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小行星含水蚀变过程中γ射线诱导的氨基酸形成:起始溶液成分的影响。

Gamma-Ray-Induced Amino Acid Formation during Aqueous Alteration in Small Bodies: The Effects of Compositions of Starting Solutions.

作者信息

Ishikawa Akari, Kebukawa Yoko, Kobayashi Kensei, Yoda Isao

机构信息

Department of Chemistry and Life Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan.

Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan.

出版信息

Life (Basel). 2024 Jan 9;14(1):103. doi: 10.3390/life14010103.

Abstract

Organic compounds, such as amino acids, are essential for the origin of life, and they may have been delivered to the prebiotic Earth from extra-terrestrial sources, such as carbonaceous chondrites. In the parent bodies of carbonaceous chondrites, the radioactive decays of short-lived radionuclides, such as Al, cause the melting of ice, and aqueous alteration occurs in the early stages of solar system formation. Many experimental studies have shown that complex organic matter, including amino acids and high-molecular-weight organic compounds, is produced by such hydrothermal processes. On the other hand, radiation, particularly gamma rays from radionuclides, can contribute to the formation of amino acids from simple molecules such as formaldehyde and ammonia. In this study, we investigated the details of gamma-ray-induced amino acid formation, focusing on the effects of different starting materials on aqueous solutions of formaldehyde, ammonia, methanol, and glycolaldehyde with various compositions, as well as hexamethylenetetramine. Alanine and glycine were the most abundantly formed amino acids after acid hydrolysis of gamma-ray-irradiated products. Amino acid formation increased with increasing gamma-ray irradiation doses. Lower amounts of ammonia relative to formaldehyde produced more amino acids. Glycolaldehyde significantly increased amino acid yields. Our results indicated that glycolaldehyde formation from formaldehyde enhanced by gamma rays is key for the subsequent production of amino acids.

摘要

有机化合物,如氨基酸,对生命起源至关重要,它们可能是从外星来源,如碳质球粒陨石,被输送到前生物地球的。在碳质球粒陨石的母体中,短寿命放射性核素(如铝)的放射性衰变导致冰融化,并且在太阳系形成的早期阶段发生水岩蚀变。许多实验研究表明,包括氨基酸和高分子量有机化合物在内的复杂有机物质是由这种热液过程产生的。另一方面,辐射,特别是来自放射性核素的伽马射线,可以促使由甲醛和氨等简单分子形成氨基酸。在本研究中,我们研究了伽马射线诱导氨基酸形成的细节,重点关注不同起始原料对具有各种组成的甲醛、氨、甲醇和乙醇醛水溶液以及六亚甲基四胺的影响。丙氨酸和甘氨酸是伽马射线辐照产物酸水解后形成最多的氨基酸。氨基酸的形成随着伽马射线辐照剂量的增加而增加。相对于甲醛,氨含量较低时产生的氨基酸更多。乙醇醛显著提高了氨基酸产量。我们的结果表明,伽马射线增强甲醛形成乙醇醛是随后产生氨基酸的关键。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e6c8/10817335/671c73140e78/life-14-00103-g009.jpg

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