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Minerals 2019, 9(1), 36; doi:10.3390/min9010036
Origin of Blue Sapphire in Newly Discovered Spinel–Chlorite–Muscovite Rocks within Meta-Ultramafites of Ilmen Mountains, South Urals of Russia: Evidence from Mineralogy, Geochemistry, Rb-Sr and Sm-Nd Isotopic Data
Vernadsky Institute of Geochemistry and Analytical Chemistry Russian Academy of Sciences (GEOKHI RAS), 119991 Moscow, Russia
Institute for Geosciences, Johannes Gutenberg University Mainz, 55122 Mainz, Germany
Ilmen State Reserve, Chelyabinsk Region, 456317 Miass, Russia
Bahrain Institute for Pearls & Gemstones (DANAT), WTC East Tower, P.O. Box 17236 Manama, Bahrain
Institute of Geology and Petroleum Technologies, Kazan Federal University, Department of mineralogy and lithology, 420008 Kazan, Russia
Institute of Mineralogy, Ural Branch Russian Academy of Sciences, Chelyabinsk Region, 456317 Miass, Russia
Author to whom correspondence should be addressed.
Received: 19 November 2018 / Accepted: 4 January 2019 / Published: 11 January 2019
Blue sapphire of gem quality was recently discovered in spinel–chlorite–muscovite rock within meta-ultramafites near the Ilmenogorsky alkaline complex in the Ilmen Mountains of the South Urals. More than 20 minerals were found in the assemblage with the blue sapphire. These sapphire-bearing rocks are enriched in LREE and depleted in HREE (with the negative Eu anomalies) with REE distribution similar to those in miascites (nepheline syenite) of the Ilmenogorsky alkaline complex. 87Sr/86Sr ratios in the sapphire-bearing rocks varied from 0.7088 ± 0.000004 (2σ) to 0.7106 ± 0.000006 (2σ): epsilon notation εNd is −7.8. The Rb-Sr isochrone age of 289 ± 9 Ma was yielded for the sapphire-bearing rocks and associated muscovite. The blue sapphires are translucent to transparent and they have substantial colorless zones. They occur in a matrix of clinochlore-muscovite as concentric aggregates within spinel-gahnite coronas. Laser Ablation-Inductively Coupled Plasma-Mass Spectrometry (LA-ICP-MS) analyses showed values with trace elements typical for “metamorphic” blue sapphires, with Ga/Mg < 2.7, Fe/Mg < 74, Cr/Ga > 1.5 (when Cr is detectable), and Fe/Ti < 9. Sapphires overlap “metasomatic” at “sapphires in alkali basalts” field on the FeO–Cr2O3–MgO–V2O3 versus FeO + TiO2 + Ga2O3 discriminant diagram. The sapphires formed together with the spinel-chlorite-muscovite rock during metasomatism at a contact of orthopyroxenites. Metasomatic fluids were enriched with Al, HSFE, and LILE and genetically linked to the miascite intrusions of Ilmenogorsky complex. The temperature required for the formation of sapphire–spinel–chlorite–muscovite rock was 700–750 °C and a pressure of 1.8–3.5 kbar.
Keywords:corundum; blue sapphire; meta-ultramafic rocks; LA-ICP-MS; Rb-Sr and Sm-Nd isotopy; Ilmenogorsky complex; Ural Mountains; metasomatism
Sapphire is referred to the blue color variety of corundum (Al2O3) with Fe and Ti as main chromophores. Other colored sapphires are called fancy and need the color prefix (e.g., pink sapphire, colorless sapphire), apart from the red variety, which is called ruby.
Corundum, of various colors and qualities, occurs in numerous localities in the Ilmen Mountains (Figure 1a). However, gem quality sapphires are found in solely to three of them, all in situ within the primary bearing rocks (See Figure 1b, mines 298, 349, and 418) [1,2,3,4,5,6,7]. Occurrences are located inside of the state’s Ilmen Nature Reserve, though their commercial exploitation is forbidden; samples can be collected just for research purposes in close collaboration with Nature Reserve’s researchers. The most studied gem quality sapphire, of the three, is associated with alkaline syenite pegmatites (Figure 1b, mines 298 and 349), first reported by Barbot de Marni (1828) . These sapphires are genetically linked with the intrusions of miascites (a leucocratic variety of nepheline syenite discovered close to Miass in the Ilmen Mountains and named after the place of discovery).
Gem-quality sapphire mineralization also occurs within the Kyshtymsky stratum of the Ilmenogorsky complex . This stratum is included in the Saitovsky series , one of the structural units of the Vishnevogorsky–Ilmenogorsky polymetamorphic zone. This zone is a fragment of regional post-collision shear, in which the Ilmenogorsky complex is the southern unit (see more on Regional geology of Ilmenogorsky complex in ) (Figure 1a,b). The series is composed of meta-terrigenous quartzite-schist strata, which include garnet-feldspar-biotite, quartz-mica, and garnet-feldspar-amphibole schists; quartzites and quartzite-gneisses; and, units with mafic–ultramafic affinities. Lenses and lenticular bodies within this association are made up of olivine-enstatite, enstatite, talc-anthophyllite, talc-carbonate, tremolite-anthophyllite rocks, and various amphibolites . SHRIMP U-Pb zircon dating from these rocks reflects the complex evolution of the series: ~1.3 Ga (relict cores of terrigenous zircon); from about 460 to ~420 Ma (stage of metamorphic evolution), ~320 Ma, and ~280 Ma (stages of collisional deformation), for more information see . The dimensions of the mafic–ultramafic units, which host the sapphires, the thickness of the schists and quartzites, and their structural relationships vary widely (Figure 1c).
Gem quality sapphires were found as aggregates within chlorite-phlogopite; hosted by meta-ultramafic rocks. They were discovered at a depth of approximately 300 m in a drill core situated at the southern part of the Ilmen State Reserve . In 2003, one of the authors (Sergey N. Nikandrov) found gem-quality sapphire in the similar micaceous (commonly muscovite) association, located between the lakes Bolshoy Tatkul and Bolshoe Miassovo (mine 418, see Figure 1b). Pink sapphires and rubies were previously found in mafic–ultramafic rocks, but this is the first occurrence of sapphires within such a spinel–chlorite–muscovite metasomatic rock.
Sapphires of gem quality are rare and they are principally found in secondary placer deposits; these are found seldom in situ and only in a few types of primary host rocks . Research on gem quality sapphires found in situ in primary rocks, e.g., as those recently discovered in spinel–chlorite–muscovite rock within meta-ultramafites near the Ilmenogorsky alkaline complex in the Ilmen Mountains of the South Urals, may provide clues to the unknown petrogenesis of those from secondary placer occurrences. The present article is the first complete characterization of these sapphires, focusing on their genesis. For this, local geology and petrography were studied as well as the mineralogy, chemistry, and isotopy of corundum–spinel–chlorite–mica rocks. The results are also compared to those that were acquired on other gem-quality sapphires found in the Ilmen Mountains (syenite pegmatites) and checked their possible linkage as well as with those from other deposits for better understanding the gem corundum genesis.
