Refinement of the Crystal Structure of Ramsayite (Lorenzenite) Rurro Krvnxas

Total Page:16

File Type:pdf, Size:1020Kb

Refinement of the Crystal Structure of Ramsayite (Lorenzenite) Rurro Krvnxas American Mineralogist, Volume 72, pages 173-177, 1987 Refinementof the crystal structure of ramsayite (lorenzenite) M,q.RKru R. SuNonBnc Department of Inorganic Chemistry, University of Helsinki, Vuorikatu 20, SF-00100 Helsinki 10, Finland Ml.nrtr LnHrrNnN Department of Geology, University of Helsinki, Snellmaninkatu 5, SF-00170 Helsinki 17, Finland Rurro KrvnxAs Department of Inorganic Chemistry, University of Helsinki, Vuorikatu 20, SF-00100 Helsinki 10, Finland Ansrn-c.cr The lattice parameters and crystal structure of ramsayite, NarTirSirOr, have been re- determined from a specimenfrom the Kola Peninsula.The spacegroup is Pbcn v/rth Z : 4; a : 8.7128(10),b : 5.2327(5),and c : 14.481(2)A. ttre anisotropicrefinement of the data using 778 reflections produced an R value of 0.026. The coordination polyhedron around Ti is a markedly distorted octahedron with no center of symmetry. Around Na there are seven oxygen atoms (Na-O distancesin the range 2.307-2.602 A); these poly- hedra form dimers by sharing three oxygens. The SiOo tetrahedra form pyroxene-type chainsin the direction ofthe b axis by sharingtwo oxygenswith the neighboringtetrahedra. The two remaining oxygensare sharedby two Ti atoms. Two vicinal TiOu polyhedra also share two oxygens(common edge),and the third facial oxygen is shared with the third TiOu polyhedron. These pairs of polyhedra lie approximately parallel to the a-b and a-c planes,respectively. INrnooucrroN ExpnnIltnNTAL DETAILS The two mineral namesramsayite and lorenzeniterefer The material used for study was from the collections of the to the samespecies (Kraus and Mussgnug,1941; Sahama, Mineralogical Museum, University of Helsinki. According to the 1947; Bogglld, 1953).Lorenzenite was found on an ex- original Russian label, the specimen(no. 4937) was collectedin pedition to southern Greenlandin 1897 (Flink, 1901), 1922 by the A. E. Fersman expedition and originates from the occurringin a nephelinesyenite. Chemical analysis showed Lujavr-Urt (:tovozero) alkali massif. Ramsayitefrom the same by Sahama(1947). that it contained ll.92o/o ZrOr. Later o\ in 1922, A. E. specimenwas chemically analyzed The specimenis a coarse-grainednepheline syenite (lujavrite) Fersman's expedition found a related mineral in the and has, in addition to greenishnepheline and microcline, red- nephelinesyenite of the Kola Peninsula.No Zr was found dish-brown eudialite and dark brown ramsayite as its major in this species(Kostyleva, 1937). Because there are very components. The most common accessorymineral is aegirine marked similarities in the crystal forms as well as in the (acmite). The subhedral ramsayite and eudialite crystals range chemical composition of the two minerals, their chemical up to 3 cm in diameter. The reader is referred to Kostyleva composition was redetermined by Sahama (1941). He (1937)and Masov et al. (1966)for thoroughdescriptions ofthe found less than 0.2o/oZrO, in both minerals; moreover, properties of the Lovozero ramsayite. ramsayite and lorenzenite specimens showed similar The powder-diffraction data of Lovozero ramsayite were re- (1974). compositions. Becausethere is a wide variation in the corded and treated as describedin detail by Lehtinen In this connection, it may be mentioned that the diffractogram of parameters reported for the unit cell (Table 1) and be- lorenzenite powder (Sahama, 1947) from Narsarsuk (Narssars- causethe R value (0.128) ofan earlier X-ray study of suk), Greenland, is virtually identical with that of the Lovozero poor ramsayitewas rather (Ch'in-Hanget al., 1969),we ramsayite. The observed and calculated d values are given in undertook redeterminations of both unit-cell parameters Table 2.r and the crystal structure. The single-crystalstudy