Mendum, J.R., Barber, A.J., Butler, R.W.H., Flinn, D., Goodenough, K.M., Krabbendam, M., Park, R.G. & Stewart, A.D. 2009. Lewisian, Torridonian and Moine Rocks of Scotland, Geological Conservation Review Series No. 34, JNCC, Peterborough. The original source material for these web pages has been made available by the JNCC under the Open Government Licence 3.0. Full details in the JNCC Open Data Policy
Chapter 2 Lewisian Gneiss Complex of the Outer Hebrides
Introduction
J.R. Mendum
The Outer Hebrides comprise a chain of islands some 210 km long, ranging from the largest, Lewis and Harris in the north, through North Uist, Benbecula, and South Uist, to Barra, Mingulay and finally Berneray in the south. They include a multitude of smaller islands, and the more-outlying Flannan Islands, Shiant Islands, Sula Sgeir and North Rona. Although most of the islands were strongly scoured during Quaternary glaciations, there has been significant post-glacial build-up of peat, notably thick in some rock basins, and of blown sand and machair on the western side of the Uists and Barra.
The bedrock geology of the Outer Hebrides is dominated by Archaean and Proterozoic gneissose and subsidiary schistose rocks collectively termed the 'Lewisian Gneiss Complex'. Originally called the 'fundamental gneisses' of Scotland, they were renamed by Murchison (1862) after the island of Lewis. Although of broadly similar age and origin to the mainland Lewisian rocks of north-west Scotland (Chapter 3), the exact geological relationships between the two areas remain somewhat contentious. The two basement areas are separated by a dominantly Mesozoic-age sedimentary basin, which lies mainly beneath the Sea of the Hebrides and the Minches. Recent isotopic dating of zircons from the Lewisian Gneiss Complex has shown that the ages of the gneiss protoliths and metasedimentary elements vary across the complex. Times of emplacement of the main igneous bodies and of reworking also span a much greater period than originally envisaged (Kinny and Friend, 1997; Friend and Kinny, 2001). The Lewisian rocks of the mainland and Outer Hebrides apparently had distinctly separate geological histories prior to c. 1500 Ma, but the two areas have been in fairly close proximity since c. 1100 Ma, and both acted as part of the foreland to the Caledonian Orogeny.
Geological history
The Lewisian Gneiss Complex is a product of a multi-phase depositional, intrusive, deformational and metamorphic history that spans the time period between some 3100 million years ago and some 400 million years ago. The main lithologies result from a combination of different age and type of protolith, and different amounts and degrees of structural and metamorphic reworking. The generalized history of the Lewisian Gneiss Complex in the Outer Hebrides is summarized in
Two major periods of tectonometamorphic activity have been recognized; the Scourian and Laxfordian events. During the Scourian event the main elements of the gneiss complex were formed. The bulk of the rocks were originally granodioritic, tonalitic and basaltic intrusions emplaced at mid- or lower crustal levels and subjected to deformation and metamorphism (gneiss formation) between 3100 Ma and 2500 Ma. Granite bodies and microdiorite sheets were intruded near the end of the Archaean in what is termed the 'late Scourian' at around 2600 Ma (Fettes et al., 1992). There followed the widespread intrusion of the 'Younger Basic' Suite of dolerite and basalt dykes and lenticular sheets in the Palaeoproterozoic at around 2400 Ma. Significant later accretion of possibly arc-related metasedimentary and metavolcanic rocks and intrusion of the South Harris Igneous Complex occurred at around 1880 Ma. The gneisses and earlier igneous bodies were reworked significantly between 1850 Ma and 1600 Ma, during the Laxfordian event, and it is the resultant Laxfordian folds, fabrics and metamorphic mineralogy that dominate the Lewisian rocks of the Outer Hebrides.
Subsequently, the Hebridean block was subjected to considerable uplift and erosion, and was the site of the formation of the Outer Hebrides Fault Zone (OHFZ). This gently ESE-dipping, complex structure is the product of several periods of compressional, strike-slip and extensional movements. The fault zone coincides approximately with a suture resulting from Lewisian terrane amalgamation between c. 1500 Ma and 1100 Ma (Friend and Kinny, 2001), and may have formed originally as a Grenvillian (c. 1100 Ma) thrust belt (Fettes et al., 1992; Imber et al., 2002). It was reactivated as an extensional structure at the time of deposition of the later parts of the Torridonian succession (c. 1000 Ma). Subsequent reactivation and further development occurred near the end of the Caledonian Orogeny during the main Scandian WNW-directed thrusting event at c. 435–425 Ma (Fettes et al., 1992). This was rapidly followed by further extension, which gave rise to dip-slip movements. Development of the roughly coincident Minch Fault occurred in the Mesozoic, and this structure later controlled the nature of the Palaeogene basic igneous activity that peaked at around 58 Ma.
Previous work
The Outer Hebrides were first visited for geological purposes by J. MacCulloch (1819) who carried out a cursory survey. Unlike the Scottish mainland, the Geological Survey did not map the islands in the late 19th and early 20th centuries, and T.J. Jehu and R.M. Craig of the University of Edinburgh undertook the first systematic study in the 1920s. The results were described in a series of reports in the Transactions of the Royal Society of Edinburgh between 1923 and 1934. Jehu and Craig recognized the main elements of Hebridean geology including the South Harris Igneous Complex, the Outer Hebrides Fault Zone, the mafic and ultramafic bodies, and the main outcrops of granites. A further gap in research followed, and it was only following the publication of J. Sutton and J.V. Watson's (1951) seminal work on the mainland Lewisian that work resumed in the Outer Hebrides. R. Dearnley mapped parts of South Harris (Dearnley, 1963) and also attempted to correlate wider features of Hebridean geology with the mainland (Dearnley, 1962a). Later, together with F.W. Dunning, he recognized the importance of the deformation state of a suite of Palaeoproterozoic mafic dykes, here termed the 'Younger Basic' Suite, which are equivalent to the Scourie Dyke Suite of mainland north-west Scotland (Dearnley and Dunning, 1968). This work focused on detailed studies of well-exposed coastal sections in Benbecula and South Uist and first recognized the heterogeneity and rapid spatial variations in the Laxfordian strain patterns. Also in the 1960s, Janet Watson, assisted by numerous PhD students at Imperial College, London, carried out a programme of work to map and understand the solid geology of the Outer Hebrides. A co-operative project with the Geological Survey to produce maps and reports followed. Areas not covered by PhD theses were mapped at 1:10 000 scale, existing material was compiled, and petrographical studies and chemical analyses of the main lithologies were carried out. The end result was the compilation of four 1:100 000-scale maps (Institute of Geological Sciences, 1981) and an accompanying memoir that included separate structural maps at 1:100 000 scale (Fettes et al., 1992).
