JOURNAL OF PETROLOGY Journal of Petrology, 2015, Vol. 56, No. 2, 299–324 doi: 10.1093/petrology/egv001 Advance Access Publication Date: 11 February 2015 Original Article Halogen Element and Stable Chlorine Isotope Fractionation Caused by Fluid–Rock Interaction (Bamble Sector, SE Norway) Christof Kusebauch1*, Timm John1,2, Jaime D. Barnes3, Andreas Klügel4 and Håkon O. Austrheim5 1 Institut für Mineralogie, Westfälische Wilhelms-Universität Münster, Corrensstr. 24, D-48149 Münster, Germany, Institut für Geologische Wissenschaften, Freie Universität Berlin, Berlin 12249, Germany, 3Jackson School of Geoscience, University of Texas, Austin, TX 78759, USA, 4FB-Geowissenschaften, University of Bremen, Bremen 28359, Germany and 5Department of Geoscience, University of Oslo, Oslo 0316, Norway 2 *Corresponding author. Telephone: þ49 251 83 33506. Fax: þ49 251 83 38397. E-mail: [email protected] Received December 3, 2013; Accepted January 2, 2015 ABSTRACT Pervasive interaction between rock and fluid produces regional-scale alteration and/or metasomatism of rock units. The middle and upper crustal rocks from the Bamble sector (SE Norway) show a complex history of metamorphic and metasomatic events, accompanied by ore deposit formation, which provides an excellent context for investigation of regional-scale fluid–rock interaction. Halogens are important agents of rock alteration and ore metal transportation in such hydrothermal regimes. Here we use F, Cl, Br and I concentrations and stable chlorine isotope ratios (d37Cl) to trace the metasomatic evolution of two gabbroic bodies and understand the interplay between localized and pervasive fluid flow in the upper crust. An alteration sequence was sampled from pristine gabbro to an amphibolitic shear zone, showing progressive amphibolitization and scapolitization caused by pervasive fluid ingress. Halogen concentrations and ratios suggest the evolution of a single fluid, causing enrichment of Cl, Br and I in samples nearest the shear zone. Owing to the differences in fluid–mineral distribution coefficients, fluid–mineral interaction resulted in either enrichment or depletion of halogens in the fluid as it reacted pervasively with the gabbro. Although scapolite formation leads to progressive desalination of the fluid near the shear zone, increasing Cl concentrations in amphibole near the gabbro reflect an increase in salinity towards the unaltered gabbro owing to desiccation of the fluid. The formation of alteration minerals mainly governs changes in the halogen chemistry of the fluid, showing that halogens do not behave fully conservatively during fluid–rock interaction. Nevertheless, the evolving fluid has a feedback on the stability of alteration minerals such as scapolite and biotite, which form only close to the shear zone. The Br/Cl and I/Cl ratios of the most highly altered samples are 3 10–3 and 25 10–6, respectively, and overlap with the range of ratios measured for marine pore fluids. Remobilization of evaporites would have produced distinctly lower halogen ratios and can be ruled out as a fluid source. The unaltered gabbro has d37Cl values near 0% and a similar value is inferred for the infiltrating fluid. Minimally altered samples, noted by the presence of <20 vol. % amphibole, have negative d37Cl values (average ¼ –06 6 01%). The d37Cl values increase (up to þ 1% nearest the shear zone) with increasing evidence of fluid–rock interaction towards the shear zone. Mixing of different Cl reservoirs (i.e. gabbro and fluid) cannot explain the observed changes in the d37Cl values. Instead, isotopic fractionation owing to Rayleigh distillation with a fractionation factor of 10010 can explain the observed negative d37Cl values of the alteration sequence by the evolution of a single fluid during fluid–rock interaction. An additional kinetic component during fractionation may have C The Author 2015. Published by Oxford University Press. All rights reserved. For Permissions, please e-mail: [email protected] V 299 300 Journal of Petrology, 2015, Vol. 56, No. 2 enhanced the observed changes in chlorine isotope values. We speculate that these processes are the reason for the large spread of d37Cl values found in many stable Cl studies for single reservoirs. Key words: Bamble sector; Cl isotopes; fluid evolution; halogen ratios; Rayleigh fractionation INTRODUCTION Fluid–rock interaction causes element mobilization and in some cases fractionation of their isotopes. Fluid–rock interaction is further responsible for the formation of economic mineral deposits and has consequences for the petrophysical properties of the affected rocks and the geodynamics of the related large-scale systems. Mass transport is most efficient in channelized flow systems, where fluid flow controls not only the redistribution but also the quantities of the elements (WilliamsJones & Heinrich, 2005; Zack & John, 2007; Ague, 2011; Richards, 2011; Williams-Jones et al., 2012). Mobilization of economically valuable elements (usually occurring in trace amounts in rocks), as well as regional-scale alteration or metasomatism of rock units, also requires pervasive interaction between rock and fluid. Field evidence suggests that fluid–rock interaction in various geodynamic settings may occur pervasively on regional scales, but is in fact locally concentrated along and adjacent to veins and shear zones (Austrheim, 1987; Bach & Frueh-Green, 2010; Engvik et al., 2011; John et al., 2012). It is thus of importance to understand how fluid–rock interaction occurs with respect to flux of fluid, number of fluid flow events and potential sources of fluid. Chemical tracers (e.g. halogens) and fluid-composition indicative minerals (e.g. amphibole, biotite, apatite) help to better understand fluid flow patterns and reaction front propagation leading to the formation of alteration minerals. Furthermore, they provide information about fluid pulses and their origins. Halogens (F, Cl, Br, I) can be used to characterize these fluids as they are major anions in metasomatic fluids, but only minor or trace elements in the bulk solid (e.g. Kullerud, 1996; Kullerud & Erambert, 1999; Markl & Bucher, 1998; Svensen et al., 1999; John et al., 2011). Therefore, halogen concentrations and ratios in mineral phases that formed during fluid–rock interaction reflect fluid characteristics, rather than features inherited from the pristine solid. The strongly different ionic radii of halogens (F < Cl < Br < I) lead to different partitioning between minerals and fluid. As F– and Cl– are relatively small, they are capable of replacing OH– in hydrous minerals (e.g. biotite, amphibole, apatite). In contrast, I– and Br– are larger in size and are less compatible in silicate minerals. Halogen ratios are characteristic of different halogen reservoirs such as pore fluids, evaporites, mantle fluids and sedimentary fluids (e.g. John et al., 2011; Kendrick et al., 2011) and can be used to trace the source of the metasomatic fluids derived from these reservoirs. Owing to the different partitioning behaviour of halogens, their ratios (e.g. Br/Cl, I/Cl) are potentially a powerful tool to investigate fluid–rock reactions. Chlorine isotopes provide another means to trace fluid–rock interactions. As Cl concentrations in fluids are relatively high compared with those in silicates, a recorded isotopic signal probably reflects fluid source characteristics rather than inherited silicate characteristics. Chlorine isotope compositions, given in standard d notation, where d37Cl ¼ {[(37Cl/35Cl)sample – (37Cl/35Cl)SMOC]/(37Cl/35Cl)SMOC} 1000 and SMOC is Standard Mean Ocean Chloride, for most geologically relevant reservoirs vary between –8 and þ3% (e.g. Barnes & Sharp, 2006; John et al., 2010; Sharp et al., 2013, and references therein). The limited range and overlapping values for different rock reservoirs hinders the application of Cl isotopes as a source tracer for unaltered rock. Fractionation of Cl isotopes occurs mainly during fluid–rock interaction (e.g. Eggenkamp et al., 1995; Markl et al., 1997; Gleeson & Smith, 2009; Amundson et al., 2012; Barnes & Cisneros, 2012; Selverstone & Sharp, 2013) and is indicated by hydrothermally altered rocks. Accordingly, changing Cl isotope ratios within one suite of altered rocks reflect changes in the fluid. The Bamble sector (SE Norway) is a well-studied high-grade metamorphic terrane (Bingen et al., 2005), which experienced metasomatic alteration during the Sveconorwegian orogeny (c. 1090–1040 Ma) (e.g. Engvik et al., 2011). Extensive fluid infiltration during this event led to several mineral replacement reactions (Nijland & Touret, 2001; Harlov et al., 2002; Engvik et al., 2008, 2009; Engvik & Austrheim, 2010), almost all occurring in intrusive and metamorphic rocks to an extent that the mineral assemblage of the protolith cannot be identified. Metasomatism is linked to the formation of several iron-oxide and phosphate ore deposits in the region (Nijland et al., 1998b, and references therein). Gabbros of early Sveconorwegian age are affected by this fluid infiltration and exhibit various metasomatic features. These include a penetrative amphibolitization adjacent to shear zones, a scapolitization event altering pristine plagioclase to scapolite, and an albitization reaction front replacing plagioclase and scapolite with albite (Nijland et al., 1998a; Engvik et al., 2008, 2011). The later alteration also shows formation of prehnite, pumpellyite and analcime, indicating a possible lowgrade metamorphism of unknown age. Although the size of the alteration zones varies from centimetres to tens of metres in different outcrops, the related reaction sequences are always the same (Engvik et al., 2011). Although the metamorphic history of this high-grade terrane is largely understood (Bingen et al., 2008b), the Journal of Petrology, 2015, Vol. 56, No. 2 impact of metasomatism on the related metamorphic reactions is still poorly constrained. Here, we use halogen concentrations, ratios and chlorine isotope ratios to investigate the fluid history of the Bamble sector. We focus on the origin and evolution of the fluids causing the major alteration (i.e. amphibolitization and scapolitization) observed in gabbroic bodies. Furthermore, possible mechanisms leading to fractionation of chlorine isotopes are discussed and implications formulated. GEOLOGICAL SETTING The Bamble sector (SW Norway), part of the Precambrian basement of southern Norway, consists of amphibolite- to granulite-facies metamorphosed rocks. Together with the Kongsberg sector, which shows similar lithologies, the Bamble sector (Fig. 1a) is interpreted as the collision zone between the Telemarkia terrane (western Norway) and the Iddefjorden terrane (eastern Sweden) (Bingen et al., 2005, 2008b). Most lithologies in the Bamble sector are ortho- and paragneisses formed during the Sveconorwegian orogeny (Fig. 1b). The oldest orthogneisses of the sector formed between 157 and 152 Ga. Embedded in the SW–NE-striking metasedimentary rocks are gabbro-tonalitic and charnockitic rocks intruded between 1200 and 1150 Ma (Ransom et al., 1995). Granulite-facies rocks have been dated at 1150–1125 Ma by monazite U–Pb dating (Cosca et al., 1998; Bingen et al., 2008a). Estimated peak metamorphic conditions are 07 GPa and 800 C, inferred from garnet–pyroxene thermobarometry (Harlov, 2000). A younger amphibolite-facies overprint (1105–1080 Ma) is observed in many metapelites and amphibolites (Cosca et al., 1998). High fluid flux events metasomatized most metamorphic and intrusive rocks during the late Sveconorwegian (1090–1040 Ma) (Engvik et al., 2011). Scapolitization and albitization are widespread alteration features in many lithologies (Nijland et al., 1998b). Notably, gabbroic bodies display two or more distinguishable alteration fronts (Engvik et al., 2011). Scapolitization is observed in many gabbroic bodies and occurs as reaction fronts starting from shear zones and veins. Pristine gabbro in these altered bodies exists as lenses between shear zone networks. Temperature and pressure conditions for the scapolitization of the Bamble sector are estimated to be 600–700 C and 02–04 GPa (Nijland & Touret, 2001; Engvik et al., 2011). Rb–Sr ages, determined from phlogopite, date the scapolitization at 