geological society, london, special publications a damara

doi:10.1144/SP294.14 2008; v. 294; p. 257-278 Geological Society, London, Special Publications

W. Passchier D. R. Gray, D. A. Foster, J. G. Meert, B. D. Goscombe, R. Armstrong, R. A. J. Trouw and C.

GondwanaA Damara orogen perspective on the assembly of southwestern

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A Damara orogen perspective on the assembly of southwestern

Gondwana

D. R. GRAY1, D. A. FOSTER2, J. G. MEERT2, B. D. GOSCOMBE3, R. ARMSTRONG4,

R. A. J. TROUW5 & C. W. PASSCHIER6

1School of Earth Sciences, University of Melbourne, Melbourne, 3010, Vic. Australia

(Now at Geostructures Pty Ltd, Melbourne)

(e-mail: [email protected])2Department of Geological Sciences, University of Florida, Gainesville,

FL, 32611-2120, USA3School of Earth and Environmental Sciences, The University of Adelaide,

Adelaide 5005, SA. Australia4School of Earth Sciences, The Australian National University, Canberra, Australia

5Instituto de Geociencias, Universidade Federal do Rıo de Janeiro, 21949-900

Rıo de Janeiro, Brazil6Institut fur Geoswissenschaften, Johannes Gutenberg University, 55099 Mainz, Germany

Abstract: The Pan-African Damara orogenic system records Gondwana amalgamation involvingserial suturing of the Congo–Sao Francisco and Rıo de la Plata cratons (North Gondwana) from580 to 550 Ma, before amalgamation with the Kalahari–Antarctic cratons (South Gondwana) aspart of the 530 Ma Kuunga–Damara orogeny. Closure of the Adamastor Ocean was diachronousfrom the Aracuaı Belt southwards, with peak sinistral transpressional deformation followed bycraton overthrusting and foreland basin development at 580–550 Ma in the Kaoko Belt and at545–530 Ma in the Gariep Belt. Peak deformation/metamorphism in the Damara Belt was at530–500 Ma, with thrusting onto the Kalahari Craton from 495 Ma through to 480 Ma. Couplingof the Congo and Rıo de la Plata cratons occurred before final closure of the Mozambique andKhomas (Damara Belt) oceans with the consequence that the Kuunga suture extends intoAfrica as the Damara Belt, and the Lufilian Arc and Zambezi Belt of Zambia. Palaeomagneticdata indicate that the Gondwana cratonic components were in close proximity by c. 550 Ma, sothe last stages of the Damara–Kuunga orogeny were intracratonic, and led to eventual out-stepping of deformation/metamorphism to the Ross–Delamerian orogen (c. 520–500 Ma)along the leading edge of the Gondwana supercontinental margin.

Understanding supercontinent reconstructionrequires detailed knowledge of the orogens thatbind the former continental fragments together.Apart from knowledge of palaeomagnetic polesfor the constituent cratonic masses, this includesthe component lithofacies, the gross crustal archi-tecture, the geometry of the major fault and shearzones as well as the thermal and temporal aspectsof deformation, metamorphism and magmatism.For West Gondwana supercontinent construction(Fig. 1) this requires understanding of Brasiliano/Pan-African orogenesis, as West Gondwana ismade of a mosaic of cratons linked by a complexset of Pan-African/Brasiliano fold belts (Fig. 2).

The Pan-African Damara orogen of Namibia(Fig. 3) reflects part of the West Gondwana suture.It provides connection between the Brasiliano

orogens of South America through the Ribeira andDom Feliciano belts of southern Brazil (Fig. 2) andis related to convergence between the Rıo de laPlata and the Congo and Kalahari cratons of SouthAmerica and Southern Africa (e.g., Prave 1996).The Damara orogen consists of three componentarms that define a three-pronged orogenic system orcollisional triple junction (Coward 1981, 1983;Hoffman et al. 1994). These component fold beltsare the NNW-trending northern coastal arm orKaoko Belt, the S-trending southern coastal arm orGariep Belt and the ENE-trending Inland Branch orDamara Belt (e.g., Kroner 1977; Martin & Porada1977a, b; Miller 1983a). The Damara Belt extendsunder cover into Botswana and ultimately links withthe Lufilian Arc and the Zambezi, Mozambique andLurio belts (see Goscombe et al. 2000; Hanson 2003).

From: PANKHURST, R. J., TROUW, R. A. J., BRITO NEVES, B. B. & DE WIT, M. J. (eds) West Gondwana:Pre-Cenozoic Correlations Across the South Atlantic Region. Geological Society, London, Special Publications,294, 257–278. DOI: 10.1144/SP294.14 0305-8719/08/$15.00 # The Geological Society of London 2008.

Questions remain regarding the timing and cir-cumstances of accretion of the cratonic continentalfragments, the relative positions of the cratonic frag-ments over time, and the presence and widths ofocean basins between the fragments. Tectonic scen-arios range from ensimatic models with oceanbasins that developed with oceanic lithosphere (e.g.,Barnes & Sawyer 1980; Kasch 1983a; John et al.2003) through to ensialic models of failed Cambrianintracratonic rifting (e.g., Martin & Porada1977a, b; Trompette 1997). Despite similar questionsand discussions in the detailed works on the Damaraorogen published in the early 1980s (e.g., Martin &Eder 1980; Miller 1983b) the nature, size andsubstrate to the respective ocean basins, their tectonicsettings of ocean closure, and the presence, or lackof subduction systems, as well as the directions ofsubduction, are still uncertain.

This paper revisits these issues in the light of themost recent geological, geochronological and ther-mochronological data for the Damara orogen. Aspart of this analysis the paper investigates the geo-logical components of the Damara orogen and sum-marises the most recent data on (1) the structuralstyle and crustal architecture, (2) the metamorph-ism, (3) geochronological and thermochronologicalconstraints and (4) deformation kinematics. It is a

review paper that attempts to link these datawith the time-equivalent belts of South America.It also updates and revises the tectonic evolutionof the various belts that make up the Damaraorogen, particularly in the context ofGondwana amalgamation.

Background

Connections between the orogenic components ofAfrica and South America were first recognisedby du Toit (1937), as part of his Samfrau orogenicZone of Permo-Triassic age. Porada (1979, 1989)investigated more fully the genetic links betweenthe different parts of the Pan-African Damaraorogen and the Brasiliano Ribeira orogen with adetailed review of Damara orogen geologicalrelationships, including regional stratigraphy,structure and metamorphism.

Porada (1989) argued that the Damara orogenicsystem originated as a three-pronged continental riftsystem at c. 1000 Ma, where the Damara Belt wasconsidered as a failed rift or aulocogen. This scen-ario includes two episodes; the Katangan at 900–750 Ma and the Damaran at 750–500 Ma. Morerecently, Trompette (1997) argued for West

Fig. 1. Map of Gondwana showing the positions of the cratonic nuclei and the orogenic belts that weld thesupercontinent together. The younger orogens occur along the supercontinent margins. The map region shown inFigure 2 is outlined by the heavy-lined box. SF, Sao Francisco Craton; RP, Rıo de la Plata Craton.