In the 1970s differing views were put forward regarding the number of major basic dyke suites in the Outer Hebrides. Bowes and Hopgood (1975) and Taft (1978) argued for several suites, and Coward (1973a,b), Francis (1973) and Davies et al. (1975) suggested that there is effectively only a single suite. Fettes et al. (1992) discussed the problem and the latter viewpoint was upheld. More-recent work has focused on the Outer Hebrides Fault Zone (OHFZ), describing its long and complex structural history (Sibson, 1977a; Fettes and Mendum, 1987; Butler et al., 1995; Imber et al., 1997, 2001, 2002), and dating of the various elements in the Lewisian Gneiss Complex (Cliff et al., 1998; Whitehouse, 1990a; Friend and Kinny, 2001; Whitehouse and Bridgwater, 2001; Mason et al., 2004a,b; Mason and Brewer, 2005). In addition there has been detailed mapping, and geochemical and metamorphic studies in the south-west part of South Harris, notably on the various elements of the South Harris Igneous Complex, but also on the Langavat and Leverburgh metasedimentary belts (e.g. Witty, 1975; Dickinson and Watson, 1976; Horsley, 1978; Baba, 1997; Mason and Brewer, 2005). Baba (1998, 1999a,b) carried out detailed mapping and petrographical studies of the Leverburgh metasedimentary rocks and has described very high-pressure metamorphic assemblages, indicative of deep subduction.
Major lithologies
Mapping out and delineating the various elements of the Lewisian Gneiss Complex is difficult, even in well-exposed ground. Hence, the overall gneiss is generally represented on maps as a single unit, but discrete elements can be mapped out in places
Scourian
The protoliths of the Lewisian Gneiss Complex formed during the Archaean between 3150 Ma and 2500 Ma, and the tectonometamorphic processes that affected them during this period are assigned to the Scourian event. The oldest protoliths are metasedimentary enclaves and banded mafic and ultramafic intrusions. By analogy with Greenland, and from isotopic considerations, these units are probably between 3150 million years old and 2850 million years old (Friend and Kinny, 2001). The metasedimentary rocks are mainly brownish-weathering, schistose semipelites or rusty impure quartzose psammites. They occur typically as lenticular zones 5–50 m wide and show poorly defined contacts with the surrounding banded orthogneisses. The semipelites are recognized by their biotite-garnet-bearing assemblages, although in parts they also include sillimanite, staurolite, cummingtonite-gedrite and anthophyllite (Coward et al., 1969). Around Loch Sgioport (Skipport), Coward et al. (1969) also reported the rare occurrence of both clinopyroxene and orthopyroxene in metasedimentary rocks, although later work has failed to substantiate this mineralogy Anthophyllite is common in some of the quartzose gneisses, notably near Scolpaig in the North Uist Coast GCR site. The metasedimentary lithologies are intruded by Scourian felsic and mafic orthogneisses and are cross-cut locally by Scourian aplitic and pegmatitic granite veins. Discrete belts of more-variable metasedimentary rocks, for example those found in South Harris and around Nis in northern Lewis, were once assigned to the Archaean (see Fettes et al., 1992), but are now known to be Palaeoproterozoic in age (Friend and Kinny, 2001; Whitehouse and Bridgwater, 2001).
Spatially associated with metasedimentary rocks, particularly in the Uists and Benbecula, are lithologically distinct, compositionally finely banded, planar and lenticular, mafic-ultramafic bodies. These are termed the 'Older Basic' Suite and show ultramafic to felsic banding on a centimetre- to metre-scale. They form bodies tens to hundreds of metres across, generally with interleaved felsic orthogneiss or metasedimentary units. In South Uist bodies occur in linear belts
In the eastern part of South Uist a granulite-facies mafic metadiorite, the Corodale Gneiss (also called 'Eastern Gneiss'), occurs in the hangingwall of the Outer Hebrides Fault Zone (Coward, 1972; Fettes et al., 1992). The body exhibits relict igneous, possibly cumulate, banding in parts. This ranges from ultramafic to felsic on a centimetre- to metre-scale. In addition there appears to be an overall gradation from lower, more-mafic, parts up into more-felsic diorite. Sm-Nd and Pb-Pb whole-rock dating gives ages of 2770 ± 140 Ma and 2900 ± 100 Ma respectively, implying that this distinctive lithology is also of Archaean age and formed during the Scourian event (Whitehouse, 1993). The gneiss is bounded on its western side by a prominent thrust feature defined mainly by pseudotachylite breccia. Cataclastic fabrics and features are common throughout the unit, but on its eastern side it also shows evidence of low-grade retrogression and mylonitization. It is bounded to the east by mylonites and 'mashed' felsic gneisses. Similar foliated and fractured garnet-bearing metadiorite lithologies occur around the Butt of Lewis adjacent to the Ness Anorthosite and metasedimentary units. Whitehouse and Bridgwater (2001) obtained ion-microprobe U-Th-Pb zircon ages from the diorite showing that their protolith formed at c. 2700–2800 Ma, with Pb loss at c. 2300 Ma, and new zircon rim growth during the early Laxfordian event at c. 1860 Ma. A partly foliated, uniform metadiorite body is also exposed along the coast north-east of the Abhainn Bhuirgh (Borve River)
These metasedimentary and basic meta-igneous units were intruded by voluminous Archaean tonalitic and granodioritic sheeted intrusions, which now form the bulk of the quartzofeldspathic gneisses. In the literature they have been termed 'grey gneisses', but in this volume they are generally termed 'felsic gneisses'. Numerous small- to medium-sized mafic and minor ultramafic intrusions also form part of this igneous suite. The intrusions were apparently emplaced at mid- to lower crustal levels (> 15 km), mainly between c. 2900 Ma and 2700 Ma, and soon after emplacement were subjected to recrystallization, migmatization and gneiss formation under middle-amphibolite- to granulite-facies conditions (D1s and D2s events). These Scourian gneisses are the ubiquitous, typically banded, coarse-grained, felsic and mafic orthogneisses that form the bulk of the Lewisian Gneiss Complex. They vary from white to shades of grey, reflecting their feldspar and quartz content, and generally contain thin layers or lenticular bands rich in black biotite and dark-green hornblende. Discrete amphibolite layers and pods that range from a few millimetres up to tens of metres thick are also abundant. No major fold structures can be recognized now in the gneisses, but they have a strong, pervasive gneissose foliation and minor folds are present. Larger Scourian unbanded foliated mafic bodies up to several hundred metres across, normally amphibolite, but now partly migmatized or agmatized, have been mapped at various localities in North Lewis. They occur between the Abhainn Chuil (River Coll) and Abhainn Ghriais (River Gress) north of Stornoway, on the Eye peninsula, and on Muirneag
