No Job Name Neoproterozoic metamorphic evolution of the Isbjørnhamna Group rocks from south-western Svalbardpor_186 250..264 Jaroslaw Majka,1 Jerzy Czerny,2 Stanislaw Mazur,3 Daniel K. Holm4 & Maciej Manecki2 1 Department of Earth Sciences, Uppsala University, Villavägen 16, SE-75236 Uppsala, Sweden 2 Department of Mineralogy, Petrography and Geochemistry, AGH–University of Science and Technology, 30 Mickiewicza Av., PL-30059 Kraków, Poland 3 GETECH, Kitson House, Elmete Hall, Elmete Lane, Leeds, LS8 2LJ, UK 4 Department of Geology, Kent State University, Kent, OH 44242, USA Abstract A metamorphosed volcano-sedimentary complex constitutes the Caledonian basement in the south-western part of Wedel Jarlsberg Land, Svalbard. Field, textural and previous thermochronologic data indicate a weak, localized meta- morphic Caledonian overprint (M2). Deformed M1 isograds and variation in pressure–temperature estimates indicate a pervasive Neoproterozoic amphibolite-facies metamorphism that pre-dates large-scale Caledonian age folding. Garnet–biotite and garnet–Al silicate–plagioclase (GASP) geother- mobarometry of the Isbjørnhamna Group mica schists, and their comparison with the K2O–FeO–MgO–Al2O3–SiO2–H2O (KFMASH) petrogenetic grid, indi- cates a peak pressure of ca. 11 kbar, and a peak temperature of ca. 670°C during M1 metamorphism. A cooling rate of ca. 5°C My-1 is estimated on the basis of geothermobarometry and the available U–Th–total Pb and Ar–Ar data. Keywords Caledonides; geothermobarometry; metapelites; Neoproterozoic; Spitsbergen. Correspondence Jaroslaw Majka, Department of Earth Sciences, Uppsala University, Villavägen 16, SE-75236 Uppsala, Sweden. E-mail: jaroslaw.majka@geo.uu.se doi:10.1111/j.1751-8369.2010.00186.x Southern Wedel Jarlsberg Land (Fig. 1) uniquely pre- serves a record of Neoproterozoic metamorphism on Spitsbergen, Svalbard. In situ uranium–thorium–lead electron microprobe (U–Th–Pb EMP) ages of metamor- phic monazites from a Proterozoic volcano-sedimentary complex date amphibolite-grade metamorphism at ca. 643 Mya (Majka et al. 2008). The northern extent of this Neoproterozoic metamorphism is bounded by the Vimsodden–Kosibapasset zone (VKZ), which is a major strike–slip shear zone with sinistral kinematics (Fig. 2; Mazur et al. 2009). The VKZ separates the Neoproterozoic metamorphic complex from the remaining part of the south-western terranes of Svalbard, which were sub- jected to younger, early Palaeozoic metamorphism (Gee & Tebenkov 2004; Czerny et al. 2010). The occurrence of a Neoproterozoic metamorphic domain in south-western Spitsbergen has important bearing on terrane concepts for Svalbard construction in general, and specifically for its proposed correlation with the Timanide metamorphic belt of north-eastern Europe (Mazur et al. 2009). A better understanding of the nature and extent of Neo- proterozoic metamorphism and associated pervasive deformation, compared with earlier reports (Smulikowski 1965; Czerny et al. 1993; Majka et al. 2004), is an essen- tial prerequisite for testing between, and refining, the tectonic models proposed for this region. In this study we: (1) quantify the peak pressure and temperature condi- tions for Neoproterozoic metamorphism; (2) verify the correlation between the peak of metamorphism and the pervasive deformational fabric; (3) define zones of pro- gressive metamorphism and the relationship between isograds and major tectonic structures; and (4) constrain the cooling history of this Neoproterozoic complex. Our study is based on extensive fieldwork supported by results of microstructural analysis and geothermobarometric calculations. Geological setting The south-western part of Spitsbergen island exposes an elongate north–south trending metamorphic basement exhumed within the axial zone of an Early Palaeogene fold-and-thrust belt (e.g., Lowell 1972; Dallmann et al. 1993; Braathen et al. 1995; Bergh et al. 1997). This elevated basement high consists of Precambrian to Early Palaeozoic rocks, the deformation and metamor- phism of which were originally ascribed solely to the Caledonian orogeny (e.g., Holtedahl 1926; Ohta 1982; Harland 1985; Harland et al. 1992). However, the occur- rence of regionally extensive unconformities that are Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd250 mailto:majka@geo.uu.se associated with metamorphic and lithological contrasts (e.g., Sandford 1956; Krasil’ščikov 1979; Birkenmajer 1975; Bjørnerud 1990) and geochronological studies both provide evidence that the Caledonian basement includes Proterozoic crustal domains juxtaposed by Early Palaeozoic tectonic events (e.g., Peucat et al. 1989; Balashov et al. 1995; Gee et al. 1995; Hellman et al. 1997; Johansson et al. 2004; Pettersson et al. 2009). These domains, together with their sedimentary cover, are interpreted to be individual tectonostratigraphic terranes assembled during the Caledonian orogeny (e.g., Harland 1972; Harland & Gayer 1972; Gee & Page 1994). Based on important contrasts in stratigraphy, structural develop- ment and tectonothermal evolution, the Caledonian rocks of Svalbard have been divided into eastern, north- western and south-western terranes (Fig. 1; Gee 1986; Gee & Page 1994; Gee & Tebenkov 2004). North of Isfjorden, the south-western terranes of Svalbard include a blueschist–eclogite allochthon known as the Vestgötabreen complex (e.g. Ohta 1979) that yielded argon-40 (40Ar)–argon-39 (39Ar) mineral cooling ages of ca. 460 My (Dallmeyer et al. 1990). The complex is non-conformably overlain by Middle Ordovician conglomerates and limestones (Armstrong et al. 1986), succeeded by Late Ordovician to Early Silurian turbidites (Scrutton et al. 1976). The metamorphic basement, together with its Early Palaeozoic cover, is thrust over a succession of diamictites of inferred Vendian age (Gee & Tebenkov 2004). To the south of Isfjorden, the south- western terranes consist of a Meso- to Neoproterozoic Fig. 1 Geological sketch map of the Svalbard Archipelago (modified from Gee & Tebenkov 2004). Neoproterozoic metamorphism in southern SvalbardJ. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd 251 metamorphic complex, which is divided into three units: Isbjørnhamna, Eimfjellet and Deilegga groups (Birkenmajer 1981, 1991). The latter is non-conformably overlain by the low-grade Neoproterozoic Sofiebogen Group, comprising a succession of conglomerates, lime- stones and dolomites passing up into fine-grained siliciclastic rocks (Bjørnerud 1990; Czerny et al. 1993; Gee & Tebenkov 2004). The Sofiebogen Group is capped by Vendian tillites of the Kapp Lyell Group, and comprises a thick series of diamictites (Bjørnerud 1990; Dallmann et al. 1990; Harland et al. 1993). The Cambro–Ordovician succession is tectonically emplaced atop the Proterozoic complexes (Dallmann et al. 1993; Mazur et al. 2009). Wedel Jarlsberg Land, located in the southern part of the south-western terranes (Fig. 2), consists of two Prot- erozoic basement blocks with contrasting metamorphic histories. The northern block comprises rocks of the metasedimentary Deilegga and Sofiebogen groups, which are separated by a Late Proterozoic angular unconformity (Torellian unconformity; Birkenmajer 1975). The south- ern block corresponds to a stratified volcano-sedimentary polymetamorphic complex that consists of a metasedi- mentary sequence known as the Isbjørnhamna Group and a metavolcanic succession of the Eimfjellet Group (Birkenmajer 1958; Czerny et al. 1993). The Isbjørn- hamna Group is composed of garnet–mica schists, paragneisses, calc-silicate rocks and marbles subjected to amphibolite-grade Barrovian metamorphism, which was followed by greenschist facies metamorphism (Smulikowski 1965; Majka et al. 2004). The Eimfjellet Group consists of quartzites, amphibolites and green- schists, accompanied by minor metarhyolites and muscovite schists. These rocks were subjected to green- schist to lower amphibolite facies (Czerny et al. 1993). The contact between the two crustal blocks exposed in the south-western part of Wedel Jarlsberg Land between the Hornsund fjord and Torellbreen glacier is represented by the ca. 2 km wide VKZ. The deformation zone is char- acterized by a heterogeneous array of structures formed during ductile shear deformation. Structural features of the VKZ indicate bulk sinistral strike-slip to oblique-slip shear strain formed under greenschist facies conditions. Thermochronologic data obtained from the Isbjørn- hamna and Eimfjellet groups indicate a Neoproterozoic age of metamorphism. 40Ar–39Ar step heating of mineral separates yielded a 616 My age for hornblende from the Fig. 2 Geological sketch map of the south- western part of Wedel Jarlsberg Land (modified from Czerny et al. 1993). Neoproterozoic metamorphism in southern Svalbard J. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd252 Eimfjellet Group, and 585–575 My ages for muscovite from the Isbjørnhamna Group (Manecki et al. 1998). Manecki et al. (1998) interpreted these ages as represent- ing a previously unrecognized episode of Neoproterozoic reheating, probably connected with the opening of the Iapetus Ocean. Corroborating evidence of a Neoprotero- zoic tectonothermal event is provided by a metamorphic monazite age of 643 � 9 My recently obtained from the Isbjørnhamna Group (Majka et al. 2008). This age was interpreted to represent the progressive phase of a regional metamorphic event, as monazite grains enclosed in garnet porphyroblasts yielded the same age as matrix monazite grains. A somewhat younger Neoproterozoic age (615 My) was obtained on zircons separated from an anatectic pegmatite, which intrudes the Isbjørnhamna Group (Majka et al. 2007). Description of metamorphic units The Isbjørnhamna Group consists of the Skoddefjellet, Ariekammen and Revdalen formations, representing an originally continuous sedimentary succession (Birkenmajer 1975). Skoddefjellet Formation The Skoddefjellet Formation is composed of interlayered paragneisses and mica schists. Typical prograde mineral assemblages in these rocks are Qtz + Pl + Bt + Ms � Grt � Chl with greater quantities of plagioclase in parag- neisses and garnet in mica schists. The mica schists are well foliated with common garnet and biotite porphyroblasts. The matrix is mainly com- posed of quartz, plagioclase (<15% vol.) and phyllo- silicates. Biotite occurs mainly within the foliation planes, in the pressure shadows of garnet and as a product of garnet decomposition. Additionally, biotite forms porphy- roblasts transverse to the foliation and enriched in small graphite inclusions. Very rarely biotite occurs as inclu- sions in garnet. Muscovite