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Article

The Effects of High-Grade Metamorphism on Cr-Spinel from the Archean Sittampundi Complex, South India

1
Department of Mathematics and Geosciences, University of Trieste, 34128 Trieste, Italy
2
Department of Earth Sciences, Manipur University, Imphal 795003, India
3
Department of Environmental Sciences, University of Derby, Derby DE22 1GB, UK
4
Department of Geosciences, Swedish Museum of Natural History, SE-10405 Stockholm, Sweden
*
Authors to whom correspondence should be addressed.
Minerals 2021, 11(12), 1370; https://doi.org/10.3390/min11121370
Submission received: 7 October 2021 / Revised: 29 November 2021 / Accepted: 30 November 2021 / Published: 3 December 2021

Abstract

:
We investigated the crystal and structural behavior of Cr-bearing spinels from the Archean chromitites of Sittampundi (India), which had been subjected to very high-grade metamorphism. The structural data show that their oxygen positional parameters are among the highest ever recorded for Cr-bearing spinels with similar Cr# and Mg# and very similar to those found for other Archean occurrences. The general agreement between electron microprobe and Mössbauer data indicates that the analyzed spinels are stoichiometric. It is therefore most likely that the PH2O and Ptotal values as well as both the oxygen fugacity and the temperature reached during high-grade metamorphism inhibited the possibility of the non-stoichiometry of chromites, contrary to what can happen in ophiolites, where non-stoichiometry has recently been documented.

1. Introduction

The Neoarchaean Sittampundi Complex in southern India [1] is a metamorphosed anorthositic complex within the Palghat–Cauvery Suture Zone (PCSZ), preserving an original igneous stratigraphy, including chromitites overprinted by high-grade metamorphic assemblages [2,3,4,5] that, according to Sajiev et al. [6,7], could be retrograded from eclogite-facies assemblages.
Cr-spinel is useful as an indicator of the crystallization condition in a wide range of geological environments. It also records modifications induced during subsequent prograde or retrograde metamorphism of host rocks. The chemical durability of the chromite makes it useful as a petrogenetic indicator in ultramafic rocks in which metamorphic recrystallization has obliterated other primary fingerprints [8,9,10]. Changes in the composition and structure of chromite from ultramafic complexes during metamorphic modification have been studied by several researchers [11,12,13,14]. The relationships between compositional and structural parameters in natural Cr-spinels have been considered by several authors, providing a new approach to the understanding of mechanisms of spinel crystallization in magmatic and metamorphic environments [15,16,17,18,19,20,21,22,23]. The intracrystalline distribution of cations in spinels is a function of the thermodynamic parameters, including temperature, pressure and composition. Natural samples exhibit a non-equilibrium distribution of cations that depends on the thermodynamic parameters controlling the equilibrium order and the pressure-temperature-time path the crystals experienced. The ordering process involves short-range diffusion of cations, along with the breaking of bonds and a large kinetic barrier [24]. The equilibrium temperature corresponding to the observed order of a sample is called its closure temperature, TC [25]; TC provides insight on (1) a lower limit of the maximum temperature that the rock experienced and (2) a comparative cooling rate. Although the geothermometer modelled by [26] is mainly used for Mg-Al spinels, [27] found out that is suitable for Cr-rich compositions as well. The commonly used intercrystalline thermometers are those by [28,29], using olivine-Cr-spinel pairs, even if [30] showed that they do not always show an appropriate equilibration temperature.
In this study, we report the results of a structural-chemical investigation of chromite crystals extracted from the chromitite seams hosted by meta-anorthosite from the Sittampundi complex. We have taken up this work (a) to increase the database for Cr-spinels in chromitites of high-alumina continental layered intrusions, as crystal-chemical studies on spinels from layered chromitites are limited to a few places only, such as the Bushveld, Stillwater, Rum and Amsaga complexes [31,32,33,34] and Fiskenæsset [35] and (b) to verify whether relationships exist between the structural and compositional parameters of the spinels and a high grade of metamorphism of the chromitites.

