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Laboratoire de Géologie de Lyon |  |
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Laboratoire de Géologie de Lyon | |
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| HAL : hal-00684109, version 1 |
| DOI : 10.1126/science.1219509 |
| Fiche détaillée |  Récupérer au format |
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| Science 335, 6075 (2012) 1477-1480 |
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| Silicon Isotope Evidence Against an Enstatite Chondrite Earth |
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Caroline Fitoussi 1, 2Bernard Bourdon 1, 2 |
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| (03/2012) |
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| The compositions of Earth materials are strikingly similar to those of enstatite chondrite meteorites in many isotope systems. Although this suggests that Earth largely accreted from enstatite chondrites, definitive proof of this model has been lacking. By comparing the silicon (Si) isotope signatures of several extraterrestrial materials with terrestrial samples, we show that they cannot be explained by core-formation scenarios involving a bulk Earth of enstatite chondrite composition. Si isotope similarities between the bulk silicate Earth and the Moon preclude the existence of a hidden reservoir in the lower mantle, a necessary condition of the enstatite chondrite model, and require an equilibrium process after the Moon-forming impact. A three-end-member chondritic mixing model for Earth reconciles the Si isotope similarities between enstatite chondrites and Earth. |
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| 1 : | Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE) |
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CNRS : UMR5276 – INSU – Université Claude Bernard - Lyon I – École Normale Supérieure - Lyon |
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| 2 : | Institute of Geochemistry and Petrology |
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Swiss Federal Institute of Technology in Zurich (ETH Zurich). |
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| Domaine | : | Planète et Univers/Sciences de la Terre |
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| FORMING GIANT IMPACT – INNER SOLAR-SYSTEM – OXYGEN-ISOTOPE – CORE FORMATION – CHEMICAL-COMPOSITION – ACCRETION – HETEROGENEITY – ELEMENTS – MODELS – METAL |
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| hal-00684109, version 1 | |
| http://hal.archives-ouvertes.fr/hal-00684109 | |
| oai:hal.archives-ouvertes.fr:hal-00684109 | |
| Contributeur : Marie Chebance | |
| Soumis le : Vendredi 30 Mars 2012, 15:34:59 | |
| Dernière modification le : Lundi 14 Mai 2012, 09:46:56 | |
