Constraints on the genesis of orbicular granites and sulphide mineralization in the Koperberg Suite, South Africa and the Diana’s Pool area, Zimbabwe
Date
2024
Authors
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Journal ISSN
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Publisher
University of the Witwatersrand, Johannesburg
Abstract
This work tackles a long-standing problem in petrology, the formation of orbicular granitoids. These bodies occur as entire facies or as areas enriched in orbicules within distinct facies of plutons. Some European examples are highly prized for their decorative qualities. However, their origin is a matter of much debate going back to times when the origins of granitoids themselves were not obvious and are confused by topics such as ‘granitization’ and over-exaggeration of metasomatic effects. Here, poorly studied outcrops of orbicular rocks from the Matopos granite batholith in the Diana’s Pool area, Zimbabwe and the Koperberg Suite, South Africa are tackeld. Enzman (1953) and Garvie (1969; 1971) studied the Koperberg Suite and the Diana’s Pool orbicules, respectively and employed field observations and petrography to examine and characterize the genesis of these rocks. However, there is little evidence presented to confirm their theories on how these rocks formed as previous work lacks detailed geochemical, mineral chemistry and isotope data to support Enzman and Gravie’s conclusions on the genesis of these rocks. Furthermore, there is no connection between the metallogenesis of the sulphide mineralization and the origin of orbicular rocks, which is a unique characteristic of particular orbicule sites in the Koperberg Suite.
This study focuses on four different orbicular bodies (Orbicule Koppie, Henderson South, Henderson North and Hoogkraal Lease) from the Koperberg Suite, hosted in lithologies ranging from diorite to pyroxenite compositions. The orbicules from different orbicular share similar characteristics. Coarse- grained felsic cores, fine-grained and alternating ferromagnesian and feldspathic shells, and coarse- grained to pegmatitic matrices characterize them. The orbicules are generally spherical to ellipsoidal in shape, however, some appear to be abraded and deformed (e.g., Orbicule Koppie). The compositions and grain sizes of cores and the matrix are comparable in all localities. Both the matrix and the cores are medium- to coarse-grained and dominated by plagioclase (the matrix probably in slightly lesser proportions), microcline (in variable proportions, and seemingly absent in some cores), quartz, biotite, magnetite and orthopyroxene (in the case of Hoogkraal Lese, Henderson North and Henderson South). Contrary to the cores and matrix, shells are fine-grained and exhibit polygonal textures. In addition to this, the shells are dominated by biotite and orthopyroxene.
Plagioclase in the Henderson North and Henderson South orbicules is more calcic than plagioclase in Hoogkraal Lease and Orbicule Koppie orbicules. Biotite in the Henderson North and the Orbicule Koppie orbicules is more magnesian than those at Henderson South and Hoogkraal Lease orbicules. Plagioclase in the Henderson North orbicules are characterized by elevated and radiogenic initial 87Sr/86Sr ratios than the other orbicule localities. There is also a variation in 87Sr/86Sr ratios within the individual orbicular structures (cores, shells and matrices) in individual localities. The orbicules at Henderson South, Orbicule Koppie and the Jubilee Pit host a bornite-dominated sulphide assemblage where disseminated chalcopyrite and bornite grains are characterized by granular textures and chalcopyrite is replaced by magnetite and bornite. Bismuth, Ni and Se in these sulphides appear to partition into bornite while Ag, In, Cd, Sn, Mn, Ge and Co partition into chalcopyrite.
Diana’s Pool orbicular samples exhibit closely packed orbicules in a granitic matrix characterized by different types of orbicules containing coarse-grained felsic cores, fine-grained and alternating ferromagnesian and feldspathic shells, and a coarse-grained to pegmatitic matrix. The orbicules are generally spherical to ellipsoidal in shape, however, some appear to be abraded and deformed. The compositions and grain sizes of cores and the matrix are comparable. Both the matrix and the cores are medium- to coarse-grained and dominated by plagioclase (the matrix probably in slightly lesser proportions), microcline (in variable proportions, and seemingly absent in some cores), quartz, biotite and accessory hornblende and magnetite. Contrary to the cores and matrix, shells are fine-grained and exhibit polygonal textures. In addition to this, the shells are dominated by biotite and magnetite; however, they do not contain hornblende. Plagioclase in cores, shells and matrices shows an almost complete overlap of An contents. Biotite composition in the shells is significantly less magnesian than in core and matrix, whose compositions overlap. Initial 87Sr/86Sr ratios from plagioclase in shells are slightly more radiogenic than in the matrix and cores.
Formation of both the Koperberg Suite and Diana’s Pool orbicules has been attributed to metasomatic processes. However, modelling of the Koperberg Suite orbicules using the Magma Chamber Simulator and a variety of textural and geochemical constraints rules out a metasomatic origin. The quartz + biotite-dominated diorite (Orbicule Koppie) and the pyroxene-diorites (Hoogkraal Lease, Henderson South, Henderson North), together with more felsic anorthosite and the more mafic pyroxenites, are all produced by progressive AFC + recharge processes, where the magma was most likely anatectic melts of the country rocks that were at granulite grade. In both Diana’s Pool and the Koperberg Suite, cores are autoliths, which are plagioclase-rich, cumulate, or rim fragments reworked by new magma
inputs or injections. Heterogeneous nucleation leading to the formation of orbicular shells around the cores is attributed to adiabatic decompression of magma pulses ascending in dykes leading to superheating and resorption of early solids, and volatile exsolution, inducing undercooling, supersaturation, and shell crystallization. An alternative process that triggered superheating is magma mixing (e.g., Henderson South and Henderson North). The coarse-grained matrix crystallized later, after the orbicules formed, creating the groundmass, and locking the orbicules in place. The deformation of shells and cores (e.g., Orbicule Koppie and Diana’s Pool) suggests that the orbicules continued to evolve in the presence of a melt (matrix material) until they were emplaced at their present setting.
The in situ sulphide assemblages in the Koperberg Suite have been reassessed in view of recent research on sulphide behavior. The bornite-chalcopyrite assemblage is atypical of the intermediate solid solution (iss) assemblage (chalcopyrite and pyrrhotite) observed in most Cu-Ni magmatic sulphide deposits. The high concentrations of trace elements that are incompatible with monosulphide solid solution and the depletion of Ni and Co in the sulphides are consistent with the derivation of sulphides from a Cu-rich sulphide melt that separated from a Ni-rich sulphide melt prior to magma emplacement and orbicule formation. The oxidation and Cu-enrichment of a sulphide melt that formed the mineralization in the orbicules and Koperberg Suite more generally began prior to the emplacement of the silicate Koperberg Suite magmas that formed the orbicules, suggesting no link between orbicule genesis and sulphide metallogenesis.
Description
A thesis submitted in fulfillment of the requirements for the degree of Doctor of Philosophy Faculty of Science, University of the Witwatersrand, Private Bag 3, Johannesburg, 2050, South Africa 2024
Keywords
Orbicular granites, Koperberg suite, Sulphides, Metallogenesis, Matopos
Citation
Dumisa, Senamile Siyaya. (2024). Constraints on the genesis of orbicular granites and sulphide mineralization in the Koperberg Suite, South Africa and the Diana’s Pool area, Zimbabwe [PhD thesis, University of the Witwatersrand, Johannesburg]. WireDSpace.https://hdl.handle.net/10539/41826