wasperformed with a Nicolet P3 four- Besides a variation in cell parameters, there is also circle diftactometer. The unit-cell parameterswere obtained from variation in the reported spacegroups (Table l). In par- l8 independent high-angle reflections by using least-squares ticular, Shurtz (1955) showed that the spacegroup ob- methods. The details of the intensity measurementsare given in tained by Kraus and Mussgnugis wrong. Moreover, the Table 3. During data collection, one standard reflection was quality of indexingon the JCPDScard l8-1262 doesnot t Tables 2 and 4, order Document AM- seem to be satisfactory. About half the reflections are To receive copies of 87-325 from the BusinessOfrce, Mineralogical Societyof Amer- unindexed, and the number of the spacegroup on the ica, 1625 I Street,N.W., Washington, D.C. 20006. Pleaseremit card should be 60 rather than 50. $5.00 in advancefor the microfiche. 0003-o04x/87/0l 02{ r 73$02.00 173 174 SUNDBERGET AL.: REFINEMENTOF THE CRYSTALSTRUCTURE OF RAMSAYITE(LORENZENITE) Table1. Latticeparameters and spacegroups reported for ramsayite(lorenzenite) S.g. Ref. 14.51 8.73 5.22 Pbcn Krausand Mussgnug(1941)" 14.51 8.76 5.23 Pbcn Krausand Mussgnug(1941)o 14.26 8.57 5.09 Pnca Belovand Belyaev(1949) 8.66 ( 1n 14.42 Pbcn Shurtz(1955)" 14.518(3) 8.e76(3) 5.081(5) Pnca ch'in-Hanget al (1969) 14.52 8.98 5.09 Pnca Povarennykh(1972) 8.66 14.42 5.18 Pcnb Robertset al. (1974) 14.54 8.75 J.ZJ Pnca JCPDS,card 18-1262(1980) 8.707(3) 5.234(4) 14.492(3) Pbcn This workd 8.7128(1 0) 5.2327(5) 14.487(2\ Pbcn This work" b dpowder-diffraction " Ramsayite; lorenzenite;"synthetic lorenzenite; method; "single-crystal method. measuredafter every 39 reflections.The intensitiesof the former There is, however, one exception: The first coordinate of showed only statistical variation. The data were corrected for our 03 is 0.3336,whereas the correspondingearlier value Lorentz-polarization effectsand also for absorption, since the ry' is 0.431.The presentrefined atomic coordinatesand tem- scansshowed significant variation. The refinement ofthe struc- peraturefactors are shown in Table 5. The structure (Fig. ture was carried out using the x-RAy 76program (Stewart, 1976) l) consistsof pyroxene-type [SirOu]- chains running ap- and a Univac 1108 computer. The atomic coordinatesreported proximately in the direction of the b axis and having 05 earlier (Ch'in-Hang et al., 1969)were transformedto spacegroup 04 of the silicate chain is Pbcn and then used as the starting parameters.After anisotropic as the bridging oxygen atom. refinement, the final R value was 0.026 and R* was 0.035 (l/o'? bonded to one Ti only, whereas03 of the chain connects weights).Anomalous dispersion corrections for Ti, Na, and Si two neighboring Ti atoms. The TiOu octahedralie in two were obtained from Ibers and Hamilton (1974). The observed adjacent layers, alternating in each layer with chains of and calculatedstructure factors are given in Table 4 (seefootnote NaO, polyhedra. This alTangement generatesa close- l). packing system of unique type (the ramsayite type). The bond lengths and anglesare shown in Table 6. Rnsur-rs AND DrscussroN Lattice parameters TiOu polyhedron The lattice parametersobtained are shown in Table I The TiOu polyhedron is a considerably distorted octa- togetherwith valuesreported earlier. The precision ofthe hedron, with six nonequivalent Ti-O bond lengths(in the parametersfrom the literature was, in most cases,difficult range 1.820to 2.181 A) and with Ti lying off-center.Al- to evaluate becauseno standard deviations were given. though one of the coordinatesfor 03 differs significantly However, the lattice parametersreported by Ch'in-Hang from the value reportedby Ch'in-Hang et al. (1969),the et al. (1969) deviate significantlyfrom our values.It seems averageof the bond lengths (1.99 A) is identical to the probable that the poor R value they obtained is due to correspondingaverage of the earlier