2016
DOI: 10.1016/j.gca.2016.05.013
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Rapid Cenozoic ingrowth of isotopic signatures simulating “HIMU” in ancient lithospheric mantle: Distinguishing source from process

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Cited by 50 publications
(23 citation statements)
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“…206 Pb and 208 Pb can change due to rapid ingrowth caused by relatively recent addition of U and Th to the melt source whereas 207 Pb will not change significantly. Recent studies have demonstrated that the metasomatic signature and trace element (including Th and U) enrichment in the lithospheric xenoliths is consistent with addition of a metasomatic component related to carbonatite/CO 2 -rich melts (Scott et al, 2014a(Scott et al, , 2014bMcCoy-West et al, 2016) which would create a lithospheric reservoir where rapid ingrowth of radiogenic Pb can occur. We stress that for the purpose of this study, the type of metasomatic enrichment (carbonatite or silicate melt) is not crucial, as long as enriched domains with high U+Th/Pb are created.…”
Section: Himu-like Source Enrichmentmentioning
confidence: 95%
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“…206 Pb and 208 Pb can change due to rapid ingrowth caused by relatively recent addition of U and Th to the melt source whereas 207 Pb will not change significantly. Recent studies have demonstrated that the metasomatic signature and trace element (including Th and U) enrichment in the lithospheric xenoliths is consistent with addition of a metasomatic component related to carbonatite/CO 2 -rich melts (Scott et al, 2014a(Scott et al, , 2014bMcCoy-West et al, 2016) which would create a lithospheric reservoir where rapid ingrowth of radiogenic Pb can occur. We stress that for the purpose of this study, the type of metasomatic enrichment (carbonatite or silicate melt) is not crucial, as long as enriched domains with high U+Th/Pb are created.…”
Section: Himu-like Source Enrichmentmentioning
confidence: 95%
“…This implies that the intraplate magmas are unlikely to be derived from melting of ancient pyroxenite/eclogite residing in the asthenospheric mantle. Under the proposed asthenosphericsource model (Hoernle et al, 2006;Timm et al, 2010;McGee et al, 2013), the observed enrichment of lithospheric mantle documented by Scott et al (2014aScott et al ( , 2014b, McCoy-West et al (2016), Scott et al (2016) and Dalton et al (2017) would have occurred when enriched basaltic melts derived from melting of carbonated pyroxenite in the asthenosphere ascended through the lithosphere. However, this is inconsistent with (1) the lack of radiogenic 207 Pb/ 204 Pb ratios associated with ancient enriched domains; (2) the presence of cooling diffusion profiles of pyroxenes in the Cenozoic-erupted peridotite xenoliths which require that lithospheric mantle enrichment occurred before xenolith entrainment (Scott et al, 2014a(Scott et al, , 2014bMcCoy-West et al, 2016;Dalton et al, 2017); and (3) the unradiogenic Pb isotopic compositions for the local asthenosphere in the Cretaceous, as approximately represented by Tasman MORB (Mortimer et al, 2012).…”
Section: Mantle Source Of the Westland Dike Swarmmentioning
confidence: 99%
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