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Article

Crystal Chemistry, Thermal and Radiation-Induced Conversions and Indicatory Significance of S-Bearing Groups in Balliranoite

by
Nikita V. Chukanov
1,2,*,
Anatoly N. Sapozhnikov
3,
Roman Yu. Shendrik
2,3,
Natalia V. Zubkova
2,
Marina F. Vigasina
2,
Nadezhda V. Potekhina
2,
Dmitry A. Ksenofontov
2 and
Igor V. Pekov
2
1
Federal Research Center of Problems of Chemical Physics and Medicinal Chemistry, Russian Academy of Sciences, 142432 Chernogolovka, Moscow Region, Russia
2
Faculty of Geology, Moscow State University, 119991 Moscow, Russia
3
Vinogradov Institute of Geochemistry, Siberian Branch of Russian Academy of Sciences, 664033 Irkutsk, Russia
*
Author to whom correspondence should be addressed.
Minerals 2023, 13(6), 822; https://doi.org/10.3390/min13060822
Submission received: 30 May 2023 / Revised: 14 June 2023 / Accepted: 14 June 2023 / Published: 16 June 2023

Abstract

:
Crystal-chemical features of a sulfide-bearing variety of the cancrinite-group mineral balliranoite from the Tuluyskoe lapis lazuli deposit, Baikal Lake area, Siberia, Russia, have been investigated using a multimethodic approach based on infrared (IR), Raman, and electron spin resonance (ESR), as well as ultraviolet, visible and near infrared (UV–Vis–near IR) absorption spectroscopy methods, luminescence spectroscopy, electron microprobe analysis, selective sorption of CO2 and H2O from annealing products, and single-crystal X-ray structure analysis. Holotype balliranoite and its sulfate analogue, davyne, were studied for comparison. The crystal-chemical formula of the studied sample from Tultuyskoe is Na5.4K0.1Ca2.4(Si6Al6O24)Cl2[(CO3)0.7(SO4)0.18S*0.95Cl0.1(H2O)0.16], where the content of the wide zeolite channel is given in square brackets; S* is total sulfide sulfur occurring as disordered S2●−, cis- and trans-S4, S52−, minor S3●−, and HS groups. The presence of S52− and HS groups, the absence of CO2 molecules, and the association with pyrrhotite and Fe-free pargasite indicate that the studied sample crystallized under highly reducing, low-temperature conditions, unlike holotype balliranoite whose formation was related to the Somma-Vesuvius volcanic complex, Italy. Irradiation of balliranoite from Tultuyskoe with X-rays results in the transformations of polysulfide groups other than S3●− into S3●− in accordance with the scheme: S52− → S2●− + S3●−; 3S2●− → 2S3●− + e; S4 + S2●− + e → 2S3●−; S4 + S2●− + e → 2S3●−; S4 + S52− + e → 3S3●− (e = electron).

1. Introduction

Various extra-framework anions, radical anions, and neutral molecules (SO42−, SO32−, PO43−, CO32−, C2O42−, Cl, HS, OH, F, Sn2− with n from 1 to 5, Sn with n from 1 to 4, where “” means unpaired electron, Sn0 with n = 4 or 6, CO2, COS, and H2O) occurring in cancrinite- and sodalite-group minerals [1,2,3,4,5,6,7,8,9,10,11,12,13,14] are considered as important markers of redox conditions and fugacities of volatile components during rock formation [14,15,16,17]. The S-bearing extra-framework species are most diverse and indicate wide variations of the oxidation degree of sulfur, polymerization degree of sulfide sulfur, and charges of S-bearing species. Unlike the majority of minerals of the cancrinite and sodalite groups from volcanic complexes, their counterparts from metasomatic lapis lazuli deposits contain sulfur in both oxydized (sulfate, SO42−) and reduced (mainly, polysulfide, rarely monosulfide, S2−, as well as HS, or sulfite, SO32−) forms, which reflects reducing conditions of their formation [4,5,6,9,12,13,14,17,18].
Balliranoite, ideally (Na,K)6Ca2(Si6Al6O24)Cl2(CO3), is a rare cancrinite-group mineral first discovered at the Somma-Vesuvius volcanic complex, Campania, Italy [19]. This mineral forms a solid-solution series with davyne, (Na,K)6Ca2(Si6Al6O24)Cl2(SO4) [20,21]. Structurally, both minerals are closely related to cancrinite, Na7Ca[Al6Si6O24](CO3)1.5·2H2O, and vishnevite, (Na,K)8[Al6Si6O24](SO4)·2H2O [22,23,24], as well as their high-chloride analogue, betzite, Na6Ca2(Al6Si6O24)Cl4, recently discovered in a xenolith hosted by alkaline basalt of the Bellerberg paleovolcano, Eifel Mountains, Germany [25]. The aluminosilicate frameworks of balliranoite, davyne, and betzite contain columns of cancrinite cages hosting (Ca···Cl) chains and wide channels which contain the CO32−, SO42−, and Cl anions, as well as extra-framework cations (Na+, K+, and minor Ca2+). Columns of cancrinite cages of other minerals with the cancrinite-type aluminosilicate frameworks host (Na···H2O) chains. Based on the content of the columns of cancrinite cages, the two-layer cancrinite-group minerals can be subdivided into the subgroup of cancrinite sensu stricto and the davyne subgroup [26]. Unlike balliranoite, davyne and intermediate members of the balliranoite-davyne solid-solution series are rather widespread minerals known in numerous localities [1,20,22,27,28,29,30].
The rarity of balliranoite may be caused by the combination of two extra-framework anions which are characteristic for cancrinite-group members from different geological environments: CO32−, occurring in wide channels, is typical for the minerals formed in intrusive complexes, whereas Cl is more common for cancrinite-group minerals from volcanic complexes [24]. However, there is a specific formation, the skarn-like lazurite-bearing metasomatites related to relatively abyssal rocks, in which cancrinite-group minerals demonstrate crystal-chemical features rather similar to those from low-pressure volcanic rocks. This paper describes crystal-chemical features of an unusual sulfide-bearing variety of balliranoite from the Tultuyskoe lapis lazuli deposit (Baikal Lake area, Siberia, Russia) belonging to this formation. The application of a multimethodic approach based on infrared (IR) absorption; Raman; electron spin resonance (ESR); ultraviolet, visible, and near infrared (UV–Vis–NIR) absorption spectroscopy; spectroscopy of luminescence; electron microprobe analysis; selective sorption of CO2 and H2O from annealing products; and single-crystal X-ray structure analysis made it possible to identify ten (!) extra-framework components occurring in this sample. Additionally, radiation-induced and thermal transformations of sulfide-bearing balliranoite were studied.