A further period of late-Scourian (c. 2600 Ma) igneous activity resulted in the intrusion of locally significant ultramafic, dioritic, monzonitic and granitic bodies in parts of the Outer Hebrides (Fettes et al., 1992). These intrusions all apparently cross-cut the Scourian gneissose banding and are variably deformed by the later Laxfordian events. They are best seen in eastern Barra in the hangingwall of the Outer Hebrides Fault Zone. The relationships between the various elements are particularly well displayed around Earsairidh, notably at the Leinis (Leanish) GCR site. Here, microdiorite sheets and dykes, and monzodiorite, monzonites and granite bodies intrude granulite-facies Scourian felsic gneisses containing hornblendite pods. The intrusive lithologies show no manifest signs of Laxfordian reworking and are cut by undeformed 'Younger Basic' dykes. The microdiorites are fine- to medium-grained, and range from dark-grey, melanocratic to pale-grey, leucocratic varieties. They occur as discordant but folded sheets and dykes up to 1 m thick, commonly with internal flattened and tightly folded mafic schlieren and a prominent related biotite fabric. Good examples are seen farther north on the island of Fuday
The late-Scourian 'granites' in Barra are of two distinct types: (a) pink, medium-grained equigranular monzonites that occur as irregular sheets up to 10 m thick around Earsairidh, and (b) pale-grey to salmon-pink, coarse-grained augen granites that form intrusive sheets in the metadiorites east of Castlebay. The monzonites consist of potash feldspar (string perthite), plagioclase, quartz (< 5%), foxy-red biotite, minor altered hornblende and magnetite/ilmenite. The augen granites are composed of potash-feldspar aggregates (microdine microperthite and string perthite) with quartz, plagioclase and biotite. Accessory iron oxides and apatite are common. Larger sheeted and lenticular late-Scourian granitic intrusions, in part porphyritic, are also found in the northern and western parts of North Uist, on Berneray, in north-west Lewis, and on the Eye peninsula.
All of these elements were deformed by a late-Scourian episode of deformation and metamorphism that resulted in the formation of asymmetrical folds and gave rise to the regional NNE trend of the overall gneiss foliation (D3s). Shear zones that post-date these structures are also recognized (D4s). Late-Scourian quartz-feldspar pegmatites and pegmatitic granites occur sporadically throughout the Outer Hebrides.
The 'Younger Basic' Suite
The Scourian events were followed by a period of localized deformation and metamorphism between c. 2500 Ma and 2250 Ma, termed the Inverian event', by analogy with the similar-age event documented on the mainland, notably around Scourie and Lochinver (see 'Introduction', Chapter 3). However, in the Outer Hebrides this event apparently pre-dates the 'Younger Basic' Suite and thus is Scourian (D3s, D4s) by definition, yet on the mainland it appears to be coeval with, and to post-date, the emplacement of the Scourie Dyke Suite. However, between 2500 Ma and 2000 Ma, the Outer Hebrides generally appears to have been a relatively stable area, although the currently exposed rocks still remained at mid-crustal levels. At around 2420 Ma the Scourian elements were intruded by a suite of mafic to ultramafic dykes, sheets and lenticular intrusions, with possible later phases of dyke intrusion up to c. 2000 Ma (see 'Introduction' to Chapter 3; Heaman and Tarney, 1989). This predominantly mafic intrusive suite, known in the Outer Hebrides as the 'Younger Basic' Suite, is broadly correlated with the Scourie Dyke Suite of the mainland (see Fettes et al., 1992), although Mason and Brewer (2004) argue on geochemical grounds that they represent separate dyke-swarms. The dykes are concentrated in zones with an apparent east to south-east trend and form part of a wide zone of Palaeoproterozoic mafic dykes that has been mapped in Greenland and on Baffin Island. The dykes act as an important marker, here separating an early Scourian period of crustal accretion, deformation and metamorphism from a later Laxfordian period of pervasive tectono-thermal reworking and granite intrusion
The bulk of the 'Younger Basic' dykes are metadolerites of continental tholeiite affinity; locally, olivine metadolerites, metanorites and serpentinized picrite and pyroxenite pods also occur. The dykes, sheets and pods vary from a few centimetres to over tens of metres and more rarely to hundreds of metres in thickness. One particularly large lenticular body centred on Carra-crom
In addition to the metadolerites, the 'Younger Basic' Suite includes a suite of massive, coarse-grained, grey to brown, pitted weathering, norites and picrites, known as the 'Cleitichean Beag dykes' after their type locality (Fettes et al., 1992). They are typically undeformed and form elongate pods with their long axes aligned north-west. Occurrences lie in two roughly E-trending zones, the more northerly extending east from Great Bernera to Cleitichean Beag
A number of ultramafic pods and several small ultramafic to mafic layered intrusions are also found in south and central Lewis and North Harris. These bodies are relatively fresh and the pods commonly form 'trails' across the Scourian gneisses. In fact 24 separate pods are mapped within a distinct 3 km-wide zone in central Lewis, which extends ENE from Loch Morsgail
They are mainly peridotites but dunites and pyroxenites also occur. Typically they consist of olivine, partly serpentinized, and large orthopyroxene plates up to 3 cm or even 5 cm long.
