Petrography and Mineral Chemistry of Ultramafic and Related Inclusions from the Orapa A/K-1 Kimberlite Pipe, Botswana by Richard P

Total Page:16

File Type:pdf, Size:1020Kb

Petrography and Mineral Chemistry of Ultramafic and Related Inclusions from the Orapa A/K-1 Kimberlite Pipe, Botswana by Richard P PETROGRAPHY AND MINERAL CHEMISTRY OF ULTRAMAFIC AND RELATED INCLUSIONS FROM THE ORAPA A/K-1 KIMBERLITE PIPE, BOTSWANA BY RICHARD P. TOLLO '-- Lesotho (/) ~ Q,) Q,) -E 0 0 I{) 500 meters generalized cross-section of a kimberlite pipe modified after Hawthorne ( 197 5) CONTRIBUTION NO. 39 DEPARTMENT OF GEOLOGY AND GEOGRAPHY UNIVERSITY OF MASSACHUSETIS AMHERST, MASSACHUSETIS PETROGRAPHY AND MINERAL CHEMISTRY OF ULTRAMAFIC AND RELATED INCLUSIONS FROM THE ORAPA A/K-1 KIMBERLITE PIPE, BOTSWANA by RICHARD PAUL TOLLO Contribution No. 39 Department of GeoJogy and Geography University of Massachusetts Amherst, Massachusetts August, 1982 paAJaSaE S4q~lE TTV OtTOl tnad p~aqOJE TABLE OF CONTENTS ACKNOWLEDGEMENT xi ABSTRACT . xiii Chapter I. INTRODUCTION 1 The Orapa A/K-1 Kimberlite Pipe 1 Determinative Methods 3 II. OXIDE DISCRETE NODULES .. 6 Ilmenite . • • • • • . • • • 6 Rutile and Ilmenite-Rutile Intergrowths 33 III. SILICATE DISCRETE NODULES 65 Clinopyroxene • • • • 65 Ilmenite-Clinopyroxene Intergrowth 79 Garnet . 86 Knorringite Garnet-Clinopyroxene-Chromite Intergrowth • • • • • . • • . • . • • . • . 101 IV. ECLOGITE NODULES • 112 Introduction • • 112 Petrography 112 Phase Chemistry 121 Geothermometry and Geobarometry 150 V. DISCUSSION •.. 158 VI. SUMMARY A}ID CONCLUSIONS 177 REFERENCES 182 APPENDIX A: LISTING OF THE INDIVIDUAL ELECTRON MICROPROBE ANALYSES USED IN THE CONSTRUCTION OF FIGURE 7 196 APPENDIX B: SUMMARY OF THE EXPERIMENTAL CONDITIONS INVOLVED IN THE ILMENITE-RUTILE SYNTHESIS EXPERIMENTS . • • . 202 iii LIST OF TABLES Table lo Average chemical compositions of individual ilmenite discrete nodules from Orapa - nodule interiors 18 2o Chemical compositions of coexisting ilmenite and rutile in ilmenite-rutile intergrowth nodules from Orapa and Jagersfontein o o o o o 0 o o o o o • • o • • 0 42 3. Calculated bulk compositions for selected coarse lamellar ilmenite-rutile intergrowth nodules from Orapa and Jagersfontein 0 • o o o • • • • o o • 0 55 4. Comparison of X-ray diffraction data for niobian rutile discrete nodule 1/0R-406 from Orapa and "ilmenorutile" (JCPDS 1111-396) o • • • • • o • • o • • o • o • . • • 61 5. Chemical composition of niobian rutile discrete nodule 1/0R-406 from Orapa compared to lunar rutile o 63 6. Average chemical compositions of individual clino­ pyroxene discrete nodules from Orapa 0 0 • • 0 • 66 7o Average chemical compositions of coexisting clino­ pyroxene and ilmenite from Orapa nodule t/430B • • 82 8o Average chemical compositions of individual garnet discrete nodules from Orapa 0 o • 0 • • • • o 0 • 87 9. Average chemical compositions of coexisting garnet, clinopyroxene, and chromite from Orapa nodule 1/431 104 lOo Petrographic data for representative eclogite nodules from Orapa • • o • • o o • o o . • • 113 llo Average chemical compositions of garnet grains in individual eclogite nodules from Orapa o . o 122 12o Average chemical compositions of clinopyroxene grains in individual eclogite nodules from Orapa o o o 131 13. Average chemical compositions of rutile grains in individual eclogite nodules from Orapa • • • 0 • 143 14. Average chemical compositions of ilmenite grains in individual eclogite nodules from Orapa . • • 146 v Table 15. Representative analyses of individual amphibole grains in Orapa eclogite nodules #105 and #109 . • . • • • . 148 16. Comparative temperature estimates for garnet discrete nodules containing clinopyroxene inclusions from Orapa . 159 17. Comparative temperature estimates for ilmenite-bearing eclogites and ilmenite-clinopyroxene intergrowth nodule #430B from Orapa • • • • • • • • . • • • • • • • 162 18. Individual electron microprobe analyses of ilmenite discrete nodule #411A used in the construction of the chemical contour map presented in Figure 7 of the text . 