Introduction
Titano- and zirconosilicates are typical phases constituting the mafic mineral assemblages of highly peralkaline SiO2-undersaturated and -oversaturated rocks and contribute to the chemical budget of the high-field-strength elements (HFSE), the rare earth elements (REE) and Y during the evolution of these systems in both the magmatic and post-magmatic crystallisation stages. Furthermore, mineral assemblages and compositions may give relevant clues to access the main intensive parameters of these crystallisation environments, as well as the alkalinity and volatile fugacities in the magma (e.g. Nichols and Carmichael, Reference Nicholls and Carmichael1969; Marks et al., Reference Marks, Hettmann, Schilling, Frost and Markl2011; Andersen et al., Reference Andersen, Erambert, Larsen and Selbekk2010; Siachoque et al., Reference Siachoque, Vilalva and Vlach2022).
Among the known titanosilicates, narsarsukite is a relatively rare inosilicate with the IMA accepted formula Na2(Ti,Fe3+)Si4(O,F)11, crystallising in the I4/m space group (e.g. Anthony et al., Reference Anthony, Bideaux, Bladh and Nicchols2003). It was first described in a pegmatite from Narsarsuk, Greenland, by Flink (Reference Flink1901) and its crystal structure was determined by Pyatenko and Pudovkina (Reference Pyatenko and Pudovkina1960) and Peacor and Buerger (Reference Peacor and Buerger1962). Recently, Schingaro et al. (Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017) revisited the narsarsukite structure and suggested the extended formula Na4{Ti1–x4+,Mx 3+)[O1–x(OH,F)x]}2(Si8O20) with 0 < x ≤ 1. The structure is composed of 4-periodic double chains of [Si4O10]2 tetrahedra connected into tubes and to chains of corner-sharing Ti(O5,OH,F)-octahedra. The tubes are parallel to the c-axis, and the 7-coordinated Na+ cations are located in the cavities between the tubes and the octahedral chains. According to the structure hierarchy of the chain-, ribbon- and tube-silicates developed by Day and Hawthorne (Reference Day and Hawthorne2020), based on the connectedness of one-dimensional polymerisation of the (TO4)n – tetrahedra, the narsarsukite structure belongs to the 3T8 group. This means that the connectivity of the [SiO4]4– tetrahedron has a value of 3 and the number of these tetrahedra is 8 in the repeat structural unit.
Narsarsukite occurs in several volcanic and plutonic, mainly SiO2-oversaturated, peralkaline rocks, pegmatites and hornfels. It is associated commonly, in addition to quartz and alkali-feldspars, with aegirine, arfvedsonite, pectolite, various titanosilicates, such as aenigmatite, astrophyllite, neptunite and bafertisite, and zirconosilicates, such as elpidite (e.g. Birkett et al., Reference Birkett, Trzcienski and Stirling1996; Siachoque et al., Reference Siachoque, Vilalva and Vlach2022).
The main crystallochemical features of narsarsukite are well-established in the mineralogical literature (e.g. Wagner et al., Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991; Read, Reference Read1991; Birkett et al., Reference Birkett, Trzcienski and Stirling1996; Schingaro et al., Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017). Wagner et al. (Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991) discussed infrared and Mössbauer spectroscopic results, whereas Schingaro et al. (Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017) provided micro-Fourier transform infrared and X-ray photoelectron spectroscopy data. Eu3+-doped narsarsukite was synthesised by the sol-gel method (e.g. Balmer et al., Reference Balmer, Bunker, Wang, Peden and Su1997) and was shown to have luminescence properties (Rainho et al., Reference Rainho, Lin, Rocha and Carlos2003).
Notwithstanding the wealth of data available on narsarsukite, there is a paucity of systematic studies that combine textural and compositional features, particularly those comparing the characteristics of magmatic and post-magmatic crystallisation generations. These are relevant aspects to consider, as more than one textural generation of the mafic minerals (e.g. magmatic vs. hydrothermal) is common in peralkaline rocks (e.g. Siachoque et al., Reference Siachoque, Vilalva and Vlach2022). Additionally, although some electron microprobe data for Y and Ce have been made by Read (Reference Read1991) and Birkett et al. (Reference Birkett, Trzcienski and Stirling1996), REE data are still scarce and complete analyses exist only for peralkaline granites from the Strange Lake Complex (Vasyukova and Williams-Jones, Reference Vasyukova and Williams-Jones2019).