Secondary hornblende and phlogopite are present, as are minor clinopyroxene and accessory magnetite, chromite and chrome-spinel (Fettes et al., 1992). The layered intrusive bodies include the layered cumulate body at Maaruig
Belts of metasedimentary rocks and the South Harris Igneous Complex
Following emplacement of the 'Younger Basic' Suite there is evidence for the existence of tectonically active volcanic arc environments, marked by the deposition of varied sedimentary and volcanic sequences in restricted, at least partly ocean-floored, basins. The resultant infill is now represented by the Leverburgh and Langavat belts of South Harris, and the Ness Belt of north Lewis. Park et al. (2001) documented a similar scenario for the formation of the Loch Maree Group metasedimentary succession near Gairloch at between 2200 Ma and 2000 Ma. SHRIMP U-Pb zircon ages from the Langavat and Leverburgh metasedimentary rocks (Friend and Kinny, 2001) showed a range from 2780–1880 Ma for the detrital cores, and c. 1885 Ma and 1875 Ma for metamorphic rims. Sm-Nd data obtained by Cliff et al. (1998) also indicated a post-Archaean origin for the metasedimentary rocks and 207Pb-206Pb detrital zircon ages obtained by Whitehouse and Bridgwater (2001) were in the range 2150–1830 Ma. The data suggest that the metasedimentary successions were deposited in a volcanic arc environment around 1890–1880 Ma, rapidly followed by subduction, deformation and intrusion of the South Harris Igneous Complex (SHIC), all accompanied by amphibolite- to granulite-facies metamorphism.
The Leverburgh Belt, 1–1.7 km wide
Both belts are intruded by elements of the SHIC, which consists of four major meta-igneous lithologies: metagabbro, meta-anorthosite, metanorite and metadiorite. Metagabbros are very abundant as sheets and pods, and also constitute a major part of the Roineabhal layered metagabbro–anorthosite body. The upper anorthositic part of this body is the largest occurrence of anorthosite in the UK and was proposed as a site for a superquarry to supply white aggregate for use mainly as reflective road-stone. However, in the light of the unique scenery, geology, ecology and culture of South Harris the proposed quarry site at Lingreabhagh (Lingarabay) became the subject of a public enquiry in the 1990s (see Roineabhal GCR site report, this chapter). The metanorite body lies partly in the Sound of Harris and bounds the Leverburgh Belt to the south-west. The meta-diorite is generally mafic, in parts verging on gabbroic, and is the largest individual intrusion of the SHIC at c. 30 km2. It also contains an elongate body of metatonalite some 9 km long and 100–150 m wide near Bagh Steinigidh. There are also numerous associated ultramafic pods, including serpentinized lherzolites, meta-pyroxenites (websterites) and hornblendites, all metamorphosed under granulite-facies metamorphic conditions. This last event has been dated at c. 1870–1880 Ma using both U-Pb zircon techniques (Cliff et al., 1998; Friend and Kinny, 2001; Whitehouse and Bridgwater, 2001) and Sm-Nd whole-rock methods (Cliff et al., 1983). The SHIC was intruded at lower crustal levels and crystallized initially under medium-pressure granulite-facies conditions. The presence of sillimanite in the adjacent metasedimentary rocks implies pressures of c. 9 kbar (25–30 km depth) and temperatures of c. 850° C. Subsequently the rocks were further recrystallized under high-pressure granulite-facies conditions and locally sapphirine-orthopyroxene-kyanite-bearing assemblages were formed in the pelites. Baba (1998, 1999a) used the metamorphic mineralogies to construct a pressure–temperature path that reached a peak of 12–13 kbar and 8000–900° C. These conditions were attributed to a subduction-arc collision model, which would be consistent with the overall tholeiitic to calc-alkaline trends shown by the extensive geochemical data for the SHIC (Baba, 1999b).
Quartzose psammites and striped amphibolites, the latter again possibly metavolcanic in origin (cf. Langavat Belt lithologies), also occur in northern Lewis around Nis (Ness). They are intruded by a somewhat altered and strongly tectonized anorthosite. Whitehouse (1990b) obtained whole-rock Sm-Nd isotopic data and a Pb-Pb isochron from three samples of the Ness Anorthosite. These implied that the body was probably emplaced around 2300–2200 Ma and was affected by granulite-facies metamorphism at 1860 ± 240 Ma.
Laxfordian events
The pervasive Laxfordian reworking of the Archaean (Scourian) and Palaeoproterozoic elements of the Lewisian Gneiss Complex took place under amphibolite-facies conditions between 1800 Ma and 1550 Ma. It resulted in folding, imposition of locally pervasive planar and linear fabrics, and migmatization. It terminated with the intrusion of late-stage granite sheets and veins and pegmatitic rocks, accompanied by significant uplift. In the Outer Hebrides the state of the generally abundant 'Younger Basic' dykes allows the intensity of the Laxfordian deformational and metamorphic effects to be assessed. In contrast to the mainland where Laxfordian reworking is effectively absent over wide areas, Laxfordian reworking is pervasive in the Outer Hebrides with the exception of parts of eastern Barra and local low-strain areas, notably in the Uists and Benbecula. It is these exceptional areas that are described in several of the GCR site reports (e.g. Leinis, Gearraidh Siar and Baile a' Mhanaich, North Pabbay, North Uist Coast).
