Introduction
Tourmaline is the most widespread borosilicate mineral in the Earth's crust, typically occurring in granites and granite pegmatites as well as in sedimentary and metamorphic rocks (van Hinsberg et al., Reference van Hinsberg, Henry and Dutrow2011a, Reference van Hinsberg, Henry and Marschall2011b; Dutrow and Henry, Reference Dutrow and Henry2018; Henry and Dutrow, Reference Henry and Dutrow2018). The compositional complexity of this mineral arises from its general formula, which can be written as XY3Z6T6O18(BO3)3V3W, where X = Na+, K+, Ca2+, □ (= vacancy); Y = Mg2+, Fe2+, Mn2+, Li+, Al3+, Fe3+, Cr3+, V3+, Ti4+; Z = Al3+, Fe3+, Cr3+, V3+, Mg2+, Fe2+; T = Si4+, Al3+, B3+; B = B3+; V = (OH)–, O2–; and W = (OH)–, F–, O2–.
Due to the occurrence of an extensive short-range order, which can impose extremely slow diffusion rates of the constituents in the structure, tourmalines can, once formed, retain their original composition (e.g. Hawthorne and Dirlam, Reference Hawthorne and Dirlam2011; van Hinsberg et al., Reference van Hinsberg, Henry and Dutrow2011a, Reference van Hinsberg, Henry and Marschall2011b; Bosi, Reference Bosi2018). Thus, they are able to preserve the chemical-physical variation of the crystallisation environment during crystal growth (e.g. Agrosì et al., Reference Agrosì, Bosi, Lucchesi, Melchiorre and Scandale2006). Moreover, the extensive P−T stability range of tourmalines make them an efficient geological tool for investigating P−T−X conditions in all crustal settings within the Earth (van Hinsberg et al., Reference van Hinsberg, Henry and Dutrow2011a, Reference van Hinsberg, Henry and Marschall2011b). As a result, tourmaline is an excellent petrogenetic indicator that can provide information about the formation and evolution of complex crystals over time, acting as a ‘geologic DVD’ (Dutrow and Henry, Reference Dutrow and Henry2011).
Multicoloured tourmalines of pastel or light colours with dark crystal terminations at the analogous pole (the c– side of the crystal) are characteristics of Elba Island pegmatites, Italy. These terminations are usually black, though can appear in different colours such as brown, green, red–violet, and blue. Such more-or-less dark-coloured terminations may occur as narrow overgrowths, but can also compose a significant zone of the crystals, such as in the case of some elbaite crystals which are overgrown by aggregates of long parallel needles (Pezzotta, Reference Pezzotta2021).
The formation of the dark-coloured overgrowths in Elba tourmalines is related to physico-chemical variations in the crystallisation environment during the latest stages of tourmaline crystal growth. Such changes are consequent to the partial destabilisation of the pocket environment in which the tourmalines grew. The opening of the geochemical system due to pocket rupture has been suggested by several authors. However, the detailed events that led to chemical changes in the pocket environment resulting in the growth of late-stage tourmalines remain unclear. Some authors propose that fracturing of the pocket allowed the introduction of external fluids coming from other regions of consolidated pegmatite that infiltrated the host rock and modified the chemical environment (e.g. Foord Reference Foord1976; Aurisicchio et al., Reference Aurisicchio, Ottolini and Pezzotta1999; Selway et al., Reference Selway1999; London, Reference London2006). In accord with this view, Dutrow and Henry (Reference Dutrow and Henry2000, Reference Dutrow and Henry2016, Reference Dutrow and Henry2018) proposed that external fluids reacted with the host-rock and, in these conditions, tourmaline crystals dissolved to alter their composition with the generation of a late-stage fibrous Fe-rich tourmaline characterised by an external fluid signature. In contrast, Novák and Taylor (Reference Novák and Taylor2000) suggested that an internal source of Fe must be sought for the origin of Fe-rich late-stage tourmalines. In agreement with this latter consideration, Černý (Reference Černý2000) assessed that extensive leaching and corrosion of the cavity-lining and cavity-coating minerals of the pegmatite, could lead to variations in the composition of the cavity fluid. Buřival and Novák (Reference Buřival and Novák2015) suggested that the chemical change in the cavity system is the result of hydrothermal alteration of the cavity-lining minerals by late-stage fluids, which developed in the final stages of pegmatite crystallisation. Additionally, Felch et al. (Reference Felch, Falster and Simmons2016) inferred that the observed corrosion and leaching of cavity-lining spessartine garnet crystals, was the result of reactions with late-stage hydrothermal fluids that originated and migrated from adjacent highly evolved miarolitic cavities. More recently, Bosi et al. (Reference Bosi, Pezzotta, Altieri, Andreozzi, Ballirano, Tempesta, Cempírek, Škoda, Filip, Čopjacová, Novák, Kampf, Scribner, Groat and Evans2022) and Altieri et al. (Reference Altieri, Pezzotta, Skogby, Hålenius and Bosi2022) proposed that the pocket rupture event, possibly related to thermal contraction during the cooling of the rock, led to mechanical brittle deformation of the enclosing pegmatite by the formation of late-stage fractures. This allowed the highly-reactive late-stage cavity fluids to permeate the fractures surrounding the cavity where the early-crystallised cavity-lining and cavity-coating Fe- and Mn-rich minerals were hosted. Leaching and corrosion processes ascribed to the late-stage cavity fluids led to the hydrothermal alteration of such minerals, with the subsequent release of Fe, and occasionally Mn, in the pocket environment.