Narsarsukite is a common and widespread accessory mineral in the strongly peralkaline alkali-feldspar granites of the Papanduva Pluton, Morro Redondo Complex, in the Neoproterozoic A-type Graciosa Province, south-southeastern Brazil (Gualda and Vlach, Reference Gualda and Vlach2007). This work presents and discusses textural and compositional data (major, minor and trace elements) for magmatic and post-magmatic narsarsukite generations. We also examine the behaviour of REE in this mineral and contribute to the mineralogical knowledge of the province and similar occurrences worldwide.
The Papanduva Pluton
The Papanduva Pluton, with ~60 km2 and irregular surface contours (Fig. 1), is a peralkaline intrusion of the Morro Redondo Complex in the Neoproterozoic (ca. 580 Ma) Graciosa Province, south-southeastern Brazil (Gualda and Vlach, Reference Gualda and Vlach2007; Vlach et al., Reference Vlach, Siga, Harara, Gualda, Basei and Vilalva2011; Vilalva and Vlach, Reference Vilalva and Vlach2014; Vilalva et al., Reference Vilalva, Simonetti and Vlach2019). The pluton is composed of slightly greyish hypersolvus holo- to leucocratic alkali-feldspar granites showing significant variations in structure, texture and mineralogy. These variations have been grouped and mapped as massive, cataclastic, and foliated fine-, medium- and coarse-grained petrographic facies, accompanied by some microgranites. See Vilalva (Reference Vilalva2007), Vilalva and Vlach (Reference Vilalva and Vlach2014) and Vilalva et al. (Reference Vilalva, Vlach and Simonetti2016) for detailed petrographic descriptions and textural and compositional characterisation of the rock-forming felsic and mafic minerals. The granites are highly ferroan [FeOT/(FeOT+MgO) ≥ 0.96], and have SiO2 contents of 74–78 wt.% and Na2O+K2O contents of 8.9–9.3 wt.%. The peralkaline index [(Na2O+K2O)/Al2O3 molar] is between 1.04 and 1.28, and the HFSE contents are relatively high, up to 2430 ppm (Vilalva and Vlach, Reference Vilalva and Vlach2014).
The most evolved and highly peralkaline foliated facies (Fig. 2) have sub-magmatic, close-to-solidus, deformational structures with variable intensity. They have a fine- to medium-grained porphyroclastic to protomylonitic textures, with orientated and deformed megacrysts of mesoperthite, arfvedsonite and quartz in a fine-grained, sometimes saccharoidal, matrix with alkali-feldspars (microcline and albite), quartz and mafic minerals. Millimetric miarolitic cavities or vugs (partially filled with accessory phases) occur in some samples. In most hand samples, yellowish minerals (mainly narsarsukite and zirconosilicates) can be seen. The accessory and rare phases include earlier-, late- and/or post-magmatic generations of aenigmatite, astrophyllite, narsarsukite, elpidite and other unidentified zirconosilicates of Na and K, neptunite, britholite-(Ce), nacareniobsite-(Ce), turkestanite, bastnäsite-(Ce), allanite-(Ce), titanite, anatase, together with fluorite and several unidentified phases (see Vilalva and Vlach, Reference Vilalva and Vlach2010, Vilalva et al., Reference Vilalva, Vlach and Simonetti2013; Siachoque et al., Reference Siachoque, Vilalva and Vlach2022). Siachoque et al. (Reference Siachoque, Vilalva and Vlach2022) present an interpretation for the relative sequence of crystallisation of these minerals based on textural evidence. Narsarsukite is the most abundant rare accessory mineral in these rocks, reaching up to 3.2 vol.%.
