Murun Massif, Aldan Shield of the Siberian Craton: a Simple Story for an Intricate Igneous Complex
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Mineral Processing
Mineral Processing Foundations of theory and practice of minerallurgy 1st English edition JAN DRZYMALA, C. Eng., Ph.D., D.Sc. Member of the Polish Mineral Processing Society Wroclaw University of Technology 2007 Translation: J. Drzymala, A. Swatek Reviewer: A. Luszczkiewicz Published as supplied by the author ©Copyright by Jan Drzymala, Wroclaw 2007 Computer typesetting: Danuta Szyszka Cover design: Danuta Szyszka Cover photo: Sebastian Bożek Oficyna Wydawnicza Politechniki Wrocławskiej Wybrzeze Wyspianskiego 27 50-370 Wroclaw Any part of this publication can be used in any form by any means provided that the usage is acknowledged by the citation: Drzymala, J., Mineral Processing, Foundations of theory and practice of minerallurgy, Oficyna Wydawnicza PWr., 2007, www.ig.pwr.wroc.pl/minproc ISBN 978-83-7493-362-9 Contents Introduction ....................................................................................................................9 Part I Introduction to mineral processing .....................................................................13 1. From the Big Bang to mineral processing................................................................14 1.1. The formation of matter ...................................................................................14 1.2. Elementary particles.........................................................................................16 1.3. Molecules .........................................................................................................18 1.4. Solids................................................................................................................19 -
Petroleum Geology and Resources of the Dnieper-Donets Basin, Ukraine and Russia
Petroleum Geology and Resources of the Dnieper-Donets Basin, Ukraine and Russia By Gregory F. Ulmishek U.S. Geological Survey Bulletin 2201-E U.S. Department of the Interior U.S. Geological Survey U.S. Department of the Interior Gale A. Norton, Secretary U.S. Geological Survey Charles G. Groat, Director Version 1.0, 2001 This publication is only available online at: http://geology.cr.usgs.gov/pub/bulletins/b2201-e/ Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement by the U.S. Government Manuscript approved for publication July 3, 2001 Published in the Central Region, Denver, Colorado Graphics by Susan Walden and Gayle M. Dumonceaux Photocomposition by Gayle M. Dumonceaux Contents Foreword ....................................................................................................................................... 1 Abstract.......................................................................................................................................... 1 Introduction .................................................................................................................................. 2 Province Overview ....................................................................................................................... 2 Province Location and Boundaries................................................................................. 2 Tectono-Stratigraphic Development ............................................................................. -
Micro-FTIR and EPMA Characterisation of Charoite from Murun Massif (Russia)
Hindawi Journal of Spectroscopy Volume 2018, Article ID 9293637, 6 pages https://doi.org/10.1155/2018/9293637 Research Article Micro-FTIR and EPMA Characterisation of Charoite from Murun Massif (Russia) Maria Lacalamita Dipartimento di Scienze della Terra, Università di Pisa, 56126 Pisa, Italy Correspondence should be addressed to Maria Lacalamita; [email protected] Received 21 December 2017; Accepted 20 February 2018; Published 3 April 2018 Academic Editor: Javier Garcia-Guinea Copyright © 2018 Maria Lacalamita. