Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun

Author:

Kobayashi Kensei1ORCID,Ise Jun-ichi1,Aoki Ryohei1,Kinoshita Miei1,Naito Koki1,Udo Takumi1,Kunwar Bhagawati2ORCID,Takahashi Jun-ichi1,Shibata Hiromi3,Mita Hajime4ORCID,Fukuda Hitoshi5,Oguri Yoshiyuki6,Kawamura Kimitaka2ORCID,Kebukawa Yoko1ORCID,Airapetian Vladimir S.789ORCID

Affiliation:

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

2. Chubu Institute of Advanced Studies, Chubu University, 1200 Matsumoto-cho, Kasugai 487-8501, Japan

3. SANKEN (The Institute of Scientific and Industrial Research), Osaka University, Ibaraki 567-0047, Japan

4. Department of Life, Environment and Applied Chemistry, Faculty of Engineering, Fukuoka Institute of Technology, Fukuoka 811-0295, Japan

5. Open Facility Center, Tokyo Institute of Technology, Meguro-ku, Tokyo 152-8550, Japan

6. Institute of Innovative Research, Tokyo Institute of Technology, Tokyo Institute of Technology, Meguro-ku, Tokyo 152-8550, Japan

7. NASA Goddard Space Flight Center/Sellers Exoplanetary Environments Collaboration, Greenbelt, MD 20771, USA

8. Department of Physics, American University, Washington, DC 20016, USA

9. Graduate School of Advanced Integrated Studies in Human Survivability, Kyoto University, Sakyo-ku, Kyoto 606-8501, Japan

Abstract

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.

Funder

Japan Society for the Promotion of Science

JSPS Joint Research Program, implemented in association with DFG

NASA/GSFC Sellers Exoplanet Environments Collaboration

Fundamental Laboratory Research

NASA Planetary Science Division’s Internal Scientist Funding Model (ISFM), HST-XMM Newton Cycle 27 and NICER Cycle 2 programs

International Space Science Institute and the supported International Team 464

Publisher

MDPI AG

Subject

Paleontology,Space and Planetary Science,General Biochemistry, Genetics and Molecular Biology,Ecology, Evolution, Behavior and Systematics

Reference85 articles.

1. 13C-Depleted carbon microparticles in >3700-Ma sea-floor sedimentary rocks from west Greenland;Rosing;Science,1999

2. Constraining the time interval for the origin of life on Earth;Pearce;Astrobiology,2018

3. Origin of life;Haldane;Ration. Ann.,1929

4. Oparin, A.I. (1938). Origin of Life, Dover.

5. A production of amino acids under possible primitive earth conditions;Miller;Science,1953

Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares;The Astrophysical Journal;2024-01-01

2. Exploring the photometric variability of ultra-cool dwarfs with TESS;Monthly Notices of the Royal Astronomical Society;2023-11-27

3. Can comets deliver prebiotic molecules to rocky exoplanets?;Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences;2023-11

4. Exploring the Interaction of Cosmic Rays with Water by Using an Old-Style Detector and Rossi’s Method;Particles;2023-08-30

5. Miller’s spark;Nature Reviews Chemistry;2023-08-18

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3