Samples and analytical procedures
The analytical work was carried out at the GeoAnalitica facility, Institute of Geosciences, University of São Paulo. After conventional petrographic analysis, seven samples from the foliated facies were chosen for major, minor and some trace-element analysis with the electron microprobe analyser (EMPA). Three of these samples were further analysed for trace elements using laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS). The locations of the samples are shown in Fig. 1.
Electron microprobe analyses
Electron microprobe analyses were performed using the JEOL-JXA8600S and JEOL JXA-FE8530 electron microprobes. The latter instrument is equipped with a field emission electron gun. Both these instruments have five wavelength dispersive (WD) and one energy dispersive (ED) spectrometers. Quantitative WDS spot analysis was performed with the JEOL-JXA8600S equipment, and compositional mapping was obtained using a combination of WDS and EDS signals with the JEOL JXA-FE8530 equipment. The WDS analytical conditions were 15 kV, 20 nA and 5–10 μm for the column accelerating voltage, beam current and diameter, respectively. The analytical routine is summarised in Supplementary Table S1. Fluorine and Na were measured simultaneously in the first spectrometric round to minimise their loss. The matrix effect correction and conversion of the raw data to mass oxides were performed using PROZA software (Bastin and Heijligers, Reference Bastin and Heijligers1990). The analytical errors, checked against standards readings, are lower than 2% relative for the major, between 5 and 10% relative for the minor, and higher for trace elements. Back-scattered electron (BSE) images and compositional maps were obtained with a focused beam and the same analytical conditions. The dwell time for maps was set to 50 ms.
Literature data suggest that Fe in narsarsukite occurs mainly as Fe3+ (Wagner et al., Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991; Birkett et al., Reference Birkett, Trzcienski and Stirling1996; Schingaro et al., Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017). Its structural formula has been alternatively computed considering seven total cations or 11 (O+F). The first scheme does not account for potential vacancies in the Na site (Wagner et al., Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991) and might result in some excess in the Si and Ti sites in addition to in the O site, and the second scheme does not allow for the possible entry of (OH)1– anions in the structure. Considering these drawbacks, we computed the structural formulae according to both approaches. We used the first scheme for the analytical data to better examine the substitution of O2– by F–1 in the O sites.
Laser ablation inductively coupled plasma mass spectrometry analysis
Laser ablation inductively coupled plasma mass spectrometry analysis was performed using Quadrupole Elan 6100DRC equipment from Perkin Elmer coupled with a UP-213 laser ablation system from NewWave Research, provided with a 213 nm Nd-doped YAG laser, following the procedures described in Andrade (Reference Andrade2016). The analyses were carried out in raster mode with spot sizes varying from 30 to 50 μm. Back-scattered electron images were used to guide the selection of areas to be analysed.
The laser beam fluence and repetition rate were set at 8.5 J/cm2 and 4 Hz, respectively. The following isotopes were measured: 7Li, 9Be, 25Mg, 31P, 42Ca, 45Sc, 49Ti, 51V, 52Cr, 55Mn, 59Co, 65Cu, 66Zn, 69Ga, 85Rb, 88Sr, 89Y, 90Zr, 93Nb, 95Mo, 118Sn, 133Cs, 137Ba, 139La, 140Ce, 141Pr, 143Nd, 147Sm, 151Eu, 155Gd, 159Tb, 163Dy, 165Ho, 166Er, 169Tm, 173Yb, 175Lu, 179Hf, 181Ta, 208Pb, 232Th and 238U. The total acquisition time was set to 120 s, distributed equally between blank and ion signal measures. The signal integration and dwell times were 8.33 and 1.66 ms, respectively. The daily rate of oxide generation was controlled holding ThO+ formation below 1%. Glitter software (Griffin et al., Reference Griffin, Powell, Pearson, O'Reilly and Sylvester2008) was used for data acquisition, treatment, and conversions to concentrations. The synthetic NIST glass SRM-610 and the average TiO2 content previously measured by WDS were used as external and internal standards, respectively.