occurs mainly in foliation planes, in the pressure shadows of garnet and sometimes replacing garnet porphyroblasts. Primary chlorite occurs in the foliation planes, whereas secondary chlorite replaces micas in the pressure shadows of garnet and occurs as rosettes within the matrix. The accessory phases comprise tourmaline, apatite, zircon, monazite, epidote group minerals, titanite, ilmenite, hematite, pyrite, pyro- tite and chalcopyrite. Ariekammen Formation The Ariekammen Formation is characterized by the occurrence of carbonate rocks. The formation mostly consists of carbonate–mica schists, with irregular bands of mica schists, paragneisses of the Skoddefjellet type and minor marble intercalations. A mineral assemblage characteristic of carbonate-mica schists comprises Cal + Qtz + Bt + Grt + Pl + Ms � Ep, with Ca-enriched plagio- clase and accessory minerals similar to those found in the Skoddefjellet Formation. Additionally, some schist variet- ies contain rare mejonite. Notably, a thin discontinuous horizon of yellow and white marble occurs in the middle of the formation. Porphyroblasts of garnet up to 6 cm in diameter are abundant at the base of this horizon. Revdalen Formation The Revdalen Formation represents a uniform sequence of rusty weathered mica schist composed of Qtz + Pl + Ms � Bt � Grt � St � Ky � Cld � Chl. Metamorphic isograds within these rocks are defined by the local pres- ence of chloritoid, staurolite or kyanite. The mica schists are well foliated with numerous garnet porphyroblasts and rare transversal biotite and staurolite porphyroblasts. The matrix mostly consists of quartz and phyllosilicates and minor plagioclase. Muscovite occurs in all varieties of the Revdalen mica schists, whereas biotite is absent from chloritoid-bearing samples, which tend to be rich in primary chlorite. All phyllosilicate types can be found in the pressure shadows of garnet and staurolite, and both micas exist as inclusions in garnet. Rare kyanite occurs in samples containing garnet and/or staurolite. The remain- ing accessory phases comprise abundant tourmaline, zircon, monazite, apatite, epidote (sometimes allanite), titanite, rutile, and Fe-oxides and -sulphides. Addition- ally, some younger Fe-oxyhydroxides and carbonates are also present. Description of textures The Isbjørnhamna metapelites exhibit a penetrative planar S1 foliation, a well-developed L1 mineral stretch- ing lineation, particularly in the Skoddefjellet mica schists, and locally developed S–C fabrics (most common in the Revdalen Formation). The S1 foliation is expressed by aligned phyllosilicates and flattened garnet and stau- rolite porphyroblasts (Fig. 3). Deformation resulted in the ductile flattening of garnets and the development of asymmetric pressure shadows filled with biotite, musco- vite, quartz and plagioclase. The flattened and slightly rotated garnets often contain helicitic inclusions. Inclu- sion trails in rare euhedral garnet porphyroblasts, occurring in low strain zones, parallel the S1 foliation. Some staurolite porphyroblasts are slightly flattened and accompanied by pressure shadows filled with muscovite and quartz. In many cases, however, staurolite grains are Neoproterozoic metamorphism in southern SvalbardJ. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd 253 inclusion-free and euhedral, with only narrow asymmet- ric mica-filled pressure shadows. The transversal character of biotite porphyroblasts is expressed by the orientation of their cleavage planes that are oblique to the S1 foliation. The cleavage is underlined by common graphitic encrustations, possibly representing a relict S0 layering. The biotite porphyroblasts are flat- tened and accompanied by asymmetric tails of fine- grained biotite. M1 metamorphism Metamorphic isograds are well-defined within the metapelites of the Revdalen Formation. For samples col- lected in the north-western part of the study area, from the western limb of a north–south trending anticline out- cropping in the Rålstranda, the prograde M1 mineral assemblage is defined by Grt + Cld + Ms + Chl + Qtz � Pl. Chloritoid-bearing and biotite-absent metapelites occur exclusively in the region of the Russepynten cape. East- wards from that region, the mineral assemblage changes into Grt + Bt + Ms + Qtz � Pl � Chl and farther east into Grt + St + Ms + Bt + Qtz � Pl � Chl. By contrast, in the east and south-eastern part of the study area (Revdalen, Skålfjelldalen and Fugleberget), the mineral paragenesis is defined by the occurrence of Grt + Ms + Bt + Qtz � Pl, whereas only in a very few cases are additional kyanite or kyanite and staurolite recorded. The rare occurrence of Al-saturated phases is related to local changes in bulk rock composition. In the schists from the Rålstranda area, very fine-grained progressive allanite and epidote were observed, whereas farther east and south the dominant rare earth element-bearing phase is monazite. The transition of allanite into monazite is con- sistent with the increasing metamorphic grade within the Revdalen Formation to the east because allanite is stable only at upper greenschist to lower amphibolite facies conditions; with increasing temperatures, allanite is Fig. 3 Photomicrographs of (a) slightly rotated anhedral garnet with asymmetrically developed pressures shadows and its relationship to biotite; (b) deformed and slightly rotated staurolite; (c) deformed large biotite; and (d) retrogressive rosette-shaped chlorite. Neoproterozoic metamorphism in southern Svalbard J. