Geochemical Features and Mineral Associations of Differentiated Rocks
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Paolovite Pd2sn C 2001-2005 Mineral Data Publishing, Version 1
Paolovite Pd2Sn c 2001-2005 Mineral Data Publishing, version 1 Crystal Data: Orthorhombic. Point Group: 2/m 2/m 2/m. As irregular grains embedded in other minerals. Twinning: Polysynthetic. Physical Properties: Hardness = n.d. VHN = 329–378 (10 g load). D(meas.) = n.d. D(calc.) = 11.08 Optical Properties: Opaque. Color: Lilac-rose. Luster: Metallic. Pleochroism: Dark lilac-rose to pale rose. R1–R2: (400) — , (420) 44.4–46.5, (440) 44.6–47.2, (460) 45.0–48.2, (480) 45.5–49.1, (500) 45.9–50.3, (520) 46.7–51.6, (540) 47.7–52.8, (560) 49.0–54.1, (580) 50.9–55.4, (600) 52.9–56.7, (620) 55.3–57.7, (640) 57.7–59.2, (660) 59.8–59.5, (680) 61.5–60.3, (700) 62.7–60.6 Cell Data: Space Group: P bnm. a = 8.11(1) b = 5.662(6) c = 4.324(2) Z = 4 X-ray Powder Pattern: Oktyabr deposit, Russia. 2.28 (100), 2.16 (70), 1.955 (50), 2.36 (40), 1.397 (40), 1.315 (40), 1.120 (40) Chemistry: (1) (2) (3) Pd 64.8 64.3 64.19 Pt 2.5 Sn 35.5 35.0 35.81 Sb 0.3 Bi 0.2 Total 103.3 99.3 100.00 (1) Oktyabr deposit, Russia; by electron microprobe, corresponding to (Pd1.98Pt0.04)Σ=2.02Sn0.98. (2) Western Platinum mine, South Africa; by electron microprobe, corresponding to Pd2.02Sn0.98. (3) Pd2Sn. Occurrence: In Cu–Ni sulfide ores; in cubanite–chalcopyrite, cubanite–talnakhite, and cubanite–mooihoekite assemblages (Oktyabr deposit, Russia). -
Podiform Chromite Deposits—Database and Grade and Tonnage Models
Podiform Chromite Deposits—Database and Grade and Tonnage Models Scientific Investigations Report 2012–5157 U.S. Department of the Interior U.S. Geological Survey COVER View of the abandoned Chrome Concentrating Company mill, opened in 1917, near the No. 5 chromite mine in Del Puerto Canyon, Stanislaus County, California (USGS photograph by Dan Mosier, 1972). Insets show (upper right) specimen of massive chromite ore from the Pillikin mine, El Dorado County, California, and (lower left) specimen showing disseminated layers of chromite in dunite from the No. 5 mine, Stanislaus County, California (USGS photographs by Dan Mosier, 2012). Podiform Chromite Deposits—Database and Grade and Tonnage Models By Dan L. Mosier, Donald A. Singer, Barry C. Moring, and John P. Galloway Scientific Investigations Report 2012-5157 U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior KEN SALAZAR, Secretary U.S. Geological Survey Marcia K. McNutt, Director U.S. Geological Survey, Reston, Virginia: 2012 This report and any updates to it are available online at: http://pubs.usgs.gov/sir/2012/5157/ For more information on the USGS—the Federal source for science about the Earth, its natural and living resources, natural hazards, and the environment—visit http://www.usgs.gov or call 1–888–ASK–USGS For an overview of USGS information products, including maps, imagery, and publications, visit http://www.usgs.gov/pubprod To order this and other USGS information products, visit http://store.usgs.gov Suggested citation: Mosier, D.L., Singer, D.A., Moring, B.C., and Galloway, J.P., 2012, Podiform chromite deposits—database and grade and tonnage models: U.S. -
Handbook of Iron Meteorites, Volume 3
Sierra Blanca - Sierra Gorda 1119 ing that created an incipient recrystallization and a few COLLECTIONS other anomalous features in Sierra Blanca. Washington (17 .3 kg), Ferry Building, San Francisco (about 7 kg), Chicago (550 g), New York (315 g), Ann Arbor (165 g). The original mass evidently weighed at least Sierra Gorda, Antofagasta, Chile 26 kg. 22°54's, 69°21 'w Hexahedrite, H. Single crystal larger than 14 em. Decorated Neu DESCRIPTION mann bands. HV 205± 15. According to Roy S. Clarke (personal communication) Group IIA . 