Lab 2: Mineral Properties and Non-Silicate Minerals
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A Vibrational Spectroscopic Study of the Silicate Mineral Harmotome Â
Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy 137 (2015) 70–74 Contents lists available at ScienceDirect Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy journal homepage: www.elsevier.com/locate/saa A vibrational spectroscopic study of the silicate mineral harmotome – (Ba,Na,K)1-2(Si,Al)8O16Á6H2O – A natural zeolite ⇑ Ray L. Frost a, , Andrés López a, Lina Wang a,b, Antônio Wilson Romano c, Ricardo Scholz d a School of Chemistry, Physics and Mechanical Engineering, Science and Engineering Faculty, Queensland University of Technology, GPO Box 2434, Brisbane, Queensland 4001, Australia b School of Chemistry and Chemical Engineering, Tianjin University of Technology, No. 391, Bin Shui West Road, Xi Qing District, Tianjin, PR China c Geology Department, Federal University of Minas Gerais, Belo Horizonte, MG 31270-901, Brazil d Geology Department, School of Mines, Federal University of Ouro Preto, Campus Morro do Cruzeiro, Ouro Preto, MG 35400-00, Brazil highlights graphical abstract We have studied the mineral harmotome (Ba,Na,K)1- 2(Si,Al)8O16Á6H2O. It is a natural zeolite. Raman and infrared bands are attributed to siloxane stretching and bending vibrations. A sharp infrared band at 3731 cmÀ1 is assigned to the OH stretching vibration of SiOH units. article info abstract Article history: The mineral harmotome (Ba,Na,K)1-2(Si,Al)8O16Á6H2O is a crystalline sodium calcium silicate which has Received 31 March 2014 the potential to be used in plaster boards and other industrial applications. It is a natural zeolite with cat- Received in revised form 7 July 2014 alytic potential. Raman bands at 1020 and 1102 cmÀ1 are assigned to the SiO stretching vibrations of Accepted 28 July 2014 three dimensional siloxane units. -
Carbonation and Decarbonation Reactions: Implications for Planetary Habitability K
American Mineralogist, Volume 104, pages 1369–1380, 2019 Carbonation and decarbonation reactions: Implications for planetary habitability k E.M. STEWART1,*,†, JAY J. AGUE1, JOHN M. FERRY2, CRAIG M. SCHIFFRIES3, REN-BIAO TAO4, TERRY T. ISSON1,5, AND NOAH J. PLANAVSKY1 1Department of Geology & Geophysics, Yale University, P.O. Box 208109, New Haven, Connecticut 06520-8109, U.S.A. 2Department of Earth and Planetary Sciences, Johns Hopkins University, 3400 N. Charles Street, Baltimore, Maryland 21218, U.S.A. 3Geophysical Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, D.C. 20015, U.S.A. 4School of Earth and Space Sciences, MOE Key Laboratory of Orogenic Belt and Crustal Evolution, Peking University, Beijing 100871, China 5School of Science, University of Waikato, 101-121 Durham Street, Tauranga 3110, New Zealand ABSTRACT The geologic carbon cycle plays a fundamental role in controlling Earth’s climate and habitability. For billions of years, stabilizing feedbacks inherent in the cycle have maintained a surface environ- ment that could sustain life. Carbonation/decarbonation reactions are the primary mechanisms for transferring carbon between the solid Earth and the ocean–atmosphere system. These processes can be broadly represented by the reaction: CaSiO3 (wollastonite) + CO2 (gas) ↔ CaCO3 (calcite) + SiO2 (quartz). This class of reactions is therefore critical to Earth’s past and future habitability. Here, we summarize their significance as part of the Deep Carbon Obsevatory’s “Earth in Five Reactions” project. In the forward direction, carbonation reactions like the one above describe silicate weathering and carbonate formation on Earth’s surface. Recent work aims to resolve the balance between silicate weathering in terrestrial and marine settings both in the modern Earth system and through Earth’s history. -
Carbonation and Decarbonation Reactions: Implications for Planetary Habitability K
