A Pressure-Temperature Phase Diagram for Zircon at Extreme Conditions
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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. -
Coesite Inclusions: Microbarometers in Diamond
Coesite Inclusions: Microbarometers in Diamond Ren Lu GIA Laboratory, New York Mineral inclusions in diamond provide valuable information for decoding their thermobarometric, mechanical, and mineralogical conditions during and after diamond formation deep within the earth’s mantle. Coesite, a polymorph of silica (SiO2), shares the same chemical composition as quartz but has a different crystal structure and a higher Mohs hardness Anthony et al., 1990). Coesite forms at pressures greater than 2 GPa (i.e., 20,000 times atmospheric pressure). It has been found in high-impact meteorite craters and as inclusions in minerals and diamonds in ecologites in ultrahigh-pressure metamorphic terrains (Sobolev et al., 1999). Mineral inclusions in diamonds record the physical and chemical history of diamond formation; consequently, they provide a window to processes occurring in the deep interior of the mantle. Microscopic Raman spectroscopy is a very effective “fingerprint” technique for identifying unknown materials such as inclusions in gems, because Raman spectral features closely correlate to the crystal structure and chemistry of a material. Furthermore, this technique is nondestructive and requires virtually no sample preparation. We recently examined a suite of high-quality pink diamonds set in a bracelet. These stones were type Ia and exhibited gemological and spectral characteristics typical of the rarest group of high-quality Argyle pink diamonds (refer to table 2 in Shigley et al., 2001). A cluster of mineral inclusions were present in a 0.21 ct marquise in the intense to vivid purple-pink color range (figure 1). Raman spectra were collected with a Renishaw inVia confocal Raman system interfaced with 488, 514, 633, and 830 nm laser excitations. -
Volcanic-Derived Placers As a Potential Resource of Rare Earth Elements: the Aksu Diamas Case Study, Turkey
minerals Article Volcanic-Derived Placers as a Potential Resource of Rare Earth Elements: The Aksu Diamas Case Study, Turkey Eimear Deady 1,*, Alicja Lacinska 2, Kathryn M. Goodenough 1, Richard A. Shaw 2 and Nick M. W. Roberts 3 1 The Lyell Centre, British Geological Survey, Research Avenue South, Edinburgh EH14 4AP, UK; [email protected] 2 Environmental Science Centre, British Geological Survey, Nicker Hill, Keyworth NG12 5GG, UK; [email protected] (A.L.); [email protected] (R.A.S.) 3 Environmental Science Centre, NERC Isotope Geosciences Laboratory, Nicker Hill, Keyworth NG12 5GG, UK; [email protected] * Correspondence: [email protected]; Tel.: +44-(0)131-6500217 Received: 15 February 2019; Accepted: 26 March 2019; Published: 30 March 2019 Abstract: Rare earth elements (REE) are essential raw materials used in modern technology. Current production of REE is dominated by hard-rock mining, particularly in China, which typically requires high energy input. In order to expand the resource base of the REE, it is important to determine what alternative sources exist. REE placers have been known for many years, and require less energy than mining of hard rock, but the REE ore minerals are typically derived from eroded granitic rocks and are commonly radioactive. Other types of REE placers, such as those derived from volcanic activity, are rare. The Aksu Diamas heavy mineral placer in Turkey has been assessed for potential REE extraction as a by-product of magnetite production, but its genesis was not previously well understood. REE at Aksu Diamas are hosted in an array of mineral phases, including apatite, chevkinite group minerals (CGM), monazite, allanite and britholite, which are concentrated in lenses and channels in unconsolidated Quaternary sands. -
Revision 1 Extreme Fractionation from Zircon to Hafnon in the Koktokay No
This is a preprint, the final version is subject to change, of the American Mineralogist (MSA) Cite as Authors (Year) Title. American Mineralogist, in press. (DOI will not work until issue is live.) DOI: http://dx.doi.org/10.2138/am.2013.4494 6/19 1 Revision 1 2 3 Extreme fractionation from zircon to hafnon in the Koktokay No. 4 1 granitic pegmatite, Altai, northwestern China 5 6 Rong Yin1, Ru Cheng Wang1,*, Ai-Cheng Zhang1, Huan Hu1, Jin Chu Zhu1, Can Rao2, and 7 Hui Zhang3 8 9 1State Key Laboratory for Mineral Deposits Research, School of Earth Sciences and 10 Engineering, Nanjing University, Nanjing 210093, China; 11 2Department of Earth Sciences, Zhejiang University, Hangzhou 310027, China; 12 3Institute of Geochemistry, Chinese Academy of Sciences, Guiyang, 550002, China. 13 14 *E-mail: [email protected] 15 Always consult and cite the final, published document. See http://www.minsocam.org or GeoscienceWorld This is a preprint, the final version is subject to change, of the American Mineralogist (MSA) Cite as Authors (Year) Title. American Mineralogist, in press. (DOI will not work until issue is live.) DOI: http://dx.doi.org/10.2138/am.2013.4494 6/19 16 ABSTRACT 17 The Koktokay No. 1 pegmatite is a Li–Cs–Ta-rich granitic pegmatite located in Altai, 18 northwestern China. Zircon is present in most textural zones of this pegmatite and in its 19 contact zone with surrounding metagabbro. Here we describe the detailed associations of 20 zircon with other minerals, and the internal textures and chemistry of the zircons. -
