Barite Scale Control at the Soultz-Sous-Forêts (France) EGS Site

Total Page:16

File Type:pdf, Size:1020Kb

Barite Scale Control at the Soultz-Sous-Forêts (France) EGS Site PROCEEDINGS, Thirty-Eighth Workshop on Geothermal Reservoir Engineering Stanford University, Stanford, California, February 24-26, 2014 SGP-TR-202 Barite Scale Control at the Soultz-sous-Forêts (France) EGS Site Julia Scheiber1, Andrea Seibt2, Johannes Birner3, Nicolas Cuenot1, Albert Genter1 and Wilfried Moeckes1 1GEIE, “Exploitation Minière de la Chaleur”, Route de Soultz, 67250 Kutzenhausen, France [email protected], [email protected], [email protected], [email protected] 2BWG Geochemische Beratung GmbH, Seestraße 7A, 17033 Neubrandenburg, Germany [email protected] 3GTN Geothermie Neubrandenburg GmbH, Seestraße 7A, 17033 Neubrandenburg, Germany [email protected] Keywords: barite, scaling, NORM, radiation protection, scale inhibitor, EGS ABSTRACT Scale formation in the surface and subsurface installations of the Soultz geothermal power plant affect negatively operational performance of the geothermal cycle. The Soultz EGS site operates a naturally fractured granitic reservoir percolated by Na-Ca-Cl brine with Total Dissolved Solids (TDS) up to 100 g/l. Geothermal brine is produced at 160°C/20 bars and re-injected at 70°C/18 bars. For power production, an Organic Rankine Cycle (ORC) is installed which includes three heat exchanger units, one evaporator and two preheaters. The heat transfer in this binary cycle is limited continuously by formation of scales in the tubular heat exchangers. Due to the temperature decrease of 90 K in the ORC heat exchanger system, strontium rich barite (Ba0.6Sr0.4SO4) becomes oversaturated and forms a homogenous scaling layer. Additionally, minor amounts of sulfide minerals like galena (PbS) are present. Those scales form an insulation layer inside of the heat exchanger tubes and decreases thereby efficiency of the heat transfer between geothermal and organic fluid. In consequence, cleaning operations for scale removal are required in regular time intervals to keep up efficiency of energy production. During cleaning and disposal operations, strict regulations for safety at work have to be followed due to radiation-protection regulations. The scales have to be classified as NORM (Naturally Occurring Radioactive Material) related to the presence of 226Ra and 210Pb, incorporated by chemical substitution in the scales. Moreover, the inner diameter of the reinjection wells decrease slowly but continuously by deposition of scales. Recently, well loggings proofed the existence of a progressing precipitation front inside of the injection wells versus depth which can reach the open-hole section as a function of injected brine volume and brine temperature. For reasons of safety at work and long-term power plant operation, the formation of barite needs to be inhibited continuously. Therefore, several inhibitors, based on phosphonic-acid, were tested in laboratory experiments. These studies included tests for calcium tolerance, effectiveness and dose rate adjustment by tube blocking tests. Out of these products, Diethylenetriaminepentakis (methylenephosphonic acid) (DTPMP), showed the best results for barite inhibition. Therefore it was selected for additional tests which investigated long-term efficiency, thermal stability and reservoir rock–inhibitor interactions. The inhibitor suppressed successfully barite formation for 24 h at 90°C in contact with reservoir rock. Geothermal fluids trapped within deep-seated fractured crystalline rocks from the Upper Rhine Valley must be carefully investigated in order to minimize scaling (sulfate, sulfide) in geothermal power plants and seriously limit the natural radioactivity associated with. At the Soultz site an inhibitor injection system was designed, installed and tested for continuously inhibitor injection and on-site efficiency tests showed very good results during short time tests. 1. INTRODUCTION The geothermal power plant of Soultz-sous-Forêts is located in the NE of France, 50 km NE of Strasbourg, at the western rim of the Upper Rhine Graben (URG). The Graben structure was formed by a Tertiary rift system accompanied with the formation of a thermal anomaly of increased heat flow. Within the geothermal anomaly of the URG are a few areas located where the temperature gradient is even higher in comparison to surrounding areas. Temperature measurements in petroleum wells at the Pechelbronn oil field indicated one of these very local temperature anomalies to be connected to the Soultz horst, first mentioned by Haas and Hoffmann, (1929). 