207Pb-Excess in Carbonatitic Baddeleyite As the Result of Pa Scavenging from the Melt
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Baddeleyite Microstructures in Variably Shocked Martian Meteorites: an Opportunity to Link Shock Barometry and Robust Geochronology
51st Lunar and Planetary Science Conference (2020) 2302.pdf BADDELEYITE MICROSTRUCTURES IN VARIABLY SHOCKED MARTIAN METEORITES: AN OPPORTUNITY TO LINK SHOCK BAROMETRY AND ROBUST GEOCHRONOLOGY. L. G. Staddon1*, J. R. Darling1, N. R. Stephen2, J. Dunlop1, and K. T. Tait3,4. 1School of Environment, Geography and Geoscience, University of Portsmouth, UK; *[email protected], 2Plymouth Electron Microscopy Centre, Plymouth University, UK, 3Department of Earth Sciences, University of Toronto, Canada, 4Royal Ontario Museum, Toronto, Canada. Introduction: Baddeleyite (monoclinic ZrO2; m- [6]. Shergottites in which plagioclase has undergone ZrO2) has recently been shown to be capable of provid- complete transformation to maskelynite (S4), suggest- ing robust crystallisation ages for shergottites via in- ing shock pressures of at least ~29 GPa [6], are repre- situ U-Pb isotopic analyses [1,2]. However, in contrast sented by enriched shergottites NWA 8679 and NWA to experimental work [3], these studies also highlight 7257. Both samples are similarly evolved lithologies, that U-Pb isotope systematics of baddeleyite can be abundant in late stage phases such as Fe-Ti oxides, Cl- strongly modified by shock metamorphism. Up to apatite and Si- and K- rich mesostasis, though NWA ~80% radiogenic Pb loss was recorded within North- 7257 is doleritic [9,10]. Enriched basaltic shergottite west Africa (NWA) 5298 [1], with close correspond- NWA 5298 represents the most heavily shocked mar- ence of U-Pb isotopic ratios and baddeleyite micro- tian meteorite studied here (S6), containing both structures [4]. Combined microstructural analysis and maskelynite and vesicular plagioclase melt [4]. U-Pb geochronology of baddeleyite therefore offers Baddeleyite grains >2 µm in length were located tremendous potential to provide robust constraints on via a combination of automated backscattered electron crystallisation and impact ages for martian meteorites. -
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 -
The Stability of Lead Isotopes from Thorium
MAY 24, I9I7] NATURE ---------------------------------------------------------245 but I Prof. Stefan lYle:yer may be I .have pointed out the unsuitability of makmg some exammatwn of the radiations of the thonum mmerals for age determination or correlation material, and the results he obtains will therefore be and this is particularly so i.n the case of minerals of very great value in deciding this point. the Palreozoic igneous rocks of Langesundfjord, Nor FREDERICK SoDDY. way. Mr. Lawson and myself based our former con Aberdeen, May 14. that lead could not be the end product of thonum largely on analyses of these minerals. How . PRO.F. SoDDY. having given me the privilege of read e:ver, I have recalculated the ratiQs on the assump mg h1s letter m advance, I should like to take the twn that thonum has one-seventh the lead-producing opportunity of directing attention to the geological age power of uranium, and it is satisfactory to find that :>f the thorium minerals of Ceylon, and to a few further when thorium is less than five times a·s abundant statistics bearing on the suggestion that only 35 per uranium, the ratios agree as closely on th'ts calculation cent. of thorium produces a stable isotope of lead. as do the simple lead-ratios. When thorium is more than five times as abundant as uranium neither set I a!ll to my friend, Mr. E. J. Wayland, late of ratios gives any approach to agreement although of Ceylon, for the follow mg prov1s1onal classdicat10n (in order of age) of the the minerals from anv one locality agree am'ong them older rocks of the island :- selves. -