198 19. Summary of experimental conditions for individual runs involved in the ilmenite-rutile intergrowth e-xperiments . 203 vi LIST OF ILLUSTRATIONS Figure 1. Generalized distribution of kimberlite clusters and major tectonic units in Botswana 2 2a. Typical inequigranular polycrystalline texture developed in the interior region of an ilmenite nodule . 9 2b. Well-developed, angular-polygonal polycrystalline texture viewed near the periphery of an ilmenite nodule . 9 2c. Polycrystalline texture developed at the periphery of an otherwise homogeneous ilmenite nodule . • ••• 11 2d. Prominent twinning lamellae oriented along probable crystallographically equivalent directions in an ilmenite grain at a nodule periphery • • . • • • 11 2e. Anisotropic shear fabric developed in the interior region of an otherwise homogeneous ilmenite nodule • 13 2f. Heavy surface pitting developed in the interior region of an ilmenite nodule • • • • • • . • • • . • • • • 13 3. Generalized sequence of events believed to result in the range of textural features observed in the ilmenite discrete nodule suite from Orapa 15 4a. Compositions of the ilmenite discrete nodule suite from Orapa plotted in the ternary system ilmenite­ geikielite-hematite • . • • . • • • . 22 4b. Compositions of homogeneous and completely poly­ crystalline discrete nodules plotted in the ternary system ilmenite-geikielite-hematite • . • •• 22 5. Plot of MgO and cr2o3 content for the ilmenite discrete nodule suite from Orapa . • • . • . • 24 6. Compositional variation along core-to-periphery microprobe traverses of three ilmenite discrete nodules • • • • . • • • . • • . • • . • . • . 26 vii Figure 7. Chemical contour map of the MgO content (~xpressed as weight percent) of ilmenite discrete nodule specimen ti411A • • • • • • • • • • • • . • • • 28 8. Plot of MgO versus FeO content for the ilmenite discrete nodule suite from Orapa • • • • . 31 9. Plot of Cr versus Ni for the ilmenite discrete nodule suite from Orapa • • • • • • • . 32 10. Generalized classification of ilmenite-rutile intergrowth textures • • • • • • • • • • . 35 lla. Typical lamellar-type ilmenite lamellae oriented along nearly orthogonal planes within the host rutile . 38 llb. Rim ilmenite situated along the nodule periphery and branching inward to form typical ilmenite lamellae characteristic of the lamellar type of ilmenite­ rutile intergrowth nodules at Orapa • . • • • 38 12. Compositions of rutiles from kimberlitic nodules, meteorites, lunar surface materials, and terres­ trial rocks plotted in terms of atomic percent Ti versus (Nb5++er3++Ta5+) • • • . • • • . 46 13. Compositions of niobian rutiles from kimberlitic nodules and various alkalic igneous rocks plotted in terms of atomic percent Nb-Fe-Ta • . • . • 47 14. Compositions of coarse lamellar, patchy, and atoll­ type ilmenite intergrowths within rutile plotted in the ternary system ilmenite-geikielite- hemati te . 49 15. Calculated average bulk composition of coarse l~ellar ilmenite-rutile nodules from Orapa and Jagersfontein plotted in the hypothetical armalcolite compositional space Ti4+-(Fe2++Mg2+)­ cr3+, assuming a ± 5 percent relative error inherent in the modal analyses • • • • • . • . 57 16. Summary of ilmenite-rutile experimental results plotted in terms of temperature and -log f02 . 59 viii Figure 17. Compositions of the clinopyroxene discrete nodule suite from Orapa plotted in the conventional pyroxene quadrilateral system diopside-enstatite­ ferrosilite-hedenbergite . • • • . • • • . • 70 18. Compositions of selected clinopyroxene discrete nodules from Orapa plotted in terms of the "Others" components VIriJ12Na-IVA1 • • • 72 19a. Compositions of the clinopyroxene discrete nodule suite from Orapa plotted as a function of chrome content versus Mg/(Mg+Fe) ratio ••••.