1400 m of sediments, clays, sands, marls, lacrustine limestone and sandstone, cover the crystalline, granitic basement at the Soultz location, Schnaebele et al. (1948). The Paleozoic granitic basement includes two different types of granite. A grey porphyritic monzo-granite to about 4500 m depth and a fine grained two-mica granite deeper. At levels above 4500 m, the fine grained two mica granite intersects part-wise the monzo-granite as dike structures. Top of the crystalline basement is highly hydrothermally altered and fractured, Genter (1989). Fractures occur either as individual fractures or in clustered zones up to 10-20 m thickness, Genter et al. (2010). Primary minerals like biotite and plagioclase show intense alteration or replacement by secondary minerals like illite, chlorite, corrensite, tosudite, geodic quartz, calcite, dolomite and sulfides as well as locally kaolinite in the well GPK-1, Genter and Traineau (1992). The Soultz-sous-Forêts project started in 1987, with the aim to develop heat exploitation of deep reservoirs in hot dry rocks (HDR) by creating an artificial deep heat exchanger in a closed environment, Gérard and Kappelmeyer (1987). Therefore, one exploration well, EPS-1, and four deep wells, GPK-1 to GPK-4, were drilled between 1987 and 2005 down to the crystalline basement of the Rhine Graben. During drilling and well testing it became obvious that native brine was circulating through the fracture network of 1 Scheiber, Seibt, Birner, Cuenot, Genter and Moeckes the naturally fractured granite, Genter and Traineau (1992), Genter et al. (2010). The original HDR design was found to be obsolete. Nevertheless, permeability of the reservoir decreased with increasing depth and the initially low permeability was improved by hydraulic and chemical stimulations, creating an Enhanced Geothermal System (EGS), Gérard et al. (2006). The power plant, equipped with an Organic Rankine Cycle (ORC) unit, was designed and installed between 2007 and 2009 with an estimated capacity of 2.2 MWe. During power plant operation scale formation in the surface installations was observed and was recognized as serious issue for power plant operation and safety at work. 2. SCALE FORMATION AT THE SOULTZ EGS SITE The formation of scales in the surface and subsurface installations of the Soultz geothermal power plant, is connected with circulation and cooling of geothermal brine of high salinity, 97 g/l Total Dissolved Solids, Sanjuan et al. (2010), Seibt (2011). Scale deposition is strongly connected to the cold part of the power plant due to the significant temperature decrease of 90 K from 160˚C to 70˚C in the ORC tube heat exchanger. Temperature decrease affects the saturation state of dissolved minerals in the brine and strontium rich barite (Ba0.6Sr0.4SO4) becomes oversaturated and forms thin and brittle deposits, Figure 1. Additionally, minor fractions of galena (PbS) and trace amounts of mixed sulfides ((Fe,Sb,As)Sx) are formed, Sanjuan et al. (2011), Scheiber et al. (2012) and Nitschke (2012). Fine sulfide crystals cover the dominant barite layer, Figure 2. Sulfate and sulfide scales are deposited in the heat exchanger system, inside of equipment downstream to the injection well and even inside of the injection wells. Figure 1: Scale deposits in the ORC main heat exchanger cap. Thin and brittle barite scales were flushed out of the heat exchanger tubes into the cap during operation. (Picture: GEIE, 2011) Figure 2: Electron microscope exposure of a scale cross section in the back scattered mode (BSED). A thin layer of sulfides, approximately 5-10 μm, covers the surface of the dominating barite layer, which has an average thickness of 200 μm. The deposit was sampled from the main ORC heat exchanger. Picture from Scheiber et al. (2012). Barite and galena scales at Soultz have to be classified as NORM (Naturally Occurring Radioactive Material) due to the presence of 226Ra and 210Pb, Cuenot (2013). Those radionuclides accumulate in the scales by chemical substitution of 226Ra in barite/celestine and 210Pb in galena during mineral formation, e.g. Doerner and Hoskins (1925), Ceccarello et al. (2004), Curti et al. (2010), Kudryavskii and