2. Materials and Methods
Five transparent to translucent colorless to blue corundum of gem quality and their solid inclusions from mine 418 were analyzed by the electron microprobe analyses (EMPA) at GEOKHI RAS using Cameca SX100 (CAMECA, Gennevilliers, France) and wavelength-dispersive (WDS) detection mode with 15 kV acceleration voltage, 30 nA beam current, and 3 µm beam size. Four studied sapphire samples present pronounced colorless and blue zones and one sample was completely colorless (Figure 2b,c and Table S1). A set of natural and synthetic reference materials was used for calibration and instrument-stability monitoring. An overlap correction was applied for V > Ti, Cr > V, Sc > Ta, and Nd > Ce. The detection limits for the measured elements varied for different analytical sessions and were less than 0.01 wt. %. Raman spectra were acquired to identify the inclusions inside the sapphires at the Gemological Institute of America laboratory (Carlsbad, CA, USA) using a Renishaw inVia Raman spectrometer combined with optical microscope. The system was coupled with Ar+ laser emitting at 514 nm with a power of 10 mW on the sample. All of the measurements were from 200 to 2000 cm−1, with a 60 s acquisition time, three cycles, at a resolution of about 1.5 cm−1, and under 50× magnification at a room temperature. Rayleigh scattering was blocked using a holographic notch filter. Backscattered light was dispersed using a grating with 1800 grooves/mm. The spectrometer was calibrated at 520.7 cm−1 using Si as a reference.
Laser Ablation-Inductively Coupled Plasma-Mass Spectrometry (LA-ICP-MS) was performed on all five corundum samples that were previously analyzed by wavelength-dispersive electron microprobe analyses (WDS EMPA). Twenty-seven spots were measured on both blue and colorless zones (three spots on blue-colored zones of each four sapphire samples, one sapphire sample is completely colorless). Analysis took place in GEOKHI RAS using a New Wave Research UP-213 Nd:YAG laser (New Wave Research, Inc., Fremont, CA, USA) combined with Element-XR (Thermo Finnigan, Waltham, MA, USA) ICP-MS. Trace-element compositions were determined by monitoring 6Li, 9Be, 24Mg, 27Al, 44Ca, 47Ti, 51V, 53Cr, 55Mn, 57Fe, 59Co, 60Ni, 66Zn, 71Ga, 88Sr, 89Y, 91Zr, 93Nb, 181Ta, 208Pb, and ablating a material with a spot size of 55 µm at a repetition rate of 4 Hz and an energy density of about 21.17 J/cm2. Warm up/background time was 90 s, dwell time was 100 s, and wash out time was 120 s. NIST SRM 610 and NIST SRM 612 glasses (National Institute of Standards and Technology; U.S. Department of Commerce: Gaithersburg, MD) were used as the reference materials and ATHO as an unknown for quality control (QCM). The time-resolved signal was processed in Glitter commercial software using 27Al as the internal standard applying the theoretical value of 52.93 wt. % of Al in pure crystalline α-Al2O3 for analyzing the corundum unknowns. The measured concentrations of reference material and QCM agree for all elements within 10% and 15%, respectively, of preferable values by . This larger discrepancy between the measured and preferable values can be attributed to isobaric interferences that cannot be resolved with the instrumentation used .
Absorption spectra on randomly oriented blue colored zones of sample No1 and No2 were recorded at Kazan Federal University at room temperature by using SHIMADZU UV-3600 spectrometer (Shimadzu Corp, Kyoto, Japan). Spectra were acquired from 185 to 3300 nm, with a data interval and spectral bandwidth of 1 nm and a scan rate of 300 nm/min.
2.2. Host Rocks
Ten samples extracted from different rock types at mine 418, identified macroscopically, of about 100–150 g, were selected for host rock analyses (see Figure 3a and Table S2). Whole-rock major element analyses of these samples were performed at GEOKHI RAS using Energy Dispersive X-ray Fluorescence spectrometer (EDXRF) AXIOS Advanced (PANalytical B.V., Almelo, The Netherlands). The equipment provides the determination the quantitative concentrations of elements from oxygen to uranium from about 10−4 to 100 wt. %. The whole-rock trace element measurements were done in the Institute of Mineralogy Ural Brach Russian Academy of Sciences by using Inductively Coupled Plasma-Mass Spectrometer (ICP-MS) Agilent 7700×. Agilent and GSO provided reference multi-element solutions for ICP-MS on all measured trace elements; BCR-2 basalt glass was used as the internal standard. The values of the relative standard deviations during the measurement did not exceed the values established for this analytical equipment.
For Rb-Sr and Sm-Nd isotope studies, powder from two samples containing gem quality sapphire (K418-12 and K418-13, Table S2) was produced. The samples 12-1, 12-2, 13-1, and 13-2 were taken from the 100–150 g of samples 418-12 and 418-13 used previously for EDXRF and ICP-MS. Another 2 samples (rock1 and rock2) from a bigger portion of about 1 kg of sample 418-13 with sapphire, spinel, feldspar, and muscovite in minerals association, as well, as two muscovites (mica1 and mica2) extracted from appropriate samples rock1 and rock2 were chosen to constrain the Rb-Sr age. Sample dissolution was carried out in a mixture of hydrofluoric and nitric acids (5:1) on a shaker under incandescent lamps during three days. After evaporation, 1 mL of concentrated HCl acid was added three times to a dry residue. Rb, Sr, and REE were collected using fluoroplastic chromatographic columns with DowexW 50 × 8 synthetic ion-exchange resin. The collection was done by stepwise elution with 2.2 acid normality (n) of HCl (for Rb and Sr) and 4.0n HCl (for the Sm + Nd). From the REE mixture, Sm and Nd were collected by stepwise elution with 0.15n HCl, 0.3n HCl, and 0.7n HCl using polyethylene columns with synthetic ion-exchange resin Ln-spec. The isotopic studies took place on a Finnigan™ Triton multi-collector thermal ionization mass-spectrometer (TIMS) by ThermoFisher Scientific (Waltham, MA, USA) at GEOKHI RAS while using a two-tape (Re-Re) ion source for Rb, Sm, and Nd and a single-tape (Re) ion source for Sr. Measurements were performed in static mode with simultaneous recordings of ion currents for different isotopes. For the elimination of mass-dependent interference, normalization was carried out according to the exponential law for 86Sr/88Sr = 0.1194 and 148Nd/144Nd = 0.241572. The analyses of the international standards Sr-SRM-987 and Nd-LaJolla monitored the reproducibility and correctness of isotope measurements for Sr and Nd. The average value of 87Sr/86Sr = 0.710236 ± 0.000009 (2σ) and 143Nd/144Nd = 0.512095 ± 0.000006 (2σ). Concentrations of Rb, Sr, Sm, and Nd were determined by isotopic dilution using 85Rb-84Sr and 149Sm-150Nd tracers. The data-reduction was performed using in-lab software. Isoplot4.13 for Excel  was used for isochrone diagram with MSWD = 4.1.