The folding and metamorphism occurred early in the Laxfordian event and two main phases can be distinguished (Coward et al., 1970; Fettes et al., 1992). The earlier event (D2/) resulted in pervasive gently dipping foliation and variably developed lineation. Close to tight folding on both small- and larger-scales is common, and F2 fold axes plunge gently to the north-west and south-east in the Uists and Benbecula, but more steeply to the SSE to south-west in South Harris. In northern Lewis F2 fold axes are more generally east or west plunging and are commonly subhorizontal. The later phase (D31) resulted in regional asymmetrical folding with broad hinge zones and attenuated steep limbs. The kilometre-scale F3 broad asymmetrical open antiforms and tight pinched-in synforms define the overall structural pattern of the gneissose foliation and pre-Laxfordian elements of the Lewisian Gneiss Complex in the Uists and Barra. Here, fold axes typically plunge gently to moderately to the north-west or south-east, with subvertical axial planes striking north-west or NNW The related S3 foliation/schistosity is well developed on attenuated fold limbs and in some fold hinge zones but is absent over large areas. The North Uist Coast and North Pabbay GCR sites amply illustrate the range of Laxfordian fold styles and related strain variations. In South Harris F3 fold axes plunge south-east, possibly controlled by the pre-existing orientation of the metasedimentary belts and the SHIC. However, in western North Harris they plunge at shallow angles to the west or to the ESE with F3 axial planes striking east–west and generally dipping steeply south. The sparse data in Lewis shows that, where present, F3 fold axes normally plunge gently north-east, and related axial planes dip moderately to steeply eastwards.
The Palaeoproterozoic metasedimentary belts show abundant tight folding and fabric development attributed to D2L and D3L, with any pre-Laxfordian angular relationships strongly modified. Friend and Kinny (2001) showed that the metamorphic event in the adjacent reworked Scourian quartzofeldspathic gneisses occurred at c. 1680 Ma, just prior to the emplacement of the abundant Laxfordian granites. However, as at least part of the deformation in the Langavat Belt post-dates these granites, some of the deformation and metamorphism must be post-Laxfordian. The SHIC does show regional inversion and subsequent large-scale folding, both generally attributed to Laxfordian tectonometamorphic events (Coward et al., 1970; Witty, 1975; Horsley, 1978). These tectonic events are early in the local structural chronology and may in fact be coeval with the early granulite-/upper-amphibolite-facies metamorphism at c. 1875 Ma. However, the extensive development of shear zones and amphibolite-facies retrogression, both marginal to and within the main SHIC bodies, is certainly attributable to Laxfordian events.
In the more water-deficient granulite-facies gneisses and the larger 'Younger Basic' bodies, Laxfordian reworking is normally limited to both small- and large-scale shear-zone development (e.g. Caisteal Odair in the North Uist Coast GCR site), and locally the formation of pseudotachylite. In places Laxfordian recrystallization and migmatization has resulted in the development of a coarse-grained gneissosity grading locally into a pegmatitic or agmatitic texture, with the original Scourian elements being masked or even erased. However, in many areas it is difficult to separate the earlier Scourian migmatitic textures from the Laxfordian effects unless 'Younger Basic' dykes are present. Laxfordian migmatization is best seen in the quartzofeldspathic gneisses in the western parts of Harris and south-west Lewis. Its occurrence relates to the development of Laxfordian granites, but migmatization normally pre-dates emplacement of the granite sheets and dykes. Where agmatization is well developed, F3 folding is locally associated with the generation of pegmatite. Farther north and east in Lewis migmatitic textures are not abundant. Here, D2L deformation and metamorphic features are dominant and D3L effects are apparently restricted to small-scale shear-zones and minor open folding. In South Uist and Barra, Laxfordian migmatization also occurs sporadically to the west of the Outer Hebrides Fault Zone, although here Scourian effects are normally dominant (Fettes et al., 1992).
Laxfordian granites
The Laxfordian granites post-date the main deformation episodes and are best developed in the western part of North Harris and southwestern Lewis where they form the Uig Hills-Harris Granite Vein-Complex (Fettes et al., 1992). Here, granite, porphyritic granite and leucogranite form a complex intermixture of sheets, veins and lenses up to several hundred metres thick. The granites are typically white to pink, medium-grained, biotite monzogranites, but the leucogranites range from aplitic to pegmatitic in texture. A development of late-stage aplitic granites and quartz-feldspar pegmatites is manifest as both discrete veins and more-diffuse zones at the margins of sheets and at granite-country rock contacts. In the Uig Hills the granites locally contain abundant microcline phenocrysts; this appears to be a late-stage magmatic effect. In parts the granites here are foliated and even mylonitic, particularly toward the margins of the granite complex. Fettes et al. (1992) reported several instances of aplitic and pegmatitic granites cross-cutting foliated granite, suggesting that deformation closely followed intrusion (e.g. west of Mangersta at
The granites have silica values between 68% and 75% and their geochemistry is typical of calc-alkaline suites. The restricted compositional range of the exposed granites is compatible with fractionation from more-basic parental magmas at c. 5 kbar. Aside from the Uig Hills-Harris Granite Vein-Complex, small Laxfordian granite bodies are found on An Cliseam (Clisham) and east of Aird Asaig in North Harris, at Dail Beag (Dalbeg) in west Lewis, and on the lower northern slopes of Beinn Mhòr in South Uist. They also occur as smaller veins scattered throughout the Outer Hebrides.
Granites from South Harris were dated by van Breemen et al. (1971), who obtained an Rb-Sr isochron age of 1713 Ma and a U-Pb bulk zircon age of 1678 Ma (recalculated). More recently, Friend and Kinny (2001) obtained U-Pb SHRIMP zircon ages of 1674 Ma and 1683 Ma from granite sheets in South and North Harris respectively, which they interpreted as the age of emplacement. They drew attention to the age difference between the Laxfordian granites on the mainland (1854 Ma) and those in the Outer Hebrides.