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Combined micro-Fourier transform infrared (micro-FTIR) and electron probe microanalyses (EPMA) were performed on a single crystal of charoite from Murun Massif (Russia) in order to get a deeper insight into the vibrational features of crystals with complex − structure and chemistry. The micro-FTIR study of a single crystal of charoite was collected in the 6000–400 cm 1 at room ° temperature and after heating at 100 C. The structural complexity of this mineral is reflected by its infrared spectrum. The analysis revealed a prominent absorption in the OH stretching region as a consequence of band overlapping due to a combination of H O and OH stretching vibrations. Several overtones of the O-H and Si-O stretching vibration bands were 2 − − observed at about 4440 and 4080 cm 1 such as absorption possibly due to the organic matter at about 3000–2800 cm 1.No significant change due to the loss of adsorbed water was observed in the spectrum obtained after heating. -
Pan-African Orogeny 1
Encyclopedia 0f Geology (2004), vol. 1, Elsevier, Amsterdam AFRICA/Pan-African Orogeny 1 Contents Pan-African Orogeny North African Phanerozoic Rift Valley Within the Pan-African domains, two broad types of Pan-African Orogeny orogenic or mobile belts can be distinguished. One type consists predominantly of Neoproterozoic supracrustal and magmatic assemblages, many of juvenile (mantle- A Kröner, Universität Mainz, Mainz, Germany R J Stern, University of Texas-Dallas, Richardson derived) origin, with structural and metamorphic his- TX, USA tories that are similar to those in Phanerozoic collision and accretion belts. These belts expose upper to middle O 2005, Elsevier Ltd. All Rights Reserved. crustal levels and contain diagnostic features such as ophiolites, subduction- or collision-related granitoids, lntroduction island-arc or passive continental margin assemblages as well as exotic terranes that permit reconstruction of The term 'Pan-African' was coined by WQ Kennedy in their evolution in Phanerozoic-style plate tectonic scen- 1964 on the basis of an assessment of available Rb-Sr arios. Such belts include the Arabian-Nubian shield of and K-Ar ages in Africa. The Pan-African was inter- Arabia and north-east Africa (Figure 2), the Damara- preted as a tectono-thermal event, some 500 Ma ago, Kaoko-Gariep Belt and Lufilian Arc of south-central during which a number of mobile belts formed, sur- and south-western Africa, the West Congo Belt of rounding older cratons. The concept was then extended Angola and Congo Republic, the Trans-Sahara Belt of to the Gondwana continents (Figure 1) although West Africa, and the Rokelide and Mauretanian belts regional names were proposed such as Brasiliano along the western Part of the West African Craton for South America, Adelaidean for Australia, and (Figure 1). -
Timing of Metamorphism in the Arabian-Nubian Shield Constrained by In-Situ U-Pb Dating of Accessory and Major Metamorphic Phases
Geophysical Research Abstracts Vol. 20, EGU2018-15645-1, 2018 EGU General Assembly 2018 © Author(s) 2018. CC Attribution 4.0 license. Timing of metamorphism in the Arabian-Nubian Shield constrained by in-situ U-Pb dating of accessory and major metamorphic phases Leo J. Millonig (1,2), Richard Albert Roper (1), Axel Gerdes (1), and Dov Avigad (2) (1) Department of Geosciences, Goethe University Frankfurt, Germany, (2) Institute of Earth Sciences, Hebrew University of Jerusalem, Israel The Arabian-Nubian Shield (ANS), which forms the northern branch of the East African Orogen, evolved from intra-oceanic island arcs into a mature continental crust in the course of ∼300 m.y. of Neoproterozoic Pan-African orogeny. The metapelitic Elat Schist in southern Israel records two metamorphic events that affected the northern part of the ANS, but the significance, extent and the exact timing of these events is controversially discussed. Previous geochronological studies on metamorphic monazite, in conjunction with field evidence, indicate that the main period of regional amphibolite-facies metamorphism occurred at ∼620 Ma, just prior to and coeval with regional-scale intrusions of late-orogenic granitoids. However, other field observations from the Elat area provide evidence that regional metamorphism also occurred prior to ∼705 Ma. This older age is inferred from an E- W trending, vertically-foliated, ∼705 Ma greenschist-facies dike swarm, which cross-cuts the shallow-dipping foliation of the garnet-bearing Elat Schist, thus indicating a more prolonged metamorphic evolution. In order to gain a more comprehensive understanding of the metamorphic history of this area, we apply in-situ U-Pb dating of monazite, garnet and staurolite to garnet-, garnet-staurolite-, and staurolite-bearing schists from the Elat area. -
