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从零到英雄:在模拟冥古宙环境的水环境中,由乙炔、氨和一氧化碳无氰形成氨基酸和酰胺。

From Zero to Hero: The Cyanide-Free Formation of Amino Acids and Amides from Acetylene, Ammonia and Carbon Monoxide in Aqueous Environments in a Simulated Hadean Scenario.

作者信息

Seitz Christian, Geisberger Thomas, West Alexander Richard, Fertl Jessica, Eisenreich Wolfgang, Huber Claudia

机构信息

Bayerisches NMR Zentrum, Strukturelle Membranbiochemie, Technische Universität München, Lichtenbergstr. 4, 85748 Garching, Germany.

出版信息

Life (Basel). 2024 Jun 1;14(6):719. doi: 10.3390/life14060719.

DOI:10.3390/life14060719
PMID:38929702
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11204499/
Abstract

Amino acids are one of the most important building blocks of life. During the biochemical process of translation, cells sequentially connect amino acids via amide bonds to synthesize proteins, using the genetic information in messenger RNA (mRNA) as a template. From a prebiotic perspective (i.e., without enzymatic catalysis), joining amino acids to peptides via amide bonds is difficult due to the highly endergonic nature of the condensation reaction. We show here that amides can be formed in reactions catalyzed by the transition metal sulfides from acetylene, carbon monoxide and ammonia under aqueous conditions. Some α- and β-amino acids were also formed under the same conditions, demonstrating an alternative cyanide-free path for the formation of amino acids in prebiotic environments. Experiments performed with stable isotope labeled precursors, like NHCl and C-acetylene, enabled the accurate mass spectroscopic identification of the products formed from the starting materials and their composition. Reactions catalyzed using the transition metal sulfides seem to offer a promising alternative pathway for the formation of amides and amino acids in prebiotic environments, bypassing the challenges posed by the highly endergonic condensation reaction. These findings shed light on the potential mechanisms by which the building blocks of life could have originated on early Earth.

摘要

氨基酸是生命最重要的组成部分之一。在翻译的生化过程中,细胞以信使核糖核酸(mRNA)中的遗传信息为模板,通过酰胺键依次连接氨基酸来合成蛋白质。从益生元的角度来看(即无酶催化),由于缩合反应具有高度的吸能性质,通过酰胺键将氨基酸连接成肽是困难的。我们在此表明,在水相条件下,过渡金属硫化物催化的反应中,乙炔、一氧化碳和氨之间可形成酰胺。在相同条件下还形成了一些α-和β-氨基酸,这表明在益生元环境中形成氨基酸存在一种无需氰化物的替代途径。使用稳定同位素标记的前体(如NHCl和C-乙炔)进行的实验,能够通过精确的质谱鉴定由起始原料形成的产物及其组成。过渡金属硫化物催化的反应似乎为益生元环境中酰胺和氨基酸的形成提供了一条有前景的替代途径,绕过了高度吸能的缩合反应带来的挑战。这些发现揭示了生命组成部分可能在早期地球上起源的潜在机制。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/e3af703748f5/life-14-00719-sch004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/79e8cdf59f8a/life-14-00719-sch001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/e4024e9c9cd1/life-14-00719-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/5235f139652b/life-14-00719-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/a383cefd0d7f/life-14-00719-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/8f94421cb9c1/life-14-00719-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/f6b99d6961a2/life-14-00719-sch002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/f7f62416e608/life-14-00719-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/f7ac8fea4c6f/life-14-00719-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/211b652a100a/life-14-00719-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/9f7fd893c0a4/life-14-00719-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/b67d65f468da/life-14-00719-sch003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/e3af703748f5/life-14-00719-sch004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/79e8cdf59f8a/life-14-00719-sch001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/e4024e9c9cd1/life-14-00719-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/5235f139652b/life-14-00719-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/a383cefd0d7f/life-14-00719-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/8f94421cb9c1/life-14-00719-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/f6b99d6961a2/life-14-00719-sch002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/f7f62416e608/life-14-00719-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/f7ac8fea4c6f/life-14-00719-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/211b652a100a/life-14-00719-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/9f7fd893c0a4/life-14-00719-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/b67d65f468da/life-14-00719-sch003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6b6e/11204499/e3af703748f5/life-14-00719-sch004.jpg

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