Journal
JOURNAL OF PETROLOGY
Volume 62, Issue 8, Pages -Publisher
OXFORD UNIV PRESS
DOI: 10.1093/petrology/egab059
Keywords
post-orogenic mafic magmatism; melt-melt immiscibility; A-type granites; Koperberg Suite; Namaqua-Natal orogenic belt; Steenkampskraal REE-Th deposit
Categories
Funding
- University of Johannesburg (Faculty of Science)
- CIMERA Centre of Excellence for Mineral Deposit Research by the Department of Science and Innovation (DSI)
- National Research Foundation (NRF), South Africa
- French National Research Agency [ANR-10-LABX-21 -RESSOURCES21]
- Grand Est region via the program 'Jeunes chercheurs' 2020
- NRF through IPRR
- NRF-NEP [93208]
- DSI-NRF CIMERA
- NRF-CPRR-2018 [113403]
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The research reveals the presence of monazite-magnetite bearing veins and granitoid dykes in the Bushmanland Subprovince of the Mesoproterozoic Namaqua-Natal orogenic belt in southern Africa, formed between 1050 and 1010 Ma during late-Namaqua granulite-facies metamorphism and the Spektakel Suite magmatism. Notably, the monazite-rich veins and granitoid dykes in the southern part of the Bushmanland Subprovince show more radiogenic Nd isotopic compositions compared to those in the northern part, indicating a genetic link.
The Bushmanland Subprovince of the Mesoproterozoic Namaqua-Natal orogenic belt in southern Africa hosts numerous occurrences of monazite-magnetite-(biotite-apatite-sulfide)-bearing veins and granitoid dykes, including the Steenkampskraal vein system, which is one of the highest-grade REE-Th ore deposits in the world. Here, we provide whole-rock geochemical data along with zircon and monazite U-Pb dates and monazite Sm-Nd isotope analyses of these REE-Th-rich veins and granitoid dykes. The U-Pb geochronology indicates that the monazite-rich veins and granitoid dykes formed between 1050 and 1010 Ma, contemporaneously with late-Namaqua granulite-facies metamorphism. They are also coeval with the Koperberg Suite mafic magmas at 1060-1020 Ma and the late stage of a major event of A-type granitoid magmatism that occurred from 1100 to 1030 Ma (i.e. the Spektakel Suite). Similar to the mafic intrusive rocks from the Koperberg Suite, monazite-rich veins and granitoid dykes, located in the southern part of the Bushmanland Subprovince, have more radiogenic Nd isotopic compositions (epsilon Nd(t) similar to -1 to zero) than equivalent dykes and veins to the north (epsilon Nd(t) similar to -12 to -6). Mafic rocks of the Koperberg Suite reach Th and La concentrations of >400 ppm that significantly exceed those of other rock types from the region, except for the monazite-rich veins and granitoid dykes, which suggests a genetic link between these rocks. Within veins and granitoid dykes, monazite, biotite and magnetite are commonly anhedral and occur interstitially between the felsic minerals; they are, thus, late crystallizing phases. The whole-rock REE-Th concentrations of the granitoid dykes increase with Fe-Mg contents. Therefore, their incompatible element enrichment is not linked to assimilation-fractional crystallization processes. The Nd isotopic signature as well as Fe-Mg- and REE-Th-rich character of the Koperberg Suite and monazite-rich granitoid dykes might reflect partial melting of lithospheric mantle domains, metasomatized during previous Namaqua subduction events, and the mixing of mantle-derived melts with REE-Th-rich metamorphic fluids during their ascent through the crust. We propose that the monazite-magnetite vein mineralizations represent Fe-P-rich immiscible liquids that exsolved from mantle-derived magmas with compositions similar to the most mafic and monazite-rich granitoid dykes. Within this petrogenetic model, conjugate silicate-rich immiscible liquids formed the more felsic granitoid dykes characterized by lower modal abundances of biotite, magnetite and monazite. Although they do not reach similarly high REE-Th concentrations, other A-type granitoids from the region, represented by the Spektakel Suite, also share geochemical affinities with mafic igneous rocks from the Koperberg Suite; they may have originated by melting of underplated equivalents of these late-orogenic mafic rocks.
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