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Titel Experimental study of carbonate-silicate-metal equilibria at pressures to 30 GPa: New insights into deep volatile cycles
VerfasserIn Konstantin Litasov, Anton Shatskiy, Yingwei Fei, Eiji Ohtani
Konferenz EGU General Assembly 2010
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 12 (2010)
Datensatznummer 250038165
 
Zusammenfassung
Carbon and hydrogen are among the most important, but uncertain constituents in the Earth’s deep interior. In this presentation we will review resent results on carbonate-silicate-metal equilibria at pressures up to about 30 GPa using multianvil technique. In situ X-ray diffraction experiments were performed at the synchrotron radiation facility SPring-8. We have studied the following systems: MgCO3+SiO2, CaCO3+SiO2, MgCO3+Fe, and CaCO3+Fe. Preliminary results from in situ measurements for the MgCO3+H2O+Fe and CaCO3+H2O+Fe systems and from laboratory experiments on peridotite and eclogite, coexisting with ultra-reduced C-O-H fluids, will also be discussed. The reaction of MgCO3+SiO2 = MgSiO3+CO2 was studied using both the multianvil and diamond anvil cell (DAC) technique. We observed melting reaction at pressures up to about 32 GPa. Decarbonation was observed at pressures below 6 GPa and, surprisingly, in the short pressure interval of wadsleyite + stishovite stability (in MgSiO3 system) near 16 GPa. In all other experiments reaction proceeds with the formation of MgSiO3 phase and melt. The Mg/Si ratio of partial melt, coexisting with Mg-perovskite, was 1.7-2.0, whereas at lower pressures this ratio is 2.3-2.5. Formation of Mg-perovskite was observed in DAC experiments at pressures 25-100 GPa, however, CO2 was not detected by in situ X-ray diffraction or in situ Raman spectroscopy, which may indicate melting reaction at higher pressure also. The reaction CaCO3+SiO2 = CaSiO3+CO2 was studied at pressures 3-22 GPa. In contrast to the Mg-system we observed the formation of CO2 fluid at 6-10 GPa and melting at 16-17 GPa. The partial melt has a Ca/Si ratio of 2.3-3.0. The reactions MgCO3+Fe and CaCO3+Fe were also studied at 6 and 15-16 GPa. We observed fast formation of Fe3C in the Mg-system at 900-1000oC, according to the reaction MgCO3+5Fe=Fe3C+3(Fe0.67Mg0.33)O. In the Ca-system the reaction proceeds with formation of Fe3C and Ca-rich melt with a Ca/Fe ratio of near 4. In discussion, we outline (a) relative stability of Fe-hydride and Fe-carbide and their role in core formation and metal precipitation, (b) possibility of carbonate reduction during deep subduction, (c) possible role of melting in COH-fluid equilibria with mantle assemblages, (d) comparison of mantle solidi under reduced and oxidized conditions up to lower mantle P-T conditions.