A Review of in Situ Isotopic Studies of the Oklo and Bangombé Natural Fission Reactors Using Microbeam Analytical Techniques
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Download PDF About Minerals Sorted by Mineral Name
MINERALS SORTED BY NAME Here is an alphabetical list of minerals discussed on this site. More information on and photographs of these minerals in Kentucky is available in the book “Rocks and Minerals of Kentucky” (Anderson, 1994). APATITE Crystal system: hexagonal. Fracture: conchoidal. Color: red, brown, white. Hardness: 5.0. Luster: opaque or semitransparent. Specific gravity: 3.1. Apatite, also called cellophane, occurs in peridotites in eastern and western Kentucky. A microcrystalline variety of collophane found in northern Woodford County is dark reddish brown, porous, and occurs in phosphatic beds, lenses, and nodules in the Tanglewood Member of the Lexington Limestone. Some fossils in the Tanglewood Member are coated with phosphate. Beds are generally very thin, but occasionally several feet thick. The Woodford County phosphate beds were mined during the early 1900s near Wallace, Ky. BARITE Crystal system: orthorhombic. Cleavage: often in groups of platy or tabular crystals. Color: usually white, but may be light shades of blue, brown, yellow, or red. Hardness: 3.0 to 3.5. Streak: white. Luster: vitreous to pearly. Specific gravity: 4.5. Tenacity: brittle. Uses: in heavy muds in oil-well drilling, to increase brilliance in the glass-making industry, as filler for paper, cosmetics, textiles, linoleum, rubber goods, paints. Barite generally occurs in a white massive variety (often appearing earthy when weathered), although some clear to bluish, bladed barite crystals have been observed in several vein deposits in central Kentucky, and commonly occurs as a solid solution series with celestite where barium and strontium can substitute for each other. Various nodular zones have been observed in Silurian–Devonian rocks in east-central Kentucky. -
Subterranean Production of Neutrons, $^{39} $ Ar and $^{21} $ Ne: Rates
Subterranean production of neutrons, 39Ar and 21Ne: Rates and uncertainties Ondrejˇ Srˇ amek´ a,∗, Lauren Stevensb, William F. McDonoughb,c,∗∗, Sujoy Mukhopadhyayd, R. J. Petersone aDepartment of Geophysics, Faculty of Mathematics and Physics, Charles University, V Holeˇsoviˇck´ach 2, 18000 Praha 8, Czech Republic bDepartment of Chemistry and Biochemistry, University of Maryland, College Park, MD 20742, United States cDepartment of Geology, University of Maryland, College Park, MD 20742, United States dDepartment of Earth and Planetary Sciences, University of California Davis, Davis, CA 95616, United States eDepartment of Physics, University of Colorado Boulder, Boulder, CO 80309-0390, United States Abstract Accurate understanding of the subsurface production rate of the radionuclide 39Ar is necessary for argon dating tech- niques and noble gas geochemistry of the shallow and the deep Earth, and is also of interest to the WIMP dark matter experimental particle physics community. Our new calculations of subsurface production of neutrons, 21Ne, and 39Ar take advantage of the state-of-the-art reliable tools of nuclear physics to obtain reaction cross sections and spectra (TALYS) and to evaluate neutron propagation in rock (MCNP6). We discuss our method and results in relation to pre- vious studies and show the relative importance of various neutron, 21Ne, and 39Ar nucleogenic production channels. Uncertainty in nuclear reaction cross sections, which is the major contributor to overall calculation uncertainty, is estimated from variability in existing experimental and library data. Depending on selected rock composition, on the order of 107–1010 α particles are produced in one kilogram of rock per year (order of 1–103 kg−1 s−1); the number of produced neutrons is lower by ∼ 6 orders of magnitude, 21Ne production rate drops by an additional factor of 15–20, and another one order of magnitude or more is dropped in production of 39Ar. -
Monitored Natural Attenuation of Inorganic Contaminants in Ground