D. R. GRAY ET AL.258

Fig. 2. Map of the Brasiliano and Pan-African orogens defining the amalgamation sutures of West Gondwana betweenthe South American and African cratonic nuclei. The composite orogenic system is made up different componentbelts and orogens, including from north to south the Aracauı–West Congo orogen, the Ribeira Belt, the DomFeliciano–Kaoko Belts and the Gariep Belt. Geological relationships including fault traces from the Aracauı orogen arefrom Pedrosa-Soares et al. (2001), the Ribeira Belt from Heilbron & Machado (2003), the Dom Feliciano Belt fromBasei et al. (2000) and Frantz & Botelho (2000), and the Kaoko Belt from Goscombe et al. (2003a, b; 2005a, b).

DAMARA OROGEN IN GONDWANA ASSEMBLY 259

Gondwana supercontinent aggregation from 900 to600 Ma, involving a two-stage evolution with intra-cratonic rifting (ensialic) at c. 600 Ma followed bybasin closure at 520 Ma.

The timing of ocean basin closure has beendisputed. Stannistreet et al. (1991) proposedthat the Khomas Ocean between the Congo andKalahari cratons (i.e., the Damara Belt) closedbefore the southern part of the AdamastorOcean between the Rıo de la Plata and Kalaharicratons (Gariep Belt), in contrast to Prave (1996)who used sedimentological evidence to argue theopposite. Ocean closure, particularly for the Ada-mastor Ocean is generally accepted as being dia-chronous, closing initially in the north (KaokoBelt) and migrating southwards with a ‘zipclosure’ action (e.g., Germs & Gresse 1991;Gresse & Germs 1993; Stannistreet et al. 1991;Frimmel & Frank 1998; Maloof 2000). Mostrecent geochronology/thermochronology of theDamara orogen (e.g., Goscombe et al. 2005b;Gray et al. 2006) linked with existing data(e.g., Frimmel & Frank (1998) for the Gariep;Kukla (1993) and Jung & Mezger (2003) forthe Damara Belt) supports closure of the northernAdamastor Ocean resulting in the Kaoko Belt,then the southern Adamastor Ocean producingthe Gariep Belt and finally the Khomas Ocean,suturing along the Damara Belt.

Recent provenance studies utilising U–Pbanalyses of detrital zircon populations haveestablished linkages between the various lithos-tratigraphic units on both sides of the AtlanticOcean and have helped to establish or confirmtectonic evolutionary scenarios. For example,Frimmel et al. (1996) argued for west-directedsubduction beneath the Rıo de la Plata Craton,which has been supported by the provenancedata of Basei et al. (2005). Similar detritalzircon populations in the Rocha (Dom FelicianoBelt), Oranjemund and Stinkfontein groups(Gariep Belt) establish basin/sedimentation lin-kages that require subduction in the southernAdamastor Ocean beneath the Rıo de la PlataCraton.

Recent palaeomagnetic studies and/or reviewsof Gondwana palaeomagnetism (Rapalini 2006;Tohver 2006) suggest that West Gondwana was acoherent block by 550 Ma, as there is a singleApparent Polar Wander Path for its componentsfrom this time onwards, requiring continent–continent collisions for the Damara and Gariepbelts at this time. However, the detailed geochro-nology/thermochronology presented in Goscombeet al. (2005b) and Gray et al. (2006) reviewed inthis paper greatly refines this and allows anew revised look at the tectonics of WestGondwana amalgamation.

Damara Orogen crustal architecture:

overview

Lithostratigraphy

The major geological components of the Damaraorogen (Fig. 3) are the Archaean–Proterozoic base-ment inliers, the Damara Sequence passive margincarbonates that rimmed the ocean basins betweenthe cratons (Otavi facies), the deeper water turbi-dites within the ocean basins (Swakop facies) andthe foreland basin deposits (molasse) of theMulden and upper Nama (Fish River Sub-Group)groups of northern and southern Namibia, respect-ively. The basement comprises continental-scaleovoid cratonic nuclei, partly contained withinNamibia (Fig. 3a) and now preserved either aslarge inliers, the Kunene and Kamanjab inliers ofthe Congo Craton in northern Namibia and base-ment of the Kalahari Craton in the SouthernMargin Zone of the Damara Belt and borderingthe eastern margin of the Gariep Belt in southernNamibia (Figs 3 & 4). Basement is also exposedin the cores of smaller, elongated domes withinthe Central Zone of the Damara Belt and in antifor-mal nappes and thrust slivers in the Kaoko Belt(Fig. 4c).

Deposition of the Damara Sequence spanned theNeoproterozoic between at least 770 and 600 Ma(Miller 1983a; Prave 1996; Hoffman et al. 1994).The basal Damara Sequence is represented byrift-related siliciclastic rocks of the Nosib Group,comprised of quartzites, conglomerates and are-nites. Quartz-syenite, alkaline ignimbrite andalkali-rhyolite units in the upper Nosib Grouphave U–Pb and Pb–Pb zircon ages ranging from757+1 to 746+2 (Hoffmann et al. 1994;Hoffman et al. 1998: de Kock et al. 2000), con-straining the minimum age of the Nosib Group tobe approximately 750 Ma (Prave 1996; Hoffmanet al. 1998). The overlying Otavi Group is domi-nated by turbiditic greywacke with pelitic schistsand psammites and rare mafic schists. Within thissuccession are two turbiditic carbonate formations,parts of which are correlated with regional diamic-tite horizons that are elsewhere interpreted as 750–735 Ma and 700 Ma in age (Hoffman et al. 1994;Frimmel 1995; Hoffman et al. 1998; Folling et al.1998). The uppermost Otavi Group is the wide-spread Kuiseb Formation, which is comprised ofturbiditic greywacke and pelite schists with thincalc-silicate bands (Fig. 3).

Structure

The belts that make up the Damara orogen (Fig. 3),or the arms of the collisional triple junction, havedistinct structural trends and style (Figs 4 & 5).


Fig. 3. Geological map of the Damara orogen showing the main geological units, the major faults, and the distributionof plutonic rocks and Swakop Group turbidites (map modified from geological map of Namibia). Inset (a) showsthe relative positions of the component fold belts and the Congo and Kalahari cratons. The locations of profiles A–A0,B–B0 and C–C0 from Figure 4 are shown. WKZ, Western Kaoko Zone; CKZ, Central Kaoko Zone; EKZ,Eastern Kaoko Zone; TPMZ, Three Palms Mylonite Zone; PMZ, Purros Mylonite Zone; ST, Sesfontein Thrust(Kaoko Belt). AF, Autseib Fault; OmSZ, Omaruru Shear Zone; OkSZ, Okahandja Shear Zone; NZ, Northern Zone;CZ, Central Zone; SZ, Southern Zone; SMZ, Southern Margin Zone (Damara Belt). MT, Marmora Terrane; PNZ, PortNolloth Zone; RPT, Rosh Pinah Thrust; ET, Eksteenfontein Thrust (Gariep Belt).