The Stability, Electronic Structure, and Optical Property of Tio2 Polymorphs
The stability, electronic structure, and optical property of TiO2 polymorphs Tong Zhu and Shang-Peng Gaoa) Department of Materials Science, Fudan University, Shanghai 200433, P. R. China Phonon density of states calculation shows that a new TiO2 polymorph with tridymite structure is mechanically stable. Enthalpies of 9 TiO2 polymorphs under different pressure are presented to study the relative stability of the TiO2 polymorphs. Band structures for the TiO2 polymorphs are calculated by density functional theory with generalized gradient approximation and the band energies at high symmetry k-points are corrected using the GW method to accurately determine the band gap. The differences between direct band gap energies and indirect band gap energies are very small for rutile, columbite and baddeleyite TiO2, indicating a quasi-direct band gap character. The band gap energies of baddeleyite (quasi-direct) and brookite (direct) TiO2 are close to that of anatase (indirect) TiO2. The band gap of the newly predicted tridymite-structured TiO2 is wider than the other 8 polymorphs. For optical response calculations, two-particle effects have been included by solving the Bethe-Salpeter equation for Coulomb correlated electron-hole pairs. TiO2 with cotunnite, pyrite, and fluorite structures have optical transitions in the visible light region. I. INTRODUCTION 1,2 Even after half a century of research, investigation of the fundamental properties of TiO2 crystal phases remains very important properly due to their important role to effectively utilize solar energy. For instance, 3 4 photocatalytic splitting of water into H2 and O2, photovoltaic generation of electricity, degradation of 5,6 7 environmentally hazard materials, and reduction of CO2 into hydrocarbon fuels. -
U-Pb (And U-Th) Dating of Micro-Baddeleyite
UU--PbPb (and(and UU--ThTh)) datingdating ofof micromicro--baddeleyitebaddeleyite 30 μm Axel K. Schmitt UCLA SIMS, NSF National Ion Microprobe Facility Collaborators:Collaborators: T.T. MaMarkrk HarrisonHarrison (UCLA)(UCLA) KevinKevin ChamberlainChamberlain (University(University ofof Wyoming)Wyoming) BaddeleyiteBaddeleyite (BAD(BAD--üü--LLĒĒ--iteite)*)* basicsbasics • chemical formula: ZrO2 • monoclinic (commonly twinned) • minor HfO2, TiO2, FeO, SiO2 • U between ~200 – 1000 ppm • low common Pb, Th/U <<0.2 • wide range of occurrences (terrestrial and extraterrestrial) • mafic and ultramafic rocks (basalt, gabbro, diabase) • alkali rocks (carbonatite, syenite) • mantle xenoliths (from kimberlites) • metacarbonates • impact-related rocks (tektites) Wingate and Compston, 2000 *National*National LibraryLibrary ServiceService forfor thethe BlindBlind andand PhysicallyPhysically HandicappeHandicappedd (NLS),(NLS), LibraryLibrary ofof CongressCongress BaddeleyiteBaddeleyite dating:dating: applicationsapplications andand examplesexamples BulkBulk analysisanalysis (TIMS)(TIMS) • Mafic dikes and layered intrusions (e.g., Heaman et al., 1992) • Detrital baddeleyite (e.g., Bodet and Schärer, 2000) InIn--situsitu methodsmethods (SIMS,(SIMS, LALA ICPICP MS,MS, EPMA)EPMA) • Mafic dikes and gabbros (e.g., Wingate et al., 1998; French et al., 2000) • SNC meteorites (Herd et al., 2007: 70±35 Ma and 171±35 Ma) MicroMicro--baddeleyitebaddeleyite analysis:analysis: inin--situsitu advantagesadvantages • Bulk analysis difficulties: • time-intensive, highly -
