Organic Hazes as a Source of Life's Building Blocks to Warm Little Ponds on the Hadean Earth

被引:3
作者
Pearce, Ben K. D. [1 ]
Horst, Sarah M. [1 ]
Sebree, Joshua A. [2 ]
He, Chao [1 ,3 ]
机构
[1] Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21218 USA
[2] Univ Northern Iowa, Dept Chem & Biochem, Cedar Falls, IA 50614 USA
[3] Univ Sci & Technol China, Sch Earth & Space Sci, Hefei, Peoples R China
来源
PLANETARY SCIENCE JOURNAL | 2024年 / 5卷 / 01期
基金
加拿大自然科学与工程研究理事会;
关键词
TITAN THOLINS; AMINO-ACIDS; SUPER-EARTH; ATMOSPHERE; CHEMISTRY; HYDROLYSIS; MOLECULES; EVOLUTION; ORIGIN; BASES;
D O I
10.3847/PSJ/ad17bd
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Over 4 billion years ago, Earth is thought to have been a hazy world akin to Saturn's moon Titan. The organic hazes in the atmosphere at this time could have contained a vast inventory of life's building blocks and thus may have seeded warm little ponds for life. In this work, we produce organic hazes in the lab in atmospheres with high (5%) and low (0.5%) CH4 abundances and analyze the solid particles for nucleobases, amino acids, and a few other organics using GC/MS/MS to obtain their concentrations. We also analyze heated (200 degrees C) samples from the high methane organic haze experiment to simulate these particles sitting on an uninhabitable surface. Finally, we use our experimental results and estimates of atmospheric haze production as inputs for a comprehensive numerical pond model to calculate the concentrations of nucleobases from organic hazes in these environments. We find that organic hazes typically provide up to 0.2-6.5 mu M concentrations of nucleobases to warm little ponds for potentially habitable Hadean conditions. However, without seepage, uracil and thymine can reach similar to 100 mu M concentrations, which is the present lower experimental limit to react these species to form nucleotides. Heating samples leads to partial or complete decay of biomolecules, suggesting that biomolecule stockpiling on the hot surface is unlikely. The ideal conditions for the delivery of life's building blocks from organic hazes would be when the Hadean atmosphere is rich in methane, but not so rich as to create an uninhabitable surface.
引用
收藏
页数:20
相关论文
共 44 条
[21]   Haze production rates in super-Earth and mini-Neptune atmosphere experiments [J].
Horst, Sarah M. ;
He, Chao ;
Lewis, Nikole K. ;
Kempton, Eliza M. -R. ;
Marley, Mark S. ;
Morley, Caroline V. ;
Moses, Julianne I. ;
Valenti, Jeff A. ;
Vuitton, Veronique .
NATURE ASTRONOMY, 2018, 2 (04) :303-306
[22]   Nucleic acid bases in Titan tholins and possible genetic systems in the Titan liquidosphere [J].
Kawai, Jun ;
Kebukawa, Yoko ;
McKay, Christopher P. ;
Kobayashi, Kensei .
LIFE SCIENCES IN SPACE RESEARCH, 2019, 20 :20-29
[23]   THE FORMATION OF ORGANIC COMPOUNDS ON THE PRIMITIVE EARTH [J].
MILLER, SL .
ANNALS OF THE NEW YORK ACADEMY OF SCIENCES, 1957, 69 (02) :260-275
[24]   A wet heterogeneous mantle creates a habitable world in the Hadean [J].
Miyazaki, Yoshinori ;
Korenaga, Jun .
NATURE, 2022, 603 (7899) :86-+
[25]   Chemistry of Temperate Super-Earth and Mini-Neptune Atmospheric Hazes from Laboratory Experiments [J].
Moran, Sarah E. ;
Horst, Sarah M. ;
Vuitton, Veronique ;
He, Chao ;
Lewis, Nikole K. ;
Flandinet, Laurene ;
Moses, Julianne, I ;
North, Nicole ;
Orthous-Daunay, Francois-Regis ;
Sebree, Joshua ;
Wolters, Cedric ;
Kempton, Eliza M-R ;
Marley, Mark S. ;
Morley, Caroline, V ;
Valenti, Jeff A. .
PLANETARY SCIENCE JOURNAL, 2020, 1 (01)
[26]   Titan's Primordial Soup: Formation of Amino Acids via Low-Temperature Hydrolysis of Tholins [J].
Neish, Catherine D. ;
Somogyi, Arpad ;
Smith, Mark A. .
ASTROBIOLOGY, 2010, 10 (03) :337-347
[28]  
Pavlov AA, 2001, GEOLOGY, V29, P1003, DOI 10.1130/0091-7613(2001)029<1003:OHIESE>2.0.CO
[29]  
2
[30]  
Pearce B. K. D., 2023, Wet Dry Cycling Numerical Pond Model, DOI [10.5281/zenodo.10210594, DOI 10.5281/ZENODO.10210594]