••• 74 19b. Compositions of the clinopyroxene discrete nodule suite from Orapa plotted as a function of chrome content versus Ca/(Ca+Mg) ratio ••••..•• 74 19c. Compositions of the clinopyroxene discrete nodule suite from Orapa plotted as a function of chrome content versus Na20 • • • • • • • • • • • • • . 75 19d. Compositions of the clinopyroxene discrete nodule suite from Orapa plotted as a function of chrome content versus Al2D3 • • • . • • • • • • . 75 20. Detailed drawing of a polished section through Orapa nodule #430B comprised of ilmenite inter­ grown with clinopyroxene and polymineralic alteration products 80 21. Compositions of the garnet discrete nodule suite from Orapa plotted in terms of mole percent Ca-Mg-Fe • • . • • • • . • • . • . 94· 22. Compositions of the garnet discrete nodule suite from. Orapa plotted as function of chrome content versus Mg/(Mg+Fe) ratio . • • . • . • • . • • • • • . • 96 23. Plot of Mg/(Mg+Fe) ratio versus Ti02 content for the garnet discrete nodule suite from Orapa . 97 24. Detailed drawing of a thin section through Orapa nodule #431 comprised of green garnet intergrown with clinopyroxene and chrornite • • • . • . • 102 ix Figure 25. Summary plot of (CaO + MgO) content versus cr 2o3 content for kimberlitic green garnets, garnet inclusions in diamonds, garnets from peridotite xenoliths in kimberlite, and low-chrome garnet discrete nodules . • • . • . 107 26. Summary plot of garnet compositions taken from the literature for eclogitic inclusions in kimber- li tes • • • • • • . • • • . 129 27. Summary plot of clinopyroxene compositions taken from the literature for eclogitic inclusions in kimberli tes . • • • • . 138 28. Average compositions of garnets and clinopyroxenes coexisting in eclogite xenoliths from Orapa plotted in terms of Ca-Mg-Fe components . 140 29a. Compositions of garnet discrete nodules and garnets in eclogites from Orapa plotted in terms of MgO/(MgO+FeO) ratio and Cr203 content 141 29b. Compositions of clinopyroxene
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]
  • 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]
  • About Our Mineral World
    About Our Mineral World Compiled from series of Articles titled "TRIVIAL PURSUITS" from News Nuggets by Paul F. Hlava "The study of the natural sciences ought to expand the mind and enlarge the ability to grasp intellectual problems." Source?? "Mineral collecting can lead the interested and inquisitive person into the broader fields of geology and chemistry. This progression should be the proper outcome. Collecting for its own sake adds nothing to a person's understanding of the world about him. Learning to recognize minerals is only a beginning. The real satisfaction in mineralogy is in gaining knowledge of the ways in which minerals are formed in the earth, of the chemistry of the minerals and of the ways atoms are packed together to form crystals. Only by grouping minerals into definite categories is is possible to study, describe, and discuss them in a systematic and intelligent manner." Rock and Minerals, 1869, p. 260. Table of Contents: AGATE, JASPER, CHERT AND .............................................................................................................................2 GARNETS..................................................................................................................................................................2 GOLD.........................................................................................................................................................................3 "The Mystery of the Magnetic Dinosaur Bones" .......................................................................................................4
    [Show full text]
  • Nomenclature of the Garnet Supergroup