Relict Zircon Inclusions in Muong Nong-Type Australasain Tektites: Implications Regarding the Location of the Source Crater
Lunar and Planetary Science XXXI 1196.pdf RELICT ZIRCON INCLUSIONS IN MUONG NONG-TYPE AUSTRALASAIN TEKTITES: IMPLICATIONS REGARDING THE LOCATION OF THE SOURCE CRATER. B. P. Glass, Geology Department, University of Delaware, Newark, DE 19716, USA ([email protected]) Introduction: Over the last thirty years we Australasian tektite samples from which we have have recovered crystalline inclusions from ap- identified inclusions; however, not all of the recov- proximately forty Muong Nong-type tektites from ered inclusions have been identified by XRD. the Australasian tektite strewn field in order to Based on appearance, the percent of inclusion- learn more about the nature of the parent material bearing specimens containing zircon is probably and the formation process [e.g., 1, 2]. More re- 100% or very close to it. Nearly all the zircons cently we have used geographic variations in con- are opaque white and their X-ray patterns show centration (number/gm) of crystalline inclusions to extreme X-ray asterism. However, of the 28 zir- indicate the possible location of the source crater cons identified by X-ray diffraction, only two [3]. The purpose of this abstract is to summarize (both from the same specimen whose place of ori- all the presently available data regarding relict gin is unknown) produced X-ray diffraction pat- zircon inclusions recovered from Australasian terns indicating that baddeleyite may be present. Muong Nong-type tektites and to discuss implica- The X-ray patterns from these two grains con- tions regarding the possible location of the source tained the two strongest lines for baddeleyite and crater which has still not been found. -
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 -
Phase Decomposition Upon Alteration of Radiation-Damaged Monazite–(Ce) from Moss, Østfold, Norway
MINERALOGY CHIMIA 2010, 64, No. 10 705 doi:10.2533/chimia.2010.705 Chimia 64 (2010) 705–711 © Schweizerische Chemische Gesellschaft Phase Decomposition upon Alteration of Radiation-Damaged Monazite–(Ce) from Moss, Østfold, Norway Lutz Nasdala*a, Katja Ruschela, Dieter Rhedeb, Richard Wirthb, Ljuba Kerschhofer-Wallnerc, Allen K. Kennedyd, Peter D. Kinnye, Friedrich Fingerf, and Nora Groschopfg Abstract: The internal textures of crystals of moderately radiation-damaged monazite–(Ce) from Moss, Norway, indicate heavy, secondary chemical alteration. In fact, the cm-sized specimens are no longer mono-mineral monazite but rather a composite consisting of monazite–(Ce) and apatite pervaded by several generations of fractures filled with sulphides and a phase rich in Th, Y, and Si. This composite is virtually a ‘pseudomorph’ after primary euhedral monazite crystals whose faces are still well preserved. The chemical alteration has resulted in major reworking and decomposition of the primary crystals, with potentially uncontrolled elemental changes, including extensive release of Th from the primary monazite and local redeposition of radionuclides in fracture fillings. This seems to question the general alteration-resistance of orthophosphate phases in a low-temperature, ‘wet’ environment, and hence their suitability as potential host ceramics for the long-term immobilisation of ra- dioactive waste. Keywords: Chemical alteration · Monazite–(Ce) · Radiation damage · Thorium silicate 1. Introduction eventually to the formation of a non-crys- to undergo chemical alteration, and its in- talline form.[1,2] Such normally crystalline, crease with cumulative radiation damage, The accumulation of structural damage irradiation-amorphised minerals are com- ii) how exactly chemical alteration proc- generated by the corpuscular self-irra- monly described by the term ‘metamict’.[3] esses take place, and iii) as to which de- diation of minerals containing actinide The metamictisation process is controlled gree these materials (i.e. -
Raman Spectroscopic Study of Variably Recrystallized Metamict Zircon from Amphibolite-Facies Metagranites, Serbo-Macedonian Massif, Bulgaria
