In this issue
This New Mineral Names has entries for 11 new minerals, including alfredopetrovite, bussyite-(Y), colinowensite, esquireite, ferromerrillite, fluornatropyrochlore, fluor-schorl, hogarthite, shilovite, tapiaite, waimirite-(Y).
Alfredopetrovite[*]
A.R. Kampf, S.J. Mills, B.P. Nash, B. Thorne and G. Favreau (2016) Alfredopetrovite, a new selenite mineral from the El Dragón mine, Bolivia. European Journal of Mineralogy, 28(2), 479-484.
Alfredopetrovite (IMA 2015-026), ideally Al2(Se4+O3)3·6H2O, is a new selenite mineral from the El Dragón mine, Antonio Quijarro Province, Potosí Department, Bolivia. The mine exploited a telethermal deposit consisting of a single selenide vein hosted by sandstones and shales. The main primary mineral is a Co-rich krut’aite-penroseite. Clausthalite, petrovicite, watkinsonite, eldragónite, and grundmannite were crystallized from later solutions. Alfredopetrovite is a secondary mineral and occurs in vugs in a krut’aite-penroseite-dolomite-goethite matrix. Other closely associated secondary minerals are: ahlfeldite, allophane, calcite, chalcomenite, favreauite, felsobányaite, malachite, and molybdomenite. Alfredopetrovite forms colorless to blue (transmit chalcomenite color) drusy/scaly coatings and compact balls up to 0.5 mm. Individual crystals are up to ~0.1 mm. Crystals are transparent with a white streak and a vitreous luster. The mineral is brittle with a smooth curved fracture and no apparent cleavage. Mohs hardness is 2½ The density was not measured because crystal fragments are virtually invisible in density liquids; Dcalc = 2.504 g/cm3. Alfredopetrovite is optically uniaxial (+), ω = 1.554(2), and ε = 1.566(2) (white light); non-pleochroic. The average of 3 electron probe WDS analyses [wt% (range)/wt% normalized to 100%] is: CuO 1.27 (1.04-1.46)/1.09, CoO 0.12 (0.10-0.15)/0.10, NiO 0.51 (0.35-0.68)/0.44, Al2O3 20.99 (20.41-22.04)/18.12, SeO2 69.63 (68.83-70.36)/60.12, H2O (by structure analysis) 23.30/20.12, total 115.82/99.99. The high total is due to dehydration in vacuum and under electron beam. The empirical formula based on 15 O apfu is Al1.94Cu0.07Ni0.03Co0.01Se2.95O15H12.16. IR data was not obtained. The strongest lines in the X-ray powder diffraction pattern are [d Å (I; hkl)]: 7.63 (55; 100), 6.22 (55; 101), 5.37 (26; 002), 4.398 (40; 110,102), 3.404 (100; 112), 2.783 (50; 211), 2.606 (22; 203), 1.661 (26; 410,322,314,116). The unit-cell parameters refined from the powder data are: a = 8.7978(14), c = 10.7184(18) Å, V = 718.5 Å3. Alfredopetrovite is hexagonal, space group P62c. The single crystal unit-cell parameters are: a = 8.818(3), c = 10.721(2) Å, V = 722.0 Å3, and Z = 2. The crystal structure was refined to R1 = 0.0268 for 240 observed [Fo > 4σFo] reflections. The structure is comprised of fairly regular AlO6 octahedra and Se4+O3 triangular pyramids. Three Se4+O3 pyramids link two adjacent AlO6 octahedra forming a [Al(H2O)3]2(Se4+O3)3 unit. These units are bonded only via hydrogen bonds yielding a structure with relatively large channels along [001]. The configuration of the cluster is similar to that of the distinctive unit in the NASICON (sodium super-ionic conductor) structure, commonly referred as a lantern unit. The mineral is named in honor of Alfredo Petrov (b. 1955), geologist/mineralogist and an avid mineral collector for his contributions to mineralogy and geology of Bolivia and as well for his contributions to mineral collector’s community as an author of a numerous publications and an active manager of http://www.mindat.org. Four cotypes (one of those is also cotype for favreauite) are deposited in the Natural History Museum of Los Angeles County, Los Angeles, U.S.A. One cotype specimen (it is also a cotype of favreauite) is housed in the Museum Victoria, Australia. D.B.
Bussyite-(Y)[*]
J.D. Grice, R. Rowe and G. Poirier (2015) Bussyite-(Y), a new beryllium silicate mineral species from Mont Saint-Hilaire, Quebec. Canadian Mineralogist, 53(2), 235-248.
