Zircon ages defining deposition of the Palaeoproterozoic Soutpansberg Group and further evidence for Eoarchaean crust in South Africa
Introduction
The northern part of the Kaapvaal Craton, Southern Africa, is largely made up of Archaean granitoid-greenstone rocks, whereas the adjacent Central Zone of the Limpopo Belt is dominated by Archaean to Palaeoproterozoic granulite-facies ortho- and paragneisses (Robb et al., 2006, Kramers et al., 2006; Fig. 1). The granitoid-greenstone suites are predominantly Meso- to Neoarchaean in age, and the granulite-facies assemblages in the Central Zone of the Limpopo Belt are interpreted to have resulted from collision between the Kaapvaal and Zimbabwe Cratons at about 2.65 Ga and from dextral transpression in the Central Zone at about 2.0 Ga, aided probably by magmatic underplating (Holzer et al., 1998, Schaller et al., 1999, Kramers et al., 2011, Kramers and Mouri, 2011, Zeh et al., 2011, Zeh and Gerdes, 2012, Laurent et al., 2013). The Central Zone of the Limpopo Belt contains metasedimentary rocks that are at least partly derived from Eo- to Palaeoarchaean crust (Jaeckel et al., 1997, Kröner et al., 1999, Buick et al., 2003, Zeh et al., 2007, Zeh et al., 2008). The above rock types are locally overlain by erosional remnants of red bed successions that include the Blouberg Formation and the Waterberg, Palapye and Soutpansberg Groups (Fig. 2). These mainly clastic sedimentary sequences are interpreted as molasse-type deposits, sourced by erosion of an extensive mountain chain as a result of the Limpopo orogeny (Callaghan et al., 1991, Barker et al., 2006, Dorland et al., 2006, Corcoran et al., 2013), but their depositional ages are not well known. This study is aimed at better defining the depositional age of the Soutpansberg Group, one of the most widespread post-orogenic successions, and to identify the source region of the sediments.
Section snippets
Geological framework
The geological relationships of the post-Limpopo orogeny clastic deposits are briefly described below. Rocks of the steeply dipping Blouberg Formation, which are entirely clastic, occur as a string of minor scattered occurrences with a maximum preserved thickness of 1200 m (Bumby et al., 2001, Barker et al., 2006; Fig. 2). The sediments overlie the ca.10 km wide Palala Shear Belt, a crustal-scale strike-slip fault zone, separating the Kaapvaal Craton from the Limpopo Belt farther north. The
. Regional setting
The Soutpansberg Group, a volcano-sedimentary suite, is developed and preserved above the Palala Shear Belt, which separates the Kaapvaal Craton in the south (Southern Marginal Zone) from the Central Zone of the Limpopo Belt in the north (Fig. 1b). This prominent structure is a crustal-scale, deep-seated terrane boundary with the mylonitic rocks attaining a width of over 10 km (Schaller et al., 1999). The Southern Marginal Zone is mainly composed of ortho- and paragneisses with zircon U–Pb ages
Previous geochronology
In general, the upper age limit for initiation of Soutpansberg deposition is constrained by the waning phases of strike-slip movement along the Palala Shear Belt and the intrusion of the Entabeni Granite (Fig. 2). Ductile movement along the Palala Shear Belt ceased at about 1.97 Ga (Schaller et al., 1999), and the Entabeni Granite with SHRIMP zircon ages of 2021 ± 5 Ma (Dorland et al., 2006) and 2023 ± 6 Ma (Zeh et al., 2009) is overlain by the Soutpansberg strata.
There are as yet no precise
Analytical methods
X-ray fluorescence (XRF) analyses were carried out at the Council for Geoscience Geochemistry Laboratory in Pretoria. A PANalytical Axios X-ray fluorescence spectrometer, equipped with a 4 kW Rh tube, was used to determine major element concentrations on fused glass disks and trace element concentrations on pressed powder pellets. Quality control was ascertained by repeat analyses of an internal standard.
The samples selected for zircon dating weighed about 5–7 kg, and were reduced by rock
Petrography and geochemistry
A simplified stratigraphic column of the Soutpansberg Group, also showing the stratigraphic position of the samples, is given in Fig. 4. GPS co-ordinates of the sample localities are presented in Table 1. The samples studied are all pyroclastic rocks. Their geochemical compositions are shown in Table 2.
Sample GB 07-20 is from the lower succession (Sibasa Formation; Fig. 4) and is an ash flow tuff, informally known as Natal House tuff, which is underlain by shale and quartzite. The rock is
Zircon U–Pb dating
Zircon grains from Sample GB 07-20 are transparent to semi-transparent and light yellow in colour. They occur essentially as rounded crystals with some preserving stubby, prismatic morphologies (100–150 μm long, length to width ratio of 1.1–2.0, Fig. 5). Many are zoned zircon grains with core-rim relationships, whereas some grains show oscillatory zoning (Fig. 5). Thirty eight zircon grains were analysed, and the results are presented in Table 3 and Fig. 6. Twenty one spots yielded concordant
Depositional age of the Soutpansberg Group
Commonly zircons with a rounded shape are interpreted as inherited (xenocrystic) or detrital grains, with the latter thought to have been mechanically rounded during transportation in a sedimentary environment (e.g. Heubeck et al., 2013).
A detrital origin for all the zircon grains in this study, however, seems at odds with our thin section studies and field observations, which do not indicate any reworking of the ash flows or an admixture of sedimentary material. We therefore suggest that at
Conclusions
The surprising, yet disappointing aspect of our study is that we were not able to unambiguously identify igneous zircon grains that were undoubtedly associated with magmatic activity and would therefore reflect emplacement of the Soutpansberg pyroclastic rocks. However, our data set and fieldwork strongly suggest that at least the youngest zircon grains are not detrital, but rather magmatic, with their rounded shapes caused by resorption in a magma chamber prior to eruption. We therefore
Acknowledgements
This contribution is from the Chemical Geodynamics Joint Laboratory of HKU and Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, and was supported by research grants from the University of Hong Kong, the Germany/Hong Kong Joint Research Scheme sponsored by the Research Grant Council of Hong Kong and the German Academic Exchange Service (DAAD) (grant_HK033/12), and was also supported by a research grant of the State Key Laboratory of Isotope Geochemistry, Guangzhou Institute of
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