Discreditation of Bobdownsite and the Establishment of Criteria for the Identification of 2– Minerals with Essential Monofluorophosphate (PO3F )
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Synthesis of Magnesium- and Silicon-Modified Hydroxyapatites By
www.nature.com/scientificreports OPEN Synthesis of Magnesium- and Silicon-modifed Hydroxyapatites by Microwave-Assisted Method Received: 17 January 2019 Liudmila A. Rasskazova1, Ilya V. Zhuk1, Natalia M. Korotchenko1, Anton S. Brichkov1, Accepted: 19 September 2019 Yu-Wen Chen 2, Evgeniy A. Paukshtis1, Vladimir K. Ivanov1, Irina A. Kurzina 1 & Published: xx xx xxxx Vladimir V. Kozik1 Nanopowders of hydroxyapatite (HA), modifed by magnesium (MgHA) and by silicon (SiHA) were obtained by liquid-phase microwave synthesis method. X-ray difraction and IR spectroscopy results 2+ 4− showed that Mg and SiO4 ions were present in the synthesized products both as secondary phases and as part of the HA phase. Whitlockite was found in the magnesium-modifed HA (MgHA) and larnite was found in the silicon-modifed HA (SiHA); ion substitution for both materials resulted in solid solutions. In the synthesized samples of modifed HA, the increase of particle size of powders was in the order HA < SiHA < MgHA, which was calculated through data specifc surface area and measured pycnometric density of the powders. The Lewis acid sites (Ca2+, Mg2+, Si4+) were present using spectral probes on the surface of the samples of HA, MgHA, and SiHA, and the acidity of these sites decreased in the order SiHA > MgHA > HA. The rates of calcium phosphate layer deposition on the surface of these materials at 37 °C in the model simulated body fuid solution showed similar dependence. Te problem of fnding material for implantation has existed since ancient times. However, towards the end of the twentieth century the requirements for such materials and an informed and scientifcally grounded application began to form. -
(M = Ca, Mg, Fe2+), a Structural Base of Ca3mg3(PO4)4 Phosphors
crystals Article Crystal Chemistry of Stanfieldite, Ca7M2Mg9(PO4)12 (M = Ca, Mg, Fe2+), a Structural Base of Ca3Mg3(PO4)4 Phosphors Sergey N. Britvin 1,2,* , Maria G. Krzhizhanovskaya 1, Vladimir N. Bocharov 3 and Edita V. Obolonskaya 4 1 Department of Crystallography, Institute of Earth Sciences, St. Petersburg State University, Universitetskaya Nab. 7/9, 199034 St. Petersburg, Russia; [email protected] 2 Nanomaterials Research Center, Kola Science Center of Russian Academy of Sciences, Fersman Str. 14, 184209 Apatity, Russia 3 Centre for Geo-Environmental Research and Modelling, Saint-Petersburg State University, Ulyanovskaya ul. 1, 198504 St. Petersburg, Russia; [email protected] 4 The Mining Museum, Saint Petersburg Mining University, 2, 21st Line, 199106 St. Petersburg, Russia; [email protected] * Correspondence: [email protected] Received: 1 May 2020; Accepted: 25 May 2020; Published: 1 June 2020 Abstract: Stanfieldite, natural Ca-Mg-phosphate, is a typical constituent of phosphate-phosphide assemblages in pallasite and mesosiderite meteorites. The synthetic analogue of stanfieldite is used as a crystal matrix of luminophores and frequently encountered in phosphate bioceramics. However, the crystal structure of natural stanfieldite has never been reported in detail, and the data available so far relate to its synthetic counterpart. We herein provide the results of a study of stanfieldite from the Brahin meteorite (main group pallasite). The empirical formula of the mineral is Ca8.04Mg9.25Fe0.72Mn0.07P11.97O48. Its crystal structure has been solved and refined to R1 = 0.034. Stanfieldite from Brahin is monoclinic, C2/c, a 22.7973(4), b 9.9833(2), c 17.0522(3) Å, β 99.954(2)◦, 3 V 3822.5(1)Å . -
Multiscale Characterization of Bone Mineral: New Perspectives in Structural Imaging Using X-Ray and Electron Diffraction Contrast Mariana Verezhak
