Computer Science
Scientific paper
Jul 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987gecoa..51.2011y&link_type=abstract
Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 51, July 1987, p. 2011-2017. Research supported by the Korea Science and
Computer Science
10
Chemical Fractionation, Gas Discharges, Isotope Effect, Meteoritic Composition, Oxygen Isotopes, Ozone, Chemical Reactions, Molecular Gases, Oxygen 17, Oxygen 18, Symmetry
Scientific paper
Isotopic fractionation processes in the formation of O3 by 20-kV 60-kHz discharge of O2 in a fused silica container at 77 K are investigated experimentally, with a focus on the effects of changes in the isotopic composition of O2, the O2 pressure, the degree of O3 formation, and the discharge geometry on the isotope abundances in the postdischarge O2 and O3. The results are presented in tables and graphs and compared with the predictions of theoretical models involving vibrational anharmonicity and symmetry effects on O3 predissociation. In experiments using O2 enriched with O-17 and O-18, the heavy isotope is enriched in the residual O2 and not in the O3, whereas the opposite is true when atmospheric isotope abundances are used. It is inferred that the predissociation rate depends on the symmetry and mass of the O3 molecules and not on self-shielding or symmetry effects in the reactant O2. The potential value of the present findings for studies of anomalous isotope abundances in meteorites is indicated.
Epstein Samuel
Yang Jongmann
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