Transport of extraterrestrial biomolecules to the Earth: problem of thermal stability.
The idea of extraterrestrial delivery of organic matter to the early Earth is especially attractive at present and is strongly supported by the detection of a large variety of organic compounds, including amino acids and nucleobases, in carbonaceous chondrites. Whether these compounds can be delivered by other space bodies is unclear and depends primarily on capability of the biomolecules to survive high temperatures during atmospheric deceleration and impacts to the terrestrial surface. In the present study we estimated survivability of simple amino acids (alpha-aminoisobutyric acid, L-alanine, L-valine and L-leucine), purines (adenine and guanine) and pyrimidines (uracil and cytosine) under rapid heating to temperatures of 400 to 1000 degrees C under N2 or CO2 atmosphere. We have found that most of the compounds studied cannot survive the temperatures substantially higher than 700 degrees C; however at 500-600 degrees C, the recovery can be at a per cent level (or even 10%-level for adenine, uracil, alanine, and valine). Implications of the data for extraterrestrial delivery of the biomolecules are discussed.
Basiuk
V A
VA
Laboratorio de Quimica de Plasmas y Estudios Planetarios, Instituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico, Mexico. basiuk@nuclecu.unam.mx
Douda
J
J
Navarro-Gonzalez
R
R
D000225:Adenine / Q000737:chemistry; D000596:Amino Acids / Q000737:chemistry*; D019443:Cosmic Dust; D003596:Cytosine / Q000737:chemistry; D018534:Earth, Planet; D019418:Evolution, Chemical; D005118:Extraterrestrial Environment; D006147:Guanine / Q000737:chemistry; D006358:Hot Temperature; D019110:Meteoroids; D000069497:Origin of Life; D010084:Oxidation-Reduction; D010316:Particle Size; D010879:Piperazines / Q000138:chemical synthesis; D014498:Uracil / Q000737:chemistry
D000596:Amino Acids; D019443:Cosmic Dust; D010879:Piperazines; D014498:Uracil; D006147:Guanine; D003596:Cytosine; D000225:Adenine