2013
DOI: 10.1016/j.gca.2012.10.018
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Melting experiments on the Udachnaya kimberlite at 6.3–7.5GPa: Implications for the role of H2O in magma generation and formation of hydrous olivine

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Cited by 53 publications
(26 citation statements)
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“…These estimates overlap the water content of kimberlitic magmas (5-10 wt%; Kavanagh and Sparks 2009;Sokol et al 2013), consistent with the interpretation that Type IB eclogites were modified by kimberlite-related melts/fluids shortly before eruption (Huang et al 2012a). Kimberlitic melts are part of a compositional spectrum extending to carbonatites (Gudfinnsson and Presnall 2005;Girnis et al 2011;Sokol et al 2013), which may contain less water than kimberlitic melts.…”
Section: Metasomatism Versus Water Contentsupporting
confidence: 78%
“…These estimates overlap the water content of kimberlitic magmas (5-10 wt%; Kavanagh and Sparks 2009;Sokol et al 2013), consistent with the interpretation that Type IB eclogites were modified by kimberlite-related melts/fluids shortly before eruption (Huang et al 2012a). Kimberlitic melts are part of a compositional spectrum extending to carbonatites (Gudfinnsson and Presnall 2005;Girnis et al 2011;Sokol et al 2013), which may contain less water than kimberlitic melts.…”
Section: Metasomatism Versus Water Contentsupporting
confidence: 78%
“…Numerous experimental studies have focused on the formation of melts under cratonic pressure-temperature-composition conditions, with the emerging consensus that both CO 2 and H 2 O are necessary for melting to occur in cratons (Foley, 1989;Foley et al, 2009;Brey et al, 2008Brey et al, , 2009Girnis et al, 2011;Novella and Frost, 2014;Sokol and Kruk, 2015;Sokol et al, 2013Sokol et al, , 2014Sokol et al, , 2015Sharygin et al, 2015). In most cases, experimental melts are low to very low in silica, spanning the compositional range from carbonatites to kimberlites.…”
Section: Accepted M Manuscriptmentioning
confidence: 99%
“…Menzies and Hawkesworth, 1987;Erlank et al 1987) and several exotic magma types such as kimberlites and lamproites are likely formed, at least in part, as a result of H 2 O lowering the mantle solidus (e.g. Kushiro et al, 1968;Kawamoto and Holloway, 1997;Sokol et al, 2013). H 2 O induced melting of the deep mantle has also been proposed to explain a number of geophysical observations such as the Earth's seismic low velocity zone (Lambert and Wyllie, 1970;Mierdel et al, 2007) and possible low velocity layers present on top of the transition zone (Tauzin et al, 2010) and immediately below it (Schmandt et al, 2014).…”
Section: Introductionmentioning
confidence: 99%