Regardless of our efforts, reliable quantitative trace-element data for the post-magmatic narsarsukite generation was considerably more difficult to acquire. This is because of the small dimensions of the crystals, their common lamellar or fibrous habit, and their close association with arfvedsonite and aegirine. We were only able to obtain two reliable analyses, which were for crystals replacing arfvedsonite. Most of the other analyses were discarded as the measured Ca and Mg contents were relatively high, well above 400 and 300 ppm, respectively, and thus were considered to be mixed, non-representative values.
Results
Textural features
Two generations of narsarsukite were identified on the basis of their textural and compositional features. The most typical characteristics of each generation, as observed under the petrographic microscope, are shown in Fig. 3.
The first generation occurs as interstitial euhedral to subhedral (1–2 mm long) crystals formed during the late-magmatic crystallisation stage and show some textural features similar to those described for narsarsukite in the Strange Lake granites (Birkett et al., Reference Birkett, Trzcienski and Stirling1996). These crystals have platy to tabular habits (a >> c) with high relief and second-order birefringence colours, with a weak colourless to pinkish pleochroism. Most larger crystals are zoned, with pinkish colours, high birefringence in their cores, and almost colourless and lower birefringence rims (Fig. 3a–d). Some crystals have a relatively homogenous and clean core surrounded by an intermediate poikilitic zone populated with a significant number of minute inclusions and a thin clean rim (Fig. 3a,b; cf. also Fig. 4). Deformed (bent and with some translational slip features) crystals are common (Fig. 3c). These crystals are very susceptible to alteration and several samples have been replaced by tiny brownish aggregates composed of late alteration minerals, including titanite, bastnäsite, phyllosilicate minerals and other unidentified phases. A remarkable texture observed in interstitial and relatively smaller crystals and in the intermediate and sometimes the rim zones of larger crystals, is a poikilitic intergrowth between narsarsukite and euhedral to subhedral albite laths (Fig. 3e).
The second generation consists of tiny crystals (≤ 1 mm long) with subhedral, lamellar and fibrous habits and seems to be less susceptible to late alteration. They occur mainly as minute inclusions in recrystallised quartz rims, as isolated crystals or crystal aggregates developed along the contacts between the other minerals (Fig. 3f), along fractures and cleavage planes of arfvedsonite and aegirine (Fig. 3g,h) or as irregular aggregates within arfvedsonite (Fig. 3i). The observed textural relationships, particularly those shown in Fig. 3h,i indicate that this generation replaces previous arfvedsonite and possibly aegirine.
A back-scattered electron image and qualitative compositional maps for Ti, Zr, Al, Fe and Nb for the magmatic crystals depicted in Fig. 3a,b are presented in Fig. 4. The images show the main zoning pattern observed in most large narsarsukite crystals, with relatively Zr- and Nb-rich and Fe- and Al-poor crystal cores. The poikilitic intermediate and the external rim crystalline zones are almost Zr-free. Furthermore, some areas have irregular Fe and Nb (sectorial?) zoning. The high-Zr and low-Ti phase intergrowth with narsarsukite in the intermediate poikilitic zone is an unidentified zirconosilicate with some Na and K, as determined from EDS qualitative analysis. This intergrowth might alternatively represent the co-precipitation of narsarsukite and a zirconosilicate still in the magmatic stage, indicating the saturation of alkali-bearing zirconosilicates in the melt or fluid-induced post-magmatic exsolution of the Zr-rich phase leaving a Zr-poor narsarsukite host. The most external and Ti-, Al-rich zones might represent late- to post-magmatic overgrowths.
Compositions and variability
Representative compositions for magmatic and post-magmatic narsarsukite are given in Tables 1 (WDS) and 2 (LA-ICP-MS). The complete dataset is given in Supplementary Tables S2 and S3, including structural formulae computed on the basis of seven cations and 11 (O+F) for the WDS data, and analytical errors and average standard readings (SRM-610 and SRM-612, from NIST, and BCR-2G, from USGS) used for analytical control for the LA-ICP-MS data.
