Rubies and Sapphires from Snezhnoe, Tajikistan
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Mineralogy and Geochemistry of Ocelli in the Damtjernite Dykes and Sills, Chadobets Uplift, Siberian Craton: Evidence of the Fluid–Lamprophyric Magma Interaction
minerals Article Mineralogy and Geochemistry of Ocelli in the Damtjernite Dykes and Sills, Chadobets Uplift, Siberian Craton: Evidence of the Fluid–Lamprophyric Magma Interaction Anna A. Nosova 1,*, Ludmila V. Sazonova 1,2, Alexey V. Kargin 1 , Elena O. Dubinina 1 and Elena A. Minervina 1 1 Institute of Geology of Ore Deposits, Petrography, Mineralogy and Geochemistry, Russian Academy of Sciences (IGEM RAS), 119017 Moscow, Russia; [email protected] (L.V.S.); [email protected] (A.V.K.); [email protected] (E.O.D.); [email protected] (E.A.M.) 2 Geology Department, Lomonosov Moscow State University, 119991 Moscow, Russia * Correspondence: [email protected]; Tel.:+7-499-230-8414 Abstract: The study reports petrography, mineralogy and carbonate geochemistry and stable iso- topy of various types of ocelli (silicate-carbonate globules) observed in the lamprophyres from the Chadobets Uplift, southwestern Siberian craton. The Chadobets lamprophyres are related to the REE-bearing Chuktukon carbonatites. On the basis of their morphology, mineralogy and relation with the surrounding groundmass, we distinguish three types of ocelli: carbonate-silicate, containing carbonate, scapolite, sodalite, potassium feldspar, albite, apatite and minor quartz ocelli (K-Na-CSO); carbonate–silicate ocelli, containing natrolite and sodalite (Na-CSO); and silicate-carbonate, con- taining potassium feldspar and phlogopite (K-SCO). The K-Na-CSO present in the most evolved Citation: Nosova, A.A.; Sazonova, damtjernite with irregular and polygonal patches was distributed within the groundmass; the patches L.V.; Kargin, A.V.; Dubinina, E.O.; consist of minerals identical to minerals in ocelli. Carbonate in the K-Na-CSO are calcite, Fe-dolomite Minervina, E.A. -
EVIDENCE for MAGMATIC-HYDROTHERMAL ACTIVITY on MARS from Cl-RICH SCAPOLITE in NAKHLA
45th Lunar and Planetary Science Conference (2014) 1620.pdf EVIDENCE FOR MAGMATIC-HYDROTHERMAL ACTIVITY ON MARS FROM Cl-RICH SCAPOLITE IN NAKHLA. J. Filiberto1, C.A. Goodrich2, A.H. Treiman3, J. Gross4, and P.A. Giesting1, 1Southern Illinois University, Geology Dept, Carbondale, IL 62901 USA, [email protected], 2Planetary Science Institute, Tucson AZ 85719 USA. 3Lunar and Planetary Institute, Houston, TX 77058 USA, 4American Museum of Natural History, New York, NY USA. Introduction: Scapolite is a common terrestrial The melt inclusion containing the Cl-scapolite (Fig. hydrothermal, metamorphic, and metasomatic mineral 1) is dominated by high-Ca pyroxene, K-feldspar and which forms by the reaction of plagioclase and a Cl- or K-rich glass, with minor chromite, Fe-sulfides, Fe-Ti CO2-rich fluid [1-3]. It is less common as a primary oxides, and alteration material [9]. The occurrence of igneous phase, but has been reported as megacrysts, the scapolite appears to be texturally equivalent to the phenocrysts, and oikocrysts in alkali-rich basaltic K-feldspar or the glass (i.e., interstitial to the pyrox- magmas [4-6]. Based on reflectance spectra, scapolite enes), and may therefore be replacing, or contempora- has also been suggested to exist on the surface of Mars neous with, one of these phases. It contains ~3.9 wt.% as a possible alteration mineral [7]. Cl, and has the formula (Na2.8Ca0.7K0.3)3.9(Si8.3Al3.7)12ClO24. Scapolite has three main end member composi- It is almost pure end-member marialite with little tions: marialite (Na4Al3Si9O24Cl), meionite meionite component (Fig. 2). -
Sulfate-Rich Scapolite on Mars?