Structural grain is NNW-trending in the Kaokoand Gariep Belts, but is ENE-trending in theDamara Belt (Fig. 5). Both coastal arms are sinis-tral transpressional belts (Kaoko Belt: Durr &Dingeldey 1996; Maloof 2000; Passchier et al.2002; Goscombe et al. 2003a, b and GariepBelt: Davies & Coward 1982; Frimmel 1995;Halbich & Alchin 1995), whereas the DamaraBelt is a divergent orogen that formed duringhigh-angle convergence between the Congo andKalahari cratons (Coward 1981; Miller 1983a;Porada et al. 1983). The junction betweenthe southern Kaoko Belt and the Damara Belt(Fig. 3) is the distinctive Ugab Zone withcomplex fold interference (Coward 1983;Porada et al. 1983; Maloof 2000; Passchieret al. 2002; Goscombe et al. 2004).

The Kaoko Belt is dominated by twoNNW-trending crustal-scale shear zones and inter-linking shear zones that define orogen-scale shearlenses and similar-trending arcuate shear zonesdefine the major boundaries in the Gariep Belt(Fig. 5). The Damara Belt consists of fault- andshear-bounded zones of varying structural stylefrom north to south: a fold-thrust belt displayingcomplex fold interference, a granite-dominatedinner-zone with elongate, WNW-trending basementcored domes and Damara Sequence basins, and inthe south a transposed schist belt and another mar-ginal fold-thrust zone with basement-cored foldnappes (Fig. 5).

Each belt of the Damara orogen is dominated bycraton-vergent, imbricate thrust–shear zonesystems (Fig. 4). Both the Kaoko and Gariep beltshave crustal architectures with inferred west-dipping decollements (Fig. 4a, c). In the KaokoBelt the steeply west-dipping mylonite zones andinclined E-vergent basement-cored fold-nappesare considered to be rooted in this decollement(Goscombe et al. 2005a). The Gariep Belt geometry(Fig. 4c) has a composite, obducted ophiolite thrust-nappe, overlying imbricate faults in the passivemargin sequence (Frimmel 1995). In contrast, theDamara Belt is an asymmetric, doubly vergentorogen (Fig. 4b). The southern margin is definedby a wide zone of intense, north-dipping, shear-dominated transposed fabrics (Southern Zone) andbasement-cored fold-nappes bordering the KalahariCraton (Southern Margin Zone). The NorthernZone is a craton-vergent, fold-thrust belt without astrongly sheared transposed zone. The Northernand Southern Margin zones must have decollementsdipping away from the respective cratons (Fig. 4b).

Metamorphism

The Damara orogen shows contrasting styles ofmetamorphism. The Kaoko Belt consists of high-grade amphibolite to granulite facies metamorphicrocks (Orogen Core of the Western Kaoko Zone)juxtaposed against intermediate-pressure amphibo-lite facies rocks (Escape Zone of the Central

Fig. 4. Simplified structural profiles across the Kaoko, Gariep and Damara belts of the Damara orogen. (a) Crustalarchitecture of the Kaoko Belt (modified from Goscombe et al. 2003a). (b) Crustal architecture of the GariepBelt (modified from Von Veh 1983 in Frimmel & Frank 1998). (c) Crustal architecture of the Damara Belt ofthe Damara orogen (modified from Miller & Grote 1988: profiles on Damara orogen 1:500,000 Map sheets). Forlocation of the profiles see Figure 1. Note (a) and (c) are transpressional belts underlain by inferred west-dippingdecollements and (b) shows an asymmetric orogen profile with an inferred former subduction interface, now thrust/shear zone system, penetrating to Moho depth beneath the Southern Zone.


TN

TN

MN

MN

14

14Omangambo pluton

Omangambo pluton

Deformation: Transpression 575–550 Ma Buckling 535–505 Ma

40

35

GARIEP

BELT100 km

ARAMADTLEB

KA

OK

O

BELT

dnaleroF nrehtuoS

dnaleroF nrehtroNbasement

basement

Windhoek

TNMN14°

interference zone between Kaoko and Damara Belts

inferred bulk shear couple

apparent shortening direction (orthogal to regional fold hingelines)

upper plate (hanging wall)transport direction

stretching lineation

elongation direction (stretch) based on strain marker

dominant foliation

crenulation cleavage

fold vergence direction

Thrust loading: ~ 545 Ma

Post-tectonic granites

530–520 Ma


494–484 Ma

DAMARA BELT

GARIEP BELT


535–505 Ma

KAOKO BELT

MetamorphismM1: ~ 540 MaM2: 520–510 Ma

MetamorphismM1: 655–645 MaM2: 580–550 MaM3: 535–505 ma

Intra-continental 780–740 Marifting

Ocean crust ~630–600 Ma

Accretionary wedge ~575 MaCollision ~547–543 Ma

Intra-continental 780–746 Marifting

Thrusting ~550–540 Ma (Naukluft nappes)

Fig. 5. Summary map of deformation kinematic data for the Damara orogen with insets providing a summary of thetiming of key geological processes for each of the component fold belts. Kinematic data is based on the author’sunpublished Namibian dataset. Note the fold vergence direction is drawn orthogonal to regional fold hinge lines.


Kaoko Zone) in the footwall of the Purros MyloniteZone (PMZ, Fig. 3) and low-grade greenschist-facies rocks of the foreland or Eastern Kaoko Zonebelow the Sesfontein Thrust (ST, Fig. 3) (Goscombeet al. 2003a, 2005a; Will et al. 2004). The belt showsmarked thermal partitioning into a heterogeneousthough largely high-grade and high averagethermal gradient Orogen Core bounded by majorshear zones, and an inverted Barrovian-seriesmargin of intermediate pressure with basement-cored fold-nappes thrust onto the Congo Craton.Peak metamorphic conditions for the high-gradeparts of the Orogen Core were 800–840 8C and 6–8 kbar, and between 500 and 690 8C and 8–9 kbarin the Escape Zone. The Coastal Terrane of thewestern Kaoko Zone (CT, Fig. 3) experienced twometamorphic events: an early high-grade migmatiticevent of c. 725 8C and 7 kbar and, during transpres-sional reworking, conditions of 550 8C and 4.5 kbar(Goscombe et al. 2005a).