2. Geology and Petrography

The Sittampundi complex belongs to the metamorphosed Archean layered anorthosite complex. The study area forms a part of the granulite terrane of south India. Major rock types are chromitite-bearing meta-anorthosite, amphibolite, basic granulite, two-pyroxene granulite, leptynite, biotite gneiss and pink granite. Subramanian [2] carried out a detail systematic study of the Sittampundi complex (Figure 1).
Sajeev et al. [6] reported retrogressed eclogite within the orthopyroxene free meta-gabbro, with the garnet of the rock hosting needles of rutile and omphacite. They suggested the assemblage as the peak eclogite facies condition of the rock. However, several authors have suggested that the high-grade metamorphism of the Sittampundi complex culminated at 11–12 Kbar pressure and 700–800 °C [37,38,39]. The peak metamorphic conditions were later overprinted by fluid influx and decompression-related retrograde a ssemblages. Although there is local preservation of primary igneous textures, almost all the primary minerals recrystallized during the high-grade metamorphism and obliterated the igneous textures and minerals. Felsic magma intruded the Sittampundi layered Complex at about 2.51 Ga, and, successively, the rock sequence underwent granulite facies (2450–2500 Ma) and amphibolite facies (500–720 Ma) metamorphism. The amphibolite facies metamorphism caused the modification of some chromites to Cr-poor green spinel [40]. Chromitite occurs exclusively within meta-anorthosite as discontinuous layered bands/lenses of varying thickness, with a maximum of 5 m within anorthosites and consisting of more than 60% chromite grains.
Earlier workers reported that the chromitites contain FeAl-rich chromites concentrated in layers between amphibole-rich layers, with a dominant mineralogy of amphibole − spinel − plagioclase ± sapphirine [7,36,41]. These authors suggested the existence of original highly calcic plagioclase (>An95), FeAl-rich chromite and magmatic amphibole, which are consistent with a derivation from a parental magma of hydrous tholeiitic composition.
Samples used for crystal-chemical investigation were culled from chromitites (chromite + rutile + calcic amphibole ± anthophyllite ± clinochlore). The samples studied were collected from conformable chromitite lenses within meta-anorthosite (Figure 2a) on a foot track in the western part of Karungalpatti, Salem District, Tamil Nadu.
According to [40], chromite compositions in Sittampundi show large variations in their chemical parameters, such as Cr/(Cr + Al) (Cr# = 0.26–0.60), Mg/(Mg + Fe2+) (Mg# = 0.40–0.45) and Fe3+/(Fe3+ + Al + Cr) (Fe3+# = 0.20–0.24), depending on textural type and nature of the associated phases, and occur within discontinuous bands within clinopyroxenite and highly calcic anorthosite. Previous Mössbauer studies on some chromites from Sittampundi, developed by [42], show that Fe2+ and Fe3+ occur at both tetrahedral and octahedral sites and that the Fe3+/ΣFe ratio is in the range 0.45–0.48. The oxygen positional parameters reported in that paper, calculated through chemical and Mössbauer analyses, are 0.2561 and 0.2603. While the first one is rather unreliable, being very similar to those of completely inverted spinels such as magnetite, the second value is rather close to that of 0.2607 recorded in an oxidized Cr-spinel recovered from a terra rossa soil [43]. Another study on Cr-spinel from Sittampundi is the one by [44], which, following those of [45,46,47] among the others, studied the Raman shifts of these samples.
Chromite occurs as granular aggregates in close association with amphiboles in the meta-anorthosite hosted chromitites. The rock shows a schistose texture, displaying the preferred orientation of amphiboles. Chromite, amphibole, chlorite and plagioclase form the major components. Chromite is also present as inclusions within the amphibole (Figure 2c). Chromite abundance is between 40% and 75% in the studied samples. The original igneous texture of the chromitite, such as chromite cumulate texture, igneous layering, etc., is preserved. The chromite grains are euhedral to subhedral (Figure 2c,d). Euhedral chromite grains are in common with well-defined grain boundaries and fracture zones. Some chromite grains of pseudohexagonal grain boundaries indicate their recrystallization (Figure 2b).