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd254 replaced by monazite (e.g., Ferry 2000; Janots et al. 2007). Retrogressive stage of M1 metamorphism A retrogressive alteration was associated with cooling after the peak of M1 metamorphism. In many cases, retrogression resulted in the partial or complete replace- ment of garnet by the assemblage of Bt + Ms + Pl + Q � Chl or Pl + Q � Chl. Partial replacement of biotite by chlorite may also be related to this phase of metamorphic evolution. Additionally, the partial or even complete replacement of monazite by apatite–allanite–epidote coronas in some samples is a common reaction indicative of late-metamorphic cooling (e.g., Ferry 2000; Majka & Budzyń 2006, Janots et al. 2007, Broska & Majka 2008). The character of the retrogressive changes and the mineral assemblage synchronously formed suggest that retrogression took place shortly after the peak of M1 metamorphism. Weak Caledonian M2 overprint The Isbjørnhamna Group belongs to Proterozoic base- ment exposed in the core of the West Spitsbergen fold- and-thrust belt. The main Caledonian structure in the study area is the VKZ trending from north-west to south- east (Czerny et al. 1993; Mazur et al. 2009). The effects of Caledonian deformation are widespread to the north of this zone. Contrastingly, southwards from the VKZ, Caledonian overprint rapidly dies out in the rigid amphibolite facies tectonic block, including the Isbjørn- hamna Group. Only the rocks of the Eimfjellet Group, which are adjacent to the VKZ, experienced intense Cale- donian mylonitization (Mazur et al. 2009), whereas the rocks of the Isbjørnhamna Group do not reveal any sig- nificant Caledonian reworking, except in a few relatively thin zones of altered rocks, usually parallel with VKZ. The only visible effect of the Caledonian event is the partial or sometimes complete chloritization of garnet, biotite and staurolite, as well as the alteration of musco- vite porphyroblasts to sericite. Additionally, in some cases Caledonian alterations are expressed by the development of sericite reaction rims on kyanite, and by sericitization of staurolite and plagioclase. These changes probably took place under static conditions, as indicated by the common growth of rosette-like chlorite neoblasts (Fig. 3). Mineral chemistry Selected minerals were chemically analysed using wave- length dispersive spectrometry with the 100SX electron microprobe (Cameca, Grennevilliers Cedex, France) at the Inter-Institute Analytical Complex for Minerals and Synthetic Substances, University of Warsaw. The operat- ing conditions were set at 15 kV, 20 nA and 20 s of the counting time using natural and synthetic standards. The data were calculated using atomic number, absorption and fluorescence (ZAF) corrections. Garnets Garnets were analysed along rim-core-rim profiles. Por- phyroblasts of garnet were selected from different metamorphic zones within the Revdalen and the Skod- defjellet formations. Representative traverses are shown in Fig. 4. A common feature of garnets from the kyanite- free mica schists (i.e., samples 206, 214 and 125) is the systematic increase of pyrope content from the core to rims, and the contemporary decrease of Fe/(Fe + Mg) and spessartine content. The rimward decrease of Fe/(Fe + Mg) is characteristic of the increase of tempera- ture under upper greenschist and amphibolite facies conditions (Spear 1993). The bell-shaped spessartine profile also suggests prograde growth zoning during a one-stage chemical reaction (Tracy 1982). The slight increase of spessartine content that was observed in some garnet rims may be related to the consumption of garnet. Notably, garnet from the staurolite-bearing mica schists reveals a decrease of Fe/(Fe + Mg) towards the rims, but in the rims this tendency changes and Fe/(Fe + Mg) is flat or even slightly increased. The almandine content in this garnet systematically increases towards the rims, but in the rims it decreases. The opposite trend is evident for the grossular content, which systematically decreases towards the rims, but rapidly increases in the rims. The variation of grossular and almandine content in garnets co-existing with staurolite may have been caused by the onset of staurolite crystallization (see also Janák et al. 2001): the onset of staurolite crystallization could modify local chemical equilibrium during garnet crystallization, decreasing the almandine content in garnet, as observed in our samples. Contemporaneously, the observed enrichment in Ca is probably caused by the reduction of crystallization of plagioclase in response to the appear- ance of a new Al-saturated phase (e.g., staurolite). Nevertheless, the smooth shape of decreasing spessartine content suggests prograde growth during a single meta- morphic event. The compositional variation in garnet from the kyanite-bearing mica schist (i.e., sample 124) is complex. In all cases the profiles are strongly disturbed, probably as a result of the presence of numerous tiny inclusions and the diffusion that occurred between them and the hosting garnet. Nevertheless, the almandine and pyrope zoning Neoproterozoic metamorphism in southern SvalbardJ. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd 255 suggest garnet growth during prograde metamorphism, although the distribution of spessartine and grossular content seem to be homogenized. If so, this homogeniza- tion may have occurred during an early stage of retrogression (Spear 1993), connected with a general decrease of pressure. Garnets from the high-Al Revdalen Formation schists (i.e., samples 124 and 206) are characterized by relatively lower grossular and higher almandine content, compared with low-Al Revdalen Formation and Skoddefjellet For- mation schists (samples 125 and 214, respectively). Staurolite Staurolite porphyroblasts as well as staurolite enclosed in garnets do not reveal any chemical zonation. They are Fe-staurolites, with Fe in the range of 1.55–1.74 atoms per formula unit (apfu) and Mg in the range of Fig. 4 Examples of typical profiles through garnets from samples 124 (high-Al mica schist of Revdalen Formation, zone 4, diameter = 1.7 mm), 125 (low-Al mica schist of the Revdalen Formation; diameter = 1.5 mm), 206 (high-Al mica schist of the Revdalen Formation, zone 2, diameter = 1.3 mm), 214 (low Al mica schist of the Skoddefjellet Formation, diameter = 1 mm), showing the differences in garnet zoning between high-Al Revdalen Formation, low-Al Revdalen Formation and low-Al Skoddefjellet Formation mica schists, as well as within zones 2 and 4 in the Revdalen Formation. Neoproterozoic metamorphism in southern Svalbard J. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd256 0.21–0.29 apfu. The Fe/(Fe + Mg) ratio is in the range 0.85–0.88 (Table 1). Biotite Biotite contains VIAl in the range of 0.653–0.86 apfu and Fe/(Fe + Mg) in the range of 0.57–0.697 (Table 2). Ti content in the biotites scatters in the range of 0.085– 0.295 apfu, which is characteristic for biotites from mesozonal rocks of Barrovian facies series (Henry et al. 2005). Only biotites occurring in foliation planes in the vicinity of garnets were used for further geothermobaro- metric calculations, except sample 124, where we used matrix biotite not in contact with garnet. Plagioclase Plagioclase crystals differ from each other, depending on their position in the fabric of the mica schists. Plagioclase grains in contact with garnet or partially replacing it have an anorthite content in the range of 0.1–0.17. Plagioclase grains from the matrix are characterized by a relatively lower level of anorthite molecules of 0.09–0.12 (Table 1). These porphyroblasts probably crystallized near the maximum pressure conditions during the D1 deforma- tion. Plagioclase grains characterized by the higher level of anorthite molecules presumably formed early during the first stage of decompression, after the pressure asso- ciated with the peak of metamorphism, but still under increasing temperature. The lower An plagioclases, located in the matrix, were used for further geobaro- metrical calculations. Pressure–temperature estimates Metamorphic zones The petrography and mineral chemistry of the Isbjørn- hamna Group described above point to regional amphibolite facies metamorphism. The observed mineral parageneses in the metapelites are grouped into four metamorphic zones: zone 1, with Cld + Chl + Grt paragenesis in high-Al mica schists, and Chl + Bt + Grt paragenesis in low-Al mica schists; zone 2, with Fig. 5 Sample locations with the temperatures obtained and boundaries of mineral zones within the Isbjørnhamna Group. Neoproterozoic metamorphism in southern SvalbardJ. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd 257 Table 1 Chemical composition of plagioclases used for garnet–Al silicate–plagioclase (GASP) geobarometry (with obtained pressures) and chemical composition of staurolites from the Isbjørnhamna Group metapelites. Pl Sample St Sample 124-1 124-2 124-3 218-1 218A-2 204-core 204-rim 206-core 206-rim SiO2 64.853 66.114 65.742 64.918 65.944 SiO2 27.815 27.827 27.544 27.473 Al2O3 22.478 21.669 21.677 21.950 21.393 TiO2 0.428 0.596 0.509 0.638 CaO 3.114 2.095 2.306 3.325 2.513 Al2O3 53.190 54.364 53.379 53.274 FeO 0.098 0.074 0.059 0.456 0.031 MgO 1.391 1.208 1.112 0.988 BaO 0.000 0.000 0.072 na na CaO 0.006 0.024 0.000 0.000 Na2O 10.167 10.422 10.181 9.735 10.198 MnO 0.070 0.038 0.037 0.030 K2O 0.022 0.000 0.031 0.039 0.007 FeO 14.839 13.934 13.478 13.227 Total 100.733 100.374 100.068 100.423 100.086 ZnO 0.034 0.033 0.202 0.286 H2O 2.149 2.167 2.129 2.123 Si 2.839 2.891 2.886 2.853 2.894 Total 99.922 100.191 98.390 98.039 Al 1.160 1.117 1.122 1.137 1.106 Ca 0.146 0.098 0.108 0.157 0.118 Si 3.880 3.851 3.879 3.880 Fe 0.004 0.003 0.002 0.017 0.001 Ti 0.045 0.062 0.054 0.068 Ba 0.000 0.000 0.001 na na Al 8.745 8.867 8.859 8.867 Na 0.863 0.884 0.867 0.829 0.868 Mg 0.289 0.249 0.233 0.208 K 0.001 0.000 0.002 0.002 0.000 Ca 0.001 0.004 0.000 0.000 Total 5.013 4.992 4.988 4.995 4.987 Mn 0.008 0.005 0.004 0.004 Fe 1.731 1.613 1.587 1.562 Ab 85.420 90.000 88.610 83.907 88.032 Zn 0.004 0.003 0.021 0.030 An 14.460 10.000 11.090 15.891 11.968 Total 14.703 14.654 14.637 14.619 Or 0.120 0.000 0.180 0.202 0.000 Cs 0.120 0.000 0.180 — — Fe/(Fe+Mg) 0.857 0.866 0.872 0.882 P(kbar) 9.84 11.22 11.29 6.60 8.77 Derived 2s errors of ca. 0.8 kbar for geobarometry (Holdaway 2000, 2001) have been used. Table 2 