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Gamma-Ray-Induced Amino Acid Formation in Aqueous Small Bodies in the Early Solar System
[Image: see text] Carbonaceous chondrites contain life’s essential building blocks, including amino acids, and their delivery of organic compounds would have played a key role in life’s emergence on Earth. Aqueous alteration of carbonaceous chondrites is a widespread process induced by the heat prod...
Autores principales: | , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
American Chemical Society
2022
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Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9801502/ https://www.ncbi.nlm.nih.gov/pubmed/36589881 http://dx.doi.org/10.1021/acscentsci.2c00588 |
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author | Kebukawa, Yoko Asano, Shinya Tani, Atsushi Yoda, Isao Kobayashi, Kensei |
author_facet | Kebukawa, Yoko Asano, Shinya Tani, Atsushi Yoda, Isao Kobayashi, Kensei |
author_sort | Kebukawa, Yoko |
collection | PubMed |
description | [Image: see text] Carbonaceous chondrites contain life’s essential building blocks, including amino acids, and their delivery of organic compounds would have played a key role in life’s emergence on Earth. Aqueous alteration of carbonaceous chondrites is a widespread process induced by the heat produced by radioactive decay of nuclides like (26)Al. Simple ubiquitous molecules like formaldehyde and ammonia could produce various organic compounds, including amino acids and complex organic macromolecules. However, the effects of radiation on such organic chemistry are unknown. Hence, the effects of gamma rays from radioactive decays on the formation of amino acids in meteorite parent bodies are demonstrated here. We discovered that gamma-ray irradiation of aqueous formaldehyde and ammonia solutions afforded a variety of amino acids. The amino acid yields had a linear relationship with the total gamma-ray dose but were unaffected by the irradiation dose rates. Given the gamma-ray production rates in the meteorite parent bodies, we estimated that the production rates were reasonable compared to amino acid abundances in carbonaceous chondrites. Our findings indicate that gamma rays may contribute to amino acid formation in parent bodies during aqueous alteration. In this paper, we propose a new prebiotic amino acid formation pathway that contributes to life’s origin. |
format | Online Article Text |
id | pubmed-9801502 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2022 |
publisher | American Chemical Society |
record_format | MEDLINE/PubMed |
spelling | pubmed-98015022022-12-31 Gamma-Ray-Induced Amino Acid Formation in Aqueous Small Bodies in the Early Solar System Kebukawa, Yoko Asano, Shinya Tani, Atsushi Yoda, Isao Kobayashi, Kensei ACS Cent Sci [Image: see text] Carbonaceous chondrites contain life’s essential building blocks, including amino acids, and their delivery of organic compounds would have played a key role in life’s emergence on Earth. Aqueous alteration of carbonaceous chondrites is a widespread process induced by the heat produced by radioactive decay of nuclides like (26)Al. Simple ubiquitous molecules like formaldehyde and ammonia could produce various organic compounds, including amino acids and complex organic macromolecules. However, the effects of radiation on such organic chemistry are unknown. Hence, the effects of gamma rays from radioactive decays on the formation of amino acids in meteorite parent bodies are demonstrated here. We discovered that gamma-ray irradiation of aqueous formaldehyde and ammonia solutions afforded a variety of amino acids. The amino acid yields had a linear relationship with the total gamma-ray dose but were unaffected by the irradiation dose rates. Given the gamma-ray production rates in the meteorite parent bodies, we estimated that the production rates were reasonable compared to amino acid abundances in carbonaceous chondrites. Our findings indicate that gamma rays may contribute to amino acid formation in parent bodies during aqueous alteration. In this paper, we propose a new prebiotic amino acid formation pathway that contributes to life’s origin. American Chemical Society 2022-12-07 2022-12-28 /pmc/articles/PMC9801502/ /pubmed/36589881 http://dx.doi.org/10.1021/acscentsci.2c00588 Text en © 2022 The Authors. Published by American Chemical Society https://creativecommons.org/licenses/by/4.0/Permits the broadest form of re-use including for commercial purposes, provided that author attribution and integrity are maintained (https://creativecommons.org/licenses/by/4.0/). |
spellingShingle | Kebukawa, Yoko Asano, Shinya Tani, Atsushi Yoda, Isao Kobayashi, Kensei Gamma-Ray-Induced Amino Acid Formation in Aqueous Small Bodies in the Early Solar System |
title | Gamma-Ray-Induced
Amino Acid Formation in Aqueous
Small Bodies in the Early Solar System |
title_full | Gamma-Ray-Induced
Amino Acid Formation in Aqueous
Small Bodies in the Early Solar System |
title_fullStr | Gamma-Ray-Induced
Amino Acid Formation in Aqueous
Small Bodies in the Early Solar System |
title_full_unstemmed | Gamma-Ray-Induced
Amino Acid Formation in Aqueous
Small Bodies in the Early Solar System |
title_short | Gamma-Ray-Induced
Amino Acid Formation in Aqueous
Small Bodies in the Early Solar System |
title_sort | gamma-ray-induced
amino acid formation in aqueous
small bodies in the early solar system |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9801502/ https://www.ncbi.nlm.nih.gov/pubmed/36589881 http://dx.doi.org/10.1021/acscentsci.2c00588 |
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