1040–1068 Ma and therefore at a late stage of the Sveconorwegian orogenesis (Engvik et al., 2011). Albitites occur as larger bodies (3 km length, 100–300 m thickness) in mafic and felsic rocks (Engvik et al., 2008) on a regional scale. The albitites occur as products of metasomatism and are formed as alteration rims along cracks or as penetrating veins in host-rocks. Areas with a high density of veins underwent almost complete albitization, and only minor remnants of the 301 host-rock can be found (Engvik et al., 2008). Nijland & Touret (2001) estimated the temperature for the albitization in the Bamble area to be at 350–450 C. Assemblages of prehnite, pumpellyite and analcime found coexisting with the albite suggest even lower temperatures for the last alteration event. Although no age data for the albitization in the Bamble sector are available, a Sveconorwegian age can be assumed as albitization in the Modum complex of the Kongsberg terrane (also SE Norway), which has a similar metamorphic history, has an age of 1080 Ma based on U–Pb chronology (Munz et al., 1994). Fluid inclusions from granulite-facies rocks are usually CO2 rich, whereas inclusions from amphibolitefacies rocks show a more aqueous or saline (from 30 wt % NaCl to halite saturation) composition (Hoefs & Touret, 1975; Touret, 1985). Both CO2 and NaCl strongly influence the water activity of the fluid as well as the stabilities of coexisting minerals indicative of metamorphic facies, which is of importance as changes in the fluid composition lead to changes in the mineral assemblage of metamorphic rocks. The Bamble sector contains several important ironore and apatite deposits that were mined in past centuries (Nijland et al., 1998b) and are interpreted to originate from hydrothermal interaction of host-rocks with metasomatic fluids. FIELD RELATIONS AND SAMPLE DESCRIPTION Fluid flow in the Bamble area reveals both a pervasive and a channelized pattern depending on the scale of observation. Herein, the term pervasive is used to describe a penetrative fluid flow causing alteration (fully or partly) in a rock volume of interest. The distinction between pervasive and channelized fluid flow is not necessarily mutually exclusive, as fluid flow that looks pervasive on a large scale can be channelized on a smaller scale. Fluid flow in the Bamble area appears pervasive on a regional scale (100 km by 20 km) as hydrothermal alteration affects almost every rock type. On the outcrop scale (10–1000 m) the fluid flow pattern becomes a fluid network with a high density of shear zones and veins of variable size in which fluid flow is localized. On a decimetre to centimetre scale these localized fluids pervasively infiltrate the host-rock and cause alteration starting at the wall-rock next to the main fluid pathways (Fig. 2a–c). On a microscopic scale, no filled veins but rather fractures providing possible pathways for the infiltrating fluid are observed. Additionally, pervasive fluid flow along grain boundaries is inferred from altered phases that are not connected to fractures. To understand the interplay between localized (in shear zones) and pervasive fluid flow (decimetre to centimetre scale) in the Bamble area, two different metagabbros were sampled. The Valberg metagabbro is located 2 km north of Kragerø and is 15 km in diameter (Fig. 1b). The complex consists mainly of altered gabbro containing shear 302 Journal of Petrology, 2015, Vol. 56, No. 2 Fig. 1. (a) Regional map showing the location of the Bamble area (B); (b) geological map of the northeastern part of the Bamble area showing the sample sites (stars) near Kragerø (Valberg) and at the shore of Langøy [from Norwegian Geological Survey (NGU) databases]. zones and veins that range from centimetres to metres in thickness. Lenses of pristine olivine–orthopyroxene–clinopyroxene gabbro vary from 05 to 30 m in length and thickness (Fig. 2a and b). The primary gabbro is pervasively altered from the shear zones towards the centre of the lenses. Metre-thick veins and shear zones consist of coarse-grained albite and amphibole, whereas smaller veins mainly consist of pargasitic amphibole. An alteration sequence was sampled from the Valberg metagabbro consisting of five samples showing different alteration stages (pristine gabbro, amphibolitized gabbro, scapolitized gabbro, shear zone) according to their distance from the shear zone (Fig. 2b). The Langøy metagabbro is exposed over >1 km2 along the coastline. Similar to the Valberg metagabbro, the protolith gabbro at Langøy was continuously amphibolitized and scapolitized, with the highest alteration always adjacent to shear zones and veins. Compared with Valberg, the Langøy samples show a lesser extent of deformation and are highly localized in shear zones. Larger veins and shear zones contain almost monomineralic amphibolite, whereas smaller veins are usually filled with scapolite. To investigate the alteration sequence of the Langøy metagabbro in detail, a 30 cm 20 cm 10 cm sized block was sampled (Fig. 2c). The block shows an alteration sequence, including scapolitization and amphibolitization, with an increasing degree of alteration towards the shear zone. To gain information on small-scale changes within the alteration sequence, the block was first sliced perpendicular to the shear zone to prepare thin sections. Afterwards the block was sliced into 15 pieces (plus one pristine gabbro sample for comparison) of 15–2 cm thickness parallel to the shear zone for whole-rock and mineral separates analyses. ANALYTICAL METHODS Halogen extraction Sliced rock samples were washed in ultra-pure water (18 MX), then dried and crushed with a hardened steel hammer. One aliquot of crushed rock sample was Journal of Petrology, 2015, Vol. 56, No. 2 303 Fig. 2. Field relations and location of sample specimens: (a) metre-sized blocks of unaltered gabbro (in grey) surrounded by ‘augen’-like shear-zone structures and an albitic vein (grey lines), Valberg; (b) metre-sized block of unaltered gabbro (grey) with increasing alteration towards amphibolitic shear zones; circles indicate sample positions in the Valberg outcrop; (c) block (27 cm in length) of metagabbro from the second sampling location on the island of Langøy containing the whole alteration sequence including amphibolitization, scapolitization and the amphibolitic shear zone; (d) thin sections of the complete alteration sequence of Langøy sample (c) showing an increasing amount of amphibole (green) and biotite (brown) with decreasing distance to the amphibolitic shear zone (right side); (e) Langøy sample: modal abundances of major minerals according to their distance from the shear zone shown in (d) [with zero being the boundary between wall-rock and shear zone; values on the right side of zero belong to the shear zone, and those to the left side to the altered wall-rock; pristine gabbro (PG) as reference]. powdered using an agate mortar. Another aliquot of each rock sample was washed again in ultra-pure water, dried and split into different sized portions by sieving. After magnetic separation, amphibole, biotite and scapolite were handpicked from sieve fraction 125–250 mm and pulverized using an agate mortar. Rock and mineral powders were washed five times in ultrapure water for 10 min and slowly dried at 60 C overnight. 304 Halogens were extracted using the pyrohydrolysis method described by Barnes & Sharp (2006), in which rock and/or mineral powders were melted in a continuous flow of ultra-pure water vapor. The water vapor, containing the released halogens, was condensed and collected in 005N NaOH and 0005N Na2SO3 solution (Schnetger & Muramatsu, 1996). The solution was split into aliquots for isotope and concentration analyses. Chlorine isotopes Chlorine isotope ratios were measured using the technique of Barnes & Sharp (2006) as modified from Eggenkamp et al. (1994). Extracted chlorine was converted to AgCl via reaction with an excess of AgNO3. AgCl was filtered from the sample solution, dried and reacted with CH3I under vacuum to produce CH3Cl. The gaseous CH3Cl was purified of excess CH3I on a gas chromatographic column and analysed using a ThermoElectron MAT253 isotope ratio mass spectrometer at the University of Texas in Austin. The long-term reproducibility for d37Cl values is 602%, based on the average of three internal seawater standards and an internal serpentinite rock standard. Halogen concentrations Halogen concentrations in the extraction solution were determined following the procedure described by John et al. (2011). Fluorine and Cl were analysed by ion chromatography (IC) (Metrohm 761 Compact IC system) at the University of Münster. Detection limits of F and Cl via ion chromatography were 100 ng ml–1 and 50 ng ml–1, respectively. Almost all sample solutions have F– concentrations slightly above or below the detection limit. Concentrations of Cl, Br and I were measured by inductively coupled plasma mass spectrometry (ICP-MS) using a ThermoFinnigan Element2 system at the University of Bremen equipped with a self-aspiring micro-flow nebulizer and a PEEK cyclonic spray chamber. To minimize memory effects, samples and blanks were prepared with a 5% NH4OH solution (p.a. quality), and a blank was analysed before each sample (see Bu et al., 2003). Extraction solutions were diluted 1:1 with NH4OH and spiked with 1 mg ml–1 Te as internal standard. The isotopes 35Cl, 79Br and 127I were analysed in medium resolution and 79Br additionally in high resolution; both 79Br determinations yielded essentially identical results. Calibration used five solutions with concentrations up to 10 ng ml–1 for Br and I and 1000 ng ml–1 for Cl. The lower limit of detection (3r) for the extraction solutions is 16 ng ml–1 for Cl, 04 ng ml–1 for Br and 006 ng ml–1 for I. Nine replicate analyses of a representative aliquot having Cl, Br and I concentrations of 3830, 75 and 07 ng ml–1, respectively, yielded a precision of 13–22%. Halogen concentrations in rock and mineral samples were calculated from the concentration of the extraction solutions. John et al. (2011) determined the Journal of Petrology, 2015, Vol. 56, No. 2 quantitative yield by multiple analysis of reference material (JB-2) following this method to be within 10% error. Electron microprobe analysis (EMPA) Quantitative analyses of mineral compositions were carried out using a JEOL 8900 electron microprobe at the University of Münster, equipped with four wavelength-dispersive spectrometers. Typical beam conditions were 20 kV acceleration voltage, a 15 nA beam current, a focused beam of 1 mm spot size and 5–10 s counting time on the peak. Natural as well as synthetic minerals were used for standardization of major elements. Standardization of halogens was done using natural tugtupite (for Cl) and fluorite (for F). X-ray diffraction (XRD) Abundances of phases were measured by powder XRD of bulk-rocks using a Phillips X’pert 9 diffractometer and X’pert ‘Highscore’ software package for quantification. Oxygen isotope measurements Amphibole mineral separates were prepared for oxygen isotope analysis by coarsely crushing 10 g of gabbro sample. The crushed material was then sieved, washed in deionized water and rinsed with HCl, and amphibole mineral grains were handpicked using a binocular microscope to ensure purity. Approximately 20 mg of separated amphibole was measured using the laser fluorination method of Sharp (1990). Samples were separately heated by a CO2 laser in the presence of BrF5 and then cryogenically purified using the silicate extraction line at the University of Texas at Austin. Once the O2 was purified, the d18O values were measured on a ThermoElectron MAT 253 gas source mass spectrometer. To check for precision and accuracy, garnet standard UWG-2 (d18O value ¼ þ58%) (Valley et al., 1995) and two in-house quartz standards, Lausanne-1 (d18O value ¼ þ181%) and Gee Whiz (d18O 18 value ¼ þ126%), were run. All d O values are reported relative to SMOW, where the d18O value of NBS-28 is þ965%. Precision is 601%. RESULTS Petrography and mineral chemistry Gabbro protolith The pristine gabbro consists mainly of plagioclase (pl with An60–70), orthopyroxene (opx with En70–75), clinopyroxene (cpx with Di65–70) and olivine (ol with Fo68–75). Apatite (ap) of heterogeneous composition (XCl ¼ 02–09, XOH ¼ 01–08, XF < 001) and ilmenite are minor phases. Olivine shows kelyphitic coronae of orthopyroxene locally intergrown with spinel that are in turn surrounded by a fine-grained amphibole–spinel corona (Fig. 3a). Coronitic and matrix opx are compositionally indistinguishable from each other. De Haas et al. (2002) interpreted opx coronae between pl and ol in gabbros from the Arendal area (SW Norway) to be of magmatic Journal of Petrology, 2015, Vol. 56, No. 2 305 Fig. 3. Back-scattered electron images and Si, Na and Cl element maps showing replacement reactions: (a) reaction rims between olivine and plagioclase in least altered parts of the sequence near the gabbro; (b) replacement of plagioclase by scapolite (6 spinel) indicating first scapolitization; (c) replacement of ilmenite by biotite leaving a corona of zircons, indicating the former grain shape of the ilmenite; (d) micrometre-sized halite crystal found in the least altered part of the sequence (26 cm distance to the shear zone). (super-solidus) origin. Amphibole–spinel coronae of the same assemblage are interpreted to originate from interaction of the opx coronae with late-stage magmatic fluids during cooling of the gabbro. Amphibole from the pristine gabbro has Cl concentrations of 02–04 wt % determined by EMPA (Supplementary Data) and is pargasitic in composition with high TiO2 (up to 2 wt %) and K2O (<06 wt %) concentrations. Pinkish plagioclase (An60–70) exists as millimetre-sized euhedral laths. The inner part of the sample contains the least altered metagabbro. Olivine is mostly replaced by pyroxene, but spinel can still be found as remnants of the gabbro assemblage as inclusions in pyroxene and amphibole. Opx and cpx have coronae of Cl-rich amphibole (Cl > 10 wt %) occurring as micrometre-sized crystals with random orientation or with palisade-structure between pyroxene and plagioclase. In general, secondary amphibole contains between 2 and 3 atoms per formula unit (a.p.f.u.) Al and >07 a.p.f.u. Na, making it pargasitic in composition (Fig. 4). The highest Al concentrations are found in amphiboles surrounding opx, whereas lower Al concentrations are found in amphiboles close to cpx. TiO2 concentrations (01–04 wt %) in secondary amphiboles are lower than those in the magmatic amphiboles. Plagioclase from this zone is not altered and has the same composition as plagioclase from the protolith. The reaction of plagioclase with pyroxene to form amphibole marks the beginning of the amphibolitization process. Samples from this early alteration sequence contain micrometre-sized halite crystals (Fig. 3d). To preserve salt crystals during sample preparation, samples were either sawn only in oil or investigated as cracked fragments. Halite crystals observed in samples prepared with both techniques were situated in irregular-shaped holes and cracks between amphibole grains. They do not originate from a fluid inclusion within a single mineral as fluid inclusions are not observed in the whole sample sequence. KCl, a typical high-temperature salt (Markl & Bucher, 1998), was not found. Amphibole zone The amphibole zone is characterized by the progressive replacement of the two pyroxenes by Al-rich amphibole. Modal abundance of amphibole increases from 12% (unaltered gabbro) to 55% (completely amphibolitized gabbro) with decreasing distance to the shear Journal of Petrology, 2015, Vol. 56, No. 2 amphibolitization scapolitization amphibolitization scapolitization 1 3 0.8 2 0.6 0.8 6 0.7 5.5 #Mg 0.9 6.5 2 1 1 0.5 1 1.8 0.5 1.6 PG −25 −20 −15 −10 −5 0 PG −25 −20 −15 −10 −5 0 K2O (wt.%) 0.6 Cl (wt.%) Ca (a.p.f.u) TiO2(wt.%) Si (a.p.f.u) Al (a.p.f.u) 4 Na (a.p.f.u) 306 0 distance to shear zone (cm) Fig. 4. Element distribution in amphibole from the Langøy alteration sequence with increasing distance from the shear zone towards the least altered gabbro (PG); box (horizontal line indicates mean; size of box indicates standard deviation) and whisker bars (1r) representation of EMPA data for each sample (outliers as þ); a.p.f.u. and Mg# calculated from concentration data on the basis of 23 O. zone; simultaneously, the abundance of magmatic mafic mineral relicts decreases (px 32% in pristine gabbro to 0% in altered gabbro; Fig. 2e). Although amphibole is mainly pargasitic in composition it shows highly variable Mg# (060–075) and TiO2 (01–14 wt %), Al2O3 (12–20 wt %) and K2O (02–05 wt %) concentrations (Fig. 4). Microprobe analyses of Cl in amphibole reveal decreasing concentrations towards the shear zone, from more than 1 wt % on average (maximum 13 wt %) to 04 wt % on average for each section. Fluorine concentrations of amphibole were below the detection limits of EMPA. Plagioclase from this zone shows slight sericitization in the mineral cores and incipient replacement by scapolite at the rims. Cl-rich apatite is replaced by homogeneous OH-rich apatite (XCl ¼ 02, XOH ¼ 08, XF < 005). Scapolite zone The transition from the amphibole to the scapolite zone is defined by the appearance of scapolite (Ma57–65) and Ti-rich biotite (14–17 wt % TiO2) as major phases. The modal abundance of scapolite increases within this zone from 5% nearest the amphibole zone to 36% nearest the shear zone. Simultaneously, the abundance of biotite increases from 0% to 17%. Biotite has Cl concentrations (by EMPA) of 02–03 wt % and F concentrations below detection limit. Scapolite has low S with a maximum 01 wt % SO4, but different amounts of Cl and CO3 (defining the end members marialite [Na4Al3Si9O24(Cl)] and meionite [Ca4Al6Si6O24(CO3)]. Chlorine concentrations (by EMPA) in scapolite vary between 20 and 28 wt % and show a slight trend of increasing Cl towards the shear zone. CO2 concentrations were calculated using the meionite content of scapolite, which in turn was calculated following Hassan & Buseck (1988) by using the coupled exchange of (Na4.Cl)Si2 and (NaCa3.CO3)Al2 to be 0378 6 0034. Calculated CO2 concentrations are of the order of 197 6 018 wt %. Amphibole from the scapolite zone is coarser-grained and more homogeneous in composition than amphibole from the amphibolitization zone. On average, it has slightly lower Al2O3 (13–16 wt %, corresponding to 24–26 a.p.f.u.) and Na2O (24–31 wt %, corresponding to 06–08 a.p.f.u) concentrations, but higher TiO2 concentrations (04–07 wt %) compared with amphibole formed in the first alteration zone (Fig. 4). EMPA of Cl in amphibole gives average concentrations of 04 wt %. Magmatic plagioclase and ilmenite are absent. Apatite from the scapolite zone is heterogeneous (XCl ¼ 01–02, XOH ¼ 05–09, XF ¼ 0–03) within single crystals and shows the highest F concentrations Journal of Petrology, 2015, Vol. 56, No. 2 3 Scapolite 2.5 wt.% Cl (EMPA) of 15 wt % close to the shear zone. Albite, analcime, calcite and tourmaline are accessory minerals that occur close to the shear zone, indicating the transport of B, Na and CO2 during metasomatism. The latter assemblage possibly reflects the albitization event, as albite and analcime typically replace scapolite. Analcime and albite also grow on the 001 planes of single biotite grains (Fig. 3c), producing a swelling structure within biotite grains. Although albitization is an important regional metasomatic event, it is minimal in the studied rocks and might have happened at a later stage. 307 2 1.5 Biotite 1 Shear zone The shear zone consists of monomineralic amphibole of pargasitic composition (Al 14–15 wt %, corresponding to 24–25 a.p.f.u; Na 27–30 wt %, corresponding to 07–08 a.p.f.u) with high TiO2 (07–09 wt %) concentration, Cl of 04 wt % and a Mg# of 07. Halogen chemistry In the following section halogen data for solid phases are calculated from the halogen concentrations of pyrohydrolysis extraction solutions measured by IC (F) and ICP-MS (Cl, Br, I), if not explicitly stated otherwise. Solids used for pyrohydrolysis were either bulk samples or picked mineral separates that represent a homogenized fraction of possibly heterogeneous minerals from one sample. Comparison of average Cl concentrations obtained by EMPA and pyrohydrolysis for different minerals and mineral separates of the same sample give identical values within uncertainties for most pairs (Fig. 5). Differences between the two methods for scapolite might result from a contamination of hand-picked separates with plagioclase intergrown with scapolite. In this case, the amount of scapolite melted for extraction would be lower than inferred for calculations, leading to an underestimation of Cl concentration. The similarity of EMPA and ICP-MS analyses provides an additional indicator of the absence of fluid inclusions in amphibole, as pyrohydrolysis would liberate halogens from fluid inclusions whereas EMPA measurements would be not affected by fluid inclusions. Amphibole zone Bulk-rock halogen concentrations vary widely along the sequence (Fig. 6, Table 1). The pristine gabbro has relatively low halogen concentrations (F ¼ 104 mg g–1; Cl ¼ 1495 mg g–1; Br ¼ 32 mg g–1; I ¼ 005 mg g–1) compared with concentrations in the least altered samples from the amphibole zone (F ¼ 159 mg g–1; Cl ¼ 3801 mg g–1; Br ¼ 141 mg g–1; I ¼ 046 mg g–1). However, the Br/Cl and I/ Cl ratios are similar (Fig. 6e and f). Metagabbros from the amphibole zone reveal only a small spread in F, Cl and Br concentrations (F ¼ 49–122 mg g–1; Cl ¼ 3801– 4900 mg g–1; Br ¼ 88–141 mg g–1), except for two samples close to the scapolite zone, which have very high F concentrations up to 964 mg g–1. This sudden increase in F is detected only in bulk samples, which may contain Amphibole 0.5 0 0 0.5 1 1.5 2 2.5 wt.% Cl (pyrohydrolysis) 3 Fig. 5. Comparison of Cl concentration measured by EMPA (average Cl content of biotite, amphibole and scapolite with 1r error) and by ICP-MS of extraction solution (with 1r error of nine replicates) of mineral separates from the same sample. undetected minor phases (e.g. fluorite, hydrogarnet) that might incorporate F. Secondary hydrogarnets found in other metamorphic rocks from the Bamble sector can contain high F concentrations of up to 16 wt % (Visser, 1993), but are not observed in the studied sample sequence. The only observed F-bearing mineral in the whole sequence is apatite, which in the amphibole zone is, however, F-poor <05 wt %). Therefore, a nonuniform distribution of apatite or an undetected F-bearing mineral could account for local high F concentrations. The maximum iodine concentration (087 mg g–1) was detected in the centre of the amphibole zone. Chlorine and Br concentrations slightly increase from 4900 to 8060 mg g–1 and from 101 to 185 mg g–1, respectively, towards the scapolite zone, whereas the I concentration remains constant (Fig. 6d). The similar distribution of Cl and Br leads to a limited variation in Br/Cl ratios (19 10–3 to 37 10–3). As bulk I and Cl concentrations show little variation in this part of the sequence, I/Cl ratios do not change systematically and vary between 70 10–6 and 120 10–6 (Table 1). Amphibole is a major sink for halogens, especially for Cl, in this zone. As the infiltrating fluid reacts with the gabbro, newly formed amphibole dominates the Cl budget. Amphibole in the pristine gabbro has higher Br and F concentrations, but similar I and lower Cl concentrations, compared with amphiboles from the first alteration zone. Amphibole from the least altered samples has a high Cl content of 11 wt %; single amphibole grains incorporate >13 wt % Cl, measured by EMPA. Although bulk Cl concentrations are constant in the amphibolitization zone, Cl concentrations in amphibole decrease towards the shear zone, in the same way as the modal abundance of amphibole increases (Fig. 3e). At the transition to the scapolitization zone amphibole 308 Journal of Petrology, 2015, Vol. 56, No. 2 bulk amph scapo bio Cl(wt%) 2 1.5 b) a) 100 10 1 Br(µg/g) 2.5 0.5 1 c) d) 1 100 0.1 I(µg/g) F(µg/g) 1000 10 f) 1000 1 0.1 100 PG −25 −20 −15 −10 −5 0 distance to shear zone (cm) PG −25 −20 −15 −10 −5 0 I/Cl (*10-6) Br/Cl (*10-3) e) 10 distance to shear zone (cm) Fig. 6. Chlorine, Br, F and I concentrations, and Br/Cl and I/Cl ratios of bulk samples and mineral separates from the Langøy alteration sequence. has Cl concentrations of 040–045 wt %. Bromine concentrations in amphibole show a similar trend to Cl concentrations, with the highest