Rakhimova (2007) and Zielinski et al. (2001). The geothermal brine takes up radionuclides by rock-fluid interaction in the reservoir by natural fluid circulation in fractured granite which is a naturally radioactive rock, Degering and Köhler (2009), Degering and Köhler (2011), Eggeling (2010) and Eggeling et al. (2013). Three serious issues are connected with the precipitation of industrial scales, classified as NORM, in the surface installations of the Soultz power plant: First, scales act as an insulation material in the tube heat exchanger which leads to a significant efficiency decrease in the heat transfer. In consequence, extensive time and cost consuming cleaning procedures had to be applied. Second, specific protection regulation for workers and for scale disposal needed to be followed due to the presence of radionuclides in the scales. Those scales are considered as radioactive
Recommended publications
  • Barite (Barium)
    Barite (Barium) Chapter D of Critical Mineral Resources of the United States—Economic and Environmental Geology and Prospects for Future Supply Professional Paper 1802–D U.S. Department of the Interior U.S. Geological Survey Periodic Table of Elements 1A 8A 1 2 hydrogen helium 1.008 2A 3A 4A 5A 6A 7A 4.003 3 4 5 6 7 8 9 10 lithium beryllium boron carbon nitrogen oxygen fluorine neon 6.94 9.012 10.81 12.01 14.01 16.00 19.00 20.18 11 12 13 14 15 16 17 18 sodium magnesium aluminum silicon phosphorus sulfur chlorine argon 22.99 24.31 3B 4B 5B 6B 7B 8B 11B 12B 26.98 28.09 30.97 32.06 35.45 39.95 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 potassium calcium scandium titanium vanadium chromium manganese iron cobalt nickel copper zinc gallium germanium arsenic selenium bromine krypton 39.10 40.08 44.96 47.88 50.94 52.00 54.94 55.85 58.93 58.69 63.55 65.39 69.72 72.64 74.92 78.96 79.90 83.79 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 rubidium strontium yttrium zirconium niobium molybdenum technetium ruthenium rhodium palladium silver cadmium indium tin antimony tellurium iodine xenon 85.47 87.62 88.91 91.22 92.91 95.96 (98) 101.1 102.9 106.4 107.9 112.4 114.8 118.7 121.8 127.6 126.9 131.3 55 56 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 cesium barium hafnium tantalum tungsten rhenium osmium iridium platinum gold mercury thallium lead bismuth polonium astatine radon 132.9 137.3 178.5 180.9 183.9 186.2 190.2 192.2 195.1 197.0 200.5 204.4 207.2 209.0 (209) (210)(222) 87 88 104 105 106 107 108 109 110 111 112 113 114 115 116
    [Show full text]
  • Mineralogy of the Martian Surface
    EA42CH14-Ehlmann ARI 30 April 2014 7:21 Mineralogy of the Martian Surface Bethany L. Ehlmann1,2 and Christopher S. Edwards1 1Division of Geological & Planetary Sciences, California Institute of Technology, Pasadena, California 91125; email: [email protected], [email protected] 2Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109 Annu. Rev. Earth Planet. Sci. 2014. 42:291–315 Keywords First published online as a Review in Advance on Mars, composition, mineralogy, infrared spectroscopy, igneous processes, February 21, 2014 aqueous alteration The Annual Review of Earth and Planetary Sciences is online at earth.annualreviews.org Abstract This article’s doi: The past fifteen years of orbital infrared spectroscopy and in situ exploration 10.1146/annurev-earth-060313-055024 have led to a new understanding of the composition and history of Mars. Copyright c 2014 by Annual Reviews. Globally, Mars has a basaltic upper crust with regionally variable quanti- by California Institute of Technology on 06/09/14. For personal use only. All rights reserved ties of plagioclase, pyroxene, and olivine associated with distinctive terrains. Enrichments in olivine (>20%) are found around the largest basins and Annu. Rev. Earth Planet. Sci. 2014.42:291-315. Downloaded from www.annualreviews.org within late Noachian–early Hesperian lavas. Alkali volcanics are also locally present, pointing to regional differences in igneous processes. Many ma- terials from ancient Mars bear the mineralogic fingerprints of interaction with water. Clay minerals, found in exposures of Noachian crust across the globe, preserve widespread evidence for early weathering, hydrothermal, and diagenetic aqueous environments. Noachian and Hesperian sediments include paleolake deposits with clays, carbonates, sulfates, and chlorides that are more localized in extent.