determination. The inaccurate lattice parameters and the film method they averagevalue falls halfway between the two values cor- used. respondingto the Ti4+-O and Ti3+-O bond lengths, cal- culated from the sum ofthe effectiveionic radii, 1.96 and Outline of the structure 2.02 A, respectively(Shannon, 1976). However, it seems The outline of the structure obtained in this study is that even when Ti has the oxidation number +4, there similar to that reported earlier (Ch'in-Hang et al., 1969). is considerable variation in the bond lengths. In BauTi,rOoo,among I I TiO6 polyhedra, the Ti-O dis- Table3. Crystal,intensity collection, and refinement tances tend to have greater values when Ti does not lie data at the center of symmetry (Hofmeister and Tillmanns, 1984).Moreover, the chemicalanalysis (Sahama, 1947) Formula NarTi2SirO, to assumethat the valence state of Ti is Tia+. Formulaweight 341.95 leads us F(000) 664 The off-center distortion is well known in the poly- z 4 morphs of TiOr, where variations in temperature and Density(g.cm{) Observed 3.45(5) pressure produce significant changesboth in symmetry Calculated 3.44 around Ti(I$ and in the bonding parameters (Simons Space group Pbcn (4i) and Dachille, 1967; Horn et al., 1972;'Meagher andLag- Crystal dimensions(mm) 0.11x0.13x0.20 Radiation MoKa (X : 0.71069A) er, 1979). It has been proposed that the ferroelectricity 2, limits 5'< 2d < 60' and the accompanying distortion of the TiOu coordina- Scan rate 0.9'to 29.3'/min polyhedron in perovskite-type crystals may have their Abs. coefficient(cm-') 30.3 tion Number of independentreflec- origin in a second-order Jahn-Teller effect (Bersuker, tions measured 1167 1966). > Uniquedata used [Fo 6"(F.)] 778 In one direction the TiOu pseudo-octahedraform a di- SUNDBERG ET AL.: REFINEMENT OF THE CRYSTAL STRUCTURE OF RAMSAYITE GORENZENITD 175 Table5. The atomiccoordinates
Recommended publications
  • 19660017397.Pdf
    .. & METEORITIC RUTILE Peter R. Buseck Departments of Geology and Chemistry Arizona State University Tempe, Arizona Klaus Keil Space Sciences Division National Aeronautics and Space Administration Ames Research Center Mof fett Field, California r ABSTRACT Rutile has not been widely recognized as a meteoritic constituent. show, Recent microscopic and electron microprobe studies however, that Ti02 . is a reasonably widespread phase, albeit in minor amounts. X-ray diffraction studies confirm the Ti02 to be rutile. It was observed in the following meteorites - Allegan, Bondoc, Estherville, Farmington, and Vaca Muerta, The rutile is associated primarily with ilmenite and chromite, in some cases as exsolution lamellae. Accepted for publication by American Mineralogist . Rutile, as a meteoritic phase, is not widely known. In their sunanary . of meteorite mineralogy neither Mason (1962) nor Ramdohr (1963) report rutile as a mineral occurring in meteorites, although Ramdohr did describe a similar phase from the Faxmington meteorite in his list of "unidentified minerals," He suggested (correctly) that his "mineral D" dght be rutile. He also ob- served it in several mesosiderites. The mineral was recently mentioned to occur in Vaca Huerta (Fleischer, et al., 1965) and in Odessa (El Goresy, 1965). We have found rutile in the meteorites Allegan, Bondoc, Estherville, Farming- ton, and Vaca Muerta; although nowhere an abundant phase, it appears to be rather widespread. Of the several meteorites in which it was observed, rutile is the most abundant in the Farmington L-group chondrite. There it occurs in fine lamellae in ilmenite. The ilmenite is only sparsely distributed within the . meteorite although wherever it does occur it is in moderately large clusters - up to 0.5 mn in diameter - and it then is usually associated with chromite as well as rutile (Buseck, et al., 1965), Optically, the rutile has a faintly bluish tinge when viewed in reflected, plane-polarized light with immersion objectives.