values (54 mg g–1) in the least altered part of the sequence and lower values (17 mg g–1) close to the second (scapolitization) alteration zone. Iodine concentrations in amphibole vary between 02 and 07 mg g–1 in the amphibolitization zone, without a distinct trend. Fluorine in amphibole has concentrations between 89 and 180 mg g–1. Halogen ratios for amphibole are 035 10–3 to 051 10–3 for Br/Cl and 38 10–6 to 113 10–6 for I/Cl. Apatite appears as an accessory phase (modal abundance <1% determined from optical observations) in all samples and was not picked as mineral separates; however, single apatite grains were analysed by EMPA. Apatite from the amphibolitization zone has Cl concentrations between 08 and 14 wt % and low F concentrations of less than 05 wt %. Scapolitization zone Bulk-rock concentrations of Cl and Br increase from the transition to the amphibolitization zone towards the scapolitization zone to values of 1 wt % for Cl and 27–33 mg g–1 for Br and vary little within the scapolitization zone. Although iodine concentrations (03– 04 mg g–1) vary less than Cl concentrations for the whole scapolitization zone, the increasing Cl concentrations lead to decreasing I/Cl ratios (from 93 10–6 to 27 10–6) from the amphibolitization zone towards the shear zone. Simultaneously, Br/Cl ratios increase from 19 10–3 to 3 10–3 towards the shear zone. Amphiboles from the scapolitization zone show little halogen variability, in the range of 041–044 wt % for Cl, 12–27 mg g–1 for Br and 021–064 mg g–1 for I. Therefore, Br/Cl ratios vary little between 034 10–3 and 064 10–3 and I/Cl ratios between 47 10–6 and 130 10–6. Fluorine is elevated (with the exception of one measurement) compared with the amphibolitization zone, with concentrations ranging from 184 to 245 mg g–1. In scapolite halogen concentrations increase towards the shear zone. Average F, Cl, Br, and I concentrations range from 43 mg g–1, 19 wt %, 77 mg g–1, and 073 mg g–1 close to the amphibolitization zone to 97 mg g–1, 24 wt %, 102 mg g–1 and 1 mg g–1 close to the shear zone, respectively. As scapolite is a solid solution between marialite (Cl-rich) and meionite (CO3-rich), the increase in Cl concentration needs to be charge balanced, probably by a decrease of CO3 in scapolite. Halogen ratios of all scapolite samples fall within a small range (Br/ Cl ¼ 36 10–3 to 42 10–3; I/Cl ¼ 34 10–6 to 42 10–6). Biotite is another halogen-bearing mineral phase from the scapolitization zone, but incorporates less Cl (018–020 wt %) compared with amphibole and scapolite. The concentrations of F, Br and I in biotite increase with decreasing distance to the shear zone, from 131 to 336 mg g–1 F, 11 to 55 mg g–1 Br and 053 to 279 mg g–1 I (Fig. 6d). In this context, the highest concentrations of F, Br and I and exceptionally high halogen ratios (Br/Cl ¼ 23 10–3 and I/Cl 1169 10–6) are found in the sample closest to the shear zone, which shows some alteration of biotite (i.e. growth of analcime between Journal of Petrology, 2015, Vol. 56, No. 2 309 Table 1: Halogen concentrations, d37Cl and d18O values in bulk-rocks, amphibole, biotite and scapolite from Langøy and Valberg alteration sequences Locality Sample Assemblage cm to F Cl Br I SZ (mg g–1) (mg g–1) (mg g–1) (mg g–1) F/Cl (103) Br/Cl (103) I/Cl (106) d37Cl d18O Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Valberg Valberg Valberg Valberg Valberg Amphibole Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Langøy Valberg Valberg Valberg Valberg Valberg Biotite Langøy Langøy Langøy Langøy Langøy Valberg Scapolite Langøy Langøy Langøy Langøy Langøy Valberg Valberg BAM 3-5 BAM 3-4-1 BAM 3-4-2 BAM 3-4-3 BAM 3-4-4 BAM 3-4-5 BAM 3-4-6 BAM 3-4-7 BAM 3-4-8 BAM 3-4-9 BAM 3-4-10 BAM 3-4-11 BAM 3-4-12 BAM 3-4-13 BAM 3-4-14 BAM 3-4-15 BAM 21-1 BAM 21-2-III BAM 21-5 BAM 21-3-III BAM 21-3-I ol–px–amph–pl px–amph–pl px–amph–pl px–amph–pl px–amph–pl amph–pl amph–pl amph–pl amph–pl–scp–bio amph–pl–scp–bio amph–pl–scp–bio amph–scp–bio amph–scp–bio amph–scp–bio amph–scp–bio amph ol–px–amph–pl amph–pl amph–scp–bio amph–scp amph — 264 24 218 198 177 159 14 114 94 76 57 42 25 07 –08 147 47 27 16 0 104 159 85 99 122 73 49 397 964 162 131 140 106 159 131 187 122 550 231 98 215 1495 3801 5098 5097 4803 4554 4960 4900 5419 6555 8060 10213 9727 11036 9864 5534 777 7136 11430 16410 10902 32 141 129 98 92 88 125 101 109 125 185 276 277 334 294 79 10 88 455 1093 41 0047 0460 0358 0402 0569 0872 0579 0456 0424 0390 0321 0376 0359 0298 0366 0398 0081 0393 0369 0382 0375 6938 4192 1669 1940 2532 1608 990 8102 17795 2470 1625 1374 1088 1436 1331 3380 15761 7705 2018 600 1968 216 370 254 192 191 193 252 206 202 191 230 270 285 303 298 142 123 123 398 666 037 3158 12101 7023 7885 11858 19148 11670 9310 7820 5944 3977 3682 3691 2703 3706 7186 10455 5512 3226 2326 3443 –01 BAM 3-5 BAM 3-4-3 BAM 3-4-4 BAM 3-4-5 BAM 3-4-6 BAM 3-4-7 BAM 3-4-8 BAM 3-4-9 BAM 3-4-10 BAM 3-4-11 BAM 3-4-12 BAM 3-4-13 BAM 3-4-14 BAM 3-4-15 BAM 21-1 BAM 21-2-III BAM 21-5 BAM 21-3-III BAM 21-3-I Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole Amphibole — 218 198 177 159 14 114 94 76 57 42 25 07 –08 147 47 27 16 0 348 157 113 119 89 180 125 135 245 201 17 198 184 383 405 165 128 151 132 7042 10683 8887 8181 7594 6313 4441 4122 4057 4409 4417 4361 4234 4725 3200 5942 4505 4969 10971 82 54 38 34 33 23 17 13 16 17 15 22 27 21 16 12 32 57 10 0393 0669 0341 0417 0470 0712 0583 0218 0537 0238 0212 0640 0432 0574 0179 1005 0522 0693 0637 4936 1470 1271 1460 1166 2846 2813 3284 6048 4568 396 4544 4357 8108 12658 2776 2846 3036 1200 116 051 042 041 043 036 038 031 040 038 034 050 064 044 050 020 070 115 010 5578 6259 3841 5098 6187 11272 13129 5296 13228 5407 4789 14677 10211 12144 5601 16917 11598 13937 5810 03 –06 –04 –02 00 03 04 00 01 03 05 BAM 3-4-10 BAM 3-4-11 BAM 3-4-12 BAM 3-4-13 BAM 3-4-14 BAM 21-5 Biotite Biotite Biotite Biotite Biotite Biotite 76 57 42 25 07 27 131 192 176 159 336 51 1828 1939 2009 1949 2382 2965 14 11 19 26 55 22 0583 0529 0815 0657 2787 0574 7191 9926 8743 8139 14093 1715 075 058 096 131 232 073 31899 27300 40564 33684 116986 19378 00 02 04 BAM 3-4-10 BAM 3-4-11 BAM 3-4-12 BAM 3-4-13 BAM 3-4-14 BAM 21-5 BAM 21-3-III Scapolite Scapolite Scapolite Scapolite Scapolite Scapolite Scapolite 76 57 42 25 07 27 16 43 43 61 63 97 33 724 19113 21441 22378 23774 24090 23748 22377 771 799 809 929 1016 1191 1621 1618 0727 0823 1000 0956 0897 0785 225 198 272 264 402 141 3236 403 373 361 391 422 502 724 8468 3389 3677 4208 3968 3779 3508 02 00 02 –06 –02 –02 –02 07 05 06 04 00 03 05 07 05 01 10 12 05 08 09 00 04 –03 –02 00 51 37 54 51 34 55 55 68 72 72 67 70 74 73 10 04 02 –07 –05 SZ, shear zone. biotite laths). This alteration might be the reason for a decoupling of Cl and Br in this sample (Fig. 6e). For all other samples Br/Cl ratios vary between 058 10–3 and 13 10–3 and I/Cl ratios between 273 10–6 and 405 10–6. Apatite has highly variable F concentrations (by EMPA) from less than 01 wt % to 15 wt % with a trend of increasing values towards the shear zone, whereas Cl concentrations are constant with an average value of 10 6 03 wt %. Although apatite might affect the F budget of the bulk-rock, it plays only a minor role in the budget of Cl (and probably Br and I) as its abundance is too low compared with all other halogen-bearing phases. 310 Journal of Petrology, 2015, Vol. 56, No. 2 1.5 2 scapolitization amphibolitization a) δ 37Cl 1 1 scapolitization amphibolitization b) 1σ error 0.5 0 0 -0.5 bulk -1 -1.5 amph scapo bio 1σ error PG -25 -20 -15 -10 -5 distance to shear zone (cm) 0 -1 -2 -147 -47 -27 -16 0 distance to shear zone (cm) Fig. 7. d37Cl values of (a) Langøy sample sequence and (b) Valberg sample sequence for bulk-rocks, amphibole, scapolite and biotite according to their distance to the shear zone. Chlorine isotope geochemistry Pristine gabbro The unaltered Langøy gabbro has a d37Cl value of –01 6 02% (Fig. 7a), similar to values from a depleted mantle reservoir (Sharp et al., 2007, 2013; John et al., 2010). Amphibole separated from the pristine gabbro has a slightly higher d37Cl value of þ03 6 02%, but still within analytical uncertainty of the bulk measurement. Sequence The d37Cl values of bulk samples from the sequence vary between –06 and þ 07%, with a clear tendency of lower values towards the unaltered zone (Fig. 7a, Table 1). With increasing degree of alteration, d37Cl values from the amphibole zone increase until a maximum of þ06% is reached close to the transition to the scapolite zone. Samples across this transition show decreasing values (to a minimum of 0%). However, within the scapolite zone d37Cl values increase again and reach a maximum (þ07%) close to the shear zone, which itself has a d37Cl value of þ05%. Mineral separates The d37Cl values of amphibole separates range from –06 to þ1%, similar to the bulk samples. The amphibole d37Cl values are lowest in the least altered part of the section, also similar to the bulk samples (Fig. 7a). The d37Cl values increase towards the shear zone, but show a local minimum (0%) at the transition between the scapolite zone and amphibole zone. Separated scapolite shows minimal variation in its isotopic composition throughout the sequence and has an average value of þ02 6 01%. The d37Cl values of biotite separates range from 0 to þ1% and decrease with increasing distance from the shear zone (Fig. 7a). Bulk d37Cl values are consistent with the weighted average d37Cl of each of the mineral phases. Therefore, the dominant Cl-bearing phase of each zone controls the overall bulk d37Cl value. The small variation in d37Cl for different minerals (i.e. amphibole, scapolite and biotite) in one single sample indicates the absence of a significant fractionation of Cl isotopes between different silicates. However, an isotopic fractionation between fluid and silicates cannot be excluded. Oxygen isotopes d18O values of amphiboles (Table 1) from each sample were measured to estimate fluid:rock ratios (f/r) during alteration. Amphibole from the pristine gabbro has a d18O value of þ51%, which falls in the isotopic range for mantle-derived rocks. Owing to minimal oxygen isotope fractionation between silicate melt and crystallizing minerals at magmatic temperatures (typically <1% for most phases), most mantle-derived minerals will have similar d18O values to the bulk upper mantle (þ55%) (Eiler, 2001; Sharp, 2007). In the amphibolitization zone, the d18O values of amphibole range from þ34 to þ55%, and d18O shows higher values in the scapolitization zone, as well as the shear zone, ranging from þ67 to þ74%. Valberg metagabbro Samples from the Valberg metagabbro show the same alteration sequence as the Langøy samples. Adjacent to the amphibolitic shear zone, the scapolitization zone is characterized by the mineral assemblage scapolite, amphibole and biotite. Close to the shear zone biotite forms isolated grains, whereas further from the shear zone it forms clusters, similar to biotite in the Langøy samples. Furthermore, the width of the scapolitization zone is larger (30 cm wider) than that of the scapolitization zone in the Langøy sample sequence. The amphibolitization zone adjacent to the scapolitization zone is also larger, as amphibole-rich metagabbro is still present 1 m away from the shear zone. Shearing, indicated by a high density of micrometre-sized cracks and veins, is more prominent in the Valberg samples compared with the Langøy sample and may be the reason for the enlarged alteration zones, as the higher fluid flux in microveins accelerates pervasive fluid flow (Zack & John, 2007). Halogens Halogen concentrations and d37Cl values of the Valberg samples are in the same range as those in the Langøy sequence (Table 1). Although the Valberg sequence Journal of Petrology, 2015, Vol. 56, No. 2 bulk amph scapo bio Cl(wt%) 2 1.5 b) a) 100 10 1 Br(µg/g) 2.5 311 0.5 1 c) d) 100 0.1 0.01 10 e) Br/Cl (*10-3) I(µg/g) 1 f) 100 1 0.1 -147 amphibolitization -47 scapolitization amphibolitization -27 -16 0 -147 distance to shear zone (cm) -47 scapolitization -27 -16 0 I/Cl (*10-6) F(µg/g) 1000 10 distance to shear zone (cm) Fig. 8. Halogen concentrations and ratios of Valberg metagabbro samples. was sampled in less detail, changes in halogen concentrations (Fig. 8) and d37Cl values within the various zones follow similar trends to