2023
DOI: 10.1089/ast.2023.0007
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The Origin and Early Evolution of Life: Homochirality Emergence in Prebiotic Environments

Carolina Chieffo,
Anastasiia Shvetsova,
Fryni Skorda
et al.
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Cited by 6 publications
(23 citation statements)
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“…Feature 1: Carbon is abundant on Earth. It has been estimated that the atmosphere, water bodies, and biosphere on Earth contain 9×10 11 , 36×10 11 , and 5.5×10 11 tons of carbon, respectively [23,24]. There is also abundant carbon in stones, coals, petroleum, natural gas, and methane hydrates on Earth.…”
Section: Special Features Of H0-cbss (Carbon Atoms)mentioning
confidence: 99%
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“…Feature 1: Carbon is abundant on Earth. It has been estimated that the atmosphere, water bodies, and biosphere on Earth contain 9×10 11 , 36×10 11 , and 5.5×10 11 tons of carbon, respectively [23,24]. There is also abundant carbon in stones, coals, petroleum, natural gas, and methane hydrates on Earth.…”
Section: Special Features Of H0-cbss (Carbon Atoms)mentioning
confidence: 99%
“…Figure 1 illustrates how simple CBSs, along with other substances, can form complex CBSs due to energy absorption. Certain H1-CBSs, such as HCN, CO2, and CH4, along with other materials, form H2-CBSs, like amino acids, nucleotides, and monosaccharides, through some energy-absorbing organic synthesis reactions under the laws of thermodynamics and organic chemistry [6][7][8][9][10][11][12][13][14][15]. Similarly, certain H2-CBSs, along with other materials, form H3-CBSs, like proteins, nucleic acids, and lipids, through some energy-absorbing organic synthesis reactions under the laws of thermodynamics and organic chemistry [7][8][9].…”
Section: The Driving Force Mechanismmentioning
confidence: 99%
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