5.48% Ni, 0.5 3% Co, 0.23% P, 61 ppm Ga, 170 ppm Ge, the main mass now weighs 16.3 kg and measures 22 x 15 x 43 ppm Ir. 13 em. A large end piece of 7 kg and several slices have been removed, leaving a cut surface of 17 x 10 em. The mass has HISTORY a relatively smooth domed surface (22 x 15 em) overlying a A mass was found at the coordinates given above, on concave surface with irregular depressions, from a few em the railway between Calama and Antofagasta, close to to 8 em in length. There is a series of what appears to be Sierra Gorda, the location of a silver mine (E.P. Henderson chisel marks around the center of the domed surface over 1939; as quoted by Hey 1966: 448). Henderson (1941a) an area of 6 x 7 em. Other small areas on the edges of the gave slightly different coordinates and an analysis; but since specimen could also be the result of hammering; but the he assumed Sierra Gorda to be just another of the North damage is only superficial, and artificial reheating has not Chilean hexahedrites, no further description was given. -
Accretion of Water in Carbonaceous Chondrites: Current Evidence and Implications for the Delivery of Water to Early Earth
ACCRETION OF WATER IN CARBONACEOUS CHONDRITES: CURRENT EVIDENCE AND IMPLICATIONS FOR THE DELIVERY OF WATER TO EARLY EARTH Josep M. Trigo-Rodríguez1,2, Albert Rimola3, Safoura Tanbakouei1,3, Victoria Cabedo Soto1,3, and Martin Lee4 1 Institute of Space Sciences (CSIC), Campus UAB, Facultat de Ciències, Torre C5-parell-2ª, 08193 Bellaterra, Barcelona, Catalonia, Spain. E-mail: [email protected] 2 Institut d’Estudis Espacials de Catalunya (IEEC), Edif.. Nexus, c/Gran Capità, 2-4, 08034 Barcelona, Catalonia, Spain 3 Departament de Química, Universitat Autònoma de Barcelona, 08193 Bellaterra, Catalonia, Spain. E-mail: [email protected] 4 School of Geographical and Earth Sciences, University of Glasgow, Gregory Building, Lilybank Gardens, Glasgow G12 8QQ, UK. Manuscript Pages: 37 Tables: 2 Figures: 10 Keywords: comet; asteroid; meteoroid; meteorite; minor bodies; primitive; tensile strength Accepted in Space Science Reviews (SPAC-D-18-00036R3, Vol. Ices in the Solar System) DOI: 10.1007/s11214-019-0583-0 Abstract: Protoplanetary disks are dust-rich structures around young stars. The crystalline and amorphous materials contained within these disks are variably thermally processed and accreted to make bodies of a wide range of sizes and compositions, depending on the heliocentric distance of formation. The chondritic meteorites are fragments of relatively small and undifferentiated bodies, and the minerals that they contain carry chemical signatures providing information about the early environment available for planetesimal formation. A current hot topic of debate is the delivery of volatiles to terrestrial planets, understanding that they were built from planetesimals formed under far more reducing conditions than the primordial carbonaceous chondritic bodies. -
A Sheffield Hallam University Thesis
An evaluation of river catchment quality in relation to restoration issues. AHMED, Badria S. Available from the Sheffield Hallam University Research Archive (SHURA) at: http://shura.shu.ac.uk/19204/ A Sheffield Hallam University thesis This thesis is protected by copyright which belongs to the author. The content must not be changed in any way or sold commercially in any format or medium without the formal permission of the author. When referring to this work, full bibliographic details including the author, title, awarding institution and date of the thesis must be given. Please visit http://shura.shu.ac.uk/19204/ and http://shura.shu.ac.uk/information.html for further details about copyright and re-use permissions. Return to Learning Centre of issue Fines are charged at 50p per hour 2 6 JUL J U X V U l 1 V /-L i REFERENCE ProQuest Number: 10694084 All rights reserved INFORMATION TO ALL USERS The quality of this reproduction is dependent upon the quality of the copy submitted. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. Also, if material had to be removed, a note will indicate the deletion. uest ProQuest 10694084 Published by ProQuest LLC(2017). Copyright of the Dissertation is held by the Author. All rights reserved. This work is protected against unauthorized copying under Title 17, United States Code Microform Edition © ProQuest LLC. ProQuest LLC. 789 East Eisenhower Parkway P.O. Box 1346 Ann Arbor, Ml 4 8 1 0 6 - 1346 An Evaluation of River Catchment Quality in Relation to Restoration Issues. -
Cu-Fe-S Phases in Lunar Rocks