American Mineralogist, Volume 104, pages 1369–1380, 2019 Carbonation and decarbonation reactions: Implications for planetary habitability k E.M. STEWART1,*,†, JAY J. AGUE1, JOHN M. FERRY2, CRAIG M. SCHIFFRIES3, REN-BIAO TAO4, TERRY T. ISSON1,5, AND NOAH J. PLANAVSKY1 1Department of Geology & Geophysics, Yale University, P.O. Box 208109, New Haven, Connecticut 06520-8109, U.S.A. 2Department of Earth and Planetary Sciences, Johns Hopkins University, 3400 N. Charles Street, Baltimore, Maryland 21218, U.S.A. 3Geophysical Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, D.C. 20015, U.S.A. 4School of Earth and Space Sciences, MOE Key Laboratory of Orogenic Belt and Crustal Evolution, Peking University, Beijing 100871, China 5School of Science, University of Waikato, 101-121 Durham Street, Tauranga 3110, New Zealand ABSTRACT The geologic carbon cycle plays a fundamental role in controlling Earth’s climate and habitability. For billions of years, stabilizing feedbacks inherent in the cycle have maintained a surface environ- ment that could sustain life. Carbonation/decarbonation reactions are the primary mechanisms for transferring carbon between the solid Earth and the ocean–atmosphere system. These processes can be broadly represented by the reaction: CaSiO3 (wollastonite) + CO2 (gas) ↔ CaCO3 (calcite) + SiO2 (quartz). This class of reactions is therefore critical to Earth’s past and future habitability. Here, we summarize their signifcance as part of the Deep Carbon Obsevatory’s “Earth in Five Reactions” project. In the forward direction, carbonation reactions like the one above describe silicate weathering and carbonate formation on Earth’s surface. Recent work aims to resolve the balance between silicate weathering in terrestrial and marine settings both in the modern Earth system and through Earth’s history. -
Nature of Interlayer Material in Silicate Clays of Selected Oregon Soils
AN ABSTRACT OF THE THESIS OF PAUL C, SINGLETON for the Ph.D. in Soils (Name) (Degree) (Major) Date thesis is presented July 28, 1965 Title NATURE OF INTERLAYER MATERIAL IN SILICATE CLAYS OF SELECTED OREGON SOILS - Redacted for Privacy Abstract approved = ajor professor) Ç A study was conducted to investigate the nature of hydroxy interlayers in the chlorite -like intergrade clays of three Oregon soils with respect to kind, amount, stability, and conditions of formation. The clays of the Hembre, Wren, and Lookout soils, selected to represent weathering products originating from basaltic materials under humid, subhumid, and semi -arid climatic conditions respectively, were subjected to a series of progressive treatments designed to effect a differential dissolution of the materials intimately asso- ciated with them. The treatments, chosen to represent a range of increasing severity of dissolution, were (1) distilled water plus mechanical stirring, (2) boiling 2% sodium carbonate, (3) buffered sodium citrate -dithionite, (4) boiling sodium hydroxide, and (5) preheating to 400 °C for 4 hours plus boiling sodium hydroxide. Extracts from the various steps of the dissolution procedure were chemically analyzed in order to identify the materials removed from the clays. X -ray diffraction analysis and cation exchange capacity determinations were made on the clays after each step, and any differences noted in the measured values were attributed to the removal of hydroxy interlayers from the clays. Hydroxy interlayers were found to occur more in the Hembre and Wren soils than in the Lookout soil, with the most stable interlayers occurring in the Wren. Soil reaction was one of the major differences between these soils. -
O Lunar and Planetary Institute Provided by the NASA Astrophysics Data System WHITLOCKITE SATURATION
WHITLOCKITE SATURATION IN LUNAR BASALTS, J.E. Dickinson and P.C. Hess, Dept. of Geological Sciences, Brown University, Providence, RI 02912 As part of a continuing program initiated to evaluate the evolution of late-stage lunar magmas and the possible effects of crystallization of minor phases on their geochemistry, we have determined the saturation surface for whitlockite, Ca (PO ), in a liquid composition produced by crystallization of KREEP basalt 15386 lf~able1). Whitlockite is by far the most abundant phos- phate mineral in lunar rocks and in all probability is more abundant than other minor phases such as zircon, zirccnolite, monazite, and tranquillityite (1). Whitlockite is also an