The Gariep Belt is mostly of low metamorphicgrade (Frimmel 2000), with greenschist-to-transitional amphibolite facies conditions in theimbricated passive margin sequences of the PortNolloth Zone (PNZ, Fig. 3) (Fig. 4c). Temperaturesranged from 400 8C to 500 8C and pressures from2.5 to c. 3 kbar (Frimmel 2000). The ChameisComplex melange of the Marmora Terrane (MT,Fig. 3) records sub-blueschist, subduction-relatedmetamorphism and peak temperatures of 500 8C to550 8C and pressures of c. 6 kbar (Frimmel 2000).

The Damara Belt consists of a central high-T/low-P, granite-dominated belt, flanked by the North-ern, Southern, and Southern Margin zones (NZ, SZand SMZ, Fig. 3), which have intermediate-T/intermediate-P metamorphism (Kasch 1983a). Thegranite-dominated Central Zone (CZ, Fig. 3) under-went peak temperatures of c. 750 8C and pressures ofc. 5.0–6.0 kbar (Kasch 1983a; Jung et al. 2000).Post-kinematic granites are largely confined to theCentral and Northern Zones of the Damara Belt(Fig. 3). These granitoids are typically compositebodies, some concentrically zoned, with at leastthree intrusive phases ranging from syenite tobiotite granite and late-stage aplite dykes. TheSouthern Zone underwent peak temperatures of c.600 8C and pressures of c. 10 kbar (Kasch 1983a).The Northern Zone of the Damara Belt shows along-strike variation in metamorphism during north-southconvergence, with low-P contact metamorphismwith anticlockwise P–T paths dominating in thewest (Ugab, Fig. 3) and higher-P (Barrovianseries) metamorphism with clockwise P–T pathsin the east (Goscombe et al. 2005a). The easternpart of the Northern Zone has peak metamorphicconditions of 635 8C and 8.7 kbar and experienceddeep burial, high-P/moderate-T Barrovian meta-morphism (Goscombe et al. 2005a).

Orogen kinematics

Structurally the Gariep Belt shows bulk SE-directedtransport (Fig. 5) partitioned into (a) strike-slipfaulting (Davies & Coward 1982) and longitudinalor NW–SE stretching in the northern part and inmajor shear zones of the Marmora sheet (Davies& Coward 1982; Gresse 1994) and (b) very strongaxial elongation or NE–SW stretching in thesouthern arc (Gresse 1994). In the outer GariepBelt, particularly near the contact between theHolgat and Stinkfontein groups (Port NollothZone), the development of sheath folds duringtransposition (Gresse 1994) reflects very highshear strains.

Folds in the Gariep Belt change character andvergence around the Gariep Arc (see Fig. 18 ofGresse 1994). In the NE outer arc, defined by theNE-trending Rosh Pinah thrust (RPT, Fig. 3), thefolds are more open, east-vergent and associatedwith east-directed thrusting. Southwards, aroundthe arc where the Eksteenfontein thrust (ET,Fig. 3) is north-trending, these folds becometighter and isoclinal, and have SE-vergence. Here,the early folds are overprinted by NE-vergent F2

folds (Gresse 1994), associated with a north- toNW-trending crenulation cleavage suggestive of alate component of margin-orthogonal compression(cf. fig. 4 of Frimmel 2000).

In the Kaoko Belt a zone of craton-vergent,basement-cored, isoclinal fold-nappes in theCentral Kaoko Zone (Fig. 3) or Escape Zoneappear to extrude from the dominant, medialPurros Mylonite Zone (PMZ, Fig. 3) (Goscombeet al. 2005a, b). These fold-nappes coincide witha swing in the lineation pattern to higher angles(up to 70–808) to the grain of the orogen, reflectinga component of high-angle escape towards theorogen margin (Durr & Dingeldey 1996; Goscombeet al. 2003a, 2005a). The Orogen Core, or easternpart of the Western Kaoko Zone inboard of theThree Palms Mylonite Zone (TPMZ, Fig. 3), con-tains shear-zone bounded domains of sheared mig-matites with steep foliations and sub-horizontallineations, a single domain of lower-grade chevron-folded turbidites and reworked basement gneissslivers (Goscombe et al. 2003a, b). CoastalTerrane migmatitic gneisses and orthogneisseswere down-graded and heterogeneously reworkedby steep mid-amphibolite facies foliations anddiscrete shear zones (Goscombe et al. 2005a).

The Damara Belt shows high-angle convergence(Fig. 5) and lacks evidence of oblique or transcur-rent movements, despite arguments for sinistralmovements and top-to-the-SW tectonic transportby Downing & Coward (1981) and Coward (1981,1983). Shear bands, developed in Kuiseb Formationschist and units of the Southern Margin Zone


indicate north-over-south movement in a north–south transport direction (Fig. 5). Variably noth-dipping, asymmetric crenulations and mesoscopicfolds reflect a bulk south-directed shear strain(Fig. 5). High-strain at the basement/covercontact is shown by deformed conglomerates inthe cover (Chuos Formation), down-dip stretchinglineations and mylonitic basement. The frontallobes of the Hakos fold-nappe (Fig. 3) displayprolate strains with the stretch direction at highangles to the transport direction as shown byshear bands.

The Central Zone of the Damara Belt displayscontrasting kinematic behaviour with orogen-parallel stretch and shortening at high angles tothe orogen at different levels (Oliver 1994; Kisterset al. 2004). During high-grade metamorphismand migmatization, the deeper levels of theCentral Zone underwent pure shear deformation,with lateral orogen-parallel stretch (Kisters et al.2004). This is in marked contrast to interpretationsof SW-directed orogen-parallel extrusion (e.g.,Downing & Coward 1981; Oliver 1994), wherethe domes were interpreted as large, SW-facingsheath folds rooted in the northeast Central Zoneand requiring top-to-the-SW transport in a crustalscale shear zone (Downing & Coward 1981;Coward 1981, 1983). At shallower crustal levelsthe Central Zone has undergone crustal thickening,orogen-normal shortening by folding andNE-directed thrusting (Kisters et al. 2004).

Within the Southern and Southern Margin zonesmajor south-directed bulk shear strain deformationwas responsible for crustal-scale underthrusting ofthe Kalahari Craton northwards (Fig. 4c), aswell as continued thrusting and crustal thickeningalong the margins of the orogen. Crustal thickeningand burial along this margin led to the Barrovianmetamorphism. Significant magmatic underplatingrelated to extension in the lower part of the overrid-ing plate, led to marked magmatism and younger,high-T/low-P metamorphism in the Central Zone.

Temporal aspects of deformation,

metamorphism and magmatism of the

Damara Orogen: review

Geochronological studies in the Kaoko Belt (Gos-combe et al. 2005b), in the Damara Belt (Jung &Mezger 2003) and in the Gariep Belt (Frimmel &Frank 1998), as well as a geochronological/thermo-chronological study across the Damara orogen(Gray et al. 2006) provide a more comprehensivepicture of the tectonothermal evolution of theorogen (Fig. 6).