the Langøy samples (Fig. 7b). DISCUSSION A detailed investigation of the mineral reaction history is crucial to understand the geochemical evolution of the fluid. Observed mineral reactions are caused by changed chemical potentials owing to infiltration of a metasomatic fluid under constant temperature and pressure conditions. The continuing fluid–rock interaction will not only alter the composition of the rock, but also progressively change the fluid composition, especially if the water:rock ratio is low. Here, we present a case study in which a highly saline fluid is infiltrating a dry gabbro, causing various mineral replacement reactions. These reactions lead to a continuing desiccation of the fluid until halite is precipitated and the fluid is completely consumed. Chlorine concentration in amphibole is used to monitor the changing salinity of the fluid. Changes in d37Cl values with distance to the shear zone probably result from Rayleigh fractionation of Cl isotopes during incorporation of Cl from the fluid into the forming mineral phases (Gleeson & Smith, 2009). Oxygen isotope data reveal fluid:rock ratios (f/r) of <02 for the amphibolitization zone, indicating a rockdominated environment, and 2–14 for the scapolitization zone, indicating a more fluid-dominated regime. Correlations among the changing mineral assemblages, the mineral chemistry, and the chemical evolution of the fluid on a small scale are critical to understanding metasomatism and related ore genesis on a regional scale (Smith et al., 2013). We focus on the Langøy sequence for the discussion as the two sample sites indicate essentially identical mineral reactions and changing mineral compositions with increasing metasomatism. The sample sequence from Langøy is more detailed compared with that from Valberg and alteration is clearly caused by pervasive fluid infiltration adjacent to the main fluid pathway. Mineral replacement reaction The alteration reactions leading to the various zones in the sequence are similar to those described by Engvik et al. (2011). All alteration reactions are referred to as mineral replacement reactions because newly formed minerals start growing either as coronae around magmatic crystals or at the expense of pristine coronae, until the primary phases are completely consumed. Opx (6 spinel) coronae around olivine, as well as amphibole–spinel coronae around pre-existing opx (6 spinel) coronae (Fig. 3a), are present in the most pristine samples and are probably of magmatic origin (de Haas et al., 2002). However, less altered samples (indicated by a low abundance of amphibole) are almost olivine free. The rare olivine appears to be replaced by pyroxene first, which is then replaced by amphibole, rather than the olivine being directly reacted to amphibole. Orthopyroxenes of probably different origin (i.e. magmatic coronae or products of olivine replacement) 312 Journal of Petrology, 2015, Vol. 56, No. 2 are chemically indistinguishable from each other. However, all pyroxenes show amphibole coronae (Fig. 3a) caused by the reactions Clinopyroxene ðDi65–70 Þ þ Plagioclase ðAn60–70 Þ þ H2 O ! Pargasite (1a) Orthopyroxene ðEn70–75 Þ þ Plagioclase ðAn60–70 Þ þ H2 O ! Pargasite: (1b) Reactions (1a) and (1b) are characteristic for the amphibolitization zone and lead to the mineral assemblage pargasite þ plagioclase 6 apatite 6 ilmenite. Increasing alteration leads to a complete replacement of all pyroxene, removing all coronitic textures. Alteration occurring in the second alteration zone (scapolitization) includes the following reaction: Ilmenite þ Kþ þ Mg2þ þ Al3þ þ Si4þ þ H2 O ! Biotite þ Ti4þ : (2) Biotites grown from this reaction have high TiO2 concentrations (up to 2 wt %) and contain many micromtre-sized zircon inclusions (Fig. 3c). The zircons form a three dimensional framework, which reflects the former grain boundaries of the replaced ilmenite (Austrheim et al., 2008). Scapolite was formed by a reaction of magmatic plagioclase with a highly saline, CO2-containing fluid: PlagioclaseðAn60–70 Þ þ Naþ þ Cl– þ CO2 ! Scapolite ðMa57–67 Þ: (3) Local Al excess owing to the replacement reaction leads to the formation of sub-micrometre- to micrometre-sized spinel crystals at the reaction front (Fig. 3b). Greenish spinel is found only in the narrow transition zone between the two alteration zones and is no longer observed when all plagioclase is replaced. The formation of other Al-rich phases (sapphirine, corundum) during plagioclase to scapolite replacement (Engvik & Austrheim, 2010) is a metasomatic reaction feature and occurs only on small spatial scales. The formation of scapolite with a meionite component of 33–43% indicates the presence of CO2 in the fluid in addition to the high halogen content. Amphiboles in the scapolitization zone are coarser grained and compositionally homogeneous compared with the amphibolitization zone in which several different pargasitic amphibole types can be distinguished by composition (e.g. different Ti, Na, Cl, and Al concentrations) and by origin (e.g. magmatic cooling products, coronae surrounding opx or cpx). Therefore, it is likely that a recrystallization process chemically homogenized the amphibole. Fluid:rock ratio Fluid:rock ratios (f/r) were estimated using the d18O values of the amphibole that originates from fluid–rock interaction. The f/r (in mole fraction) can be defined as f df rock di rock ¼ i r d fluid ðdf rock Drock–fluid Þ (4) where dirock, dfrock and difluid are the isotope ratios of the initial rock, final rock and initial fluid, respectively, and Drock–fluid is the equilibrium fractionation between the final rock and the fluid. This equation was used to calculate f/r for each sample assuming a single pass of fluid through the rock (e.g. Sharp, 2007). To calculate f/r ratios for the Bamble alteration sequence, dirock is assumed to be equal to the isotopic ratio of pristine amphibole (þ51%) and dfrock is assumed to be equal to average measured d18O values of amphibole in the altered zone (þ102%). The Drock–fluid was calculated following Zheng (1993) to be –28% for the equilibrium fractionation between pargasite and H2O at the assumed temperature of metasomatism (600 C). Although difluid cannot be measured directly, it can be estimated in two ways. First, the d18O value of shear zone amphibole can be used to calculate a fluid value as these amphiboles should have experienced the most interaction with fluid. Shear zone amphibole has a d18O value of þ73%, corresponding to a fluid with þ101% taking equilibrium partitioning at 600 C into account. Second, data from the literature were used to compare the oxygen isotope composition of the shear zone amphibole with other phases. Broekmans et al. (1994) reported d18O values for calcite found in scapolite-bearing veins that cross-cut metagabbros from the Bamble area to range from þ102 to þ235%. As a best approximation of their data, we calculated a d18O value for the Bamble fluid of þ93%, assuming an equilibrium fractionation of þ09% (Hu & Clayton, 2003) between calcite with the lowest values (d18O ¼ 102%) and fluid at 600 C. Although the value calculated from the literature is lower than that calculated from the shear zone amphibole, they agree reasonably well, as the second value was calculated from the lowest d18O value and, therefore, represents a minimum value for the fluid. Further calculations of f/r ratios were carried out using a difluid of 101%. Amphibole from the amphibolitization zone has almost identical d18O values to amphibole from pristine gabbro. Consequently, calculated f/r values assuming a single-pass case of the fluid are low (<02), indicating a rock-dominated regime for the amphibolitization zone. Fluid:rock ratios of samples from the scapolitization zone vary between 25 and 14, indicating a clearly fluiddominated regime if a single-pass case is assumed. Assuming a multi-pass case (or an evolving fluid) lowers the calculated f/r significantly to a maximum of 11 for the scapolitization zone and of <01 for the amphibolitization zone. Fluid:rock ratios might be overestimated because using the d18O values of the shear zone amphibole to represent difluid carries the implicit assumption that these were formed under completely fluid-dominated Journal of Petrology, 2015, Vol. 56, No. 2 Mantle (Kendrick et al. 2012) SW sca po liti zat ion fore arc sediments (Kendrick et al. 2011) (John et al. 2011) S apoScapop tes tes lites sw e v traje apor. ctory 5 amphibolitization Bio t ites 1 Evaporites The pervasive metasomatism in the Bamble sector occurs on a regional scale and affects not only gabbros, but almost all magmatic and metamorphic rocks (Engvik et al., 2008, 2011). Therefore, a large quantity of external fluid is required to allow this extensive alteration. On a metre scale, fluid–rock interaction is localized in zones of enhanced permeability, such as veins and shear zones, and their adjacent wall-rocks. Fluid inclusions from neighbouring metasediments (Fig. 1b) and quartz veins have high NaCl concentrations (up to 25 wt % and higher as indicated by NaCl daughter crystals found within the inclusions) (Touret, 1985; Nijland et al., 1998a). This saline fluid was also enriched in K, Mg, B and P, as can be inferred from newly formed minerals (Engvik et al., 2011). The origin of these brines is still under debate. Possible sources are as follows: (1) deeply infiltrating fluids derived from overlying sediment sequences (Munz et al., 1995; Nijland & Touret, 2001); (2) fluids from prograde metamorphosed, deeply buried sediments (Engvik et al., 2011); (3) late-stage magmatic fluids; (4) fluids derived from the mobilization of evaporites (Touret, 1985; Engvik et al., 2011). Tourmalines from different alteration zones (i.e. scapolitization and albitization) of Bamble rocks have d11B values of –6 to þ26%, indicating a fluid component derived from a marine environment (Bast et al., 2014). Chlorine concentrations in the upper mantle are low (1–4 mg g–1) (Saal et al., 2002), but are higher and extremely variable (1–4000 mg g–1) in basaltic melts derived from a mantle source (Kendrick et al., 2012). The most pristine gabbro sample from Langøy has a Cl concentration of 1495 mg g–1, which is within the Cl concentration range for mantle-derived magmas. However, an additional gain of Cl from interaction with the infiltrating hydrothermal fluid cannot be excluded. Bromine and iodine concentrations (Br 32 mg g–1; I 004 mg g–1) in -3 Origin of the fluid the pristine gabbro are elevated compared with averaged literature data for mid-ocean ridge basalt (MORB; Edmond et al., 1979; Schilling et al., 1980; Deruelle et al., 1992; Jambon et al., 1995; John et al., 2011), but are similar to concentrations in enriched (E)-MORB glasses from Macquarie Island (Br 038–45 mg g–1; I 001–0109 mg g–1) (Kendrick et al., 2012). Br/Cl and I/Cl ratios (Fig. 9) in the least altered sample are similar to those for E-MORB from Macquarie Island, which Kendrick et al. (2012) considered is representative of present-day mantle. Therefore, the halogen ratios of the most pristine Langøy gabbro may represent the halogen ratios of its mantle source. Bulk Br/Cl and I/Cl ratios of altered samples result from interaction of halogen-poor, pristine gabbro with a halogen-rich metasomatic fluid, which leads to the formation of minerals incorporating different amounts of halogens. The characteristics of the infiltrating metasomatic fluid are best represented by the most strongly altered samples adjacent to the shear zone, as these were fluid-dominated and in contact with the initial fluid composition. Halogen concentrations and ratios of the fluid are given by the partition coefficient (Dmin ¼ chalmin/ chalfluid) between mineral and fluid. If the Dmin values are known, a bulk partition coefficient (Dbulk) can be calculated. Partition data for Br and I between fluid and minerals of interest (i.e. amphibole, scapolite and biotite) are lacking, but are probably smaller than for Cl. Following lattice strain theory, one would expect DCl > DBr > DI for amphibole, scapolite and biotite. Without knowing the exact partition coefficients, we can constrain the halogen ratios of the initial fluid by applying the relative order (DCl > DBr > DI) of partition coefficients to the measured halogen concentrations of the most strongly altered samples. Consequently, Br/Cl Br/Cl (*10) conditions. Although this agrees with a difluid calculated using the lowest reported value of calcite, Broekmans et al. (1994) argued that the low values (102–106%) of the vein calcite are probably the result of the strong interaction of fluid with the wall-rock (metagabbro). If the high d18O values of 20% observed for other vein calcite from the same metagabbro were used for the calculations, f/r of both alteration zones would be <<1 and the scapolitization zone would also be strongly rock-dominated. Even though the estimation of the isotopic composition of the initial fluid and its evolution owing to fractionation create uncertainties in the f/r calculations, a strongly rock-dominated regime for the amphibolitization zone and a less rock-dominated regime for the scapolitization zone is a robust conclusion. This is further expressed by the different degree of alteration in the amphibolitization zone (low) and scapolitization zone (complete), which indicates a decreasing amount of fluid towards the pristine part of the sequence. 