Bussyite-(Y) (IMA 2014-060), (Y,REE,Ca)3(Na,Ca)6MnSi9Be5 (O,OH,F)34, is a new mineral species from the Poudrette quarry (level 7), Mont Saint-Hilaire, Quebec, Canada. It occurs in a small alkaline pegmatite as embedded dark brown prismatic crystals inside massive white analcime. It differs from associated aegirine prisms by rectangular cross sections. Other associated minerals include microcline, sérandite, calcite, cappelenite-(Y), catapleiite, charmarite-2H and -3T, fluorite, helvine, kupletskite, perraultite, and tainiolite. The bussyite-(Y) crystals are prismatic to bladed, blocky, sometimes radiating, and reach up to 3 mm. The mineral is transparent to translucent, with a white streak and vitreous luster. It is brittle with a perfect {101} cleavage and splintery fracture; Mohs hardness is ~4. The density was not measured due to the small grain size; Dcalc = 3.11 g/cm3. Bussyite-(Y) is non-pleochroic, optically biaxial (-) with α = 1.583(2), β = 1.593(2), γ = 1.600(2), 2Vmeas = 68(2)°, 2Vcalc = 79°; Z^c = 33° (β obtuse), Y = b, and X = [101]. Dispersion was not observed. Fine lamellar twinning, parallel to the elongation, was noted in some crystals. On the IR spectrum of bussyite-(Y) a low broad peak at 3500-2500 cm-1 and 4 minor peaks in the 2500-2000 cm-1 range are assigned to OH stretching vibrations. The large broad peak centered at 967 cm-1 assigned to [SiO4] and [BeO4] stretching modes with shoulders at 1008 and 1036 cm-1 likely due to the shorter bonds between Be and Si and OH and F. The moderate sharper peaks at 859, 705, and 647 cm-1 are assigned to the [SiO4] and [BeO4] bending modes. The average of 3 electron probe WDS analysis [wt% (ranges)] is: Na2O 8.21 (8.07-8.43), K2O 0.08 (0.50-0.10), BeO 9.75 (by structure refinement), CaO 5.25 (5.16-5.36), MnO 2.93 (2.57-3.20), BaO 0.03 (0-0.06), FeO 0.40 (0.25-0.60), A2O3 0.29 (0.21-0.34), Y2O3 7.58 (7.37-7.79), La2O3 0.48 (0.40-0.60), Ce2O3 2.66 (2.37-3.09), Pr2O3 0.55 (0.40-0.64), Nd2O3 2.85 (2.81-2.93), Sm2O3 1.45 (1.23-1.58), Eu2O3 0.013 (0.12-0.17), Gd2O3 1.97 (1.57-2.21), Tb2O3 0.31 (0.25-0.40), Dy2O3 2.20 (1.81-2.46), Ho2O3 0.39 (0.33-0.48), Er2O3 0.93 (0.86-1.07), Tm2O3 0.16 (0.12-0.20), Yb2O3 0.46 (0.36-0.60), Lu2O3 0.01 (0.01-0.01), Nb2O5 0.20 (0.15-0.25), SiO2 39.62 (38.96-40.03), ThO2 2.21 (1.90-2.43), F 3.49 (3.39-3.66), Cl 0.03 (0.02-0.03), H2O 5.10 (by structure refinement), -O=(F+Cl)2 1.48, total 98.15. The empirical formula based on the 34 anions pfu is: (Y0.87Nd0.22Ce0.21Dy0.15Gd0.14Sm0.11Er0.06Pr0.04La0.04Yb0.03Ho0.03Tb0.02Tm0.01Eu0.01Ca0.79Th0.11)Σ2.84 (Na3.45Ca0.43K0.02)Σ3.90 (Mn0.54Fe0.07)Σ0.61 (Si8.59Be5.08Al0.07)Σ13.74 (O24.11OH5.89)Σ30 (F2.39OH1.60Cl0.01)Σ4. The strongest lines of the powder X-ray diffraction pattern [d Å (I%; hkl)] are: 8.049 (
Colinowensite[*]
B. Rieck, H. Pristacz and G. Giester (2015) Colinowensite, BaCuSi2O6, a new mineral from the Kalahari Manganese Field, South Africa and new data on wesselsite, SrCuSi4O10. Mineralogical Magazine, 79(7), 1769-1778.