* All Fe as Fe2O3; n.d. = not detected; 1= magmatic, 2 = post-magmatic; c = core, i = intermediate and r = crystalline rim zones; pk = poikilitic, ra = replacing arfvedsonite. See also Supplementary Table S2.
MR-02A, MR-06 and MR-21 = magmatic; MR-2A(*) = post-magmatic, replacing arfvedsonite. n.d. = not detected; n.a. = not analysed. See also Supplementary Table S3.
The most significant compositional variations are observed for Zr, Al, Fe3+ and Nb, all of which occupy the octahedral [Ti]-site. The contents (wt.%) of ZrO2, Al2O3, Fe2O3 and Nb2O5 vary in the ranges 5.95–0.28, 0.96–0.39, 7.24–3.75, 1.21–0.08, respectively, in the magmatic narsarsukite, and in the ranges 0.27–0.00, 3.10–0.50, 7.42–4.17, 0.76–0.00, respectively, in the post-magmatic narsarsukite. The magmatic generation is richer in Zr and, on average, poorer in Al compared to the post-magmatic generation. Among the divalent cations, MnO has concentrations lower than 0.12 and is higher in magmatic crystals. BaO and CaO are lower than 0.16, and their contents lie in similar ranges in both generations, whereas K2O is ≤ 0.15 (all quantities in wt.%).
The variations of Al and Fe3+ with Zr are shown in Fig. 5a. A slight decrease of both Al and Fe3+ with increasing Zr is observed in the compositional zoning of the larger crystals of the magmatic generation. These compositional relationships strongly support the textural interpretations that indicate two contrasted crystallisation generations. In addition to its higher contents, Al also has a significantly wider variation range in the post-magmatic crystals. The Al/Fe3+ ratio is a suitable variable to discriminate between narsarsukite generations in the Papanduva Pluton, being almost constant around 0.2 in the magmatic generation and between 0.2 and 1.2 in the post-magmatic generation. Notably, Al and Fe3+ contents show a positive correlation in the magmatic crystals, but a negative correlation in the post-magmatic crystals (Fig. 5b). The Fe3+ contents in narsarsukite reached maximum values at the transition between the magmatic and post-magmatic crystallisation stages. In the first case, Al and Fe3+ increase at an almost constant ratio of 1:4, a feature observed in all larger and zoned analysed crystals. In the second case, Al increases and Fe3+ decreases in a proportion close to 1:1.
In addition to the homovalent substitutions of Ti by Zr and Fe3+ by Al, the entry of trivalent cations in the narsarsukite structure is described by the heterovalent substitutions 2R4+ = R3++ R5+ (1) and R4++ O2– = R3+ + F1– (2), where R3+, R4+ and R5+ mainly represent (Al, Fe3+), (Ti, Zr) and Nb, respectively (Wagner et al., Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991; Birkett et al., Reference Birkett, Trzcienski and Stirling1996; Schingaro et al., Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017). These substitutions are plotted in Fig. 6. Wagner et al. (Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991) also suggested that the substitution R4+ + 2O2– = R2+ + 2F–1 accounts for the entry of divalent cations (Mn, Mg, Ca and Ba), which occur in much lower concentrations in our samples (see Tables 1 and S2). Reaction (1) gives an excellent negative correlation for our dataset, with a determination coefficient R 2 = 0.93 (Fig. 6a). However, it plays a minor role in the entry of the R3+ cations, as the Nb contents are much lower (≤ 0.036 atoms per formula unit, apfu) than Al and Fe3+, which sum up to 0.456 apfu. Thus, reaction (2), for which we only obtained a moderate negative correlation with a slope of –1.19 and R 2 = 0.61 (Fig. 6b), is by far the most important in explaining the observed compositional variations. There are no significant and systematic variations in F or Nb between the magmatic and post-magmatic generations and the higher values of R3++F1– plotted in Fig. 6b reflect mainly the higher quantities of Al+Fe3+ in post-magmatic narsarsukite. The data points have a significant dispersion in this diagram and the slope departs from the ideal value of –1. These features are in part due to the non-consideration of some R3+ cations, such as the REE and Y, however it is most probably due to the entry of variable contents of (OH)–1 anions in the O site, according to the extended narsarsukite formula suggested by Schingaro et al. (Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017).