1357 The Canadian Mineralogist Vol. 44, pp. 1357-1366 (2006) RAMAN SPECTROSCOPIC STUDY OF VARIABLY RECRYSTALLIZED METAMICT ZIRCON FROM AMPHIBOLITE-FACIES METAGRANITES, SERBO-MACEDONIAN MASSIF, BULGARIA ROSITSA TITORENKOVA§ Central Laboratory of Mineralogy and Crystallography, Bulgarian Academy of Sciences, Acad. G. Bonchev Street 107, 1113 Sofi a, Bulgaria BORIANA MIHAILOVA Mineralogisch-Petrographisches Institut, University of Hamburg, Grindelallee 48, D–20146 Hamburg. Germany LUDMIL KONSTANTINOV Central Laboratory of Mineralogy and Crystallography, Bulgarian Academy of Sciences, Acad. G. Bonchev Street 107, 1113 Sofi a, Bulgaria ABSTRACT We investigated zircon from high-grade metagranites of the Serbo-Macedonian Massif, in Bulgaria, by cathodoluminescence (CL), back-scattered-electron imaging, electron-microprobe analysis, and Raman microspectroscopy. The structural state in various zones was assessed using: (i) the position and width of the Raman peak near 1008 cm–1, (ii) the relative Raman intensity –1 of the symmetrical and anti-symmetrical SiO4 modes, (iii) the width of the peaks near 357 and 439 cm , and (iv) the occurrence of extra Raman scattering near 162, 509, 635 and 785 cm–1. The analyzed zones are divided into two main groups: (A) areas with a well-resolved Raman peak near 1008 cm–1, and (B) areas with a very weak Raman scattering near 1008 cm–1. Group B can be classifi ed into two subgroups: (B-i) dark zones in CL images, with a high concentration of uranium (up to 7000 ppm), and (B-ii) outermost bright zones in CL images with a concentration of U lower than that in the inner areas and commonly below the detection limit. -
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. -
Thirty-Fourth List of New Mineral Names
MINERALOGICAL MAGAZINE, DECEMBER 1986, VOL. 50, PP. 741-61 Thirty-fourth list of new mineral names E. E. FEJER Department of Mineralogy, British Museum (Natural History), Cromwell Road, London SW7 5BD THE present list contains 181 entries. Of these 148 are Alacranite. V. I. Popova, V. A. Popov, A. Clark, valid species, most of which have been approved by the V. O. Polyakov, and S. E. Borisovskii, 1986. Zap. IMA Commission on New Minerals and Mineral Names, 115, 360. First found at Alacran, Pampa Larga, 17 are misspellings or erroneous transliterations, 9 are Chile by A. H. Clark in 1970 (rejected by IMA names published without IMA approval, 4 are variety because of insufficient data), then in 1980 at the names, 2 are spelling corrections, and one is a name applied to gem material. As in previous lists, contractions caldera of Uzon volcano, Kamchatka, USSR, as are used for the names of frequently cited journals and yellowish orange equant crystals up to 0.5 ram, other publications are abbreviated in italic. sometimes flattened on {100} with {100}, {111}, {ill}, and {110} faces, adamantine to greasy Abhurite. J. J. Matzko, H. T. Evans Jr., M. E. Mrose, lustre, poor {100} cleavage, brittle, H 1 Mono- and P. Aruscavage, 1985. C.M. 23, 233. At a clinic, P2/c, a 9.89(2), b 9.73(2), c 9.13(1) A, depth c.35 m, in an arm of the Red Sea, known as fl 101.84(5) ~ Z = 2; Dobs. 3.43(5), D~alr 3.43; Sharm Abhur, c.30 km north of Jiddah, Saudi reflectances and microhardness given. -
Carnegie/DOE Alliance Center (CDAC): a CENTER of EXCELLENCE for HIGH PRESSURE SCIENCE and TECHNOLOGY
CARNEGIE/DOE ALLIANCE CENTER A Center of Excellence for High Pressure Science and Technology Supported by the Stockpile Stewardship Academic Alliances Program of DOE/NNSA Year Three Annual Report September 2006 Russell J. Hemley, Director Ho-kwang Mao, Associate Director Stephen A. Gramsch, Coordinator Carnegie/DOE Alliance Center (CDAC): A CENTER OF EXCELLENCE FOR HIGH PRESSURE SCIENCE AND TECHNOLOGY YEAR THREE ANNUAL REPORT 1. Overview 1.1 Mission of CDAC 3 1.2 Highlights from Year 3 4 1.3 Year 3 Work Plan and Milestones 6 2. Scientific Progress 2.1 High P-T Phase Relations and Structures 10 2.2 P-V-T EOS Measurements 19 2.3 Phonons, Vibrational Thermodynamics and Elasticity 22 2.4 Plasticity, Yield Strength and Deformation 26 2.5 Electronic and Magnetic Structure and Dynamics 27 2.6 High P-T Chemistry 36 3. Education, Training, and Outreach 3.1 CDAC Graduate Students and Post-doctoral Associates 40 3.2 CDAC Collaborators 43 3.3 Undergraduate Student Participation 47 3.4 DC Area High School Outreach 49 3.5 Synergy of 21st Century High-Pressure Science and Technology Workshop 50 3.6 Visitors to CDAC 56 3.7 High Pressure Seminars 58 4. Technology Development 4.1 High P-T Experimental Techniques 60 4.2 Facilities at Brookhaven, LANSCE, and Carnegie 64 4.3 Commissioning and Activities at HPCAT 66 5. Interactions with NNSA/DP National Laboratories 5.1 Overview 67 5.2 Academic Alliance and Laboratory Collaborations 69 6. Management and Oversight 6.1 CDAC Organization and Staff 71 6.2 CDAC Oversight 73 6.3 Second Year Review 74 7.