2. Materials and Methods

2.1. Samples

Three samples were studied. The most detailed data have been obtained for sulfide-bearing balliranoite (below, Sample 1) from the abandoned Tultuyskoe (another name: Tultuy, or Tultui) lapis lazuli deposit situated in the valley of Tultuy, a left tributary of the Malaya Bystraya river, Baikal Lake area, Siberia, Russia. The Tultuyskoe deposit was discovered in 1852 by G. M. Permikin. Its specific feature distinguishing it from other lapis lazuli occurrences of the Baikal Lake area is the abundance of cancrinite-group minerals (mainly, afghanite, with the subordinate roles of tounkite and balliranoite) as well as the sodalite-group member vladimirivanovite, an orthorhombic analogue of minerals belonging to the lazurite–haüyne solid-solution series [21].
Sample 1 contains light green to greenish yellow grains of sulfide-bearing balliranoite embedded in granular calcite aggregates up to 2 cm across (Figure 1). These aggregates occur in calcite marble containing accessory pyrrhotite, amphibole, and dolomite. Other minerals closely associated with sulfide-bearing balliranoite are fluorapatite, sodalite, and pargasite.
Samples 2 and 3 were studied for comparison. These samples were partly characterized by us earlier [19,29].
Sample 2 is the holotype specimen of balliranoite from the Somma-Vesuvio volcanic complex [19]. It occurs as colorless equant and prismatic crystals up to 1 mm × 1 mm × 2 mm (Figure 2) in cavities of metasomatic rock composed of orthoclase, phlogopite, clinohumite, calcite, diopside, pargasite, haüyne, and fluorapatite. The empirical formula of balliranoite from Sample 2 is Na4.70Ca2.53K0.73(Si6.02Al5.98O23.995)Cl2.34(CO3)0.82(SO4)0.27·0.12H2O. It is hexagonal, space group P63; a = 12.695(2) Å, c = 5.325(1) Å, V = 743.2(2) Å3, and Z = 1.
Sample 3 is davyne from Sar’e Sang, the famous lapis lazuli deposit in Afghanistan. It forms light blue aggregates in association with lazurite, diopside, and calcite (Figure 3). Its empirical formula is Na5.1Ca2.0K0.8(Si6.0Al6.0O24)Cl2.0(SO4)0.9(S2●−)0.1 and parameters of the unit cell are a = 12.773(1), c = 5.334(1) Å; space group P63 [29].

2.2. Analytical Methods

In order to obtain IR absorption spectra, powdered samples were mixed with anhydrous KBr, pelletized, and analyzed using an ALPHA FTIR spectrometer (Bruker Optics, Karlsruhe, Germany) at a resolution of 4 cm−1 as described in [5,6,8,12,13]. A total of 16 scans were collected for each spectrum. The IR spectrum of an analogous pellet of pure KBr was used as a reference.
The Raman spectra have been obtained for randomly oriented grains using an EnSpectr R532 spectrometer based on an OLYMPUS CX 41 microscope (Enhanced Spectrometry, San Jose, CA, USA) coupled with a diode laser (λ = 532 nm) at room temperature [5,8,12,15]. The spectra were recorded in the range from 100 to 4000 cm−1 with a diffraction grating (1800 gr mm−1) and spectral resolution of about 6 cm−1. The output power of the laser beam was in the range from 15 to 20 mW. The diameter of the focal spot on the sample was 5–20 μm. The backscattered Raman signal was collected with 10× and 40× objectives; signal acquisition time for a single scan of the spectral range was 1 s, and the signal was averaged over 100 scans. Crystalline silicon was used as a standard.
The assignment of bands in the IR and Raman spectra was carried out using data from [5,6,7,8,9,12,13,14,15,16,18,31,32,33,34].
The absorption spectra of a 1.1 mm thick fragment of Sample 1 in the UV–Vis–NIR range were measured at room temperature using a Lambda 950 spectrophotometer (Perkin-Elmer, Shelton, CT, USA) as described in [12,13].
Irradiation of Sample 1 was carried out with a low-pressure mercury lamp at room temperature for 30 min from both sides. X-ray irradiation was carried out at room temperature using an X-ray tube with a Pd anode with an applied voltage of 25 kV and a current of 20 mA.
ESR spectra of Sample 1 were measured on a randomly oriented grain with a RE-1306 X-band spectrometer (KBST, Smolensk, Russia) at room temperature and at 77 K as described in [12,15]. For low-temperature measurements, a quartz ampoule with the sample was placed in a flooded nitrogen quartz cryostat.
The luminescence excitation spectra were measured on an LS-55 spectrofluorometer (Perkin-Elmer, Shelton, CT, USA) in a cryostat at a temperature of 77 K. The luminescence spectra were measured on a spectrometer based on an MDR-2 monochromator (LOMO, Saint-Petersburg, Russia) using a diffraction grating with 600 lines per millimeter, upon excitation with a 405 nm semiconductor laser. The spectra registration was carried out using a Hamamatsu H10721-04 photomodule (Hamamatsu, Sendai, Japan).
The single-crystal XRD studies were carried out using an Xcalibur S diffractometer (OXFORD DIFFRACTION, Oxford, UK) equipped with a CCD detector (MoKα radiation, λ = 0.71073 Å), operating at 50 kV and 40 mA. More than a hemisphere of three-dimensional data was collected at room temperature from the crystal of 0.35 × 0.54 × 0.82 mm3 in size. Data reduction was performed using the CrysAlisPro Version 1.171.37.35 [35]. The data were corrected for Lorentz factor and polarization effects.
Five EDS-mode electron microprobe analyses of Sample 1 were carried out on an analytical suite including a digital scanning electron microscope Tescan VEGA-II XMU equipped with an energy-dispersive spectrometer (EDS) INCA Energy 450 with semiconducting Si (Li) detector Link INCA Energy and wave-dispersive spectrometer (WDS) Oxford INCA Wave 700, produced by Tescan Orsay Hld., Brno, Czech Republic. The analyses were performed at an accelerating voltage of 20 kV, current of 120 to 150 pA, and beam diameter of 120 nm. The diameter of the excitation zone was below 5 μm. The following standards were used: albite for Na, potassium feldspar for K, wollastonite for Ca, synthetic Al2O3 for Al, SiO2 for Si, FeS2 for S, and NaCl for Cl. Contents of other elements with atomic numbers > 6 are below detection limits.
The H2O content was determined by means of the Penfield method. In order to determine the content of carbonate groups, selective sorption of CO2 was carried out on askarite sorbent (an asbestiform matter saturated by NaOH) from gaseous products obtained by heating of the mineral at 1080 °C in oxygen at 1 atm.

