Mass‐Independent Isotope Fractionation of Molybdenum and Ruthenium and the Origin of Isotopic Anomalies in Murchison
Open Access
- 20 August 2006
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 647 (2) , 1506-1516
Abstract
Dauphas et al.'s model for the nucleosynthetic origin of Mo and Ru anomalies in meteorites leaves the case of Murchison (CM2) unexplained. We explore the possibility that such a discrepancy is due to mass-independent effects controlled by nuclear field shift with, in particular, "staggering" between odd and even masses. We first demonstrate the existence of such mass-independent fractionation of Mo and Ru isotopes by chemical exchange of Mo and Ru between DC18C6 crown ether and aqueous solutions. Our results fit the nuclear field shift theory of Bigeleisen. We then review the correlation between the mean-square charge radius (which controls the nuclear field shift) and the isotopic anomalies found in an Allende CAI and in Murchison. Although Mo and Ru in the Allende CAI show a clear indication of nucleosynthetic components, the mass-independent anomalies observed in Murchison show a strong correlation with the nuclear charge distribution. We therefore argue that some isotopic anomalies observed in meteorites may be due to nuclear field shift rather than nucleosynthetic processes. Such effects are temperature dependent and may represent either genuine nebular processes or analytical artifacts. This new interpretation may help assess the existence of anomalies due to the extinct isotopes 97Tc and 98Tc.Keywords
This publication has 29 references indexed in Scilit:
- The cosmic molybdenum–ruthenium isotope correlationEarth and Planetary Science Letters, 2004
- A consistent set of nuclear rms charge radii: properties of the radius surface R(N,Z)Atomic Data and Nuclear Data Tables, 2004
- Molybdenum Stable Isotopes: Observations, Interpretations and DirectionsReviews in Mineralogy and Geochemistry, 2004
- In search of extant Tc in the early solar system: 98Ru and 99Ru abundances in iron meteorites and chondritesChemical Geology, 2003
- Molybdenum Evidence for Inherited Planetary Scale Isotope Heterogeneity of the Protosolar NebulaThe Astrophysical Journal, 2002
- Mass-dependent and mass-independent isotope effects of zinc in chemical exchange reactions using liquid chromatography with a cryptand stationary phasePhysical Chemistry Chemical Physics, 2001
- Neutron Capture in Low‐Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance SignaturesThe Astrophysical Journal, 1999
- Temperature dependence of the isotope chemistry of the heavy elements.Proceedings of the National Academy of Sciences, 1996
- Nuclear Size and Shape Effects in Chemical Reactions. Isotope Chemistry of the Heavy ElementsJournal of the American Chemical Society, 1996
- Calculation of Equilibrium Constants for Isotopic Exchange ReactionsThe Journal of Chemical Physics, 1947