    [Show full text]
  • I Identification and Characterization of Martian Acid-Sulfate Hydrothermal
    Identification and Characterization of Martian Acid-Sulfate Hydrothermal Alteration: An Investigation of Instrumentation Techniques and Geochemical Processes Through Laboratory Experiments and Terrestrial Analog Studies by Sarah Rose Black B.A., State University of New York at Buffalo, 2004 M.S., State University of New York at Buffalo, 2006 A thesis submitted to the Faculty of the Graduate School of the University of Colorado in partial fulfillment of the requirement for the degree of Doctor of Philosophy Department of Geological Sciences 2018 i This thesis entitled: Identification and Characterization of Martian Acid-Sulfate Hydrothermal Alteration: An Investigation of Instrumentation Techniques and Geochemical Processes Through Laboratory Experiments and Terrestrial Analog Studies written by Sarah Rose Black has been approved for the Department of Geological Sciences ______________________________________ Dr. Brian M. Hynek ______________________________________ Dr. Alexis Templeton ______________________________________ Dr. Stephen Mojzsis ______________________________________ Dr. Thomas McCollom ______________________________________ Dr. Raina Gough Date: _________________________ The final copy of this thesis has been examined by the signatories, and we find that both the content and the form meet acceptable presentation standards of scholarly work in the above mentioned discipline. ii Black, Sarah Rose (Ph.D., Geological Sciences) Identification and Characterization of Martian Acid-Sulfate Hydrothermal Alteration: An Investigation
    [Show full text]
  • Efflorescent Iron Sulfate Minerals: Paragenesis, Relative Stability, and Environmental Impact
    American Mineralogist, Volume 88, pages 1919–1932, 2003 Efflorescent iron sulfate minerals: Paragenesis, relative stability, and environmental impact JEANETTE K. JERZ* AND J. DONALD RIMSTIDT Department of Geological Sciences, Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061, U.S.A. ABSTRACT This study of a pyrrhotite-dominated massive sulfide deposit in the Blue Ridge province in south- western Virginia shows that sulfate minerals formed by the oxidation of the pyrrhotite transform from one to another by a combination of oxidation, dehydration, and neutralization reactions. Significant quantities of sulfate minerals occur in the underground adits (Area I) and under overhangs along the high sidewall of the adjoining open pit (Area II). Samples from this site were analyzed to determine mineralogy, equilibrium relative humidity, chemical composition, and acid generation potential. In Area I, pyrrhotite oxidizes to marcasite + melanterite, which eventually oxidizes to melanterite + sul- furic acid. Melanterite is extruded from the rocks as a result of the volume change associated with this reaction. It accumulates in piles where halotrichite, copiapite, and fibroferrite form. In Area II, FeSO4 solutions produced by pyrrhotite oxidation migrate to the exposed pit face, where they evaporate to form melanterite. The melanterite rapidly dehydrates to form rozenite, which falls into a pile at the base of the wall, where melanterite, copiapite, and halotrichite are present. The observed paragenesis a a can be understood using a log O2 – log H2O diagram that we developed from published thermody- namic data and observations of coexisting phases. Dissolution experiments showed that fibroferrite-rich samples had the highest acid producing po- tential, followed by copiapite-rich samples and then halotrichite-rich samples.
    [Show full text]
  • Mineralogical and Geochemical Indicators of Subaerial Weathering in the Pozzolane Rosse Ignimbrite (Alban Hills Volcanic District, Italy)
    Georgia State University ScholarWorks @ Georgia State University Geosciences Theses Department of Geosciences 4-27-2010 Mineralogical and Geochemical Indicators of Subaerial Weathering in the Pozzolane Rosse Ignimbrite (Alban Hills Volcanic District, Italy) Jennifer M. Dickie Georgia State University Follow this and additional works at: https://scholarworks.gsu.edu/geosciences_theses Part of the Geography Commons, and the Geology Commons Recommended Citation Dickie, Jennifer M., "Mineralogical and Geochemical Indicators of Subaerial Weathering in the Pozzolane Rosse Ignimbrite (Alban Hills Volcanic District, Italy)." Thesis, Georgia State University, 2010. https://scholarworks.gsu.edu/geosciences_theses/23 This Thesis is brought to you for free and open access by the Department of Geosciences at ScholarWorks @ Georgia State University. It has been accepted for inclusion in Geosciences Theses by an authorized administrator of ScholarWorks @ Georgia State University. For more information, please contact [email protected]. MINERALOGICAL AND GEOCHEMICAL INDICATORS OF SUBAERIAL WEATHERING IN THE POZZOLANE ROSSE IGNIMBRITE (ALBAN HILLS VOLCANIC DISTRICT, ITALY) by JENNIFER M. DICKIE Under the direction of Dr. Daniel Deocampo ABSTRACT The Pozzolane Rosse ignimbrite [PR] (457±4 ka) in the Alban Hills Volcanic District, Rome, Italy was exposed ~ 40 ka prior to a subsequent volcanic event which coverd it entirely. XRF, XRD, and clay separation results from PR samples from INGV and CA1 boreholes and Castel di Leva quarry show evidence of paleopedogenesis. All locations display loss of base cations, loss of K is consistent with XRD datat showing dissolution or alteration of leucite to analcime. Accumulation of Al and high L.O.I. support XRD evidence of 1:1 clay species at upper depth.