The magmatic and post-magmatic narsarsukite compositions from the Papanduva Pluton are compared in the ternary Fe3+–Al–Zr diagram (Fig. 7) with those of other important worldwide occurrences, which includes peralkaline SiO2-oversaturated rocks, an alkaline pegmatite from Narsarsuk, the type locality, and hornfels associated with SiO2-undersaturated rocks (nepheline syenites). They show an extensive variation range that overlaps with most of the available compositions. For example, the magmatic narsarsukite from Papanduva has almost as much Zr as narsarsukite in comendite from the Sirwa Massif, near Ouarzazate (Southern Morrocco), the occurrence with the highest Zr contents reported to date (Wagner et al., Reference Wagner, Parodi, Semet, Robert, Berrahma and Velde1991). In contrast, the post-magmatic Papanduva narsarsukite can have almost as low Fe3+ contents as the specimen in the Illutalik trachyte dyke (Upton et al., Reference Upton, Macdonald, Hill, Jefferies and Ford1976), from Illutalik (formerly spelled Igdlutalik) Island, Kujalleq (Greenland). The narsarsukite from lamprophyre dykes of the Murun Massif (Aldan Shield, Russia) has the highest and lowest known Fe3+ and Al contents, respectively (Schingaro et al., Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017), whereas the specimen in comendites/pantellerites and related vugs from Mayor Island (New Zealand) present relatively high Zr contents for given Al values (Read, Reference Read1991). The Papanduva magmatic narsarsukite has a similar compositional trend to the peralkaline granites from the Strange Lake in northern Québec–Labrador, Canada (Birkett et al., Reference Birkett, Trzcienski and Stirling1996), though with relatively lower Nb and Al and higher Fe3+ contents on average. The cores of the largest crystals also have higher Zr contents.
Trace elements
The most abundant trace elements in narsarsukite are the HFSE, Y and the mid to heavy rare earth elements (MREE–HREE), whereas the LILE (large-ion lithophile element) contents are low. In Fig. 8a, we plot selected trace elements normalised to the host rocks for samples MR-2A (magmatic and post-magmatic generations) and MR-21 (magmatic). The post-magmatic narsarsukite from sample MR-2A has higher Ba and light rare earth element (LREE) contents and lower HREE and Hf contents than the magmatic narsarsukite. Tantalum was not plotted in the diagram due to data unavailability for the host rocks, however its abundances range from 38 to 500 ppm and 64 to 268 ppm in magmatic and post-magmatic crystals, and its behaviour closely follows Nb (cf. Tables 2 and S3).
The total REE and Y contents of primary narsarsukite range between 505–2353 and 473–2169 ppm, respectively. The post-magmatic crystals have lower contents, ranging from 910–864 ppm (MR-02A) and 602–2165 ppm (MR-06), respectively. The REE patterns of the magmatic generation (Fig. 8b) show high fractionation of the HREE over the LREE and within the HREE and the LREE, with average CeN/YbN, CeN/SmN and GdN/YbN ratios of 0.003, 0.295 and 0.031, respectively, and a strong negative Eu anomaly, with an average Eu* [=EuN/(SmN*GdN))0.5] = 0.09. The post-magmatic crystals have a relatively flat distribution pattern, with a similar Eu anomaly. The average data for the Strange Lake narsarsukite (Vasyukova and Williams-Jones, Reference Vasyukova and Williams-Jones2019) is also plotted in Fig. 8b for comparison. This shows considerably higher total REEs and Y (averaging 14,453 and 4872 ppm, respectively), with a significant high-fractionated average pattern and a less pronounced negative Eu anomaly.