3. Results

3.1. Chemical Composition

The chemical composition of sulfide-bearing balliranoite (Sample 1) is given in Table 1. Chemically, the mineral is quite uniform. Significant variations are observed only for the contents of calcium and sulfur. Oxygen equivalent for polysulfide groups is not calculated because they are disordered and their proportion could not be determined based on X-ray structural data. However, the total sums of analyses significantly exceeding 100% indicate that a major part of sulfur occurs in polysulfide groups. This conclusion was qualitatively confirmed by a combination of spectroscopic methods (see below). In order to subtract oxygen equivalents, exact contents of different polysulfide groups are required. Unfortunately, application of a complex of spectroscopic methods provides only qualitative information on the contents of these groups.
The empirical formula of Sample 1 based on 12 (Si + Al) atoms per formula unit is H0.33Na5.31K0.13Ca2.59(Al6.00Si6.00O24)S*1.13Oy(CO3)0.69Cl2.09, where S* is total sulfur and Oy is oxygen belonging to sulfate groups and H2O molecules.

3.2. Infrared Spectroscopy

The IR spectra of the studied samples are given in Figure 4. They contain bands of stretching (in the range of 950–1130 cm−1), mixed (550–700 cm−1), and bending (below 500 cm−1) vibrations of the aluminosilicate framework, partly overlapping with weaker bands of stretching and bending modes of sulfate anions (in the ranges of 1100–1200 and 610–620 cm−1, respectively). Bands at 3300 to 3368 cm−1 correspond to O–H stretching vibrations of H2O molecules. Weak bands in the range from 710 to 780 cm−1 may be due to combination modes [25].
IR spectra of both balliranoite samples differ from that of davyne by the presence of additional bands of asymmetric stretching and out-of-plane bending modes of CO32− groups (in the ranges of 1390–1520 and 850–880 cm−1, respectively). As compared to holotype balliranoite, Sample 1 shows additional bands of CO32− groups at 880, 1395, 1434 and 1477 cm−1, which indicates the presence of carbonate groups in a different local environment. The shoulder at 685 cm−1 may correspond to trans-S4 symmetric stretching ν3 mode.
In the IR spectrum of holotype balliranoite (Sample 2), bands of framework stretching and bending bands are poorly resolved, which may be due to the presence of Fe3+ defects in the framework which were detected with luminescence (see below), or a partial disordering of Si and Al. The peak at 2352 cm−1 corresponds to antisymmetric stretching vibrations of CO2 molecules occurring in the channel.

3.3. Raman Spectroscopy

Unlike IR spectroscopy, Raman spectroscopy is very sensitive to the presence of different species containing sulfide sulfur. However, the application of Raman spectroscopy can be complicated by luminescence. Figure 5 shows uncorrected Raman spectra of the studied samples. Strong luminescence is observed as a combination of at least three very broad peaks centered in the ranges of 1500–2000, 2700–3100 and 3300–3600 cm−1 which may be due to the presence of Mn2+, S2●− and Fe3+ centers, respectively [5,14,15,36].
The Raman spectrum of balliranoite from Tulyui in the range of 1200–3800 cm−1 contains weak bands at ~1640 and 2564 cm−1 corresponding to S3●− overtone (3’ν1) and HS stretching mode, respectively [6,7,8,12,15].
Corrected Raman spectra of balliranoite (the Samples 1 and 2) in the range of 150–1250 cm−1 are shown in Figure 6. In the Raman spectrum of holotype balliranoite, only bands of CO32−, SO42−, and aluminosilicate framework are observed (Table 2). The Raman spectrum of balliranoite from Tultuyskoe contains in this region additional bands of S2●−, S3●−, cis-S4, trans-S4, and S52−. Their assignment made using data from [5,6,7,8,9,12,13,14,15,16,18,19,20,21,22] is given in Table 2.
After irradiation of Sample 1 with X-rays, its color changed to blue, bands of S2●−, S4, S4, and S52− in the Raman spectrum disappeared, intensities of the bands corresponding to S3●− increased significantly, and the bands of SO42−, CO32−, and HS remained unchanged (curve a in Figure 7, Table 3). The wavenumber of the band of S3●− symmetric stretching vibrations (542 cm−1) of the irradiated sample is somewhat less than typical values of analogous bands in sodalite-group minerals (544–546 cm−1).
Heating of Sample 1 in air at 600 °C for 1 h results in the formation of two phases. The Raman spectrum of Phase 1 (curve b in Figure 7, Table 3) is similar to that of irradiated Sample 1. The main distinctions of the Raman spectrum of Phase 1 are a lowering of the intensity of the band of HS and significant shifts of all bands of S3●− towards lower wavenumbers.
The Raman spectrum of Phase 2 in Sample 1 in air at 600 °C for 1 h (Figure 8) contains bands of stretching vibrations of HS (at 2566 cm−1), CO32− (at 1058 and 1082 cm−1), SO42− (at 987 cm−1), S2●− (at 602 cm−1), S3●− (at 535 cm−1), and S52− (at 422 and 457 cm−1). The bands of S52− are narrow and not split, which indicates the presence of only one conformer of this anion, unlike initial Sample 1. Strong luminescence observed it the range of 800–3500 cm−1 is related to the presence of the S2●− radical anions. Periodic structure of the luminescence spectrum may be a result of interference of laser radiation on thin platelets along cleavage planes formed as a result of cracking the sample during its heating. All other Raman bands of Phase 2 are due to vibrations of the aluminosilicate framework and lattice vibrations (soft acoustic modes). Taking into account that S3●− is the most stable polysulfide species [32], one can suppose that Phase 2 is an intermediate product of the transformation of Sample 1 into Phase 1.
Heating of Sample 1 in air at 800 °C for 6 h resulted in the decomposition of a major part of the aluminosilicate framework and the formation of an orthosilicate whose strong bands are observed at 880, 849, 795, 394, 326, and 166 cm−1 (curve c in Figure 7). The remaining bands correspond to relicts of a cancrinite-type phase with extra-framework S3●−, SO42−, CO32−, and HS anions (the bands at 532, 985, 1059, and 2554 cm−1, respectively).