Multiscale characterization of bone mineral: new perspectives in structural imaging using X-ray and electron diffraction contrast Mariana Verezhak To cite this version: Mariana Verezhak. Multiscale characterization of bone mineral: new perspectives in structural imag- ing using X-ray and electron diffraction contrast. Materials Science [cond-mat.mtrl-sci]. Communauté Universite Grenoble Alpes, 2016. English. tel-01576447 HAL Id: tel-01576447 https://hal.archives-ouvertes.fr/tel-01576447 Submitted on 23 Aug 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. THESIS In order to obtain the grade of DOCTOR OF GRENOBLE ALPES UNIVERSITY Specialty: Physics/Nanophysics Ministerial order: 7 August 2006 Presented by « Mariana / VEREZHAK » Thesis supervised by « Marie/PLAZANET » and co-supervised by « Aurélien/GOURRIER » Prepared at Laboratory of Interdisciplinary Physics at Doctoral School of Physics of Grenoble Multiscale characterization of bone mineral: new perspectives in structural imaging using X-ray and electron diffraction contrast Thesis is publically defended on « 28 October 2016 », in front of the jury composed of : Prof. Franz BRUCKERT Grenoble INP UGA, President of jury Dr. Aurélien GOURRIER LIPhy, Grenoble, co-Director of thesis Prof. Thomas LAGRANGE Institute of Technology of Lausanne, Examiner Dr. -
Program and Abstracts
The Atlantic Geoscience Society (AGS) La Société Géoscientifique de l’Atlantique 45th Colloquium and Annual Meeting Special Sessions: • Special Session: In Memory of Dr. Trevor MacHattie (1974 - 2018) • Paleontology and Sedimentology in Atlantic Canada: In Memory of Dr. Ron Pickerill (1947 – 2018) • Current Research in Carboniferous Geology in the Atlantic Provinces • Minerals, metals, melts, and fluids associated with granitoid rocks: new insights from fundamental studies into the genesis, melt fertility, and ore-forming processes • Earth Science Outreach in the Maritime Provinces • Geohazards: Recent and Historical General Sessions: Current Research in the Atlantic Provinces February 7-9, 2019 Fredericton Inn, Fredericton, New Brunswick PROGRAM WITH ABSTRACTS We gratefully acknowledge sponsorship from the following companies and organizations: Department of Energy and Resource Development Geological Surveys Branch Department of Energy and Mines Department of Energy and Mines Geological Surveys Division Petroleum Resources Division Welcome to the 45th Colloquium and Annual Meeting of the Atlantic Geoscience Society in Fredericton, New Brunswick. This is a familiar place for AGS, having been a host several times over the years. We hope you will find something to interest you and generate discussion with old friends and new. AGS members are clearly pushing the boundaries of geoscience in all its branches! Be sure to take in the science on the posters and the displays from sponsors, and don’t miss the after-banquet jam and open mike on Saturday night. For social media types, please consider sharing updates on Facebook and Twitter (details in the program). We hope you will be able to use the weekend to renew old acquaintances, make new ones, and further the aims of your Atlantic Geoscience Society. -
Petrography, Mineralogy, and Geochemistry of Lunar Meteorite Sayh Al Uhaymir 300
Meteoritics & Planetary Science 43, Nr 8, 1363–1381 (2008) Abstract available online at http://meteoritics.org Petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300 Weibiao HSU1*, Aicheng ZHANG1, Rainer BARTOSCHEWITZ2 , Yunbin GUAN3, Takayuki USHIKUBO3, Urs KRÄHENBÜHL4, Rainer NIEDERGESAESS5, Rudolf PEPELNIK5, Ulrich REUS5, Thomas KURTZ6, and Paul KURTZ6 1Laboratory for Astrochemistry and Planetary Sciences, Lunar and Planetary Science Center, Purple Mountain Observatory, 2 West Beijing Road, Nanjing, 210008, China 2Bartoschewitz Meteorite Lab, Lehmweg 53, D-38518 Gifhorn, Germany 3Department of Geological Sciences, Arizona State University, Tempe, Arizona 85287, USA 4Abteilung für Chemie und Biochemie, Universität Bern, Freiestr. 3, CH-3012 Bern, Switzerland 5GKSS Forschungszentrum GmbH, Institut für Küstenforschung, Max-Planck-Strasse, D-21502 Geesthacht, Germany 6Henckellweg 25, D-30459 Hannover, Germany *Corresponding author. E-mail: [email protected] (Received 24 May 2007; revision accepted 19 March 2008) Abstract–We report here the petrography, mineralogy, and geochemistry of lunar meteorite Sayh al Uhaymir 300 (SaU 300). SaU 300 is dominated by a fine-grained crystalline matrix surrounding mineral fragments (plagioclase, pyroxene, olivine, and ilmenite) and lithic clasts (mainly feldspathic to noritic). Mare basalt and KREEPy rocks are absent. Glass melt veins and impact melts are present, indicating that the rock has been subjected to a second impact event. FeNi metal and troilite grains were observed in the matrix. Major element concentrations of SaU 300 (Al2O3 21.6 wt% and FeO 8.16 wt%) are very similar to those of two basalt-bearing feldspathic regolith breccias: Calcalong Creek and Yamato (Y-) 983885. However, the rare earth element (REE) abundances and pattern of SaU 300 resemble the patterns of feldspathic highlands meteorites (e.g., Queen Alexandra Range (QUE) 93069 and Dar al Gani (DaG) 400), and the average lunar highlands crust. -