The relatively recent discovery of some cavities in the Rosina Pegmatite in San Piero in Campo allowed careful collection of many, mostly elbaitic, tourmaline crystals characterised by a variety of dark-coloured overgrowths. Paragenetic and structural information of the pegmatite were also recorded (Pezzotta, Reference Pezzotta2021). This investigation is focused on the crystal-chemical characterisation of an elbaitic multicoloured tourmaline crystal found in the cavity which has been naturally broken into two fragments. It is characterised by dark-coloured overgrowths, respectively purplish-red at the analogous pole, and yellow–orange at the antilogous pole. This crystal has also been selected because it is representative of the texture of the tourmaline crystals occurring in cavities of many other Elba pegmatites that underwent a similar chemico-physical evolution (Pezzotta, Reference Pezzotta2021).
In this investigation we correlated structural evidence, fracturing of the pocket producing breakage of tourmaline crystals, to the late-stage tourmaline generation.
Occurrence and sample description
The Rosina pegmatite is located a few hundred metres south of the San Piero in Campo village, Elba Island, Italy, and since its discovery in early 1990, has been mined for both collectibles and specimens suitable for scientific research (Pezzotta, Reference Pezzotta2021). The pegmatite is hosted in a porphyritic monzogranite at the eastern border of the Monte Capanne pluton (Fig. 1a) and has a complex shape, trending roughly N–S with a variable dip angle of 40–75°W (Pezzotta, Reference Pezzotta2000). The major productive section of the body is ~14 m long and 0.6–2.1 m wide. In general, the shallowest portions of the pegmatite body were characterised by mostly aplitic textures with minor coarse-grained pegmatitic lenses, whereas at greater depths, the body becomes more pegmatitic and divides into two major branches that are interconnected by several small veinlets (Pezzotta, Reference Pezzotta2000; Bosi et al., Reference Bosi, Pezzotta, Altieri, Andreozzi, Ballirano, Tempesta, Cempírek, Škoda, Filip, Čopjacová, Novák, Kampf, Scribner, Groat and Evans2022).
Fig. 1. (a) Geological map of Elba Island. The occurrence area of the analysed tourmaline samples (San Piero in Campo, Elba Island, Italy) is marked at the edge of the Monte Capanne granite (after Trevisan, Reference Trevisan1951 and modified by Pezzotta, Reference Pezzotta2021). (b) The analysed tourmaline crystal fragments. The first fragment (7 mm in length) was collected as it is (fragment I), whereas the other two parts (30 and 15 mm in length, respectively) were originally connected as a single fragment (fragment II) that broke during collection from the pocket. OGX, OGY, OGZ and OGR indicate the dark-coloured overgrowths. Scale bar = 1 cm.
The Rosina pegmatite belongs to the LCT family. This pegmatite is commonly miarolitic, with abundant small to medium size pockets and a series of medium to large pockets (up to ~80 dm3 in volume), and is significantly asymmetric in terms of textures, mineralogy and geochemistry. The axial core–miarolitic zone, which is rich in lepidolite, petalite and pollucite, divides the body into a medium-grained lower section enriched in albite with minor K-feldspar, quartz, spessartine, patches of sekaninaite and comb-texture tourmaline, and an upper coarse-grained section enriched in feldspar with minor albite, quartz and tourmaline. Cavities found at shallower levels contain dark-coloured tourmalines, together with pale-blue aquamarine and spessartine. In contrast, cavities found at deeper levels contain abundant polychrome and rose tourmalines with variable Mn and Fe content, morganite, petalite, pollucite and spessartine (Orlandi and Pezzotta, Reference Orlandi and Pezzotta1996; Pezzotta, Reference Pezzotta2000; Bosi et al., Reference Bosi, Pezzotta, Altieri, Andreozzi, Ballirano, Tempesta, Cempírek, Škoda, Filip, Čopjacová, Novák, Kampf, Scribner, Groat and Evans2022).