Chemical composition of garnets and biotites used for geothermometry and obtained temperatures. Sample Grt Bt Py Alm Grs Sps Fe/(Fe + Mg) Fe/(Fe + Mg) Ti Temp. 103 9.685 77.446 11.045 1.824 0.889 0.578 0.235 604 104 8.337 79.280 11.623 0.759 0.905 0.579 0.190 574 106 4.887 67.799 19.082 8.233 0.933 0.613 0.194 542 111 9.490 75.572 11.779 3.158 0.888 0.614 0.085 675 119 9.312 74.120 14.692 1.876 0.888 0.640 0.182 668 123 8.521 76.359 11.180 3.940 0.900 0.634 0.231 631 124 8.830 81.673 6.581 2.916 0.902 0.594 0.222 655 125 6.010 71.476 19.426 3.088 0.922 0.655 0.282 597 126 7.536 70.953 16.620 4.891 0.904 0.618 0.143 616 203 6.679 66.571 22.196 4.554 0.909 0.517 0.173 553 204 8.033 84.134 5.774 2.059 0.913 0.583 0.158 580 206 7.402 89.433 1.945 1.220 0.924 0.576 0.203 519 208 8.672 67.678 20.397 3.252 0.886 0.627 0.169 671 211 6.166 71.925 17.383 4.526 0.921 0.657 0.178 648 214 10.195 74.263 13.343 2.199 0.879 0.623 0.232 667 216 10.090 80.443 6.284 3.183 0.889 0.572 0.192 596 217 10.376 82.923 3.292 3.409 0.889 0.627 0.209 642 218 13.610 80.204 4.727 1.458 0.855 0.582 0.185 624 219 8.218 71.436 20.230 0.116 0.897 0.572 0.137 634 220 7.867 72.259 9.391 10.484 0.902 0.637 0.234 633 221 6.559 76.095 16.880 0.466 0.921 0.626 0.148 574 222 8.337 79.280 11.623 0.759 0.905 0.579 0.190 661 Derived 2s errors of ca. 25°C for geothermometry (Holdaway 2000, 2001) have been used. Neoproterozoic metamorphism in southern Svalbard J. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd258 Chl + Grt + St � Bt paragenesis in high-Al mica schists, and Grt + Chl + Bt paragenesis in low-Al mica schists; zone 3, with Grt + St + Bt + Ky � Chl assemblage in high-Al mica schists and Grt + Bt + St � Chl in low-Al mica schists; zone 4, with Grt + Ky + Bt in high-Al mica schists and Grt + Bt in low-Al mica schists. Metamorphic isograds are defined on the first occur- rence of the AFM mineral. The boundary between zones 1 and 2 was delineated by the first appearance of stauro- lite. The mineral assemblage for zone 2 was recognized only in one sample of high-Al mica schists, and thus the boundary between zones 1 and 2 is speculative. The boundary between zones 2 and 3 is defined by the broad appearance of biotite and staurolite and between zones 3 and 4 by the disappearance of staurolite. The observed parageneses and metamorphic zones suggest a sequence of index mineral reactions characteristic of continuously increasing pressure–temperature (P–T) conditions from upper greenschist to middle/upper amphibolite facies conditions at moderate to high pressure. Metamorphic zoning without a chloritoid + biotite assemblage is well recognized in several kyanite-bearing metamorphic com- plexes (e.g., Spear 1993; Bucher and Frey 1994). Geothermobarometry We used the garnet–Al silicate–plagioclase (GASP) geoba- rometer (Holdaway 2001) to quantitatively estimate the peak pressure conditions. The pressure was calculated only in samples containing an Al2SiO5 polymorph (kyanite in this case). Only five plagioclase–garnet pairs were analysed in both samples, mainly because of strong retrogressive changes. Those analysed, however, were not affected by strong retrogression. The results obtained are in the range of 9.84–11.3 kbar for sample 124, and 6.6–8.77 kbar for sample 218 (see Table 2 and Fig. 5 for the location of samples), and are relatively consistent with pargeneses observed in the investigated samples. For peak temperature estimation, the garnet–biotite geothermometer (Holdaway et al. 1997; Holdaway 2000) was used. The temperatures were calculated for a norma- tive pressure of 9 kbar on the basis of mineral paragenesis and previous preliminary pressure estimates (Majka 2003; Majka et al. 2004). The lowest Fe/(Fe + Mg) values (usually rim) were used for further geothermometrical calculations. The calculated temperatures are scattered in the range of 530–675°C (Fig. 5; Table 2). The general tendency observed in the Isbjørnhamna Group is that calculated temperatures increase from 519 to 604°C in the Rålstranada area (samples 103, 104, 106 and 203), and from 624 to 675°C in the upper Revdalen area (samples 119, 123, 124, 208, 217 and 218), which appears in the core of the Ariebreen anticline (samples 111, 211 and 214). Slightly lower temperatures (596– 634°C) were recorded for the samples collected from the south and south-east limb of the Ariebreen anticline (samples 216, 219 and 220). Similarly, for the samples from the Fuglebereget–Vesletuva area (samples 125, 126, 221 and 222), temperatures in the range of 574–628°C were obtained. Comparison of geothermobarometrical results and KFMASH petrogenetic grid The K2O–FeO–MgO–Al2O3–SiO2–H2O (KFMASH) petro- genetic grid (Spear & Cheney 1989) was used to better constrain the P–T path based on our geothermobaromet- ric results. Only the samples from the Revdalen Formation, showing well-developed metamorphic zona- tion, were used. Observed mineral prageneses of high-Al mica schists can be represented by the KFMASH system. The Fe/(Fe + Mg) ratios in analysed minerals decreases in the order garnet > staurolite > biotite, similar to many metapelites from all over the world (e.g., Thompson 1976; Spear 1993). Therefore, we decided to ignore the minor components MnO, Na2O, TiO2 and CaO while choosing the petrogenetic grid. The paragenetic mineral assemblage