American Mineralogist, Volume 58, pages 952-954, 1973 Cu-Fe-SPhases in LunarRocks LawnnNcn A. Tevronl Departmentol Geosciences,Purdue Uniuersity, Lalaye t te, I ndiana47 907 KBNNrrn L. Wnrrnus Departmentof Applied Earth Sciences,Stanlord Uniaersity, Stanford, Calilornia 943 0 5 Abstract The sulfide minerals reported to be present in lunar rocks include troilite, mackinawite, the discredited mineral "chalcopyrrhotite", sphalerite, chalcopyrite, and cubanite. Apollo 12 sam- ple l2D2l,l34 contains these last two minerals, and the first chemical analyses of the Cu-Fe-S phases are presented. These minerals occur along cracks and grain boundaries within troilite and are probably exsolution products formed at low temperatures (i.e, 100"-300'C) from a cupriferous troilite. Introduction Cu-Fe-S Minerals The opaqueminerals, although constituting only a "Chalcopyrrhotite", a discreditedmineral (Yund minor amount of a given sample,have proven useful and Kullerud, 1966; Cabri, 7967) , hasbeen reported as indicators of the genesisand cooling histories of from Apollo 12, 14, and 15 rocks (El Goresyet al, the lunar rocks (e.9., Reid, 1971; Taylor and Mc- l97la,b; 1972a,b). It wasdescribed as a yellowish, Callister, 19721,Taylor et al, I973b). The most chalcopyrite-coloredphase which appearsisotropic abundant opaque mineral is ilmenite, and many of and is alwaysfound within troilite. It is probablethat the oxide phasesin lunar rocks are unique (e.6'., this phase is either talnakhite, a mineral originally armalcolite as per Anderson et al, l97A). In addi- describedby Cabri (1967) andhaving a composition tion to native Fe metal, native Cu, and schreibersite, of CusFesSro(Cabri and Harris, 1971) near chal- the remaining opaqueminerals consistof sulfides. -
Chapter 9 Gold-Rich Porphyry Deposits: Descriptive and Genetic Models and Their Role in Exploration and Discovery
SEG Reviews Vol. 13, 2000, p. 315–345 Chapter 9 Gold-Rich Porphyry Deposits: Descriptive and Genetic Models and Their Role in Exploration and Discovery RICHARD H. SILLITOE 27 West Hill Park, Highgate Village, London N6 6ND, England Abstract Gold-rich porphyry deposits worldwide conform well to a generalized descriptive model. This model incorporates six main facies of hydrothermal alteration and mineralization, which are zoned upward and outward with respect to composite porphyry stocks of cylindrical form atop much larger parent plutons. This intrusive environment and its overlying advanced argillic lithocap span roughly 4 km vertically, an interval over which profound changes in the style and mineralogy of gold and associated copper miner- alization are observed. The model predicts a number of geologic attributes to be expected in association with superior gold-rich porphyry deposits. Most features of the descriptive model are adequately ex- plained by a genetic model that has developed progressively over the last century. This model is domi- nated by the consequences of the release and focused ascent of metalliferous fluid resulting from crys- tallization of the parent pluton. Within the porphyry system, gold- and copper-bearing brine and acidic volatiles interact in a complex manner with the stock, its wall rocks, and ambient meteoric and connate fluids. Although several processes involved in the evolution of gold-rich porphyry deposits remain to be fully clarified, the fundamental issues have been resolved to the satisfaction of most investigators. Explo- ration for gold-rich porphyry deposits worldwide involves geologic, geochemical, and geophysical work but generally employs the descriptive model in an unsophisticated manner and the genetic model hardly at all. -
Sulfide/Silicate Melt Partitioning During Enstatite Chondrite Melting