    [Show full text]
  • High Temperature Sulfate Minerals Forming on the Burning Coal Dumps from Upper Silesia, Poland
    minerals Article High Temperature Sulfate Minerals Forming on the Burning Coal Dumps from Upper Silesia, Poland Jan Parafiniuk * and Rafał Siuda Faculty of Geology, University of Warsaw, Zwirki˙ i Wigury 93, 02-089 Warszawa, Poland; [email protected] * Correspondence: j.parafi[email protected] Abstract: The subject of this work is the assemblage of anhydrous sulfate minerals formed on burning coal-heaps. Three burning heaps located in the Upper Silesian coal basin in Czerwionka-Leszczyny, Radlin and Rydułtowy near Rybnik were selected for the research. The occurrence of godovikovite, millosevichite, steklite and an unnamed MgSO4, sometimes accompanied by subordinate admixtures of mikasaite, sabieite, efremovite, langbeinite and aphthitalite has been recorded from these locations. Occasionally they form monomineral aggregates, but usually occur as mixtures practically impossible to separate. The minerals form microcrystalline masses with a characteristic vesicular structure resembling a solidified foam or pumice. The sulfates crystallize from hot fire gases, similar to high temperature volcanic exhalations. The gases transport volatile components from the center of the fire but their chemical compositions are not yet known. Their cooling in the near-surface part of the heap results in condensation from the vapors as viscous liquid mass, from which the investigated minerals then crystallize. Their crystallization temperatures can be estimated from direct measurements of the temperatures of sulfate accumulation in the burning dumps and studies of their thermal ◦ decomposition. Millosevichite and steklite crystallize in the temperature range of 510–650 C, MgSO4 Citation: Parafiniuk, J.; Siuda, R. forms at 510–600 ◦C and godovikovite in the slightly lower range of 280–450 (546) ◦C.
    [Show full text]
  • Carbonate, Sulfate and Phosphate Minerals Groups
    University of Anbar Collage of Science Department of Geology Minerals / 1st stage. Carbonate, Sulfate and Phosphate Minerals Groups Assistant lecturer Nazar Zaidan Khalaf Carbonate, Sulfate and phosphate minerals groups Lecture seven Carbonate mineral group 2- • The carbonate minerals contain the anionic complex CO3 , ,which is triangular in its coordination—i.e., with a carbon atom at the center and an oxygen atom at each of the corners of an equilateral triangle. These anionic groups are strongly bonded individual units and do not share oxygen atoms with one another. The triangular carbonate groups are the basic building units of all carbonate minerals and are largely responsible for the properties particular to the class. • The common anhydrous (water-free) carbonates are divided into three groups that differ in structure type: calcite, aragonite, and dolomite. • The copper carbonates azurite and malachite are the only notable hydrous varieties. • This anion group usually occurs in combination with calcium, sodium, uranium, iron, aluminum, manganese, barium, zinc, copper, lead, or the rare-earth elements. The carbonates tend to be soft, soluble in hydrochloric acid, and have a marked anisotropy in many physical properties (e.g., high birefringence) as a result of the planar structure of the carbonate ion. • There are approximately 80 known carbonate minerals, but most of them are rare. The commonest varieties, calcite, dolomite, and aragonite, are prominent constituents of certain rocks: calcite is the principal mineral of limestone's and marbles; dolomite occurs as a replacement for calcite in limestone's, and when this is extensive the rock is termed dolomite; and aragonite occurs in some recent sediments and in the shells of organisms that have calcareous skeletons.
