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

Guillaume Caro (), Bernard Bourdon, Alex N. Halliday and Ghylaine Quitté
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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

Nature, 2008, vol. 452, issue 7185, 336-339

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.

Date: 2008
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DOI: 10.1038/nature06760

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