THE REGOLITH PORTION of the LUNAR METEORITE SAYH AL UHAYMIR 169 A. Al-Kathiri1, 2, E. Gnos1 and B. A. Hofmann3 1Institut Für Ge
69th Annual Meteoritical Society Meeting (2006) 5098.pdf THE REGOLITH PORTION OF THE LUNAR METEORITE SAYH AL UHAYMIR 169 A. Al-Kathiri1, 2, E. Gnos1 and B. A. Hofmann3 1Institut für Geologie, Universität Bern, Baltzerstrasse 1, CH- 3012 Bern, Switzerland 2Directorate General of Commerce and Industry, Ministry of Commerce and Industry, Salalah, Sultanate of Oman. 3Naturhistorisches Museum der Burgergemeinde Bern, Bernastrasse 15, CH-3005 Bern, Switzerland. Introduction: SaU 169 is a complete, light gray- greenish stone (70 x 43 x 40 mm) with a mass of 206.45 g found in the Sultanate of Oman in January 2002. The rock consists of two contrasting lithologies. Approximately 87 vol% consists of a holocrystalline, fine-grained poikilitic polymict KREEP-rich im- pact melt breccia, the other 13 vol% are shock-lithified regolith [1]. Discussion: The regolith shows two formation stages and contains the following clasts: Ti-poor to Ti-rich basalts, gab- bros to granulites, and regolith breccias. The younger regolith additionally contains a highland gabbronorite clast with anorthite (An96-97), forsteritic (Fo85) and fayalitic (Fo12) mineral clasts, and impact melt glass shards. The average regolith bulk chemical composition and its REE content lie between the soil and regolith breccias of Apollo 12 and 14 , with more affinity with Apollo 14 [2,3,4]. The largest KREEP breccia clast in the regolith is identi- cal in its chemical composition and total REE content to the ITE- rich high-K KREEP rocks of the Apollo 14 landing site, pointing to a similar source. The regolith shows characteristic lunar ratios of Fe/Mn (74-80) and K/U (535-1682). -
Evaluation of a Fluorapatite-Spinel Ceramic As a Bone Implant Denginur Aksaci Iowa State University
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1981 Evaluation of a fluorapatite-spinel ceramic as a bone implant Denginur Aksaci Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Materials Science and Engineering Commons Recommended Citation Aksaci, Denginur, "Evaluation of a fluorapatite-spinel ceramic as a bone implant " (1981). Retrospective Theses and Dissertations. 6961. https://lib.dr.iastate.edu/rtd/6961 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS This was produced from a copy of a document sent to us for microfilming. While the most advanced technological means to photograph and reproduce this document have been used, the quality is heavily dependent upon the quality of the material submitted. The following explanation of techniques is provided to help you understand markings or notations which may appear on this reproduction. 1. The sign or "target" for pages apparently lacking from the document photographed is "Missing Page(s)". If it was possible to ubtain the missing page(s) or section, they are spliced into the film along with adjacent pages. This may have necessitated cutting through an image and duplicating adjacent pages to assure you of complete continuity. 2. When an image on the film is obliterated with a round black mark it is an indication that the film inspector noticed either blurred copy because of movement during exposure, or duplicate copy. -
0.10(PO4)2 -Tricalcium Phosphates with Me2+ = Mn, Ni, Cu
