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 10(exp 7) yrs. This would give a concentration of 3 x 10(exp -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 10(exp 7) yrs, which decomposes all the organic compounds. A number of workers have calculated the influx of c...
Carbon, and molecules made from it, have already been observed in the early Universe. During cosmic ...
The ions, radicals, and molecules observed in comets may be derived intact or by partial decompositi...
With growing evidence for a heavy bombardment period ending 4–3.8 billion years ago, meteorites and ...
The necessary condition for the synthesis of organic compounds on the primitive earth is the presenc...
It is proposed that the AIB amino acids at the K/T boundary were synthesized during entry of a comet...
Some primitive meteorites are carbon-rich objects containing a variety of organic molecules that con...
The role photochemical reactions in the early Earth's atmosphere played in the prebiotic synthesis o...
Stellar nucleosynthesis of heavy elements such as carbon allowed the formation of organic molecules ...
Stellar nucleosynthesis of heavy elements such as carbon allowed the formation of organic molecules ...
Aqueous chemistry within carbonaceous planetesimals is promising for synthesizing prebiotic organic ...
The synthesis of prebiotic organic compounds is a key step in the origin of life. Sources of these m...
Thirty years ago it was suggested that comets impacting on the primitive Earth may have represented ...
Comets may have been a major source of volatile elements and organic material on the early Earth. Be...
Several abiotic chemical processes acting in several different astrophysical and cosmogonic environm...
Lifeless planets with CO2 atmospheres produce CO by CO2 photolysis. On planets around M dwarfs, CO i...
Carbon, and molecules made from it, have already been observed in the early Universe. During cosmic ...
The ions, radicals, and molecules observed in comets may be derived intact or by partial decompositi...
With growing evidence for a heavy bombardment period ending 4–3.8 billion years ago, meteorites and ...
The necessary condition for the synthesis of organic compounds on the primitive earth is the presenc...
It is proposed that the AIB amino acids at the K/T boundary were synthesized during entry of a comet...
Some primitive meteorites are carbon-rich objects containing a variety of organic molecules that con...
The role photochemical reactions in the early Earth's atmosphere played in the prebiotic synthesis o...
Stellar nucleosynthesis of heavy elements such as carbon allowed the formation of organic molecules ...
Stellar nucleosynthesis of heavy elements such as carbon allowed the formation of organic molecules ...
Aqueous chemistry within carbonaceous planetesimals is promising for synthesizing prebiotic organic ...
The synthesis of prebiotic organic compounds is a key step in the origin of life. Sources of these m...
Thirty years ago it was suggested that comets impacting on the primitive Earth may have represented ...
Comets may have been a major source of volatile elements and organic material on the early Earth. Be...
Several abiotic chemical processes acting in several different astrophysical and cosmogonic environm...
Lifeless planets with CO2 atmospheres produce CO by CO2 photolysis. On planets around M dwarfs, CO i...
Carbon, and molecules made from it, have already been observed in the early Universe. During cosmic ...
The ions, radicals, and molecules observed in comets may be derived intact or by partial decompositi...
With growing evidence for a heavy bombardment period ending 4–3.8 billion years ago, meteorites and ...