The relationship between δ18O values and incompatible element and radiogenic isotope enrichment in the Mashikiri nephelinites, of the Karoo LIP, southern Africa

Abstract

The Mashikiri nephelinites (MN) are the earliest and most incompatible element-enriched magmas of the Karoo LIP. Their Zr/Nb ratios of ∼1.8 are distinct from most Karoo LIP mafic rocks, which have Zr/Nb from 10 to 18 (average ∼ 16). Low εNd (−6 to −22) with initial 87Sr/86Sr ratios of 0.7046 to 0.7073 have previously been explained as due to their derivation from ancient metasomatized mantle lithosphere by low degrees of partial melting. Olivine and pyroxene phenocrysts from the MN have δ18O values ranging from 5.30 to 5.96‰, and 5.50 to 6.61‰, respectively, and crystallization was from magmas having δ18O values that vary from 6.0 to 6.6‰, up to 0.9‰ higher than magmas derived from a depleted mantle source. There is no correlation between δ18O value and indications of either crustal contamination, such as SiO2 and Pb content, or fractional crystallization, such as Mg-number and Ni and Zr content. High δ18O values are, therefore, a feature of the mantle source. There is no relationship between δ18O value and indicators of mantle metasomatism such as εNd, alkalinity, or incompatible trace element concentrations and processes that enriched the magma in 18O are, therefore, unrelated to mantle metasomatism.High δ18O values in the mantle are most likely to be due to the presence of recycled crust e.g. eclogite or pyroxenite. A mixed peridotite-eclogite mantle source could have been formed by emplacement of oceanic crust into the base of the craton during Archaean subduction. Subsequent metasomatic veining that variably infiltrated the mantle, including the high-δ18O component, before eruption of the lavas would allow extremely negative εNd values to develop.