Archaean Basin Margin Geology and Crustal Evolution: an East Pilbara Traverse

Total Page:16

File Type:pdf, Size:1020Kb

Archaean Basin Margin Geology and Crustal Evolution: an East Pilbara Traverse Research article Journal of the Geological Society Published online June 6, 2017, updated August 30, 2017 https://doi.org/10.1144/jgs2016-127 | Vol. 174 | 2017 | pp. 1090–1112 Archaean basin margin geology and crustal evolution: an East Pilbara traverse Wouter Nijman1*, Armelle Kloppenburg2 & Sjoukje T. de Vries1 1 Department of Earth Sciences, Faculty of Geosciences, Utrecht University, PO Box 80115, 3508 TC Utrecht, the Netherlands 2 4DGeo Structural Geology, Daal en Bergselaan 80, 2565 AH The Hague, the Netherlands * Correspondence: [email protected] Abstract: A palinspastic reconstruction of a 100 km long traverse through Archaean rocks of the East Pilbara, Western Australia, includes new observations of the deformation preceding the now visible greenstone belt pattern. The restoration is time-calibrated with all available U–Pb datings. Between incompletely preserved basin sequences, two superposed Palaeoarchaean volcano-sedimentary basins (the Coongan and Salgash Basins) are separated by an eastwards time-transgressive interface tentatively interpreted as an onlap surface. For over 140 Ma, the basin margin architecture was structurally controlled by superposed extensional growth fault arrays (D1) with associated dyke swarms in a curved pattern spatially not related to that of the actual distribution of granite domes and greenstone belts. The basins are interpreted to have formed by collapse after arching above hotspots due to phase transitions by mini-subduction of slabs of cooled water-saturated basalt towards the base of an originally c. 45 km mafic crust. At c. 3.31 Ga, the extension was replaced by plate-driven regional NW–SE compression (D2) inferred from NW-over-SE shear and ramp-and-flat thrusts, partly reversing offsets of the D1 extension. The recognition of widespread D2 pre-doming compression is important because it triggered the c. 3.18 Ga start of formation of the dome-and-keel pattern (D3) visible today, which culminated at c. 2.9 Ga. Supplementary material: Eight figures, numbered ‘Supplementary material fig. a–h’, and a GPS list of observation sites are available at: https://doi.org/10.6084/m9.figshare.c.3808243 Received 28 September 2016; revised 19 April 2017; accepted 21 April 2017 Throughout the last three decades of research on the Archaean, the important facies changes and, if so, are these driven by the crustal old intriguing questions about the nature of the early Earth’s crust, structural development? An early example of such an approach its rigidity and thickness, the style of its structural development and related to our study area can be found in DiMarco & Lowe (1989). In the balance between vertical diapirism (Hamilton 1998) and Utrecht University’s project the emphasis was on the relationship tangential plate motion (De Wit 1998) played, and still play, an between sedimentation and structural control, both in the Pilbara important role (e.g. Blewett 2002; McCall 2003; Hickman 2004; and the South African Barberton Greenstone Belt, a relationship for Van Kranendonk et al. 2004, 2007; Van Kranendonk 2010a; De Wit the Palaeoarchaean (3.6 – 3.2 Ga) that turned out to be difficult to et al. 2011; Van Hunen & Moyen 2012; Gerya 2016). compare with Phanerozoic settings. For the Mesoarchaean Concurrent with the extensive 1:100 000 mapping project of the (3.2 – 2.8 Ga), on the contrary, the influx of the first large Geological Survey of Western Australia (GSWA) in the Archaean volumes of coarse-clastic arkosic sandstones, both in the Pilbara Pilbara Craton of NW Australia (for summaries see Hickman and in Barberton (Zegers et al. 1998), heralded the facies 2012a; Hickman & Van Kranendonk 2012), Utrecht University (the assemblage familiar to Phanerozoic orogens related to plate motion. Netherlands) was running a project with a twofold approach: one At present, opinions diverge on the timing of the successive