Colinowensite (IMA 2012-060), ideally BaCuSi2O6, is new mineral species from the central-eastern ore body of the Wessels mine, Kalahari Manganese Field, Northern Cape Province, South Africa. It was found in 2 specimens which both contain a subset of typical paragenesis of Ba-, Sr-, and Cu-bearing silicates effenbergerite-wesselsite, lavinskyite, scottyite, and diegogattaite, in close association with pectolite, quartz, aegirine, and richterite, minerals of the garnet group and a number of manganese and iron oxides with a dominance of hausmannite and hematite. Sugilite, which is generally found in the same paragenesis, is almost completely absent on these specimens. Colinowensite forms purple to dark blue (when thicker) vitreous subhedral crystals up to 100 × 100 × 50 μm with a purple streak. The crystal forms {100} and {110} are observed while {001} is always present as a cleavage planes. No fluorescence is observed under UV radiation. The mineral is brittle, with uneven fracture, and the estimated Mohs hardness is ~4. The density by micropicnometry is 4.20(5); Dcalc = 4.236 g/cm3. Colinowensite is not soluble in acids except HF. It shows very intense absorption in the range 450-620 nm, rendering the mineral almost opaque. Optical measurements in this range lack any confidence. They are feasible below and above this range, albeit with a relatively large estimated error. Colinowensite is uniaxial (-), with ω = 1.740(20), ε = 1.735(20) (420 nm) and ω = 1.745(20), ε = 1.730(20) (650 nm). It is very strongly pleochroic from purple along the c axis to blue in a perpendicular direction. The average of electron probe WDS analysis of 5 fragments (4 spots each) [wt% (range)] is: CuO 22.53 (22.09-22.98), BaO 43.43 (42.58-4.29), SiO2 34.04 (33.71-34.37), total 100.00. No other elements detectable by electron probe were found. The empirical formulae based on 6 O apfu is Ba1.00Cu1.00Si2.00O6. No IR data was obtained. The strongest lines of the powder X-ray diffraction pattern [d Å (I%; hkl)] are: 5.577 (31; 004), 4.997 (30; 020), 4.560 (31; 022), 3.533 (70; 220), 2.985 (100; 224), 2.499 (57; 040), 2.280 (23; 044), 1.767 (19; 440). The parameters of the tetragonal unit cell refined from the powder data are a = 9.9762(4), c = 22.3200(9) Å, V = 2221.4 Å3. The single crystal unit-cell parameters are a = 9.967(1), c = 22.290(2) Å, V = 2214.4 Å3, Z = 16, space group I41/acd. The crystal structure solved and refined to R1 = 0.021 based on 1379 unique Fo > 4σ(Fo) reflections. Colinowensite is a cyclosilicate with a 4-membered single rings [Si4O12]8-, arranged in sheets parallel to (001). CuO4 squares sharing corners with four neighboring silicate rings within a sheet. Ba2+ cations are bonded to 10 O atoms in irregular coordination. Colinowensite is the natural analog of the well-studied synthetic pigment referred to as Chinese or Han purple, which is found on artifacts from ancient and imperial China. The mineral was named for the mineral collector and finder of the new species, Colin R. Owens (b. 1937), of Somerset West, South Africa. Type material is deposited in the collection of the Institut für Mineralogie und Kristallographie, University of Vienna, Austria. The X-ray structure refinement of single crystals taken from the newly collected wesselsite is also provided in the paper. Wesselsite belongs to the gillespite type of compounds with general formula ABSi4O10 (A = Ca, Sr, Ba; B = Cr, Fe, Cu). The crystal structure is characterized by 4-membered rings of SiO4 tetrahedra, [Si4O10]4-, which are connected into infinite sheets parallel to (001). Cu atoms in nearly planar square coordination are attached on both sides of the sheets. Adjacent layers are linked together by the Sr atoms in distorted square-antiprismatic coordination. Based on microprobe and refined site occupancy data, the composition of studied wesselsite is close to Sr0.9Ba0.1CuSi4O10. The parameters of the tetragonal unit-cell are: a = 7.374(1), c = 15.636(2) Å, V = 850.2 Å3, space group P4/ncc, Z = 4. The complete solid solution has been observed for the synthetic compounds and in wide range between natural wesselsite and effenbergerite. Contrary to this, no significant Ba-Sr substitution was found in colinowensite and scottyite and no isotypic strontium copper silicates are known. D.B.
Esquireite[*]
A.R. Kampf, R.M. Housley, G.E. Dunning and R.E. Walstrom (2015) Esquireite, BaSi6O13·7H2O, a new layer silicate from the barium silicate deposits of California. Canadian Mineralogist, 53(1), 3-12.