Eight petrographic thin-sections of visually monolithic host rocks (samples 418-3, 418-4, 418-6, 418-7, 418-9. 418-10, 418-11, and 418-14), 24 randomly chosen corundum-spinel-chlorite-mica (sample 418-12) and one corundum-spinel (sample 418-13) wafers were studied for petrography (see Table S2). Ten of these wafers with different corundum morphology were used to perform the chemical composition of minerals found in association with corundum by EMPA at the Institute of Mineralogy Ural Branch Russian Academy of Sciences (Miass, Russia) using the electron microscope REMMA—202 M coupled to energy-dispersive spectrometer LZ-5. The operating conditions are 20–30 kV acceleration voltage and 4–6 nA beam current. The beam sizes varied from 1 to 2 µm. A set of natural and synthetic reference materials was used for calibration and instrument-stability monitoring.
3.1. Geology and Petrology of Sapphire-Bearing Rocks and Meta-Ultramafic Host Rocks
Sapphire occurrence is a plate-shaped symmetrical-zonal body with traces of considerable deformation, with a dip azimuth of 330°; dip angle is 40°; and, its thickness varies from 1.0 to 1.3 m (Figure 3a). The mine 418 with sapphire-spinel-chlorite-muscovite rock was opened from the surface by a trench measuring about 4 × 9 m (Figure 3b). The block of meta-ultramafites hosting corundum-spinel-chlorite-muscovite rock occupied the first tens of meters and up to about 35 m along the drainage ditch (Figure 3a). The meta-ultramafic host rocks consist of purely mono-mineral coarse-grained enstatite up to 4–5 cm in length with minor olivine and clinopyroxene; in some areas, they are replaced by talc and chrysotile-asbestos. Besides, there is a completely replaced pyrite by goethite in the rock. In the surface subsoil layer, there are chalcedony-quartz concretions up to 10 cm in length, while limonite and supergenic carbonate developed along the cracks of host rocks.
The following zones are distinguished by the structure of host and corundum-bearing rocks (from the selvage to the center, Figure 3b): 1. Meta-ultramafic host rock, which is macroscopically composed of orthopyroxene and clinopyroxene, and minor olivine, have clearly visible brittle deformations (sample 418-7, Table S2); 2. The ferruginated and carbonated meta-ultramafic host rock of the near-selvage zone has a common brownish-orange color; its minerals are almost completely replaced by quartz and carbonate; however, relics of olivine were still detectable (sample 418-6); 3. Talc zoning in the meta-ultramafic host rock (sample 418-4) alternates towards the center on a dense green-colored rock (sample 418-3). The transition to green-colored rock is smooth from almost mono-mineral talc to mono-mineral amphibole. In the amphibole zone, in addition to the monoclinic amphibole (actinolite-tremolite), rhombic anthophyllite was also detected; 4. The central zone is strongly affected by both weathering and deformation processes and it consists of lenticular lenses of various compositions (mica -sample 418-11-, actinolite, actinolite-mica, micaceous pockets with corundum, spinel pockets). In this zone, actinolite-tremolite rock is replaced by shallow rot; only small fragments remain in individual lenses (samples 418-9 and 418-10). The corundum, spinel, and other minerals that accompany them (Figure 2a–c) came from this zone during mineralogical studies described below (samples 418-12, 13, and 14).
3.2. Mineralogy of Sapphire-Hosted Micaceous Lenses
Two sapphire associations were identified, accompanied by spinel. In one, sapphire forms transparent to translucent crystals within the spinel corona. In the other, one lens is an assembly of small (sized about 1 cm) transparent to translucent corundum crystals with almost black spinel, not forming a corona around corundum crystals.
More than 20 major, minor, and accessory minerals are associated with sapphires. Some minerals are common (spinel, clinochlore etc.) and others represent rare or single findings (Ni-bearing sulfide mineralization and baddeleyite) (Table S3. Their texture relationships in regard of sapphire are shown in Table S4. Most minerals were identified under the optic microscope and by Raman Spectroscopy; chemical compositions of minerals were analyzed by EMPA and are presented in Tables S5–S12.
3.2.1. Major Minerals
Minerals of spinel- MgAl2O4 -gahnite ZnAl2O4 series were common detected in 3 mm thick dark green to black-colored corona around sapphire crystals, as well as in inclusions (Figure 4a). The dark-green to black color is likely due to Fe; Co traces (up to 0.28 wt. %) may also contribute to the coloration. Induction surfaces (i.e., surfaces of synchronous growth) that were detected between spinel and sapphire suggest their synchronous growth. However, spinel most likely started crystallizing at a slightly later stage and when sapphire was already growing in the system. Gahnite appears in spinel areas with higher ZnO contents (up to 22 wt. %). In zonal grains, ZnO values varied from 2.46 to 7.47 wt. % (Table S5). Muscovite KAl2(AlSi3O10)(OH)2 formed micaceous lenses with embedded corundum, as well as micro-inclusions (up to 0.2 mm) within chlorite group minerals (Figure 4b). Muscovite is characterized by a higher MgO content from 0.5 to 2.5 wt. % in comparison to stoichiometric muscovite (Table S6). Clinochlore Mg5Al(AlSi3O10)(OH)8 and amesite Mg2Al(AlSiO5)(OH)4 form inclusions and rather large ingrowths (up to 5 mm) around spinel, inclusions within spinel, and in fractures along the border of corundum and spinel (Figure 4b). These minerals were also found in the rims around the uraninite-brockite and monazite-(Ce) (for the chemical composition, Table S6). Anorthite CaAl2Si2O8 (An100) is found in the “spinel lenses” forming crystals that are sized up to 3 mm in the intergrowth with amphibole and chlorite group minerals (see chemical composition in Table S7). All identified major minerals are syngenetic with sapphire.