    [Show full text]
  • Tundrite-(Ce) Na3(Ce; La)4(Ti; Nb)2(Sio4)2(CO3)3O4(OH) ² 2H2O C 2001 Mineral Data Publishing, Version 1.2 ° Crystal Data: Triclinic
    Tundrite-(Ce) Na3(Ce; La)4(Ti; Nb)2(SiO4)2(CO3)3O4(OH) ² 2H2O c 2001 Mineral Data Publishing, version 1.2 ° Crystal Data: Triclinic. Point Group: 1: Crystals acicular along [001] and °attened on 010 , to 3 cm; as stellate groups and spherulitic masses. Twinning: On 010 , producing f g f g pseudorhombohedra. Physical Properties: Cleavage: Pronounced on 010 . Fracture: Splintery. f g Tenacity: Brittle. Hardness = 3 D(meas.) = 3.70{4.12 D(calc.) = 4.06 » Optical Properties: Transparent. Color: Brownish yellow, greenish yellow to bright light green. Streak: Yellowish gray. Luster: Vitreous to adamantine. Optical Class: Biaxial (+). Pleochroism: Weak; X = pale yellow; Z = greenish yellow. Orientation: Z c = 4 {14 . ® = 1.743 ¯ = 1.80 ° = 1.88 2V(meas.) = 76 ^ ± ± ± Cell Data: Space Group: P 1: a = 7.533(4) b = 13.924(6) c = 5.010(2) ® = 99±52(2)0 ¯ = 70±50(3)0 ° = 100± 59(2)0 Z = 1 X-ray Powder Pattern: Il¶³maussaq intrusion, Greenland. 13.49 (100), 2.505 (100), 3.448 (90), 2.766 (90), 3.535 (80), 6.784 (70), 1.914 (70) Chemistry: (1) SiO2 10.03 TiO2 12.20 La2O3 8.57 Ce2O3 24.38 Nd2O3 10.25 RE2O3 5.80 Nb2O5 3.44 CaO 0.75 Na2O 8.20 CO3 16.38 Total [100.00] (1) Il¶³maussaq intrusion, Greenland; by electron microprobe, C con¯rmed by loss on ignition; original analysis given as elements, here recalculated to oxides, corresponding to Na3:17(Ce1:78Nd0:73La0:63RE0:41Ca0:16)§=3:71(Ti1:83Nb0:31)§=2:14(SiO4)2:00(CO3)3:27O4:25: Occurrence: In pegmatite veins associated with nepheline syenites.
    [Show full text]
  • Washington State Minerals Checklist
    Division of Geology and Earth Resources MS 47007; Olympia, WA 98504-7007 Washington State 360-902-1450; 360-902-1785 fax E-mail: [email protected] Website: http://www.dnr.wa.gov/geology Minerals Checklist Note: Mineral names in parentheses are the preferred species names. Compiled by Raymond Lasmanis o Acanthite o Arsenopalladinite o Bustamite o Clinohumite o Enstatite o Harmotome o Actinolite o Arsenopyrite o Bytownite o Clinoptilolite o Epidesmine (Stilbite) o Hastingsite o Adularia o Arsenosulvanite (Plagioclase) o Clinozoisite o Epidote o Hausmannite (Orthoclase) o Arsenpolybasite o Cairngorm (Quartz) o Cobaltite o Epistilbite o Hedenbergite o Aegirine o Astrophyllite o Calamine o Cochromite o Epsomite o Hedleyite o Aenigmatite o Atacamite (Hemimorphite) o Coffinite o Erionite o Hematite o Aeschynite o Atokite o Calaverite o Columbite o Erythrite o Hemimorphite o Agardite-Y o Augite o Calciohilairite (Ferrocolumbite) o Euchroite o Hercynite o Agate (Quartz) o Aurostibite o Calcite, see also o Conichalcite o Euxenite o Hessite o Aguilarite o Austinite Manganocalcite o Connellite o Euxenite-Y o Heulandite o Aktashite o Onyx o Copiapite o o Autunite o Fairchildite Hexahydrite o Alabandite o Caledonite o Copper o o Awaruite o Famatinite Hibschite o Albite o Cancrinite o Copper-zinc o o Axinite group o Fayalite Hillebrandite o Algodonite o Carnelian (Quartz) o Coquandite o o Azurite o Feldspar group Hisingerite o Allanite o Cassiterite o Cordierite o o Barite o Ferberite Hongshiite o Allanite-Ce o Catapleiite o Corrensite o o Bastnäsite
    [Show full text]
  • Mineral Processing
    Mineral Processing Foundations of theory and practice of minerallurgy 1st English edition JAN DRZYMALA, C. Eng., Ph.D., D.Sc. Member of the Polish Mineral Processing Society Wroclaw University of Technology 2007 Translation: J. Drzymala, A. Swatek Reviewer: A. Luszczkiewicz Published as supplied by the author ©Copyright by Jan Drzymala, Wroclaw 2007 Computer typesetting: Danuta Szyszka Cover design: Danuta Szyszka Cover photo: Sebastian Bożek Oficyna Wydawnicza Politechniki Wrocławskiej Wybrzeze Wyspianskiego 27 50-370 Wroclaw Any part of this publication can be used in any form by any means provided that the usage is acknowledged by the citation: Drzymala, J., Mineral Processing, Foundations of theory and practice of minerallurgy, Oficyna Wydawnicza PWr., 2007, www.ig.pwr.wroc.pl/minproc ISBN 978-83-7493-362-9 Contents Introduction ....................................................................................................................9 Part I Introduction to mineral processing .....................................................................13 1. From the Big Bang to mineral processing................................................................14 1.1. The formation of matter ...................................................................................14 1.2. Elementary particles.........................................................................................16 1.3. Molecules .........................................................................................................18 1.4. Solids................................................................................................................19