    [Show full text]
  • SASSOLITE FRON{ the KRA\,IER BORATE DISTRICT, CALIFORNIA* Gnoncn L. Surrn .C.Nl Hv Ar-Uoxo,T U. S. Geologicol Suraey, Menlo Park
    THE AMERICAN MINERALOGIST. VOL. 43, NOVEMBER DECEMBER, 1958 SASSOLITE FRON{ THE KRA\,IER BORATE DISTRICT, CALIFORNIA* Gnoncn L. Surrn .c.NlHv Ar-uoxo,t U. S. GeologicolSuraey, Menlo Park,California, LNDDwrcur L. Sewvon, Trona, ColiJornia ABSTRACT Sassolite(H3BO:), previously unreported from the Kramer Borate District, California, was found near the base oI the borate-bearing shalesunderlying the ore body. Probertite, ulexite, colemanite, borax, and kernite, all founcl within the borate body, produce alkaline borate solutions (pH values of 8.3 to 9.2) when dissolveclin water. Thus the presence of sassolite,which forms in an acidic environment, is distinctly anomalous. Sodium, borate, and sulfate form the major poltions of the water-soluble materials in the sassolite-bearingrocks; calcium and iron form Jesserconcentrations. Efforescences of copiapite, mirabilite, sassolite, ulexite, borax and a little calcite and halite confirm the presenceof their constituents in the wall rocks The phase relationships between Na2SO4- Na2B4OrHaBOrH:O thus approximate the limiting conditions under which the sassolite probably formed. It is concluded that after lithification, sulfuric acid was formed by oxida- tion oI iron sulfidesby groundwater; this reacted rvith earlier formed borates to form acidic trorate solutions, and from these sassolite was deposited at some temperature belorv about 35". The optical properties and r-ray patterns of sassoliteand copiapite are givenl an analy- sis of the copiapite shor,vsit to contain iron, sulfate, and minor copper and phosphate. INrnoouctrox Sassolite,not previously reported from the Kramer Borate District, was found by two of the writers in the mine of the California Borate Company. Sassoliteis normally the product of an acidicenvironment.
    [Show full text]
  • Warren, J. K., 2010, Evaporites Through Time: Tectonic, Climatic And
    Earth-Science Reviews 98 (2010) 217–268 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Evaporites through time: Tectonic, climatic and eustatic controls in marine and nonmarine deposits John K. Warren Petroleum Geoscience Program, Department of Geology, Chulalongkorn University, 254 Phayathai Road, Pathumwan, Bangkok 10330, Thailand article info abstract Article history: Throughout geological time, evaporite sediments form by solar-driven concentration of a surface or Received 25 February 2009 nearsurface brine. Large, thick and extensive deposits dominated by rock-salt (mega-halite) or anhydrite Accepted 10 November 2009 (mega-sulfate) deposits tend to be marine evaporites and can be associated with extensive deposits of Available online 22 November 2009 potash salts (mega-potash). Ancient marine evaporite deposition required particular climatic, eustatic or tectonic juxtapositions that have occurred a number of times in the past and will so again in the future. Keywords: Ancient marine evaporites typically have poorly developed Quaternary counterparts in scale, thickness, evaporite deposition tectonics and hydrology. When mega-evaporite settings were active within appropriate arid climatic and marine hydrological settings then huge volumes of seawater were drawn into the subsealevel evaporitic nonmarine depressions. These systems were typical of regions where the evaporation rates of ocean waters were at plate tectonics their maximum, and so were centred on the past latitudinal equivalents of today's horse latitudes. But, like economic geology today's nonmarine evaporites, the location of marine Phanerozoic evaporites in zones of appropriate classification adiabatic aridity and continentality extended well into the equatorial belts. Exploited deposits of borate, sodium carbonate (soda-ash) and sodium sulfate (salt-cake) salts, along with evaporitic sediments hosting lithium-rich brines require continental–meteoric not marine-fed hydrologies.
