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Titel Mineral inclusions in sublithospheric diamonds from Juina, Brazil: Subducted protoliths, carbonated melts and protokimberlite magmatism
VerfasserIn Michael Walter, Galina Bulanova, Chris Smith, Lora Armstrong, Simon Kohn, Jon Blundy, Luiz Gobbo
Konferenz EGU General Assembly 2010
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 12 (2010)
Datensatznummer 250036190
 
Zusammenfassung
A suite of Type II Diamonds from the Cretaceous Collier 4 kimberlite pipe, Juina Kimberlite Field, Brazil, include syngenetic mineral inclusions comprising a remarkable range of compositions that include calcium- and titanium-rich perovskite, Ca-rich majoritic garnet, olivine, TAPP phase, CAS phase, K-hollandite phase, SiO2, FeO, native iron, low-Ni sulphides, and Ca-Mg carbonate. The diamonds also exhibit a range in carbon isotopic composition (δ13C ) that effectively spans that observed in the global diamond population. Diamonds with heavy, mantle-like δ13C (-5 to -10) contain mineral inclusions indicating a transition zone origin from mafic protoliths. Diamonds with intermediate δ13C (-12 to -15) contain inclusions with chemistry indicating crystallization from near-primary and differentiated carbonated melts derived from oceanic crust in the deep upper mantle or transition zone. Diamonds with extremely light δ13C (~ -25) host inclusions with chemistry akin to high pressure-temperature phases expected to form in the transition zone from subducted pelagic sediments. Collectively, the Collier 4 diamonds and their inclusions indicate multi-stage growth histories in dynamically changing chemical environments. A 206Pb/238U age of 101±7 Ma on a CaTiSi-perovskite inclusion is close to the kimberlite emplacement time (93.1 ±1.5 Ma). This young inclusion age, together with the chemical and isotopic characteristics indicating the role of subducted materials, suggest a model in which the generation of sublithospheric diamonds and their inclusions, and the proto-kimberlite magmas, are related genetically to the interaction of subducted lithosphere and a Cretaceous plume.