group working from originally deeper crustal levels of metamorphic deformation phases with respect to the onset of greenstone belt and highly deformed rocks upwards, the other from uppermost formation, the latter since Collins et al. (1998) generally related to a crustal and less metamorphic rocks downwards, in order to meet in process of crustal convective overturn. Here, we distinguish three conclusions about the structural development of the craton. successive phases of deformation: D1 extension, D2 compression Mapping at a range of scales, including detailed (c. 1:10 000) and D3 related to steepening of the greenstone sequence and mapping of relatively small key areas (Figs 1 and 2), was combined geomorphological ‘belt’ development. The term ‘phase’ should be with geochronological efforts to determine the larger-scale absolute understood as an – in comparison to the Phanerozoic – long-lasting time relationships. The work related to the Pilbara was published in episode of uniform, though possibly pulsating, structural regime. PhD theses1 (Zegers 1996; Beintema 2003; Kloppenburg 2003; De The evident and high demand for geochronological data in these Vries 2004; Strik 2004; Van den Boorn 2008) and in articles studies of Archaean rock resulted in a wealth of SHRIMP and Argon (see further references in this paper). datings. Notwithstanding the density of the sampling and the With respect to the Palaeoarchaean, important questions to be relative accuracy and precision of the age determination, the tackled were: what could be learned about the crustal structural methods are still insufficient to assess, for instance, continuity or development and the driving force behind it from sedimentological discontinuity within the stratigraphic column. Therefore, it is an characteristics such as basin shape and fill? From a sedimentolo- obvious pitfall to oversimplify stratigraphic correlations and gical perspective specifically: are we, or are we not, dealing with overlook lateral variations in stratigraphy. We present a synthesis of our bottom-up and top-down approaches, aiming to identify relationships between structural development and 1Publications of the Utrecht Pilbara project are indicated with * in the list of references. sedimentary response. To that end we revisited East Pilbara and © 2017 The Author(s). Published by The Geological Society of London. All rights reserved. For permissions: http://www.geolsoc.org.uk/permissions. Publishing disclaimer: www.geolsoc.org.uk/pub_ethics Archaean basins, East Pilbara traverse 1091 compiled a c. 100 km long east–west traverse through the craton continuation of the Doolena Gap Greenstone Belt over the (Fig. 2;locationmapinFig. 1). It extends from Bamboo Creek Talga Talga River along the south side of the Muccan through the Coppin Gap and Marble Bar belts westwards over the Dome. North Pole Dome to just beyond the Mulgandinnah Fault zone. The (3) the Marble Bar Sector, the north-striking, western part of traverse integrates data from previous publications with new the Marble Bar Greenstone Belt; observations from key locations along the traverse (Fig. 2, sites 1 – (4) the Glen Herring Synclinorium (new name after Glen 22; see GPS list of the locations in the Supplementary material). Herring Creek); and The traverse combines well-preserved Palaeo- and Mesoarchaean (5) the North Pole Dome (further abbreviated as NP Dome). structural, sedimentological and volcanological features with a To avoid unnecessary complexity in the description, the relatively good time control from U–Pb datings (Figs 2 and 3b). A name ‘Panorama Greenstone Belt’ for the greenstone cover stepwise palinspastic reconstruction of the traverse (Fig. 3a→b→c; of the NP Dome will not be used. legend in Fig. 1) allows for an interpretation of the basin configuration and concurrent lateral facies changes. In combination with interpretations of structures that formed at originally deeper Remarks on the stratigraphical correlation crustal levels, we arrive at a model of structural evolution of the The legend (Fig. 1) of the corridor