3.2.2. Minor Minerals
Apatite group minerals Ca5(PO4)3(OH,F,Cl) were found within corundum fractures and chlorite group minerals as prismatic epigenetic inclusions up to 1 mm in length (Figure 4c). Its composition varies from chlorapatite to fluorapatite to hydroxylapatite (Table S8). Zircon ZrSiO4 forms small zonal epigenetic inclusions (up to 0.1 mm in length) within the fractures of corundum, chlorite group minerals, and spinel. Besides zircon, the amphibole group minerals and apatite (Figure 4c) also fill out these fractures. Zircons contain up to 3.16–4.73 wt. % of HfO2 (Table S9). Protogenetic diaspore AlO(OH), along with clinochlore forms rims around inclusions of uraninite, intergrowth with clinochlore within corundum (Figure 4d), and platy aggregates in the fractures of barium feldspar. Diaspore contain up to 0.1 wt. % of SiO2 and 0.34 wt. % of FeOtot. Millerite NiS forms micro-inclusions (up to 15 µm) within corundum, spinel, and chlorite group minerals; the mineral is found in association with maucherite, heazlewoodite, and galena (Figure 5a). The FeOtot content of millerite varies from 2 to 20 wt. % (Table S10). Maucherite Ni11As8 was detected in the intergrowth with heazlewoodite and millerite in crystals sized to 15 µm (for chemical composition, Table S10). Microlite group minerals (Na,Ca)2Ta2O6(O,OH,F) were found in small (up to 0.1 mm) grains and cube-octahedral crystals within chlorite group minerals (Figure 5b). Minerals characterized by the high UO2 content (up to 11.34 wt. %); values of WO3 and Nb2O5 both vary up to 3.15 wt. % and 3.57 wt. %; ThO2 is 1.2 wt. % and Y2O3 1.61 wt. %. Nickeline NiAs is found as inclusions within clinochlore and dravite; the size of mineral varied up to 20 µm (Figure 5c and Table S9). Uraninite UO2 forms zonal micro-inclusions that are sized up to 150 µm (Figure 5d). The atomic number (pfu) is up to 0.41 in the mineral. Allanite-(Ce) (CaCe)(Al2Fe2+)(Si2O7)(SiO4)O(OH)—dissakisite-(Ce) (CaCe)(Al2Mg)(Si2O7)(SiO4)O(OH) form zonal-sectorial and mosaic-like crystals up to 0.2 mm in length (Figure 5f); the oscillatory zonation is due to the different concentrations of CaO and REE (Table S11). Monazite-(Ce) Ce(PO4) has been found along the cracks of dissakisite-(Ce) grains, forming crystals of up to 20 μm in length (Figure 5f). CaO content ranges from 0.38 to 8.25 wt. % in the mineral, Ce2O3 values vary from 23.11 to 37.53 wt. %, and La2O3 is 10–22 wt. %; in some analyses, additional SiO2 and ThO2 were detected (Table S9). Ni-bearing and REE-mineralization are likely syngenetic in origin.
3.2.3. Accessory Minerals
Vigezzite or fersmite (Ca,Ce)(Nb,Ta,Ti)2O6 forms likely syngenetic elongate-prismatic inclusions up to 70 µm long within clinochlore (Figure 5e). The content of Nd2O3 is about 3.5 wt. % in the mineral; La2O3 values vary up to 2.16 wt. %, Pr2O3 is up to 1.15 wt. %; and, FeOtot up to 1 wt. %.
Heazlewoodite Ni3S2 is associated with corundum, spinel, clinochlore, and millerite. The size of the mineral is less than 0.3 mm. It contains up to 1.22 wt. % of FeOtot . Galena PbS is found in intergrowth with millerite in the form of crystals sized up to 10 µm (Figure 5a and Table S10). Gersdorffite NiAsS is identified within the inner part of a zonal aggregate composed of heazlewoodite and galena in contact between chlorite group minerals and corundum. CoO content in the mineral varies up to 13 wt. % (Table S10). The Ni- and Pb-bearing mineralization is likely syngenetic in origin. Dravite Na(Mg3)Al6(Si6O18)(BO3)3(OH)3(OH) forms brownish-colored syngenetic or protogenetic crystals up to 3 cm in length. It lies in micaceous lenses in association with corundum and in “spinel lenses”. The mineral contains lower FeO and CaO values in comparison with stoichiometric dravite; two values are up to 1.6 wt. % and 0.5 wt. %. Rutile TiO2 forms syngenetic micro-inclusions within spinel sized up to 50 µm. The mineral is characterized by high tantalum content (up to 31.79 wt. % of Ta2O5) and Nb2O5 values of up to 1.46 wt. %. Hyalophane (K,Ba)Al(Si,Al)3O8 forms likely epigenetic micro-inclusions along the fractures within the chlorite group minerals; mineral size is up to 60 µm. BaO content in hyalophane is about 6 wt. % (Table S7). Celsian Ba(Al2Si2O8) forms lamellar epigenetic crystals and aggregates in fractures along a boundary between corundum and amesite; mineral size varies from 5 µm to 30 µm. BaO values in mineral are up to 33.67 wt. % (Table S7). Marialite (Na,Ca)4[Al3Si9O24]Cl forms syngenetic inclusions within chlorite group minerals sized up to 20 µm; Cl content in the mineral is about 1.7 wt.%, CaO is 11 wt. %, Na2O is about 7 wt. % (Table S7). Pargasite NaCa2(Mg4Al)Si6Al2O22(OH)2 and tschermakite ☐(Ca2)(Mg3Al2)(Al2Si6O22)(OH)2 form syngeneitc micro-inclusions (up to 150 µm) within clinochlore of “spinel lenses” (Table S12). Baddeleyite ZrO2 is found as an epigenetic micro-inclusion within zircon sized up to 5 µm.
3.3. Sapphire Mineralogy, Geochemistry, and UV-Vis-NIR Spectroscopy
Sapphires practically always form single crystals, with colorless translucent to blue transparent zones, sized up to 4 cm in length. Only small, less than 1ct, sapphires of gem quality can be faceted. A dark-green to black colored spinel-gahnite corona practically always surrounds sapphire crystals (Figure 2a–c). The shape of sapphire-spinel aggregates is often irregular and rounded due to numerous outgrowths of muscovite and clinoclore. Less common (in one or two lenses), there are short-prismatic and barrel-shaped sapphire crystals; however, without flat faces that are caused by intergrowth with the muscovite and spinel.
LA-ICP-MS measurements from different zones of sapphires are presented in Table 1. The position of analyzed spots is shown in Figure 3b,c. Mg, Ti, V, Cr, Fe, and Ga, elements commonly used to trace the geological origin were the only detected element of this method [14,15]. Si may also be present as a trace of sapphires; however, it cannot be measured by LA-ICP-MS due to high interference of 27AlH+ with 28Si+ and 28SiH with 29N-N . In the blue-colored spots, Mg ranges from 11 to 23 parts per million weight (ppmw), Ti ranges from 92 to 279 ppmw, V from b.d.l. to 1 ppmw and Cr values ranges from b.d.l. to 87 ppmw (except one analyses detected 520 ppmw likely due to the ablation of diaspore inclusion; its spot was excluded from the plots provided below), relatively low Fe content (from 732 to 1021 ppmw), and fairly low Ga values (from 9 to 31 ppmw). The absorption spectra were comparable with those that were observed on sapphires of metamorphic or metasomatic origin and similar to those from Ilmen Mountains linked with syenite pegmatites [6,17]. Values of trace elements, such as Mg, Ti, Fe, Cr, Ga, and their ratios—Ga/Mg, Fe/Ti, Fe/Mg, and Cr/Ga have been used for the determination of the origin of “magmatic” versus “metamorphic” blue sapphires [14,15]. LA-ICP-MS trace element measurements of the studied sapphires showed Ga/Mg < 2.7, Fe/Mg < 74, Cr/Ga > 1.5, and Fe/Ti < 9, which is typical of sapphires of metamorphic origin [14,15]. On a Fe versus Ga/Mg diagram and a Fe-Ti × 10-Mg × 100 ternary plot , all measured corundum samples plotted in the overlapping field of “metamorphic” and “plumasitic” sapphires (Figure 6 and Figure 7). Using the FeO–Cr2O3–MgO–V2O3 versus FeO + TiO2 + Ga2O3 discriminant diagram of , the studied sapphires plot slightly off the bottom of the overlapping area with rubies found in “mafic–ultramafic rocks” and more in the field of “metasomatic” sapphires and sapphires in “alkali basalts” (Figure 8a,b). In the discriminant factor diagram by , the Ilmen sapphires within meta-ultramafites are plotted to the “plumasitic” field and they are close to those from skarns, which is mostly caused by their enrichment with Ti (Figure 9).
