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Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun
Life most likely started during the Hadean Eon; however, the environmental conditions which contributed to the complexity of its chemistry are poorly known. A better understanding of various environmental conditions, including global (heliospheric) and local (atmospheric, surface, and oceanic), alon...
Autores principales: | , , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
MDPI
2023
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10221653/ https://www.ncbi.nlm.nih.gov/pubmed/37240748 http://dx.doi.org/10.3390/life13051103 |
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author | Kobayashi, Kensei Ise, Jun-ichi Aoki, Ryohei Kinoshita, Miei Naito, Koki Udo, Takumi Kunwar, Bhagawati Takahashi, Jun-ichi Shibata, Hiromi Mita, Hajime Fukuda, Hitoshi Oguri, Yoshiyuki Kawamura, Kimitaka Kebukawa, Yoko Airapetian, Vladimir S. |
author_facet | Kobayashi, Kensei Ise, Jun-ichi Aoki, Ryohei Kinoshita, Miei Naito, Koki Udo, Takumi Kunwar, Bhagawati Takahashi, Jun-ichi Shibata, Hiromi Mita, Hajime Fukuda, Hitoshi Oguri, Yoshiyuki Kawamura, Kimitaka Kebukawa, Yoko Airapetian, Vladimir S. |
author_sort | Kobayashi, Kensei |
collection | PubMed |
description | Life most likely started during the Hadean Eon; however, the environmental conditions which contributed to the complexity of its chemistry are poorly known. A better understanding of various environmental conditions, including global (heliospheric) and local (atmospheric, surface, and oceanic), along with the internal dynamic conditions of the early Earth, are required to understand the onset of abiogenesis. Herein, we examine the contributions of galactic cosmic rays (GCRs) and solar energetic particles (SEPs) associated with superflares from the young Sun to the formation of amino acids and carboxylic acids in weakly reduced gas mixtures representing the early Earth’s atmosphere. We also compare the products with those introduced by lightning events and solar ultraviolet light (UV). In a series of laboratory experiments, we detected and characterized the formation of amino acids and carboxylic acids via proton irradiation of a mixture of carbon dioxide, methane, nitrogen, and water in various mixing ratios. These experiments show the detection of amino acids after acid hydrolysis when 0.5% (v/v) of initial methane was introduced to the gas mixture. In the set of experiments with spark discharges (simulation of lightning flashes) performed for the same gas mixture, we found that at least 15% methane was required to detect the formation of amino acids, and no amino acids were detected in experiments via UV irradiation, even when 50% methane was used. Carboxylic acids were formed in non-reducing gas mixtures (0% methane) by proton irradiation and spark discharges. Hence, we suggest that GCRs and SEP events from the young Sun represent the most effective energy sources for the prebiotic formation of biologically important organic compounds from weakly reducing atmospheres. Since the energy flux of space weather, which generated frequent SEPs from the young Sun in the first 600 million years after the birth of the solar system, was expected to be much greater than that of GCRs, we conclude that SEP-driven energetic protons are the most promising energy sources for the prebiotic production of bioorganic compounds in the atmosphere of the Hadean Earth. |
format | Online Article Text |
id | pubmed-10221653 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2023 |
publisher | MDPI |
record_format | MEDLINE/PubMed |
spelling | pubmed-102216532023-05-28 Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun Kobayashi, Kensei Ise, Jun-ichi Aoki, Ryohei Kinoshita, Miei Naito, Koki Udo, Takumi Kunwar, Bhagawati Takahashi, Jun-ichi Shibata, Hiromi Mita, Hajime Fukuda, Hitoshi Oguri, Yoshiyuki Kawamura, Kimitaka Kebukawa, Yoko Airapetian, Vladimir S. Life (Basel) Article Life most likely started during the Hadean Eon; however, the environmental conditions which contributed to the complexity of its chemistry are poorly known. A better understanding of various environmental conditions, including global (heliospheric) and local (atmospheric, surface, and oceanic), along with the internal dynamic conditions of the early Earth, are required to understand the onset of abiogenesis. Herein, we examine the contributions of galactic cosmic rays (GCRs) and solar energetic particles (SEPs) associated with superflares from the young Sun to the formation of amino acids and carboxylic acids in weakly reduced gas mixtures representing the early Earth’s atmosphere. We also compare the products with those introduced by lightning events and solar ultraviolet light (UV). In a series of laboratory experiments, we detected and characterized the formation of amino acids and carboxylic acids via proton irradiation of a mixture of carbon dioxide, methane, nitrogen, and water in various mixing ratios. These experiments show the detection of amino acids after acid hydrolysis when 0.5% (v/v) of initial methane was introduced to the gas mixture. In the set of experiments with spark discharges (simulation of lightning flashes) performed for the same gas mixture, we found that at least 15% methane was required to detect the formation of amino acids, and no amino acids were detected in experiments via UV irradiation, even when 50% methane was used. Carboxylic acids were formed in non-reducing gas mixtures (0% methane) by proton irradiation and spark discharges. Hence, we suggest that GCRs and SEP events from the young Sun represent the most effective energy sources for the prebiotic formation of biologically important organic compounds from weakly reducing atmospheres. Since the energy flux of space weather, which generated frequent SEPs from the young Sun in the first 600 million years after the birth of the solar system, was expected to be much greater than that of GCRs, we conclude that SEP-driven energetic protons are the most promising energy sources for the prebiotic production of bioorganic compounds in the atmosphere of the Hadean Earth. MDPI 2023-04-28 /pmc/articles/PMC10221653/ /pubmed/37240748 http://dx.doi.org/10.3390/life13051103 Text en © 2023 by the authors. https://creativecommons.org/licenses/by/4.0/Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/4.0/). |
spellingShingle | Article Kobayashi, Kensei Ise, Jun-ichi Aoki, Ryohei Kinoshita, Miei Naito, Koki Udo, Takumi Kunwar, Bhagawati Takahashi, Jun-ichi Shibata, Hiromi Mita, Hajime Fukuda, Hitoshi Oguri, Yoshiyuki Kawamura, Kimitaka Kebukawa, Yoko Airapetian, Vladimir S. Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun |
title | Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun |
title_full | Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun |
title_fullStr | Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun |
title_full_unstemmed | Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun |
title_short | Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun |
title_sort | formation of amino acids and carboxylic acids in weakly reducing planetary atmospheres by solar energetic particles from the young sun |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10221653/ https://www.ncbi.nlm.nih.gov/pubmed/37240748 http://dx.doi.org/10.3390/life13051103 |
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