3. Materials and Methods

3.1. X-ray Single Crystal Diffraction

In total, four Cr-spinels have been analyzed by means of X-ray single crystal diffraction and electron microprobe. X-ray diffraction data were recorded on an automated KUMA-KM4 (K-geometry) diffractometer (KUMA, Wroclaw, Poland), using MoKα radiation, monochromatized by a flat graphite crystal. Data were collected, according to [48], with up to 55° of 2θ in the ω-2θ scan mode (scan width 1.8°2θ, counting times from 20 to 50 s, depending on the peak standard deviation). Twenty-four equivalent reflections of (12, 8, 4), at about 80° of 2θ were accurately centered at both sides of 2θ, and the α1 peak barycenter was used for cell parameter determination. Structural refinement using the SHELX-97 program [49] was carried out against Fo2hkl in the Fd-3m space group (with the origin at −3 m), since no evidence for different symmetry appeared. Scattering factors were taken from [50,51]. The crystallographic data are presented in Table 1.

3.2. Electron Microprobe Analysis

Ten to fifteen spot analyses were performed on the same Cr-spinels used for X-ray data collection, using a CAMECA-SX50 electron microprobe (EPMA) (CAMECA, Gennevilliers Cedex, France) at IGG-CNR (Istituto di Geoscienze e Georisorse-Consiglio Nazionale delle Ricerche, Padua, Italy), operating at 15 kV and 15 nA. A 20 s counting time was used for both peak and total background. Synthetic MgCr2O4 and FeCr2O4 spinels were used for Mg, Cr and Fe determination, Al2O3 for Al, MnTiO3 for Ti and Mn, NiO for Ni and sphalerite for Zn. The following diffracting crystals were used: TAP for Al and Mg, PET for Ti and Ti, and LIF for Cr, Fe, Mn, Ni, V and Zn. Raw data were reduced by a PAP-type correction software provided by CAMECA. The mineral chemical analyses are reported in Table 1.

3.3. Cation Distribution

According to [52,53], several different procedures may be adopted to determine cation distribution; satisfactory results can generally be obtained by combining data from single-crystal X-ray structural refinements and electron microprobe analyses. In fact, this approach simultaneously takes into account both the structural and chemical data, reproducing the observed parameters by optimizing cation distributions. Differences between measured and calculated parameters are minimized by a function F(x), taking in consideration different observed quantities such as a0, u, T- and M- m.a.n. (mean atomic number), atomic proportions, and constraints imposed by the crystal chemistry (total charges and T and M site populations). Several minimization cycles of F(x) were performed up to convergence. A summary of the procedure can be found in [54]. The obtained cation distributions are listed in a in Table 1.

3.4. Mössbauer Spectroscopic Analysis

Optical examination of the samples show minute amounts of opaque phases (magnetite) at the grain boundaries, which could be magnetically separated after crushing each to a fine powder under acetone.
Clean chromite crystals were selected under an optical microscope. About 50 mg of each sample was used, distributed as 28 mg/cm2 of sample in the sample holder, as calculated via RECOIL 1.04 computer software [55,56]. Room temperature Mössbauer measurements were carried out on clean chromite separates with a 25 mCi57Co source in a Rh matrix, which was driven at constant acceleration in a triangular mode. The Doppler energies from the 14.4 keV γ-rays were detected with a YAlO3:Ce scintillation counter. Mössbauer measurements were repeated on replicas of all samples to check the consistency of our measurements.
MossA (ver. 1.01a), a computer program developed by Prescher et al. [57], utilizing a full transmission integral with a normalized Lorentzian source line-shape, was used to fit the Lorentzian lines of the folded data. A fitting model consisting of three doublets assigned to Fe2+ and one doublet assigned to Fe3+, as used by Lenaz et al. [58], was adopted to fit the spectra. In addition, to obtain accurate quantification of Fe3+/ΣFe for the chromite spectra, correction for the difference between the recoil-free fractions was applied to the chromite doublets for Fe2+ and Fe3+ at the tetrahedral and octahedral sites, respectively, at room temperature, based on previous studies [59,60,61,62], and calculated from the sample composition and the procedure enumerated.
For accurate quantification of Fe3+/ΣFe for the chromite spectra, we used the following unified equation, which incorporates the recoil free fractions, 0.687 and 0.887, for the observed Fe2+ and Fe3+, respectively:
Fe 3 + Σ Fe = [ 1 1 ( 0.7745 x R + 1 ) ]
where R is the (Fe3+/Fe2+) ratio of the observed Fe-cations in the chromite doublets.
Mössbauer parameters obtained for centroid shift δ, quadrupole splitting, ΔEQ and the full width at half-maximum Γ, together with the averages of (Fe3+/∑Fe) ratios for the samples and their respective replicas, are shown in Table 2. The identification of criteria for Fe-cation sites is based on the relative centroid shift δ-values, following previous reports by [62,63,64]: [δ-Fe3+T] < [δ-Fe3+M] < [δ-Fe2+T] < [δ-Fe2+M]. The site occupancy was determined from the area ratios of the doublets.