Discussion and final remarks
Textures and compositions of narsarsukite
Narsarsukite is a common accessory in strongly peralkaline granites from the Papanduva Pluton. It formed both in the magmatic and the post-magmatic crystallisation environments. Late-magmatic, relatively larger and compositionally zoned crystals were followed by poikilitic intergrowths between narsarsukite and albite formed in the latest melt pockets. Similar aegirine + albite, arfvedsonite + albite, and aenigmatite + albite intergrowths occur in the Papanduva Pluton. The albite laths within these intergrowths are almost pure (Ab ≥ 98% molar) and have significantly high Fe2O3 contents (Vilalva, Reference Vilalva2007). These intergrowths suggest co-precipitation of these phases and closely resemble the so-called khibinitic texture typical of the SiO2-undersaturated eudialyte-bearing, agpaitic, nepheline syenites (khibinites, e.g. Gerasimovsky et al., Reference Gerasimovsky, Volkov, Kogarko, Polyakov and Sørensen1974; Ulbrich and Ulbrich, Reference Ulbrich and Ulbrich2000). Therefore, albite (as an Al2O3-saturated phase) stabilised at the end of the magmatic crystallisation. Conversely, the fibrous narsarsukite crystals or crystals aggregates that appear interstitially or replace arfvedsonite and aegirine are typically post-magmatic (hydrothermal).
The Papanduva narsarsukite covers the compositional range for Fe3+, Al and Zr described in the literature. A well-defined Fe3+ inflection marks the compositional limit between the magmatic and the post-magmatic generations, with the latter being Zr-poor and Al-rich. This inflection reflects that Fe3+ was less available in the fluids and preferentially partitioned into other Fe3+-bearing phases, such as aegirine (cf. below). The increasing contribution of Al-bearing late fluids also contributed to this inflection. The relative proportions for the main R4+, R3+ and R5+ cations and O2– and F1– suggest the presence of some (OH)1– anions in the O site, in agreement with the findings of Schingaro et al. (Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017).
The narsarsukite investigated has significant total REE and Y (up to 2350 and 2170 ppm) contents. However, these contents are considerably lower than those reported for the narsarsukite in the Strange Lake Complex (Vasyukova and Williams-Jones, Reference Vasyukova and Williams-Jones2019), which also has highly fractionated REE patterns and smaller negative Eu anomalies. This difference could be due to the higher contents of HFSE and REE in the granites from Strange Lake, or to the occurrence of a different set of accessories competing for the REE and Y. The REE and other R3+ cations enter the six-fold coordinated [Ti]-site, which is significantly distorted in narsarsukite (Schingaro et al., Reference Schingaro, Mesto, Lacalamita, Scordari, Kaneva and Vladykin2017). The effective ionic radii (Shannon, Reference Shannon1976) of VITi4+ is 61 pm, and this explains the increasing preference for the smaller HREE in this site. However, even VILu3+, the smallest REE, has an effective radius (~86 pm), significantly higher than VITi4+, and this limits the maximum REE and Y contents in narsarsukite. The REE patterns obtained for the hydrothermal crystals replacing amphibole are characterised by relatively flat distribution patterns with higher LREE abundances, characteristics that are similar to those observed in hydrothermal zircon (e.g. Hoskin, Reference Hoskin2005; Vlach, Reference Vlach2022).
The replacement of arfvedsonite and aegirine by narsarsukite
The replacement of arfvedsonite and possibly aegirine by narsarsukite during the post-magmatic crystallisation stage suggests the involvement of relatively Ti-rich late fluids in the mineralogical evolution of the host granites. This is supported by the occurrence of hydrothermal Ti-minerals such as neptunite, titanite and anatase in miarolitic cavities and vugs within the granites (Vilalva, Reference Vilalva2007).
In this sense and considering idealised end-members, narsarsukite might be formed through the following replacement reactions:
and
The hydrothermal replacement of arfvedsonite by narsarsukite is probably favoured in relatively oxidising conditions. If Na metasilicate (Na2Si2O5) or a similar compound and SiO2 species are available in the fluid, aegirine will be formed preferentially instead of hematite, according to the reaction:
Importantly, the occurrence of contrasted magmatic and hydrothermal aegirine generations and hydrothermal aegirine replacing arfvedsonite are standard features in these rocks (e.g. Vilalva et al., Reference Vilalva, Vlach and Simonetti2016; Vasyukova and Williams-Jones, Reference Vasyukova and Williams-Jones2019).