in samples with the lowest metamorphic grade in the Revdalen Formation, which crop out in the Russepynten cape area, indicates that these rocks were metamorphosed above the chloritoid and garnet isograds. The lack of biotite in this mica schist variety does not mean that these rocks were formed below the biotite isograd. In accordance with the KFMASH system, the co-existence of chloritoid, chlorite and garnet in the paragenesis means that chloritoid-bearing mica schists could have been formed in the temperature range of 450–520°C. Only above the temperature of ca. 520°C is chlorite replaced by the garnet–biotite assemblage. Simi- larly, chloritoid can be unstable, but in very specific cases it is stable up to 550°C (Bucher & Frey 1994). More eastwards but still in the Rålstranda and Torbjørnsenfjellelt areas the index mineral assemblage changes into Grt + Bt + Chl, Grt + St � Bt � Chl and Grt + Bt + St � Chl. Such a change means an increase in temperature above 520°C for samples without staurolite, and a further increase in temperature above 550°C in rocks containing staurolite. The stability of the latter paragenesis is restricted much more by pressure than by temperature. Generally, the maximum temperature of staurolite stability decreases with an increase in pressure. The obtained temperature of 580°C for sample 204 prob- ably corresponds to a pressure of 8–9 kbar. Further east in the upper Revdalen Valley region, stau- rolite disappears from the paragenesis, and is replaced by kyanite. This paragenetic mineral assemblage is stable Neoproterozoic metamorphism in southern SvalbardJ. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd 259 above a temperature of 630°C at 11 kbar. The results from geothermobarometry are consistent (sample 124) at ca. 646°C and a maximum pressure of ca. 11 kbar. Addition- ally, the probable homogenization of garnet from this sample suggests that the rock was metamorphosed under relatively high-grade conditions. Rocks from the north-eastern part of the study area contain both kyanite and staurolite. This mineral assem- blage is stable in a relatively small P–T field at temperatures of ca. 640–680°C and pressures of ca. 9–10 kbar. The geothermobarometrical results for this variety of the Revdalen mica schists yielded a tempera- ture of ca. 628°C and pressures of 6.6–8.77 kbar. The 628°C temperature is fairly consistent with the stability field of the Grt + Bt + St + Ky paragenesis, and the pres- sure is within error of the expected pressure field. In the remaining two samples (217 and 125), no Al-saturated phases were observed, as expected for the low bulk Al content in these rocks. Nevertheless, the temperatures of 636°C for sample 217 and 597°C for sample 125 are reasonable. Sample 217 was collected not far away from samples 218 and 124, and a similar tem- perature estimation therefore seems likely. Sample 125 comes from the area at the south-eastern extremity of the Revdalen Formation, and the temperature obtained is comparable with that calculated for sample 126 (Fig. 5). As the transformation of kyanite into sillimanite or andalusite is not documented in the studied rocks, cooling possibly took place within the kyanite stability field. Accordingly, the retrograde part of the P–T path obtained for the Revdalen mica schists does not cross the boundaries of sillimanite and andalusite stability fields (Fig. 6). Cooling rate Using previous geochronological data (Manecki et al. 1998; Majka et al. 2008) and thermometrical results pre- sented in this paper, it is possible to reconstruct the cooling history of the Isbjørnhamna Group. Manecki et al. (1998) reported 585–575 My 40Ar–39Ar cooling ages for muscovite from the Isbjørnhamna Group and a 616 My 40Ar–39Ar cooling age for hornblende from the overlying Eimfjellet Group. The closing temperatures for muscovite and hornblende are ca. 350°C and ca. 550°C, respectively. Majka et al. (2008) obtained a 643 My U–Th–total Pb age for monazites located both in the matrix of mica schists and enclosed in garnet porphyro- Fig. 6 K2O–FeO–MgO–Al2O3–SiO2–H2O (KFMASH) petrogenetic grid (modified from Spear & Cheney 1989; Spear & Cheney unpubl. data) with the pressure–temperature (P–T) path marked for the Isbjørnhamna Group rocks. Neoproterozoic metamorphism in southern Svalbard J. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd260 blasts, constraining the growth of garnet in the Isbjørnhamna Group at 643 Mya. From the data men- tioned above and with three points on the age– temperature diagram, we construct a nominal cooling path for the Neoproterozoic metamorphic volcanic terrane (Fig. 7). The generally smooth shape of the cooling path suggests a cooling rate of ca. 5°C My-1. Such a cooling rate corresponds well with those reported from the Neoproterozoic Pan-African orogens (e.g., Möller et al. 2000). On average, cooling rates increase through geological time, and are an order of magnitude faster in Phanerozoic than in Precambrian settings (Dunlap 2000). Despite the unavoidable simplifications, the compilation of temperature–time (T–t) paths by Willigers et al. (2002) shows that a cooling rate around 5°C My-1 is typical of Neoproterozoic orogens. Two possible forms of the T–t path for the Isbjørnhamna Group are proposed (Fig. 7). One assumes a moderate reheating at ca. 480 