important component of mesosiderites, reported average modal phosphate abundances in mesosiderites ranging from 0.0-3.7% (avg. 1.9%) (2). Even higher phosphate abundances (up to 9.4%) have been observed in basaltic lithic clasts of presumed impact melt origin found in mesosiderites (3). Analyses of lunar whitlockites commonly show Ce203and Y203 contents up to 3 wt% and REE contents that may be as high as 1-2 wt% for La203and Nd203 de- creasing to levels of -0.1-0.2 wt% for the HREE (1). It has been shown that whitlockite is generally more enriched in REE's relative to chondrites than other minor phases in the same rock (4). Uranium and thorium may also be present in significant amounts although other minerals may contain more. Whit- lockite may, therefore, be an important reservoir of rare earth and heat producing elements. In addition, the amount of FeO and MgO in whitlockite is variable (Table 1). -
Validation of Zeolites to Maximize Ammonium and Phosphate Removal from Anaerobic Digestate by Combination of Zeolites in Ca and Na Forms Page 1
Validation of zeolites to maximize ammonium and phosphate removal from anaerobic digestate by combination of zeolites in Ca and Na forms Page 1 Abstract Ammonium and phosphate are fundamental nutrients for human life, but their excess in water can lead to eutrophication, an uncontrolled growth of biomass with a consequent deficit of oxygen (hypoxia) that can be really dangerous for water life. This excess is principally due to human activities such as industry and agriculture (detergents, fertilizers) and the problem is expected to grow during next years. Then, it is necessary to find an efficient, simple and low cost technology able to remove the nutrients from water in order to avoid environmental damages. Moreover, the population growth, the constant improvement in agriculture and the consequent increase in fertilizers demand have made the recovery of nutrient from water a real need, as it has been estimated that a 20% of the total needs of Europe could be recovered from wastewaters. Although both ammonium and phosphate have to be recovered from wastewater, their simultaneous removal by means of one adsorbent material has rarely been reported hitherto. The merit of using one material for the simultaneous removal is obvious, even if it has not been achieved yet. In general, most of the solutions proposed for the simultaneous removal of ammonium and phosphate are based on the use of two types of reagents. A large list of removal technologies, ranging from biological to physic-chemical methods, have been widely studied: in this work, zeolites in Ca and Na forms were evaluated as sorbents for phosphate and ammonium from synthetic water and real anaerobic digestate. -
Origin and Metal Content of Magmatic Sulfides in Cu-Au Mineralizing Silicic Magmas
Introduction Based on work by Keith et al. (1997) at the Bingham and Tintic mining districts in Utah, evidence from the Bajo de la Alumbrera complex, and preliminary evidence from other porphyry systems, Halter et al. (2002a) proposed that the destabilization of magmatic sulfides and dissolution temperature of sulfide metals into magmatic ore fluids is responsible for producing the characteristic Au/Cu ratios shared by both the magmatic sulfides and the bulk ore body. This study compares the copper, silver and gold content and ratios of magmatic sulfide inclusions related to the Cu±Mo porphyry system of Yerington, Nevada, USA, and the high-sulfidation epithermal Au- Cu system of Yanacocha, Peru. These two groups of magmatic rocks are compared with one another to test whether or not the metal contents and ratios of magmatic sulfides in each large mining district dictate the average metal content and metal ratios of bulk ores. Samples of volcanic rocks spanning around 4 Ma from pre-ore to syn- ore in the Yanacocha district were chosen to determine the variation of sulfide mineralogy and metal content, and correlate these with mineralizing events. Laser Ablation Inductively Coupled Plasma Mass Spectrometry (LA-ICPMS) and electron microprobe analysis were used to directly determine the metal contents of magmatic sulfide inclusions. A methodology for LA-ICPMS analysis of sulfides was developed for the OSU instrumentation, and included standardization, lab protocols, and estimation of detection limits of relevant trace metals. 2 Geologic Setting and Background Information Where there is sufficient quantity of sulfide sulfur in a silicate melt, sulfide saturation may occur to produce immiscible sulfide and silicate liquids (Ebel and Naldrett, 1997). -