The new mineral esquireite (IMA 2014-066), ideally BaSi6O13·7H2O was found at the Esquire #1 claim along Rush Creek, eastern Fresno County, California, U.S.A. (36°58′25″N 119°15′01″W), and in Ba-silicate lens on the NW slope of Trumbull Peak, Mariposa County, California, U.S.A. (37°41′31″N 119°51′51″W). This is the 18th new species to be described from these localities. Esquireite forms as the result of contact metamorphism of Ba-rich sediments on sanbornite cleavage surfaces and along fractures transverse to cleavages. It is also often found in intimate association with or embedded in white, massive witherite and/or opal. All three minerals appear to be low-temperature hydrothermal alteration products of sanbornite, with opal postdating esquireite. At the Esquire #1 claim esquireite is also associated with cerchiaraite-(Al), kampfite, macdonaldite, pyrrhotite, quartz, titantaramellite, and traskite. At Trumbull Peak, it is also associated with fencooperite, gillespite, macdonaldite, quartz, and titantaramellite. Esquireite occurs as colorless transparent rectangular blades, elongated and striated parallel to [010] and flattened on {001}. Twinning is common on {001}. The streak is white, the luster is vitreous to pearly. The mineral shows no fluorescence under UV radiation. It is brittle with irregular fracture and Mohs hardness is ~2. Two cleavages are observed: perfect on {001} and fair on {100}. The density (by flotation in an aqueous solution of sodium polytungstate) is Dmeas = 2.18(2) g/cm3; Dcalc = 2.237 g/cm3. The mineral is insoluble and unreactive in concentrated HCl, H2SO4, HNO3, and NaOH. Esquireite is optically biaxial (+), with α = 1.477, β = 1.481, γcalc = 1.492 (white light), 2Vmeas = 63.8(6)°; Y = b, Z^ c ≈ 22°. No dispersion or pleochroism was observed. The average of the WDS electron probe analyses (wt% for 4 points from Esquire #1 claim samples and 2 from Trumbull Peak crystals) along with the ranges (in parentheses) are: BaO 25.65 (25.06-26.20), SiO2 63.60 (62.88-64.53), H2O (based upon the crystal structure) 22.41, total 111.66 (due to dehydration under vacuum). The data normalized to a total of 100% are BaO 22.97, SiO2 56.96, H2O 20.07. The empirical formula (based on 20 O apfu) is Ba0.95Si6.00O20H14.10. The strongest lines in the X-ray powder diffraction pattern obtained in powdered sample by Gandolfi-type motion [d Å (I%; hkl)] are: 7.02 (38; 002), 5.11 (33; 201), 4.649(66; 003,
Ferromerrillite[*]
S.N. Britvin, S.V. Krivovichev and T. Armbruster (2016) Ferromerrillite, Ca9NaFe2+(PO4)7, a new mineral from the Martian meteorites, and some insights into merrillite-tuite transformation in shergottites. European Journal of Mineralogy, 28, 125-136.
Ferromerrillite (IMA 2006-039), ideally Ca9NaFe2+(PO4)7, is a new mineral found as an accessory phase in shergottites, in the basaltic and olivine-phyric subgroups of those meteorites, where merrillite is found substantially enriched in iron, which substitutes for magnesium. Two basaltic shergottites have been studied for definition of the new mineral: Shergotty (the type occurrence) and Los Angeles (Warren et al. 2004). Ferromerrillite associated with clinopyroxene and maskelynite (the impact-melted plagioclase glass). Twenty anhedral grains of 15-20 pm in size have been extracted from sample of Shergotty and 30 grains of 20-50 pm in size from the sample of Los Angeles. Ferromerrillite grains are colorless and have no observable cleavage. They are non-fluorescent under short- and long-wave ultraviolet light. Luster is vitreous. Mohs hardness is ~5. In the immersion liquids (n = 1.625) grains are colorless and non-pleochroic. Ferromerrillite is optically uniaxial (-) to anomalously biaxial with 2 V up to 20°. Refractive indexes are ω = 1.623 and 1.624; ε = 1.621 and 1.621 for the mineral from Shergotty and Los Angeles, respectively (wavelength not reported). The density of the mineral from Shergotty could not be measured due to the scarcity of the material; Dcalc = 3.11 g/cm3. The density of the mineral from Los Angeles is Dmeas = 3.14 g/cm3 (sink-float method) Dcalc = 3.17 g/cm3. The average of 8 (Shergotty sample) and 10 (Los Angeles sample) electron probe EDS analyses (ranges not reported) [wt%, Shergotty/wt%, Los Angeles] is: Na2O 1.7/1.4, CaO 46.8/47.0, MgO 1.5/0.9, FeO 3.5/5.2, P2O5 46.2/45.7, total 99.7/100.2. The empirical formula, based on 28 O apfu, is Ca9.00(Na0.60Ca0.07)Σ0.67
Comment: No direct determination of Fe3+ content has been provided by the authors in their description. The authors discuss the iron oxidation state on the basis of statistical analysis of correlation of lattice parameters and composition of M sites of known whitlockite-type compounds with available chemical analyses of merrillite samples and of the calculated bond valence values obtained from refined structure data. They conclude that all iron is divalent in the studies samples of ferromerrillite. However, the authors report Fe3+ in the formulas reported at Tables 2 and 3. These are probably an uncorrected error left from a previous version of the draft manuscript and these Fe3+ should not be taken into account nor mentioned in future work. Oxidation state in martian minerals is a debated item and therefore particular attention should be paid to avoid propagation of erroneous data unsupported by strong evidences.
References cited
Warren, P.H., Greenwood, J.P., and Rubin, A.E. (2004) Los Angeles: a tale of two stones. Meteoritics Planetary Science, 39, 137-156.
Fluornatropyrochlore[*]
J. Yin, G. Li, G. Yang, X. Ge, H. Xu and J. Wang (2015) Fluornatropyrochlore, a new pyrochlore supergroup mineral from the Boziguoer rare earth element deposit, Baicheng County, Akesu, Xinjiang, China. Canadian Mineralogist, 53(3), 455-460.