    American Mineralogist, Volume 98, pages 785–811, 2013 IMA REPORT Nomenclature of the garnet supergroup EDWARD S. GREW,1,* ANDREW J. LOCOCK,2 STUART J. MILLS,3,† IRINA O. GALUSKINA,4 EVGENY V. GALUSKIN,4 AND ULF HÅLENIUS5 1School of Earth and Climate Sciences, University of Maine, Orono, Maine 04469, U.S.A. 2Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta T6G 2E3, Canada 3Geosciences, Museum Victoria, GPO Box 666, Melbourne 3001, Victoria, Australia 4Faculty of Earth Sciences, Department of Geochemistry, Mineralogy and Petrography, University of Silesia, Będzińska 60, 41-200 Sosnowiec, Poland 5Swedish Museum of Natural History, Department of Mineralogy, P.O. Box 50 007, 104 05 Stockholm, Sweden ABSTRACT The garnet supergroup includes all minerals isostructural with garnet regardless of what elements occupy the four atomic sites, i.e., the supergroup includes several chemical classes. There are pres- ently 32 approved species, with an additional 5 possible species needing further study to be approved. The general formula for the garnet supergroup minerals is {X3}[Y2](Z3)ϕ12, where X, Y, and Z refer to dodecahedral, octahedral, and tetrahedral sites, respectively, and ϕ is O, OH, or F. Most garnets are cubic, space group Ia3d (no. 230), but two OH-bearing species (henritermierite and holtstamite) have tetragonal symmetry, space group, I41/acd (no. 142), and their X, Z, and ϕ sites are split into more symmetrically unique atomic positions. Total charge at the Z site and symmetry are criteria for distinguishing groups, whereas the dominant-constituent and dominant-valency rules are critical in identifying species. Twenty-nine species belong to one of five groups: the tetragonal henritermierite group and the isometric bitikleite, schorlomite, garnet, and berzeliite groups with a total charge at Z of 8 (silicate), 9 (oxide), 10 (silicate), 12 (silicate), and 15 (vanadate, arsenate), respectively.
    [Show full text]
  • Garnets from the Camafuca-Camazambo Kimberlite (Angola)
    Anais da Academia Brasileira de Ciências (2006) 78(2): 309-315 (Annals of the Brazilian Academy of Sciences) ISSN 0001-3765 www.scielo.br/aabc Garnets from the Camafuca-Camazambo kimberlite (Angola) EUGÉNIO A. CORREIA and FERNANDO A.T.P. LAIGINHAS Departamento de Geologia, Faculdade de Ciências da Universidade do Porto Praça de Gomes Teixeira, 4050 Porto, Portugal Manuscript received on November 17, 2004; accepted for publication on June 13, 2005; presented by ALCIDES N. SIAL ABSTRACT This work presents a geochemical study of a set of garnets, selected by their colors, from the Camafuca- Camazambo kimberlite, located on northeast Angola. Mantle-derived garnets were classified according to the scheme proposed by Grütter et al. (2004) and belong to the G1, G4, G9 and G10 groups. Both sub-calcic (G10) and Ca-saturated (G9) garnets, typical, respectively, of harzburgites and lherzolites, were identified. The solubility limit of knorringite molecule in G10D garnets suggests they have crystallized at a minimum pressure of about 40 to 45 kbar (4– 4.5 GPa). The occurrence of diamond stability field garnets (G10D) is a clear indicator of the potential of this kimberlite for diamond. The chemistry of the garnets suggests that the source for the kimberlite was a lherzolite that has suffered a partial melting that formed basaltic magma, leaving a harzburgite as a residue. Key words: kimberlite, diamond, garnet, lherzolite, harzburgite. INTRODUCTION GEOCHEMICAL STUDY OF GARNETS The Camafuca-Camazambo kimberlite belongs to The geochemical study of mantle-derived garnets a kimberlite province comprising over a dozen of occurring in kimberlites progressed remarkably in primary occurrences of diamond, located along- recent years, as their chemistry is not only a possible side the homonymous brook which is a tributary of indicator of the presence of diamonds in their host the Chicapa river, in the proximity of the Calonda rock but also their abundance is a likely indicator of village, northeast Angola (Fig.