3.4. Whole-Rock Geochemistry
EDXRF measurements of hosted meta-ultramafic and corundum-bearing rocks are presented in Table S13. According to the powder EDXRF values, meta-ultramafic host rocks have high SiO2 content up to 50–61 wt. %, MgO was about 20–32 wt. %, CaO was 0.29–17.24 wt. %, Fe2O3 was 2.9–8.2 wt. %, Al2O3 was 0.11–3.97 wt. %, and low alkaline elements concentrations were also detected (in total, about 0.1–0.2 wt. %). Micaceous lenses with corundum and spinel, however, showed high MgO and Al2O3 contents (the two are about 16–25 wt. % and 16.26–38.52 wt. %, respectively), combined with variable SiO2 (25–80 wt. %), 3.44–9.5 wt. % of Fe2O3, 0.26–1.39 wt. % of CaO, and low concentration of alkaline elements (Na2O + K2O ≤ 1 wt. %) . Thus, sapphire-bearing rocks show higher Al2O3 and K2O, however, lower SiO2 values than those detected in meta-ultramafites, but similar concentrations of Na2O, MgO, CaO, and TiO2 (Figure 10). As for numerous metasomatic deposits, there are difficulties in the calculation of mass balance for the newly discovered sapphire-spinel-chlorite-muscovite rock, its formation occurred with significant mass-transfer. The aluminum that is required for the formation of corundum is commonly passive in weakly acidic and neutral conditions; the transfer of aluminum is possible in alkaline and strongly acidic conditions . The mobility of aluminum in a complex with sodium was previously discussed . In the case of this sapphire occurrence, Al was particularly mobile and it was most likely transported by fluids that are linked to miascites (Table S13 and the later discussion). Additionally, sapphire-bearing rocks were enriched with LIL-elements, such as Ba (Ba-felspars), P (apatite), and Sr (as a trace-element in feldspar and muscovite), which came from miascite-generated fluids as well. However, the sources of Mg and some siderophyle elements (Ni) are linked likely to meta-ultramafic host rocks; their parts were re-worked by metasomatic fluids.
ICP-MS measurements are shown in Table S13. The distribution of REE in micaceous lenses has the general trend—an enrichment with LREE as compared to HREE (Figure 11a). This phenomenon is possibly due to the inclusions of LREE-bearing minerals, e.g., monazite-(Ce), allanite-(Ce) or others. In the meta-ultramafic host rocks, this trend is less pronounced or it disappears: REE contents normalized to chondrite are almost the same for both LREE and HREE. Nearly all of the studied rocks show negative Eu anomalies. The REE trend of these corundum-bearing rocks is close to that observed for Ilmen corundum-bearing syenite pegmatites (Sorokina et al., unpublished data) and to that of corundum syenite pegmatites hosted by ultramafic rocks in the French Pyrénées . Enrichment in HSFE was also noted (mine 418); commonly observed for alkaline-ultramafic associations of the platform type (ultramafic rocks, syenites–carbonatites etc.; ), and similar to those of miaskite (nepheline syenite) of the Ilmenogorsky complex. On a trace element diagram normalized to primitive mantle (Figure 11b), all studied rocks present distinct K and Ti negative anomalies. However, the sapphire-bearing rocks also show positive Ta and Gd anomalies, but with different Sr anomalies.
3.5. Rb-Sr and Sm-Nd Isotope Measurements
Rb-Sr and Sm-Nd isotope measurements of sapphire-bearing rocks 418-12 and 418-13 previously analyzed by EDXRF and ICP-MS are presented in Table S14. As well, two samples of 418-13 rock containing feldspar and two samples of mica extracted from appropriated rock sample 418-13 associated with sapphire mineralization were analyzed in order to constrain the Rb-Sr age. Obtained values of Rb, Sr, Sm, and Nd by TIMS are closely similar or comparable to those that were received by ICP-MS (Tables S12 and S13). 87Sr/86Sr for samples 418-12 and 418-13 are varied from 0.708764 ± 0.000010 (2σ) to 0.710587 ± 0.000006 (2σ). For mica samples, these values are higher and vary from 0.711371 ± 0.000008 to 0.714131 ± 0.000016. The calculated Rb-Sr isochrone age for three rock samples and mica-2 sample is 289.3 ± 8.7 Ma (2σ), MSWD is 4.1 (Figure 12). Note, the calculated Rb-Sr age for another mica sample (mica-1) with three rock samples gave much higher error (352 ± 35 Ma) and higher MSWD (72), which was likely due to the secondary alteration of muscovite samples mica-1. (87Sr/86Sr)289 of all samples recalculated on 289 Ma are about 0.707351 to 0.707919. 143Nd/144Nd for the samples 418-12 and 418-13 are 0.5122 ± 0.000008 (2σ) and 0.5122 ± 0.000012 (2σ), εNd(289 Ma) is −7.8. The obtained high 87Sr/86Sr ratios and low εNd correspond to the formation of the newly discovered corundum-bearing rocks under the significant influence of crustal fluids.
4.1. Suggested Petrogenesis of Sapphire in the Meta-Ultramafic Host Rocks of the Ilmen Mountains
The studied blue sapphires surrounded by spinel coronas embedded in chlorite-muscovite matrix present metasomatites that are found within meta-ultramafic host rocks. These host rocks are most likely formed after metasomatic alteration (serpentinization) of orthopyroxenites; i.e., containing orthopyroxene with minor olivine and clinopyroxene. While the orthopyroxenites were formed at about 1.3 Ga and are related to the Saitovsky series of Kyshtimsky strata of the Ilmenogorsky complex, Rb-Sr and Sm-Nd isotopic data indicate their linkage with enriched mantle domains of types EM1 and EM2 .