4. Results

The composition of the analyzed grains of Cr-spinel is quite similar to Cr# in the range 0.46–0.49 and Mg# in the range 0.32–0.44, as calculated from analyses where Cr2O3 is in the range 35–39 wt.%, Al2O3 24–27 wt.%, MgO 7–9 wt.% and FeOtot 28–30 wt.% (Table 1). Other oxides that were detected are MnO, TiO2 and NiO, with concentrations below 0.30 wt.%.
The structural parameters considered are the cell edges that range between 8.2364 (4) and 8.2477 (4) Å and the oxygen positional parameter, u, between 0.2633 (1) and 0.2637 (1). This last parameter is related to the oxygen packing distortion within the lattice. The ideal cubic-close packed structure shows u = 0.25, but it is observed that u is higher than 0.25 for all four samples of Cr-bearing spinels. The observed distortion is a consequence of similar M-O and T-O bond distances (u = 0.2625 when distances are equal) [65]. Previous studies suggested that 0.2625 and, consequently, the T-O and M-O bond distances are related to the cooling history experienced by the mineral. Slow cooling allows the cations to accommodate at their preferred site, i.e., trivalent cations at the octahedral M site and divalent cations at the tetrahedral T site. On the contrary, rapid cooling causes a disordered cation distribution between the two sites, with trivalent and divalent cations in both T and M sites. As can be seen in Table 1 and Table 2, the values found for these Cr-spinels are among the highest recorded u values, thereby pointing to very slow cooling rates. The degree of inversion, i, i.e., the amounts of trivalent cations at T site or divalent cations at M site, is in the range of 0.066–0.092 atoms per formula unit.
Figure 3 shows spectra of samples 5B and 30B_rep, as typical examples of Mössbauer spectra, for a four-doublet fitting model, which provided a good χ2–value for the fitting of the Sittampundi chromite spectra. As the spectra show limited resolution, which is typical for this type of chromite, the assignment of individual doublets to specific sites is uncertain. However, the Fe3+/ΣFe ratios obtained are considerably more reliable, as the Fe3+ absorption is well constrained by the asymmetry of the two main high- and low-velocity components in the measured spectra, where the Fe3+ contribution occurs entirely within the low-velocity component.
Table 2 shows the room temperature Mössbauer data for (a) all samples and (b) the repeated runs on replicas. The calculated average of their respective corrected (Fe3+/Fe) ratios in the Tables are, 0.13, 0.17 and 0.10, respectively.
According to microprobe analyses, structural refinement and Mössbauer analyses data, the values of (Fe3+/ΣFe) ratios in the Sittampundi chromite-spinels are in the range 10–18%. However, on the basis of the values of the quadrupole splittings of the Fe3+ doublets, it appears all Fe3+ ions preferentially occupy the T-site.