Lunar and Planetary Science XXXVIII (2007) 1152.pdf Sulfate-rich Scapolite on Mars? J.J. Papike, J.M. Karner, and C.K. Shearer Astromaterials Institute, Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, New Mexico 87131 INTRODUCTION also shows selected bonds to neighboring Ca atoms. The surface of Mars shows abundant evidence for This configuration is remarkably stable in P-T space sulfur activity over a prolonged period in martian discussed below. history. Evidence goes back to the Viking landers in STABILITY 1976 but more recent orbital and landed in situ Figure 3 illustrates the stability field of SM [3]. The missions, including the two MER rovers, which are diagram shows that SM can be stable over the still active, confirm this. The identification of the pressure interval ~ 10 to 27 Kb at 1200 degrees C. sulfate jarosite with ferric iron confirms highly This corresponds to a depth interval of ~90 – 243 km oxidizing conditions near the martian surface. We depth in Mars (Fig. 4). In this depth range SM may speculate that conditions oxidizing enough to crystallize if the fO2 is high enough for S to exist as + crystallize a SO4 containing scapolite exist in the 6 . lower martian crust or upper mantle. This scapolite TERRESTRIAL OCCURENCES could be a important reservoir for sulfate in Mars and Terrestrial occurrences of igneous scapolite are might form either directly from sulfur-rich, oxidizing discussed in [2,4, and 5]. Boivin and Camus [4] magmas or by metasomatism of previously discuss a scapolite assemblage found as megacrysts crystallized plagioclase in basalt. -
Metasomatic Alteration Associated with Regional Metamorphism: an Example from the Willyama Supergroup, South Australia
Lithos 54Ž. 2000 33±62 www.elsevier.nlrlocaterlithos Metasomatic alteration associated with regional metamorphism: an example from the Willyama Supergroup, South Australia A.J.R. Kent a,),1, P.M. Ashley a,2, C.M. Fanning b,3 a DiÕision of Earth Sciences, UniÕersity of New England, Armidale, NSW, 2351, Australia b Research School of Earth Sciences, The Australian National UniÕersity, Canberra, ACT, 0200, Australia Received 20 October 1998; accepted 12 May 2000 Abstract The Olary Domain, part of the Curnamona Province, a major Proterozoic terrane located within eastern South Australia and western New South Wales, Australia, is an excellent example of geological region that has been significantly altered by metasomatic mass-transfer processes associated with regional metamorphism. Examples of metasomatically altered rocks in the Olary Domain are ubiquitous and include garnet±epidote-rich alteration zones, clinopyroxene- and actinolite-matrix breccias, replacement ironstones and albite-rich alteration zones in quartzofeldspathic metasediments and intrusive rocks. Metasomatism is typically associated with formation of calcic, sodic andror iron-rich alteration zones and development of oxidised mineral assemblages containing one or more of the following: quartz, albite, actinolite±hornblende, andradite-rich garnet, epidote, magnetite, hematite and aegerine-bearing clinopyroxene. Detailed study of one widespread style of metasomatic alteration, garnet±epidote-rich alteration zones in calc-silicate host rocks, provides detailed information on the timing of metasomatism, the conditions under which alteration occurred, and the nature and origin of the metasomatic fluids. Garnet±epidote-bearing zones exhibit features such as breccias, veins, fracture-controlled alteration, open space fillings and massive replacement of pre-existing calc-silicate rock consistent with formation at locally high fluid pressures and fluidrrock ratios. -
INVESTIGATION of a CAT's-EYE SCAPOLITE from SRI LANKA by K