3.4. Absorption Spectroscopy in the NIR/Vis/UV Ranges

The absorption spectrum of Sample 1 (curve 1 in Figure 9) shows a broad absorption band in the region of 1.45–2.4 eV. With the transition to the ultraviolet region of the spectrum, an increase in absorption is observed. The observed broad band has an asymmetric shape and can be decomposed into two Gaussians with maxima at 2.05 and 2.31 eV and a width of 0.33 eV. Previously, similar bands were observed for S4-containing haüyne and assigned to neutral S4 molecules having trans and cis conformations [13].
After irradiation of Sample 1 with a low-pressure mercury lamp (with wavelengths of 193 and 253 nm) or X-ray irradiation, the absorption in the region of 1.6–2.4 eV (with a maximum at about 2.1 nm) increases (Figure 9, curves 2 and 3) and the sample acquires a deep blue color.

3.5. ESR Spectroscopy

In the ESR spectrum of the original Sample 1, only a sextet from Mn2+ (with a fine structure of the sextet components) was observed. After irradiation, an additional ESR signal appears, with the g-tensor components g1 = 2.053, g2 = 2.040 and g3 = 2.001 (Figure 10). The intensity of the Mn2+ sextet does not change after irradiation.

3.6. Luminescence Spectroscopy

When Sample 1 is excited with a 405 nm radiation, a broad luminescence band is observed with a maximum at 645 nm and a pronounced vibrational structure (Figure 11). The distance between phonon repetitions is about 595 cm−1. Similar luminescence bands were previously observed for other microporous minerals in the form of a wide band with a maximum at 580 nm for marinellite, 620 nm for biachellalite, 640 nm for tugtupite [14], 610 nm for hackmanite [37], 625 nm for sapozhnikovite [7], 650 nm for haüyne [5,13], 600 nm for afghanite, 640 nm for nosean, and 630 nm for kyanoxalite [12].

3.7. Crystal Structure

The crystal structure was solved with direct methods and refined to R = 0.0476 for 1191 independent reflections with I > 2σ(I) using SHELX software package [38] with anisotropic treatment of all atoms except S, C, and corresponding O atoms of sulfate and carbonate groups. The structure was studied in the frame of hexagonal space group P63. The unit cell parameters are a = 12.6874(4), c = 5.32039(17) Å, V = 741.68(5) Å3. As previously reported holotype balliranoite from the Somma–Vesuvio volcanic complex [19], the studied crystal is merohedrally twinned with an inversion center as a twinning operator; the 0.54:0.46 ratio of twin components was found.
In the crystal structure of the studied crystal as well as in the holotype balliranoite [19], Al and Si atoms are ordered among tetrahedral sites, which is typical for cancrinite-group minerals. The average <Si–O> and <Al–O> distances in tetrahedra are 1.625 and 1.722 Å, respectively. The aluminosilicate framework is the same as reported for holotype balliranoite.
Calcium cations are located at the centers of bases of the cancrinite cages. The Ca site is characterized by the partial occupancy factor of 0.949(14). Ca2+ cations occupy eight-fold polyhedra with six Ca–O bonds varying from 2.566(5) to 2.629(5) Å and two Ca–Cl bonds with the distances of 2.646(8) and 2.686(8) Å. Unlike the structure of balliranoite from the Somma–Vesuvio volcanic complex, in the studied crystal all Cl anions are statistically distributed over three symmetry-related sites slightly offset from the three-fold axis, and at the last stages of the refinement their site occupancy factors were fixed at 0.33.
Two Na-dominant sites statistically replacing each other are located in the wide channel of the framework. The occupancy factors of these sites refined on the basis of the Na scattering curve are 0.51(8) and 0.56(9). This corresponds to the total number of electrons of 11.77 which is in a good agreement with chemical data and corresponds to the (Ca,K) admixture of 10%.
Three crystallographically nonequivalent C sites were found from difference Fourier synthesis at the center of the wide channel. Two of them (C1 and C2) are located very close to the corresponding sites in the structure of holotype balliranoite [19], while the third site (C3) is a new one. A set of constraints was introduced in the refinement. In particular, CO32− groups were considered to be planar, with the same z coordinate of C and O atoms. The position of the S site found in balliranoite from the Somma–Vesuvio volcanic complex [19] is vacant in the studied sample. The refinement showed that two of three C sites (C2 and C3) contain additional components, and it was assumed that S atoms statistically replace C at their sites. O atoms of the C1O3 groups showed higher occupancy factor than C1 and were assumed to participate also in SO4 tetrahedra forming the common base of two tetrahedra with opposite orientation. The fourth vertices of the SO4 tetrahedra were fixed at corresponding distances from the S sites. At the last stage of the refinement, the occupancies of C, S, and corresponding O sites were fixed according to chemical data and for preservation of reliable parameters of atomic displacements: C1, C2, C3 sites have site occupancy factors of 0.18, 0.08, and 0.09, respectively, and S atoms replacing C2 and C3–0.06 and 0.03, respectively. S atoms of polysulfide groups could not be localized because of their low occupancy factors and strong disordering in the wide channel. The arrangement of the main extra-framework components in the wide channel is shown in Figure 12.