The tourmaline crystal samples investigated were found, together with several other crystals, in a relatively large, flat, oblate pocket of ~80 dm3 in volume (90 × 65 cm, up to 25 cm high), not affected by any weathering alteration, and in the core zone of the pegmatite body. The distribution of the minerals and the rock structures of this pocket reflect the typical asymmetric compositional and textural zoning of this dyke. The roof of the cavity was composed mostly of coarse-grained K-feldspar crystals, with quartz, minor albite, petalite and a few multicoloured tourmaline and pink beryl crystals. The floor of the cavity was mostly composed of medium-grained albite, with quartz, petalite, numerous multicoloured tourmaline crystals, and minor K-feldspar crystals and pollucite. Thin radial fractures penetrating from the miarolitic cavity into the surrounding pegmatite are evident in the Rosina pegmatite (Fig. 2), suggesting some phenomena of partial cavity collapse. As a result, we propose that the highly-reactive cavity fluids locally infiltrate these fractures, leading to late-stage corrosion and alteration of the previously-crystallised cavity-lining minerals. These processes are supported by the occurrence of fractured and decoloured biotite crystals, as well as altered spessartine garnet and petalite in the intermediate and lower border zone of the pegmatite (Fig. 2).
Fig. 2. E–W section of the Rosina pegmatite (~60 cm in thickness), with the different textures and mineralogical zonation labelled. The altered cavity-lining minerals as well as late-stage fractures (red arrows) are also marked. Scale bar = 10 cm.
Experimental methods
Sample preparation
The crystal fragments (Fig. 1b) were glued to a glass slide using epoxy resin, with their length parallel to the surface of the slide. A slice of each fragment was cut along the growth direction (crystallographic c-axis) and subsequently ground and polished to produce a flat surface with a uniform thickness of 500 μm for electron microprobe analysis (EMPA).
For spectroscopic analyses, fragments were glued to a glass slide using a thermoplastic resin and cut along the c-axis, as described above, with a thickness of ~1100 μm. Before analyses, slices were further thinned to a suitable thickness and doubly polished.
Electron microprobe analysis
Compositional data were collected along two traverses (A–B and C–D) parallel to the c-axis (Fig. 3). The first one (A–B) was conducted from the base to the termination of each crystal fragment, with an average step size of 800 μm, except for where it passed through the overgrowths, labelled as OGX, OGR and OGZ, where the step size was reduced to 130, 120 and 350 μm, respectively, to capture more fine-scale detail. A second short traverse (C–D), with a step size of 80 μm, was conducted to analyse a lateral overgrowth, labelled as OGY, and located on the prismatic section of the crystal. Electron microprobe analysis was undertaken using a CAMECA SX50 at the Istituto di Geologia Ambientale e Geoingegneria (CNR of Rome, Italy) operating in wavelength-dispersion mode with an accelerating potential of 15 kV, a sample current of 15 nA and a beam diameter of 10 μm. Eighty-seven spot analyses were collected. Minerals and synthetic compounds were used as reference materials as follows: wollastonite (Si, Ca); magnetite (Fe); rutile (Ti); corundum (Al); karelianite (V); fluorophlogopite (F); periclase (Mg); jadeite (Na); orthoclase (K); rhodonite (Mn); and metallic Cr. The PAP correction procedure for quantitative electron probe micro analysis was applied (Pouchou and Pichoir, Reference Pouchou, Pichoir, Heinrich and Newbury1991). Relative error on data was <5% and detection limits <0.03 wt.%.
Fig. 3. Upper panel: results of compositional analysis of the tourmaline crystal fragments along two traverses (A–B and C–D). Lower panel: thin section of the analysed tourmaline fragments, with the traverses parallel to the c-axis represented by solid lines. OGX, OGR, OGY and OGZ are used for the different overgrowths.
Optical absorption spectroscopy
Polarised room-temperature optical absorption spectra of the overgrowths (OGX, OGR, OGY and OGZ) were obtained in the range of 35000–11000 cm–1 (286–909 nm) at a spectral resolution of 1 nm on doubly polished sections, using an AVASPEC-ULS2048×16 spectrometer attached via a 400 μm ultraviolet (UV) optical fibre cable to a Zeiss Axiotron UV-microscope. The diameter of the circular measure aperture was 50 μm. A 75 W xenon arc lamp was used as a light source and Zeiss Ultrafluar 10× lenses served as the objective and condenser. A UV-quality Glan-Thompson prism, with a working range from 40000 to 3704 cm–1 was used as a polariser. Data in the near infrared (NIR) range (11000–5000 cm–1) were obtained at a spectral resolution of 4 cm–1 using a Bruker Vertex 70 spectrometer equipped with a halogen-lamp source and CaF2 beam-splitter, coupled to a Hyperion 2000 IR-microscope equipped with a ZnSe wire-grid polariser and an InSb detector. The beam was collimated using an adjustable rectangular aperture with edges varying from 50–80 μm.
Determination of site populations
The wt.% of element oxides determined by EMPA were used to calculate the atomic fractions (atoms per formula unit, apfu). The B content was assumed to be stoichiometric (B = 3.00 apfu). Lithium was estimated using the procedure of Pesquera et al. (Reference Pesquera, Gil-Crespo, Torres-Ruiz, Torres-Ruiz and Roda-Robles2016). The (OH) content was calculated by charge balance with the assumption (T + Y + Z) = 15.00 apfu and 31 anions (Tables 1, 2, 3 and 4).