Monazite, Rhabdophane, Xenotime & Churchite
Monazite, rhabdophane, xenotime & churchite: Vibrational spectroscopy of gadolinium phosphate polymorphs Nicolas Clavier, Adel Mesbah, Stephanie Szenknect, N. Dacheux To cite this version: Nicolas Clavier, Adel Mesbah, Stephanie Szenknect, N. Dacheux. Monazite, rhabdophane, xenotime & churchite: Vibrational spectroscopy of gadolinium phosphate polymorphs. Spec- trochimica Acta Part A: Molecular and Biomolecular Spectroscopy, Elsevier, 2018, 205, pp.85-94. 10.1016/j.saa.2018.07.016. hal-02045615 HAL Id: hal-02045615 https://hal.archives-ouvertes.fr/hal-02045615 Submitted on 26 Feb 2020 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. Monazite, rhabdophane, xenotime & churchite : vibrational spectroscopy of gadolinium phosphate polymorphs N. Clavier 1,*, A. Mesbah 1, S. Szenknect 1, N. Dacheux 1 1 ICSM, CEA, CNRS, ENSCM, Univ Montpellier, Site de Marcoule, BP 17171, 30207 Bagnols/Cèze cedex, France * Corresponding author: Dr. Nicolas CLAVIER ICSM, CEA, CNRS, ENSCM, Univ Montpellier Site de Marcoule BP 17171 30207 Bagnols sur Cèze France Phone : + 33 4 66 33 92 08 Fax : + 33 4 66 79 76 11 [email protected] - 1 - Abstract : Rare-earth phosphates with the general formula REEPO4·nH2O belong to four distinct structural types: monazite, rhabdophane, churchite, and xenotime. -
Metamorphism
Title page INTRODUCING METAMORPHISM Ian Sanders DUNEDIN EDINBURGH LONDON Contents Contents v Preface ix Acknowledgements x 1 Introduction 1 1.1 What is metamorphism? 1 1.1.1 Protoliths 1 1.1.2 Changes to the minerals 1 1.1.3 Changes to the texture 3 1.1.4 Naming metamorphic rocks 3 1.2 Metamorphic rocks – made under mountains 3 1.2.1 Mountain building 3 1.2.2 Directed stress, pressure and temperature in a mountain’s roots 4 1.2.3 Exhumation of a mountain’s roots 6 1.3 Metamorphism in local settings 6 1.3.1 Contact metamorphism 7 1.3.2 Hydrothermal metamorphism 7 1.3.3 Dynamic metamorphism 9 1.3.4 Shock metamorphism 9 2 The petrography of metamorphic rocks 11 2.1 Quartzite and metapsammite 11 2.1.1 Quartzite 11 2.1.2 Metapsammite 13 2.2 Metapelite 13 2.2.1 Slate 14 2.2.2 Phyllite and low-grade schist 16 2.2.3 Minerals and textures of medium-grade schist 17 2.2.4 The regional distribution of minerals in low- and medium-grade schist 20 2.2.5 Pelitic gneiss and migmatite 22 2.2.6 Metapelite in a contact aureole 23 2.2.7 The significance of Al2SiO5 for inferring metamorphic conditions 23 2.3 Marble 24 2.3.1 Pure calcite marble 24 2.3.2 Impure marble 26 2.3.3 Metasediments with mixed compositions 29 CONTENTS 2.4 Metabasite 30 2.4.1 Six kinds of metabasite from regional metamorphic belts 31 2.4.2 The ACF triangle for minerals in metabasites 36 2.4.3 P–T stability of metabasites, and metamorphic facies 38 vi 2.4.4 A metabasite made by contact metamorphism 40 2.5 Metagranite 41 2.5.1 Granitic gneiss and orthogneiss 41 2.5.2 Dynamic metamorphism -
An Overview of Phosphate Mining and Reclamation in Florida
An Overview of Phosphate Mining and Reclamation in Florida Casey Beavers Graduate Committee: Dr. Rex Ellis, Chairman Dr. Edward Hanlon Dr. Greg MacDonald April 2013 Introduction Phosphate has significant economic importance in Florida, yet 70% of surveyed Florida residents claimed that they were uninformed about the industry (Breeze, 2002). Residents who are aware of phosphate mining and fertilizer manufacturing in Florida tend to have strong opinions either in favor or in opposition to its presence. This document is meant to provide an overview of phosphate mining and reclamation in Florida to address the following questions: Why do we care about phosphate? Why is phosphate mined in Florida? How is phosphate mined? Who is impacted by Florida phosphate mining? What happens to the land after mining? What are