    [Show full text]
  • Partitioning of Chromium Between Garnet and Clinopyroxene: first-Principle Modelling Versus Metamorphic Assemblages
    Eur. J. Mineral., 32, 387–403, 2020 https://doi.org/10.5194/ejm-32-387-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Partitioning of chromium between garnet and clinopyroxene: first-principle modelling versus metamorphic assemblages Sarah Figowy, Benoît Dubacq, Yves Noël, and Philippe d’Arco Sorbonne Université, CNRS-INSU, Institut des Sciences de la Terre de Paris, ISTeP UMR 7193, 75005 Paris, France Correspondence: Sarah Figowy (sarah.fi[email protected]) Received: 30 December 2019 – Revised: 28 May 2020 – Accepted: 15 June 2020 – Published: 3 July 2020 Abstract. Understanding the geochemical behaviour of trace and minor elements in mineral assemblages is of primary importance to study small- and large-scale geological processes. Partition coefficients are frequently used to model the chemical evolution of minerals and fluids during melting and in metamorphic rocks of all grades. However, kinetic effects hampering equilibrium partitioning may invalidate the modelling. This study aims at calculating partition coefficients and testing their applicability in natural mineral assemblages, choosing Cr in garnet and clinopyroxene via exchange with Al as a case study. First-principle modelling has been com- bined with measurements and element mapping to estimate partition coefficients for Cr and the deviation from equilibrium. Results highlight the role of crystal chemistry over the strain field around point defects, controlling the dynamics of the Cr3C D Al3C exchange between clinopyroxene and garnet. Ab initio calculations allowed estimation of Cr partition coefficients between garnet and clinopyroxene, using a thermodynamic approach based on endmembers and mixing models simplified for trace element behaviour.
    [Show full text]
  • Properties of Minerals for Processing
    2 C h a p t e r Properties of Minerals for Processing 2.1 SAMPLING Sampling is a process of obtaining a small portion from a large quantity of a similar material such that, it truly represents the composition of the whole lot. It is an important step before testing of any material in the laboratory. Sampling of homogeneous materials is easy as compared to heterogeneous materials and hence, has to be conducted carefully. It is so because unlike heterogeneous materials, homogeneous materials have a uniform composition. However, almost all metallurgical materials are heterogeneous in nature. 2.1.1 Sampling of Ores/Minerals The process of sampling is complicated because of the following reasons: (1) A large variety of constituents are present in ores and minerals. (2) There is a large variation in the distribution of these constituents throughout the material. (3) In many cases, weight of the sample may vary from, 0.5 to 5 gm or 10 gm. Small fraction from large quantity like 50 to 250 tonnes are not true representative of the entire lot. The size of the sample required for testing depends on the method of testing and the testing machine which is used. However, sampling may involve three operations, namely, crushing and/or grinding, mixing and finally cutting. These operations may be executed repeatedly wherein the quantity of sample can be reduced to a desired weight. Sampling should be based on the relation between maximum particle size and the amount of sample. The size of ore/mineral particles taken for sampling depends on uniformity of composition, i.e., if the composition is more uniform, smaller particle size of the sample is taken and vice versa.
    [Show full text]
  • Geikielite from the Naataniemi Serpentinite Massif, Kuhmo
    32'7 The Canadian M ine ralo gist Vol. 32, pp. 327-332 (1994) GEIKIELITEFROM THE NAATANIEMI SERPENTINITE MASSIF, KUHMOGREENSTONE BELT, FINLAND ruSSI P. LIPO, JOUNI I. WOLLO, VESA M. NYL{NEN ANDTALINO A. PIIRAINEN Departmentof Geology,University of Oulu,SF-90570 Oulu 57, Finland Arsrtecr Geikielite has only occasionallybeen reponed as an accessoryphase in metamorphosed,hydrothermally altered mafic and ultramafic rocks. This paperrepons a new occurence,in serpentiniteof the Niin$iniemimassif, in the Kuhmo greenstonebelt, easternFinland. Electron-microprobeanalyses show that its compositionranges from IlmroHem2GeiusPyhtrto Ilm2aGeir6Pyhto.The geikielitein theserocks is richerin Mn thanthat previously reported in serpentinizedultramafic rocks. Keywords:geikielite, serpentinite,Niiiitiiniemi, Kuhmo greenstonebelt, Finland. SoMMARS Il est