Table 1. Representative compositions and atoms per formula unit (apfu) for the overgrowths OGX and OGR in the tourmaline crystals studied from San Piero in Campo, Elba Island, Italy. Average values and data for representative analysed spots are reported.
a Calculated by stoichiometry (see text)
b All Fe was considered to be Fe3+, with the exception of the OGR overgrowth, based on the OAS results
c Estimated with the procedure of Pesquera et al. (Reference Pesquera, Gil-Crespo, Torres-Ruiz, Torres-Ruiz and Roda-Robles2016)
d Determined by OAS
Errors for oxides and fluorine are standard deviations (in brackets); ‘–’ indicates not detected.
Table 2. Representative compositions and atoms per formula unit (apfu) for the overgrowths OGY and OGZ in the tourmaline crystals studied from San Piero in Campo, Elba Island, Italy. Average values and data for representative analysed spots are reported.
a Calculated by stoichiometry (see text)
b All Fe was considered to be Fe3+, with the exception of the OGR overgrowth, based on the OAS results
c Estimated with the procedure of Pesquera et al. (Reference Pesquera, Gil-Crespo, Torres-Ruiz, Torres-Ruiz and Roda-Robles2016)
d Determined by OAS
Errors for oxides and fluorine are standard deviations (in brackets); ‘–’ indicates not detected.
Table 3. Representative compositions and atoms per formula unit (apfu) for fragment I, prismatic section of the tourmaline crystals studied from San Piero in Campo, Elba Island, Italy. Average values and data for representative analysed spots are reported.
a Calculated by stoichiometry (see text)
b Estimated with the procedure of Pesquera et al. (Reference Pesquera, Gil-Crespo, Torres-Ruiz, Torres-Ruiz and Roda-Robles2016)
Errors for oxides and fluorine are standard deviations (in brackets); ‘–’ indicates not detected.
Table 4. Representative compositions and atoms per formula unit (apfu) for fragment II, prismatic section of the tourmaline crystals studied from San Piero in Campo, Elba Island, Italy. Average values and data for representative analysed spots are reported.
a Calculated by stoichiometry (see text)
b Estimated with the procedure of Pesquera et al. (Reference Pesquera, Gil-Crespo, Torres-Ruiz, Torres-Ruiz and Roda-Robles2016)
Errors for oxides and fluorine are standard deviations (in brackets); ‘–’ indicates not detected.
On the basis of the apfu, the site populations (see ‘Mineral formulae’ below) for each overgrowth and prismatic section of the two tourmaline crystal fragments were calculated following the site allocation of ions recommended by Henry et al. (Reference Henry, Novák, Hawthorne, Ertl, Dutrow, Uher and Pezzotta2011).
Results
Composition
Variations in composition for selected elements (in wt.%) along crystal traverses are shown in Fig. 3. Results reveal that each fragment is characterised by low Mn and Fe contents, except for the dark-coloured overgrowths (OGX, OGY, OGZ and OGR) where the MnO and FeO content increase sharply up to ~7 wt.% and 1 wt.%, respectively. The initial part of fragment I contains a slight enrichment in MnO, starting from a value of ~2 wt.% that progressively decreases below 0.3 wt.%, and then abruptly increases at beginning of the OGX overgrowth. The variation in content of selected elements (in wt.%) along the overgrowths are given in Fig. 4. Vanadium, Cr and Mg were always below detection limits (<0.03 wt.%) in the samples investigated.
Fig. 4. Compositional analysis of all the overgrowths (OGX, OGR, OGY and OGZ) observable in the tourmaline crystal fragments. Scale bar = 100 μm.
Compositions for selected representative spots analysed as well as the average values of each overgrowth (Tables 1, 2) and prismatic section (Tables 3, 4) of the two tourmaline crystal fragments are given in Tables 1–4. A full dataset from electron microprobe analysis for all samples analysed is available as Supplementary material. Note that in the overgrowths the oxidation state of Fe was assumed to be +3 as indicated by the presence of Mn3+ revealed by optical absorption spectroscopy (OAS), except for the OGR overgrowth, which contains Fe2+ (see below).
Compositional diagrams showing data from spot analysis relative to the prismatic section of fragment I and II, and the four different overgrowths are given in Fig. 5.
Fig. 5. Compositional diagrams determined by EMPA. Each point represents the result in apfu of a single spot analysis. The spot data for the different overgrowths (OGX, OGR, OGY and OGZ) and the prismatic sections of the two fragments (PS I and PS II) are distinguished by coloured labels. (a) X-site occupancy; (b) Y-site occupancy; (c) plot of 2Li vs. (Fe+Mn); (d) plot of F vs. Na; (e) plot of Ca vs. Ti; (f) ternary plot of Na/(Na + X□) vs. Mn/(Mn + 2Li) vs. F. Arrows highlight the compositional evolution trend from the prismatic section to the overgrowth. Dashed circles highlight the different distribution of the points relating to the overgrowth at the antilogous pole (OGR) compared to the other overgrowths (OGX, OGY and OGZ).