Late-Laxfordian pegmatitic granites and quartz-feldspar pegmatites are also widespread, with notable large examples at Sletteval and Ceapabhal (Chaipaval) in South Harris, which were worked for feldspar during the 1939–1945 war. The pegmatites occur generally in small swarms, with individual veins typically 1–2m across, although they do range up to 25 m wide. On Taransay, pegmatitic granites form between 25% and 75% of the exposed rock. They are generally white and pink, very coarse grained, and consist of perthitic microcline, quartz, albitic plagioclase, and biotite. Accessory minerals include magnetite (abundant), zircon, allanite, tourmaline, uraniferous minerals and in places garnet. Numerous other accessory minerals have been documented (Knorring and Dearnley, 1960; Knorring, 1959). In the Leverburgh Belt the pegmatitic granites are muscovite bearing. In South Harris they have been dated by various methods and were intruded mainly between 1700 Ma and 1500 Ma (Giletti et al., 1961; Bowie, 1964; Mason and Brewer, 2005).
Post-Laxfordian uplift
A history of progressive uplift and metamorphism at shallower crustal levels during the Laxfordian event has been documented from the meta-igneous bodies within the SHIC and the adjacent Leverburgh and Langavat belts (Dickinson and Watson, 1976; Horsley, 1978; Cliff et al., 1983; Baba, 1998). Elsewhere, only parts of the uplift history are preserved. Following Laxfordian deformation, metamorphism, and granite and pegmatite emplacement, the Lewisian Gneiss Complex was further exhumed by significant uplift and erosion. Kelley et al. (1994) obtained laser-probe Ar-Ar ages of 1430 ± 30 Ma and 1450 ± 50 Ma from biotites in the orthogneisses below the OHFZ on Grimsay. These date the closure of the Ar isotopic system in biotite by cooling, reflecting the rate and timing of post-Laxfordian uplift. By c. 1000 Ma the level of erosion was probably not greatly different to that at present.
It is unclear as to whether compressional episodes relating to parts of the Grenvillian orogenic event affected the Lewisian Gneiss Complex of the Hebrides. It certainly strongly affected pre-existing gneissose complexes in Canada and Sweden. Cliff and Rex (1989) obtained Rb-Sr biotite ages from 25 samples taken mostly from South and North Harris, but extending into central Lewis as far north as Carloway. These showed a range of closure ages between 1655 Ma and 954 Ma, mostly reflecting the post-Laxfordian uplift. In the granulite-facies rocks of the SHIC biotite ages are older, ranging from 1628 Ma to 1346 Ma, but north-east of the Langavat Belt the Rb-Sr ages generally cluster around 1200–1000 Ma. Mason and Brewer (2005) suggested that dextral-normal movements may have occurred at this time, focused on the later mylonitic rocks in the Langavat Belt. Older ages are recorded in Harris and Lewis from granulite-facies gneisses, the Maaruig ultramafic body and Laxfordian quartzofeldspathic pegmatites. Cliff and Rex (1989) suggested that the ages were compatible with uplift of the Outer Hebridean Lewisian rocks at the time of Torridonian deposition and that they may well have acted as a source of sedimentary material.
Outer Hebrides Fault Zone
The Outer Hebrides Fault Zone (OHFZ) is a coherent, but complex, zone of ductile and brittle high-strain rocks and fault rocks that extends down the eastern side of the Outer Hebrides. It stretches for over 170 km from Tolsta Bay in Lewis, to Sandray, south of Barra
The OHFZ includes gently to moderately SSE-dipping thrusts and extensional fault-zones, marked by pseudotachylite breccia, mylonites, ultramylonites, and phyllonites. Fault gouge is found along later along-strike and across-strike faults. Between the thrusts and faults are significant thicknesses of more-massive cataclastic gneisses and protomylonitic gneisses, aptly termed 'Mashed Gneiss' by Jehu and Craig (1925). The zone is unique in the UK in that it contains abundant examples of pseudotachylite. The different elements range in age from post-Laxfordian (c. 1650–1100 Ma) to Caledonian (Scandian c. 430–420 Ma) and Mesozoic (in part Permo-Triassic). The history of the zone has been summarized by Fettes et al. (1992) and more recently by Imber et al. (2001, 2002).
Rock types
Pseudotachylite is a black glassy rock when fresh, which results from localized frictional melting of the relatively dry country rock along fault planes during seismic movements. Subsequently the glass is typically devitrified and retrogressed to a grey or brown, very fine-grained material as in the Outer Hebrides examples. Its melt origin is indicated in places by feldspar microlites, and it commonly includes angular to rounded fragments of quartz, feldspar and more rarely hornblende. Once frictional heat has generated a melt, there is a sudden release of the pent-up energy and the melt cools very rapidly; the process lasts only seconds. Hence, the thickness of melt produced along generation planes is limited during individual seismic movements. Thicker zones are due to migration of melt away from the generation surface and/or multiple seismic movements. Jehu and Craig (1923), Sibson (1975, 1977a) and Fettes et al. (1992) all noted the features and occurrences of pseudotachylite, which are particularly well displayed in South Uist and Barra. The Cnoc an Fhithich GCR site in north-west Barra provides excellent examples.
In the Outer Hebrides pseudotachylite is commonly intermixed with cataclasite, an aphanitic, structureless, cohesive, fragmental breccia with the fragments < 0.2 mm across, which results from rock comminution in fault-or shear-zones. It commonly weathers grey or brown. Where fluids are present and the deformation processes have been more ductile, mylonite results. This forms distinct planar zones up to 30 m or 40 m thick consisting of fissile to flaggy, typically finely colour-banded, pale-green to fawn and even cream, fine-grained rock. Quartz, muscovite, chlorite, epidote and sericite are the dominant minerals that define the banding, whereas plagioclase feldspar and hornblende generally form more-resistant augen. Titanite (after ilmenite) is common in the more-mafic rock-types. In contrast to pseudotachylite, mylonites formed along mostly aseismic shear- and fault-zones by ductile processes, involving mainly recrystallization and grain-size reduction, grain-boundary sliding, and concomitant metamorphic changes of mineralogy. If the degree of strain was very high, the mylonites can be extremely fine grained and are termed 'ultramylonite'. The mineralogy and textures vary, dependent on the ambient pressure and temperature conditions. Lower amphibolite-facies mylonites have been found locally in south-east Lewis around Ceann Shiphoirt (Seaforth Head)
The term 'Mashed Gneiss' encompasses the brecciated, partially cataclastic, and protomylonitic orthogneisses that make up much of the OHFZ. In many places the gneissic foliation has become disorientated to such an extent that the rock resembles a fine to coarse breccia. Pseudotachylite is common in this zone, as is cataclasite, but the gneiss and the fault rocks are typically retrograded.