    [Show full text]
  • Mineral to Metal: Processing of Titaniferous Ore to Synthetic Rutile (Tio2) and Ti Metal
    Mineral to Metal: Processing of Titaniferous Ore to Synthetic Rutile (TiO2) and Ti metal Dr Jeya Ephraim, Mineral to Metal May 11 – 13, 2015 * Hilton Birmingham Metropole Hotel * Birmingham, United Kingdom Objective To produce ultra pure high grade synthetic rutile (TiO2) from ilmenite ore and Ti metal from anatase or rutile Dr Jeya Ephraim, Mineral to Metal May 11 – 13, 2015 * Hilton Birmingham Metropole Hotel * Birmingham, United Kingdom Outline 1. Introduction 2. Why titaniferous minerals? 3. Processing Methods for synthetic rutile (TiO2) (i) Alkali Roasting (ii) Reduction followed by leaching 5. Results and discussion 6. Commercialisation 7. Conclusion 8. Bradford Metallurgy on Ti metal powder production 9. Future Plans Dr Jeya Ephraim, Mineral to Metal May 11 – 13, 2015 * Hilton Birmingham Metropole Hotel * Birmingham, United Kingdom Introduction • Titanium always exist as bonded to other elements in nature. • It is the ninth-most abundant element in the Earth. • It is widely distributed and occurs primarily in the minerals such as anatase, brookite, ilmenite, perovskite, rutile and titanite (sphene). • Among these minerals, only rutile and ilmenite have economic importance Dr Jeya Ephraim, Mineral to Metal May 11 – 13, 2015 * Hilton Birmingham Metropole Hotel * Birmingham, United Kingdom Ilmenite deposit in Chavara, Kerala, India Dr Jeya Ephraim, Mineral to Metal May 11 – 13, 2015 * Hilton Birmingham Metropole Hotel * Birmingham, United Kingdom Applications of TiO2 • White powder pigment - brightness and very high refractive index - Sunscreens use TiO2 - high refractive index - protect the skin from UV light. • TiO2 – photocatalysts - electrolytic splitting of water into hydrogen and oxygen, - produce electricity in nanoparticle form -light-emitting diodes, etc.
    [Show full text]
  • First Terrestrial Occurrence of Titanium
    875 Thz Caradian M fuc ralo g is t Vol.35, pp. 875-885(1997) FIRSTTERRESTRIAL OCCURRENCE OF TITANIUM.RICH PYRRHOTITE, MARCASITEAND PVRITEIN A FENITIZEDXENOLITH FROMTHE KHIBINA ALKALINE COMPLEX. RUSSIA ANDREI Y. BARKOVT nxp KAUKO V.O. LAAJOKI Irxtiruteof Geosciencesand Astrorcmy, University of Oula FIN-90570OuIW FinLand YT]RIP.MEN'SHIKOV Geological Instirute, Kola Science Cente, Russian Acadenry of Scimces, 14 Fersman Street, Apatity 1M200 , Russia TUOMO T. AI.APIETI Instituteof Geoscierrcesand Astrotnnry, University of Ouh+FN-90570 OuIu Finlnnl SEPPOJ. SryONEN Instiarcof ElcctronOptics, University of OuhaFN-90570 Ouh+ Finlnnd ABSTRACT The first terrestrial titanium-rich sulfides, the fust natural niobium-rich sulfide FeMgSe, fluorine-rich (ca. 6 wt.Vo D end-memberphlogopite (S().04 wLTo FeO) and ferroan alabandite occurlocally in aheterogeneous xenolit\ enclosed within nepheline syenite in the l(hifiaa alkalins gs6plex, Kola Peninsul4 northwestem Russia- This assemblage is exclusively associated with an alkali-feldspar-rich rock, probably fenite. Associat€d ninerals include corundum, Nb-Zr-bearing rutile and monazite. The maximum Ti content reaches 3.9 w.7o in pynhotite and 2 wt.7o in marcasite and pyrite, which represent prducts of replacement of the pynhotite. Titanium is distributed rather homogeneously within single grains of the pyrrhotite; however, a strong grain-to-gain variation is observed. The Tl-rich sulfides invariably contrin an elevated level ofvanadium (0.2-0 .4 wr.Vo).T\e results indicate that both Ti and V enter into solid solution in the sulfides. Presumably, there is an environmental similarity between the occurrences ofTl-bearing sulfides in trftibina and in meteorites (enstatite chondrites), where Tl-bearing hoilite occurs.
