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The petrogenesis of group 2 ultrapotassic kimberlites from Finsch Mine, South Africa |
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| Authors: | K J Fraser C J Hawkesworth |
| Institution: | a Department of Earth Sciences, The Open University, Milton Keynes, MK7 6AA, England b Price Waterhouse, Management Consultants, 1 Blytheswood Square, Glasgow, G2 4AD, Scotland |
| Abstract: | Major, trace element and radiogenic isotope results are presented for a suite of hypabyssal kimberlites from a single pipe, at the Finsch Mine, South Africa. These are Group 2 kimberlites characterised by abundant phlogopite ± serpentine ± diopside; they are ultrabasic (SiO2 < 42 wt.%%) and ultrapotassic (K2O/Na2O > 6.9) igneous rocks, they exhibit a wide range in major element chemistry with SiO2 = 27.6?41.9 wt. % and MgO = 10.4?33.4 wt. %. (87Sr/86Sr)i=0.7089 to 0.7106, εNd is ?6.2 to ?9.7 and they have unradiogenic (207Pb/204Pb)i contents which ensure that they plot below the Pb-ore growth curve. They have high incompatible and compatible element contents, a striking positive array between Y and Nb which indicates that garnet was not involved in the within suite differentiation processes, and a negative trend between K/Nb and Nb contents which suggests that phlogopite was involved. In addition, some elements exhibit an unexpected order of relative incompatibility for different trace elements which suggests that the intra-kimberlite variations are not primarily due to variations in the degree of partial melting. The effects of fractional crystallization are difficult to establish because for the most part they have been masked by the entrainment of 50–60% mantle peridotite. Thus, the Finsch kimberlites are interpreted as mixtures of a melt component and entrained garnet peridotite, with no evidence for significant contamination with crustal material. The melt component was characterised by high incompatible element contents, which require both very small degrees of partial melting, and source regions with higher incompatible element contents than depleted or primitive mantle. Since the melt component was the principal source of incompatible elements in the kimberlite magma, the enriched Nd, Sr and Pb isotope ratios of the kimberlite are characteristic of the melt source region. The melt fractions were therefore derived from ancient, trace elements enriched portions of the upper mantle, most probably situated within the sub-continental mantle lithosphere, and different from the low 87Sr/86Sr garnet peridotite xenoliths found at Finsch. Within the sub-continental mantle lithosphere old, incompatible element enriched source regions for the kimberlite melt fraction are inferred to have been overlain by depleted mantle material which became entrained in the kimberlite magma. |
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