crystals Article 2+ New Ca2.90(Me )0.10(PO4)2 β-tricalcium Phosphates with Me2+ = Mn, Ni, Cu: Synthesis, Crystal-Chemistry, and Luminescence Properties Angela Altomare 1, Rosanna Rizzi 1, Manuela Rossi 2 , Asmaa El Khouri 3, Mohammed Elaatmani 3, Veronica Paterlini 4, Giancarlo Della Ventura 5 and Francesco Capitelli 6,* 1 Istituto di Cristallografia–CNR, Via G. Amendola, 122/O, 70126 Bari, Italy; [email protected] (A.A.); [email protected] (R.R.) 2 Dipartimento di Scienze della Terra dell’Ambiente e delle Risorse, Università di Napoli Federico II, Via Mezzocannone 8, 80134 Naples, Italy; [email protected] 3 Faculté des Sciences Semlalia, BP 2390, Université Cadi Ayyad, Marrakech 40000, Morocco; [email protected] (A.E.K.); [email protected] (M.E.) 4 Luminescent Materials Laboratory, Università di Verona, Ca’ Vignal, Strada Le Grazie 15, 37134 Verona, Italy; [email protected] 5 Dipartimento di Scienze, Università Roma Tre, Largo S. L. Murialdo 1, 00016 Monterotondo (Rome), Italy; [email protected] 6 Istituto di Cristallografia–CNR, Via Salaria Km 29.300, 00016 Monterotondo (Rome), Italy * Correspondence: [email protected]; Tel.: +39-06-90672161 Received: 19 April 2019; Accepted: 28 May 2019; Published: 1 June 2019 2+ ( ) β Abstract: Ca2.90Me0.10 PO4 2 (with Me = Mn, Ni, Cu) -tricalcium phosphate (TCP) powders were synthesized by solid-state reaction at T = 1200 ◦C and investigated by means of a combination of scanning electron microscopy (SEM) equipped with energy dispersive X-ray spectroscopy (EDS), powder X-ray diffraction (PXRD), Fourier transform infrared (FTIR) spectroscopy, and luminescence spectroscopy. -
Dahllite and Whitlockite from Amatuku Islet, Tuvalu
SHORT COMMUNICATIONS 123 mentale du r6le de la monazite. These de l'Institut [Manuscript received 7 March 1988; National Polytechnique de Lorraine, 117 pp. revised 5 April 1988] Radominsky, M. F. (1875) Reproduction artificielle de la monazite et de la xenotime. C. R. Aead. Sei. Paris, 80, 304-7. ~) Copyright the Mineralogical Society KEYWORDS: monazite, RE phosphates, hydrothermal synthesis, microprobe standards. Centre de Recherches Petrographiques et Gkochimiques, J. M. MONTEL* B.P. 20, 54501, Vandoeuvre Les Nancy Cedex, France F, LHOTE Universitk de Nancy I, 54500, Vandoeuvre les Nancy, France J. M. CLAUDE * Present Address: CNRS, U.A.10, 5 rue Kessler, 63000 Clermont Ferrand, France. MINERALOGICAL MAGAZINE, MARCH 1989, VOL. 53, PP. 123 5 Dahllite and whitlockite from Amatuku islet, Tuvalu PHOSPHATIC limestones and a related soil were phosphatic biocalcarenties and biocalcirudites described from collections made by the first Royal forming the phosbergs. Texturally the rocks are Society coral-reef-boring expedition to Funafuti grainstones with sorting being moderate to good in 1896 (Cooksey, 1896; David and Sweet, 1904, within any one layer. In the rudites, rounded clasts Judd, 1904; Sollas, 1904; cf. Cullis, 1904). Al- commonly vary up to 12.5 cm but the main range though there is some geographic uncertainty about is between 20 and 60 mm. Arenites are well the source of some of Judd's samples, the speci- rounded, medium to coarse sands in which gran- mens came from three localities on Funafuti, the ules consisting of entire tests of calcarinid and largest being on Amatuku. soritinid foraminifera are frequent (Fig. 1a). Fines Occurrence. -
Synthesis, Characterization and Process Optimization of Bone Whitlockite
nanomaterials Article Synthesis, Characterization and Process Optimization of Bone Whitlockite Sadaf Batool 1, Usman Liaqat 1 , Zakir Hussain 1,* and Manzar Sohail 2 1 School of Chemical and Materials Engineering (SCME), National University of Sciences & Technology (NUST), Sector H-12, 44000 Islamabad, Pakistan; [email protected] (S.B.); [email protected] (U.L.) 2 Department of Chemistry, School of Natural Sciences (SNS), National University of Sciences & Technology (NUST), Sector H-12, 44000 Islamabad, Pakistan; [email protected] * Correspondence: [email protected]; Tel./Fax: +0092-51-9085-5200 Received: 26 July 2020; Accepted: 20 August 2020; Published: 17 September 2020 Abstract: Whitlockite, being the second most abundant bio-mineral in living bone, finds huge applications in tissue regeneration and implants and its synthesis into its pure form has remained a challenge. Although precipitation of whitlockite phase has been reported recently in many publications, effects of various parameters to control such phase as well as conditions for the bulk preparation of this extremely important bio-mineral have not been investigated so far. In this work, we report the precipitation of pure whitlockite phase using common precursors. As reported in the literature, whitlockite is stable in a narrow pH range, therefore; optimization of pH for the stabilization of whitlockite phase has been investigated. Additionally, in order to narrow down the optimum conditions for the whitlockite precipitation, effect of temperature and heating conditions has also been studied. The obtained solids were characterized using powder X-ray diffraction (PXRD), Fourier transform infrared spectroscopy (FTIR), Raman spectroscopy, scanning electron microscopy (SEM) and thermogravimetric analysis (TGA). -