5. Discussion

In terms of mineralogy and field relations, the Sittampundi chromitites are remarkably similar to anorthosite-hosted chromitites in the Neoarchean Fiskenæsset anorthositic complex, Greenland. In Figure 4, we compare the structural parameters of the studied Cr-spinels with those of other occurrences that are similar in age. In fact, there are some other Archean occurrences, such as the Fiskenæsset and Ujragassuit (Greenland) [35], Amsaga (Mauritania) [34], Inyala and Rhonda (Limpopo belt, Zimbabwe) [35], detrital Cr-spinels from Banavara [66], as well as the Bushveld and Stillwater Complexes [31,33]. Moreover, the figure comprises the Cr-spinels in seams entrapped within anorthosites from the Paleogene Rum Layered Complex [32].
In Amsaga, the chromites can be found associated with different matrix minerals, according to the metamorphic grade that affected the rocks. Those with the higher u values are metamorphosed in amphibolite facies and are very close to the parameters exhibited by Sittampundi Cr-spinels. Fiskenæsset chromitites, even if their paragenesis also includes pargasitic amphiboles, as in Sittampundi, have to be considered as primary and not metamorphosed [67,68]. In order to estimate the intracrystalline closure temperatures of the Cr-spinels, we applied to our samples the geothermometer of [26]. This geothermometer takes into account the Mg and Al content of the Cr-spinels and their distribution amongst the octahedral and tetrahedral sites. The presence of other cations is accounted for by coefficients present in the equation of the geothermometer. The calculated intracrystalline closure temperature (Tc) for the Sittampundi Cr-spinels is in the range of 715–965 °C. The computed intracrystalline closure temperature is more or less in agreement with the temperature obtained by topological constraints and quantitative geothermometry of the area [39,41]. In Figure 5, we compare these temperatures with those of Rum, Fiskenæsset and Amsaga complexes. It is possible to see that those from Rum are the lowest (521–653 °C), while the others are more or less comparable.
It is interesting to note that Amsaga Cr-spinels record an intracrystalline closure temperature higher than that of the amphibolite facies; thus, it is possible they still retain the primary closure temperature after crystallization. Sittampundi Cr-spinels underwent a granulite facies metamorphism. Sunder Raju [70] noticed that the pristine composition of the chromites is preserved despite intense metamorphic and tectonic processes. In this case, the highest temperatures are comparable with those of the metamorphism, but they extend down to about 700 °C. It is pertinent to remember that the intracrystalline closure temperature is the temperature recording the last Mg-Al exchange between T and M sites and not the temperature of crystallization. Thus, they suffered a high temperature metamorphism and then slowly cooled until their actual Tc was achieved.
In the past few years, some papers have dealt with the possibility of non-stoichiometry in Cr-spinels from different occurrences. This was determined using a combination of techniques, including structural refinement, electron microprobe and Mössbauer analysis. The authors [18,71,72] found some Cr-spinels from ophiolites to be non-stoichiometric, i.e., showing structural vacancies in the lattice due to the oxidation of Fe2+ to Fe3+. Furthermore, some authors [73,74] also documented the existence of minor vacancies in Cr-spinels from the Bushveld layered complex and some Antarctica mantle xenoliths, respectively. However, when the same combined approach was used for other ophiolites (Shetland, UK, [75]; Leka, Norway, [76]) and the Amsaga complex in Mauritania ([34], no vacancies were detected. Using both the conventional- and point-57Co-source methods, [58] showed how, in some cases, there can be large discrepancies in the (Fe3+/ΣFe) ratios calculated via structural refinement, electron microprobe and Mössbauer analyses. The reason, for example, is that the larger samples used in conventional Mössbauer techniques include several different grains, which could have a range of very different degrees of oxidation. Here, we can see that the values of Fe3+/ΣFe obtained for the Sittampundi Cr-spinels using various experimental techniques are very similar, thus allowing us to conclude that these samples of spinel are stoichiometric.
Although chemical modifications related to sub-solidus re-equilibration and metamorphic hydrothermal processes can significantly influence the primary high-T composition of Cr-spinel, the composition of chromite in chromitite bodies can still be used as a petrogenetic and geotectonic indicator [77]. Suita and Streider [78] showed that the core of Cr-spinel grains in massive chromitites conserves the primary chemical composition, regardless of the metamorphic changes. Notably, the degree of metamorphic re-equilibration in metamorphosed chrome-spinels depends on the ratio of PH2O and Ptotal. According to [79], when PH2O is about 25% of Ptotal, a complete metamorphic re-equilibration occurs; however, where it is lower, relict igneous cumulate textures are preserved. In fact, ref. [80] suggested that in high pressure conditions, there is no resetting of the primary igneous composition of chromites. The composition of mantle fluid phases attending magmatic and metasomatic processes strongly depends on oxygen fugacity (fO2). So, in the C-H-O system, the fluid phase consists mainly of CO2 and H2O in relatively oxidizing conditions close to the fayalite-magnetite-quartz (FMQ) solid buffer, H2O and CH4 in moderately oxidizing conditions between the FMQ and iron-wüstite (IW) buffers, and CH4 below IW [81]. For Albanian ophiolites, [82] found that the pre-oxidation Δlog(fO2)FMQ values range from −3.2 to +2.3 log units, with most values close to or higher than the FMQ buffer, while the post-oxidation Δlog(fO2)FMQ values are systematically the highest, ranging from +0.5 to +2.9 log units. A report by [62] showed that there are two groups of spinels in ophiolites from Oman, with different oxygen fugacities. The calculated oxygen fugacities for the low Fe3+/ΣFe ratio group are between 1.9 and 2.7 log units above the FMQ buffer, while samples from the high Fe3+/ΣFe ratio group yield higher oxygen fugacities, between 3.2 and 3.4 log units above the FMQ buffer. It is therefore most likely that the PH2O and Ptotal values, as well as both the oxygen fugacity and the temperature reached during different processes, inhibits the possibility of non-stoichiometry of chromites from amphibolite-granulite-eclogite facies, as in Amsaga and Sittampundi, contrary to what can happen in ophiolites.

