Origin of organic compounds in carbonaceous chondrites.
Carbonaceous chondrites, a class of primitive meteorite, have long been known to contain their complement of carbon largely in the form of organic, i.e., hydrocarbon-related, matter.  Both discrete organic compounds and an insoluble, macromolecular material are present.  Several characteristics of these materials provide evidence for their abiotic origin.  The principal formation hypotheses have invoked chemistry occurring either in the solar nebula or on the parent body.  However, recent stable isotope analyses of the meteorite carboxylic acids and amino acids indicate that they may be related to interstellar cloud compounds.  These results suggest a formation scheme in which interstellar compounds were incorporated into the parent body and subsequently converted to the present suite of meteorite organics by the hydrothermal process believed to have formed the clay minerals of the meteorite matrix.
Cronin
J R
JR
Department of Chemistry, Arizona State University, Tempe 85287-1604, USA.
D000596:Amino Acids / Q000032:analysis*; D002244:Carbon / Q000032:analysis*; D055598:Chemical Phenomena; D002621:Chemistry; D003903:Deuterium / Q000032:analysis*; D018559:Exobiology; D005118:Extraterrestrial Environment; D006838:Hydrocarbons / Q000032:analysis*; D019110:Meteoroids
D000596:Amino Acids; D006838:Hydrocarbons; D002244:Carbon; D003903:Deuterium