The metasomatism required for the formation of these rocks with blue sapphires took place around 289.3 ± 8.7 Ma (measured by Rb-Sr dating of sapphire-bearing rocks and mono-mineral muscovite associated with sapphires). This age represents the cooling age after the metamorphic peak (transpression) that occurred in the Ilmenogorsky complex at about 330–320 Ma during the Uralian orogeny . The metasomatic fluids formed after the partial melting of miascites occurred in the region (440–420 Ma). These fluids were also the source of HFSE, LILE, and alumina (remobilized under alkaline conditions [21,22]) needed for corundum formation, and transported these chemical elements at a minimum distance of about 4 km (calculated from the eastern flank of Ilmenogorsky complex) reaching the meta-ultramafic rocks. In Figure 11, similar REE trends between miascites and corundum-bearing rocks in mine 418 are presented (i.e., enrichment of LREE as compared to HREE), which is an important evidence of the metasomatic fluid source. Partial melting of miascites is associated with the formation of migmatities with more acidic composition from albitites to even granites. In the Ilmenogorsky miascite massif, alumina remobilization can also be associated with the formation of zeolitic veins and zeolitizated zones of pegmatites, filling late-forming zones with aluminum hydroxides (gibbsite, nordstrandite, boehmite, diaspore).
Desilication also took place during the contact of fluids with ultramafic rocks and sapphire formation. Desilication is commonly observed during corundum crystallization in numerous deposits worldwide ([1,29,30], etc.). The importance of buffering capacity of ultramafic host rocks with respect to silica in the Greenland ruby deposit has been previously shown . In this deposit, the meta-ultramafic host rocks show similar buffering capacity in respect to the desilication of Al-bearing alkaline fluids that are linked to miascites. Initial ultramafic rocks are also most likely the source of Mg required for spinel and chlorite formation found in metasomatites linked with the corona around the sapphires, as well as the source of Ni for nickel-bearing minerals.
Sapphire crystallization was likely caused by the breakdown of diaspore possibly by the following reaction: 2diaspore → corundum + H2O. Note, diaspore formed in meta-ultramafic host rock likely due to a previous metasomatic event that is linked with the partial melting of miascites. A previous metasomatic event was likely a significant time before the deposition of sapphire-bearing metasomatites. Chlorite formation occurred during the metasomatic reworking of meta-ultramafic host rocks. Meanwhile, the spinel corona most likely formed as a consequence of metasomatic fluid-chlorite interactions with the corundum as a reaction rim. Under decreasing pressure and temperature, muscovite crystallized during the breakdown of corundum: corundum + orthoclase + H2O → muscovite; previously observed for a corundum-mica-tourmaline rock hosted by ultamafites of New Zealand .
Experiments have shown that blue sapphires (incorporation of Ti and Fe into the corundum lattice) can be formed at around 700 °C after muscovite and biotite, along with a peraluminous silicic melt at 2 kbar (water pressure) . Corundum and hercynite spinel also coexist with orthoclase-rich feldspar and biotite at 750 °C . Besides, other experiments have shown that muscovite can still be stable, slightly above 700 °C and at about 1.8 kbar  (Figure 13a). Thus, it seems that sapphire-spinel-clinochlore-muscovite metasomatites formed at a temperature around 700–750 °C and pressure about 1.8–3.5 kbar; at the eutectic point of corundum + orthoclase + H2O ↔ muscovite; where the three minerals are in equilibrium (Figure 13b).
4.2. Comparison with Sapphire and Ruby from Metasomatites
To date, only pink sapphires to rubies (probably none of them of gem quality) were found in metasomatites within the ultramafic host rocks; e.g., they are known in the eastern Transvaal  and in the Barberton greenstone belt  of South Africa, in Zimbabwe , and in Westland, New Zealand . Ruby-fuchsite rock, ‘verdite’ from Zimbabwe is enriched in Ni as represented by gersdorfitte (NiAsS), which is also the case of the described occurrence in the Ilmen Mountains, in which andalusite, chlorite, margarite, tourmaline, diaspore, rutile, and native Bi are present as well. However, in Zimbabwe, ‘verdite’, which occurs in bodies a few kilometers length, was formed as the result of post-volcanic, pre-metamorphic exhalative alteration of komatiitic lavas . Another approach to the genesis of ‘verdite’ suggests an alteration of ultramafic rocks in a high-temperature low-pH hydrothermal solution carrying LILE . Ruby-bearing boulders of metasomatic origin from Westland in New Zealand, as is the case of the described occurrence, are found embedded in micaceous matrix associated, however, with fuchsite, margarite, and tourmaline . In New Zealand, similarly to the described Ilmen sapphire occurrence, the crystallization of minerals in association with corundum required significant mass-transfer during the metasomatic process, possibly 50–90% . Regionally metamorphosed pink sapphire to ruby deposits within an ultramafic protolith in Paranesti in Greece were also reported . In common with the Ilmen sapphires, the Paranesti rubies are characterized by spinel-picotite inclusions. Spinel inclusions and Ni-bearing sulfides were also found within sapphires from some Australian occurrences . However, the spinel inclusions in these sapphires are more Co-rich than Zn-rich, as is the case in the present Ilmen sapphires (Table S5). An inclusion of Zn-rich spinel within sapphire is also reported from a placer in Kedrovka, in the Russian Far East .
4.3. Comparison of Chemical Data with Sapphires from Other Geological Environments
In a Fe versus Ga/Mg diagram , all measured corundum samples were plotted to “metamorphic” and “plumasitic” population fields (Figure 6), clearly away from the “magmatic” blue sapphires that are found within syenite pegmatites of Ilmen Mountains (see again [6,17]). However, these trace-element diagrams should be used with the caution and possibly revised, since it was found that some of the sapphires from magmatic deposits could be plotted in the “metamorphic field” [46,47]. It is probably important to refine these plots using solely data of gem-quality samples and to group them by color (e.g., plot sapphire and rubies separately), taking into account that most of trace elements used for these are corundum chromophores (e.g., Fe, Ti, Mg, Cr, V). For instance, as shown in Figure S1, the population field is more scattered when plotting colorless opaque sapphires together with those of blue color.
On the FeO–Cr2O3–MgO–V2O3 versus FeO + TiO2+ Ga2O3 discriminant diagram (Figure 8), the plot is slightly away from the area with rubies in “mafic–ultramafic rocks” and is mostly in the field with “metasomatic” sapphires and sapphires in “alkali basalts”. The UV-Vis-NIR spectra of studied sapphires were comparable to those that were observed on sapphires of metamorphic or metasomatic origin.
Most gem-quality sapphires are mined from placers of unclear primary and possibly diverse origins. Studies of gem-quality sapphires that are found in situ within host rocks may provide clues to the petrogenesis of those found in secondary occurrences.