Mya, the approximate time of metamorphism in the northern tec- tonic block of Wedel Jarlberg Land (Mazur et al. 2009). The other postulates a decrease of the cooling rate from 575 Mya onwards. Further thermochronological studies are necessary to differentiate between these two possibilities. Concluding remarks The Revdalen Formation is a <200 m thick continuous horizon that provides an excellent marker for investigating lateral changes in P–T metamorphic conditions. On the basis of the metamorphic mineral zonation and P–T estimates, an increase of P–T conditions from west (Rålstranda area) to east (Revdalen Valley area) is observed. Only the slight south-eastward temperature decrease in the Fugleberget area departs from this general trend. Taking into account the thermometric results from the Skoddefjellet mica schists, a similar trend in temperature change can be extrapolated for the entire Isbjørnhamna Group. Maximum temperatures were obtained from the core of the Ariebreen anticline, whereas the calculated temperatures continuously decrease toward the limbs of this antiform and the western part of the study area. This relationship indicates that large-scale folding of the Isbjørnhamna Group occurred after the peak of meta- morphism. Because the folds are crosscut by the VKZ, displacement along this shear zone must have been even later. Indeed, the isograds defined for the Revdalen For- mation are oblique to the trend of the VKZ. In summary, the peak temperature and pressure conditions of Neopro- terozoic metamorphism are estimated at ca. 670°C and �11 kbar. The geothermobarometric results are consistent with previous preliminary estimates of the P–T rock- forming conditions (Smulikowski 1965; Czerny et al. 1993; Majka et al. 2004). The microstructural observations show that the perva- sive fabric of the Isbjørnhamna rocks formed under conditions close to the peak of metamorphism. As the constructed isograds are oblique to the foliation and litho- logical contacts, the penetrative deformation must have slightly preceded the peak temperature. The latter was followed by the folding of already developed foliation before the initiation of the VKZ. Considering that the VKZ was developed in the Early Ordovician (Mazur et al. 2009), the structural grain of the Isbjørnhamna Group and the entire southern tectonic block of Wedel Jarlsberg Land must have been formed in Neoproterozoic to Cambrian times. The T–t path of the Isbjørnhamna Group shows cooling at a rate of ca. 5°C My-1, interpreted to be related to slow erosion controlled exhumation, rather than rapid uplift connected to tectonic activity. Notably, cooling continued undisturbed at least until the Early Ordovician, the time of postulated juxtaposition of the Neoproterozoic complex against the northern part of Svalbard’s south- western terrane. Our data confirm that the southern tectonic block of Wedel Jarlsberg Land represents a fragment of a Neopro- terozoic orogen, with a well-preserved structural grain and metamorphic zonation. This Neoproterozoic domain seems to be entirely exotic compared with Svalbard’s remaining terranes, and is only weakly overprinted by Caledonian metamorphism. The Neoproterozoic terrane could not have been derived from the North American margin, as postulated for the rest of Svalbard’s crustal Fig. 7 Hypothetical cooling paths for the Isbjørnhamna Group, based on data published by Manecki et al. (1998), Majka et al. (2008) and this paper. Path 1 assumes moderate reheating at ca. 480 Mya, whereas path 2 pos- tulates a decrease in the cooling rate from 575 Mya onwards. Neoproterozoic metamorphism in southern SvalbardJ. Majka et al. Polar Research 29 2010 250–264 © 2010 the authors, journal compilation © 2010 Blackwell Publishing Ltd 261 fragments (Gee & Tebenkov 2004). Instead, its presence is more in line with models suggesting large-scale strike-slip displacements during the Early Palaeozoic assembly of the Svalbard Archipelago (e.g., Harland & Gayer 1972; Harland 1985; Gee & Page 1994). The most straightfor- ward explanation for the origin of the Neoproterozoic terrane is a derivation from the Timanide belt of north- eastern Europe. However, such a correlation has two important implications that require further verifica- tion and discussion. Firstly, the Neoproterozoic orogeny must have commenced at least before the opening of the Iapetus Ocean, as the Svalbard Archipelago is separated from Europe by Caledonian sutures (Gee & Tebenkov 2004). Secondly, the linkage between south- western Svalbard and the Timanide belt cannot be recon- ciled with the large-scale Early Palaeozoic rotation of Baltica that has been postulated by Hartz & Torsvik (2002). Ongoing studies characterizing the metamorphic, structural and magmatic histories of Neoproterozoic circum-Arctic terranes are necessary in order to better constrain Neoproterozoic paleogeographic reconstruc- tions and the proposed younger tectonic evolution models for the region (Amato et al. 2009). Acknowledgements This research was supported by MNiSzW grant no. 2P04D03930. JM was also supported by the Swedish Institute, Visby Programme and Ymer-80 Foundation. We are grateful to two anonymous reviewers for their con- structive comments improving the manuscript, and to L. 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