map presents the dated Archaean crust of the Pilbara, which in several aspects differs from stratigraphical sequence used in this paper. The following the protocontinental model proposed by Van Kranendonk et al. correlations differ from those made in the GSWA maps: (2015a). North Pole, McPhee and Razorback Cherts: the Razorback Chert of the Coppin Gap Sector ( just south of site 11 in Fig. 2)is The East Pilbara traverse observed correlated here with the McPhee Chert in the Marble Bar Sector (sites 12 – 15) and the North Pole Chert (Dresser Fm) in the NP Corridor map and construction of the traverse Dome (site 20). As a consequence, the underlying sequence of the Razorback Chert is designated to the Talga Talga Subgroup Corridor map and traverse (De Vries et al. 2006; cf. section ‘Razorback Chert and Shear Zone’ Primary sources for the corridor map (Fig. 2) and the cross-section below). (Fig. 3a)are: Mount Ada Basalt, Apex Fm and the Antarctic Creek Member: in (1) the new 1:100 000 GWSA geological map sheets: North the NP Dome the top of the Mt Ada Basalt is placed at the contact Shaw (2nd edn, Hickman 2012b; explanatory note by Van with the, in places discontinuous, felsic volcanic/chert unit known Kranendonk 2000), Marble Bar (Hickman & Van as the Antarctic Creek Member (stratigraphic level of sites 10c and Kranendonk 2008), Coongan (Van Kranendonk 2004; 22) of the Mt Ada Basalt (Australian Stratigraphic Units Data Base). 207 206 explanatory note by Van Kranendonk 2010b), Muccan The age of the Antarctic Creek Member ( Pb/ Pb age of 3470.1 (Williams 1998; explanatory note by Williams 1999) and ± 1.9 Ma, Byerly et al. 2002) corresponds with that of the lower part Mt Edgar (map and explanatory note by Williams & Bagas of the Duffer Fm further to the east in the Bamboo Creek Sector. We 2007a, b); notice that these map sheets will be further consider the felsic volcanic component of the member as a pinch- mentioned in the text without references; out of the Duffer Fm between the Mt Ada Fm and the next younger – – 207 206 (2) new field observations, air photo and satellite image basalt unit, the Apex Fm.
Recommended publications
  • Thomas Spring Thesis (PDF 7MB)
    RECONSTRUCTION OF THE PHYSICAL VOLCANOLOGICAL PROCESSES AND PETROGENESIS OF THE 3.5GA WARRAWOONA GROUP PILLOW BASALT OF THE WARRALONG GREENSTONE BELT, PILBARA CRATON WESTERN AUSTRALIA Thomas Frederick David Spring Bachelor of Applied Science (Geology) Submitted in fulfilment of the requirements for the degree of Master of Applied Science (Geoscience) School of Earth, Environment and Biological Science Faculty of Science and Engineering Queensland University of Technology 2017 Abstract The formation of Earth’s continental crust initiated in the early Archean and has continued to the present day. In the early Archean, the Earth was substantially hotter than the present day leading to dramatically different tectonic processes. Early Archean tectonic processes have to be inferred from the rare well-preserved remnants of Archean crust. Models for the formation of Archean crust include large scale mantle melting associated with mantle plumes to generate thick basaltic to ultramafic crust. This crust than undergoes partial melting and internal differentiation to more felsic compositions. The Pilbara craton provides an ideal area for research into the Archean crust, with some of Earth oldest crust being preserved in relatively low strain and low metamorphosed greenstone belts. The volcanic cycles preserved in the greenstone belts of the Paleoarchean East Pilbara Terrane of the Pilbara craton represent the type example of plume-derived volcanism in the early Earth. Here I investigate the lithostratigraphy, volcanology and depositional environment of a volcanic and sedimentary succession ascribed to the Warrawoona group of the East Pilbara Supergroup from the Eastern Warralong Greenstone belt of the East Pilbara Terrane. In addition, I investigate the petrogenesis of well-preserved basaltic samples from the pillow basalt sequence ascribed to the Mt Ada Basalts in the study area.
