A theoretical investigation of isotopic anomalies of xenon in terrestrial and extra-terrestrial samples

Details A theoretical investigation of isotopic anomalies of xenon in terrestrial and extra-terrestrial samples A theoretical investigation of isotopic anomalies of xenon in terrestrial and extra-terrestrial samples

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977stin...7811959s&link_type=abstract

Final Technical Report, 1972 - 1977 Grambling State Univ., LA. Dept. of Chemistry.

Computer Science

Meteoritic Composition, Rare Gases, Solar System, Xenon Isotopes, Argon Isotopes, Isotopes, Krypton Isotopes, Supernova Remnants

Scientific paper

The abundance and isotopic composition of noble gases in meteorites is discussed in relation to the composition of the early solar system. Carbonaceous chondrites contain a unique Xenon-X, which is rich in heavy and light isotopes. Variations in the occurrence of type-X and type-Y (the normal component) noble gases are of such magnitude that neither the injection of material from a nearby supernova nor presence of presolar grains can account for the anomalies in meteorites. Therefore, it is suggested that the entire solar system may have condensed from the debris of a single local supernova.

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