The description of fluornatropyrochlore (IMA 2013-056), with a general formulae (Na,Pb,Ca,REE,U)2Nb2O6F changes status of this mineral from possible new species (Christy and Atencio 2013) to an officially approved species according current nomenclature of the pyrochlore supergroup (Atencio et al. 2010). The mineral was found in the alkali granite intruded into Silurian marble at the Boziguoer REE deposit, Baicheng County, Akesu, Xinjiang Autonomous Region, China (42°13′14″N; 81°54′29″E). It is closely associated with microcline, albite, aegirine, sodic amphibole, biotite, zircon, rutile, thorite, fluorite, fluocerite-(Ce), columbite-(Fe), xenotime-(Y), astrophyllite, chevkinite-(Ce), and fergusonite-(Y). Fluornatropyrochlore forms translucent to transparent brownish yellow to reddish orange, anhedral, rarely subhedral grains from 0.02 to 0.25 mm with an adamantine luster and light yellow streak. The mineral does not fluoresce in UV light. No cleavage or parting was observed. It is brittle with Mohs hardness 4-4/2. The density was not measured; Dcalc = 5.375 g/cm3. Fluornatropyrochlore is optically isotropic, n = 2.10(5) (589.9 nm). FTIR spectrum show the absence of bands of OH or H2O groups with only single peak at 931 cm-1. The average of 10 electron probe WDS analysis on 2 grains [wt%, (range)] is: Na2O 6.80 (3.33-9.30), K2O 0.01 (0-0.04), CaO 2.01 (1.69-2.22), MgO 0.01 (0-0.05), FeO 0.05 (0-0.15), SrO 0.03 (0-0.11), PbO 16.17 (14.75-18.77), Ce2O3 4.29 (3.76-5.41), La2O3 1.65 (1.37-1.93), Nd2O3 0.41 (0-0.62), Y2O3 0.42 (0.17-0.67), SiO2 0.03 (0-0.09), TiO2 1.36 (0.72-1.91), UO2 5.81 (4.21-7.36), Ta2O5 3.00 (1.33-4.00), Nb2O5 53.42 (51.71-56.16), F 3.19 (2.33-4.12), Cl 0.02 (0-0.06), ThO2 0.48 (0.13-1.41), Sb2O5 0.01 (0-0.07), ZrO2 0.01 (0-0.13), MnO 0.04 (0-0.11), SnO2 0.34 (0.23-0.41), -O=(F,Cl)2, total 98.21. Ba, Al, and P were found below detection limit of 0.01 wt%. The empirical formula based on 7 anions pfu is: (Na1.03Pb0.34Ca0.17U0.10Th0.01Ce0.12La0.05Y0.02Nd0.0OΣ1.85 (Nb1.88Ti0.08Ta0.06Sn0.0OΣ2.03O6.21F0.79. The strongest lines in the powder XRD pattern are [d Å (I; hkl)]: 6.074 (3; 111), 3.042 (100; 222), 2.628 (38; 004), 1.859 (34; 044), 1.582 (15; 226), 1.515 (4; 444), 1.3137 (2; 008), 1.2045 (3; 266), 1.1726 (2; 048), 1.0712 (1; 448). The mineral is cubic with a = 10.5053(10) Å, V = 1159.4 Å3, Z = 8, space group Fd
References cited
Atencio, D., Andrade, M.B., Christy, A.G., Gieré, R., and Kartashov, P.M. (2010) The pyrochlore supergroup of minerals: Nomenclature. Canadian Mineralogist, 48, 673-698.
Christy, A.G., and Atencio, D. (2013) Clarification of status of species in the pyrochlore supergroup. Mineralogical Magazine, 77, 13-20.
Fluor-Schorl[*]
A. Ertl, U. Kolitsch, M.D. Dyar, H.-P. Meyer, G.R. Rossman, D.J. Henry, M. Prem, Th. Ludwig, L. Nasdala, C.L. Lengauer, E. Tillmanns and G. Niedermayr (2016) Fluor-schorl, a new member of the tourmaline supergroup, and new data on schorl from the cotype localities. European Journal of Mineralogy, 28(1), 163–177.
Fluor-schorl (IMA 2010-067), ideally
References cited
Henry, D.J., Novák, M., Hawthorne, F.C., Ertl, A., Dutrow, B.L., Uher, P., and Pezzotta, F. (2010) Nomenclature of the tourmaline supergroup minerals. American Mineralogist, 96, 895–913.
Hogarthite[*]
A.M. Mcdonald, P. Tarassoff and G.Y. Chao (2015) Hogarthite, (Na,K)2CaTi2Si10O26·8H2O, a new member of the lemoynite group from Mont Saint-Hilaire, Quebec: Characterization, crystal structure determination, and origin. Canadian Mineralogist, 53(1), 13–30.