The Chlorine Isotope Composition of Martian Meteorites 2. Implications for the Early Solar System and the Formation of Mars
Meteoritics & Planetary Science 1–16 (2016) doi: 10.1111/maps.12591 The chlorine isotope composition of Martian meteorites 2. Implications for the early solar system and the formation of Mars Zachary SHARP1,2,*, Jeffrey WILLIAMS1, Charles SHEARER3, Carl AGEE3, and Kevin McKEEGAN4 1Earth and Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131–0001, USA 2Center for Stable Isotopes, University of New Mexico, Albuquerque, New Mexico 87131–0001, USA 3Institute of Meteoritics, University of New Mexico, Albuquerque, New Mexico 87131–0001, USA 4Earth and Space Sciences, University of California, Los Angeles, California 90095–1567, USA *Corresponding author. E-mail: [email protected] (Received 15 July 2015; revision accepted 29 October 2015) Abstract–We determined the chlorine isotope composition of 16 Martian meteorites using gas source mass spectrometry on bulk samples and in situ secondary ion microprobe analysis on apatite grains. Measured d37Cl values range from À3.8 to +8.6&. The olivine- phyric shergottites are the isotopically lightest samples, with d37Cl mostly ranging from À4 to À2&. Samples with evidence for a crustal component have positive d37Cl values, with an extreme value of 8.6&. Most of the basaltic shergottites have intermediate d37Cl values of À1to0&, except for Shergotty, which is similar to the olivine-phyric shergottites. We interpret these data as due to mixing of a two-component system. The first component is the mantle value of À4toÀ3&. This most likely represents the original bulk Martian Cl isotope value. The other endmember is a 37Cl-enriched crustal component. We speculate that preferential loss of 35Cl to space has resulted in a high d37Cl value for the Martian surface, similar to what is seen in other volatile systems. -
The Regolith Portion of the Lunar Meteorite Sayh Al Uhaymir 169
Meteoritics & Planetary Science 42, Nr 12, 2137–2152 (2007) Abstract available online at http://meteoritics.org The regolith portion of the lunar meteorite Sayh al Uhaymir 169 A. AL-KATHIRI1, 2*, E. GNOS1, 3, and B. A. HOFMANN4 1Institut für Geologie, Universität Bern, Baltzerstrasse 1, CH-3012 Bern, Switzerland 2Directorate General of Commerce and Industry, Ministry of Commerce and Industry, Salalah, Oman 3Muséum d’histoire naturelle de Genève, 1, route de Malagnou, CP 6434, CH-1211 Geneva 6, Switzerland 4Naturhistorisches Museum der Burgergemeinde Bern, Bernastrasse 15, CH-3005 Bern, Switzerland *Corresponding author. E-mail: [email protected] (Received 13 February 2006; revision accepted 25 June 2007) Abstract–Sayh al Uhaymir (SaU) 169 is a composite lunar meteorite from Oman that consists of polymict regolith breccia (8.44 ppm Th), adhering to impact-melt breccia (IMB; 32.7 ppm Th). In this contribution we consider the regolith breccia portion of SaU 169, and demonstrate that it is composed of two generations representing two formation stages, labeled II and III. The regolith breccia also contains the following clasts: Ti-poor to Ti-rich basalts, gabbros to granulites, and incorporated regolith breccias. The average SaU 169 regolith breccia bulk composition lies within the range of Apollo 12 and 14 soil and regolith breccias, with the closest correspondence being with that of Apollo 14, but Sc contents indicate a higher portion of mare basalts. This is supported by relations between Sm-Al2O3, FeO-Cr2O3-TiO2, Sm/Eu and Th-K2O. The composition can best be modeled as a mixture of high-K KREEP, mare basalt and norite/troctolite, consistent with the rareness of anorthositic rocks.