6. Conclusions

According to the combined results from structural refinement, electron microprobe and Mössbauer analyses of the Sittampundi Cr-spinels, the following can be concluded:
(i)
Oxygen parameters of the studied Cr-spinels are close to the Amsaga chromites.
(ii)
The computed intracrystalline closure temperature of the Cr-spinels is comparable to the reported temperatures obtained by topological constraints and quantitative geothermometry.
(iii)
Estimated values of Fe3+/ΣFe ratios obtained by using different techniques are similar and establish that the studied Sittampundi Cr-spinels are stoichiometric.
(iv)
Structural refinement study of Cr-spinels could be important in discriminating the various tectonic domains.

Author Contributions

Conceptualization, D.L. and B.M.; methodology, D.L., B.M., J.A. and H.S.; formal analysis, D.L., B.M., J.A. and H.S.; writing—original draft preparation, D.L., B.M., J.A. and H.S.; writing—review and editing, D.L. and B.M. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Data Availability Statement

Not applicable.

Acknowledgments

The Italian C.N.R. financed the installation and maintenance of the microprobe laboratory in Padua. R. Carampin and L. Tauro are kindly acknowledged for technical support. H.S. acknowledges support from the Swedish Research Council. J.A would like to thank the College of Science and Engineering, University of Derby, for their support in his Mössbauer spectroscopy research. B.M. would like to thank S. Mitra for the encouragement to carry out this research work.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. Geological map of the Sittampundi Complex. Modified from [2,36].
Figure 1. Geological map of the Sittampundi Complex. Modified from [2,36].
Minerals 11 01370 g001
Figure 2. (a) Field photograph of discontinuous chromite seam hosted by meta-anorthosite. Person is for reference; (b) photomicrograph of polygonal faceted chromite grains within non-porous chromite; (c) chromite grains with silicate inclusions surrounded by intercumulus amphiboles; (d) back-scattered electron image of a representative chromite grain; exsolved rutile needles are seen as white needles.
Figure 2. (a) Field photograph of discontinuous chromite seam hosted by meta-anorthosite. Person is for reference; (b) photomicrograph of polygonal faceted chromite grains within non-porous chromite; (c) chromite grains with silicate inclusions surrounded by intercumulus amphiboles; (d) back-scattered electron image of a representative chromite grain; exsolved rutile needles are seen as white needles.
Minerals 11 01370 g002
Figure 3. Examples of 57Fe Mössbauer spectra obtained at room temperature for samples 5B and 30B rep. Fitted absorption doublets assigned to Fe2+ and Fe3+ are indicated in blue and red colors, respectively. Diamond symbols denote measured spectra, and the black curves represent summed fitted spectra.
Figure 3. Examples of 57Fe Mössbauer spectra obtained at room temperature for samples 5B and 30B rep. Fitted absorption doublets assigned to Fe2+ and Fe3+ are indicated in blue and red colors, respectively. Diamond symbols denote measured spectra, and the black curves represent summed fitted spectra.