The Kaoko Belt preserves evidence for three dis-tinct metamorphic episodes: M1 (655–645 Ma,

restricted to the westernmost Coastal Terrane), M2

(580–570 Ma) and M3 (530–505 Ma) (see Gos-combe et al. 2005a). Collision and docking of theoutboard Coastal Terrane with the rest of theKaoko Belt occurred after 645 Ma, but prior to580 Ma at the onset of transpressional orogenesisand M2 metamorphism (Goscombe et al. 2005b).During transpression the Coastal Terrane rocksequences were reworked at lower strains andlower metamorphic grade compared to the rest ofthe Kaoko Belt (Goscombe et al. 2005b). Trans-pressional orogenesis in the Kaoko Belt and UgabZone had ceased by c. 535 Ma, with cratonizationmarked by intrusion of post-kinematic granite andpegmatite between 535 Ma and 505 Ma (Goscombeet al. 2005b).

The Damara and Gariep belts both showyounger deformation and metamorphism than theKaoko Belt (Fig. 6; Gray et al. 2006). Continuedhigh-angle convergence through 530 Ma in theDamara Belt coincides with large-scale openeast–west trending folds in the Kaoko Belt(Goscombe et al. 2003a, b).

The Gariep Belt underwent thrust-nappe empla-cement onto the Kalahari Craton at c. 550–540 Ma(Frimmel & Frank 1998). Oceanic sequences in theMarmora Terrane preserve (1) an earlier seafloormetamorphism suggesting that Adamastor Oceanseafloor spreading was occurring at c. 630 Ma and(2) subduction-related metamorphism at c. 580–570 Ma, suggesting that the Adamastor Oceanwas closing at this time (Frimmel & Frank 1998).The Gariep Belt was cratonized by 520 Ma, witherosion into the Nama foreland basin commencingat c. 540 Ma (Gresse & Germs 1993; Gresse1994; Frimmel 2000). It was intruded by post-kinematic granites at c. 507 Ma (Frimmel 2000),although east-directed thrusting continued inboardwithin the Nama foreland basin through 496 Ma(Gresse et al. 1988).

The Damara Belt shows a more complex high-Tmetamorphic history from 540 to 510 Ma withmetamorphism coincident with pulses of magma-tism (Jung & Mezger 2003). Intrusion of post-kinematic A-type granites from 495 Ma to 486Ma (McDermott et al. 2000) was followed bycooling and exhumation of the Damara Beltthrough 470 Ma (Gray et al. 2006).

Damara Orogen tectonic evolution:

problems and issues

Problems pertaining to Damara orogen evolutionrelevant to Gondwana amalgamation relate to:(1) the positions of the respective cratons throughtime, (2) the sizes of the ocean basins betweenthem and (3) the positions and directions of


Fig. 6. Damara orogen and part of the Brasiliano time-space plot of recently published geochronological data includingthe 40Ar/39Ar data from Gray et al. (2006), and U–Pb data on zircon, monazite and titanite. Sources are listed inthe figure. Unsourced data is from Gray et al. (2006). The diagram highlights the major periods of magmatism,metamorphism/deformation, thrusting and cooling and exhumation. Fault and shear zone abbreviations are aslisted. WKZ, Western Kaoko Zone; CKZ, Central Kaoko Zone; EKZ, Eastern Kaoko Zone; TPMZ, Three PalmsMylonite Zone; VMZ, Village Mylonite Zone; PMZ, Purros Mylonite Zone; AMZ, Ahub Mylonite Zone; ST,Sesfontein Thrust; GMZ, Guantegab Mylonite Zone; OmL, Omaruru Lineament (Shear Zone); OkL, OkahandjaLineament (Shear Zone); JC-TCSZ, Jacutinga-Tres Coracoes Shear Zones; MGSZ-CSZ-SBSZ, Major Gercino ShearZone–Cordilhera Shear Zone–Sierra Ballena Shear Zone.


subduction zones that closed the oceanbasins. Answers to problems (1) and (2) willrequire better definition of palaeomagnetic polesin the future, and particularly for that of the

Kalahari Craton in the period 750–550 Ma.The presence and/or lack of subduction zones toclose the intervening ocean basins will nowbe addressed.

Fig. 6. (Continued.)


Intracratonic orogeny with exclusive ensialicevolution has been applied to the Damara orogen,particularly for the Damara Belt (Kroner 1977;Martin & Porada 1977a, b; Porada 1979). In thismodel the strongly deformed and metamorphosedMatchless Amphibolite is questioned as an ophio-lite remnant, despite MORB-type geochemistry(Barnes & Sawyer 1980) and a chert-Cu/Zn miner-alization association (Killick 2000) typical ofoceanic lithosphere. The lack of subduction-relatedmetamorphism is also cited as evidence againstocean closure due to subduction, although the pre-sence of eclogites in the Zambezi Belt (John et al.2003) and white schists in the Lufilian Arc(John et al. 2004), part of the continuationof the Damara Belt into Zambia, providealternative evidence.

In the Zambezi Belt, in contrast to Hanson et al.(1994) and Hanson (2003), John et al. (2003)argued for the presence of a large (.1000 kmwide) ocean basin with MORB-type eclogites andmeta-gabbros subducted to a depth of c. 90 kmduring basin closure. The timing of the eclogitefacies metamorphism is 595 + 10 Ma, suggestingthat subduction was occurring at this time, some60 Ma earlier than the c. 530 Ma peak ofmetamorphism in the central Damara Belt.

The long, apparently continuous, linear trace ofthe Matchless Amphibolite within intenselydeformed Kuiseb Formation schist of the SouthernZone in the Damara Belt is unusual but may havesimilarities to the fault-bounded Dun Mountainophiolite belt and Haast Schist of New Zealand(Gray et al. 2007). The transposed layering and pro-nounced schistosity in the Kuiseb Formation schistis almost identical to that of the central Otago partof the Haast Schist suggesting deformation undersimilar conditions in a scenario where the turbiditeis on the down-going plate of an oceanic sub-duction system (see Coombs et al. 1976). In theOtago Schist an intermediate-T/intermediate-P(Barrovian-style) metamorphism linked to wedgethickening (Mortimer 2000) has almost totally era-dicated the earlier subduction-related, intermediate-to high-P metamorphism (see Yardley 1982). Theolder metamorphism is only preserved as crossiterelics in the cores of younger amphibole andalbite porphyroblasts (see Fig. 2c of Yardley1982). Widespread metamorphic overprinting athigher temperatures appears typical of Barrovian-style thickened and metamorphosed accretionarywedges, and is therefore likely to have obliteratedany older intermediate-P to high-P metamor-phism in the Kuiseb Formation schists of theSouthern Zone.

