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

被引:16
作者
Kobayashi, Kensei [1 ]
Ise, Jun-ichi [1 ]
Aoki, Ryohei [1 ]
Kinoshita, Miei [1 ]
Naito, Koki [1 ]
Udo, Takumi [1 ]
Kunwar, Bhagawati [2 ]
Takahashi, Jun-ichi [1 ]
Shibata, Hiromi [3 ]
Mita, Hajime [4 ]
Fukuda, Hitoshi [5 ]
Oguri, Yoshiyuki [6 ,10 ]
Kawamura, Kimitaka [2 ]
Kebukawa, Yoko [1 ]
Airapetian, Vladimir S. [7 ,8 ,9 ]
机构
[1] Yokohama Natl Univ, Grad Sch Engn Sci, Dept Chem & Life Sci, 79-5 Tokiwadai,Hodogaya Ku, Yokohama 2408501, Japan
[2] Chubu Univ, Chubu Inst Adv Studies, 1200 Matsumoto Cho, Kasugai 4878501, Japan
[3] Osaka Univ, SANKEN Inst Sci & Ind Res, Ibaraki 5670047, Japan
[4] Fukuoka Inst Technol, Fac Engn, Dept Life Environm & Appl Chem, Fukuoka 8110295, Japan
[5] Tokyo Inst Technol, Open Facil Ctr, Meguro Ku, Tokyo 1528550, Japan
[6] Tokyo Inst Technol, Inst Innovat Res, Meguro Ku, Tokyo 1528550, Japan
[7] NASA, Sellers Exoplanetary Environm Collaborat, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[8] Amer Univ, Dept Phys, Washington, DC 20016 USA
[9] Kyoto Univ, Grad Sch Adv Integrated Studies Human Survivabil, Sakyo Ku, Kyoto 6068501, Japan
[10] NAT Res Ctr, Tokai, Ibaraki 3191112, Japan
来源
LIFE-BASEL | 2023年 / 13卷 / 05期
基金
日本学术振兴会;
关键词
prebiotic synthesis; cosmic rays; solar energetic particles; weakly reducing atmosphere; early Earth; amino acids; carboxylic acids; PREBIOTIC SYNTHESIS; ABIOTIC SYNTHESIS; HYDROGEN-CYANIDE; SHOCK SYNTHESIS; ORIGIN; EARTH; LIFE; AMMONIA; CARBON; CO;
D O I
10.3390/life13051103
中图分类号
Q [生物科学];
学科分类号
07 ; 0710 ; 09 ;
摘要
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.
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页数:17
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