assezrare de rencontrerla geikielite commephase accessoire dans les rochesmafiques et ultramafiquesqui ont subi des effets mdtamorphiqueset m6tasomatiques.Nous en d&rivons un exemple,d'une serpentinitedu massif de Niiiitiiniemi, dansla ceinturede rochesvertes de Kuhmo, dansla partie orientalede la Finlande.l,es analysesi la microsondedlectronique montrentque sa compositionvarie de llm2sFlem2Gei66Pyh,si Ilm2aGei56Pyh26. La geikielite dans ces roches est enrichieen Mn comparativementaux compositionsdocumentdes antdrieurement dans les rochesultramafiques serpentinis6es. (Traduit par la R6daction) Mots-cl6s: geikielite, serpentinite, Ndiitiiniemi, ceinture de roches vertes de Kuhmo, Finlande INTRoDUCTIoN Geikielite
    [Show full text]
  • Standard X-Ray Diffraction Powder Patterns
    NBS MONOGRAPH 25—SECTION 4 Standard X-ray Diffraction Powder Patterns U.S. DEPARTMENT OF COMMERCE NATIONAL BUREAU OF STANDARDS THE NATIONAL BUREAU OF STANDARDS The National Bureau of Standards is a principal focal point in the Federal Government for assuring maximum application of the physical and engineering sciences to the advancement of technology in industry and commerce. Its responsibilities include development and mainte- nance of the national standards of measurement, and the provisions of means for making measurements consistent with those standards; determination of physical constants and properties of materials; development of methods for testing materials, mechanisms, and structures, and making such tests as may be necessary, particularly for government agencies; cooperation in the establishment of standard practices for incorporation in codes and specifi- cations advisory service to government agencies on scientific and technical problems ; invention ; and development of devices to serve special needs of the Government; assistance to industry, business, and consumers m the development and acceptance of commercial standards and simplified trade practice recommendations; administration of programs in cooperation with United States business groups and standards organizations for the development of international standards of practice; and maintenance of a clearinghouse for the collection and dissemination of scientific, technical, and engineering information. The scope of the Bureau's activities is suggested in the following listing of its three Institutes and their organizatonal units. Institute for Basic Standards. Applied Mathematics. Electricity. Metrology. Mechanics. Heat. Atomic Physics. Physical Chemistry. Laboratory Astrophysics.* Radiation Phys- ics. Radio Standards Laboratory:* Radio Standards Physics; Radio Standards Engineering. Office of Standard Reference Data. Institute for Materials Research.
    [Show full text]
  • Titanite-Bearing Calc-Silicate Rocks Constrain Timing, Duration And
    *Revised Manuscript with No changes marked Click here to download Revised Manuscript with No changes marked: Rapa et al_MAIN MS.docx 1 TITANITE-BEARING CALC-SILICATE ROCKS CONSTRAIN TIMING, DURATION AND 2 MAGNITUDE OF METAMORPHIC CO2 DEGASSING IN THE HIMALAYAN BELT 3 4 Giulia Rapaa, Chiara Groppoa,b,*, Franco Rolfoa,b, Maurizio Petrellic, Pietro Moscab, 5 Diego Peruginic 6 7 8 9 aDepartment of Earth Sciences, University of Torino, Via Valperga Caluso 35, 10125 Torino, Italy 10 bIGG-CNR, Via Valperga Caluso 35, 10125 Torino, Italy 11 cDepartment of Physics and Geology, University of Perugia, Piazza Università, 06100 Perugia, Italy 12 13 *Corresponding Author 14 Chiara Groppo 15 Dept. of Earth Sciences, University of Torino 16 Via Valperga Caluso, 35 – 10125 Torino, Italy 17 Tel. +39 0116705106 18 Fax +39 0116705128 19 1 20 Abstract 21 The pressure, temperature, and timing (P-T-t) conditions at which CO2 was produced during the 22 Himalayan prograde metamorphism have been constrained, focusing on the most abundant calc- 23 silicate rock type in the Himalaya. A detailed petrological modelling of a clinopyroxene + scapolite 24 + K-feldspar + plagioclase + quartz ± calcite calc-silicate rock allowed the identification and full 25 characterization - for the first time – of different metamorphic reactions leading to the 26 simultaneous growth of titanite and CO2 production. The results of thermometric determinations 27 (Zr-in-Ttn thermometry) and U-Pb geochronological analyses suggest that, in the studied lithology, 28 most titanite grains grew during two nearly consecutive episodes of titanite formation: a near- 29 peak event at 730-740°C, 10 kbar, 30-26 Ma, and a peak event at 740-765°C, 10.5 kbar, 25-20 Ma.
