title: From the interstellar clouds, through the inner to the outer solar system: a universally distributed complex organic chemistry. Preface.
abstract: High molecular weight organic compounds are involved in the chemistry and physics of many astrophysical and planetary objects. They are or should be present in interstellar dust, in comets and meteorites, in the Giant planets and Titan, in asteroids Triton and icy satellites. They represent a class of very complex organic material, part of which may have played a role in the origin of life on Earth. Thus they directly concern prebiotic chemistry and exobiology.
authors.affiliation: LISA, CNRS and Universites, Paris, France.
authors.forename: F
authors.initials: F
authors.lastname: Raulin
authors.forename: J M
authors.initials: JM
authors.lastname: Greenberg
mesh_terms: D019443:Cosmic Dust; D019418:Evolution, Chemical; D018559:Exobiology; D005118:Extraterrestrial Environment; D019110:Meteoroids; D009930:Organic Chemicals / Q000032:analysis* / Q000737:chemistry; D016082:Solar System
chemical_list: D019443:Cosmic Dust; D009930:Organic Chemicals