Constraints on the Formation of the Archean Siilinjärvi Carbonatite-Glimmerite Complex, Fennoscandian Shield
Constraints on the formation of the Archean Siilinjärvi carbonatite-glimmerite complex, Fennoscandian shield E. Heilimo1*, H. O’Brien2 and P. Heino3 1 Geological Survey of Finland, P.O. Box 1237, FI-70211, Kuopio, Finland (*correspondance: [email protected]) 2 Geological Survey of Finland, P.O. Box 96, FI-02151, Espoo, Finland. 3 Yara Suomi Oy, Siilinjärvi mine, P.O. Box FI-71801 Siilinjärvi, Finland. Abstract The Siilinjärvi carbonatite-glimmerite complex is the The main glimmerite-carbonatite intrusion within the Table 1 Siilinjärvi ore zone rocks, modal mineralogy, Genesis oldest carbonatite deposit currently mined for phos- Siilinjärvi complex occurs as a central tabular, up to 900 and calculated major element chemistry. The Siilinjärvi glimmerite-carbonatite complex prob- Ore1 Glimmerite Carbonatite apatite Carbonatite Lamprophyre phorous, and one of the oldest known on Earth at 2610 m wide, body of glimmerite and carbonatite running the containing apatite poor dike3 ably represents a plutonic complex formed as the result ± 4 Ma. The carbonatite-glimmerite is a 900 m wide length of the complex, surrounded by a fenite margin. Micas2 65 81.5 1.2 of passage of highly potassic magmas into and through Amphibole 5 4.5 0.6 0.2 and 14.5 km long tabular body of glimmerite with sub- Unlike many other carbonatite-bearing complexes that Calcite 15 1.6 61.2 86.8 a magma chamber, and the consequent accumulation ordinate carbonatite, surroundeed by fenites. The rocks contain a sequence of phlogopite-rich rocks intruded by Dolomite 4 0.9 13.4 10.6 of crystallizing minerals, a process that was active over Apatite 10 10.4 9.9 0.8 range from nearly pure glimmerite (tetraferriphlogo- a core of carbonatite (c.f., Kovdor, Phalaborwa), at Siil- Accessorices 1 0.7 0.1 0.4 the lifetime of the magma chamber. -
Stillwellite-(Ce) (Ce, La, Ca)Bsio
Stillwellite-(Ce) (Ce; La; Ca)BSiO5 c 2001 Mineral Data Publishing, version 1.2 ° Crystal Data: Hexagonal. Point Group: 3: As °at rhombohedral crystals, to 4 cm, and massive. Twinning: Observed about [100]. Physical Properties: Cleavage: One imperfect. Fracture: Conchoidal. Hardness = 6.5 D(meas.) = 4.57{4.60 D(calc.) = 4.67 » Optical Properties: Transparent to translucent. Color: Red-brown to pale pink; colorless in thin section. Streak: White. Optical Class: Uniaxial (+) to biaxial (+). ! = 1.765{1.784 ² = 1.780{1.787 2V(meas.) = 0±{6± Cell Data: Space Group: P 31: a = 6.841{6.844 c = 6.700{6.702 Z = 3 X-ray Powder Pattern: Mary Kathleen mine, Australia. 3.43 (s), 2.96 (s), 2.13 (ms), 4.44 (m), 1.864 (m), 2.71 (mw), 2.24 (mw) Chemistry: (1) (2) (1) (2) (1) (2) SiO2 22.40 22.06 La2O3 27.95 19.12 MgO 0.06 UO2 0.22 Ce2O3 33.15 30.82 CaO 0.95 0.34 ThO2 5.41 Pr2O3 1.82 F 0.30 + B2O3 12.23 [13.46] Nd2O3 5.36 H2O 0.85 Al2O3 0.42 Sm2O3 0.34 H2O¡ 0.10 Y2O3 0.74 0.28 Fe2O3 0.18 P2O5 0.67 Total [100.00] [99.26] (1) Mary Kathleen mine, Australia; recalculated to 100.00% after removal of very small amounts of uraninite and apatite determined by separate analysis. (2) Vico volcano, near Vetralla, Italy; by electron microprobe, B2O3 calculated from stoichiometry, original total given as 99.23%; corresponds to (Ce0:50La0:31Nd0:08Th0:05Pr0:03Ca0:02Sm0:01)§=1:00B1:02Si0:97O5: Occurrence: Locally abundant as a metasomatic replacement of metamorphosed calcareous sediments (Mary Kathleen mine, Australia); in alkalic pegmatites in syenite in an alkalic massif (Dara-i-Pioz massif, Tajikistan). -
And Zircon (Zrsio) from Anorthositic Rocks of the Laramie Anorthositecomplexo Wyoming: Petrologic Consequencesand U-Pb Ages
