The contribution of cometary volatiles to the primitive Earth.
It has been estimated that during its early history the Earth captured a mass of cometary material of the order of 10(23) grams. Since carbon is supposed to be at least three times more abundant in comets than in carbonaceous chondrites (3.5% C in C 1 chondrites), it can be deduced that about 1 x 10(22) grams of carbon (as carbon compounds), was added by comets to the surface of the prebiotic Earth. This carbon value is of the same order of magnitude as the value of the organic carbon buried in the Earth's sedimentary shell, but approximately one order of magnitude lower than the Earth's surface total carbon (7 x 10(22) gm). The capture of comets by the Earth would also have contributed to generating the appropriate aqueous and reducing environmental conditions necessary for organic synthesis. Although it is possible that some of the cometary carbon compounds falling on the Earth survived, most of them were probably decomposed by the heat and shock waves of the cometary collision. Upon quenching to low temperatures, however, the reactive chemical species produced by the impact would have recombined, leading to the synthesis of a great variety of organic molecules. Laboratory experiments with radiation, heat and shock waves have demonstrated that some of the synthesized compounds are biochemical molecules: amino acids, sugars, purines, and pyrimidines. These are essential to all living systems.
Oro
J
J
Departments of Biophysical Sciences and Chemistry, University of Houston, Houston, Texas 77004, USA.
Holzer
G
G
Lazcano-Araujo
A
A
D002244:Carbon / Q000737:chemistry*; D018534:Earth, Planet; D019418:Evolution, Chemical; D005118:Extraterrestrial Environment / Q000737:chemistry*; D006859:Hydrogen / Q000737:chemistry; D019110:Meteoroids; D000069497:Origin of Life; D016082:Solar System; D014867:Water / Q000737:chemistry
D014867:Water; D002244:Carbon; D006859:Hydrogen