Chemical evolution of primitive solar system bodies.
In this paper we summarize some of the most salient observations made recently on the organic molecules and other compounds of the biogenic elements present in the interstellar medium and in the primitive bodies of the solar system.  They include the discovery of the first phosphorus molecular species in dense interstellar clouds, the presence of complex organic ions in the dust and gas phase of Halley's coma, the finding of unusual, probably presolar, deuterium-hydrogen ratios in the amino acids of carbonaceous chondrites, and new developments on the chemical evolution of Titan, the primitive Earth, and early Mars.  Some of the outstanding problems concerning the synthesis of organic molecules on different cosmic bodies are also discussed from an exobiological perspective.
Oró
J
J
Department of Biochemical and Biophysical Sciences, The University of Houston, TX 77004.
Mills
T
T
D000596:Amino Acids / Q000032:analysis / Q000138:chemical synthesis; D002625:Chemistry, Organic; D018534:Earth, Planet; D018559:Exobiology; D005118:Extraterrestrial Environment; D018535:Mars; D018543:Minor Planets; D055601:Organic Chemistry Phenomena; D000069497:Origin of Life; D018539:Saturn; D016082:Solar System; D013026:Space Flight
D000596:Amino Acids