Geology of Stone
The Geology of Stone An excerpt from the Dimension Stone Design Manual, Version VIII (May 2016) Produced and Published by the Marble Institute of America 380 East Lorain St. Oberlin, Ohio 44074 Telephone: 440-250-9222 Fax: 440-774-9222 www.naturalstoneinstitute.org © 2016 All rights reserved. No part of this document may be reproduced or transmitted in any form or by means electronic or mechanical, including photocopy, recording, or by an information storage and retrieval system, without written permission from the Natural Stone Institute. The geology of 2.0 STONE CATEGORIES Stone 2.1 Three general rock or stone categories are recognized according to their mode of 1.0 INTRODUCTION origin. This is a genetic classification, and it not only states how and under what general 1.1 Earth is geologically classified as a “stony conditions a stone was formed, but also implies planet,” as it is entirely stone (rock) of various a general compositional range. The basic stone mineral compositions and forms, excluding its groups are: water and atmosphere. 2.1.1 Igneous rock is formed by 1.2 Earth scientists prefer the term “rock,”1 solidification (cooling) or, in some cases, by while the commercial stone industry, prefers solid-state transformation3 of molten or semi- the term “stone”.2 Both words are correct in molten material in the Earth’s upper mantle or their respective frame of reference, and for crust into crystalline rock generally consisting practical purposes, interchangeable. Every of silicates (compounds with SiO4) and some type of rock or stone is composed of one or dark-colored accessory minerals such as iron more minerals. -
Thermochronology and Exhumation History of The
Thermochronology and Exhumation History of the Northeastern Fennoscandian Shield Since 1.9 Ga: Evidence From 40 Ar/ 39 Ar and Apatite Fission Track Data From the Kola Peninsula Item Type Article Authors Veselovskiy, Roman V.; Thomson, Stuart N.; Arzamastsev, Andrey A.; Botsyun, Svetlana; Travin, Aleksey V.; Yudin, Denis S.; Samsonov, Alexander V.; Stepanova, Alexandra V. Citation Veselovskiy, R. V., Thomson, S. N., Arzamastsev, A. A., Botsyun, S., Travin, A. V., Yudin, D. S., et al. (2019). Thermochronology and exhumation history of the northeastern Fennoscandian Shield since 1.9 Ga:evidence from 40Ar/39Ar and apatite fission track data from the Kola Peninsula. Tectonics, 38, 2317–2337.https:// doi.org/10.1029/2018TC005250 DOI 10.1029/2018tc005250 Publisher AMER GEOPHYSICAL UNION Journal TECTONICS Rights Copyright © 2019. American Geophysical Union. All Rights Reserved. Download date 01/10/2021 04:51:21 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/634481 RESEARCH ARTICLE Thermochronology and Exhumation History of the 10.1029/2018TC005250 Northeastern Fennoscandian Shield Since 1.9 Ga: Key Points: 40 39 • Since 1.9 Ga, the NE Fennoscandia Evidence From Ar/ Ar and Apatite Fission was characterized by a slow exhumation (1‐2 m/Myr) Track Data From the Kola Peninsula • Total denudation of the NE Roman V. Veselovskiy1,2 , Stuart N. Thomson3 , Andrey A. Arzamastsev4,5 , Fennoscandia since 1.9 Ga did not 6 7,8 7,8 9 exceed ~3‐5km Svetlana Botsyun , Aleksey V. Travin , Denis S. Yudin , Alexander V. Samsonov , • The Kola part of Fennoscandia and Alexandra V. -
Tectonic Evolution of the Mesozoic South Anyui Suture Zone, GEOSPHERE; V