The kinematics of the Southern Zone schists, bycomparison with the Otago Schist Belt of NewZealand, combined with geochemistry of the more

primitive diorites and syenites that are part of theCentral Zone early magmatic history supportsnorthward subduction of the Khomas Ocean litho-sphere beneath the attenuated leading edge of theCongo Craton; as originally suggested by Barnes& Sawyer (1980) and Kasch (1983b).

For the Kaoko Belt, the lack of ophiolitesequences or high-P metamorphism has led to intra-cratonic fold belt interpretations (Durr & Dingeldy1996; Konopasek et al. 2005). More recently, therecognition of arc affinity for the Coastal Terranehas led to proposal of a subduction-related tectonicevolution, with subduction inferred to be bothwest-directed (Machado et al. 1996; Masberget al. 2005) and further outboard east-directedsubduction (Basei et al. 2000; Goscombe &Gray 2007).

If an ocean basin closed between the African andSouth American components of the Brasiliano/Pan-African orogenic system within the KaokoZone, the suture would have to be at the proto-ThreePalms Mylonite Zone. Evidence for major crustaldisplacements with juxtaposition of distinctlydifferent aged basement either side of the PurrosMylonite Zone (Goscombe et al. 2003a, b), com-bined with the lack of ophiolite slivers and high-Pmetamorphism, suggests that both shear zones arepart of a broad, complex ‘suturing’ zone behindthe former arc (i.e. in a back-arc position),between the arc and the African continentalmargin. This ‘suturing’ involved high-T meta-morphism of turbidites deposited on the attenuatedleading edge of the Congo Craton and includeddeformation and reworking of the cratonic base-ment (Goscombe & Gray 2007). This magmaticarc could well represent the continuation of themagmatic arc recognised in the Oriental Terraneof the Ribeira Belt (Heilbron et al. 2004) withsimilar ages and/or it could be part of the granitebelt of the Dom Feliciano Belt.

Another issue for the Kaoko Belt is the inferred750–600 Ma timing of foreland basin evolution forthe Congo Craton (Prave 1996). This is problemati-cal, in that the age of the Mulden Group is inconsist-ent with the 580–550 Ma and 530 Ma periods ofdeformation that established the tectonothermalcharacter of the Kaoko Belt (Goscombe et al.2005a, b). The Mulden Group was folded and meta-morphosed prior to the late-stage thrusting event(Sesfontein Thrust), and a 750–600 Ma deposi-tional age clearly predates the timing of peak (M2)metamorphism. If the published Mulden Groupage range is correct then the sedimentary faciesand erosional hiatus of Prave (1996) must reflectinstability associated with the initial collision ofthe Coastal Terrane, and therefore the MuldenGroup sediments should contain a significantcomponent of the 650 Ma detrital zircons.


An ensimatic, subduction-related origin hasbeen accepted for the Gariep Belt, largely due tothe Chameis Complex melange of the MarmoraTerrane with its mafic and ultramafic blocks,some of which contain Na-rich amphibole(Frimmel & Hartnady 1992). Although not strictlyblueschist metamorphism, intermediate pressure(c. 6 kbar) and low temperature metamorphicconditions combined with the facies associationof melange (Chameis Complex), turbidites(Oranjemund Formation) and metavolcanic rocks(Grootderm Formation) support this contention(see descriptions and discussions in Frimmel 2000).

The direction of subduction has been discussed(see Frimmel et al. 1996), and recent provenancework on detrital zircon populations (Basei et al.2005, this volume) supports west-directed subduc-tion beneath the Rıo de la Plata Craton. This estab-lishes continuity of a linked west- or north-directedsubduction system that closed the former Adamas-tor Ocean and subsequently the Khomas Ocean toform the Gariep Belt and then the Damara Belt.

Damara Orogen tectonic evolution in a

global context

West Gondwana amalgamation is shown in a seriesof global reconstructions for different time periods

(modified from Collins & Pisarevsky 2005) incor-porating temporal and tectonothermal constraintsfrom the Damara orogen. In these tectonic recon-structions fragments of ophiolite and calc- alkalinevolcanic rocks have been used as indicators ofocean closure, the ages of metamorphism and defor-mation indicate periods of accretion and crustalthickening, and the age of post-kinematic magma-tism indicates the timing of cratonization.

780 Ma to 740 Ma (Fig. 7)

In our 750 Ma reconstruction the cratonic nucleithat eventually come together to form West Gond-wana are separated by some 308 latitude with anocean of unknown dimensions inferred betweenthe Congo and Kalahari cratonic fragments. Sucha reconstruction either contradicts or conflictswith previous interpretations of intracratonicrifting between these cratons, as represented bythe Nosib rhyolites of the Congo margin and theRosh Pinah volcanic rocks of the Kalahari margin(see fig. 7 of Frimmel & Frank 1998).

This is, however, a difficult time for which tofully constrain the palaeogeography. There are noreliable late Neoproterozoic poles from the KalahariCraton. Collins & Pisarevsky (2005) argued for aKalahari–West Australia connection based partlyon the presence of overlapping Grenvillian-age

(a)

(b)

Fig. 7. Global reconstruction of continents at 780–740 Ma with enlargement (b) showing the key geologicalconstraints during this time period from the Congo, Kalahari and Sao Francisco cratons prior to the development of thePan-African/Brasiliano orogenic system. Continental fragments are AZ, Azania; SF, Sao Francisco; RP, Rıo de laPlata; WA, West Africa; Kal, Kalahari. Data references: 1, Hoffman et al. (1996); 2, Frimmel et al. (1996).


events in the Northampton Block (Australia) andthe Namaqua–Natal belts (Kalahari Craton). Boththe Kalahari Craton and Australia have reliablepalaeomagnetic poles of Grenvillian age (1050–1100 Ma; see Meert & Torsvik 2003; Pesonenet al. 2003). These Grenvillian poles show a latitu-dinal offset between the Northampton Block andKalahari of more than 30 degrees. Thus, in ourreconstruction, we show the Kalahari Craton inproximity to the Congo–Sao Francisco craton, butdetached from it. The position of the Congo–SaoFrancisco cratons is based on the 755 Ma MboziComplex pole (Meert et al. 1995).

655 Ma to 600 Ma (Fig. 8)

Subduction-related closure begins in the northernAdamastor Ocean as evidenced by calc-alkalinemagmatism in the Aracuaı and Ribeira beltsbetween 625 Ma and 585 Ma, in the Dom FelicianoBelt from 620 Ma to c. 580 Ma (Basei et al. 2000),and from 655 Ma to 625 Ma in the Coastal Terraneof the Kaoko Belt (Masberg et al. 2005; Goscombeet al. 2005b). Collisional orogenesis was takingplace in the Brasilano orogen at c. 640 Ma with

nappe emplacements over the Sao FranciscoCraton between 640 Ma and 630 Ma (Valerianoet al. 2004, 2008), due to collision with the Parana-panema block, now hidden under the Parana Basin.