Fault zones are marked by locally intense fracturing and in parts by clay-rich fault gouge. Good examples are documented in Barra and the adjacent small islands (MacInnes et al., 2000), where they range from SE-dipping brittle thrust planes to more generally steep structures that offset the mylonitic fabrics and earlier thrust features. In South Uist, just south of Rubha Bholuim (Bolum)
Relationships between the various rock-types are clear in some areas but local examples cannot necessarily be translated to the fault zone as a whole. Good relationships are exposed in the notably wide outcrop of the OHFZ in southeast Lewis. Here, pseudotachylite veins cut early-formed amphibolite-facies mylonites in the Baile Ailein area
Distribution of features and rock types of the Outer Hebrides Fault Zone (OHFZ)
The features recognized along the length of the OHFZ vary markedly and are best considered geographically as typical of either Lewis and Harris or the Uists and Barra.
In Lewis and Harris the OHFZ affects the mainly felsic orthogneisses and a significant thickness of 'Mashed Gneiss' and gneisses with protomylonitic and cataclastic fabrics is developed. This zone extends for c. 8 km west of Stornoway and is 15 km wide in the Park district of south-east Lewis. Its western limit is marked by a thick cataclasite + retrograde pseudotachylite breccia zone that dips gently to the southeast. When traced southwards this bounding zone becomes more diffuse, and mylonites and pseudotachylite-rich zones are widespread within the OHFZ. These are well seen around Ceann Shiphoirt
In the Uists, the zone of alteration is again roughly coincident with the incoming of mylonites and phyllonites. Hence, it is only the western parts of the OHFZ outcrop that are largely unaffected by the hydrous retrogression. The fault zone is formed in the Laxfordian gneisses in North Uist and shows a broad transition from the early-formed pseudotachylite breccias at lower structural levels in the west to the later mylonites, phyllonites and folded phyllonites farther east. Note that the thrust products are out-of-sequence (cf. Moine Thrust Belt) and here reflect progressively younger periods of fault-zone activity eastwards at higher structural levels.
'Mashed Gneiss' is extensively developed on North Uist, for example east of Lochportain
On Barra the thrust at the base of the OHFZ is marked by 25–75 m of pseudotachylite, cataclasite and breccia and forms a prominent relief feature. However, the gneisses in the hanging-wall are virtually unaffected by deformation, brecciation, and so on. Laxfordian structures have been interpreted as being displaced across the thrust (Francis, 1973; Sibson, 1977a,b), and granulite-facies orthogneisses are present both above and below the thrust. Matching of features implies only limited displacement and the exposed thrust feature possibly represents a forethrust of the main OHFZ that itself lies offshore to the east in the Sea of the Hebrides.
Faulting
In addition to the dominant E-dipping thrust and extensional structures that dominate the OHFZ, normal and strike-slip faulting have also occurred at various stages of development. Stein (1988) used two-dimensional seismic reflection lines from the Minches to show that the interpreted Torridonian succession thickens westwards, and suggested that a bounding low-angle fault was active during deposition at c. 1000 Ma, at least adjacent to Lewis and Harris (see Imber et al., 2001). Butler et al. (1995) suggested that sinistral strike-slip movement took place along the OHFZ as part of its main development. They based this on the recognition of near-strike-parallel mineral lineations, quartz-feldspar porphyroblast shapes (0-type and 8-type), and shear bands in phyllonites from North Uist (Eaval–Eigneig Bheag area), the Park district of south-east Lewis, and from Scalpay. The lineations are subhorizontal to gently NE-and SW-plunging. They argued that such movement was focused along the pre-existing weak phyllonite zones, which were reactivated again in Mesozoic times to form the steeper Minch Fault that lies immediately offshore to the east of the Outer Hebrides. In the Sound of Barra, Maclnnes et al. (2000) have documented a range of faults that relate both to thrust and extensional movements on the OHFZ and to later WNW-trending sinistral faults of probable Mesozoic age that cross-cut all the earlier OHFZ structures and fabrics. Similarly orientated late faults also cut the gneisses on Barra itself and are mapped farther north in the Uists and into the Sound of Harris where they trend north-west. WNW- and NW-trending faults also form prominent features in Harris and Lewis, for example the Tarbert and Loch Liurboist (Leurbost) faults, but although some show sinistral offsets of OHFZ features, others appear to be normal or reverse faults. A 10–12 km-wide zone of NNW-trending subvertical faults stretches from Loch Seaforth (Shiphoirt) and Loch Claidh in southeast Lewis up to West and East Loch Roag in west Lewis. The faults cut OHFZ features but there is evidence of earlier more-ductile movements and areas of steep foliation within this zone.
Although the OHFZ generally has a distinct western bounding structure, pseudotachylite veins, breccias, and mylonitic gneisses related to the main fault-zone also occur extensively farther west in the Outer Hebrides (Fettes and Mendum, 1987)
Tectonic history of the Outer Hebrides Fault Zone (OHFZ)
The age and mechanisms of generation of the OHFZ are not fully known. What is clear is that the fault zone has seen a long and varied history, now represented by the various fault rocks found along its length (
Fettes et al. (1992) suggested that the foliations in the late-Laxfordian granite sheets of the Uig Hills were generated approximately coeval with their intrusion. They noted several instances of pegmatites cutting foliated granite sheets. If indeed this is the case, and the OHFZ initiation is related to this NW-directed shearing deformation, its initiation must have occurred around c. 1670 Ma. The granite sheets certainly have acted as loci for WNW-directed thrust movements, but these movements may be mainly of later age, possibly Grenvillian (c. 1100 Ma) as suggested by Imber et al. (2002). However, both time-periods record apparent uplift and extension of the gneiss complex, as shown by intrusion of granite sheets and the Grenvillian Rb-Sr closure ages (Cliff and Rex, 1989) respectively. Such conditions are not reconciled easily with compressional NW-directed thrust movements. Initial thrust movements on the OHFZ may link to transcurrent movements along major shear-zones, such as the Langavat Belt or possibly along a major structure that now lies offshore to the east in the Minches and Sea of the Hebrides. However, no compelling evidence points to a linked thrust–transcurrent faulting pattern. If Grenvillian or earlier movements did occur it is likely they resulted in the amphibolite-grade mylonites and possibly the generation of at least some of the pseudotachylite breccia zones that represent major westward thrusting.