61st Annual Meteoritical Society Meeting 5255.pdf SULFIDE/SILICATE MELT PARTITIONING DURING ENSTATITE CHONDRITE MELTING. C. Floss1, R. A. Fogel2, G. Crozaz1, M. Weisberg2, and M. Prinz2, 1McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University, St. Louis MO 63130, USA ([email protected]), 2American Museum of Natural History, Department of Earth and Planetary Sciences, New York NY 10024, USA. Introduction: Aubrites are igneous rocks thought (present only in CaS-saturated charges) has a flat REE to have formed from an enstatite chondrite-like pattern with abundances of about 0.5 x CI. precursor [1]. Yet their origin remains poorly Discussion: Oldhamite/glass D values are close to understood, at least partly because of confusion over 1 for most REE, consistent with previous results the role played by sulfides, particularly oldhamite. [4,5,6], and significantly lower than those expected CaS in aubrites contains high rare earth element based on REE abundances in aubritic oldhamite. In (REE) abundances and exhibits a variety of patterns contrast, D values for FeS are surprisingly high (from [2] that reflect, to some extent, those seen in about 0.1 to 1), given the low REE abundances of oldhamite from enstatite chondrites [3]. However, natural troilite. FeS/silicate partition coefficients experimental work suggests that CaS/silicate melt reported by [5] are somewhat lower, but exhibit a REE partition coefficients are too low to account for similar pattern. Alkali loss from the charges, the high abundances observed [4,5] and do not explain resulting in Ca-enriched glass, might provide a partial the variable patterns. -
Washington State Minerals Checklist
Division of Geology and Earth Resources MS 47007; Olympia, WA 98504-7007 Washington State 360-902-1450; 360-902-1785 fax E-mail: [email protected] Website: http://www.dnr.wa.gov/geology Minerals Checklist Note: Mineral names in parentheses are the preferred species names. Compiled by Raymond Lasmanis o Acanthite o Arsenopalladinite o Bustamite o Clinohumite o Enstatite o Harmotome o Actinolite o Arsenopyrite o Bytownite o Clinoptilolite o Epidesmine (Stilbite) o Hastingsite o Adularia o Arsenosulvanite (Plagioclase) o Clinozoisite o Epidote o Hausmannite (Orthoclase) o Arsenpolybasite o Cairngorm (Quartz) o Cobaltite o Epistilbite o Hedenbergite o Aegirine o Astrophyllite o Calamine o Cochromite o Epsomite o Hedleyite o Aenigmatite o Atacamite (Hemimorphite) o Coffinite o Erionite o Hematite o Aeschynite o Atokite o Calaverite o Columbite o Erythrite o Hemimorphite o Agardite-Y o Augite o Calciohilairite (Ferrocolumbite) o Euchroite o Hercynite o Agate (Quartz) o Aurostibite o Calcite, see also o Conichalcite o Euxenite o Hessite o Aguilarite o Austinite Manganocalcite o Connellite o Euxenite-Y o Heulandite o Aktashite o Onyx o Copiapite o o Autunite o Fairchildite Hexahydrite o Alabandite o Caledonite o Copper o o Awaruite o Famatinite Hibschite o Albite o Cancrinite o Copper-zinc o o Axinite group o Fayalite Hillebrandite o Algodonite o Carnelian (Quartz) o Coquandite o o Azurite o Feldspar group Hisingerite o Allanite o Cassiterite o Cordierite o o Barite o Ferberite Hongshiite o Allanite-Ce o Catapleiite o Corrensite o o Bastnäsite -
MACKINAWITE from SOUTH AFRICA W. C J. Van RDNSBU*.O, Geological Surtey Oj Soulh Africa, Preloria, Soulh A.[Ri Co, L. Lrbnunsbyc
TI.IE AMERICAN MINERALOGIST, VOL 52, JULY AUGUST, 1967 MACKINAWITE FROM SOUTH AFRICA W. C J. vAN RDNSBU*.o,Geological Surtey oJ Soulh Africa, Preloria,Soulh A.[rico, AND L. LrBnuNsByc, Deparlment of Geology,Llnit:ersity of Pretoria, Pre!oria,Soul h Africa. ABSTRAcT Mackinawite has been identified in mafic and ultramafic rocks of the Bushveld igneous complex and Insizwa and also in the carbonatite and pegmatoid of Loolekop, Phalaborrva complex in South Africa. The mineral occurs predominantly as somewhat irregular to oriented intergrowths in pentlandite in all these occurrences and less commonly as regular oriented lamellae in chalcopyrite and rarely in cubanite. The textural evidence suggests that mackinawite may represent an exsolution product of pentlandite, chalcopyrite and cubanite. INrnonucrroN The iron sulphide, mackinawite was recently named in a paper by Evans, et al, (1964). Natural occurrencesof this mineral f rom Finland were describedby- Kouvo et al (1963)and from the Muskox intrusion in Canada by Chamberlain and Delabio (1965). During the presentinvestigation mackinawite was distinguishedfrom valleriite in the carbonatite and pegmatoid of Loolekop, Phalaborwa complex, in the Bushveld igneous complex, and from Insizwa, Cape Province.The mode of occurrenceof the mackinawite in the carbonatite difiers somewhatfrom that in the mafic rocks of Insizwa and the Bush- veld complex. MrNnn.q.rocv The physicaland optical propertiesof mackinawitefrom the Bushveid complex,Insizwa and Loolekop are very similar and are in closeagree- ment with the propertiesgiven for the same mineral from the Muskox intrusion by Chamberlain and Delabio (1965). The mineral takes a fairly good polish,particularly after buffing with a chromic oxide slurry. -