4. Discussion

4.1. Crystal-Chemical Features of Sulfide-Bearing Balliranoite

Balliranoite from Tultuyskoe is a bright example illustrating complex chemistry and crystal chemistry of sulfur in minerals with microporous structures. The crystal-chemical formula of Sample 1 derived based on chemical data and crystal structure refinement is Hx(Na5.3Ca0.6K0.1)Ca2(Si6Al6O24)Cl2[(CO3)0.7(SO4)0.2S*0.95Cl0.1nH2O, where formula coefficients are rounded, non-cationic species occurring in the wide channel are given in square brackets, S*0.95 is total sulfide sulfur (in the S2●−, S3●−, S4, S52−, and HS groups), and Hx is hydrogen belonging to HS groups, x ~ 0.1 and n ~ 0.1. Based on the charge-balance requirement, the total charge of S*0.95 is about −0.8, which indicates a significant portion of S2− (as a part of HS or isolated S2− anions) or the presence of additional disordered SO42− groups which could not be localized during the crystal structure refinement.
The general structural formula of sulfide-bearing balliranoite can be written as (Na,Ca,K)6Ca2(Si6Al6O24)(Cl,HS)2(CO32−,SO42−,S2●−,S3●−,S4,S52−,Cl,HS)1+y·nH2O, where y < 1, n << 1, and each of the S4 and S52− species is present in two conformation states.
Specific features of the studied sample are an unusual diversity and strong disordering of extra-framework components. In particular, in the structure of sulfide-bearing balliranoite (Sample 1) there are three sites of carbonate groups instead of two sites in the holotype balliranoite sample. This is in agreement with the IR spectrum showing additional bands of asymmetric C–O stretching vibrations (at 1395, 1434, and 1477 cm−1) and non-degenerate bands of CO32− out-of-plane bending vibrations (at 880 cm−1) as compared to the holotype sample.
Among S atoms, only those belonging to SO42− groups with low occupancies were localized during the crystal structure refinement. We assume that S sites of polysulfide anions, radical anions, and molecules are characterized by very low site occupancy factors and are strongly disordered in the wide channel. This does not allow their localization using XRD data. All attempts to lower symmetry for a better localization of sulfide sulfur were unsuccessful.

4.2. Indicatory Significance of Extra-Framework Species in Balliranoite

The composition of extra-framework species in feldspathoids is considered as a marker of important characteristics of mineral-forming media, including fugacities of volatile components (H2O, O2, CO2, HF, SO2, and polysulfide compounds) [5,7,14,39,40,41]. HS and S52− anions occurring in feldspathoids are indicators of highly reducing conditions of mineral formation whereas extra-framework CO2 molecules, generally typical for members of the cancrinite and sodalite groups [5,7,12,13,14], are absent in minerals containing HS and S52− anions [7,42]. In this reference, it is important to note that all oxygen-bearing minerals associated with sulfide-bearing balliranoite (Sample 1) do not contain iron in amounts exceeding the detection limit of the electron microprobe analysis (practically, all iron occurs in pyrrhotite). In particular, the charge-balanced empirical formula of white iron-free pargasite from this assemblage is K0.07Na1.01Ca1.92(Mg4.12Al0.65Ti0.13)(Si6.38Al1.62O22)(OH)2. On the contrary, pargasite and phlogopite from the association with holotype balliranoite contain significant amounts of iron whereas sulfides are absent there.
In situ Raman spectroscopy was used to identify various S-bearing species in aqueous fluids on a model system prepared from potassium thiosulfate, sulfide, and sulfate, in a wide range of sulfur concentration, acidity, temperature, and pressure [40]. According to these data, in the hydrothermal solutions and supercritical fluid phases, the trisulfur radical anion S3●− is thermodynamically stable, along with sulfate anion, from 200 °C to at least 700 °C. The S2●− radical anion was detected in the range of 450–500 °C. In S-rich solutions, maximum abundance of neutral polysulfide groups Sn was observed at around 300 °C. At temperatures below 500 °C, the amount of S3●− is up to 10% of total dissolved sulfur, but at 600–700 °C the fraction of S3●− reaches 50% of total sulfur.
Fluid inclusions in quartz synthesized from S-bearing solutions contain SO42− and HS anions, which are stable up to 500 °C and are in equilibrium with the S3●− radical anion whose fraction increases with temperature [43].
According to the calculated phase diagram of the Fe-S system [44], at the molar ratios S/(Fe+S) > 0.5 pyrrhotite cannot coexist with pyrite at temperatures above 700 °C or below 300 °C. On the other hand, in the Fe-O-S system, at ambient pressure pyrrhotite is thermodynamically stable only at temperatures above 500 °C. Under highly reducing conditions, pyrrhotite is stable only at temperatures just slightly exceeding 500 °C [45] which corresponds to the lowest values for lazurite-bearing metasomatites of the Baikal Lake area, which formed at low pressures, in zones of tectonic unloading [46].
Phase diagram of the system Fe–S–O–H constructed at 500 °C and 4.0 kbar shows that under these conditions pyrrhotite is stable only at pH < 9 and log fO2 < −20, but only in the interval −21 < log fO2 < −20 can pyrrhotite exist in thermodynamical equilibrium with pyrite [47].
Polysulfide groups other than S3●− are unstable above 700 °C [13,15]. Moreover, there are indications of transformations of a yellow chromophore (presumably, S2●−) into S3●− as a result of long-time heating of a lazurite-related sodalite-group mineral at 500 °C [46]. Thus, one can suppose that balliranoite from Tultuyskoe crystallized under highly reducing, low-temperature (below 500 °C), near-neutral or weak-acidic conditions. It is to be noted that a major part of cancrinite-group minerals and low-symmetry sodalite-group minerals (including vladimirivanovite), which occur in lapis lazuli deposits and are most abundant in the Tultuyskoe deposit, crystallized after cubic lazurite and members of the lazurite–haüyne solid-solution series [21,46,48,49].
Holotype balliranoite (Sample 2) formed in a volcanic complex does not contain sulfide sulfur. Luminescence observed in the Raman spectrum indicates that this sample contains a trace amount of Fe3+, unlike Sample 1 which is iron-free. IR spectrum of Sample 2 shows the presence of extra-framework CO2 molecules. All these signs indicate that Sample 2 crystallized at relatively more oxidizing conditions as compared to Sample 1 and Sample 3.

