The relative importance of prebiotic synthesis on the Earth and input from comets and meteorites

Details The relative importance of prebiotic synthesis on the Earth and input from comets and meteorites The relative importance of prebiotic synthesis on the Earth and input from comets and meteorites

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ceol.symp..105m&link_type=abstract

In NASA, Washington, Fourth Symposium on Chemical Evolution and the Origin and Evolution of Life p 105 (SEE N92-13588 04-55)

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Atmospheric Chemistry, Atmospheric Composition, Comets, Electric Discharges, Formaldehyde, Hydrocyanic Acid, Meteoritic Composition, Photochemical Reactions, Reaction Kinetics, Amino Acids, Carbon Dioxide, Carbon Monoxide, Cretaceous-Tertiary Boundary, Methane, Organic Materials, Sediments, Water

Scientific paper

The prebiotic synthesis of hydrogen cyanide and formaldehyde was studied by the action of electric discharges on various model primitive atmospheres containing CH4, CO, and CO2. Photochemical production rates would also have been important and were calculated for HCN and H2CO. A reasonable rate of synthesis of amino acids from these sources is about 10 n moles/(sq cm yr) or 0.10 moles/sq cm in 107 yrs. This would give a concentration of 3 x 10-4 M in an ocean of the present size (300 liters/sq cm). The amino acids cannot accumulate over a longer period because the entire ocean passes through the 350 C submarine vents in 107 yrs, which decomposes all the organic compounds. A number of workers have calculated the influx of comets and meteorites on the primitive earth, both as a destructive process for organic compounds and for any life that was present, as well as a source of organic compounds. Some of the amino acids from the meteorite proposed to have hit the earth 65 x 106 yrs ago were detected at the Cretaceous/Tertiary boundary sediments. The problem with proposing a large scale input of organic compounds from meteorites and comets is that they must survive passage through the atmosphere and impact. There are some processes that would allow survival such as showers of centimeter to meter sized meteorites and various aerodynamic braking processes for larger objects. Even if a significant amount of the organic material survived impact, the destructive processes in the hydrothermal vents would remove these compounds on the average in 107 yrs or less. If it is assumed that the input rate was sufficient to overcome these destructive processes, then too much carbon and water, especially from comets, would have been added to the surface of the earth. It was concluded that while some organic material was added to the earth from comets and meteorites, the amount available from these sources at a given time was only a few percent of that from earth based syntheses.

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