Kelley et al. (1994) obtained laser-probe Ar-Ar ages from the matrix of a pseudotachylite vein in the immediate footwall of the OHFZ on Grimsay that gave a weighted mean of 430 ± 6 Ma. This is broadly compatible with whole-rock K-Ar dates obtained by D.C. Rex (in Sibson, 1977b) from various thrust rocks in the Uists and Barra. Pseudotachylite and cataclasite ages ranged from 2056 Ma to 442 Ma and mylonites from 471 Ma to 394 Ma. Errors are quite large and the possibility of excess radiogenic Ar from the adjacent gneisses or from included clasts is likely. S. Moorbath (also in Sibson, 1977b) reported K-Ar ages of 1120 Ma and 1140 Ma from pseudotachylite west of the OHFZ in South Uist. Again errors are large (± 44 Ma). The isotopic ages allow for movements at several periods ranging from Grenvillian to Scandian. They strongly imply that WNW-directed thrust movements did occur at around 430 Ma, coeval with major Scandian movements on the similarly orientated Moine Thrust Belt on the Scottish mainland and its northward continuation in Greenland. Deeper-level structures with similar trends and dips are interpreted on the MOIST (Moine and Outer Isles Seismic Traverse) and other BIRPS (British Institutions Reflection Profiling Syndicate) deep seismic reflection profiles that lie offshore from the Outer Hebrides (Smythe et al., 1982; Stoker et al., 1993). These Scandian tectonic movements relate primarily to the collision of Baltica and Greenland, but extended southwards to encompass the foreland areas of north-west Scotland and the Outer Hebrides. In the OHFZ these resulted in low-grade mylonites and phyllonites, first formed during WNW-directed thrusting and subsequently by WNW–ESE extension.
However, the role of the pseudotachylite breccias and 'Mashed Gneiss' is unclear. In parts they may represent Scandian compressive events that occurred prior to the ingress of fluid that culminated in mylonite formation. In other areas they may well be Grenvillian or even earlier in age as discussed above. Imber et al. (2001) and Fettes et al. (1992) postulated that the OHFZ may reflect pre-1100 Ma thrusting resulting in early mylonites, Grenvillian dextral shearing, and later dip-slip faulting at the time of Torridonian sediment deposition. This last event, at c. 1000 Ma, would have extensionally reactivated the already formed moderately ESE-dipping OHFZ thrust structure. However, Imber et al. (2001) suggested that the main episode of pseudotachylite and cataclasite formation accompanied WNW-thrusting during the Scandian Event (c. 430 Ma), followed by significant sinistral strike-slip movements focused on the phyllonite zones and later dip-slip movement in extension at c. 400 Ma. A phase of Carboniferous- to Cenozoic-age faulting is also recognized.
The magnitude of the postulated Silurian sinistral strike-slip movement is unclear. Butler et al. (1995) and Imber et al. (2001) proposed that some 90 km of relative movement occurred, distributed on the phyllonite belts throughout the Outer Hebrides. However, Maclnnes et al. (2000) found no evidence for such movements in Barra and the adjacent islands, and the proposed linking of Lewisian features between the Outer Hebrides and the mainland (e.g. Dearnley, 1962a; Lisle, 1993) may well be invalid (see Friend and Kinny, 2001). The lack of any coherent major steep structure along the OHFZ at this time, except possibly for an embryo Minch Fault offshore, would appear to make it difficult to have lateral movements on the scale envisaged.
Sibson (1977a, 1983) and Scholz (1988) suggested that major fault-zones such as the OHFZ consist of an upper crustal-seismogenic zone deforming by frictional processes, which passes down to a lower aseismic zone, deforming predominantly by viscous processes. However, Imber et al. (2001) rejected the Sibson–Scholz model, and pointed out that the various fault rocks of the OHFZ record a lengthy and complex history of thrusting and extension. They proposed an alternative model, whereby early formation of a crustal-scale hydrous phyllonite–mylonite zone acted as a locus for subsequent tectonic movements. If Friend and Kinny (2001) are correct in identifying different Archaean and Proterozoic terrains within the Lewisian Gneiss Complex of the Outer Hebrides and mainland north-west Scotland, then it is possible that the OHFZ is roughly coincident with an earlier Proterozoic-age suture that separates crustal blocks with disparate histories. The isotopic ages for the various Lewisian elements would constrain the formation of this suture to between c. 1500 Ma and 1100 Ma.
Post-Lewisian minor intrusions and sedimentary rocks
Late Caledonian intrusions are largely absent from the Outer Hebrides but an isolated appinitic diorite dyke occurs in the Uig Hills–Loch Roag area and a small diorite exposure occurs at Loch Fada in North Uist (Fettes et al., 1992).
WNW-trending, late Carboniferous, quartz-dolerite dykes occur in Barra and South Uist; where Fettes et al. (1992) reported some 10 dykes, ranging from 3 m to 45 m thick. Later thin camptonite and monchiquite dykes, of latest Carboniferous to Permian age, that also trend WNW, are found more widely through the Outer Hebrides, but are only common in South Uist.
The bulk of the minor intrusions in the Outer Hebrides are the NW-trending dolerite dykes of Palaeogene age. They are seen in many of the GCR sites. Their concentrations are such that in Barra, South Harris and Lewis, distinct swarms have been recognized (Speight et al., 1982; Fettes et al., 1992).
Post-Lewisian sedimentary rocks are limited to red-brown conglomerates and sandstones of Permo–Triassic age that occur around Stornaway and on the Eye peninsula of Lewis