Copper in South Africa-Part 11
J. S. Afr. Inst. Min. Metall., vol. 85, no. 4. Apr. 1985. pp. 109-124 Copper in South Africa-Part 11 by C.O. BEALE* SYNOPSIS This, the second and final part of a review on the subject(the first part was published in the March issue of this Jouma/), deals in detail with the 9 copper-producing companies in the Republic of South Africa. These are The Phosphate Development Corporation, Prieska Copper Mines (Pty) Ltd, Black Mountain Mineral Development Co. (Pty) Ltd, Rustenburg Platinum Holdings Ltd, Impala Platinum Holdings Ltd, Western Platinum Ltd, The O'okiep Copper Co. Ltd, Messina Ltd, and Palabora Mining Co. Ltd. The following are described for each company: background, development, geology, mining, concentration, and current situation. The last-mentioned company, being South Africa's largest producer, is dealt with in greatest detail. SAMEVATTING . Hierdie tweede en slotdeel van 'n oorsig oor die onderwerp (die eerste deal het in die Maart-uitgawe van hierdie Tydskrif verskyn) handel in besonderhede oor die 9 koperproduserende maatskappye in the Republiek van Suid- Afrika. Hulle is die Fosfaat-ontginningskorporasie, Prieska Copper Mines (Pty) Ltd, Black Mountain Mineral Develop- ment Co. (Pty) Ltd, Rustenburg Platinum Holdings Ltd, Impala Platinum Holdings Ltd, Western Platinum Ltd, The O'okiep Copper Co. Ltd, Messina Ltd, en Palabora Mining Co. Ltd. Die volgende wQfd met betrekking tot elkeen van die maatskappye bespreek: agtergrond, ontwikkeling, geologie, mynbou, konsentrsie en huidige posisie. Die laasgenoemde maatskappy, wat Suid-Afrika se grootste produsent is, word in die meeste besonderhede bespreek. THE PHOSPHATE DEVELOPMENT CORP. CFOSKOR)' This Company was formed in 1951, on Government Foskor concentrate contributes significantly to the load initiative, to exploit the apatite (phosphate) resources of on Palabora's smelter and refinery, and also the annual the Phalaborwa Igneous Complex (Fig. -
Contrasting Styles of Lead-Zinc-Barium Mineralization in the Lower Benue Trough, Southeastern Nigeria
EARTH SCIENCES RESEARCH JOURNAL Earth Sci. Res. J. Vol. 21, No. 1 (March, 2017): 7 - 16 ORE DEPOSITS Contrasting styles of lead-zinc-barium mineralization in the Lower Benue Trough, Southeastern Nigeria Ifeanyi Andrew Oha*,1, Kalu Mosto Onuoha1, Silas Sunday Dada2 1Department of Geology, University of Nigeria, Nsukka. 2Kwara State University Malete *[email protected] ABSTRACT Keywords: Lead-Zinc-Barium mineralization, In the Lower Benue Trough of Southeastern Nigeria, lead-zinc-barium mineralization occurs as widely distributed Benue Trough, epigenetic, vein deposits. epigenetic fracture-controlled vein deposits which are restricted to Albian – Turonian sediments. Detailed field studies carried out in Ishiagu, Enyigba-Ameki-Ameri, Wanikande-Wanakom, and Gabu-Oshina which together constitute the four main areas of mineralization in the Lower Benue Trough, show that mineralization appears restricted to NW-SE and N-S fractures while the more common NE-SW fractures are barren. Apart from the Enyigba area, igneous bodies are found in the vicinity of the ore deposits while in the Wanikande area, barite veins and veinlets were observed to be closely interwoven with intrusive bodies. The host lithologies are highly varied, ranging from shales to siltstones, sandstones and occasionally igneous bodies. The ore assemblage also varies remarkably, with lead:zinc:barium ratios ranging from approximately 3:1:0 at Ishiagu, to 2:1:0 at Enyigba, 1:0:2 at Wanikande and nearly 100% barite at Gabu-Oshina. Thus, there is a remarkable increase in barite content from the southwest (Ishiagu) to the northeast (Gabu). The characteristics of the ore deposits roughly fit the base metal type mineralization known as clastic dominated lead-zinc-barium deposits.