Gem-quality sapphire is known from syenite pegmatites in the Ilmen Mountains of the South Urals. An occurrence of gem-quality sapphires from these mountains was also discovered within meta-ultramafites where sapphires form concentric aggregates within spinel-gahnite coronas. Sapphires form irregular-shaped translucent to transparent crystals with colorless and blue zones. The concentric sapphire aggregates with spinel coronas are embedded in a clinochlore-muscovite matrix. In this occurrence, corundum(sapphire)–spinel(gahnite)–clinochlore-muscovite aggregates associate with anorthite (An100), apatite, zircon, diaspore, microlite, allanite-dissakisite-(Ce), monazite-(Ce), dravite, Ba-feldspars, and various Ni-bearing minerals. The mantle-generated ultramafic host rocks (orthopyroxenites) that are composed of enstatite with minor olivine have undergone significant serpentinization. Altered meta-ultramafic host rocks have high contents of SiO2 (approximately 50–61 wt. %) and MgO (approximately 20–32 wt. %), but low Al2O3 (0.11–3.97 wt. %), as well as alkaline elements concentrations (in total, about 0.1–0.2 wt. %), whereas the sapphire-bearing rocks showed high MgO (16–25 wt. %) and high Al2O3 (16.26–38.52 wt. %) contents combined with variable SiO2 (25–80 wt. %), but low concentrations of alkaline element (Na2O + K2O ≤ 1 wt. %). Most of the sapphire-bearing rocks—in contrast with the meta-ultramafic host rocks—are enriched in LREE and depleted in HREE with negative Eu anomalies. Spider REE diagrams of the studied samples are similar to those of sapphires in the syenite pegmatites, linked to intrusions of miascites (nepheline syenite) in the Ilmen Mountains. Sapphire-spinel-clinochlore-muscovite rock formed after metasomatic alteration of orthopyroxenites at a temperature around 700–750 °C and pressure about 1.8–3.5 kbar. The metasomatic fluids enriched in HFSE, LILE, and alumina formed after the partial melting of miascites (nepheline syenites), while Mg and some siderophile elements (Ni) came from mantle-generated meta-ultramafic host rocks. Formation of this metasomatic rock occurred at about 289 ± 9 Ma (Rb-Sr dating of sapphire-bearing rocks and mono-mineral muscovite associated with sapphires), representing the cooling ages after the peak metamorphism at about 330–320 Ma during the Uralian orogeny.
Sapphire crystallized after the breakdown of diaspore by the reaction: 2diaspore → corundum + H2O. Chlorite occurred during the metasomatic reworking of meta-ultramafic host rocks. However, the spinel corona surrounding sapphire aggregates most likely formed as a consequence of metasomatic fluid-chlorite interactions with the corundum. Under decreasing pressure and temperature, muscovite crystallized during the breakdown of corundum by the reaction: corundum + orthoclase + H2O → muscovite.
Despite on obvious metasomatic genesis, LA-ICP-MS analyses of blue sapphires showed Ga/Mg < 2.7, Fe/Mg < 74, Cr/Ga > 1.5, and Fe/Ti < 9, in the range of “metamorphic” sapphires. The Fe versus Ga/Mg diagram and Fe-Ti × 10-Mg × 100 ternary plot should be used with the caution and possibly revised using solely data of gem-quality samples and to group them by color.
The following are available online at https://www.mdpi.com/2075-163X/9/1/36/s1, Table S1: Description of sapphire-spinel samples used for WDS EMPA and LA-ICP-MS, Table S2: Mineral assemblage and mode of minerals in the thin-sections, Table S3: Minerals identified in association with the sapphire, Table S4: Texture relationship of minerals found in association with sapphire, Table S5: Chemical composition of spinel and gahnite, Table S6: Chemical composition of muscovite and clinochlore, Table S7: Chemical composition of feldspar group minerals and marialite, Table S8: Chemical composition of apatite group minerals, Table S9: Chemical composition of zircon and monazite-(Ce), Table S10: Chemical composition of sulphide minerals, Table S11: Chemical composition of allanite-(Ce) group minerals, Table S12: Chemical composition of amphibole group minerals, Table S13: EDXRF (wt. %) and ICP-MS (ppmw) analyses of host rocks from 418 mine, Table S14: Rb-Sr and Sm-Nd isotope measurements of corundum-bearing rocks. Figure S1: A plot of Ilmen sapphires within meta-ultramafic host rocks (blue-colored samples—bold blue circles, colorless samples—colorless circles) in a Fe versus Ga/Mg diagram showing boundaries for magmatic (MAF: Main Asian Field; magmatic sapphires in alkali basalt) and metamorphic sapphires, modified after [14,18].
E.S.S. formulated the idea of a paper, collected the samples for studying, conducted a research on the Raman spectroscopy, LA-ICP-MS, and TIMS, and their following data-reduction process, designed EDXRF and WDS EMPA experiments, assembled some tables and figures, and wrote the manuscript; M.A.R. collected the samples for host rock studying, performed the petrography of corundum-bearing and host rocks, designed the EDS EMPA and ICP-MS experiments, assembled some tables and figures, provided the field data and mineralogy of host rocks; S.N.N. performed the petrography of host rocks and provided the geological setting data; S.K. helped with data interpretation and editing of the manuscript; N.N.K. performed WSD EMPA of selected samples; A.G.N. carried out UV-Vis-NIR spectroscopy of sapphires and provided its interpretation; M.O.A. assisted with LA-ICP-MS measurements and data-reduction process; A.V.S. assisted with both sample preparation process for TIMS and TIMS measurements; Y.A.K. created some ideas for TIMS measurements and interpretation of final TIMS data; V.A.K. performed the EDS EMPA measurements.
The research has been supported by the Council on grants of the President of the Russian Federation (project no. MK-4459.2018.5); the Raman measurements and field trip to Ilmen State Reserve in 2016 were supported by Gemological Institute of America through the R.T. Liddicoat Postdoctoral Research Fellowship for one author (ESS); UV-Vis-NIR measurements were supported by Russian Government Program of Competitive Growth of Kazan Federal University.
The work in the Ilmen Natural Reserve was conducted under an agreement on scientific collaboration between the GEOKHI RAS and the Ilmen Natural Reserve. The samples used in this study were transferred by the Ilmen State Reserve for scientific purposes. The authors thank the Editor of Minerals and Guest Editors for invitation to submit the manuscript for consideration and possible contribution in a special issue on “Mineralogy and geochemistry of gems”. Pautov L.N. and Agakhanov A.A. (Fersman Mineralogical Museum RAS), Phillipova K.A. (Institute of Mineralogy Ural branch of RAS), and Medvedeva E.V. (Ilmen State Reserve Ural branch RAS) helped with electron-microprobe, ICP-MS measurements, and consultations on the topic of research. Kuz’mina T.G., Romashova T.V., Smirnov V.I., and Turkov V.A. (GEOKHI RAS) assisted in sample preparation process and EDXRF measurements. We are thankful to John Saul (Swala Gem Traders, Tanzania), four anonymous reviewers, and Guest Editor of this special issue Panagiotis Voudouris for improving the text of an earlier version of this article.