Research Paper GEOSPHERE Tectonic evolution of the Mesozoic South Anyui suture zone, GEOSPHERE; v. 11, no. 5 eastern Russia: A critical component of paleogeographic doi:10.1130/GES01165.1 reconstructions of the Arctic region 18 figures; 5 tables; 2 supplemental files; 1 animation Jeffrey M. Amato1, Jaime Toro2, Vyacheslav V. Akinin3, Brian A. Hampton1, Alexander S. Salnikov4, and Marianna I. Tuchkova5 1Department of Geological Sciences, New Mexico State University, MSC 3AB, P.O. Box 30001, Las Cruces, New Mexico 88003, USA CORRESPONDENCE: [email protected] 2Department of Geology and Geography, West Virginia University, 330 Brooks Hall, P.O. Box 6300, Morgantown, West Virginia 26506, USA 3North-East Interdisciplinary Scientific Research Institute, Far East Branch, Russian Academy of Sciences, Magadan, Portovaya Street, 16, 685000, Russia CITATION: Amato, J.M., Toro, J., Akinin, V.V., Hamp- 4Siberian Research Institute of Geology, Geophysics, and Mineral Resources, 67 Krasny Prospekt, Novosibirsk, 630091, Russia ton, B.A., Salnikov, A.S., and Tuchkova, M.I., 2015, 5Geological Institute, Russian Academy of Sciences, Pyzhevskii per. 7, Moscow, 119017, Russia Tectonic evolution of the Mesozoic South Anyui su- ture zone, eastern Russia: A critical component of paleogeographic reconstructions of the Arctic region: ABSTRACT INTRODUCTION Geosphere, v. 11 no. 5, p. 1530–1564, doi: 10 .1130 /GES01165.1. The South Anyui suture zone consists of late Paleozoic–Jurassic ultra- The South Anyui suture zone (Fig. 1) is a remnant of a Mesozoic ocean Received 19 December 2014 mafic rocks and Jurassic–Cretaceous pre-, syn-, and postcollisional sedimen- basin that separated the Arctic Alaska–Chukotka microplate from Siberia Revision received 2 July 2015 tary rocks. -
Planet Earth
© Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION © Jones & Bartlett Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE OR DISTRIBUTION NOT FOR SALE OR DISTRIBUTION Planet Earth © Jones & Bartlett1 Learning, LLC © Jones & Bartlett Learning, LLC NOT FOR SALE ORFrom DISTRIBUTION the beginning of our species, we have soughtNOT to understandFOR SALE our surroundings,OR DISTRIBUTION whether that was the soil beneath our feet or the stars in the heavens. Above, the Milky Way shimmers in silent splendor above the Dolomites in northeastern Italy. The Milky Way is a gigantic galaxy consisting of billions of stars, some stars are forming today and others dying explosively. Many of these stars have their own systems of planets, moons, and comets orbiting them. Earth is but one planet of many. Our planet© Jones orbits a& star Bartlett that is on Learning, the fringes of LLC the galaxy. Only since the beginning© Jones of & Bartlett Learning, LLC space explorationNOT in FOR the 1960s SALE have OR we seen DISTRIBUTION our planet as it really is, a tiny blue sphereNOT suspended FOR SALE OR DISTRIBUTION in nearly empty space. -
Chapter 5 the Pre-Andean Phases of Construction of the Southern Andes Basement in Neoproterozoic-Paleozoic Times
133 Chapter 5 The Pre-Andean phases of construction of the Southern Andes basement in Neoproterozoic-Paleozoic times Nemesio Heredia; Joaquín García-Sansegundo; Gloria Gallastegui; Pedro Farias; Raúl E. Giacosa; Fernando D. Hongn; José María Tubía; Juan Luis Alonso; Pere Busquets; Reynaldo Charrier; Pilar Clariana; Ferrán Colombo; Andrés Cuesta; Jorge Gallastegui; Laura B. Giambiagi; Luis González-Menéndez; Carlos O. Limarino; Fidel Martín-González; David Pedreira; Luis Quintana; Luis Roberto Rodríguez- Fernández; Álvaro Rubio-Ordóñez; Raúl E. Seggiaro; Samanta Serra-Varela; Luis A. Spalletti; Raúl Cardó; Victor A. Ramos Abstract During the late Neoproterozoic and Paleozoic times, the Southern Andes of Argentina and Chile (21º-55º S) formed part of the southwestern margin of Gondwana. During this period of time, a set of continental fragments of variable extent and allochtony was successively accreted to that margin, resulting in six Paleozoic orogenies of different temporal and spatial extension: Pampean (Ediacaran-early Cambrian), Famatinian (Middle Ordovician-Silurian), Ocloyic (Middle Ordovician-Devonian), Chanic (Middle Devonian-early Carboniferous), Gondwanan (Middle Devonian-middle Permian) and Tabarin (late Permian-Triassic). All these orogenies culminate with collisional events, with the exception of the Tabarin and a part of the Gondwanan orogenies that are subduction-related. Keywords Paleozoic, Southern Andes, Pampean orogen, Ocloyic orogen, Famatinian orogen, Chanic orogen, Gondwanan orogen, Tabarin orogen. 133 134 1 Introduction In the southern part of the Andean Cordillera (21º-55º S, Fig. 1A) and nearby areas, there are Neoproterozoic (Ediacaran)-Paleozoic basement relicts of variable extension. This basement has been involved in orogenic events prior to the Andean orogeny, which is related to the current configuration of the Andean chain (active since the Cretaceous). -
