出它们之间的差异,这些差异对甘氨酸和丙氨酸的聚合产生了影响。对于氨基酸聚合,使用了三种类似于益生元地球条件的方案:a)氨基酸和针铁矿混合并在90°C下以固态加热10天;b)氨基酸在针铁矿中湿浸渍,随后在90°C下以固态加热10天;C) 10个湿/干循环,每个循环在90°C下持续24小时。甘氨酸加针铁矿ii的实验,采用方案B和C,只产生Gly-Gly。此外,对于C方案,Gly-Gly的合成量比Ala-Ala的合成量高3倍。针铁矿i在有氨基酸和没有氨基酸的情况下均表现出EPR信号的减少。EPR信号强度的降低很可能是由于矿物缺陷的减少。对于所有方案,丙氨酸加针铁矿i或针铁矿ii的混合物产生c(Ala-Ala)。然而,对于湿/干循环,方案C的产量更高(分别为p 2 g-1和37 m2 g-1)。热分析表明,该矿物改变了氨基酸的热行为。甘氨酸热分解的主要反应是脱胺和脱水,丙氨酸热分解的主要反应是脱胺。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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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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