Conflicts of Interest
The authors declare no conflict of interest.
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Figure 1. Location and geology of Ilmen sapphire deposits in meta-ultramafic host rocks: (a) General map of Russia showing location of Ilmen Mountains within Urals; (b) Regional geologic map of Ilmenogorsky complex after  with location of corundum mines within syenite pegmatites (mines 298 and 349) and within meta-ultramafic host rocks (mine 418): 1—sedimentary-volcanogenic metamorphosed rocks of the East Urals mega-zone (Upper Devonian-Lower Carboniferous), 2—volcanogenic-sedimentary metamorphosed strata of the Saitovsky series, 3—metamorphic rocks of the Ilmensky series, 4—metamorphic rocks of the Selyankinsky series, 5—meta-ultramafic rocks, 6—syenites and nepheline syenites, 7—fenites, 8—granitoids, 9—zones of blastomylonites, 10—faults, shear zones and other tectonic contacts. White box with 418 mine is shown in details in Figure 1b; (c) Regional geologic map after  with 418 mine of sapphire-spinel-chlorite-muscovite metasomatites within meta-ultramafic host rocks at 55.178434° N, 60.292494° E: 1—Lower-Kyshtymsky stratum, generally gneiss; 2—Upper-Kyshtymsky stratum, mostly quartzite; 3—traced horizons of various rocks (biotite and amphibole gneisses, diopside-scapolitic and kyanite schists, quartzites); 4—clastoliths and bodies of amphibolites; 5—tremolite-anthophyllite meta-ultramafites; 6—enstatite (±olivine) -antophyllite meta-ultramafites; 7—granite aplite; 8—granite pegmatites and granite dikes; 9—wetlands.
Figure 2. Photographs of corundum–spinel–chlorite–muscovite rock: (a) Corundum–spinel concentric aggregates embedded in a muscovite-chlorite matrix; (b) Corundum-blue sapphire–spinel samples No-s 1–3 with spot positions for Laser Ablation-Inductively Coupled Plasma-Mass Spectrometry (LA-ICP-MS) analyses from Table 1 mounted in the epoxy resin; (c) Corundum-blue sapphire-spinel samples No-s 4 and 5 with spots positions for LA-ICP-MS analyses from Table 1 mounted in the epoxy resin. Photographs by Elena S Sorokina.
Figure 3. Local geologic maps of 418 mine showing the locations of samples for this research at 55.178434° N, 60.292494° E: (a) Geological scheme of 418 mine: 1—meta-ultramafites; 2—ferruginated meta-ultramafites; 3—talc meta-ultramafites altering toward the center on a dense actinolite rock; 4—actinolite rock; 5—micaceous lenses with corundum; 6—lenses of actinolite-micaceous rock; 7—anthophyllite-asbestos veins; (b) The outcrop of 418 mine: 1—meta-ultramafic host rock of the main unit; 2—ferruginated and carbonated meta-ultramafites of the near-selvage zone; 3—talc zone in meta-ultramafic host rock; 4—the central zone. The numbers 418–3, 418–4, 418–6, 418–7, 418–9, 418–10, 418–11, 418–12, 418–13, and 418–14 indicate the numbers of samples in Table S1.
Figure 4. Backscattered (BSE) images of corundum-spinel-chlorite samples from the central zone: (a) Corundum-spinel intergrowth with inclusions of clinochlore; (b) The rim of corundum-spinel concentric aggregate with intergrowth of clinochlore and muscovite; (c) Inclusions of apatite and zircon within corundum; and, (d) Inclusions of spinel, clinochlore, and diaspore (Ds) within corundum. Mineral abbreviations are after . BSE images by E.S. Sorokina.
Figure 5. BSE images of corundum-spinel-chlorite samples from the central zone: (a) Millerite and galena inclusions within corundum; (b) Corundum-spinel-clinochlore intergrowth with inclusion of microlite; (c) Nickeline inclusion within clinochlore; (d) Uraninite-brokkite-clinochlore concentric aggregate within spinel; (e) Vigezzite inclusion within clinochlore; and, (f) Dissakisite-(Ce)-monazite-(Ce) aggregate within clinochlore. Mineral abbreviations are after . BSE images by V.A. Kotlyarov.
Figure 6. A plot of Ilmen sapphires within meta-ultramafic host rocks (bold blue circles) in a Fe versus Ga/Mg diagram showing boundaries for magmatic (MAF: Main Asian Field; magmatic sapphires in alkali basalt) and metamorphic sapphires are modified after [14,19]. Ilmen sapphires that plots from syenite pegmatites is from .
Figure 8. (a) A plot of Ilmen sapphires within meta-ultramafic rocks (bold blue circles) in a FeO–Cr2O3–MgO–V2O3 versus FeO–TiO2–Ga2O3 diagram (in wt. %) used for the geological classification of corundum deposits are modified after . The main fields defined for the different types of gem corundum deposit are: John Saul Ruby Mine (Kenya) type (R2) is for ruby; for sapphire, syenitic rocks (S1); metasomatites (S2); xenocrysts in alkali basalt and lamprophyre (S3). The domains of ruby in mafic–ultramafic rocks and S2 are overlapping. Values of Ilmen sapphires within syenite pegmatites are after . (b) Focus on the distribution of Ilmen sapphires within metasomatites (S2) of the plot A).
Figure 12. The Rb-Sr isochrone for three sapphire-bearing rocks and one muscovite samples associated with sapphire of 418 mine in Ilmen Mountains are with yielded age at 289.3 ± 8.7 Ma (2σ), MSWD is 4.1.
Figure 13. (a) The equilibrium curve (solid and dash) for the reaction Sa (sanidine) + Crn + H2O ⇆ Mus, estimates of the equilibrium curve for the melting of sanidine and leucite—Lc (dash) in the muscovite composition, and possible relations between the assemblages Sa + Crn + H2O and Mu + Sa + Lc + H2O are modified after . (b) Phase relations in peraluminous granitic systems in terms of pressure and temperature after . The dashed line is a metastable extension of the reaction Ab (albite) + Ms (muscovite) + Qtz (quartz) + H2O = melt + aluminum silicate to 2 kbar pressure. The H2O-saturated haplogranite solidus (Ab + Or (orthoclase) + Qtz + H2O = melt) and the subsolidus second sillimanite isograd (Ms + Qtz = Or + aluminum silicate + H2O) were determined by  and . The terminal muscovite reaction Ms = Or + Crn + H2O comes from . The diagram was modified after .
Table 1. The trace-elements composition of sapphire colored zones by LA-ICP-MS 1.
|No||Spot||Color||24Mg||47Ti||51V||53Cr||57Fe||71Ga||Ga/Mg||Fe/Mg||Cr/Ga||Fe/Ti||Mg × 100||Ti × 10|
1 Cl, BL—colorless and blue sapphire zones on a Figure 3b,c. 60Ni was measured but was below the detection limit.
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