4.3. Radiation-Induced Transformations of Sulfide-Bearing Balliranoite

Previously, the appearance of a blue color and ESR signal as a result of irradiation was observed for a number of other carbonate minerals, including layered silicates of the carletonite group [50,51], cancrinite [52,53], and kyanoxalite [12]. After irradiation of these minerals, a band with a maximum in the range of 1.8–2.0 eV appeared in the absorption spectra, and an ESR signal with g1 = 2.018, g2 = 2.014, and g3 = 2.008 was observed. These bands are associated with the CO3●− radical anion. However, in the case of balliranoite (Sample 1), both the ESR signal and the absorption spectrum differ significantly from those for the CO3●− radical anion.
The observed absorption peaking at about 2.1 eV and the observed ESR spectrum of the irradiated Sample 1 can be associated with the presence of S3●− radical anions. In many microporous minerals including lazurite [6], haüyne [15], kyanoxalite and afghanite [12], and marinellite [14], a similar ESR signal and an absorption band in the 2.0–2.1 eV region associated with S3●− radical anions were previously observed (Table 4). The ESR spectra of the S3●− radical anion in kyanoxalite and afghanite are most close to the ESR spectrum of the irradiated Sample 1 (Table 3).
This ESR signal was not detected in the original balliranoite sample, whereas after irradiation it appears and the color of the sample becomes blue. Since this effect is also observed under far ultraviolet irradiation, one can suppose that photolysis of S4 molecules with the formation of S3●− may take place. Previously, photolysis of S4 molecules with the formation of S2●− was observed upon irradiation with an excimer laser at a wavelength of 248 nm [54]. Given the initial composition of Sample 1, data on the ESR and Raman spectra of irradiated Sample 1, and the fact that the radical anion S3●− is one of the most stable forms of sulfide sulfur [14], the general scheme of the observed radiation-induced transformations of polysulfide species can be written as follows:
S52− → S2●− + S3●−; 3 S2●− → 2 S3●− + e; S4 + S2●− + e → 2S3●−;
S4 + S2●− + e → 2S3●−; S4 + S52− + e → 3S3●− (e = electron).
Observed luminescence (Figure 11) is associated with S2●− radical anions, similarly to other microporous minerals [5,7,12,13,14,37]. The excitation bands at 255–375 nm could be attributed to the transitions to π and π* excited states of S2●− radical anions. However, higher energy excitation bands at 255 and 265 nm may also correspond to the excitation of the balliranoite framework [53].

4.4. Thermal Transformations of Sulfide-Bearing Balliranoite

Changes in the Raman spectrum of sulfide-bearing balliranoite when it is heated are similar to those observed when it is irradiated with X-rays. At high temperatures, the S3●− radical anion is the most stable species containing sulfide sulfur. Moreover, a part of sulfate anions transforms into S3●− on heating.
As it was shown above, heating of Sample 1 in air at 800 °C for 6 h results in the formation of an orthosilicate. This result is unexpected, taking into account that other carbonate cancrinite-group minerals (cancrinite and cancrisilite) transform into a nepheline-type aluminosilicate on heating above 700 °C [55]. On the other hand, the nepheline-related compound carnegieite, Na(AlSiO4), has a polymorph, the orthosilicate NaAl(SiO4), which is stable above 690 °C (URL https://materials.springer.com/isp/crystallographic/docs/sd_1502237 accessed on 24 May 2023). Thus, the hypothetic scheme of transformations of Sample 1 on heating up to 800 °C is: Na5.4K0.1Ca2.4(Si6Al6O24)Cl2[(CO3)0.7(SO4)0.18S*0.95Cl0.1(H2O)0.16] → (Na,K,Ca)(AlSiO4) + Ca-oxydes/chlorides + CO2(gas) + SO2(gas) + H2O(gas); (Na,K,Ca)(AlSiO4) → (Na,K,Ca)Al(SiO4), where (Na,K,Ca)(AlSiO4) is nepheline.
A low-frequency shift of the band of S3●− symmetric stretching vibrations after irradiation (towards 542 cm−1) and especially as a result of heating (towards 535 cm−1 at 600° and 532 cm−1 at 800°) indicates that transformations of different S-bearing groups into S3●− radical anion result in removal of the steric load on the latter.

5. Conclusions

The crystal-chemical data of sulfide-bearing balliranoite from Tultuyskoe (Sample 1) obtained in this work illustrate a very complex chemical behavior of sulfur-bearing and other extra-framework components in feldspathoids belonging to the cancrinite and sodalite groups. The general crystal-chemical formula of Sample 1 is (Na,K,Ca)6Ca2(Si6Al6O24)(Cl,HS)2(CO32−,SO42−,S2●−,S3●−,S4,S52−,Cl,HSnH2O.
The HS and S52− anions occurring in this sample were earlier detected only in three feldspathoids (bystrite, sulfhydrylbystrite, and sapozhnikovite) which crystallized under reducing conditions. The absence of CO2 molecules among extra-framework species and the absence of iron in associated oxygen-bearing minerals (all iron occurs in pyrrhotite) confirm reducing conditions of the formation of sulfide-bearing balliranoite.
The absorption spectrum of balliranoite from Tultuyskoe in the visible range is a superposition of partial spectra of polysulfide groups which are yellow (S2●− and S52−), blue (S3●−), pink (cis-S4), and green (trans-S4) chromophores. Luminescence of this sample is mainly due to S2●− centers.
Radiation-induced transformations of polysulfide species (S2●−, S4●−, cis- and trans-S4, and S52−) in the studied mineral result in the formation of S3●− which is the most stable polysulfide group. However, no radiolysis of CO32−, SO42−, and HS anions was observed.
Thermal transformations of sulfide-bearing balliranoite at 600° result in the transformation of most initial sulfide-bearing groups into S3●− via intermediate S2●−. At 800 °C, decomposition of the aluminosilicate framework and formation of an orthosilicate is observed.