313 Amphiboles highly altered least altered 100 1000 -6 I/Cl (*10 ) Fig. 9. Br/Cl vs I/Cl concentration ratios (by weight) of bulk-rock samples and mineral separates from Langøy compared with different fluid sources: pore fluids (Kendrick et al., 2011), evaporites (Holser, 1979), pelitic fore-arc sediments (John et al., 2011), mantle (Kendrick et al., 2012) and seawater (SW); light grey arrow indicates halogen ratio trend in scapolite zone; dark grey arrow indicates halogen ratio trend in amphibole zone. 314 Journal of Petrology, 2015, Vol. 56, No. 2 ratios and I/Cl ratios must be higher than 3 10–3 and 25 10–6, respectively, measured for samples from the scapolite zone. When comparing these ratios with those of geologically important fluid sources, they fall in the range of marine pore fluids (Fig. 9) and marine sediments, which have high Br/Cl and I/Cl ratios (John et al., 2011). Therefore, a fluid produced by prograde metamorphism of marine sediments together with liberation of coexisting pore fluids should reflect the high I/Cl ratios of the sediments and the high Br/Cl of the pore fluids (Kendrick et al., 2011). In contrast, evaporites produce fluids with very low I/Cl and Br/Cl ratios (Holser, 1979), neither of which match the ratios of the Bamble fluid. A late-stage magmatic origin of the fluid is also unlikely as magmatic fluids from ore deposits have I/Cl ratios and Br/Cl ratios similar to mantle ratios (Kendrick et al., 2001, 2011), which are too low if the partitioning between fluid and alteration minerals is considered. Cl Cl The observed correlation XBio 033XAmph (Markl & Piazolo, 1998; Markl et al., 1998) allows the calculation of NaCl activity from amphibole composition by measuring the Cl concentration in biotite and amphibole and assuming ideal mixing of OH– and Cl– in the biotite and amphibole structures. A similar approach was used to calculate NaCl activities in fluids from the Langøy metagabbro. The reaction OH-Tremolite þ Enstatite þ Anorthite þ NaClðaqÞ þSiO2 ðaqÞ ! Cl-Tremolite þ H2 O þ Albite (8a) þSpinel þ Diopside Ca2 Mg5 Si8 O22 ðOHÞ2 þ 1 5 Mg2 Si2 O6 þ2 CaAl2 Si2 O8 þ 2 NaCl ðaqÞ þ 3 SiO2 ðaqÞ ! Ca2 Mg5 Si8 O22 Cl2 þ H2 O þ 2 NaAlSi3 O8 (8b) þMgAl2 O4 þ 2 CaMgSi2 O6 Calculation of fluid salinity Besides scapolite, amphibole is a major sink for Cl during fluid–rock interaction in the scapolitization zone and the main Cl-bearing phase in the amphibolitization zone. Amphibole from the two alteration zones always originates from the reaction of the pervasively infiltrating fluid with the unaltered gabbro. Therefore, the halogen activities of the fluid should be reflected in the halogen concentrations of the amphibole. Based on the thermodynamically calculated partitioning of F–Cl–OH between micas and hydrothermal fluids (Zhu & Sverjensky, 1991, 1992) and observed correlations of XCl in biotite and coexisting amphibole, Markl et al. (1998) used the Cl concentration of amphibole to calculate the NaCl activity of fluids in a lower crustal environment. This approach is based on the following equilibrium exchange reaction for biotite: OH Biotite þ NaClðaqÞ þ Anorthite ! Cl Biotite þ Albite þ Grossular þ H2 O þ Kyanite (5a) KMg3 AlSi3 O10 ðOHÞ2 þ 2NaClðaqÞ þ 15CaAl2 Si2 O8 ! KMg3 AlSi3 O10 Cl2 þ 2NaAlSi3 O8 þ 5Ca3 Al2 Si3 O12 þH2 O þ 9Al2 SiO5 : (5b) The equilibrium constant for the reaction is 2 K¼ 5 9 aH2 O ðaClBio aAb aGrs aKy Þ : 15 2 ðaOHBio aAn aNaCl Þ (6) It follows that a specific biotite composition relates to a specific fluid composition by the expression aOH-Bio aH2 O 1 2 5 9 15 ¼ 2 K aAb aGrs aKy aAn : aCl-Bio aNaCl (7) 2 5 9 15 The term K 1 aAb aGrs aKy aAn is a constant for a given temperature, pressure, and mineral assemblage and was estimated to be 1891 (Markl et al., 1998). relates the mineral assemblage found in the metagabbro to the coexisting NaCl fluid. The equilibrium constant for this reaction is Kð9Þ ¼ 2 2 aDi aSp Þ aH2 O ðaCl-Tr aAb 2 2 a 15 a 3 aNaCl ðaOH-Tr aAn En SiO2 Þ (9) and aOH-Tr aH2 O 1 2 2 2 15 3 ¼ 2 Kð9Þ aAb aDi aSp aAn aEn aSiO2 : aCl-Tr aNaCl (10) As thermodynamic data for this reaction are lacking, thermodynamic models (e.g. supcrt92) are not applicable to calculate the equilibrium constant K(9). However, 1 2 2 2 15 3 the term Kð9Þ aAb aDi aSp aAn aEn aSiO2 can be estimated 2 empirically by using a known activity ratio (aH2 O =aNaCl ) for one fluid and the corresponding activity ratio (aCl-Tr/ aOH-Tr) for amphibole. As long as T, P, and the mineral 1 2 2 2 assemblage are constant, the term Kð9Þ aAb aDi aSp aAn 15 3 aEn aSiO2 is a constant and can be used to calculate activity ratios. In the Langøy sequence, the least-altered sample showing first signs of amphibolitization provides an assemblage that can be used to calculate this term. Newly formed amphibole from this zone has Cl contents as high as 13 wt % (measured by EMPA). Assuming an ideal two-site mixing model between Cl– Amph and OH– for amphibole, XCl is 015 and activities for OH-tremolite and Cl-tremolite are 07225 and 00225, respectively. Halite coexisting with the most Cl-rich amphiboles (Fig. 3d) indicates a fluid saturated in NaCl for these samples. Saturation concentrations (and activity ratios) for the system NaCl–H2O can be calculated by using the correlation formulae of Driesner & Heinrich (2007). For a given temperature of 600 C and pressure of 02 GPa for the Bamble metasomatic event (Nijland & Touret, 2001), a saturated fluid has a XH2 O [¼H2O/ (NaCl þ H2O)] of 055 (73 wt % NaCl), which corresponds 2 to aH2 O =aNaCl ¼ 149. The activity data for this sample, which contains halite crystals and the highest Cl Journal of Petrology, 2015, Vol. 56, No. 2 315 concentrations in amphibole, were then used to calcu1 2 2 2 15 3 late the term Kð9Þ aAb aDi aSp aAn aEn aSiO2 , which is 2155. The expression 2 aH2 O XOH ¼ 2 -Tr =21 55: 2 aNaCl XCl-Tr (11) links the fluid composition to the amphibole composition. For this calculation, Cl– is assumed to be speciated only with Naþ in the fluid, but theoretically it could be also speciated with other ions, such as Kþ and Ca2þ. Although K is important for the formation of alteration phases (i.e. biotite), Markl et al. (1998) showed that by far the most dominant uncharged species in their alteration system is NaCl. Furthermore, the observed salt crystals in the least altered sample are pure halite, indicating that NaCl was present at all alteration stages. The fact that no sylvite (KCl) was found, a common high-temperature salt, suggests that either KCl saturation was not reached, which implies that the concentration of K in the fluid was low, or the amount of K was not sufficient to produce a recognizable amount of sylvite. From petrographical observations, the former seems to be more likely as there are no stable K-rich minerals in the amphibolitization zone. Calculations based on equation (8) utilize the exchange of Cl– and OH– in amphibole within a Na-buffered reaction. A reaction buffered in K could be used in a similar manner and yield similar results. In contrast to the NaCl-buffered reaction, where the saturation of halite is used to calculate a reference NaCl/H2O ratio, there is no reference KCl/H2O ratio because KCl was not detected in the sample set, which in turn makes a calculation of KCl concentration impossible. However, even if we assume that KCl was present, it would be saturated at a fluid composition of XH2 O ¼ 044 (Chou et al., 1992). If we further assume that the most Cl-rich amphibole (13 wt % Cl) was formed in equilibrium with sylvite and fluid, rather than halite and fluid, the equilibrium constant used would shift from 2155 for NaCl to 5201 for KCl, resulting in a shift towards slightly higher values for calculated salinities. A pure NaCl-bearing fluid with an XH2 O of 078 (48 wt % NaCl) would have an XH2 O of 070 (63 wt % KCl) as a hypothetical fluid in the binary system H2O–KCl. Although mobility of Ca2þ and Fe2þ is not observed, these divalent cations may also play a role in speciating Cl–. Evolution of the fluid salinity and the effect of Clconsuming vs desiccation reactions A fluid in equilibrium with shear-zone amphiboles has 2 an XNaCl of 022 (aH2 O =aNaCl ¼ 132), giving an initial salinity of 48 wt % NaCl for the infiltrating fluid. Fluid inclusions in metasediments from Bamble also record a high-salinity composition of the fluids; hence are in accordance with our findings (Touret, 1985). Amph Constant XCl in amphibole from the scapolitization zone indicates little to no change in fluid salinity during amphibole formation (Fig. 6). The decreasing Cl concentrations in scapolite with increasing distance to the shear zone (Fig. 6) could be an indicator of changing salinity, but the capability of using scapolite as a fluid probe for NaCl concentrations is limited. Ellis (1978) investigated the exchange equilibrium of scapolite, calcite, and fluid at 750 C and 04 GPa and formulated an equation to calculate fluid compositions from coexisting scapolite. However, the application of Ellis’ formula to natural examples has been shown to be difficult (Mora & Valley, 1989; Oliver et al., 1992; Markl & Piazolo, 1998) as it lacks corrections for pressure, temperature and CO2 activity. Although scapolite cannot be Fluid used to quantify the true XNaCl , it may display changes in fluid composition and, hence, the NaCl/CO2 ratio at constant pressure and temperature. Consequently, the observed decrease in Cl concentration in scapolite with increasing distance to the shear zone (Fig. 6) can be explained by a decreasing salinity at constant CO2 activity, or increasing CO2 activity at constant salinity. Scapolite formed early during pervasive fluid infiltration of the unaltered gabbro was in equilibrium with a shear zone bulk fluid with a certain initial NaCl/CO2 ratio, hence it shows the highest Cl concentration. Owing to the formation of this Cl-rich scapolite, the NaCl/CO2 ratio in the fluid decreases. Scapolite that forms later or further away from the shear zone will therefore contain less Cl and more CO2. In the amphibolitization zone, where scapolite is not present, amphibole is the major sink for halogens and is used as a salinity probe. Average Cl concentration in amphibole increases from 04 wt % (01 a.p.f.u.) to 11 wt % (03 a.p.f.u) with increasing distance to the Fluid shear zone. Using equation (11), calculated XNaCl increases from 022 (48 wt % NaCl) to 040 (69 wt % NaCl) (Fig. 10). In the scapolite zone Cl partitions into the solid, whereas in the amphibole zone Cl is more compatible in the fluid compared with the solid. Therefore, a different process governs salinity changes in this zone. The formation of amphibole preferentially consumes OH– over Cl– from the fluid [equation (1)]; consequently, Fluid XNaCl will increase. The formation of Cl-rich amphiboles found in other localities of lower crustal fluid–rock interaction sequences shows a similar history and was described as being the result of desiccation reactions (Kullerud, 1996; Markl et al., 1998). Hence, the controlling factor for salinity changes in the sequence is the amount of newly formed amphibole (i.e. reaction progress) and the amount of water that is consumed by