The compositions of the involved primary and post-magmatic crystallising phases can be used to infer the compositional characteristics of the post-magmatic fluid. The average compositions of arfvedsonite and primary aegirine in the narsarsukite-bearing granites are given in Supplementary Table S4 (see complete data set in Vilalva et al., Reference Vilalva, Vlach and Simonetti2016). In a gain–loss diagram (Fig. 9), the replacing narsarsukite has higher contents of Be, Al, Sc, Ba, HFSE, Y, REE, Th, U and Pb, in addition to Ti, Na, Al and Si, than arfvedsonite. This suggests that the fluid phase was relatively enriched in these elements. Conversely, K, Ca, Mn, Fe and Rb were released preferentially from the amphibole to the fluid phase.
Narsarsukite in peralkaline granites and a comment on the use of the term agpaitic
Narsarsukite is a significant and widely distributed primary accessory phase in some highly peralkaline granites such as those from the Papanduva Pluton and the Strange Lake Complex. It should be included as a characteristic and diagnostic Na–Ti-bearing mineral in the assemblages of these rocks, together with other rare Ti- and Zr-minerals, such as aenigmatite, astrophyllite and elpidite.
Given the inherent difficulties and compositional complexities, experimental constraints on the crystallisation of narsarsukite and other rare Na–K–Ti–Zr-bearing phases starting from peralkaline SiO2-oversaturated compositions are rare or absent. Upton et al. (Reference Upton, Macdonald, Hill, Jefferies and Ford1976) simulated the crystallisation of a narsarsukite-bearing peralkaline trachyte under 100 MPa and saturated H2O conditions at the magnetite–hematite buffer, however narsarsukite was not observed among the products. A qualitative analysis on the relative stability of narsarsukite and other Ti-minerals for the Strange Lake case was presented by Birkett et al. (Reference Birkett, Trzcienski and Stirling1996), based on chemographic relations in the Na–Fe2+–Fe3+–Ti space.
The term ‘agpaitic’ was introduced by Ussing (Reference Ussing1912) for some nepheline syenites from the Ilímaussaq Complex (south Greenland). It is specifically recommended for peralkaline nepheline syenites containing complex Zr- and Ti-silicate minerals, with corresponding particular geochemical signatures (see also Sørensen, Reference Sørensen1960; Le Maitre, Reference Le Maitre1989). However, Vlach and Gualda (Reference Vlach and Gualda2007) used the this term to describe the mineralogy of the most evolved peralkaline granites in the Papanduva Pluton considering the widespread occurrence of titano- and zirconosilicate among the rare accessory phases. Later, Marks et al. (Reference Marks, Hettmann, Schilling, Frost and Markl2011) proposed to extend the term ‘agpaitic’ to include peralkaline granitic rocks with (K, Ti)-, (K, Zr)-, (Na, Ti)- and (Na, Zr)-bearing rare mineral assemblages such as eudialyte + aenigmatite, astrophyllite + dalyite, aenigmatite + dalyite and astrophyllite + dalyite. We agree with Marks et al. (Reference Marks, Hettmann, Schilling, Frost and Markl2011) and believe that these highly peralkaline granites, together with rhyolites, containing rare Zr- and Ti-silicate minerals might also be characterised as agpaitic to distinguish them from more common peralkaline SiO2-oversaturated rocks. However this proposal needs to be discussed further by the petrological community and is beyond the scope of this work.
Acknowledgements
The authors are grateful to staff of the GeoAnalitica facility for analytical support during laboratory work and to Fundação de Amparo à Pesquisa do Estado de São Paulo, FAPESP (Grant 2019/17343-4) for funding this research. The comments and suggestions of two anonymous referees and the Associate Editor helped to improve the manuscript and are greatly appreciated.
Supplementary material
The supplementary material for this article can be found at https://doi.org/10.1180/mgm.2023.70.
Competing interests
The authors declare none.