Author Contributions

Conceptualization, N.V.C., A.N.S., R.Y.S. and I.V.P.; methodology, N.V.C., R.Y.S. and M.F.V.; collecting of minerals, A.N.S., N.V.C. and I.V.P.; investigation, R.Y.S., N.V.C., M.F.V., N.V.Z., N.V.P. and D.A.K.; original manuscript draft preparation, N.V.C., R.Y.S. and N.V.Z.; manuscript review and editing, N.V.C., R.Y.S., N.V.Z. and I.V.P.; figures, N.V.C., R.Y.S. and N.V.Z. All authors have read and agreed to the published version of the manuscript.

Funding

Raman: ESR and UV-Vis-near IR spectroscopy, spectroscopy of luminescence, single-crystal X-ray structure study, crystal-chemical analysis and data interpretation and summarizing were supported by the Russian Science Foundation, grant No. 22-17-00006 (for N.V.C., R.Yu.S., N.V.Z., M.F.V., N.V.P. and I.V.P.), https://rscf.ru/project/22-17-00006/ (accessed on 24 May 2023). Identification of minerals, chemical analyses, as well as middle-range IR spectroscopy investigation were carried out in accordance with the state task, state registration No. AAA-A19-119092390076-7 (for N.V.C.).

Data Availability Statement

Not applicable.

Acknowledgments

The authors are grateful to Mikhail V. Voronin for a fruitful discussion.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. Balliranoite (green to greenish yellow, in calcite) from Tultuyskoe (Sample 1). Field of view width: 7 mm.
Figure 1. Balliranoite (green to greenish yellow, in calcite) from Tultuyskoe (Sample 1). Field of view width: 7 mm.
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Figure 2. Crystals of balliranoite from the Somma-Vesuvio volcanic complex (Sample 2). Field of view width: 1 mm.
Figure 2. Crystals of balliranoite from the Somma-Vesuvio volcanic complex (Sample 2). Field of view width: 1 mm.
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Figure 3. Davyne (light blue) in association with lazurite (dark blue), diopside (yellowish grey) and calcite (white) from Sar’e Sang (Sample 3). Field of view width: 18 mm.
Figure 3. Davyne (light blue) in association with lazurite (dark blue), diopside (yellowish grey) and calcite (white) from Sar’e Sang (Sample 3). Field of view width: 18 mm.
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Figure 4. IR spectra of (a) balliranoite from Tultuyskoe (Sample 1), (b) holotype balliranoite (Sample 2) and (c) davyne (Sample 3).
Figure 4. IR spectra of (a) balliranoite from Tultuyskoe (Sample 1), (b) holotype balliranoite (Sample 2) and (c) davyne (Sample 3).
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Figure 5. Uncorrected Raman spectra of (a) davyne (Sample 3), (b) balliranoite from Tultuy (Sample 1) and (c) holotype balliranoite (Sample 2) showing strong fluorescence.
Figure 5. Uncorrected Raman spectra of (a) davyne (Sample 3), (b) balliranoite from Tultuy (Sample 1) and (c) holotype balliranoite (Sample 2) showing strong fluorescence.
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Figure 6. Corrected Raman spectra of (a) balliranoite from Tultuyskoe (Sample 1) and (b) holotype balliranoite (Sample 2).
Figure 6. Corrected Raman spectra of (a) balliranoite from Tultuyskoe (Sample 1) and (b) holotype balliranoite (Sample 2).
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Figure 7. Raman spectra of (a) Sample 1 irradiated with X-rays, (b) Phase 1 in Sample 1 heated in air at 600 °C for 1 h, and (c) Sample 1 heated in air at 800 °C for 6 h.
Figure 7. Raman spectra of (a) Sample 1 irradiated with X-rays, (b) Phase 1 in Sample 1 heated in air at 600 °C for 1 h, and (c) Sample 1 heated in air at 800 °C for 6 h.
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Figure 8. Raman spectrum of Phase 2 in Sample 1 heated in air at 600 °C for 1 h.
Figure 8. Raman spectrum of Phase 2 in Sample 1 heated in air at 600 °C for 1 h.
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Figure 9. Absorption spectra of Sample 1 before irradiation (curve 1), after irradiation with a low-pressure mercury lamp (curve 2), and after irradiation with X-rays (curve 3). Dashed lines show Gaussian components of the absorption spectrum of Sample 1 before irradiation.
Figure 9. Absorption spectra of Sample 1 before irradiation (curve 1), after irradiation with a low-pressure mercury lamp (curve 2), and after irradiation with X-rays (curve 3). Dashed lines show Gaussian components of the absorption spectrum of Sample 1 before irradiation.
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Figure 10. ESR spectrum of irradiated balliranoite (Sample 1). The vertical lines show the signal from S3●− radical anions.
Figure 10. ESR spectrum of irradiated balliranoite (Sample 1). The vertical lines show the signal from S3●− radical anions.
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Figure 11. Luminescence spectrum of Sample 1 excited with a 405 nm radiation (curve 1) and luminescence excitation spectrum of Sample 1 monitored at 650 nm (curve 2), both measured at 77 K.
Figure 11. Luminescence spectrum of Sample 1 excited with a 405 nm radiation (curve 1) and luminescence excitation spectrum of Sample 1 monitored at 650 nm (curve 2), both measured at 77 K.
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Figure 12. Filling of the wide channel in the structure of sulfide-bearing balliranoite (Sample 1). Na-dominant sites are shown as big green balls, C1 site is blue, and (C,S) sites are small light-green balls. Possible S–O and C–O bonds are shown.
Figure 12. Filling of the wide channel in the structure of sulfide-bearing balliranoite (Sample 1). Na-dominant sites are shown as big green balls, C1 site is blue, and (C,S) sites are small light-green balls. Possible S–O and C–O bonds are shown.
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Table 1. Chemical composition (wt.%) of sulfide-bearing balliranoite (Sample 1).
Table 1. Chemical composition (wt.%) of sulfide-bearing balliranoite (Sample 1).
ComponentSpot Analysis No.Mean
12345
Na2O15.0015.0914.9014.7914.9514.95
K2O0.780.510.510.370.590.55
CaO12.8112.8412.8613.9113.4713.17
Al2O327.1728.0427.8728.0027.6527.75
SiO233.1132.5532.5432.8232.6532.73
SO38.328.838.867.347.788.23
Cl6.656.736.756.576.946.73
–O≡Cl−1.50−1.52−1.52−1.48−1.57−1.52
CO2-----2.75
H2O-----0.27
Total102.34103.07102.77102.32102.46105.61
Note: All sulfur is given as SO3.
Table 2. Raman bands of the studied balliranoite samples and their assignment.
Table 2. Raman bands of the studied balliranoite samples and their assignment.
Sample 1Sample 2Assignment
Wavenumber (cm−1)
202Lattice mode involving libration vibrations of
extra-framework components
209s trans-S4 bending mode (overlapping with S52− bending band) and mixed lattice modes
263 S3●− bending mode (ν2) and/or S52− bending band
293 cis-S4●− bending or Na–O stretching vibrations
343w cis-S4 mixed mode
439s, 454s425s, 457sSO42− [E2) mode] (overlapping with S52− stretching bands for Sample 1)
497 trans-S4 symmetric stretching mode
544s S3●− symmetric stretching (ν1) (possibly, overlapping with the antisymmetric stretching band of gauche- or trans-S4)
565 S5●− stretching or S3●− antisymmetric stretching (ν3) mode
596 S2●− stretching mode
671622, 668SO4 bending (ν4–F2) mode
717w719wCO32− in-plane bending vibrations
775wFramework mixed band
830 (broad) S3●− combination mode (ν1 + ν2) overlapping with framework mixed and overtone of S52− stretching bands
986s987sSO42− symmetric stretching (ν1–A1) mode
10121022Framework and/or SO32− stretching vibrations
1056s1056sCO32− symmetric stretching vibrations
1087 CO32− symmetric stretching vibrations [possibly, overlapping with SO4●− stretching band (ν3–F2)]
1130sh1105w, 1140wSO42− asymmetric (ν3–F2) mode [possibly, overlapping with S2●− overtone (2 × ν1)]
1640w S3●− overtone (3 × ν1)
2564w HS stretching mode
Note: w—weak band, s—strong band, sh—shoulder.
Table 3. Assignment of Raman bands of the products of irradiation of Sample 1 with X-rays and its heating at 600 °C for 1 h (Phase 1).
Table 3. Assignment of Raman bands of the products of irradiation of Sample 1 with X-rays and its heating at 600 °C for 1 h (Phase 1).
Irradiated (Sample 1)Heated (Phase 1)Assignment
Wavenumber (cm−1)
209166s, 206Low-frequency lattice modes
257262S3●− bending mode (ν2) and/or S52− stretching mode
280w289wLattice modes involving Na+ cations
421 S52− stretching mode 1 or framework bending vibrations
461451SO42− [E2) mode] overlapping with S52− stretching bands
542s535sS3●− symmetric stretching (ν1) and/or AlF6 stretching mode
578S3●− antisymmetric stretching (ν3), possibly, overlapping with the stretching band of S2●−
815w787S3●− combination mode (ν1 + ν2)
983988SO42− symmetric stretching vibrations [A11) mode]
1061, 1083s1069sCO32− symmetric stretching vibrations
1363w1340wS3●− combination mode (2ν1 + ν2)
16291604S3●− overtone (3 × ν1)
1860w1858wS3●− combination mode (3 × ν2 + ν1)
21652133S3●− overtone (4 × ν1)
2369wS3●− combination mode (4 × ν2 + ν1)
2563w2560wHS stretching mode
2712w2668wS3●− overtone (5 × ν1)
29792933wS3●− combination mode (5 × ν1 + ν2)
3140wS3●− overtone (6 × ν1)
Table 4. Bands of S3●− in ESR and optical absorption spectra of feldspathoids.
Table 4. Bands of S3●− in ESR and optical absorption spectra of feldspathoids.
Mineralg-Factor ComponentsAbsorption Maximum (eV)
Kyanoxalite2.050, 2.038, 2.002 [12]2.09 [12]
Afgranite2.057–2.060, 2.038, 2.002 [12]2.09 [12]
Haüyne2.056, 2.041, 2.008 [15]2,05 [15]
Haüyne2.046, 2.031, 2.010 [5]2.06 [5]
Nosean2.041, 2.031, 2.004 [12]2.07 [14]
Lazurite2.030, 2.030, 2.030 [6]2.07 [5]
Vladimirivanovite2.034, 2.004 [14]2.00 [14]
Marinellite2.039, 2.008 [14]2.10 [14]
Biachellaite2.058, 2.036, 2.002 [14]No data
Balliranoite2.053, 2.040, 2.001 (this work)2.1 [14]
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Chukanov, N.V.; Sapozhnikov, A.N.; Shendrik, R.Y.; Zubkova, N.V.; Vigasina, M.F.; Potekhina, N.V.; Ksenofontov, D.A.; Pekov, I.V. Crystal Chemistry, Thermal and Radiation-Induced Conversions and Indicatory Significance of S-Bearing Groups in Balliranoite. Minerals 2023, 13, 822. https://doi.org/10.3390/min13060822