Mineral formulae
The resulting empirical formulae written in their ordered form, relative to average compositions of each overgrowth and prismatic section of the two tourmaline crystal fragments, as well as to selected representative spots analysed, are reported in Table 5.
Table 5. Empirical formulae for the different overgrowths and prismatic sections of the tourmaline crystals investigated from San Piero Campo, Elba Island, Italy. Formulae relative to average compositions and for representative spots are reported.
aEmpirical formulae were based on the Mn2O3 content calculated by OAS data.
All these compositions are consistent with a tourmaline belonging to the alkali-group, subgroup 2 (Henry et al., Reference Henry, Novák, Hawthorne, Ertl, Dutrow, Uher and Pezzotta2011): they are Na-dominant at the X position of the general formula of tourmaline and hydroxy-dominant at W with (OH+F)– > O2– and (OH) >> F, except for the OGR overgrowth and the prismatic section of fragment I, which are fluor-species as F > OH.
All the compositions are ZAl- and Y(Al1.5Li1.5)-dominant, and thus are elbaitic, Na(Li1.5Al1.5)Al6Si6O18(BO3)3(OH)3(OH,F), from a nomenclature viewpoint (Henry et al., Reference Henry, Novák, Hawthorne, Ertl, Dutrow, Uher and Pezzotta2011). In particular, the overgrowths OGX, OGY and OGZ, can be classified as Mn-rich elbaite, whereas the overgrowth OGR is Mn-rich fluor-elbaite. Regarding the prismatic sections, fragments I and II correspond to fluor-elbaite and elbaite, respectively.
Optical absorption spectroscopy
Optical absorption spectra (E⊥c and E||c) recorded at selected spots within the differently coloured overgrowths are reported in Fig. 6. All the E⊥c spectra of the OGX, OGY and OGZ overgrowths display a main absorption band centred at ~18800 cm–1 and a weaker absorption band at ~22000 cm–1. The spectrum of the OGX overgrowth recorded at spot 1 reveals additional absorption bands at ~24500 and ~9500 cm–1. In contrast, the E⊥c spectrum recorded within the OGR overgrowth shows a different absorption pattern with two very broad bands at ~30700 and ~22700 cm–1, and very weak bands at ~27000 and ~24500 cm–1. Additional relatively weak and broad bands occur in the NIR region at ~9000 and ~14000 cm–1. All the spectra recorded in light polarised parallel to the crystallographic c-axis (E||c), have a weaker absorption and additional very sharp bands between 6700–7200 cm–1 in the NIR range ascribed to overtones of the fundamental (OH)-stretching modes.
Fig. 6. Optical adsorption spectra for the dark coloured overgrowths polarised perpendicular (E⊥c) and parallel (E||c) to the c-axis direction of selected spots in the (a) OGZ, (b) OGY, (c) OGX and (d) OGR overgrowths. (e) Optical microscopy images of the OGX, OGR, OGY and OGZ overgrowths. The location of spots used for OAS are indicated. Sample thickness: OGX = 820 μm; OGY = 902 μm; OGZ = 658 μm; OGR = 437 μm. Scale bar = 1 mm.
Discussion
Composition analysis
The four overgrowths (OGX, OGR, OGY and OGZ) of the two tourmaline crystal fragments are characterised by a dark colour and a sudden increase in MnO, which rises up to 7 wt.%. In contrast, the prismatic section of fragment I and II has a very low MnO content, with the exception of the initial part of fragment I (up to 2 wt.%) (Fig. 3). Although the four overgrowths have similar composition, OGR has slightly more TiO2, CaO and F, which increases, respectively, up to 0.40 wt.%, 0.35 wt.% and 1.2 wt.% (Fig. 4; Tables 1, 2). It should be noted that the overgrowths OGX, OGY and OGZ were formed in the direction of the analogous pole, whereas the overgrowth OGR was formed at the antilogous pole of fragment II. Although the Mn increase at the overgrowths is confirming a significant chemical evolution, the mineralogical species remain elbaite and F-elbaite. This compositional evolution trend is evident in the ternary plots of X- and Y-site occupancy (Fig. 5a,b), where overgrowths are characterised by an enrichment in Na and Mn, respectively. The increase in Mn at the overgrowths is consistent with the substitution of Li and Al at the Y site. A plot of content of 2Li vs. (Mn + Fe) at the Y site (Fig. 5c), confirms that the analysis points relating to the prismatic sections are close to an elbaite/F-elbaite composition. In contrast, data relating to the overgrowths are distributed along a trend line corresponding to a total or partial replacement of Li and Al with Mn/Fe. A plot of the content of F vs. Na (Fig. 5d) confirms the Na enrichment that characterises the overgrowths.