Minerals 11 01370 g003
Figure 4. Oxygen positional parameter, u, versus cell edge, a. Black circles: Cr-spinels from Sittampundi (this study); red circles: detrital Cr-spinels from Banavara [66]; grey circles, squares and star: Cr-spinels from Amsaga (Mauritania) in amphibole, chlorite and talc-serpentine matrix, respectively [34]; yellow, purple and green circles: Cr-spinels from Fiskenaesset and Ujragassuit (Greenland) and Zimbabwe, respectively [35]; blue squares: Cr-spinels from Rum (Scotland) [32]; green field: Cr-spinels from Bushveld and Stillwater complexes [31,33]; yellow field: Cr-spinels from Nuggihalli komatiites [69].
Figure 4. Oxygen positional parameter, u, versus cell edge, a. Black circles: Cr-spinels from Sittampundi (this study); red circles: detrital Cr-spinels from Banavara [66]; grey circles, squares and star: Cr-spinels from Amsaga (Mauritania) in amphibole, chlorite and talc-serpentine matrix, respectively [34]; yellow, purple and green circles: Cr-spinels from Fiskenaesset and Ujragassuit (Greenland) and Zimbabwe, respectively [35]; blue squares: Cr-spinels from Rum (Scotland) [32]; green field: Cr-spinels from Bushveld and Stillwater complexes [31,33]; yellow field: Cr-spinels from Nuggihalli komatiites [69].
Minerals 11 01370 g004
Figure 5. Range of intracrystalline closure temperatures (°C) for the spinel composition investigated and other occurrences of Cr-spinels from chromitites in anorthosites used for comparison (Fiskenæsset, unpublished data; Amsaga [34]; Rum [32]).
Figure 5. Range of intracrystalline closure temperatures (°C) for the spinel composition investigated and other occurrences of Cr-spinels from chromitites in anorthosites used for comparison (Fiskenæsset, unpublished data; Amsaga [34]; Rum [32]).
Minerals 11 01370 g005
Table 1. Results of structure refinement, chemistry and cation distribution. a: cell parameter (Å); u: oxygen positional parameter; R1: all (%); wR2: (%); GooF: as defined in [40]; Cr#: Cr/(Cr + Al); Mg#: Mg/(Mg + Fe2+); Fe3+#: Fe3+/(Fe3+ + Cr + Al); Tc: intracrystalline closure temperature (°C), calculated by using [26] geothermometer.
Table 1. Results of structure refinement, chemistry and cation distribution. a: cell parameter (Å); u: oxygen positional parameter; R1: all (%); wR2: (%); GooF: as defined in [40]; Cr#: Cr/(Cr + Al); Mg#: Mg/(Mg + Fe2+); Fe3+#: Fe3+/(Fe3+ + Cr + Al); Tc: intracrystalline closure temperature (°C), calculated by using [26] geothermometer.
Sample5B24B30A30B
XRDa8.2364 (4)8.2477 (3)8.2448 (4)8.2399 (4)
u0.26355 (5)0.26360 (6)0.2633 (1)0.2637 (1)
R11.832.102.562.72
wR23.924.126.086.33
GooF1.1861.3111.2441.198
EMPAMgO8.2 (1)6.80 (9)9.2 (3)6.8 (1)
Al2O327.6 (2)27.3 (3)24.1 (7)26.7 (3)
TiO20.22 (4)0.14 (3)0.23 (2)0.14 83)
Cr2O335.8 (4)36.0 (5)38.5 (8)36.4 (3)
MnO0.23 (3)0.26 (3)0.23 (3)0.26 (3)
FeOtot29.3 (4)30.2 (2)28.5 (2)30.2 (3)
NiO0.20 (3)0.12 (3)0.13 (3)0.13 (4)
Sum101.6100.8100.9100.7
T-site
Mg0.3390.2740.36440.2578
Al0.00330.02980.01010.0353
Fe2+0.56220.64880.53570.6557
Fe3+0.08660.03620.08170.0393
Mn0.0060.00690.00610.0069
Zn0.00250.00410.00160.0046
Cation distributionM-site
Al1.01870.98040.94440.9715
Cr0.86790.88540.91220.8958
