TY - JOUR
T1 - Felsic crust development in the Kaapvaal Craton, South Africa
T2 - A reference sample collection to investigate a billion years of geological history
AU - Moyen, J. F.
AU - McCoy-West, A. J.
AU - Bruand, E.
AU - Millet, M. A.
AU - Nebel, O.
AU - Cawood, P. A.
AU - Saji, N.
AU - Ladwig, A.
AU - Klaver, Martijn
AU - Elburg, M.
N1 - Funding Information:
JF Moyen reports financial support was provided by IRP BuCoMO. Emilie Bruand reports financial support was provided by ANR. Emilie Bruand reports financial support was provided by ClerVolc. Marc Alban Millet reports financial support was provided by NERC. Peter Cawood and Oliver Nebel report financial support was provided by ARC and by Monash University.This paper draws on 20 years of experience of the first author with Kaapvaal geology. Amongst the numerous colleagues who introduced us to the region, showed us rocks, facilitated access and in general, shaped our thinking on the Craton's long and complex history, we are particularly indebted to G. Stevens and A. Kisters for 20 years of geological (and friendly!) discussions; to O. Laurent, G. Nicoli and A. Vézinet for petrological and geochronological understanding of the Northern Kaapvaal; to A. Chauvet for unraveling the complex tectonic history of the same area. In Barberton, the encyclopedic knowledge of C. Heubeck on BGB's rocks, and his willingness to share it with colleagues, is gratefully acknowledged. No paper on Kaapvaal geology would be complete without mentioning C. Anhaeusser, whose work is still a source of inspiration after 50 years, whose remarkable maps are still key references. Field work was partly funded by BuCoMO, a French-South African IRP collaboration project jointly funded by the French CNRS and the South African NRF. Massimo Raveggi is thanked for analytical assistance at Monash University. Analyses at Monash were funded by ARC grant FL160100168 to PAC. This work was supported by a NERC project NIIICE (NE/R001332/1) to MAM. We would like to thank Claire Fonquernie and Krzysztof Suchorski for support in major and trace elements analyses of part of the collection and ICP-MS lab facilities at the LMV. This work was partly supported by the French Government Laboratory of Excellence initiative n° ANR-10-LABX-0006 and by the French National Research Agency (grant ANR-21-CE49-0001-01, AMNESIA, PI EB). This is Laboratory of Excellence ClerVolc contribution number 631.
Funding Information:
This paper draws on 20 years of experience of the first author with Kaapvaal geology. Amongst the numerous colleagues who introduced us to the region, showed us rocks, facilitated access and in general, shaped our thinking on the Craton's long and complex history, we are particularly indebted to G. Stevens and A. Kisters for 20 years of geological (and friendly!) discussions; to O. Laurent, G. Nicoli and A. Vézinet for petrological and geochronological understanding of the Northern Kaapvaal; to A. Chauvet for unraveling the complex tectonic history of the same area. In Barberton, the encyclopedic knowledge of C. Heubeck on BGB's rocks, and his willingness to share it with colleagues, is gratefully acknowledged. No paper on Kaapvaal geology would be complete without mentioning C. Anhaeusser, whose work is still a source of inspiration after 50 years, whose remarkable maps are still key references. Field work was partly funded by BuCoMO, a French-South African IRP collaboration project jointly funded by the French CNRS and the South African NRF. Massimo Raveggi is thanked for analytical assistance at Monash University. Analyses at Monash were funded by ARC grant FL160100168 to PAC. This work was supported by a NERC project NIIICE (NE/R001332/1) to MAM. We would like to thank Claire Fonquernie and Krzysztof Suchorski for support in major and trace elements analyses of part of the collection and ICP-MS lab facilities at the LMV. This work was partly supported by the French Government Laboratory of Excellence initiative n° ANR-10-LABX-0006 and by the French National Research Agency (grant ANR-21-CE49-0001-01 , AMNESIA, PI EB). This is Laboratory of Excellence ClerVolc contribution number 631.
