Silicon in iron meteorite metal |
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| Authors: | Andreas PACK Ingo VOGEL Claire ROLLION‐BARD Béatrice LUAIS Herbert PALME |
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| Affiliation: | 1. Centre de Recherches Pétrographiques et Géochimiques (CRPG‐CNRS), 15 rue Notre Dame des Pauvres, F–54501 Vand?uvre‐lès‐Nancy, France;2. Institut für Mineralogie, Universit?t Hannover, Callinstra?e 3, D‐30167 Hannover, Germany;3. Geowissenschaftliches Zentrum, Abteilung Isotopengeologie, Georg‐August‐Universit?t, Goldschmidtstra?e 1, D‐37077 G?ttingen, Germany;4. Insitut für Geologie und Mineralogie, Universit?tzu K?ln, Zülpicher Stra?e 49b, D‐50674 K?ln, Germany;5. Senckenberg Forschungsinstitut und Naturmuseum, Senckenberganlage 25, D‐60325 Frankfurt am Main, Germany |
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| Abstract: | Abstract– We report Si concentrations in the metal phases of iron meteorites. Analyses were performed by secondary ion mass spectrometry using a CAMECA 1270 ion probe. The Si concentrations are low (0.09–0.46 μg g?1), with no apparent difference in concentration between magmatic and nonmagmatic iron meteorites. Coexisting kamacite and Ni‐rich metal phases have similar Si contents. Thermodynamic calculations show that Fe,Ni‐metal in equilibrium with silicate melts at temperatures where metal crystallizes should contain approximately 100 times more Si than found in iron meteorites in this work. The missing Si may either occur as tiny silicate inclusions in metal or it may have diffused as Si‐metal into surrounding silicates at low temperatures. In both cases, extensive low‐temperature diffusion of Si in metal is required. It is therefore concluded that low Si in iron meteorites is a result of subsolidus reactions during slow cooling. |
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