1999
DOI: 10.1093/petroj/40.1.133
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Carbonatite Metasomatism of the Oceanic Upper Mantle: Evidence from Clinopyroxenes and Glasses in Ultramafic Xenoliths of Grande Comore, Indian Ocean

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Cited by 387 publications
(130 citation statements)
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“…Analyses of mantle xenoliths brought to the surface by such magmas have yielded a range of fO 2 which have been compiled by Foley (2012): the oceanic and continental lithosphere xenoliths equilibrated at FMQ-0.7/-1, very similar to the riftinfluenced mantle (FMQ-0.4); xenoliths from within plate oceanic settings are significantly more oxidized (FMQ+0.6) which, along with the rare findings of high fO 2 conditions in OIB basalts (see above), hint at more oxidized source regions (but see Rhodes and Vollinger, 2005). This slightly more oxidized nature of the intraplate mantle can be related to metasomatic events (Woodland et al, 1996;McCammon et al, 2001;Coltorti et al, 1999;Creighton et al, 2009), which involve infiltration-reaction of carbon dioxide and water-rich low degree melts prior to basalt production. The involvement of such low degree melts in the source regions of MORBs has been also suggested (Wallace and Green, 1988;Gaillard et al, 2008;Dasgupta et al, 2013), including for the formation of the enriched MORBs (E-MORBs)…”
Section: Magmatic Production From Up-welling Mantle Regionsmentioning
confidence: 90%
“…Analyses of mantle xenoliths brought to the surface by such magmas have yielded a range of fO 2 which have been compiled by Foley (2012): the oceanic and continental lithosphere xenoliths equilibrated at FMQ-0.7/-1, very similar to the riftinfluenced mantle (FMQ-0.4); xenoliths from within plate oceanic settings are significantly more oxidized (FMQ+0.6) which, along with the rare findings of high fO 2 conditions in OIB basalts (see above), hint at more oxidized source regions (but see Rhodes and Vollinger, 2005). This slightly more oxidized nature of the intraplate mantle can be related to metasomatic events (Woodland et al, 1996;McCammon et al, 2001;Coltorti et al, 1999;Creighton et al, 2009), which involve infiltration-reaction of carbon dioxide and water-rich low degree melts prior to basalt production. The involvement of such low degree melts in the source regions of MORBs has been also suggested (Wallace and Green, 1988;Gaillard et al, 2008;Dasgupta et al, 2013), including for the formation of the enriched MORBs (E-MORBs)…”
Section: Magmatic Production From Up-welling Mantle Regionsmentioning
confidence: 90%
“…8) and are comparatively poor in HFSE. The major and trace element compositions of such clinopyroxenes closely resemble those of clinopyroxenes resulting from carbonatitic metasomatism (Hauri et al 1993;Coltorti et al 1999;Delpech et al 2004;Yaxley et al 1991Yaxley et al , 1998. Metasomatism by a carbonatitic melt or fluid should produce extensive reaction zones around the primary orthopyroxene in harzburgites, because orthopyroxene is unstable in the presence of carbonatitic melt at low pressures and will form secondary clinopyroxene, olivine and Cr-rich spinel associated with release of CO 2 (Wyllie & Huang 1976;Yaxley et al 1991Yaxley et al , 1998Dalton & Wood 1993;Coltorti et al 1999;Laurora et al 2001;Dawson 2002).…”
Section: Metasomatic Historymentioning
confidence: 94%
“…Smallfilled circles on curves are 1% increments of melting. between distinctive mineral parageneses and the occurrence of minerals in mantle xenoliths such as amphibole, phlogopite or plagioclase, in association with major and trace element enrichments, are indicative of metasomatic processes (O'Reilly & Griffin 1988;Fabriès et al 1989Fabriès et al , 1991Ionov et al 1994;Wulff-Pedersen et al 1996;Coltorti et al 1999;Grégoire et al 2000;Frezzotti et al 2002;Delpech et al 2004;Moine et al 2004).…”
Section: Metasomatic Historymentioning
confidence: 99%
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“…The latter consist of spongy clinopyroxene, and reaction rims/patches around orthopyroxenes and spinel with 'secondary' microcrysts of olivine, clinopyroxene, feldspar, and rarely phlogopite, apatite and carbonate, as well as interstitial glassy blebs. These reaction textures, recorded in different xenolith suites from various localities of Calatrava (Humphreys et al 2008a;Villaseca et al 2010), do not reflect interaction with the host basalts and were plausibly formed at mantle depths before FE-LHERZOLITE XENOLITHS FROM CALATRAVA the exhumation of the xenoliths (Siena et al 1991;Coltorti et al 1999Coltorti et al , 2000Beccaluva et al 2001bBeccaluva et al , 2008Delpech et al 2004;Bonadiman et al 2005).…”
Section: Petrography and Mineral Chemistry Of Lherzolite Xenoliths Frmentioning
confidence: 98%