Ameican Mineralogist, Volume 80, pages I3I7-1327, 1995 Baddeleyite(ZrOr) and zircon (ZrSiO) from anorthositic rocks of the Laramie anorthositecomplexo Wyoming: Petrologic consequencesand U-Pb ages J.lvrns S. Scolrnsr* KrylN R. Cn*rnrRLArN Department of Geology and Geophysics,University of Wyoming, Laramie, Wyoming 82071, U.S.A. Ansrn-c.cr The Zr-bearing minerals baddeleyite (ZrOr) and zircon (ZrSiOo) occur within plagro- clase-rich (61-950/oplagioclase) cumulates of the Laramie anorthosite complex (LAC), southeasternWyoming. In each of the examined samples,zircon is present as relatively coarse(l-2 mm) interstitial grains, and baddeleyiteoccurs as small (0.05 mm) inclusions within cumulus plagioclase.Zircon crystallized betweencumulus plagioclasecrystals near solidus temperatures from highly fractionated, Zr-saturated liquids. The resultant shape ofzircon was controlled by the form ofthe remaining pore space.The origin ofbaddeleyite in the anorthositic rocks of the LAC is lesswell constrained.It may have crystallizedearly from the anorthositic parental magmas at relatively low silica activities; however, this would require baddeleyite saturation at extremely low Zr concentrations in the parental magmas(<< 100 ppm). Baddeleyite and zircon U-Pb agesreveal that several petrologically distinct intrusions were emplaced and crystallized in the LAC over a relatively restricted 1-3 m.y. interval aI ca. 1434 Ma. The 2o7Pb/2o6Pbages obtained for the baddeleyiteand zircon in eachsample are identical within error (+1-3 m.y.), and U concentrations are uniformly low (<240 ppm), supporting a genetically related origin for the minerals. Two anorthositic layered cumulates and a crosscutting, oxide-rich troctolite from the Poe Mountain anorthosite have crystallization agesthat are identical within error: 1434.4 + 0.6, 1434.5 + 0.6, and 1434.1 + 0.7 Ma, respectively. -
The U–Pb Zircon and Baddeleyite Ages of The
GFF ISSN: 1103-5897 (Print) 2000-0863 (Online) Journal homepage: http://www.tandfonline.com/loi/sgff20 The U–Pb zircon and baddeleyite ages of the Neoproterozoic Volyn Large Igneous Province: implication for the age of the magmatism and the nature of a crustal contaminant Leonid Shumlyanskyy, Anna Nosova, Kjell Billström, Ulf Söderlund, Per- Gunnar Andréasson & Oksana Kuzmenkova To cite this article: Leonid Shumlyanskyy, Anna Nosova, Kjell Billström, Ulf Söderlund, Per-Gunnar Andréasson & Oksana Kuzmenkova (2016) The U–Pb zircon and baddeleyite ages of the Neoproterozoic Volyn Large Igneous Province: implication for the age of the magmatism and the nature of a crustal contaminant, GFF, 138:1, 17-30, DOI: 10.1080/11035897.2015.1123289 To link to this article: http://dx.doi.org/10.1080/11035897.2015.1123289 Published online: 08 Jan 2016. Submit your article to this journal Article views: 27 View related articles View Crossmark data Citing articles: 1 View citing articles Full Terms & Conditions of access and use can be found at http://www.tandfonline.com/action/journalInformation?journalCode=sgff20 Download by: [Naturhistoriska Riksmuseum] Date: 01 April 2016, At: 05:03 GFF, 2016 Vol. 138, No. 1, 17–30, http://dx.doi.org/10.1080/11035897.2015.1123289 Article The U–Pb zircon and baddeleyite ages of the Neoproterozoic Volyn Large Igneous Province: implication for the age of the magmatism and the nature of a crustal contaminant LEONID SHUMLYANSKYY1, ANNA NOSOVA2, KJELL BILLSTRÖM3, ULF SÖDERLUND3,4, PER-GUNNAR ANDRÉASSON4 and OKSANA KUZMENKOVA5 Shumlyanskyy, L., Nosova, A., Billström K., Söderlund U., Andréasson, P.-G. & Kuzmenkova, O., 2016: The U-Pb zircon and baddeleyite ages of the Neoproterozoic Volyn Large Igneous Province: implication for the age of the magmatism and the nature of a crustal contaminant. -