Mg0.03750.04250.06830.0609
Fe2+0.04540.02190.02080.0061
Fe3+0.01860.0630.04430.057
Ni0.00490.0030.00320.0033
Ti0.0050.00330.00540.0033
Cr#0.460.480.490.47
Mg#0.380.320.440.33
Fe#0.050.050.060.05
Tc715924754966
Table 2. Mössbauer parameters and corrected (Fe3+/ΣFe) ratios obtained from (a) measurements of samples and (b) repeated measurements of three replica samples, respectively. δ = centroid shift (mm/s), ΔEQ = quadrupole splitting (mm/s), Γ = full width at half-maximum (mm/s). The averages of (Fe3+/∑Fe) ratios for the samples and their respective replicas are reported in this study.
Table 2. Mössbauer parameters and corrected (Fe3+/ΣFe) ratios obtained from (a) measurements of samples and (b) repeated measurements of three replica samples, respectively. δ = centroid shift (mm/s), ΔEQ = quadrupole splitting (mm/s), Γ = full width at half-maximum (mm/s). The averages of (Fe3+/∑Fe) ratios for the samples and their respective replicas are reported in this study.
Samples
(a)
δ
(mm/s)
ΔEQ
mm/s
Γ
(mm/s)
% AreaOxidation Stateχ2
(±0.126)
(Fe2+/ΣFe)(Fe3+/ΣFe)(Fe3+/Fe2+)(Fe3+/ΣFe) Corrected
5B0.927
0.920
0.878
0.347
1.454
0.883
2.155
0.657
0.246
0.221
0.201
0.142
40.000
21.200
18.600
20.490
Fe2+
Fe2+
Fe2+
Fe3+
1.0779.8020.490.260.166
24B0.934
0.919
0.901
0.348
1.479
0.915
2.133
0.651
0.446
0.431
0.401
0.257
36.412
25.282
21.989
16.316
Fe2+
Fe2+
Fe2+
Fe3+
1.0483.6816.320.200.131
30A0.935
0.926
0.917
0.364
1.402
2.042
0.853
0.616
0.396
0.38
0.392
0.256
31.303
25.614
22.005
21.078
Fe2+
Fe2+
Fe2+
Fe3+
1.0278.9221.080.270.168
30B0.934
0.930
0.917
0.345
1.489
0.910
2.084
0.660
0.424
0.413
0.359
0.225
37.298
30.121
19.896
12.684
Fe2+
Fe2+
Fe2+
Fe3+
1.1287.3212.680.150.101
Samples
(b)
5B
replica
0.934
0.914
0.878
0.340
1.521
0.951
2.188
0.664
0.427
0.473
0.381
0.272
31.032
29.045
18.808
21.118
Fe2+
Fe2+
Fe2+
Fe3
1.2978.8921.130.280.172
24B
replica
0.934
0.922
0.898
0.353
1.452
0.905
2.090
0.653
0.437
0.425
0.407
0.241
34.034
25.467
25.320
15.180
Fe2+
Fe2+
Fe2+
Fe3+
1.3384.8215.180.180.126
30A
replica
0.939
0.936
0.920
0.359
1.461
2.075
0.895
0.621
0.397
0.369
0.405
0.262
31.041
23.495
24.758
20.707
Fe2+
Fe2+
Fe2+
Fe3+
1.3579.2920.710.260.170
30B
replica
0.932
0.920
0.904
0.360
1.397
0.852
2.012
0.634
0.421
0.391
0.379
0.219
37.001
25.873
24.502
12.624
Fe2+
Fe2+
Fe2+
Fe3+
1.7387.3912.620.140.101
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Lenaz, D.; Maibam, B.; Adetunji, J.; Skogby, H. The Effects of High-Grade Metamorphism on Cr-Spinel from the Archean Sittampundi Complex, South India. Minerals 2021, 11, 1370. https://doi.org/10.3390/min11121370

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Lenaz D, Maibam B, Adetunji J, Skogby H. The Effects of High-Grade Metamorphism on Cr-Spinel from the Archean Sittampundi Complex, South India. Minerals. 2021; 11(12):1370. https://doi.org/10.3390/min11121370

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Lenaz, Davide, Bidyananda Maibam, Jacob Adetunji, and Henrik Skogby. 2021. "The Effects of High-Grade Metamorphism on Cr-Spinel from the Archean Sittampundi Complex, South India" Minerals 11, no. 12: 1370. https://doi.org/10.3390/min11121370

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