Publisher Copyright:
© 2024
PY - 2024/3
Y1 - 2024/3
N2 - The crust of the Kaapvaal craton accreted throughout the Archaean over nearly 1 billion years. It provides a unique example of the various geological processes that shape Earth's continental crust, and is illustrated by a reference collection of granitoids and mafic rocks (SWASA collection). This sample collection is fully characterised in term of age, major and trace elements, and documents the following multistage history of the craton. In the Barberton area, the initial stages of accretion (stage B.I, > 3.33 Ga and B.II, 3.28—3.21 Ga) correspond to the formation of a sodic (TTG) crust extracted from a near-chondritic reservoir. Stage B.III (ca. 3.1 Ga) corresponds to reworking of this crust, either through intracrustal melting, or via recycling of some material into the mantle and melting of this enriched mantle. Stage B.IV (2.85—2.7 Ga) corresponds to the emplacement of small, discrete plutons involving limited intracrustal reworking. The Northern Kaapvaal craton corresponds to a mobile belt flanking the Barberton cratonic core to the North. Stage NK.I (> 3.1 Ga) resembles stages B.I and B.II: formation of a TTG crust from a chondritic reservoir. In contrast, stage NK.II. (2.97–2.88 Ga) witnesses probable rifting of a cratonic fragment and formation of greenstone basins as well as a new generation of TTGs with both the mafic and felsic magmatism extracted from an isotopically depleted mantle (super-chondritic) reservoir. Intra-crustal reworking dominates stage NK.III (2.88–2.71 Ga), whereas sanukitoids and related granites, involving a mantle contaminated by recycled crustal material, are common during stage NK.IV (ca. 2.67 Ga). The SWASA collection are available as a reference collection to investigate the behavior of other systems of interest during a variety of crust evolution modes.
AB - The crust of the Kaapvaal craton accreted throughout the Archaean over nearly 1 billion years. It provides a unique example of the various geological processes that shape Earth's continental crust, and is illustrated by a reference collection of granitoids and mafic rocks (SWASA collection). This sample collection is fully characterised in term of age, major and trace elements, and documents the following multistage history of the craton. In the Barberton area, the initial stages of accretion (stage B.I, > 3.33 Ga and B.II, 3.28—3.21 Ga) correspond to the formation of a sodic (TTG) crust extracted from a near-chondritic reservoir. Stage B.III (ca. 3.1 Ga) corresponds to reworking of this crust, either through intracrustal melting, or via recycling of some material into the mantle and melting of this enriched mantle. Stage B.IV (2.85—2.7 Ga) corresponds to the emplacement of small, discrete plutons involving limited intracrustal reworking. The Northern Kaapvaal craton corresponds to a mobile belt flanking the Barberton cratonic core to the North. Stage NK.I (> 3.1 Ga) resembles stages B.I and B.II: formation of a TTG crust from a chondritic reservoir. In contrast, stage NK.II. (2.97–2.88 Ga) witnesses probable rifting of a cratonic fragment and formation of greenstone basins as well as a new generation of TTGs with both the mafic and felsic magmatism extracted from an isotopically depleted mantle (super-chondritic) reservoir. Intra-crustal reworking dominates stage NK.III (2.88–2.71 Ga), whereas sanukitoids and related granites, involving a mantle contaminated by recycled crustal material, are common during stage NK.IV (ca. 2.67 Ga). The SWASA collection are available as a reference collection to investigate the behavior of other systems of interest during a variety of crust evolution modes.
KW - Archaean
KW - Continental crust
KW - Kaapvaal craton
KW - SWASA
KW - Tonalite-trondhjemite-granodiorite
KW - TTG
UR - http://www.scopus.com/inward/record.url?scp=85184563202&partnerID=8YFLogxK
U2 - 10.1016/j.earscirev.2024.104680
DO - 10.1016/j.earscirev.2024.104680
M3 - Review Article
AN - SCOPUS:85184563202
SN - 0012-8252
VL - 250
JO - Earth-Science Reviews
JF - Earth-Science Reviews
M1 - 104680
ER -