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Formation of Amino Acids and Carboxylic Acids in Weakly  Reducing Planetary Atmospheres by Solar Energetic Particles from the Young SunLife 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.
Document ID
20230006802
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Kensei Kobayashi ORCID
(Yokohama National University Yokohama, Kanagawa, Japan)
Jun-ichi Ise
(Yokohama National University Yokohama, Kanagawa, Japan)
Ryohei Aoki
(Yokohama National University Yokohama, Kanagawa, Japan)
Miei Kinoshita
(Yokohama National University Yokohama, Kanagawa, Japan)
Koki Naito
(Yokohama National University Yokohama, Kanagawa, Japan)
Takumi Udo
(Yokohama National University Yokohama, Kanagawa, Japan)
Bhagawati Kunwar
(Chubu University Kasugai, Japan)
Jun-ichi Takahashi
(Yokohama National University Yokohama, Kanagawa, Japan)
Hiromi Shibata
(Osaka University Osaka, Japan)
Hajime Mita
(Fukuoka Institute of Technology Fukuoka, Japan)
Hitoshi Fukuda
(Tokyo Institute of Technology Tokyo, Tôkyô, Japan)
Yoshiyuki Oguri
(Tokyo Institute of Technology Tokyo, Tôkyô, Japan)
Kimitaka Kawamura
(Chubu University Kasugai, Japan)
Yoko Kebukawa ORCID
(Yokohama National University Yokohama, Kanagawa, Japan)
Vladimir S Airapetian
(Adnet Systems (United States) Bethesda, Maryland, United States)
Date Acquired
May 3, 2023
Publication Date
April 28, 2023
Publication Information
Publication: Life
Publisher: MDPI
Volume: 13
Issue: 5
Issue Publication Date: April 28, 2023
e-ISSN: 2075-1729
Subject Category
Solar Physics
Lunar and Planetary Science and Exploration
Funding Number(s)
WBS: 791926.02.06.01.15.02
CONTRACT_GRANT: 80GSFC23CA040
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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