    [Show full text]
  • Cafetite, Ca[Ti2o5](H2O): Crystal Structure and Revision of Chemical Formula
    American Mineralogist, Volume 88, pages 424–429, 2003 Cafetite, Ca[Ti2O5](H2O): Crystal structure and revision of chemical formula SERGEY V. K RIVOVICHEV,1,* VICTOR N. YAKOVENCHUK,2 PETER C. BURNS,3 YAKOV A. PAKHOMOVSKY,2 AND YURY P. MENSHIKOV2 1Department of Crystallography, St. Petersburg State University, University Embankment 7/9, St. Petersburg 199034, Russia 2Geological Institute, Kola Science Centre, Russian Academy of Sciences, Fersmana 14, 184200-RU Apatity, Russia 3Department of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, Indiana 46556-0767, U.S.A. ABSTRACT The crystal structure of cafetite, ideally Ca[Ti2O5](H2O), (monoclinic, P21/n, a = 4.9436(15), b = 12.109(4), c = 15.911(5) Å, b = 98.937(5)∞, V = 940.9(5) Å3, Z = 8) has been solved by direct methods and refined to R1 = 0.057 using X-ray diffraction data collected from a crystal pseudo-merohedrally twinned on (001). There are four symmetrically independent Ti cations; each is octahedrally coordi- nated by six O atoms. The coordination polyhedra around the Ti cations are strongly distorted with individual Ti-O bond lengths ranging from 1.743 to 2.223 Å (the average <Ti-O> bond length is 1.98 Å). Two symmetrically independent Ca cations are coordinated by six and eight anions for Ca1 and Ca2, respectively. The structure is based on [Ti2O5] sheets of TiO6 octahedra parallel to (001). The Ca atoms and H2O groups are located between the sheets and link them into a three-dimensional struc- ture. The structural formula of cafetite confirmed by electron microprobe analysis is Ca[Ti2O5](H2O), .
    [Show full text]
  • Occurrence, Alteration Patterns and Compositional Variation of Perovskite in Kimberlites
    975 The Canadian Mineralogist Vol. 38, pp. 975-994 (2000) OCCURRENCE, ALTERATION PATTERNS AND COMPOSITIONAL VARIATION OF PEROVSKITE IN KIMBERLITES ANTON R. CHAKHMOURADIAN§ AND ROGER H. MITCHELL Department of Geology, Lakehead University, 955 Oliver Road, Thunder Bay, Ontario P7B 5E1, Canada ABSTRACT The present work summarizes a detailed investigation of perovskite from a representative collection of kimberlites, including samples from over forty localities worldwide. The most common modes of occurrence of perovskite in archetypal kimberlites are discrete crystals set in a serpentine–calcite mesostasis, and reaction-induced rims on earlier-crystallized oxide minerals (typically ferroan geikielite or magnesian ilmenite). Perovskite precipitates later than macrocrystal spinel (aluminous magnesian chromite), and nearly simultaneously with “reaction” Fe-rich spinel (sensu stricto), and groundmass spinels belonging to the magnesian ulvöspinel – magnetite series. In most cases, perovskite crystallization ceases prior to the resorption of groundmass spinels and formation of the atoll rim. During the final evolutionary stages, perovskite commonly becomes unstable and reacts with a CO2- rich fluid. Alteration of perovskite in kimberlites involves resorption, cation leaching and replacement by late-stage minerals, typically TiO2, ilmenite, titanite and calcite. Replacement reactions are believed to take place at temperatures below 350°C, 2+ P < 2 kbar, and over a wide range of a(Mg ) values. Perovskite from kimberlites approaches the ideal formula CaTiO3, and normally contains less than 7 mol.% of other end-members, primarily lueshite (NaNbO3), loparite (Na0.5Ce0.5TiO3), and CeFeO3. Evolutionary trends exhibited by perovskite from most localities are relatively insignificant and typically involve a decrease in REE and Th contents toward the rim (normal pattern of zonation).