GEOLOGY and DEVELOPMENT of the LOMONOSOV DIAMOND DEPOSIT, NORTHWESTERN RUSSIA Karen V
FEATURE AR ICLES GEOLOGY AND DEVELOPMENT OF THE LOMONOSOV DIAMOND DEPOSIT, NORTHWESTERN RUSSIA Karen V. Smit and Russell Shor The Siberian craton in Russia hosts many of the country’s famous diamond mines.The Lomonosov mine, however, occurs within the boundaries of a different craton—the Baltic shield, most of which lies in Eu- rope. Unlike many diamond mines in South Africa, Canada, and Siberia, the Lomonosov deposit is not in a stable Archean geologic setting. Similar to the Argyle diamond mine in Australia, Lomonosov is in a younger Proterozoic orogenic (or mountain-building) region. Fancy pink diamonds at both these lo- calities likely relate to these Proterozoic tectonic processes. Along with other diamond mines in Pro- terozoic geologic regions, the Lomonosov deposit (and its fancy-color diamond inventory) demonstrates that the diamond potential of these regions should not be overlooked. ussia has been a major diamond producer for In August 2016, the authors visited the Lomonosov more than half a century. Most of its diamond deposit to document this exciting new diamond local- Rmines occur in the semi-autonomous Sakha ity. The visit included tours of the kimberlite open-pit Republic within the geological bounds of the Siberian operations, the processing plant, and the preliminary craton. However, over the last 12 years, Alrosa, a pub- diamond sorting facilities in the city of Arkhangelsk. lic joint-stock company (with both government and The authors also visited Alrosa’s central diamond sort- private ownership) operating through its subsidiary ing and sales operation, the United Selling Organisa- Severalmaz, has started development and mining at tion (USO) in Moscow. -
Review of the Cambrian Pampean Orogeny of Argentina; a 2 Displaced Orogen Formerly Attached to the Saldania Belt of 3 South Africa? 4 5 César Casqueta*, Juán A
1 Review of the Cambrian Pampean orogeny of Argentina; a 2 displaced orogen formerly attached to the Saldania Belt of 3 South Africa? 4 5 César Casqueta*, Juán A. Dahlquistb, Sebastián O. Verdecchiab, Edgardo G. 6 Baldob, Carmen Galindoa, Carlos W. Rapelac, Robert, J. Pankhurstd, Matias 7 M. Moralesb, Juán A. Murrab, C. Mark Fanninge 8 9 a Departamento de Petrología y Geoquímica, Facultad de Ciencias Geológicas, Instituto de 10 Geología Económica (CSIC), Universidad Complutense, 28040 Madrid, Spain1 11 b Centro de Investigaciones en Ciencias de la Tierra (CICTERRA), CONICET, Universidad 12 Nacional de Córdoba, Av. Vélez Sarsfield 1611, Pab. Geol., X5016CGA Córdoba, Argentina 13 c Centro de Investigaciones Geológicas, CONICET, Universidad Nacional de la Plata, 1900 La 14 Plata, Argentina 15 d Visiting Research Associate, British Geological Survey, Keyworth, Nottingham NG12 5GG, 16 UK 17 e Research School of Earth Sciences, Australian National University, Canberra, ACT 0200, 18 Australia 19 20 21 Keywords: Pampean orogeny; Saldanian orogeny; Sierras Pampeanas; Gondwana; Mara 22 terrane; collisional orogeny 23 24 25 Abstract 26 27 The Pampean orogeny of northern Argentina resulted from Early Cambrian oblique 28 collision of the Paleoproterozoic MARA block, formerly attached to Laurentia, with the 29 Gondwanan Kalahari and Rio de la Plata cratons. The orogen is partially preserved 30 because it is bounded by the younger Córdoba Fault on the east and by the Los Túneles 31 Ordovician shear zone on the west. In this review we correlate the Pampean Belt with 32 the Saldania orogenic belt of South Africa and argue that both formed at an active 33 continental margin fed with sediments coming mainly from the erosion of the 34 Brasiliano–Pan-African and East African–Antarctica orogens between ca.