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They are distinct in that their Al abundances are higher than those of the Al-depleted rocks and similar to levels in Al-undepleted komatiites. Moderately incompatible elements such as Ti, Zr, Eu, and Gd are enriched. Neither majorite fractionation nor hydrous melting in a supra-subduction zone setting could have produced these komatiites. Their high concentrations of moderately incompatible elements may have resulted from contamination of their parental melt through interaction with metasomatic assemblages in the lithospheric mantle or enrichment of their mantle source in basaltic melt components. Their Os—Nd isotopic composition is consistent with derivation from the contemporaneous convecting upper mantle. Access to content on Oxford Academic is often provided through institutional subscriptions and purchases. If you are a member of an institution with an active account, you may be able to access content in one of the following ways:. 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Oceanic Crustal Genesis and Evolution. Ore Deposits Formation. Partial Melting. Rates and Timescales of Rock-Forming Processes. Continental Collision Zones. Continental Intraplate Magmatism. Intracontinental Rifts. Large Igneous Provinces. Layered Mafic Intrusions. Metamorphic Belts. Mid-Ocean Ridges. Oceanic Intraplate Magmatism. Passive Margins. Subduction Zones. Thermodynamic Modelling. Browse all content Browse content in. Advanced Search. Search Menu. Article Navigation. Close mobile search navigation Article Navigation. Volume Journal Article. E-mail: amitava magnet. Oxford Academic. Google Scholar. Select Format Select format. Permissions Icon Permissions. Issue Section:. You do not currently have access to this article. Download all slides. Sign in Get help with access. Institutional access Sign in through your institution Sign in through your institution. 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