The new mineral hogarthite, (IMA 2009-043), (Na,K)2CaTi2Si10O26·8H2O, was discovered in vugs within metasomatically altered marble xenoliths in the Poudrette quarry, Mont Saint-Hilaire, La-Vallée-du-Richelieu RCM, Montérégie, Quebec, Canada, where it formed from a late-stage alkaline fluid enriched in SiO2 and TiO2, under conditions of low P at T < 200 °C, and possibly through crystallization of a gel. Hogarthite associated with calcite (several generations), quartz, haineaultite, labuntsovite-Mn, lemoynite, chabazite, and gmelinite-Na. Hogarthite forms dense, radiating crystal aggregates up to 0.5 × 3 mm. Individual crystals are bladed to blocky (0.05 × 0.15 × 2 mm in average), elongated by [100], flattened on {010} and bounded by the dominant pinacoid {010} and minor pinacoids {100} and {001}. Color varies from tan to white or colorless in different crystal zones. The streak is white and luster is satiny to silky or subvitreous. No fluorescence observed under UV radiation. The mineral is brittle with a perfect {010} cleavage, hackly to splintery fracture and estimated Mohs hardness of 4. Density was not measured; Dcalc = 2.40(1) g/cm3. Hogarthite is optically biaxial (+) with α = 1.567(1), β = 1.591(1), γ = 1.618(1) (λ = 590 nm), 2Vmeas = 87(1)° and 2Vcalc = 88(1)°, X = b, Y ∧ c = 15° (in the obtuse angle β), Z = a. IR/Raman spectra show bands (cm-1, rs = relatively sharp, s = sharp, b = broad, vb = very broad) at 3612rs/3607b, 3372rb, 3246b/3411vb, 3239vb (OH stretch), 1645rs/1608vb (H-O-H bend), Si-O stretch bands at 1126, 1016, 968, 935(all s)/1190b, 1052s, 942s, 902s, and Si-O stretch bands at 788s, 712s, 678s/794rb, 714rb, 679s. Other Raman sharp bands are Ti-O stretch 548, 448 cm-1, Ti-O-Si, Ti-O-Ti stretch at 295, 258, 225 cm-1, and lattice vibrations at 173, 135, 105 cm-1. The average of 21 electron probe EDS analyses obtained on 7 crystals is [wt%, (range)]: Na2O 2.37 (1.69–2.92), K2O 2.88 (2.61–3.17), CaO 6.00 (5.40–6.31), TiO2 14.44 (13.70–15.83), ZrO2 1.11 (0.48–1.73), Nb2O5 0.78 (0.42–1.24), SiO2 59.27 (57.32–60.64), H2O 14.10 (calc), total 100.95. On the basis of 34 O apfu, the empirical formula is (Na0.78K0.62◻0.51Ca0.09)Σ2.00Ca(Ti1.85Zr0.09Nb0.06)Σ2.00Si10.09O26·8H2O. The strongest lines of the X-ray powder diffraction pattern are [d Å(I; hkl)]: 8.835 (85; 001), 7.913 (100; 020), 6.849 (70;
Shilovite[*]
N.V. Chukanov, S.N. Britvin, G. Möhn, I.V. Pekov, N.V. Zubkova, F. Nestola, A.V. Kasatkin and M. Dini (2015) Shilovite, natural copper(II) tetrammine nitrate, a new mineral species. Mineralogical Magazine, 79(3), 613–623.
Shilovite (2014-016), ideally Cu(NH3)4(NO3)2, is a new mineral found at the Pabellón de Pica Mountain, near Chanabaya, Iquique Province, Tarapacá Region, Chile. Associated minerals include halite, ammineite, atacamite, and thénardite. The host rock is a gabbro that consists of amphibole, plagioclase, and minor clinochlore, and contains accessory chalcopyrite that is considered the source of Cu for shilovite. Shilovite forms imperfect, thick tabular to equant crystals up to 0.15 mm in size included in massive halite. The new mineral is deep violet blue with a violet blue streak that changes to light blue as a result of decomposition and loss of NH3. Crystals of shilovite are translucent with a vitreous luster, are sectile and show no cleavage. Density was not measured due to the small grain size of crystals and the instability of the mineral in available heavy liquids. Dcalc = 1.92 g/cm3. Mohs hardness < 2. Shilovite is optically biaxial (+), α = 1.527(2), β = 1.545(5), γ = 1.610(2), 2V ≈ 40–50°, but could not be determined accurately because the mineral decomposes rapidly in immersion liquids. 2Vcalc = 57°. Shilovite is non-fluorescent. The main absorption bands of the IR spectrum (cm-1, w = weak, s = strong) are: 3200–3700 (N-H stretching vibrations), 1700–3000w (overtones and combination modes involving N-O stretching and H-N-H bending), 1650 (degenerate bending vibrations of NH3 molecules), 1361s and 1431s (asymmetric stretching vibrations of
Tapiaite[*]
A.R. Kampf, S.J. Mills, B.P. Nash, M. Dini and A.A. Molina Donoso (2015) Tapiaite, Ca5Al2(AsO4)4(OH)4·12H2O, a new mineral from the Jote mine, Tierra Amarilla, Chile. Mineralogical Magazine, 79(2), 345–354.
