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Super-chondritic Sm/Nd ratios in Mars, the Earth and the Moon

Author

Listed:
  • Guillaume Caro

    (Laboratoire Géochimie et Cosmochimie Institut de Physique du Globe de Paris—Université Denis Diderot, 4 place Jussieu, 75252 Paris Cedex 05, France)

  • Bernard Bourdon

    (Institute of Isotope Geochemistry and Mineral Resources, ETH Zurich 8092, Zurich, Switzerland)

  • Alex N. Halliday

    (University of Oxford)

  • Ghylaine Quitté

    (Laboratoire des Sciences de la Terre Ecole Normale Supérieure de Lyon)

Abstract

Inner Solar System The neodymium–samarium system boasts two useful isotopic clocks. Decay of samarium–147 to neodymium–143 is a mainstay of studies of ancient volcanic rocks. And decay of samarium–146, with a relatively short half life of 103 million years, to neodymium–142, is a high–precision tool used for dating mantle differentiation in planetary bodies. The chronology assumes, however, that the composition of the total planet is identical to that of primitive undifferentiated meteorites called chondrites. The difference in neodymium isotope ratios between chondrites and terrestrial samples may therefore indicate the early isolation of the upper mantle, or a non–chondritic bulk Earth composition. Caro et al. present high–precision neodymium isotope data for 16 martian meteorites and show that Mars also has a non–chondritic composition. This suggests that the Earth, Moon and Mars all accreted in part of the inner Solar System with an Sm/Nd ratio about 5% higher than that of material accreted in the asteroid belt, the presumed source of chondrites.

Suggested Citation

  • Guillaume Caro & Bernard Bourdon & Alex N. Halliday & Ghylaine Quitté, 2008. "Super-chondritic Sm/Nd ratios in Mars, the Earth and the Moon," Nature, Nature, vol. 452(7185), pages 336-339, March.
  • Handle: RePEc:nat:nature:v:452:y:2008:i:7185:d:10.1038_nature06760
    DOI: 10.1038/nature06760
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