2004
DOI: 10.1016/j.chemgeo.2004.04.005
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Re–Os isotope systematics and platinum group element fractionation during mantle melt extraction: a study of massif and xenolith peridotite suites

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Cited by 296 publications
(248 citation statements)
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“…Effectively, much 278 of the HSE budget of the mantle, with the exception of Re, remains in the mantle until sulfide has 279 been completely removed, after which time Os-Ir-Ru and Pt are hosted by PGM phases rather than 280 being liberated in a silicate melt. This model is consistent with an increasing number of petrographic 281 observations indicating the presence of PGM phases in melt-depleted mantle peridotite (Luguet et al, 282 2003(Luguet et al, 282 , 2007Pearson et al, 2004;Brandon et al, 2006;Kogiso et al, 2008, Lorand et al, 2010 283 Fisher-Gödde et al, 2012). 284…”
supporting
confidence: 71%
“…Effectively, much 278 of the HSE budget of the mantle, with the exception of Re, remains in the mantle until sulfide has 279 been completely removed, after which time Os-Ir-Ru and Pt are hosted by PGM phases rather than 280 being liberated in a silicate melt. This model is consistent with an increasing number of petrographic 281 observations indicating the presence of PGM phases in melt-depleted mantle peridotite (Luguet et al, 282 2003(Luguet et al, 282 , 2007Pearson et al, 2004;Brandon et al, 2006;Kogiso et al, 2008, Lorand et al, 2010 283 Fisher-Gödde et al, 2012). 284…”
supporting
confidence: 71%
“…These Os concentrations are similar to off-cratonic spinel peridotites from around the world (e.g., Meisel et al, 2001;Pearson et al, 2004;Peslier et al, 2000;Wu et al, 2006) 188 Os ratios greater than 0.5, either due to their high Re contents (> 0.2 ppb for sample ML-2 and ML-11), or owing to their low Os contents (b 0.2 ppb for sample . 187 Os/ 188 Os ratios range from 0.1171 to 0.1263, similar to those reported for other peridotite xenoliths from Shandong Peninsula (Chu et al, 2009;Gao et al, 2002).…”
Section: Re-os Isotopesmentioning
confidence: 64%
“…The strongly 383 compatible behavior of Os during mantle melting argues against this hypothesis; melt 384 depletion normally leads to higher Os contents in refractory harzburgites than precursor 385 peridotites in cratonic and massif peridotites (e.g. Pearson et al, 2004). An alternative 386 model is that the formation of the Malaita low-T harzburgites results from 387 melt-peridotite reaction involving dissolution of garnet and pyroxenes and precipitation 388 of new forsteritic olivine (e.g., Kelemen et al, 1992).…”
Section: Mechanism and Timing Of Low-t Harzburgite Formation 371mentioning
confidence: 89%