    [Show full text]
  • The Stability of Sulfate and Hydrated Sulfate Minerals Near Ambient Conditions and Their Significance in Environmental and Plane
    Journal of Asian Earth Sciences 62 (2013) 734–758 Contents lists available at SciVerse ScienceDirect Journal of Asian Earth Sciences journal homepage: www.elsevier.com/locate/jseaes Review The stability of sulfate and hydrated sulfate minerals near ambient conditions and their significance in environmental and planetary sciences ⇑ I-Ming Chou a, , Robert R. Seal II a, Alian Wang b a U.S. Geological Survey, 954 National Center, Reston, VA 20192, USA b Department of Earth and Planetary Sciences and McDonnell Center for Space Sciences, Washington University, St. Louis, MO 63130, USA article info abstract Article history: Sulfate and hydrated sulfate minerals are abundant and ubiquitous on the surface of the Earth and also on Received 7 February 2012 other planets and their satellites. The humidity-buffer technique has been applied to study the stability of Received in revised form 5 November 2012 some of these minerals at 0.1 MPa in terms of temperature-relative humidity space on the basis of hydra- Accepted 12 November 2012 tion–dehydration reversal experiments. Updated phase relations in the binary system MgSO –H O are Available online 28 November 2012 4 2 presented, as an example, to show how reliable thermodynamic data for these minerals could be obtained based on these experimental results and thermodynamic principles. This approach has been Keywords: applied to sulfate and hydrated sulfate minerals of other metals, including Fe (both ferrous and ferric), Metal sulfate Zn, Ni, Co, Cd, and Cu. Hydrated sulfate minerals Humidity and temperature Metal–sulfate salts play important roles in the cycling of metals and sulfate in terrestrial systems, and Thermodynamics and kinetics the number of phases extends well beyond the simple sulfate salts that have thus far been investigated Terrestrial occurrence experimentally.
    [Show full text]
  • Bulletin of the Mineral Research and Exploration
    BULLETIN OF THE MINERAL RESEARCH AND EXPLORATION Foreign Edition 2014 149 CONTENTS Facies Characteristics And Control Mechanisms of Quaternary Deposits In The Lake Tuz Basin .......................................................................................................................Alper GÜRBÜZ and Nizamettin KAZANCI 1 Neotectonic-Period Characteristics, Seismicity, Geometry And Segmentation of The Tuz Gölü Fault Zone .............................................................................................................................Ak›n KÜRÇER and Y. Ergun GÖKTEN 19 Neogene Stratigraphy And Paleogeographic Evolution of The Karaburun Area, ‹zmir, Western Turkey ....................................................................................................................................................................Fikret GÖKTAfi 69 Benthic Foraminiferal Fauna of Malatya Oligo-Miocene Basin (Eastern Taurids, Eastern Turkey) .......................................................................................................................................................................Fatma GED‹K 93 Protolith Nature And Tectonomagmatic Features of Amphibolites From The Qushchi Area, West Azerbaijan, NW Iran ............................................................................................................................................................Mohssen MOAZZEN 139 Glauberite-Halite Association In Bozk›r Formation (Pliocene Çank›r›-Çorum Basin, Central Anatolia, Turkey) .....................................................................................................................................................................‹lhan
    [Show full text]
  • Sulfur on Mars from the Atmosphere to the Core Heather B
    Sulfur on Mars from the Atmosphere to the Core Heather B. Franz1, Penelope L. King2, and Fabrice Gaillard3 1NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 2Research School of Earth Sciences, Australian National University, Canberra ACT 2601, Australia 3CNRS-Université d’Orléans, ISTO, la rue de la Ferollerie, 45071 Orléans, France Abstract Observations of the martian surface from orbiting spacecraft and in situ landers and rovers, as well as analyses of martian meteorites in terrestrial laboratories, have consistently indicated that Mars is a sulfur-rich planet. The global inventory of sulfur, from the atmosphere to the core, carries widespread implications of potential geophysical, geochemical, climatological, and astrobiological significance. For example, the sulfur content of the core carries implications for core density; the speciation of igneous sulfur minerals reflects the oxidation state of the magma from which they formed; sulfur-bearing gases may have exerted control on the temperatures at the surface of early Mars; and the widespread availability of sulfur on Mars would have provided an abundant source for energy and nutrients to fuel sulfur-metabolizing microbes, such as those that arose during the emergence of primitive life on Earth. Here we provide an overview of martian sulfur and its relevance to these areas of interest, including a discussion of analytical techniques and results acquired by space missions and meteorite analyses to date. We review current studies modeling the potential effects of sulfur-bearing gases on the past martian climate and possible constraints on atmospheric composition implied by sulfur isotopic data. We also explore the importance of sulfur to the search for extinct or extant life on Mars.
    [Show full text]