    [Show full text]
  • VAALBARA and TECTONIC EFFECTS of a MEGA IMPACT in the EARLY ARCHEAN 3470 Ma
    Large Meteorite Impacts (2003) 4038.pdf VAALBARA AND TECTONIC EFFECTS OF A MEGA IMPACT IN THE EARLY ARCHEAN 3470 Ma T.E. Zegers and A. Ocampo European Space Agency, ESTEC, SCI-SB, Keplerlaan 1, 2201 AZ Noordwijk, [email protected] Abstract The oldest impact related layer recognized on Earth occur in greenstone sequences of the Kaapvaal (South Africa) and Pilbara (Australia) Craton, and have been dated at ca. 3470 Ma (Byerly et al., 2002). The simultaneous occurrence of impact layers now geographically widely separated have been taken to indicate that this was a worldwide phenomena, suggesting a very large impact: 10 to 100 times more massive than the Cretaceous-Tertiary event. However, the remarkable lithostratigraphic and chronostratigraphic similarities between the Pilbara and Kaapvaal Craton have been noted previously for the period between 3.5 and 2.7 Ga (Cheney et al., 1988). Paleomagnetic data from two ultramafic complexes in the Pilbara and Kaapvaal Craton showed that at 2.87 Ga the two cratons could have been part of one larger supercontinent called Vaalbara. New Paleomagnetic results from the older greenstone sequences (3.5 to 3.2 Ga) in the Pilbara and Kaapvaal Craton will be presented. The constructed apparent polar wander path for the two cratons shows remarkable similarities and overlap to a large extent. This suggests that the two cratons were joined for a considerable time during the Archean. Therefore, the coeval impact layers in the two cratons at 3.47 Ga do not necessarily suggest a worldwide phenomena on the present scale of separation of the two cratons.
    [Show full text]
  • Carbonaceous Cherts of the Barberton Greenstone Belt, South Africa M
    Geophysical Research Abstracts, Vol. 8, 04975, 2006 SRef-ID: 1607-7962/gra/EGU06-A-04975 © European Geosciences Union 2006 Carbonaceous cherts of the Barberton Greenstone Belt, South Africa M. van Zuilen (1), M. Chaussidon (2), C. Rollion-Bard (2), B. Luais (2), B Marty (2) (1) Institut de Physique du Globe de Paris, France ([email protected] / Tel: +33 144274833) (2) Centre de Recherche Pétrographiques et Géochimiques, Vandoeuvre les Nancy, France Some of the oldest traces of life on Earth have been found in chert horizons occur- ring in the lower 3.5 Ga Warrawoona Group (eastern Pilbara Craton, Western Aus- tralia), and in the 3.4-3.2 Ga Onverwacht Group (Barberton Greenstone Belt, South Africa). The validity of these claims strongly depends on the geological context, and especially on the process of chert formation. The origin of chert units in the War- rawoona Group has been controversial, since several deposits previously recognized as sedimentary in origin were reinterpreted as hydrothermal feeder dikes. It has been suggested that serpentinization of ocean floor basaltic crust by circulating CO2-rich fluids could have prompted hydrocarbon formation by Fischer-Tropsch (FT-) type re- actions leading to the emplacement of carbonaceous feeder dike cherts. Alternatively, chemolithoautotrophic organisms may actually have been present in such seafloor hy- drothermal systems. These two possibilities highlight the need for detailed geochem- ical studies of the various carbonaceous cherts in Archean greenstone belts in which traces of life have been reported. Here a study is presented of carbonaceous chert de- posits from the Barberton Greenstone Belt (BGB), South Africa.
