Published October 7, 2014 | Version v1
Journal article

A new feature in the internal heavy isotope distribution in ozone

  • 1. Research Center for Environmental Changes, Academia Sinica, Taipei, Taiwan (China)
  • 2. Laboratoire de Glaciologie et Géophysique de l'Environnement, CNRS, Université Joseph Fourier-Grenoble, 54 rue Molière BP96, St Martin d'Heres, 38402 (France)
  • 3. Department of Earth and Atmospheric Sciences, Purdue University, Indiana 47906 (United States)

Description

Ozone produced by discharge or photolysis of oxygen has unusually heavy isotopic composition (18O/16O and 17O/16O ratio) which does not follow normal mass fractionation rule: δ17O ∼ 0.52*δ18O, expressed as an anomaly Δ17O = δ17O − 0.52*δ18O. Ozone molecule being an open isosceles triangle can have the heavy isotope located either in its apex or symmetric (s) position or the base or asymmetric (as) position. Correspondingly, one can define positional isotopic enrichment, written as δ18O (s) or δ18O (as) (and similarly for δ17O) as well as position dependent isotope anomaly Δ17O (s) and Δ17O (as). Marcus and co-workers have proposed a semi-empirical model based in principle on the RRKM model of uni-molecular dissociation but with slight modification (departure from statistical randomness assumption for symmetrical molecules) which explains many features of ozone isotopic enrichment. This model predicts that the bulk isotope anomaly is contained wholly in the asymmetric position and the Δ17O (s) is zero. Consequently, Δ17O (as) = 1.5 * Δ17O (bulk) (named here simply as the "1.5 rule") which has been experimentally confirmed over a range of isotopic enrichment. We now show that a critical re-analysis of the earlier experimental data demonstrates a small but significant departure from this 1.5 rule at the highest and lowest levels of enrichments. This departure provides the first experimental proof that the dynamics of ozone formation differs from a statistical model constrained only by restriction of symmetry. We speculate over some possible causes for the departure

Additional details

Identifiers

Publishing Information

Journal Title
Journal of Chemical Physics
Journal Volume
141
Journal Issue
13
Journal Page Range
p. 134301-134301.15
ISSN
0021-9606
CODEN
JCPSA6

Optional Information

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