Furthermore, in many graphs it is possible to observe a different distribution of the data relating to the overgrowth at the antilogous pole (OGR) compared to the other overgrowths (OGX, OGY and OGZ). This different trend is particularly evident in the Ca vs. Ti plot (Fig. 5e), where most of the data points for the OGR overgrowth lie apart from the other ones. Interestingly, the data related to the different overgrowths follow a different compositional evolution trend in the ternary plot of Na/(Na + X□) vs. Mn/(Mn + 2Li) vs. F (Fig. 5f).
Comparison of the dark overgrowths
The dark overgrowths have been compared to ascertain if they were formed simultaneously in the same crystallisation environment. As stated above, all overgrowths are characterised by a comparable composition, which is consistent with their formation in the same environment. The antilogous overgrowth OGR compared to the analogous ones shows some differences in Ti, Ca and F content, as well as a smaller length (~500 μm for OGR, ~1000 μm for OGX and OGZ, and ~700 μm for the lateral overgrowth OGY) (Fig. 4; Tables 1, 2).
Additional evidence supporting the formation of the four overgrowths in the same crystallisation environment is provided by OAS data (Fig. 6). The overgrowth at the analogous poles (OGX, OGY and OGZ) share the same ~22000 and ~18800 cm–1 absorption bands that can be assigned to Mn3+ d–d transitions (Reinitz and Rossman, Reference Reinitz and Rossman1988; Taran et al., Reference Taran, Lebedev and Platonov1993; Ertl et al., Reference Ertl, Rossman, Hughes, Prowatke and Ludwig2005; Bosi et al., Reference Bosi, Celata, Skogby, Hålenius, Tempesta, Ciriotti, Bittarello and Marengo2021). The additional bands at ~9500 and ~24500 cm–1 observed in the spectrum recorded at spot 1 of the OGX overgrowth can be ascribed to a Mn3+ spin-allowed d–d transition and a Mn2+ spin-forbidden transition, respectively (Bosi et al., Reference Bosi, Celata, Skogby, Hålenius, Tempesta, Ciriotti, Bittarello and Marengo2021). These assignments agree with the observed purplish-red colour of these overgrowths, mainly ascribed to the presence of Mn3+ as chromophore (Pezzotta and Laurs, Reference Pezzotta and Laurs2011). On the basis of the intensity of the Mn3+ band at ~18800 cm–1 in the spectra perpendicular to the c-axis of the analogous overgrowths OGX, OGY and OGZ (Fig. 6), and using the molar extinction coefficient suggested by Reinitz and Rossman (Reference Reinitz and Rossman1988), the Mn2O3 content in these overgrowths was calculated (Table 6). The top of the overgrowths OGX, OGY and OGZ are characterised by the same contents of Mn2O3 (1.3 wt.%) with a Mn3+/Mntot ratio ranging from 0.27 to 0.39. This observation, together with the similar composition, is consistent with overgrowths formed simultaneously in the crystallisation environment. It should be noted that a second OAS analysis on the bottom part of the OGX overgrowth (spot 1), revealed a greater amount of Mn2O3 (2.93 wt.%) and a higher Mn3+/Mntot ratio. The presence of Mn3+ suggests an oxidising environment during the crystallisation of the overgrowths.
Table 6. Summary of the OAS results for selected data points on the overgrowths including observed absorption bands, total content of MnO and relative amount of Mn3+ calculated by the molar extinction coefficient.
+Absorption band present
# MnOtot content at the OAS spot was determined on the basis of the chemical analysis conducted along the considered traverses
* Calculated considering the intensity of the Mn3+ band at 18800 cm–1 in E⊥c spectra, in combination with the molar extinction coefficient of 7.5 for that absorption band (suggested by Reinitz and Rossman, Reference Reinitz and Rossman1988). Values of absorber thickness: OGX = 820 μm; OGY = 902 μm; OGZ = 658 μm; OGR = 437 μm.
The optical absorption spectra of the OGR overgrowth revealed only the presence of very weak Mn2+ spin-forbidden bands (~27000 and ~24500 cm–1), in addition to strong and very broad bands at ~30700 and ~22700 cm–1, which are caused by Mn2+–Ti4+ and Fe2+–Ti4+ IVCT (Intervalence Charge Transfer) transitions, respectively (Rossman and Mattson, Reference Rossman and Mattson1986; Taran et al., Reference Taran, Lebedev and Platonov1993). The latter two are consistent with compositional data, which revealed an increased amount of Ti in the OGR overgrowth compared to the other ones. The broad and moderately intense bands in the NIR region at ~9000 and ~14000 cm–1, which are caused by spin-allowed transitions in Fe2+ (Mattson and Rossman, Reference Mattson and Rossman1987) do not contribute to the colour of the samples. The band assignments for the OGR overgrowth agree with its yellow–orange colouration due to the presence of Mn2+ and Mn2+–Ti4+ IVCT as chromophores (Rossman and Mattson, Reference Rossman and Mattson1986; Laurs et al., Reference Laurs, Simmons, Rossman, Fritz, Koivula, Anckar and Falster2007; Pezzotta and Laurs, Reference Pezzotta and Laurs2011). Considering the comparable total MnO contents of all the dark-coloured overgrowths (~4.5 wt.%), and that OGZ, OGY and OGR belong to the same crystal fragment and therefore grew at the same time, the absence of Mn3+ d–d transitions in the OGR spectra suggests a strong preferential incorporation of Mn2+ ions in the antilogous overgrowth, even in the presence of Mn3+ in the crystallisation environment. A similar crystal-chemical behaviour is observed for Ti, Ca and F, which are preferentially incorporated at the antilogous pole (Fig. 4; Table 1). As a result, the antilogous pole shows a different growth history, with a preferential incorporation of Ca, F and Ti, as well as a selective uptake of Mn2+ over Mn3+, leading to a different colouration and tourmaline species (fluor-elbaite instead of elbaite, typical of the other overgrowths). This different behaviour is also evident in several compositional diagrams, where OGR data points occupy a different position in the plot compared to the other overgrowths (Fig. 5).
