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

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