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Optimum conditions for prebiotic evolution in extraterrestrial environments.

机译:地外环境中益生元进化的最佳条件。

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摘要

The overall goal of the dissertation was to devise synthetic pathways leading to the production of peptides and amino acids from smaller organic precursors. To this end, eight different zeolites were tested in order to determine their catalytic potential in the conversion of amino acids to peptides. The zeolites tested were either synthetic or naturally occurring. Acidic solutions of amino acids were prepared with or without zeolites and their reactivity was monitored over a four-week time interval. The kinetics and feasibility of peptide synthesis from selected amino acid combinations was investigated via the paper chromatography technique. Nine different amino acids were tested. The nature and extent of product were measured at constant time intervals. It was found that two ZSM-5 synthetic zeolites as well as the Fisher Scientific zeolite mix without alumina salts may have a catalytic potential in the conversion of amino acids to peptides. The conversion was verified by matching the paper chromatogram of the experimental product with that of a known peptide. The experimental results demonstrate that the optimum solvent system for paper chromatographic analysis of the zeolite-catalyzed self-assembly of the amino acids L-aspartic acid, L-asparagine, L-histidine, and L-serine is a 50:50 mixture of 1-butanol and acetone by volume. For the amino acids L-alanine, L-glycine, and L-valine, the optimum solvent was found to be a 30:70 mixture of ammonia and propanol by volume. A mathematical model describing the distance traveled (spot position) versus reaction time was constructed for the zeolite-catalyzed conversion of L-leucine and L-tyrosine and was found to approximately follow the function f(t) = 25 ln t. Two case studies for prebiotic synthesis leading to the production of amino acids or peptides in extraterrestrial environments were discussed: one involving Saturn's moon Titan, and the other involving Jupiter's moon Europa.; In the Titan study, it was determined that organic synthesis, based on simple precursors, may lead in the Titan environment to the production of biologically important molecules such as amino acids.; In the Europa study, three synthetic schemes using hydrogen peroxide, sulfuric acid, and hydrocyanic acid, and leading to the production of larger biologically important molecules such as amino acids were presented. (Abstract shortened by UMI.)
机译:论文的总体目标是设计合成途径,从而从较小的有机前体产生肽和氨基酸。为此,测试了八种不同的沸石,以确定它们在氨基酸向肽的转化中的催化潜力。测试的沸石是合成的或天然存在的。制备有或没有沸石的氨基酸酸性溶液,并在四个星期的时间间隔内监测其反应性。通过纸色谱技术研究了从选定的氨基酸组合合成肽的动力学和可行性。测试了九种不同的氨基酸。以恒定的时间间隔测量产物的性质和程度。已经发现,两种ZSM-5合成沸石以及不含氧化铝盐的Fisher Scientific沸石混合物在氨基酸向肽的转化中可能具有催化潜力。通过将实验产品的纸质色谱图与已知肽的色谱图进行匹配来验证转化率。实验结果表明,纸质色谱分析沸石催化的氨基酸L-天冬氨酸,L-天冬酰胺,L-组氨酸和L-丝氨酸的最佳溶剂体系是以下物质的50:50混合物: -丁醇和丙酮的体积。对于氨基酸L-丙氨酸,L-甘氨酸和L-缬氨酸,发现最佳溶剂是体积比为30:70的氨和丙醇的混合物。针对沸石催化的L-亮氨酸和L-酪氨酸的转化,建立了描述行进距离(位置)与反应时间的数学模型,发现该模型近似遵循函数f(t)= 25 ln t。讨论了两个有关在地球外环境中导致氨基酸或多肽生成的益生元合成的案例研究:一个涉及土星的卫星泰坦,另一个涉及木星的卫星欧罗巴。在泰坦研究中,已确定基于简单前体的有机合成可能会在泰坦环境中导致生物重要分子(例如氨基酸)的产生。在欧罗巴研究中,提出了三种使用过氧化氢,硫酸和氢氰酸的合成方案,这些方案导致产生更大的生物学上重要的分子,例如氨基酸。 (摘要由UMI缩短。)

著录项

  • 作者

    Abbas, Ousama H.;

  • 作者单位

    The University of Texas at El Paso.;

  • 授予单位 The University of Texas at El Paso.;
  • 学科 Chemistry General.; Biogeochemistry.; Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 2004
  • 页码 123 p.
  • 总页数 123
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 化学;生物地球化学、气体地球化学;天文学;
  • 关键词

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