2002
DOI: 10.1073/pnas.192568299
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Prebiotic synthesis from CO atmospheres: Implications for the origins of life

Abstract: Most models of the primitive atmosphere around the time life originated suggest that the atmosphere was dominated by carbon dioxide, largely based on the notion that the atmosphere was derived via volcanic outgassing, and that those gases were similar to those found in modern volcanic effluent. These models tend to downplay the possibility of a strongly reducing atmosphere, which had been thought to be important for prebiotic synthesis and thus the origin of life. However, there is no definitive geologic evide… Show more

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Cited by 144 publications
(112 citation statements)
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References 56 publications
(63 reference statements)
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“…The microbial metabolism of CO is an important component of the global carbon cycle (1,2), and CO is believed to have been present in the atmosphere of early Earth that fueled the evolution of primitive metabolisms (3)(4)(5)(6)(7). Investigations of aerobic species from the Bacteria domain have contributed important insights into microbial CO oxidation (8,9), as have investigations of anaerobes from the Bacteria domain that conserve energy by coupling CO oxidation to H 2 evolution (10)(11)(12).…”
mentioning
confidence: 99%
“…The microbial metabolism of CO is an important component of the global carbon cycle (1,2), and CO is believed to have been present in the atmosphere of early Earth that fueled the evolution of primitive metabolisms (3)(4)(5)(6)(7). Investigations of aerobic species from the Bacteria domain have contributed important insights into microbial CO oxidation (8,9), as have investigations of anaerobes from the Bacteria domain that conserve energy by coupling CO oxidation to H 2 evolution (10)(11)(12).…”
mentioning
confidence: 99%
“…Since Miller's initial publication, many laboratories have replicated and extended his results, exploring variations on the synthesis using other types of apparatus designs, gas mixtures and energy sources (Groth and Weyssenhoff 1957;Menor-Salvan et al 2009;Miller 1957aMiller , 1957bMiyakawa et al 2002aMiyakawa et al , 2002bMiyakawa et al , 2002cParker et al 2010Parker et al , 2011Ring et al 1972;Miller 1983a, 1983b), demonstrating the synthesis of a much wider variety of organic compounds. There is a consensus of the types of products obtained using similar gases, though there are important differences in the C and energy yields of various intermediate species such as HCHO and HCN (Miller and Schlesinger 1984) depending on the energy source and gas mixture used (Heinrich et al 2007), factors independent of surface conditions.…”
Section: Variations Of the Miller/urey Experiments With Respect To Thementioning
confidence: 99%
“…At low fluxes, compounds such as HCN may hydrolyze to less complex species faster than they undergo reactions that produce biologically interesting molecules (Miyakawa et al 2002a(Miyakawa et al , 2002b(Miyakawa et al , 2002c, with the specific rates depending on aqueous temperature and pH conditions. Thus, terrestrial surface conditions may also have been important factors when considering the efficiency of atmospherically-mediated organic synthesis on the primitive Earth.…”
Section: The Miller/urey Experimentsmentioning
confidence: 99%
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“…For example, more oxidized gas mixtures can be used 14,18,19 . Furthermore, using modifications of the apparatus, the energy source can be changed, for example, by using a silent discharge 4 , ultraviolet light 20 , simulating volcanic systems 4,12,21 , imitating radioactivity from Earth's crust 22 , and mimicking energy produced by shockwaves from meteoritic impacts 23 , and also cosmic radiation 18,19 .…”
Section: Introduction Of Nmentioning
confidence: 99%