
table of contents ![]() Study showing that a CO-CO2-N2-H2O atmosphere can give a … |
Biology Articles » Evolutionary Biology » Origin of Life » Prebiotic synthesis from CO atmospheres: Implications for the origins of life » Table
Table
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C yields, carbon yields; E yields, energy yields; PI, proton irradiation; HTPD, high-temperature plasma discharge; ED, electric discharge; Ura, uracil; Cyt, cytosine; Gua, guanine; Ade, adenine; Oro, orotic acid; HUra, 5-hydroxyuracil; 45DHPy, 4,5-dihydroxypyrimidine; Nic, nicotinic acid; Im, imidazole; Gly, glycine; Asp, aspartic acid; Ser, serine; Ala, alanine;
-Ala,
-alanine; Sar, sarcosine; Glygly, glycylglycine.
* The gas mixture had been irradiated for 3 h.
The carbon yields were calculated from the percentage of carbon in products based on carbon in synthesized polymers.
CO2 produced from a reaction of CO and H2O was continuously removed with Ca(OH)2 during discharge.
A CO-N2-H2O gas mixture was irradiated with 40 MeV protons generated from an SF cyclotron (Institute for Nuclear Study, University of Tokyo). Total deposited energy was 3.9 kJ. The amino acids were identified by GC/MS.
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