AMA Style

Chukanov NV, Sapozhnikov AN, Shendrik RY, Zubkova NV, Vigasina MF, Potekhina NV, Ksenofontov DA, Pekov IV. Crystal Chemistry, Thermal and Radiation-Induced Conversions and Indicatory Significance of S-Bearing Groups in Balliranoite. Minerals. 2023; 13(6):822. https://doi.org/10.3390/min13060822

Chicago/Turabian Style

Chukanov, Nikita V., Anatoly N. Sapozhnikov, Roman Yu. Shendrik, Natalia V. Zubkova, Marina F. Vigasina, Nadezhda V. Potekhina, Dmitry A. Ksenofontov, and Igor V. Pekov. 2023. "Crystal Chemistry, Thermal and Radiation-Induced Conversions and Indicatory Significance of S-Bearing Groups in Balliranoite" Minerals 13, no. 6: 822. https://doi.org/10.3390/min13060822

APA Style

Chukanov, N. V., Sapozhnikov, A. N., Shendrik, R. Y., Zubkova, N. V., Vigasina, M. F., Potekhina, N. V., Ksenofontov, D. A., & Pekov, I. V. (2023). Crystal Chemistry, Thermal and Radiation-Induced Conversions and Indicatory Significance of S-Bearing Groups in Balliranoite. Minerals, 13(6), 822. https://doi.org/10.3390/min13060822

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