    [Show full text]
  • A Specific Gravity Index for Minerats
    A SPECIFICGRAVITY INDEX FOR MINERATS c. A. MURSKyI ern R. M. THOMPSON, Un'fuersityof Bri.ti,sh Col,umb,in,Voncouver, Canad,a This work was undertaken in order to provide a practical, and as far as possible,a complete list of specific gravities of minerals. An accurate speciflc cravity determination can usually be made quickly and this information when combined with other physical properties commonly leads to rapid mineral identification. Early complete but now outdated specific gravity lists are those of Miers given in his mineralogy textbook (1902),and Spencer(M,i,n. Mag.,2!, pp. 382-865,I}ZZ). A more recent list by Hurlbut (Dana's Manuatr of M,i,neral,ogy,LgE2) is incomplete and others are limited to rock forming minerals,Trdger (Tabel,l,enntr-optischen Best'i,mmungd,er geste,i,nsb.ildend,en M,ineral,e, 1952) and Morey (Encycto- ped,iaof Cherni,cal,Technol,ogy, Vol. 12, 19b4). In his mineral identification tables, smith (rd,entifi,cati,onand. qual,itatioe cherai,cal,anal,ys'i,s of mineral,s,second edition, New york, 19bB) groups minerals on the basis of specificgravity but in each of the twelve groups the minerals are listed in order of decreasinghardness. The present work should not be regarded as an index of all known minerals as the specificgravities of many minerals are unknown or known only approximately and are omitted from the current list. The list, in order of increasing specific gravity, includes all minerals without regard to other physical properties or to chemical composition. The designation I or II after the name indicates that the mineral falls in the classesof minerals describedin Dana Systemof M'ineralogyEdition 7, volume I (Native elements, sulphides, oxides, etc.) or II (Halides, carbonates, etc.) (L944 and 1951).
    [Show full text]
  • Thermodynamic Modelling of Cr-Bearing Garnets with Implications for Diamond Inclusions and Peridotite Xenoliths
    Lithos 112S (2009) 986–991 Contents lists available at ScienceDirect Lithos journal homepage: www.elsevier.com/locate/lithos Thermodynamic modelling of Cr-bearing garnets with implications for diamond inclusions and peridotite xenoliths S. Klemme a,⁎, T.J. Ivanic b,e, J.A.D. Connolly d, B. Harte b,c a Institut für Mineralogie, Corrensstr. 24, Universität Münster, 48149 Münster, Germany b School of GeoSciences, King's Buildings, West Mains Road, University of Edinburgh, Edinburgh EH9 3JW, United Kingdom c Centre for Science at Extreme Conditions, University of Edinburgh, Erskine Williamson Building, Mayfield Road, Edinburgh EH9 3JZ, United Kingdom d Institut für Mineralogie und Petrographie, ETH Zentrum, Sonneggstrasse 5, CH-8082, Zürich, Switzerland e Geological Survey of Western Australia, Mineral House, 100 Plain Street, East Perth, WA 6004, Australia article info abstract Article history: A new approach is presented for modelling Cr-rich peridotite compositions and garnet–spinel compositions Received 8 September 2008 found in diamonds and xenoliths at conditions relevant to the deep continental Earth. Using recent Accepted 10 May 2009 experimental data, it is now possible to calculate phase relations and mineral compositions relevant to Available online 6 June 2009 pressures, temperatures, and compositions of the deep lithospheric Earth using free energy minimization techniques. Here we present calculated phase relations in Cr-rich mantle compositions from pressures of 20– Keywords: 60 kbar, and temperatures 800–1400 °C. The model is successful at modelling a wide range of natural mineral Garnet–spinel transition Peridotite compositions which are found as xenoliths in diamond-bearing kimberlites from South Africa, and is Diamond inclusion illustrated using suites of Cr-rich xenoliths from near Kimberley, South Africa.
    [Show full text]