    [Show full text]
  • Squeezing Blood from a Stone: Inferences Into the Life and Depositional Environments of the Early Archaean
    Squeezing Blood From A Stone: Inferences Into The Life and Depositional Environments Of The Early Archaean Jelte Harnmeijer A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy University of Washington MMX Programs Authorized to Offer Degree: Center for Astrobiology & Early Earth Evolution and Department of Earth & Space Sciences Abstract A limited, fragmentary and altered sedimentary rock record has allowed few constraints to be placed on a possible Early Archaean biosphere, likewise on attendant environmental conditions. This study reports discoveries from three Early Archaean terrains that, taken together, suggest that a diverse biosphere was already well- established by at least ~3.5 Ga, with autotrophic carbon fixation posing the most likely explanation for slightly older 3.7 - 3.8 Ga graphite. Chapter 2 aims to give a brief overview of Early Archaean geology, with special reference to the Pilbara’s Pilgangoora Belt, and biogeochemical cycling, with special reference to banded-iron formation. Chapter 3 reports on the modelled behaviour of abiotic carbon in geological systems, where it is concluded that fractionations incurred through autotrophic biosynthesis are generally out of the reach of equilibrium processes in the crust. In Chapter 4, geological and geochemical arguments are used to identify a mixed provenance for a recently discovered 3.7 - 3.8 Ga graphite-bearing meta-turbidite succession from the Isua Supracrustal Belt in southwest Greenland. In Chapter 5 and 6, similar tools are used to examine a newly discovered 3.52 Ga kerogenous and variably dolomitized magnetite-calcite meta- sediment from the Coonterunah Subgroup at the base of the Pilbara Supergroup in northwest Australia.
    [Show full text]
  • Geological Archive of the Onset of Plate Tectonics
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE Geological archive of the onsetprovided by espace@Curtin of plate tectonics rsta.royalsocietypublishing.org Peter A. Cawood1,2, Chris J. Hawkesworth2,3, Sergei A. Pisarevsky4, Bruno Dhuime3,5, 1 1 Research Fabio A. Capitanio andOliverNebel 1 Cite this article: Cawood PA, Hawkesworth School of Earth, Atmosphere and Environment, Monash University, CJ, Pisarevsky SA, Dhuime B, Capitanio FA, Melbourne, VIC 3800, Australia 2 Nebel O. 2018 Geological archive of the onset Department of Earth Sciences, University of St Andrews, of plate tectonics. Phil.Trans.R.Soc.A376: St Andrews, Fife KY16 9AL, UK 20170405. 3School of Earth Sciences, University of Bristol, Wills Memorial http://dx.doi.org/10.1098/rsta.2017.0405 Building, Queens Road, Bristol BS8 1RJ, UK 4ARC Centre of Excellence for Core to Crust Fluid Systems (CCFS) and Accepted:21June2018 Earth Dynamics Research Group, The Institute for Geoscience Research (TIGeR), Department of Applied Geology, Curtin One contribution of 14 to a discussion meeting University, GPO Box U1987, Perth, WA 6845, Australia issue‘Earthdynamicsandthedevelopmentof 5CNRS-UMR 5243, Géosciences Montpellier, Université de plate tectonics’. Montpellier, Montpellier, France Subject Areas: PAC, 0000-0003-1200-3826;BD,0000-0002-4146-4739; plate tectonics, geochemistry, geology ON, 0000-0002-5068-7117 Keywords: Plate tectonics, involving a globally linked system of lateral motion of rigid surface plates, is a plate tectonics, Archaean, palaeomagnetics, characteristic feature of our planet, but estimates lithosphere, early Earth of how long it has been the modus operandi of lithospheric formation and interactions range from Author for correspondence: the Hadean to the Neoproterozoic.
    [Show full text]
  • The Mesoarchaean Mosquito Creek Basin of the East Pilbara, Western Australia
    Precambrian Research 180 (2010) 251–271 Contents lists available at ScienceDirect Precambrian Research journal homepage: www.elsevier.com/locate/precamres The waning stage of a greenstone belt: The Mesoarchaean Mosquito Creek Basin of the East Pilbara, Western Australia Wouter Nijman ∗, Quintijn Clevis 1, Sjoukje T. de Vries 2 Department of Sedimentology, Faculty of Geosciences, Utrecht University, Postbus 80021, 3508 TA Utrecht, The Netherlands article info abstract Article history: The Mosquito Creek Basin stands apart in the Archaean granite–greenstone terrane of the east Pilbara Received 16 October 2009 Craton because of the rectangular outcrop but crescent-shaped subcrop, and its composition of low- Received in revised form 25 February 2010 grade metamorphic mainly turbiditic clastic sedimentary rocks. These sediments belong to the c. 2.9 Ga Accepted 9 March 2010 Mosquito Creek Formation. Tectonic interpretations of the basin have varied from a simple synclinorium, to an accretionary prism, an extensional passive margin, and more recently into a rift basin separating the Kurrana Terrane from the East Pilbara Terrane (EPT). Keywords: Combined sedimentological and structural–geological investigations show coarse-clastic fan-delta Mesoarchaean Pilbara Craton marginal facies with stacked unconformities, rimming an E–W basin centre with predominantly finer- Mosquito Creek Basin grained mass flow-dominated sediments. A N–S traverse therefore contains a complete cross-section of Archaean sedimentary basins the Mosquito Creek Basin, shortened to about 50% of its original width by tight folding and thrusting. Greenstone belt evolution The basin fill shows one major FU sequence from fan-delta sandstone to distal turbidites, unconformably overlying an older, partially preserved clastic sequence of comparable facies.