INVESTIGATION OF A CAT'S-EYE SCAPOLITE FROM SRI LANKA By K. Schmetzer and H. Bank A cut gemstone with intense chatoyancy that Furthermore, hexagonal plates up to 0.4 x 0.4 originated from Sri Lanka was determined to be a mm in size with metallic luster were determined member of the scapolite solid-solution series, Indices to be pyrrhotite in these samples (Graziani and of refraction and unit-cell dimensions were found as Gubelin, 1981). w = 1.583, e = 1.553 and2 = 12.169, = 7.569 A, This article describes a scapolite crystal from respectively; a meionite content of 69% was Sri Lanlza that was cut into a 1.68-ct cabochon established by microprobe analysis. The chatoyancy (approximately 9 mm x 5 mm) with particularly is caused by needle-like inclusions with an orientation parallel to the c-axis of the scapolite host intense chatoyancy (figure 1). The ray of light crystal. Microprobe analysis of these needles showed crossing the surface of the cabochon is relatively them to be pyrrl~otite. broad compared to the sharpness of rays in other gemstones with chatoyancy or asterism, such as the more familiar cat's-eye chrysoberyls or aste- riated corundum. The physical and chemical properties of this cat's-eye scapolite are pre- Natural scapolites are members of the solid- sented, and the cause of the distinctive chatoy- solution series marialite, Nag[(C12,S04,C03)1 (A1 ancy in this stone is explained. Si308)e],and meionite, CadClaSO+C03) (A12 1 PHYSICAL AND CHEMICAL PROPERTIES Si20g)g].Scapolite crystals of gem quality occur colorless and in white, gray, yellow, pink, and A small facet was cut and polished on the bottom violet. -
Volume 23 / No. 7 / 1993
Volume 23 No. 7. July 1993 1116 Journal of Gemmology THE GEMMOLOGICAL ASSOCIATION AND GEM TESTING LABORATORY OF GREAT BRITAIN OFFICERS AND COUNCIL Past Presidents: Sir Henry Miers, MA, D.Sc., FRS Sir William Bragg, OM, KBE, FRS Dr. G.F. Herbert Smith, CBE, MA, D.Sc. Sir Lawrence Bragg, CH, OBE, MC, B.Sc, FRS Sir Frank Claringbull, Ph.D., F.Inst.P., FGS Vice-Presidents: R. K. Mitchell, FGA A.E. Farn, FGA D.G. Kent, FGA E. M. Bruton, FGA, DGA Council of Management CR. Cavey, FGA T.J. Davidson, FGA N.W. Deeks, FGA E.A. Jobbins, B.Sc, C.Eng., FIMM, FGA I. Thomson, FGA V.P. Watson, FGA, DGA R.R. Harding, B.Sc., D.Phil., FGA, C. Geol. Members' Council A. J. Allnutt, M.Sc, G.H. Jones, B.Sc, Ph.D., P. G. Read, C.Eng., Ph.D., FGA FGA MIEE, MIERE, FGA, DGA P. J. E. Daly, B.Sc, FGA J. Kessler I. Roberts, FGA P. Dwyer-Hickey, FGA, G. Monnickendam R. Shepherd DGA L. Music R. Velden R. Fuller, FGA, DGA J.B. Nelson, Ph.D., FGS, D. Warren B. Jackson, FGA F. Inst. P., C.Phys., FGA CH. Winter, FGA, DGA Branch Chairmen: Midlands Branch: D.M. Larcher, FBHI, FGA, DGA North-West Branch: I. Knight, FGA, DGA Examiners: A. J. Allnutt, M.Sc, Ph.D., FGA G. H. Jones, B.Sc, Ph.D., FGA L. Bartlett, B.Sc, M.Phil., FGA, DGA D. G. Kent, FGA E. M. Bruton, FGA, DGA R. D. Ross, B.Sc, FGA C R. -
Minerals Found in Michigan Listed by County
Michigan Minerals Listed by Mineral Name Based on MI DEQ GSD Bulletin 6 “Mineralogy of Michigan” Actinolite, Dickinson, Gogebic, Gratiot, and Anthonyite, Houghton County Marquette counties Anthophyllite, Dickinson, and Marquette counties Aegirinaugite, Marquette County Antigorite, Dickinson, and Marquette counties Aegirine, Marquette County Apatite, Baraga, Dickinson, Houghton, Iron, Albite, Dickinson, Gratiot, Houghton, Keweenaw, Kalkaska, Keweenaw, Marquette, and Monroe and Marquette counties counties Algodonite, Baraga, Houghton, Keweenaw, and Aphrosiderite, Gogebic, Iron, and Marquette Ontonagon counties counties Allanite, Gogebic, Iron, and Marquette counties Apophyllite, Houghton, and Keweenaw counties Almandite, Dickinson, Keweenaw, and Marquette Aragonite, Gogebic, Iron, Jackson, Marquette, and counties Monroe counties Alunite, Iron County Arsenopyrite, Marquette, and Menominee counties Analcite, Houghton, Keweenaw, and Ontonagon counties Atacamite, Houghton, Keweenaw, and Ontonagon counties Anatase, Gratiot, Houghton, Keweenaw, Marquette, and Ontonagon counties Augite, Dickinson, Genesee, Gratiot, Houghton, Iron, Keweenaw, Marquette, and Ontonagon counties Andalusite, Iron, and Marquette counties Awarurite, Marquette County Andesine, Keweenaw County Axinite, Gogebic, and Marquette counties Andradite, Dickinson County Azurite, Dickinson, Keweenaw, Marquette, and Anglesite, Marquette County Ontonagon counties Anhydrite, Bay, Berrien, Gratiot, Houghton, Babingtonite, Keweenaw County Isabella, Kalamazoo, Kent, Keweenaw, Macomb, Manistee, -
Contact Zone Mineralogy and Geochemistry of the Mt. Mica Pegmatite, Oxford County, Maine
