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Titel The structure and CO2 solubility of Kimberlite melts
VerfasserIn Yves Moussallam, Yann Morizet, Pierre Florian, Mickael Laumonier, Malcom Massuyeau, Fabrice Gaillard
Konferenz EGU General Assembly 2014
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 16 (2014)
Datensatznummer 250087706
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2014-1766.pdf
 
Zusammenfassung
Kimberlitic magmas have the deepest origin of all terrestrial magmas. They are generated by low degree partial melting of carbonated mantle peridotite and may originally contain up to 30 wt% CO2. The solubility of CO2 in these melts is therefore expected to exert a prime influence on the melt buoyancy, structure and henceforth eruption dynamics. The study of Kimberlitic melt has previously been hampered by the apparent impossibility to quench them into stable glass. We have studied the CO2 solubility and molecular structure of successfully quenched CO2-bearing kimberlitic glass by FTIR, Raman and NMR spectroscopy. Our results suggest that the solubility of CO2 decreases steadily with increasing amount of network forming cations and that pressure has little effect on the solubility of CO2 for these compositions up until very shallow depth. Raman and 29Si NMR investigation suggest that the Kimberlite melt structure is more polymerised (dominated by Q1 configuration) than theoretically predicted while 13C NMR spectrum show a single resonance peak at -168 ppm similar to that of non-bridging carbonate species. Understanding the solubility and speciation of CO2 in Kimberlitic melt has strong implications regarding the carbon content of the cratonic mantle and carbon’s pathway to the surface in these tectonically lethargic settings.