Search for organic molecules in the outer solar system.
Recent developments of millimeter astronomy have led to the discovery of more and more complex molecules in the interstellar medium. In a similar way, attempts have been made to detect complex molecules in the atmospheres of the most primitive bodies of the Solar System, i.e. outer planets and comets, as well as in Titan's atmosphere. An important progress has been achieved thanks to the continuous development of infrared astronomy, from the ground and from space vehicles. In particular, an important contribution has come from the IRIS-Voyager infrared spectrometer with the detection of prebiotic molecules on Titan, and some complex organic molecules on Jupiter and Saturn. Another important result has been the observation of carbonaceous material in the immediate surroundings of Comet Halley's nucleus. In the near future, the search for organic molecules in the outer Solar System should benefit from the developments of large millimeter antennae, and in the next decade, from the operation of infrared Earth-orbiting spacecrafts (ISO, SIRTF).
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Observatoire de Paris-Meudon, Meudon, France.
D001256:Astronomy / Q000295:instrumentation / Q000379:methods*; D001272:Atmosphere / Q000032:analysis / Q000737:chemistry*; D018559:Exobiology / Q000295:instrumentation / Q000379:methods; D005118:Extraterrestrial Environment; D005740:Gases / Q000032:analysis / Q000737:chemistry*; D018538:Jupiter; D019110:Meteoroids; D018541:Neptune; D018539:Saturn; D016082:Solar System; D013055:Spectrophotometry, Infrared; D018540:Uranus
D005740:Gases