    [Show full text]
  • Tectonic Evolution of the Early Archaean Doolena Gap Greenstone Belt, East Pilbara Terrane, Western Australia
    TECTONIC EVOLUTION OF THE EARLY ARCHAEAN DOOLENA GAP GREENSTONE BELT, EAST PILBARA TERRANE, WESTERN AUSTRALIA by Daniel Wiemer (Dipl. Geol./M.Sc.) ____________________________________________ Submitted in total fulfillment of the requirements for the degree of Doctor of Philosophy (Ph.D.) Brisbane, 2017 School of Earth, Environmental and Biological Sciences Science and Engineering Faculty Queensland University of Technology Supervisor: Dr. David T. Murphy Co-supervisor: Dr. Christoph E. Schrank ii QUT Verified Signature iii Abstract Earth’s oldest preserved crust is characterised by a distinctive crustal architecture of large ovoid granitic domes surrounded by curvilinear supracrustal greenstone belts. Such dome-and-keel morphology is not generated in the present-day Earth as part of plate tectonics. This indicates that the crustal fragments preserved from the early Earth, which had higher heat generation and therefore higher temperatures, formed in a distinct non-plate tectonic style tectono-magmatic regime. Here I investigate the lithological associations, the magmatic contributions and the structural kinematics that gave rise to the distinctive Archean dome and keel morphology. In doing so I test the model of partial convective overturn for the formation of the dome-and-keel crustal architecture in which dense mafic crust overlying lower density felsic crust leads to buoyancy instabilities and crustal-scale reorganization. The 3530- 3225 Ma East Pilbara Terrane, Western Australia, contains the best preserved lithological and structural inventory associated with dome-and-keel formation, making it the archetypical early Archean dome-and-keel terrane and the perfect natural laboratory for investigating early Archaean tectonic processes. Here I present a detailed lithostratigraphic, structural, petrological, geochemical, and geochronological study of a well exposed geological transect through the dome-and-keel terrane of the transition between the western Doolena Gap greenstone belt and the Muccan Granitic Complex.
    [Show full text]
  • Formation of Early Archean Granite-Greenstone Terranes From
    Chemical Geology 551 (2020) 119757 Contents lists available at ScienceDirect Chemical Geology journal homepage: www.elsevier.com/locate/chemgeo Formation of early Archean Granite-Greenstone Terranes from a globally chondritic mantle: Insights from igneous rocks of the Pilbara Craton, T Western Australia ⁎ Andreas Peterssona,b, , Anthony I.S. Kempa, Chris M. Graya, Martin J. Whitehouseb a School of Earth Sciences, The University of Western Australia, Crawley, Australia b Swedish Museum of Natural History, Box 50 007, SE-104 05 Stockholm, Sweden ARTICLE INFO ABSTRACT Editor: Balz Kamber The continental crust grows via juvenile additions from the mantle. However, the timing of initial continent fi Keywords: stabilisation and the rate of subsequent continental growth during the rst billion years of Earth history is widely Pilbara Craton debated, in part due to uncertainty over the composition of the mantle source of new crust. Well-preserved Chondritic mantle Archean granite-greenstone terranes, as present within the Pilbara Craton (Western Australia), provide insights Granite-greenstone belts into the sources of felsic magmas and the processes of continental growth and evolution in the distant geological Archean past at the regional scale. Here, we present zircon U-Pb, O and Hf isotope data from ancient gneissic and granitic Zircon rocks of the Pilbara Craton, to decipher magma sources and the timing and processes of craton growth. There is U-Pb, Lu-Hf, O-isotopes no evidence for depleted mantle compositions, and the simplest interpretation is that the crust of the Pilbara Crustal growth Craton was generated from mantle with a chondritic Hf isotope composition. Our results indicate crustal ad- dition at ~3.59 Ga, represented by emplacement of gabbroic to anorthositic rocks.