Tapiaite (IMA 2014-024), ideally Ca5Al2(AsO4)4(OH)4·12H2O, is a new mineral found at the Jote mine, Tierra Amarilla, Copiapó Province, Atacama, Chile. Tapiaite is a late-stage, low-temperature, secondary mineral that occurs in narrow seams and vugs in the oxidized upper portion of a hydrothermal sulfide vein hosted by volcanoclastic rocks. The deeper unoxidized portion of the vein contains primary and supergene minerals including acanthite, native arsenic, Ag sulfosalts, barite, calcite, chalcopyrite, domeykite, feldspar, pyrite, quartz, native silver, and stibnite. Tapiaite associated with conichalcite, joteite, mansfieldite, pharmacoalumite, pharmacosiderite, and scorodite. Crystals occur as colorless blades up to ~0.5 mm long flattened on {101} and elongated and striated along [010]. The blades are commonly intergrown in subparallel bundles and less commonly in sprays. Forms {101}, {101}, and {111} are observed. Crystals are easily soluble in dilute HCl at room temperature and slowly soluble in H2O. Tapiaite is transparent with white streak and vitreous luster, is brittle, has splintery fracture, perfect cleavage on {101} and {101}, and shows no twinning. It does not fluoresce under UV light. The Mohs hardness is ~2–3. Density was not measured due to the crystals being too difficult to see in Clerici solution. Dcalc = 2.681 g/cm3. Tapiaite is non-pleochroic, optically biaxial (+) with α = 1.579(1), β = 1.588(1), γ = 1.610(1), 2Vmeas = 66(2)°, and 2Vcalc = 66°; X ≈ [101]; Y = b, Z ≈ [101]. The average of 5 electron probe WDS analyses on 5 crystals [wt% (range)] is: Na2O 0.09 (0.04–0.16), CaO 24.96 (24.13–25.89), CuO 0.73 (0.15–1.75), Al2O3 10.08 (9.48–10.70), Fe2O3 0.19 (0.04–0.41), As2O5 40.98 (39.84–42.56), Sb2O5 0.09 (0.07–0.13), H2O 23.46 [calculated on the basis of 11 total cations (Ca+Na+Cu+Al+Fe+As+Sb), charge balance and 32 O], total 100.58. This gives the empirical formula
Waimirite-(Y)[*]
D. Atencio, A.C. Bastos Neto, V.P. Pereira, J.T.M.M. Ferron, M. Hoshino,T. Moriyama, Y. Watanabe, R. Miyawaki, J.M.V. Coutinho, M.B. Andrade, K. Domanik, N.V. Chukanov, K. Momma, H. Hirano and M. Tsunematsu (2015) Waimirite-(Y), orthorhombic YF3, a new mineral from the Pitinga mine, Presidente Figueiredo, Amazonas, Brazil and from Jabal Tawlah, Saudi Arabia: description and crystal structure. Mineralogical Magazine, 79(3), 767–780.
Waimirite-(Y) (IMA 2013-108), orthorhombic YF3, is a new mineral found at the A-type Madeira granite (~1820 Ma), at the Pitinga mine, Presidente Figueiredo Co., Amazonas State, Brazil, as well as at Jabal Tawlah (Mount Tawlah) in the Kingdom of Saudi Arabia. At the Pitinga mine, the mineral occurs in hydrothermal veins (up to 30 mm thick) cross-cutting the albite-enriched facies associated with halloysite. Minerals in the granite are K-feldspar, albite, quartz, riebeckite, biotite, muscovite, cryolite, zircon, polylithionite, cassiterite, pyrochlore-group minerals, columbite, thorite, native lead, hematite, galena, fluorite, xenotime-(Y), gagarinite-(Y), fluocerite-(Ce), genthelvite-helvite, topaz, illite, kaolinite, and chlorite. At Jabal Tawlah, waimirite-(Y) occurs in hydrothermally altered quartz-rich microgranite, also as the main REE mineral. Associated minerals include biotite, albite, muscovite, microcline, columbite-(Fe), zircon, thorite, xenotime-(Y), samarskite-(Y), ilmenite, an undetermined Ca-Y-F mineral, euxenite-(Y), fergusonite-(Y), rutile, illite, barite, calcite, and goethite. Waimirite-(Y) formed from fluorine-rich hydrothermal fluids containing large amounts of REE. Waimirite-(Y) from Brazil occurs as aggregates of platy crystals up to ~1 μm. Forms observed (determined on synthetic YF3 only) are pinacoids, prisms, and bipyramids. Crystals are pink with white streak, are transparent to translucent with non-metallic luster, show no cleavage (synthetic YF3 shows perfect cleavage on {010}) or parting. The Mohs