    [Show full text]
  • Anorogenic Alkaline Granites from Northeastern Brazil: Major, Trace, and Rare Earth Elements in Magmatic and Metamorphic Biotite and Na-Ma®C Mineralsq
    Journal of Asian Earth Sciences 19 (2001) 375±397 www.elsevier.nl/locate/jseaes Anorogenic alkaline granites from northeastern Brazil: major, trace, and rare earth elements in magmatic and metamorphic biotite and Na-ma®c mineralsq J. Pla Cida,*, L.V.S. Nardia, H. ConceicËaÄob, B. Boninc aCurso de PoÂs-GraduacËaÄo em in GeocieÃncias UFRGS. Campus da Agronomia-Inst. de Geoc., Av. Bento GoncËalves, 9500, 91509-900 CEP RS Brazil bCPGG-PPPG/UFBA. Rua Caetano Moura, 123, Instituto de GeocieÃncias-UFBA, CEP- 40210-350, Salvador-BA Brazil cDepartement des Sciences de la Terre, Laboratoire de PeÂtrographie et Volcanologie-Universite Paris-Sud. Centre d'Orsay, Bat. 504, F-91504, Paris, France Accepted 29 August 2000 Abstract The anorogenic, alkaline silica-oversaturated Serra do Meio suite is located within the Riacho do Pontal fold belt, northeast Brazil. This suite, assumed to be Paleoproterozoic in age, encompasses metaluminous and peralkaline granites which have been deformed during the Neoproterozoic collisional event. Preserved late-magmatic to subsolidus amphiboles belong to the riebeckite±arfvedsonite and riebeckite± winchite solid solutions. Riebeckite±winchite is frequently rimmed by Ti±aegirine. Ti-aegirine cores are strongly enriched in Nb, Y, Hf, and REE, which signi®cantly decrease in concentrations towards the rims. REE patterns of Ti-aegirine are strikingly similar to Ti-pyroxenes from the IlõÂmaussaq peralkaline intrusion. Recrystallisation of mineral assemblages was associated with deformation although some original grains are still preserved. Magmatic annite was converted into magnetite and biotite with lower Fe/(Fe 1 Mg) ratios. Recrystallised amphibole is pure riebeckite. Magmatic Ti±Na-bearing pyroxene was converted to low-Ti aegirine 1 titanite ^ astrophyllite/aenigmatite.
    [Show full text]
  • Petrology of Nepheline Syenite Pegmatites in the Oslo Rift, Norway: Zr and Ti Mineral Assemblages in Miaskitic and Agpaitic Pegmatites in the Larvik Plutonic Complex
    MINERALOGIA, 44, No 3-4: 61-98, (2013) DOI: 10.2478/mipo-2013-0007 www.Mineralogia.pl MINERALOGICAL SOCIETY OF POLAND POLSKIE TOWARZYSTWO MINERALOGICZNE __________________________________________________________________________________________________________________________ Original paper Petrology of nepheline syenite pegmatites in the Oslo Rift, Norway: Zr and Ti mineral assemblages in miaskitic and agpaitic pegmatites in the Larvik Plutonic Complex Tom ANDERSEN1*, Muriel ERAMBERT1, Alf Olav LARSEN2, Rune S. SELBEKK3 1 Department of Geosciences, University of Oslo, PO Box 1047 Blindern, N-0316 Oslo Norway; e-mail: [email protected] 2 Statoil ASA, Hydroveien 67, N-3908 Porsgrunn, Norway 3 Natural History Museum, University of Oslo, Sars gate 1, N-0562 Oslo, Norway * Corresponding author Received: December, 2010 Received in revised form: May 15, 2012 Accepted: June 1, 2012 Available online: November 5, 2012 Abstract. Agpaitic nepheline syenites have complex, Na-Ca-Zr-Ti minerals as the main hosts for zirconium and titanium, rather than zircon and titanite, which are characteristic for miaskitic rocks. The transition from a miaskitic to an agpaitic crystallization regime in silica-undersaturated magma has traditionally been related to increasing peralkalinity of the magma, but halogen and water contents are also important parameters. The Larvik Plutonic Complex (LPC) in the Permian Oslo Rift, Norway consists of intrusions of hypersolvus monzonite (larvikite), nepheline monzonite (lardalite) and nepheline syenite. Pegmatites ranging in composition from miaskitic syenite with or without nepheline to mildly agpaitic nepheline syenite are the latest products of magmatic differentiation in the complex. The pegmatites can be grouped in (at least) four distinct suites from their magmatic Ti and Zr silicate mineral assemblages.