University of New Orleans ScholarWorks@UNO University of New Orleans Theses and Dissertations Dissertations and Theses Spring 5-16-2014 Contact Zone Mineralogy and Geochemistry of the Mt. Mica Pegmatite, Oxford County, Maine Kimberly T. Clark University of New Orleans, [email protected] Follow this and additional works at: https://scholarworks.uno.edu/td Part of the Geochemistry Commons, and the Geology Commons Recommended Citation Clark, Kimberly T., "Contact Zone Mineralogy and Geochemistry of the Mt. Mica Pegmatite, Oxford County, Maine" (2014). University of New Orleans Theses and Dissertations. 1786. https://scholarworks.uno.edu/td/1786 This Thesis is protected by copyright and/or related rights. It has been brought to you by ScholarWorks@UNO with permission from the rights-holder(s). You are free to use this Thesis in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights- holder(s) directly, unless additional rights are indicated by a Creative Commons license in the record and/or on the work itself. This Thesis has been accepted for inclusion in University of New Orleans Theses and Dissertations by an authorized administrator of ScholarWorks@UNO. For more information, please contact [email protected]. Contact Zone Mineralogy and Geochemistry of the Mt. Mica Pegmatite, Oxford County, Maine A Thesis Submitted to the Graduate Faculty of the University of New Orleans in partial fulfillment of the requirements for the degree of Master of Science In Earth and Environmental Science By Kimberly T. Clark B.S. -
An In-Vitro Evaluation of the Capacity of Local Tanzanian Crude Clay and Ash Based Materials in Binding Aflatoxins in Solution
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 2 November 2018 doi:10.20944/preprints201811.0021.v1 Peer-reviewed version available at Toxins 2018, 10, 510; doi:10.3390/toxins10120510 An in-vitro evaluation of the capacity of local Tanzanian crude clay and ash based materials in binding aflatoxins in solution 1,3Ayo E. M; 2G. H. Laswai; 1A. Matemu; 1M. E. Kimanya* 1 The Nelson Mandela African Institution of Science and Technology, P.O. Box 447, Arusha. Tanzania E-mails: [email protected]; [email protected]: kimanya.martin@nm-aist 2 Sokoine University of Agriculture, P.O. Box 3004, Morogoro. Tanzania, E-mail: [email protected] 3 Institute of Rural Development Planning, P.O. Box 138, Dodoma, Tanzania, E-mail: [email protected] *The corresponding author, email: kimanya.martin@nm-aist Corresponding author: Prof Martin E. Kimanya (Associate Professor of Food safety and Nutrition Sciences) P.O. Box 447, Arusha. Tanzania; e-mail: [email protected] Abstract Aflatoxins in feeds cause great health hazards to animals and in advance, to human. Potential of crude clays designated AC, KC, CC and MC and ashes VA and RA were evaluated for their capacity to adsorb aflatoxins B1 (AFB1), B2 (AFB2), G1 (AFG1) and G2 (AFG2) relative to a commercial binder MycobinderR (Evonik Industries AG) using in-vitro technique. On average, CC, VA, KC, MC, AC, RA and MycobindR adsorbed 39.9%, 51.3%, 61.5%, 62.0%, 72.6%, 84.7% and 98.1% of the total aflatoxins in buffered solution, respectively. -
Clay Minerals
American Minetralogist, Volume 65, pages 1-7, 1980 Summary of recommendations of AIPEA nomenclature committee on clay minerals S. W. BAILEY, CHAIRMAN1 Department of Geology and Geophysics University of Wisconsin-Madison Madi~on, Wisconsin 53706 Introduction This summary of the recommendations made to Because of their small particle sizes and v~riable date by the international nomenclature committees degrees of crystal perfection, it is not surprisi4g that has been prepared in order to achieve wider dissemi- clay minerals proved extremely difficult to character- nation of the decisions reached and to aid clay scien- ize adequately prior to the development of ~odem tists in the correct usage of clay nomenclature. Some analytical techniques. Problems in charactetization of the material in the present summary has been led quite naturally to problems in nomenclatute, un- taken from an earlier summary by Bailey et al. doubtedly more so than for the macroscopic~ more (1971a). crystalline minerals. The popular adoption ~ the early 1950s of the X-ray powder diffractometer for Classification . clay studies