this process. This desiccation reaction leads to the observed enrichment of NaCl in the fluid until the saturation point and the formation of halite in the least altered samples (Fig. 3d). It is likely that the consumption of fluid limits the alteration progress in the Langøy metagabbro. Fractionation of stable chlorine isotopes d37Cl values from the Langøy sample sequence display distinct trends towards lower d37Cl values with 316 Journal of Petrology, 2015, Vol. 56, No. 2 wt% NaCl 800 93 0.2 GPa 69 83 a [Fluid] N Cl s T (°C) n t io ra 500 u at 700 600 45 0.4 GPa [Salt] + [Fluid] decreasing alteration Markl et al. (1998) this study 400 0 0.2 0.4 0.6 0.8 1 XH2O Fig. 10. Salinity evolution of a saline fluid, calculated from amphibole composition (see text for details of the calculation). NaCl saturation lines after Driesner & Heinrich (2007); XH2 O ¼ H2O/(NaCl þ H2O). increasing distance from the shear zone (Fig. 7). The d37Cl values of amphibole from the scapolitization zone decrease from 09% in the shear zone to 0% close to the transition to the amphibolitization zone. The transition zone itself is characterized by slightly higher d37Cl values of 05%. However, in the amphibolitization zone, d37Cl values decrease constantly with distance from the shear zone, from 05 to –06% in the least altered sample. Chlorine concentrations in all altered samples are at least 25 times higher than Cl concentrations in the pristine gabbro; hence, most Cl is brought into the system by a single fluid event of constant isotopic composition causing scapolitization and amphibolitization. Therefore, observed changes in the isotopic composition of the altered samples must be related to changes in the fluid composition and variations require a fractionation process capable of changing the d37Cl value of the fluid. Two fractionation processes are discussed below, both of which can lead to the observed trend in d37Cl values and help to understand the Cl isotope system. Rayleigh fractionation Equilibrium isotope fractionation owing to different bonding energies was first observed for Cl in evaporation experiments, in which the precipitating salts have higher d37Cl values than the original saline water (Eggenkamp et al., 1995). Barnes & Cisneros (2012) described a positive correlation between d37Cl values and the amphibole content of samples from altered oceanic crust that can be explained by a fractionation of Cl isotopes between minerals, where 37Cl preferentially partitions into the amphibole. These findings are consistent with theoretical calculations based on vibration data for Cl in minerals, which estimate d37Cl values to be 2–3% higher (at 25 C) for minerals where Cl is bonded to þ2 cations (e.g. micas, amphiboles) than those where Cl is bonded to þ1 cations (e.g. halite) (Schauble et al., 2003). Although fractionation decreases with increasing temperature, calculations show that even at 300 C and higher it is still 1% between minerals. Additionally, fractionation of Cl isotopes between Cl strongly bonded in a crystal lattice and Cl– dissociated in a fluid is calculated to be of the order of 06 to 15% at 300 C depending on the bonding partner (Schauble et al., 2003). In the studied sample sequence, chlorine is primarily bonded to either þ2 cations in amphibole and biotite or þ1 cations in scapolite. Therefore, minor fractionation of Cl isotopes between Cl– dissociated in aqueous solution and different minerals is expected even at the rather high temperatures of the Bamble metasomatic event depending on the bonding partner. A direct observation of this fractionation between fluid and minerals is impossible as no suitable fluid inclusions exist in the sample sequence. However, the trends of decreasing d37Cl values with increasing distance to the shear zone (Fig. 7) may be explained by a Rayleigh fractionation model. Rayleigh fractionation will lead to an enrichment of one isotope in one phase and a simultaneous depletion of the same isotope in another phase. For example, in most cases minerals growing from a fluid preferentially incorporate heavier isotopes, leading to relative enrichment of lighter isotopes in the fluid (e.g. Eggenkamp et al., 1995; Marschall et al., 2009; Barnes & Cisneros, 2012). The general Rayleigh fractionation model can be formulated in terms of delta notation for Cl isotopes as d37 Cl ¼ ð1000 þ d37 Cli ÞF a–1 –1000 (12) where d37Cli and d37Cl are the initial and the final d37Cl values of the fluid phase, respectively, F is the fraction of Cl remaining in the fluid and a is the equilibrium fractionation factor between the phases at a given temperature. Calculations based on equation (12) are used to evaluate the role of Rayleigh fractionation and to model the isotopic evolution of the Bamble fluid. For parameterization, three a values (10005, 10007 and 10010) were approximated based on the calculations of Schauble et al. (2003) assuming a temperature of 600 C (Fig. 11). The d37Cli of the fluid can be calculated from averaged values of the bulk-rock and amphibole determined from the shear zone samples. The d37Cli values using the three a values are þ02%, 0% and –03%, respectively, and are all close to 0%. The fraction of Cl remaining in the fluid (F) is a critical parameter, which cannot be measured directly, but can be constrained in various ways. As a first assumption, F is taken as the fraction of the Cl inventory at a certain distance to the shear zone relative to the overall Cl inventory of the section. This necessarily assumes that all fluid entering the alteration sequence and the dissolved Cl are consumed. This assumption is justified by the observed desiccation of the fluid during amphibole formation in a Journal of Petrology, 2015, Vol. 56, No. 2 317 1.5 1.5 bulk rock 0.5 δ 37 Cl δ 37 Cl 0.5 0 −0.5 Rayleigh fract. based on: −1 −20 1.0 007 α= 1.00 10 α= −25 Progress of: Amphibolitization α= 1.0 00 5 Cl inventory −1.5 −2 amphibole dominated scapolite dominated 1 amphibole −15 0 −0.5 −1 Rayleigh fractionation 1 Rayleigh fractionation due to: Amphibolitization Scapolitization combination of both processes −1.5 Scapolitization −10 −5 0 distance (cm) Fig. 11. Calculated d37Cl values along the sampling transect by Rayleigh fractionation using equation (12) with varying fractionation coefficients (a) and two models to calculate the fraction of Cl (F). Model 1 (continuous lines): considering the consumption of Cl from the fluid, F is calculated from the Cl budget of the whole sequence; model 2 (dotted lines): the progress of each of the alteration reactions, F is calculated from the modal abundances of Cl-consuming minerals, amphibole and scapolite; d37Cl values of Bamble bulk-rocks (circles) and amphibole (diamonds) are shown for comparison. rock-dominated environment until halite saturation. A polynomial equation was fitted to the measured bulk Cl concentration data to calculate the inventory of Cl for various distances to the shear zone. Based on these data, the modelled Rayleigh fractionation trend shows decreasing d37Cl values (Fig. 11) with increasing distance to the shear zone in the range of measured d37Cl values and is able to explain the low d37Cl values in the amphibolitization zone. Although this simple model matches some of the observed isotopic features, some considerations need to be taken into account. As the number of mineral reactions involved in a Rayleigh process increases, the system becomes substantially more complicated. In the presented sequence, the Cl content of the fluid is mainly controlled by two reactions (scapolite and amphibole formation). The simple model presented considers only one process, a linear consumption of Cl from the fluid during pervasive reaction with the bulk solid. To obtain a more realistic case an additional model is needed that links the fraction of remaining Cl (F) to the progress of each of the mineral reactions and not only to Cl concentrations measured in the samples. Although the relative timing and rates of the two reactions are unknown, petrographical observations show that amphibole [equation (1)] always forms before scapolite [equation (3)] and is coarsened during scapolitization. Therefore, a contemporaneous formation of amphibole in the amphibolitization zone with scapolite and amphibole in the scapolitization zone is likely. In turn, this will cause consumption of Cl and H2O by the two alteration reactions simultaneously, but spatially at different places within the sequence until all fluid and Cl is consumed. The amount of Cl and H2O consumed is directly proportional to the reaction progress, which is indicated by the modal abundance of newly formed −2 −25 −20 −15 −10 −5 0 distance (cm) Fig. 12. d37Cl values in the sample sequence as calculated from contemporaneous Rayleigh fractionation (a ¼ 10010) in amphibole-dominated and scapolite-dominated parts of the alteration sequence. d37Cl values are calculated for bulk-rocks in equilibrium with the metasomatic fluid; d37Cl values of Bamble bulk-rocks (circles) and amphiboles (diamonds) are shown for comparison. minerals. The remaining fraction of Cl not incorporated in minerals (F) can then be inferred from the reaction progress, which is expressed by modal abundances of scapolite and amphibole (Fig. 3e). If we assume contemporaneous formation of amphibole and scapolite, high modal abundances of alteration minerals (amphibole in the amphibolitization zone and scapolite in the scapolitization zone) represent a high reaction progress and lead to high values of F as there is a sufficient quantity of fluid and Cl to form these alteration minerals. During formation of alteration minerals fluid and Cl will be consumed and F will decrease as there will be a lesser amount of Cl in the remaining, but decreasing amount of fluid. Consequently, the subsequently smaller abundance of alteration minerals indicates a decreasing reaction progress and gives a small number for F. By using the fraction F derived from the reaction progress, the Rayleigh fractionation model can be divided into two fractionation curves for the two specific alteration zones; that is, the amphibolitization zone and the scapolitization zone, respectively (Fig. 11). The d37Cl values of minerals calculated by the second model are in agreement with the measured d37Cl values of the bulk-rocks and amphibole in the sequence and show the same trends of decreasing d37Cl with increasing distance to the shear zone for both specific parts of the overall alteration zones (Fig. 12). Although scapolite from different samples shows no distinct trend (Fig. 7), d37Cl values agree within given uncertainties with isotope data for other minerals. Only the sample adjacent to the shear zone has an unexpectedly low value for scapolite compared with other Cl-bearing phases. Assuming a changing fluid to cause the observed trends in amphibole and biotite, a flat pattern of d37Cl in scapolite would mean that it has formed in equilibrium with a fluid of constant composition. In turn, this would argue for disequilibrium between scapolite and amphibole. The general observation that scapolite has slightly lower d37Cl values than other phases might be 10000 8000 6000 4000 2000 1 0.5 0 δ 37 Cl explained by the bonding of Cl to Na and the resulting lower equilibrium fractionation factor (Schauble et al., 2003). The Cl isotope composition of the infiltrating fluid can be calculated using realistic fractionation factors ranging from 10005 to 10010 (Schauble et al., 2003; Barnes & Cisneros, 2012). The infiltrating fluid had a d37Cl value near 0% (–03 to þ02%), which progressively decreased in value during fluid–rock interaction (to as low as –16 to –11%). The d37Cl values of marine pore fluids vary over a large range, between 0% for unchanged primary fluids and –8% for fluids that have undergone isotope fractionation at low-temperature caused by fluid–rock interaction, ion filtration or diffusion (Ransom et al., 1995; Spivack et al., 2002; Godon et al., 2004a; Bonifacie et al., 2007). The observed d37Cl values for the Bamble fluid fall within the upper bound of this range, which is consistent with the previously concluded origin as a marine pore fluid. Furthermore, the relatively high initial d37Cl value of 0% indicates a primary pore fluid that experienced little to no low-temperature