    [Show full text]
  • Chemical Composition and Petrogenetic Implications of Eudialyte-Group Mineral in the Peralkaline Lovozero Complex, Kola Peninsula, Russia
    minerals Article Chemical Composition and Petrogenetic Implications of Eudialyte-Group Mineral in the Peralkaline Lovozero Complex, Kola Peninsula, Russia Lia Kogarko 1,* and Troels F. D. Nielsen 2 1 Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, 119991 Moscow, Russia 2 Geological Survey of Denmark and Greenland, 1350 Copenhagen, Denmark; [email protected] * Correspondence: [email protected] Received: 23 September 2020; Accepted: 16 November 2020; Published: 20 November 2020 Abstract: Lovozero complex, the world’s largest layered peralkaline intrusive complex hosts gigantic deposits of Zr-, Hf-, Nb-, LREE-, and HREE-rich Eudialyte Group of Mineral (EGM). The petrographic relations of EGM change with time and advancing crystallization up from Phase II (differentiated complex) to Phase III (eudialyte complex). EGM is anhedral interstitial in all of Phase II which indicates that EGM nucleated late relative to the main rock-forming and liquidus minerals of Phase II. Saturation in remaining bulk melt with components needed for nucleation of EGM was reached after the crystallization about 85 vol. % of the intrusion. Early euhedral and idiomorphic EGM of Phase III crystalized in a large convective volume of melt together with other liquidus minerals and was affected by layering processes and formation of EGM ore. Consequently, a prerequisite for the formation of the ore deposit is saturation of the alkaline bulk magma with EGM. It follows that the potential for EGM ores in Lovozero is restricted to the parts of the complex that hosts cumulus EGM. Phase II with only anhedral and interstitial EGM is not promising for this type of ore.
    [Show full text]
  • Phase Relations in the Systems Titania and Titania--Boric Oxide
    This dissertation has been 65—9337 microfilmed exactly as received BEARD, William Clarence, 1934- PHASE RELATIONS IN THE SYSTEMS TITANIA AND TITANIA— BORIC OXIDE. The Ohio State University, Ph.D., 1965 M in eralogy University Microfilms, Inc., Ann Arbor, Michigan PHASE RELATIONS IN THE SYSTEMS TITANIA AND TITANIA—BORIC OXIDE DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of the Ohio State University by William Clarence Beard, B. S. The Ohio State University 1965 Approved by n Adviser Department of Mineralogy ACKNOWLEDGMENTS The author wishes to thank the people who have contributed to the preparation of this dissertation. First, to his adviser, Dr. Wilfrid Raymond Foster, for advice and suggestion of the problem; and second to other members of the faculty of the Department of Mineralogy, Drs. Henry Edward Wenden, Ernest George Ehlers, and Rodney Tampa Tettenhorst, for discussions of the problem and the reading of this dissertation, the author extends his thanks. Thanks also go to his colleague, William Charles Butterman, for assistance in the construction and main­ tenance of many pieces of experimental apparatus. Acknowledgment is made for financial support received under contract No. AF 33(616)-6509 (twenty-four months), spon­ sored by Aeronautical Research Division, Wright-Patterson Air Force Base, Ohio, as well as for a Mershon National Graduate Fellowship awarded (1962-63) by the Mershon Committee on Education in National Security; and a William J. McCaughey Fellowship (1963-64). The author is indebted to his wife, Ursula, for her constant help and encouragement. ii VITA.
    [Show full text]