The ultramafic nodules in kimberlite are little altered samples of the upper mantle. Source mantle (garnet-lherzolite), residual mantle (garnet-harzburgite and harzburgite), primary magma (ultrabasic) and high-pressure cumulates (eclogite) are all represented. Twenty-seven new analyses of ultramafic rocks and 24 new analyses of their constituent minerals are presented and used in conjunction with published data to demonstrate that the upper mantle sampled by kimberlite displays a mineralogical and chemical variation reflecting very deep seated partial melting events which produced from the rocks affected about 15% of ultrabasic primary magma at a temperature not much more than 50°C above the solidus. The majority of the subcontinental mantle section sampled by kimberlite is not, however, a totally depleted residuum, but is potentially fertile source mantle. An upper mantle model based upon the inclusions in kimberlite has conspicuously higher Mg Mg + Fe , and differs in other important respects from hypothetical “pyrolite” models and from models based on ultramafic nodules in basalts, althought it has some similarities with a model based on alpine-type garnet-peridotites. Primary magmas in equilibrium with the magnesian source rocks indicated by the kimberlite model are themselves so magnesian and poor in incompatible elements that extensive fractionation of eclogite and/or olivine is required in order to account for the chemistry of apparently parental tholeiite magmas erupted at the earth's surface. The nickel contents of these erupted magmas do not constitute a bar to previous extensive olivine fractionation.
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