At c. 630 Ma seafloor spreading was underwayin the southern Adamastor Ocean as recorded byseafloor metamorphism in Marmora Terrane ofthe Gariep Belt (Frimmel & Frank 1998).

580 Ma to 550 Ma (Fig. 9)

Arc–continent collision occurred in the RibeiraBelt (Rıo Negro arc: 595–560 Ma; Heilbron et al.2004) and in the Kaoko Belt (Coastal Terrane:pre-580 Ma; Goscombe et al. 2005b). Peakmetamorphism in the Kaoko Belt occurred at c.580–570 Ma with transpressional reworking from570–550 Ma (Goscombe et al. 2005b).

At this time (580–570 Ma) subduction-relatedmetamorphism was taking place in the southernAdamastor Ocean (Marmora Terrane, GariepBelt; Frimmel & Frank 1998) with subduction-related ocean closure in the Khomas Ocean(560–550 Ma) suggested by mafic magmatism(diorites).

Fig. 8. Global reconstruction of continents at 655–600 Ma with enlargement (b) showing palaeogeographiclithofacies distributions and the key geological constraints during this time period from the Congo, Kalahari andSao Francisco cratons prior to the development of the Pan-African/Brasiliano orogenic system. Traces of subductionzones are shown by heavy lines with barbs, where the barbs are drawn on the upper plate side and designate thesubduction zone dip. CT, Coastal Terrane of the Kaoko Belt (shown as magmatic arc); Sah, Saharan Craton; MT,Marmora Terrane of the Gariep Belt (shown as oceanic lithosphere). Other abbreviations as in Figure 7. Datareferences: 3, Masberg et al. (2005); 4, Franz et al. (1999); 5, Seth et al. (1998); 6, Goscombe et al. (2005b); 7, Frimmel& Frank (1998).


550 Ma to 500 Ma (Fig. 10)

Closure of the southern Adamastor Ocean occurredfrom c. 550 to 540 Ma (Frimmel & Frank 1998)with oblique transpressional obduction of theMarmora Terrane oceanic suite over the imbricatedpassive margin sequence (Port Nolloth Zone,Gariep Belt) and initiation of Nama sequence fore-land basin sedimentation (Gresse & Germs 1994).

Peak deformation/metamorphism took place inthe Damara Belt through the Lufilian Arc into theZambezi Belt at c. 530–520 Ma (Goscombe et al.2000; Jung & Mezger 2003; Singletary et al. 2003;John et al. 2003, 2004). The Damara Belt showsmarked magmatism and high-T/low-P metamorph-ism at this time (Kasch 1983a). At the margins ofthe orogen, over-thrusting and related crustalthickening caused intermediate-T/intermediate-P(Barrovian style) metamorphism (Northern Zone:Goscombe et al. 2004; Southern Zone: Kasch1983a, b; Kukla 1993) with thrusting of the passivemargin sequences back over the cratonic nuclei(Naukluft Nappes: c. 500 Ma; Ahrendt et al. 1977).Effects of the Damara Belt collisional deformation

are seen as broad warpings and a younger thermaland magmatic event (M3: 530–505 Ma) in theKaoko Belt (Goscombe et al. 2005b).

In the Cabo Frio domain of the Ribeira Belt rela-tively high pressure and high temperature meta-morphism at 530–510 Ma is interpreted as relatedto collision (Schmitt et al. 2004).

505 Ma to 480 Ma (Fig. 11)

Inboard transmission of stress from the outboard,Gondwana margin (Ross–Delamerian) subductionsystem caused continued thrusting (NaukluftNappes: 500–495 Ma; Ahrendt et al. 1983) andsyn-tectonic sedimentation in the Nama forelandbasin (Ahrendt et al. 1983; Gresse et al. 1988;Gresse & Germs 1993) and in the Camaqua andItajaı basins of Brazil (Gresse et al. 1996). It alsoled to shear zone reactivation in the Kaoko Belt(490–467 Ma; Gray et al. 2006) and Gariep Belt(506–495 Ma; Frimmel & Frank 1998).

Emplacement of post-tectonic A-type granitesoccurred in the Central Zone (McDermott et al.

Fig. 9. Global reconstruction of continents at 580–550 Ma with enlargement (b) showing palaeogeographiclithofacies distributions and the key geological constraints during this time period from the Congo, Kalahari andSao Francisco cratons prior to the development of the Pan-African/Brasiliano orogenic system. Traces of subductionzones are shown by heavy lines with barbs, where the barbs are drawn on the upper plate side and designate thesubduction zone dip. An, Antarctica. Other abbreviations as in Figures 7 and 8. Data references: 6, Goscombe et al.(2005b); 7, Frimmel & Frank (1998); 8, Jacob et al. (2000); 9, de Kock et al. (2000).


2000) with continued cooling and exhumation in theDamara Belt through 480 Ma (Gray et al. 2006).

Significance for Gondwana assembly

From a western African perspective, the assemblyof Gondwana shows complex suturing that doesnot reflect a simple final amalgamation of Eastand West Gondwana (Fig. 12). It is perhaps betterdescribed as an amalgamation of North (SaoFrancisco–Congo–India) and South (Kalahari–Antarctica) Gondwana during the Kuunga orogeny(550–530 Ma), as proposed by Meert (2003) andBoger & Miller (2004) for the assembly of easternGondwana. Geochronological data from SouthAmerica and southwestern Africa (Fig. 6) suggestclosure of a Khomas–Mozambique ocean from530 to 500 Ma, as part of a combined Damara–Kuunga orogeny. The composite Kuunga–Damaraorogen incorporates the Damara orogen ofNamibia, the Lufilian Arc and Zambezi Belt of

Zambia, and joins the Lurio Belt of Mozambiqueand a belt made up of the Napier Complex of Ant-arctica, and the Eastern Ghats of India. It hasdimensions comparable to the younger Ross–Dela-merian orogen (Fig. 12).