helped to solve some of the probl ms of Agreement was reached early in the international identification. Improvements in electron micro copy, discussions that a sound nomenclatur~ is necessarily electron diffraction and oblique texture electr ;n dif- based on a satisfactory classification scheme. For this fraction, infrared and DT A equipment, the de elop- reason, the earliest and most extensive efforts of the ment of nuclear and isotope technology, of high- several national nomenclature committees have been speed electronic computers, of Mossbauer spec rome- expended on classification schemes. Existing schemes ters, and most recently of the electron micr probe were collated and discussed (see Brown, 1955, Mac- and scanning electron microscope all have ai ed in kenzie, 1959, and Pedro, 1967, for examples), sym- the accumulation of factual information on clays. -
Identification Tables for Common Minerals in Thin Section
Identification Tables for Common Minerals in Thin Section These tables provide a concise summary of the properties of a range of common minerals. Within the tables, minerals are arranged by colour so as to help with identification. If a mineral commonly has a range of colours, it will appear once for each colour. To identify an unknown mineral, start by answering the following questions: (1) What colour is the mineral? (2) What is the relief of the mineral? (3) Do you think you are looking at an igneous, metamorphic or sedimentary rock? Go to the chart, and scan the properties. Within each colour group, minerals are arranged in order of increasing refractive index (which more or less corresponds to relief). This should at once limit you to only a few minerals. By looking at the chart, see which properties might help you distinguish between the possibilities. Then, look at the mineral again, and check these further details. Notes: (i) Name: names listed here may be strict mineral names (e.g., andalusite), or group names (e.g., chlorite), or distinctive variety names (e.g., titanian augite). These tables contain a personal selection of some of the more common minerals. Remember that there are nearly 4000 minerals, although 95% of these are rare or very rare. The minerals in here probably make up 95% of medium and coarse-grained rocks in the crust. (ii) IMS: this gives a simple assessment of whether the mineral is common in igneous (I), metamorphic (M) or sedimentary (S) rocks. These are not infallible guides - in particular many igneous and metamorphic minerals can occur occasionally in sediments. -
Compressibility of Sodalite and Scapolite
American Mineralogist, Volume 73, pages I120-1122, 1988 Compressibility of sodalite and scapolite Rosnnr M. Hlznx, ZacHanY D. Snanp GeophysicalLaboratory, CarnegieInstitution of Washington,280l Upton Street,N.W., Washington, D.C.20008, U.S.A. Ansrn-lcr Equation-of-stateparameters of sodalite (NaoAlrSi.O,rCl)and a meionitic scapolite(ap- proximately CaoAluSiuOroCOr)have been calculated from pressure-volumedata obtained by single-crystalX-ray diffraction techniques. Linear compressibility of cubic sodalite is 6.4 x ll-a kbar-', correspondingto a bulk modulus of 0.52 + 0.08 Mbar (assumingK : 4). The pressureresponse of tetragonal scapoliteis almost isotropic with compressibilities parallel and perpendicular to the c axis of3.5 x lO-a and 3.7 x l0-4 kbar-l, respectively; the bulk modulus is 0.90 + 0.12 Mbar. Sodalite and scapolite compress principally by deformation of the Al-Si tetrahedral framework coupled with Na-O and Ca-O bond compression,respectively. The greater compressibility of sodalite compared to scapolite is primarily a Coulombic effect, arising from the difference in bond strength of Na*-O versus Ca2*-O bonds. INrnonucrroN both sodalite (N. Komada, E. F. Westrum, Jr., B. S. Sodalite and scapolite are open framework silicates that Hemingway, M. Y. Zolotov, Y. V. Semenov,I. L. Kho- contain halides or carbonatesof Na or Ca. NaCl is an dakovsky, and L. M. Anovitz, in prep.; Taylor, 1968)and essentialcomponent of sodalite (NaoAlrSirO,rCl),where- scapolite(N. Komada, D.P.Moecher, E. F. Westrum, as coupled NaCl-CaCO. and NaSi-CaAl substitutions re- Jr., B. S. Hemingway, Y. V. Semenov, and L L.