Crystallographic Study of Uranium-Thorium Bearing Minerals in Tranomaro, South-East Madagascar
Journal of Minerals and Materials Characterization and Engineering, 2013, 1, 347-352 Published Online November 2013 (http://www.scirp.org/journal/jmmce) http://dx.doi.org/10.4236/jmmce.2013.16053 Crystallographic Study of Uranium-Thorium Bearing Minerals in Tranomaro, South-East Madagascar Frank Elliot Sahoa1, Naivo Rabesiranana1*, Raoelina Andriambololona1, Nicolas Finck2, Christian Marquardt2, Hörst Geckeis2 1Institut National des Sciences et Techniques Nucléaires (Madagascar-INSTN), Antananarivo, Madagascar 2Institute of Nuclear Waste and Disposal (INE), Karlsruhe Institute of Technology (KIT), Karlsruhe, Germany Email: *[email protected] Received September 20, 2013; revised October 21, 2013; accepted November 5, 2013 Copyright © 2013 Frank Elliot Sahoa et al. This is an open access article distributed under the Creative Commons Attribution Li- cense, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. ABSTRACT Studies are undertaken to characterize the uranium and thorium minerals of south-east Madagascar. Seven selected uranothorianite bearing pyroxenites samples from old abandoned uranium quarries in Tranomaro, south Amboasary, Madagascar (46˚28'00"E, 24˚36'00"S) have been collected. To determine the mineral micro-structure, they were inves- tigated for qualitative identification of crystalline compounds by using X-ray powder diffraction analytical method (XRD). Results showed that the uranium and thorium compounds, as minor elements, were present in various crystal- line structures. Thorium, as thorianite, is present in a simple ThO2 cubic crystalline system, whereas the uranium com- ponent of the Tranomaro uranothorianite samples is oxide-based and is a mixture of complex oxidation states and crys- talline systems. Generally called uraninite, its oxide compounds are present in more than eight phases. -
Baddeleyite Zro2 C 2001-2005 Mineral Data Publishing, Version 1 Crystal Data: Monoclinic
Baddeleyite ZrO2 c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Monoclinic. Point Group: 2/m. Crystals commonly tabular on {100} and somewhat elongated on [010], or short to long prismatic along [001], to 6 cm; rarely equant; prism faces striated k [001]; radially fibrous with concentric banding in botryoidal masses. Twinning: Ubiquitous; on {100} and {110}, both may be polysynthetic; rare on {201}. Physical Properties: Cleavage: {001} nearly perfect, {010} and {110} less perfect. Fracture: Subconchoidal to uneven. Tenacity: Brittle. Hardness = 6.5 D(meas.) = 5.40–6.02 D(calc.) = [5.83] Blue-green cathodoluminescence. Optical Properties: Transparent; in dark-colored specimens, only in thin fragments. Color: Colorless to yellow, green, greenish or reddish brown, brown, iron-black; colorless to brown in transmitted light. Streak: White to brownish white. Luster: Greasy to vitreous; nearly submetallic in black crystals. Optical Class: Biaxial (–). Pleochroism: X = yellow, reddish brown, oil-green; Y = oil-green, reddish brown; Z = brown, light brown. Orientation: X ∧ c =13◦; Y = b. Dispersion: r> v, rather strong. Absorption: X > Y > Z. α = 2.13(1) β = 2.19(1) γ = 2.20(1) 2V(meas.) = 30(1)◦ 2V(calc.) = 28◦ Cell Data: Space Group: P 21/c (synthetic). a = 5.1505(1) b = 5.2116(1) c = 5.3173(1) β =99.230(1)◦ Z=4 X-ray Powder Pattern: Phalaborwa, South Africa. 3.15 (10), 2.835 (9), 2.62 (5), 1.817 (5), 3.66 (4), 3.51 (4), 1.847 (4) Chemistry: (1) (2) (1) (2) (1) (2) SiO2 0.19 0.08 HfO2 0.93 CaO 0.06 TiO2 0.56 Fe2O3 0.82 LOI 0.28 ZrO2 98.90 97.8 FeO 1.3 Total 100.25 100.67 (1) Balangoda, Sri Lanka. -
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).