Global reconstructions based on palaeomagneticdata suggest larger separations, and therefore sig-nificant ocean basins between the Rıo de la Plata,Congo and Kalahari cratonic nuclei that eventuallydefine West Gondwana. This has a requirement ofensimatic subduction-related ocean closures,rather than ensialic, intracratonic evolutions thatwere originally proposed to explain many of theBrasiliano/Pan-African orogens. The position ofthe Kalahari Craton however, remains controver-sial. In the Collins & Pisarevsky (2005) reconstruc-tions the Kalahari Craton abuts against the WestAustralian side of the Australian craton (Fig. 6),whereas according to Meert (2003, Fig. 1) it is situ-ated outboard of a conjoined East Antarctica–Laurentia surrounded by Congo–Sao Franciscoand Rıo de la Plata. From an African perspective

Fig. 10. Global reconstruction of continents at 550–505 Ma with enlargement (b) showing palaeogeographicallithofacies distributions and the key geological constraints during this time period from the Congo, Kalahari andSao Francisco cratons during the development of the Pan-African/Brasiliano orogenic system. Traces of subductionzones are shown by heavy lines with barbs, where the barbs are drawn on the upper plate side and designatethe subduction zone dip. The thinner heavy lines in (b) are fault traces. PMZ, Purros Mylonite Zone; TPMZ, ThreePalms Mylonite Zone of the Kaoko Belt; AR, Armorica; AV, Avalonia; Fl, Florida. Other abbreviations as inFigures 7–9. Data references: 6, Goscombe et al. (2005); 7, Frimmel & Frank (1998); 8, Jacob et al. (2000); 9, de Kocket al. (2000); 10, Jung & Mezger (2003); 11, Gresse & Germs (1993).


this provides a better fit for Gondwana assembly, asshown in Figures 7–11.

The West Gondwana suture between Africa andSouth America reflects the closure of the AdamastorOcean, and provides the most detailed evolutionsequences for SW Gondwana assembly (Fig. 12b).The Brasiliano orogens of South America showmore complicated tectonic evolution with multipletectonothermal events (see also Fig. 6), althoughthe Dom Feliciano and Ribeira belts flanking theRıo de la Plata Craton experienced collisional oro-genesis with a transpressional component at thesame time as the main phase deformation in theKaoko Belt (Frantz & Botelho 2000; Heilbron &Machado 2003; Heilbron et al. 2004; Goscombeet al. 2005b). The collisional stage in the Ribeiraorogen was at 590–560 Ma and is characterisedby terranes juxtaposed by relatively steeplydipping, dextral transcurrent shear zones (Heilbronet al. 2004). In the Kaoko Belt collision immedi-ately pre-dates main phase orogenesis in theperiod from 580–550 Ma (Goscombe et al. 2005b).

The linkage between the Brasiliano and Damaraorogens is a c. 680–580 Ma magmatic arc com-ponent along the 2800 km long composite orogenicsystem (Fig. 2). In the former Adamastor Ocean,

records of arc magmatism suggest a morecomplex tectonic evolution than perhaps a simplesouthwards migration of ocean closure, althoughthis appears to be the case in the Ribeira–Dom Feli-ciano/Kaoko–Gariep part of the orogenic system.

Arc magmatism varies from 680–670 Ma in theBrasiliano belts along the west side of the Sao Fran-cisco Craton (Heilbron et al. 2004), to 650–640 Main the Coastal Terrane of the Namibian KaokoBelt (Seth et al. 1998; Franz et al. 1999), andfrom 620–580 Ma in the granite belt of the DomFeliciano Belt (Basei et al. 2000). Southwardmigration of arc magmatism is further suggestedby southward younging of the granite batholithswithin the ‘granite belt’ of the Dom FelicianoBelt; the northernmost Florianopolis Batholithhas an age of c. 620 Ma, the centrally locatedPelotas Batholith an age of c. 610 Ma, and thesouthernmost Aguia Batholith an age ofc. 580 Ma(Basei et al. 2000).

A 630–585 calc-alkaline magmatic arc in theAracuaı Belt suggests that the main arc systemmay have followed the Brasiliano trend aroundthe Sao Francisco Craton, rather than throughthe Aracuaı orogen, which shows a youngersubduction-related closure of a Red Sea-type rift

Fig. 11. Global reconstruction of continents at 505–480 Ma with enlargement (b) showing palaeogeographicallithofacies distributions and the key geological constraints during this time period from the Congo, Kalahari and SaoFrancisco cratons during the development of the Pan-African/Brasiliano orogenic system. Reconstruction (a) isbased on Figure 6 of Grunow et al. (1996). Traces of subduction zones are shown by heavy lines with barbs, where thebarbs are drawn on the upper plate side and designate the subduction zone dip. The thinner heavy lines in (b) arefault traces. ANS, Arabian/Nubian Shield; Av, Avalonia; Ar, Armorica; EA, East Antarctica; Fl, Florida; CZ, CentralZone (Damara Belt). Other abbreviations as in Figs 7–10. Data references: 6, Goscombe et al. (2005b); 11, Gresse &Germs (1993); 12, Gray et al. (2006); 13, Gresse et al. (1988); 14, Ahrendt et al. (1977); 15, Gresse et al. (1996).


Fig. 12. Ages of orogenic suturing across Gondwana (modified from fig. 10 of Meert, 2003). The Gondwanareconstruction shows the various component orogens, the orogenic ages (bold italic) reflecting the timing of peakmetamorphism/deformation, and post-orogenic ages (normal font) reflecting post-tectonic magmatism andtherefore the timing of cratonisation, for each of the component belts. The inset (b) is an enlargement of the WestGondwana suture resulting from the closure of the Adamastor Ocean. The cratons include SF (Sao Francisco), LA (LuisAlves), RP (Rıo de la Plata), Kal (Kalahari), Congo, India and Antarctica. Component belts are BB, Brasılia Belt;AB, Aracuaı Belt; RB, Ribeira Belt; KB, Kaoko Belt; DFB, Dom Feliciano Belt; GB, Gariep Belt; SB, Saldania Belt;DB, Damara Belt; LufA, Lufilian Arc; ZB, Zambezi Belt. Data sources are shown on the figure.


arm of the Adamastor Ocean (cf. Alkmin et al.2006).

In summary, the closing of the Adamastor andKhomas oceans between three continental or cra-tonic blocks, the Rıo de la Plata, Congo and Kala-hari cratons, resulted in a three-fold orogenicsystem or collisional triple junction during thewelding of the Gondwana supercontinent. Thedifferences in timing between deformation, meta-morphism, and magmatism of the component beltsof the Damara orogen provide a history ofGondwana suturing that is more refined than thepalaeomagnetic data indicating that these cratonicnuclei were together by 550 Ma.

Support for the research was from an Australian ResearchCouncil (ARC) Large Grant A00103456 awarded toD.R.G and from NSF Grant 0440188 awarded to D.A.F.The manuscript was completed by D.R.G. as part of anAustralian Professorial Research Fellowship supportedon ARC Discovery Grant DP0210178 (awarded toD.R.G.). B.G. was supported as a Post-Doctoral Fellowfrom ARC Large Grant A00103456, and he acknowledgessupport from the University of Melbourne, the Universityof Adelaide and Monash University. We thank GabbiSchneider (Director), Charlie Hoffmann (Deputy Direc-tor), Mimi Dunaiski and Thomas Bekker of the NamibianGeological Survey for support, and acknowledge discus-sions on Namibian geology with Charlie Hoffmann, RoyMiller, Paul Hoffman and Thomas Bekker. NunoMachado and Chris Hawkesworth provided usefulreviews that helped improve the manuscript.

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