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Post-emplacement serpentinization and related hydrothermal metamorphism in a kimberlite from Venetia, South Africa |
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| Authors: | G R STRIPP M FIELD J C SCHUMACHER R S J SPARKS G CRESSEY |
| Institution: | Department of Earth Sciences, University of Cambridge, Downing Street, Cambridge, CB2 3EQ, UK (); De Beers MRM R&D Group, Mendip Court, Bath Road, Wells BA5 3DG, UK; Department of Mineralogy, Natural History Museum, Cromwell Road, London SW7 5BD, UK |
| Abstract: | The common serpentine–diopside matrix assemblage in volcaniclastic kimberlite (VK) at the Venetia Mine, South Africa is ascribed to a secondary origin, because of post‐emplacement serpentinization and associated hydrothermal metamorphism. Volcaniclastic deposits with 20–30% porosity infill kimberlite pipes in the waning stages of kimberlite eruptions. Olivine macrocrysts are typically rimmed by talc and are pseudomorphed by lizardite, with minor magnetite. The fine matrix consists of mixtures of lizardite, chlorite, smectite, brucite, calcite, titanite and andradite, an assemblage which either pseudomorphed microcrysts or in‐filled voids. Locally we recognize microcryst pseudomorphs rich in sub‐microscopic mixtures of lizardite with smectite, and other microcryst pseudomorphs and void‐filling matrix rich in chlorite and lizardite. Interstitial lizardite and associated phyllosilicates (brucite, smectite and chlorite) crystallized progressively from meteoric or hydrothermally derived pore waters, and Si4+ and Mg2+ released into the fluid phase during serpentinization of olivine macrocrysts. Radial‐fibrous fringes of diopside microlites around crystals display void‐filling textures because of unrestricted growth into pore spaces. Secondary diopside is attributed to Si4+, Mg2+ and Ca2+ cations released into the fluid phase by interaction with olivine, calcite and plagioclase in siliceous xenoliths. The paucity of primary, fine‐grained groundmass phases resistant to alteration, for example, perovskite and spinel, precludes an origin for the intergrain matrix as altered interstitial ash, glass or a late‐stage kimberlite melt. Isovolumetric replacement of olivine results in a volume increase of 60% so that pore spaces in the original deposit can be easily filled up with serpentine. The source of Al3+ to form chlorite and smectite is attributed to alteration of plagioclase in xenoliths which comprise 20–30 vol.% of the deposit. Titanite, hydro‐andradite and second‐generation diopside precipitate as hydrothermal minerals from calcium‐bearing serpentinizing fluids in replacement reactions and as void‐filling minerals. Consideration of mineral equilibria in the CaO‐MgO‐SiO2‐H2O‐CO2 system constrains the common matrix assemblage of lizardite and diopside in XCO2)–T space. At 300 bar, the assemblage is stable only at temperatures below 370 °C and XCO2 < 0.01. This upper limit on temperature is well below the plausible solidus of ultrabasic magmas. Furthermore, the requirement of trace CO2 in the fluid phase implies a post‐emplacement external source rather than ‘autometamorphism’ from kimberlite‐derived fluids, because of high PCO2 commonly inferred for kimberlite magmas. |
| Keywords: | matrix post-emplacement serpentinization volcaniclastic kimberlite hydrothermal metamorphism |