The differences observed in the composition and spectroscopic analysis between the analogous and antilogous overgrowths can be related to differences in the growth process occurring at the two poles (surface energy, nucleation speed, piezo- and pyro-electrical properties) (Henry and Dutrow, Reference Henry and Dutrow1992).
The formation of the dark-coloured overgrowths is probably the result of a pocket rupture. This event changed the chemical environment within the pocket, leading to a sudden increase in the availability of Mn in the geochemical system. Although the initial part of the fragment exhibits a slight enrichment in MnO (up to 2 wt.%), this is related to the amount of Mn remaining available in the pegmatitic system after the early crystallisation of spessartine. The subsequent progressive decrease in MnO content in fragment I is the result of Mn depletion in the system due to tourmaline crystallisation. Spessartine crystallisation is recognised as an important mechanism for regulating the Mn content during the evolution of the pegmatite systems (Novák et al., Reference Novák, Selway, Černý, Chapman and Masau2000; Laurs et al., Reference Laurs, Simmons, Rossman, Fritz, Koivula, Anckar and Falster2007) and, in Elba pegmatites, spessartine garnet represents the main competitor for Mn during the evolution of the pegmatite system (Bosi et al., Reference Bosi, Pezzotta, Altieri, Andreozzi, Ballirano, Tempesta, Cempírek, Škoda, Filip, Čopjacová, Novák, Kampf, Scribner, Groat and Evans2022). Indeed, spessartine garnet in the Rosina pegmatite is present in the intermediate zone of the pegmatite, close to the miarolitic cavity (Fig. 2).
The very limited amount of Fe in the OGR overgrowth, in addition to limited amounts in all the other overgrowths, led us to exclude that this may represent the root part of the crystal. Therefore, it is reasonable to assume that this dark termination was formed on a new growth surface as a consequence of a natural breakage event which the prismatic section of the crystal underwent. Observing the two crystal fragments and disregarding the dark-coloured overgrowths, the shape of the analogous termination of fragment I and the antilogous one of fragment II match perfectly. This demonstrates that they are two crystal fragments belonging to the same original tourmaline crystal which broke during pocket collapse and on which late-stage overgrowths (OGX and OGR) occurred.
Comparison of the prismatic sections
In support of the evidence that the fragments (I and II) were part of the same original crystal, the analytical data document a perfect continuity (Fig. 7). Disregarding the data points related to the OGX and OGR overgrowths, compositional analysis revealed no significant variations for the different oxide components between the two prismatic sections, as expected if they had been joined (Fig. 7; Tables 3, 4). As consequence of the crystal breakage, OGX and OGR overgrowths have been formed on the new growth surfaces generated by the break.
Fig. 7. Compositional analysis of the two prismatic sections close to the OGX/OGR breakage.
Genetic model for the dark-coloured overgrowths
Elba tourmalines are renowned all over the world for their characteristic dark terminations, which are due to the incorporation of elements, such as Fe and/or Mn during the latest stages of crystallisation in miarolitic cavities (Pezzotta, Reference Pezzotta2021). However, the mechanisms that led to the availability of these elements in the residual fluids have previously been unclear.
