دورية أكاديمية

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

التفاصيل البيبلوغرافية
العنوان: Formation of Amino Acids and Carboxylic Acids in Weakly Reducing Planetary Atmospheres by Solar Energetic Particles from the Young Sun.
المؤلفون: Kobayashi K; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Ise JI; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Aoki R; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Kinoshita M; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Naito K; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Udo T; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Kunwar B; Chubu Institute of Advanced Studies, Chubu University, 1200 Matsumoto-cho, Kasugai 487-8501, Japan., Takahashi JI; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Shibata H; SANKEN (The Institute of Scientific and Industrial Research), Osaka University, Ibaraki 567-0047, Japan., Mita H; Department of Life, Environment and Applied Chemistry, Faculty of Engineering, Fukuoka Institute of Technology, Fukuoka 811-0295, Japan., Fukuda H; Open Facility Center, Tokyo Institute of Technology, Meguro-ku, Tokyo 152-8550, Japan., Oguri Y; Institute of Innovative Research, Tokyo Institute of Technology, Tokyo Institute of Technology, Meguro-ku, Tokyo 152-8550, Japan., Kawamura K; Chubu Institute of Advanced Studies, Chubu University, 1200 Matsumoto-cho, Kasugai 487-8501, Japan., Kebukawa Y; Department of Chemistry and Life Science, Graduate School of Engineering Science, Yokohama National University, 79-5 Tokiwadai, Hodogaya-ku, Yokohama 240-8501, Japan., Airapetian VS; NASA Goddard Space Flight Center/Sellers Exoplanetary Environments Collaboration, Greenbelt, MD 20771, USA.; Department of Physics, American University, Washington, DC 20016, USA.; Graduate School of Advanced Integrated Studies in Human Survivability, Kyoto University, Sakyo-ku, Kyoto 606-8501, Japan.
المصدر: Life (Basel, Switzerland) [Life (Basel)] 2023 Apr 28; Vol. 13 (5). Date of Electronic Publication: 2023 Apr 28.
نوع المنشور: Journal Article
اللغة: English
بيانات الدورية: Publisher: MDPI AG Country of Publication: Switzerland NLM ID: 101580444 Publication Model: Electronic Cited Medium: Print ISSN: 2075-1729 (Print) Linking ISSN: 20751729 NLM ISO Abbreviation: Life (Basel) Subsets: PubMed not MEDLINE
أسماء مطبوعة: Original Publication: Basel, Switzerland : MDPI AG, 2011-
مستخلص: 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.
References: Orig Life Evol Biosph. 1992;20:199-231. (PMID: 11537523)
Orig Life Evol Biosph. 1987;17(3-4):261-73. (PMID: 2819806)
Space Sci Rev. 2020;216(8):143. (PMID: 33328695)
Astrobiology. 2018 Mar;18(3):343-364. (PMID: 29570409)
Orig Life Evol Biosph. 1985;16(1):57-67. (PMID: 4094752)
ACS Cent Sci. 2022 Dec 28;8(12):1664-1671. (PMID: 36589881)
Science. 1971 Jul 30;173(3995):417-20. (PMID: 17770442)
Proc Natl Acad Sci U S A. 2002 Nov 12;99(23):14628-31. (PMID: 12409606)
Proc Natl Acad Sci U S A. 2020 Jun 16;117(24):13267-13274. (PMID: 32487725)
Sci Adv. 2020 Feb 26;6(9):eaax1420. (PMID: 32133393)
Nature. 2012 May 16;485(7399):478-81. (PMID: 22622572)
Orig Life Evol Biosph. 2002 Jun;32(3):195-208. (PMID: 12227424)
Astrobiology. 2021 Dec;21(12):1479-1493. (PMID: 34793260)
Orig Life Evol Biosph. 1992;22(1-4):67-107, 191-242. (PMID: 11537554)
Philos Trans A Math Phys Eng Sci. 2017 May 28;375(2094):. (PMID: 28416728)
Astrobiology. 2014 Apr;14(4):308-43. (PMID: 24697642)
Life (Basel). 2018 May 10;8(2):. (PMID: 29748464)
Sci Adv. 2022 Mar 25;8(12):eabi9743. (PMID: 35333577)
Angew Chem Int Ed Engl. 2015 Aug 17;54(34):9871-5. (PMID: 26201989)
Science. 1951 Oct 19;114(2964):416-8. (PMID: 14892746)
Astrobiology. 2017 Aug;17(8):786-812. (PMID: 28727932)
Science. 1971 Oct 1;174(4004):53-5. (PMID: 17755695)
Acc Chem Res. 2012 Dec 18;45(12):2025-34. (PMID: 22455515)
Astrobiology. 2020 Sep;20(9):1121-1149. (PMID: 32876492)
Science. 1970 Apr 24;168(3930):470-3. (PMID: 5436082)
Proc Natl Acad Sci U S A. 1963 May;49(5):737-40. (PMID: 16591096)
Science. 1999 Jan 29;283(5402):674-6. (PMID: 9924024)
Proc Natl Acad Sci U S A. 2015 Apr 7;112(14):4245-50. (PMID: 25831544)
J Mol Evol. 1983;19(5):376-82. (PMID: 6417344)
J Mol Evol. 1984;21(1):76-80. (PMID: 6442361)
Astrophys J. 2019 Aug 3;880(2):. (PMID: 32214410)
Life (Basel). 2018 Nov 04;8(4):. (PMID: 30400350)
Nature. 1992 Jan 9;355:125-32. (PMID: 11538392)
Science. 1953 May 15;117(3046):528-9. (PMID: 13056598)
Science. 1959 Jul 31;130(3370):245-51. (PMID: 13668555)
Medicina (B Aires). 2016;76(4):199-203. (PMID: 27576276)
J Mol Evol. 1983;19(5):383-90. (PMID: 6315963)
Anal Sci. 2013;29(8):777-85. (PMID: 23934557)
Nature. 1970 Dec 5;228(5275):923-6. (PMID: 5482102)
Astrobiology. 2020 Apr;20(4):429-452. (PMID: 31841362)
Chem Rev. 2020 Jun 10;120(11):4707-4765. (PMID: 32101414)
Nature. 1964 Jan 25;201:335-6. (PMID: 14109988)
Cold Spring Harb Perspect Biol. 2010 Oct;2(10):a004895. (PMID: 20573713)
Nature. 1995 Jun 29;375(6534):772-4. (PMID: 7596408)
Orig Life Evol Biosph. 1998 Apr;28(2):155-65. (PMID: 11536862)
Life (Basel). 2021 Jun 09;11(6):. (PMID: 34207658)
Crit Rev Biochem Mol Biol. 2004 Mar-Apr;39(2):99-123. (PMID: 15217990)
Orig Life Evol Biosph. 2012 Dec;42(6):533-41. (PMID: 22949128)
معلومات مُعتمدة: 19K21895, 19H01955, JP21K18648, JP21H00036 and 24221001, JPJSJRP 20181601 Japan Society for the Promotion of Science
فهرسة مساهمة: Keywords: amino acids; carboxylic acids; cosmic rays; early Earth; prebiotic synthesis; solar energetic particles; weakly reducing atmosphere
تواريخ الأحداث: Date Created: 20230527 Latest Revision: 20230530
رمز التحديث: 20230530
مُعرف محوري في PubMed: PMC10221653
DOI: 10.3390/life13051103
PMID: 37240748
قاعدة البيانات: MEDLINE