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原始地球上的蛋氨酸和其他含硫有机化合物的前体合成:基于斯坦利·米勒未发表的 1958 年实验的当代重新评估。

Prebiotic synthesis of methionine and other sulfur-containing organic compounds on the primitive Earth: a contemporary reassessment based on an unpublished 1958 Stanley Miller experiment.

机构信息

Scripps Institution of Oceanography, University of California at San Diego, La Jolla, CA 92093, USA.

出版信息

Orig Life Evol Biosph. 2011 Jun;41(3):201-12. doi: 10.1007/s11084-010-9228-8. Epub 2010 Nov 10.

DOI:10.1007/s11084-010-9228-8
PMID:21063908
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC3094541/
Abstract

Original extracts from an unpublished 1958 experiment conducted by the late Stanley L. Miller were recently found and analyzed using modern state-of-the-art analytical methods. The extracts were produced by the action of an electric discharge on a mixture of methane (CH(4)), hydrogen sulfide (H(2)S), ammonia (NH(3)), and carbon dioxide (CO(2)). Racemic methionine was formed in significant yields, together with other sulfur-bearing organic compounds. The formation of methionine and other compounds from a model prebiotic atmosphere that contained H(2)S suggests that this type of synthesis is robust under reducing conditions, which may have existed either in the global primitive atmosphere or in localized volcanic environments on the early Earth. The presence of a wide array of sulfur-containing organic compounds produced by the decomposition of methionine and cysteine indicates that in addition to abiotic synthetic processes, degradation of organic compounds on the primordial Earth could have been important in diversifying the inventory of molecules of biochemical significance not readily formed from other abiotic reactions, or derived from extraterrestrial delivery.

摘要

最近,使用现代最先进的分析方法,发现并分析了已故斯坦利·L·米勒(Stanley L. Miller)在 1958 年进行的一项未发表实验的原始提取物。这些提取物是通过对甲烷(CH(4))、硫化氢(H(2)S)、氨(NH(3))和二氧化碳(CO(2))的混合物进行放电产生的。旋光性蛋氨酸以显著的产率与其他含硫有机化合物一起形成。从含有 H(2)S 的类原始大气中形成蛋氨酸和其他化合物表明,这种类型的合成在还原条件下是稳健的,这种条件可能存在于全球原始大气中,也可能存在于早期地球的局部火山环境中。由蛋氨酸和半胱氨酸分解产生的大量含硫有机化合物的存在表明,除了非生物合成过程外,原始地球上有机化合物的降解在使具有生物化学意义的分子多样化方面可能非常重要,这些分子不易通过其他非生物反应形成,也不是来自外星体的输送。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/ee28702d0c43/11084_2010_9228_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/5630f003e357/11084_2010_9228_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/c74db464958e/11084_2010_9228_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/b69c92a496d0/11084_2010_9228_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/ee28702d0c43/11084_2010_9228_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/5630f003e357/11084_2010_9228_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/c74db464958e/11084_2010_9228_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/b69c92a496d0/11084_2010_9228_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b7c7/3094541/ee28702d0c43/11084_2010_9228_Fig4_HTML.jpg

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