    [Show full text]
  • Geochemistry of the Corunna Downs Granitoid Complex, East Pilbara Granite–Greenstone Terrane, Western Australia by L
    Technical papers Geochemistry of the Corunna Downs Granitoid Complex, East Pilbara Granite–Greenstone Terrane, Western Australia by L. Bagas1, R. H. Smithies2, and D. C. Champion3 (EPGGT; Fig. 1). This complex is unusual for the Pilbara Craton Abstract because it lacks rocks of the classic Archaean TTG series (Rapp et al., About 80% of the Archaean Corunna Downs Granitoid Complex in the 1999), although it does contain East Pilbara Granite–Greenstone Terrane consists of c. 3315 Ma tonalite, trondhjemite, and monzogranites. The monzogranites are typically highly fractionated, granodiorite (Fig. 2). This study is K rich, Al poor, and have trace element compositions consistent with based largely on geochemical remelting of an older tonalitic–trondhjemitic–granodioritic (TTG) crust analyses of about 200 samples that at a mid-crustal level. The remaining 20% of the complex comprises were collected in the early 1980s tonalites, trondhjemites, and granodiorites. Some of these granitoids (Davy, 1988) and have recently been are as old as c. 3400 Ma, but the majority are similar in age to the reanalysed by Geoscience Australia monzogranites. The tonalites, trondhjemites, and granodiorites have (formerly Australian Geological high Y and Yb, and low Sr and Al2O3 concentrations compared to Survey Organisation). classic Archaean TTGs, which are thought to form through high- pressure melting of hydrated mafic crust. In contrast to TTGs, the tonalitic, trondhjemitic, and granodioritic rocks of the complex have a low-pressure, mid- to lower-crustal, amphibolite source that was Geological setting garnet free and probably also had residual plagioclase. It is proposed that at the same time as mid-crustal melting of TTG occurred to form The CDGC has an elliptical and the monzogranites, melting of an associated mafic intraplate formed domal shape with a long axis of the tonalites, trondhjemites, and granodiorites.
    [Show full text]
  • Growth-Fault Structure and Stratigraphic Architecture of The
    Precambrian Research 149 (2006) 77–98 Growth-fault structure and stratigraphic architecture of the Buck Ridge volcano-sedimentary complex, upper Hooggenoeg Formation, Barberton Greenstone Belt, South Africa Sjoukje T. de Vries a,∗, Wouter Nijman a, Richard A. Armstrong b a Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands b Research School of Earth Sciences, The Australian National University (ANU), Canberra, ACT 0200, Australia Received 28 January 2005; received in revised form 11 April 2006; accepted 22 April 2006 Abstract The ∼3.45–3.42 Ga Buck Ridge volcano-sedimentary complex (BR-vsc) forms the uppermost part of the Hooggenoeg Formation, in the early Archaean Onverwacht Group of the Barberton Greenstone Belt, South Africa. The complex consists mainly of massive and pillowed basalts and felsic, quartz-plagioclase porphyritic rocks, which are capped by pervasively silicified sedimentary rocks. Deposition of the felsic extrusive and (volcani-)clastic sedimentary rocks occurred in shallow water to emersion, during an extensional tectonic regime. The extensional regime is expressed by a number of listric normal faults that transect the entire ∼2 km thick complex. The syndepositional (i.e. growth fault) character of the faults is indicated by variations in thickness and facies of rock units across the faults, and by systematic rotation of the fault blocks. Broadly contemporaneous with the faulting, felsic rocks intruded the complex into the highest levels. The geometry of these intrusive bodies was controlled by the major growth faults. Extension also created space for the intrusion of approximately bedding-perpendicular felsic and mafic dykes, and black chert veins.