some of the controversies of phosphate mining? The following topics will be discussed: phosphate as a resource, the geology of the Florida phosphate deposits, the economics of phosphate mining and fertilizer production, the history of mining in Florida, the regulations involved in mining, the process of phosphate mining, the reclamation or restoration of the mined areas, and lastly--the controversies surrounding phosphate mining in Florida. Phosphate Plants and animals are unable to live without phosphorus. It is an essential component in ATP, an energy-bearing compound that drives biochemical processes. Phosphorus also comprises much of the molecular composition of DNA, RNA, and phospholipids that are necessary to the function of cellular membranes. Nitrogen, another essential element, may be fixed from the atmosphere, meaning its supply is limitless. Phosphorus, present as phosphate minerals in the soil, is a non-renewable resource. -
Turquoise and Variscite by Dean Sakabe MEETING Wednesday
JANUARY 2015 - VOLUME 50, ISSUE 1 Meeting Times Turquoise and Variscite By Dean Sakabe MEETING We are starting the year off with Tur- Wednesday quoise and Variscite. January 28, 2015 Turquoise is a copper aluminum phosphate, whose name originated in 6:15-8:00 pm medieval Europe. What happened was Makiki District Park that traders from Turkey introduced the blue-green gemstone obtained Admin Building from Persia (the present day Iran) to Turquoise (Stabilized), Europeans. Who in turn associated Chihuahua, Mexico NEXT MONTH this stone with the Turkish traders, Tucson Gem & rather than the land of the stones origin. Hence they called this stone Mineral Show “Turceis” or, later in French “turquois.” Over time english speakers adopted this French word, but adding an “e” (Turquiose). The Spanish called this stone “Turquesa”. LAPIDARY The gemstone grade of Turquoise has a hardness of around 6, however Every Thursday the vast majority of turquoise falls in the softer 3–5 range. With the 6:30-8:30pm exception being the Turquoise from Cripple Creek, Colorado which is in the 7-8 range. Turquoise occurs in range of hues from sky blue to grey Makiki District Park -green. It is also found in arid places that has a high concentration of 2nd floor Arts and copper in the soil. The blue color is created by copper and the green Crafts Bldg by bivalent iron, with a little amount of chrome. Turquoise often, has veins or blotches running MEMBERSHIP through it, most often brown, but can be light gray or black DUE COSTS 2015 depending on where it was Single: $10.00 found. -
12018 Olivine Basalt 787 Grams
12018 Olivine Basalt 787 grams Figure 1: Original “mug shot” for 12018 PET showing main pieces and smaller pieces. NASA #S69-64111. Note the apparent encrustation. Introduction Mineralogy 12018 is an olivine basalt with an apparent Olivine: Kushiro et al. (1971) reported Fo -Fo for accumulation of mafic minerals. Figures 1 and 14 show 73 43 olivine phenocrysts. Walter et al. (1971) found that an apparent “encrustation” on the surface of 12018. olivine in 12018 had lower trace element contents (figure 5) than for other rocks. Petrography Walter et al. (1971) report that 12018 is comprised of Pyroxene: Walter et al. (1971), Brown et al. (1971) about 70% larger olivine and pyroxene crystals set in and Kushiro et al. (1971) determined that the pyroxene 20% variolitic matrix (figure 2). French et al. (1972) composition in 12018 did not trend towards Fe- describe the sample “as medium-grained with an enrichment (figure 4). average grain size of about 0.4 to 1.0 mm”. They found that 12018 was “virtually undeformed and no shock- Plagioclase: Plagioclase is An90-94 (Walter et al. 1971). metamorphic effects were observed.” The plagioclase in 12018 has the least trace element content (figure 6). 12018 also contains an association of fayalite-K-rich glass-phosphate that is interpreted as residual melt (El Goresy et al. 1971). Lunar Sample Compendium C Meyer 2011 Figure 3: Photomicrographsof 12018,9 showing highly mafic proportions. NASA S70-49554 and 555. Scale is 2.2 mm Figure 2: Photo of thin section of 12018 showing large cluster of mafic minerals. NASA # S70-30249.