Life in the solar system.
Life, defined as a chemical system capable of transferring its molecular information via self-replication and also capable of evolving, must develop within a liquid to take advantage of the diffusion of complex molecules. On Earth, life probably originated from the evolution of reduced organic molecules in liquid water. Organic matter might have been formed in the primitive Earth's atmosphere or near hydrothermal vents. A large fraction of prebiotic organic molecules might have been brought by extraterrestrial-meteoritic and cometary dust grains decelerated by the atmosphere. Any celestial body harboring permanent liquid water may therefore accumulate the ingredients that generated life on the primitive Earth. The possibility that life might have evolved on early Mars when water existed on the surface marks it as a prime candidate in a search for bacterial life beyond the Earth. Europa has an icy carapace. However, cryovolcanic flows at the surface point to a possible water subsurface region which might harbor a basic life form. The atmosphere and surface components of Titan are also of interest to exobiology for insight into a hydrocarbon-rich chemically evolving world. One-handed complex molecules and preferential isotopic fractionation of carbon, common to all terrestrial life forms, can be used as basic indicators when searching for life beyond the Earth.
Brack
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Centre de Biophysique Moleculaire, CNRS, Orleans, France. brack@cnrs-orleans.fr
D000596:Amino Acids / Q000737:chemistry; D001272:Atmosphere / Q000737:chemistry; D019418:Evolution, Chemical; D019143:Evolution, Molecular; D019419:Evolution, Planetary; D018559:Exobiology; D019110:Meteoroids; D000069497:Origin of Life; D012313:RNA; D016082:Solar System; D013237:Stereoisomerism; D014867:Water / Q000737:chemistry
D000596:Amino Acids; D014867:Water; D012313:RNA