    [Show full text]
  • Evidence from the 3.5–1.8 Ga Geological History of the Pilbara Region of Western Australia
    283 by Arthur H. Hickman1 and Martin J. Van Kranendonk2 Early Earth evolution: evidence from the 3.5–1.8 Ga geological history of the Pilbara region of Western Australia 1Geological Survey of Western Australia, 100 Plain St., East Perth, WA 6004, Australia. E-mail: [email protected] 2School of Biology, Earth and Environment, University of New South Wales, Randwick, NSW 2052, Australia. E-mail: [email protected] The Pilbara region of Western Australia is one of only unconformably overlying 2.21–1.79 Ga Wyloo Group in two areas on Earth – the other being the Kaapvaal Craton the Ashburton Basin followed the Ophthalmian Orogeny, of southern Africa – that contain well preserved, near- and all of these rocks were deformed by the Panhandle continuous geological records of crustal evolution from (c. 2 Ga) and Capricorn (c. 1.78 Ga) orogenies. the Paleoarchean into the late Paleoproterozoic. The Pilbara is famous for hosting fossil evidence of early Introduction life (stromatolites and microfossils), and for containing The Pilbara region of Western Australia is one of only two areas a record of the early Archean atmosphere. The geological in the world – the other being the Kaapvaal Craton of southern Africa record extends from granite–greenstone terranes and – that provides extensive exposures of well preserved Paleoarchean– overlying clastic basins of the 3.53–2.83 Ga Pilbara late Paleoproterozoic crust from which extensive information about the evolution of crustal processes, the biosphere and atmosphere has Craton, across a major unconformity, to a series of 2.78– been obtained. The Pilbara contains three major Archean– 1.79 Ga volcanic and sedimentary successions.
    [Show full text]
  • 3.5 Billion Year Old Greenstone Successions in the Pilgangoora Belt, Pilbara Craton, Australia
    Early Archaean crustal evolution: evidence from ~3.5 billion year old greenstone successions in the Pilgangoora Belt, Pilbara Craton, Australia MICHAEL GODFREY GREEN Submitted in fulfilment of the requirements for the degree of Doctor of Philosophy School of Geosciences Division of Geology & Geophysics The University of Sydney March 2001 Acknowledgements This project was conceived by Roger Buick who recognised the significance of the Pilgangoora successions in addressing crustal growth processes. I hope that this thesis goes some way towards answering the questions that occupied so many of our discussions. Thanks for your encouragement, advice and belief. Support for this project was generally funded through ARC Grants, although Sipa Resources assisted with the 1997 field season and also provided aerial photographs, maps and other assistance; thanks Mike, Pete, Walter and John. Whole- rock geochemistry was undertaken in collaboration with Paul Sylvester and isotopic studies with Sam Bowring, Mark Schmitz and Jeff Vervoort. Support to attend conferences was provided by Edgeworth David Travelling Scholarships and the Geochemical Society. I have been greatly assisted during my studies by many of the technical staff at The University of Sydney, especially Tom, Rob, Phil, Dave, George, Nancy, Maria and Erica. Thanks also to the students and academic staff who enriched my life at Sydney. A special thanks to all who shared the wonderful days in the Pilbara, particularly Mike, Owen, Ian, Kevin and even Jochen. Thanks also to Dave, Richard and Peter from AGSO. To Natalie for putting up with all my absences, especially during the last 6 months when my mind was elsewhere, no amount of thanks can repay.
    [Show full text]