alteration prior to hightemperature evolution during the Bamble metasomatic event. Journal of Petrology, 2015, Vol. 56, No. 2 Cl (µg/g) 318 −0.5 −1 −1.5 Model 1 −2 −60 Model 2 bulk rock β = 0.018 β = 0.036 −50 amphibole −40 −30 −20 −10 0 distance (cm) Fig. 13. Results of kinetic modelling of d37Cl evolution. Model 1, simple diffusion model; model 2, diffusion model including a moving boundary to consider reactive fluid flow (advection term). Significant negative d37Cl values can be observed at high b values (i.e. large kinetic fractionation between isotopes) and with a fast-moving boundary (i.e. fast alteration reactions); a b value of 0036 corresponds to a 02% fractionation of 35Cl compared with 37Cl; d37Cl values of Bamble bulk-rocks (circles) and amphiboles (diamonds) are shown for comparison. sample sequence. Using a time-independent numerical solution for Fick’s second law Kinetic fractionation Diffusion-related processes are well known to cause variations in isotopic ratios of different isotopic systems (e.g. Li, Ca, Mg; DePaolo, 2004; Richter et al., 2006; Teng et al., 2006; Dohmen et al., 2010; John et al., 2012). Owing to mass-related differences in their diffusion coefficients (D), lighter isotopes travel faster in liquid and solid media than heavier isotopes of the same element (Richter et al., 2006). This kinetic fractionation is large for isotopic systems with large relative mass differences (i.e. H, Li). For the Cl system, experimental investigations show variations in d37Cl values of several per mil depending mainly on concentration gradients and temperature (Eggenkamp & Coleman, 2009). Comparison of experimentally derived fractionation factors (Dlight/Dheavy) with natural data shows good agreement and models based on these fractionation factors give reasonable results for low-temperature systems (0–80 C) of salt and brine migration (Eggenkamp et al., 1994; Eggenkamp & Coleman, 2009; Amundson et al., 2012). Unfortunately, fractionation factors for hightemperature applications are lacking. Although diffusion coefficients of elements and species are highly dependent on temperature, calculated fractionation factors for Cl isotopes (i.e. the ratios of diffusion coefficients of 35Cl and 37Cl) show little temperature dependence (Desaulniers et al., 1986; Eggenkamp et al., 1994; Eggenkamp & Coleman, 2009). Therefore, fractionation data from low-temperature experiments might be used in principle to model high-temperature processes, such as for the Bamble metasomatic event. A numerical diffusion model was set up to validate a possible kinetic fractionation of Cl isotopes in our dc d2 c ¼D 2 dt dx (13) (where D is diffusion coefficient, c is concentration and x is distance), for each of 35Cl and 37Cl, we calculated the d37Cl value and the Cl concentration as the ratio and the sum of both isotopes, respectively, within the same run. As the model is not used to obtain any time constraints, the ratios of the diffusion coefficients (given by the fractionation factor) rather than their actual values are relevant. Therefore, D37 was calculated for various fractionation factors from the literature (Richter et al., 2006; Eggenkamp & Coleman, 2009). The kinetic fractionation model was defined using the measured Cl concentration in unaltered gabbro (using a d37Cl value of –01%), the measured Cl concentration in the most strongly altered gabbro sample (using a d37Cl value of 08%) and a profile length of 06 m. After modelling concentrations of each of the isotopes, d37Cl values were obtained by the standard formulation relative to the seawater standard (37ClSW/35ClSW ¼ 0319766; Shields et al., 1962; Godon et al., 2004b). The results of this simple model show that for the given parameters kinetic fractionation would lead to decreasing d37Cl values from 08 to –1% for a fractionation factor of 1002 (Fig. 13); that is, the lighter 35Cl isotope is 02% enriched over the heavier 37Cl. Generally, b values, which are empirically derived from the expression D1/D2 ¼ (m2/m1)b, are used to describe the magnitude of kinetic fractionation. In our case, a fractionation factor of 1002 corresponds to a b value of 0036 (as used in Fig. 13), if only Cl– is considered, or 0059 if the species NaCl is considered to be the moving species. Journal of Petrology, 2015, Vol. 56, No. 2 A more realistic model that considers an advective flow 10 times higher than the diffusive flow by computing numerically a moving boundary produces slightly more negative d37Cl values (Fig. 13). Although the modelled kinetic fractionation is able to produce d37Cl values similar to those observed in the Bamble sequence, several points argue against a purely kinetic fractionation process for the Bamble setting, as follows. 1. Concentration and d37Cl values must be modelled simultaneously (Eggenkamp & Coleman, 2009); consequently, both calculated concentration and d37Cl values must fit to the measured concentration and d37Cl values at each point of the natural sequence. With kinetic fractionation, we are only able to fit either the Cl concentration or d37Cl value. 2. As kinetic fractionation is a continuous process, it cannot produce the two trends (decreasing d37Cl values in scapolitization and amphibolitization zone) observed in the sequence (Fig. 7). 3. The observed salinity evolution showing highest NaCl concentration in the least altered gabbro argues against a purely diffusion-controlled process of Cl fractionation, because concentration gradients in Cl would lead to diffusion in the opposite direction. Nevertheless, kinetic fractionation may be a process that causes negative d37Cl values in other geological settings, also at elevated temperatures. For the studied system, it seems likely that the negative trends of d37Cl with increasing distance to the shear zone are dominantly caused by a Rayleigh fractionation-like process in a rather static system. Consequently, reaction rates must be slower than the rate of pervasive fluid ingress, but still fast enough to ensure observed fluid evolution during progressive fluid–rock interaction. Additional fractionation of Cl isotopes by a kinetic process would be capable of enhancing the calculated Rayleigh fractionation, so that the effect of each of the fractionation mechanisms could be smaller. This would allow the application of smaller fractionation factors to our calculations. The exact contribution of each fractionation process to the overall fractionation is not known, but depends on the complex interplay of mineral reaction rates and diffusion rates. Implications for using halogens and stable Cl isotopes to decipher fluid–rock interaction and fluid-source systematics Contrary to what was initially expected (John et al., 2010, 2011; Selverstone & Sharp, 2013), halogen concentrations and also d37Cl values do not behave fully conservatively during fluid–rock interaction. Smallscale heterogeneities develop adjacent to the major fluid pathways, which reflect large variability in the halogen signal on a centimetre to decimetre scale. Halogen concentrations and ratios in solids that have undergone fluid–rock interaction depend strongly on mineral-specific distribution coefficients between fluid and mineral. These are highly variable; hence different 319 minerals (e.g. amphibole, mica, scapolite, apatite) will show different halogen ratios (Fig. 9). Consequently, changes in the bulk halogen ratios of rocks may be due to changes in the abundance of halogen-bearing phases and not necessarily caused by changes in the halogen source. Using halogen ratios as a fingerprint of fluid sources can, therefore, be applied only with knowledge of the complete alteration history of the rock. Chlorine isotopes are less affected by inter-mineral fractionation factors than by Rayleigh and kinetic fractionation during fluid–rock interaction, as shown here and previously argued from fluid inclusion data by Gleeson & Smith (2009). For other isotopic systems (e.g. Li, B, Fe, Mg), it has been shown that fractionation processes are able to change d values over a large range (Teng et al., 2006; Marschall et al., 2007a, 2007b; Li et al., 2010; Penniston-Dorland et al., 2010; John et al., 2012). For example, Marschall et al. (2007b) argued that low d7Li values recorded in eclogites are the result of kinetic fractionation during diffusive influx of light Li from country rocks and measured d7Li values are not representative for the major rock type. Dynamic processes such as fluid flow, fluid–mineral reactions and diffusion govern these systems and have major impacts on the behaviour of stable isotopes and thus the measured d values of the rock. The data presented here and modelled fractionation processes also suggest a similar dependence on dynamic factors for the Cl isotope system. In fact, it may explain partly the large spread observed for the various Cl reservoirs (Barnes & Sharp, 2006; Sharp et al., 2007; Bonifacie et al., 2008; John et al., 2010; Selverstone & Sharp, 2011), especially in those affected by fluid–rock interactions. Our results have ramifications for sampling strategies. If samples are taken for reservoir studies, it is important to know the history and geometry of fluid–rock interaction in the sample area. Sampling should cover a large volume, preferably far away from any fluid pathways, to avoid or integrate over possible alterations (Fig. 14). However, alteration processes will always introduce a certain bias in d37Cl values. For studies concerning fluid flow and fluid evolution the sampling target is shifted towards fluid pathways (Fig. 14). To learn about the effects of the fluid on the wall-rock system sampling should be perpendicular to the flow structure, but if the interest is set more on the evolution of the fluid, sampling along the fluid-dominated systems (veins or shear zones) is essential. SUMMARY AND CONCLUSIONS Halogen concentrations and ratios can be powerful tools in the investigation of metasomatic settings, if careful sampling is applied. They can be used to trace fluid sources and fluid–rock interaction processes. Halogen source studies might be easily affected by a sampling bias of rock prone to fluid–rock interaction. In the Bamble area, the halogen concentrations and ratios (e.g. Br/Cl, I/Cl) of the scapolitized samples suggest that 320 Journal of Petrology, 2015, Vol. 56, No. 2 δ37Cl +1 ‰ δ37Cl 0‰ δ37Cl -1 to +1‰ 0‰ from -1 to +1 ‰ pristine gabbro +1 ‰ metagrabbro in shear zones - progressive alteration reactions - δ37Cl fractionation Fig. 14. Schematic illustration (not to scale) of fluid flow in the Bamble metagabbros. Isotopic fractionation owing to intense fluid–rock interaction causes centimetre- to decimetre- scale heterogeneities in d37Cl values where fluid flow is pervasive. fluids most probably originated from marine pore fluids and marine sediments during prograde metamorphism of their host-rocks. Remobilization of meta-evaporites or a mantle source for these fluids for the Bamble area can be excluded as these sources have very different halogen ratios. The altered metagabbro sequence shows how mineral formation was able to cause significant changes in the halogen chemistry of the involved fluid. Assuming that a brine (48 wt % NaCl) pervasively infiltrated the unaltered gabbro first, the subsequent formation of Clrich scapolite caused a decrease of the fluid salinity. The formation of amphibole during continuing fluid ingress led to increasing salinity owing to desiccation of the fluid until all fluid was consumed and the alteration process was terminated. The most evolved fluid, coexisting with the least altered gabbro, reached Cl saturation as indicated by halite formation. Journal of Petrology, 2015, Vol. 56, No. 2 321 Both the pristine gabbro and infiltrating fluid had similar d37Cl values, close to 0%. High d37Cl values of samples and mineral separates from close to the shear zone can be explained by equilibrium fractionation of Cl isotopes between fluid and alteration phases formed by reaction of the wall-rock with this fluid. Decreasing d37Cl values with increasing distance to the shear zone originate from fractionation of Cl isotopes caused either by pure Rayleigh fractionation or a combination of Rayleigh and kinetic fractionation. 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