Microstructural and paragenetic observations of the cavities in which tourmaline crystals with dark-coloured overgrowths were formed, provide evidence that such pockets are characterised by: (1) thin fractures penetrating from the cavity into the enclosing pegmatite; (2) leaching and corrosion of early-formed cavity-lining and cavity-coating Fe- and Mn-rich minerals crosscut by the fractures; (3) partial collapse of quartz and feldspar crystal aggregates; and (4) the breakage of some tourmaline crystals as a consequence of a partial pocket collapse (Bosi et al., Reference Bosi, Pezzotta, Altieri, Andreozzi, Ballirano, Tempesta, Cempírek, Škoda, Filip, Čopjacová, Novák, Kampf, Scribner, Groat and Evans2022; Altieri et al., Reference Altieri, Pezzotta, Skogby, Hålenius and Bosi2022). These features are particularly evident in the Rosina pegmatite from which the tourmaline crystals originated (Fig. 2). The pocket rupture occurred during the formation of a series of fractures penetrating the surrounding pegmatite, in which more primitive accessory minerals such as spessartine garnet and Fe-rich mica crystals were present (Fig. 2). Highly-reactive late-stage cavity fluids penetrating the fractures, allowed the corrosion of the Fe- and Mn-rich minerals causing a sudden change in the composition of the pocket crystallisation environment. Etching of spessartine garnet by late-stage reactive fluids has already been reported by London (Reference London2006) and Felch et al. (Reference Felch, Falster and Simmons2016), and similar evidence of corroded spessartine crystals occurs in the Rosina pegmatite (Fig. 8). To account for the presence of Mn both in +2 and +3 redox states in the dark-coloured overgrowths, corrosion and alteration phenomena probably occurred in a relatively oxidising environment.
Fig. 8. Examples of extensively fractured and partially corroded spessartine crystals (red arrows) ‘frozen’ in quartz and feldspars in proximity of cavities of the Rosina pegmatite. Crystals up to 6 mm in diameter. Scale bar = 10 mm.
The pocket rupture was responsible for the breakage of the crystal investigated resulting in the formation of two new growth surfaces (OGX and OGR). In our model, OGZ represents the overgrowth at the termination of the original analogous pole of the crystal, whereas OGX and OGR correspond to the overgrowths formed at the new analogous and antilogous pole surfaces, respectively, as a result of the crystal breakage. The OGY overgrowth is related to a smaller lateral crystal breakage (Fig. 9).
Fig. 9. Schematic representation of the history of growth of the tourmaline crystals investigated. (a) Step 1: tourmaline crystal growth from light green to pale pink in the direction of the analogous pole (c– side). Step 2: breakage of the crystal as a result of the pocket rupture event followed by changes in the composition of the crystallisation environment. Step 3: generation of late-stage dark-coloured overgrowths at the analogous (OGX, OGY, OGZ) and at the antilogous (OGR) poles in a Mn-rich environment. (b) Image of the tourmaline crystals investigated.
The crystal breakage strengthens the hypothesis that the cavity has undergone a mechanical destabilisation. Consequently, the tourmaline crystal fragments preserved important records not only in terms of compositional variations of the geochemical system represented by the dark overgrowths, but also in the mechanical events, i.e. the crystal breakage.
A comparison of the overgrowths at the analogous and antilogous poles provides evidence of a preferential incorporation of particular elements at growth surfaces. The antilogous pole relative to the analogous pole is characterised by a different growth rate and higher concentrations of Ca, F and Ti. The differential uptake of these elements at these poles have been described by Henry and Dutrow (Reference Henry and Dutrow1992) and van Hinsberg et al. (Reference van Hinsberg, Schumacher, Kearns, Mason and Franz2006) as a result of a combined effect of “lattice site morphology” on the different growth faces and dipolar surface charge which is related to the systematic orientation of the ring of tetrahedra. Here we report a further preference at the level of the ionic charge of the same elements. OAS data show a selective uptake of Mn2+ at the antilogous pole in the presence of a substantial amount of Mn3+ ions that preferred the analogous one. This differential uptake has never been reported previously and could be related to a greater partition coefficient for Mn3+ at the analogous surface. The preferential uptake of Mn3+ ions by the analogous growth surfaces led to a decrease in the Mn3+/Mntot ratio in the crystallising fluids. The change in this ratio can be deduced by analysing the OAS data of the more extended OGX overgrowth which is characterised by a marked decrease in Mn3+ content along the growth direction, maintaining approximately the same MnOtot content.
Conclusions
The tourmaline crystal fragments analysed illustrate the mechanical and compositional changes during the latest stages of cavity evolution as a consequence of a pocket rupture event. The comparison of the dark overgrowths formed on the direction of the analogous pole and the antilogous one in the same crystal, has provided new evidence regarding the different growing process occurring at the two poles involving Mn2+/Mn3+ ions.
This work clearly correlates structural information, i.e. fracturing of the pocket and breakage of tourmaline crystals, to late-stage tourmaline growth, and permitted definition of a genetic model for the dark-coloured overgrowths in Elba tourmaline crystals.
Acknowledgements
Sample preparation for chemical and spectroscopic analyses was carried out with the support of Dr. D. Mannetta to whom the authors express their gratitude. The authors thank M. Serracino for his assistance during chemical analyses. F.B. acknowledges funding by Sapienza University of Rome (Prog. Università 2020) and by the Italian Ministry of Education (MIUR)–PRIN 2020, ref. 2020WYL4NY. The authors thank Jan Cempírek and an anonymous reviewer for their constructive comments that helped to improve the manuscript and Principal Editor Roger Mitchell for editorial assistance.
Supplementary material
To view supplementary material for this article, please visit https://doi.org/10.1180/mgm.2022.125
Competing interests
The authors declare none.
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