hardness and density was not measured due to the small crystal size; Dcalc = 5.586 g/cm3. Waimirite-(Y) is biaxial, mean n = 1.54–1.56. It is non-fluorescent under UV radiation. Waimirite-(Y) from Saudi Arabia occurs as inclusions in an undetermined Ca-Y-F mineral where anhedral-to-subhedral crystals of several tens to several hundreds of micrometers in size are common. The mineral is colorless with white streak, is transparent with vitreous luster, shows no cleavage, has irregular to conchoidal fracture and is brittle. The density was not measured because of small grain size; Dcalc = 5.678 g/cm3. The indentation hardness VHN100 = 700 (667–786) kg/mm2 corresponding to 5–6 of the Mohs scale. It is optically biaxial (+) with 2V = 70–80° and mean refractive index n ≈ 1.60. At the IR spectrum of the material from Brazil polluted with a halloysite a strong band at 380 cm-1 (with shoulders at 400 and 440 cm-1) belongs to waimirite-(Y). IR spectrum demonstrates the absence of carbonate and borate groups. The average of 24 electron probe WDS analyses on the sample from Brazil [wt% (range)] is: F 29.27 (28.43–30.19), Y 37.25 (34.78–38.89), La 0.19 (0.01–0.28), Ce 0.30 (0.19–0.46), Pr 0.15 (0.03–0.25), Nd 0.65 (0.57–0.81), Sm 0.74 (0.66–0.87), Gd 1.86 (1.65–2.09), Tb 0.78 (0.60–0.95), Dy 8.06 (7.36–8.81), Ho 1.85 (1.47–2.35), Er 6.38 (5.80–7.24), Tm 1.00 (0.69–1.34), Yb 5.52 (4.99–6.16), Lu 0.65 (0.38–1.58), Ca 0.83 (0.71–0.97), O 2.05 (calculated by charge balance), total 97.53. This gives the empirical formula (Y0.69Dy0.08Er0.06Yb0.05Ca0.03Gd0.02Ho0.02Nd0.01 Sm0.01Tb0.01Tm0.01Lu0.01)Σ1.00[F2.54◻0.25O0.21]Σ3.00 based on 1 cation pfu. The average of 24 electron probe WDS analyses on the sample from Saudi Arabia [wt% (range)] is: F 34.34 (33.44–35.19), Y 44.61 (43.22–48.84), Ce 0.08 (0.04–0.12), Nd 0.04 (0.02–0.07), Sm 0.14 (0.11–0.18), Gd 2.95 (2.57–3.41), Tb 0.72 (0.59–0.81), Dy 7.77 (6.84–7.96), Ho 2.27 (1.95–2.50), Er 5.39 (5.05–5.68), Tm 0.69 (0.61–0.75), Yb 1.36 (1.03–1.56), Na 0.06 (0.02–0.09), Ca 0.08 (0.03–0.05), O 0.80 (by charge balance), total 101.30. This gives the empirical formula (Y0.79Dy0.08Er0.05Gd0.03Ho0.02Tb0.01Tm0.01Yb0.01)Σ1.00[F2.85O0.08◻0.07]Σ3.00 based on 1 cation pfu. The strongest lines in the X-ray powder-diffraction pattern of waimirite-(Y) from Brazil [d (Å) (I%; hkl)] are: 3.707 (26; 011), 3.623 (78; 101), 3.438 (99; 020), 3.205 (100; 111), 2.894 (59; 210), 1.937 (33; 131), 1.916 (24; 301), 1.862 (27; 230). The unit-cell parameters refined from powder-diffraction data, by analogy with the synthetic equivalent, are a = 6.386(1), b = 6.877(1), c = 4.401(1) Å, V = 193.28 Å3, Z = 4. Singlecrystal X-ray diffraction data collected on a crystal from Saudi Arabia of size 0.05 × 0.03 × 0.02 μm refined to R1 = 0.0163 for 191 unique I > 2σ(I) reflections shows waimirite-(Y) is orthorhombic, Pnma, a = 6.38270(12), b = 6.86727(12), c = 4.39168(8) Å, V = 192.495 Å3, Z = 4. Waimirite-(Y) is isomorphous with synthetic SmF3, HoF3, and YbF3. The crystal structure of waimirite-(Y) consists of Y atom that are ninefold-coordinated to form YF9 tricapped trigonal prisms. The name waimirite is for the Waimiri-Atroari Indian people of Roraima and Amazonas, while the “Y” suffix was introduced because it is a rare-earth mineral. Type material has been deposited in the Museu de Geociências, Instituto de Geociências, Universidade de São Paulo, Brazil, and in the Museu de Mineralogia Luiz Englert, Departamento de Mineralogia e Petrologia, Instituto de Geociências, Universidade Federal do Rio Grande do Sul, Brazil. Part of the cotype sample has been deposited at the University of Arizona Mineral Museum, RRUFF Project. O.C.G.
*All minerals marked with an asterisk have been approved by the IMA CNMMC.
† For a complete listing of all IMA-validated unnamed minerals and their codes, see http://pubsites.uws.edu.au/ima-cnmnc/.
© 2016 by Walter de Gruyter Berlin/Boston