Monitored Natural Attenuation of Inorganic Contaminants in Ground Water Volume 3 Assessment for Radionuclides Including Tritium, Radon, Strontium, Technetium, Uranium, Iodine, Radium, Thorium, Cesium, and Plutonium-Americium EPA/600/R-10/093 September 2010 Monitored Natural Attenuation of Inorganic Contaminants in Ground Water Volume 3 Assessment for Radionuclides Including Tritium, Radon, Strontium, Technetium, Uranium, Iodine, Radium, Thorium, Cesium, and Plutonium-Americium Edited by Robert G. Ford Land Remediation and Pollution Control Division Cincinnati, Ohio 45268 and Richard T. Wilkin Ground Water and Ecosystems Restoration Division Ada, Oklahoma 74820 Project Officer Robert G. Ford Land Remediation and Pollution Control Division Cincinnati, Ohio 45268 National Risk Management Research Laboratory Office of Research and Development U.S. Environmental Protection Agency Cincinnati, Ohio 45268 Notice The U.S. Environmental Protection Agency through its Office of Research and Development managed portions of the technical work described here under EPA Contract No. 68-C-02-092 to Dynamac Corporation, Ada, Oklahoma (David Burden, Project Officer) through funds provided by the U.S. Environmental Protection Agency’s Office of Air and Radiation and Office of Solid Waste and Emergency Response. It has been subjected to the Agency’s peer and administrative review and has been approved for publication as an EPA document. Mention of trade names or commercial products does not constitute endorsement or recommendation for use. All research projects making conclusions or recommendations based on environmental data and funded by the U.S. Environmental Protection Agency are required to participate in the Agency Quality Assurance Program. This project did not involve the collection or use of environmental data and, as such, did not require a Quality Assurance Plan. -
Tracer Applications of Noble Gas Radionuclides in the Geosciences
To be published in Earth-Science Reviews Tracer Applications of Noble Gas Radionuclides in the Geosciences (August 20, 2013) Z.-T. Lua,b, P. Schlosserc,d, W.M. Smethie Jr.c, N.C. Sturchioe, T.P. Fischerf, B.M. Kennedyg, R. Purtscherth, J.P. Severinghausi, D.K. Solomonj, T. Tanhuak, R. Yokochie,l a Physics Division, Argonne National Laboratory, Argonne, Illinois, USA b Department of Physics and Enrico Fermi Institute, University of Chicago, Chicago, USA c Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York, USA d Department of Earth and Environmental Sciences and Department of Earth and Environmental Engineering, Columbia University, New York, USA e Department of Earth and Environmental Sciences, University of Illinois at Chicago, Chicago, IL, USA f Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, USA g Center for Isotope Geochemistry, Lawrence Berkeley National Laboratory, Berkeley, USA h Climate and Environmental Physics, Physics Institute, University of Bern, Bern, Switzerland i Scripps Institution of Oceanography, University of California, San Diego, USA j Department of Geology and Geophysics, University of Utah, Salt Lake City, USA k GEOMAR Helmholtz Center for Ocean Research Kiel, Marine Biogeochemistry, Kiel, Germany l Department of Geophysical Sciences, University of Chicago, Chicago, USA Abstract 81 85 39 Noble gas radionuclides, including Kr (t1/2 = 229,000 yr), Kr (t1/2 = 10.8 yr), and Ar (t1/2 = 269 yr), possess nearly ideal chemical and physical properties for studies of earth and environmental processes. Recent advances in Atom Trap Trace Analysis (ATTA), a laser-based atom counting method, have enabled routine measurements of the radiokrypton isotopes, as well as the demonstration of the ability to measure 39Ar in environmental samples. -
MINERALIZATION in the GOLD HILL MINING DISTRICT, TOOELE COUNTY, UTAH by H
MINERALIZATION IN THE GOLD HILL MINING DISTRICT, TOOELE COUNTY, UTAH by H. M. EI-Shatoury and J. A. Whelan UTAH GEOLOGICAL AND MINERALOGIC~4L SURVEY affiliated with THE COLLEGE OF MINES AND MINERAL INDUSTRIES University of Utah~ Salt Lake City~ Utah Bulletin 83 Price $2.25 March 1970 CONTENTS Page ABSTRACT. • • . • . • . • . • • . • . • . • • • . • • . • . • .. 5 INTRODUCTION 5 GENERAL GEOLOGY. .. 7 ECONOMIC GEOLOGY. 7 Contact Metasomatic Deposits. 11 Veins. • . 11 Quartz-Carbonate-Adularia Veins 11 Quartz Veins . 15 Calcite Veins. 15 Replacement Deposits . 15 Replacement Deposits in the Ochre Mountain Limestone 15 Replacement Deposits in the Quartz Monzonite 17 HYDROTHERMAL ALTERATION. 17 Alteration of Quartz Monzonite. • 17 Alteration of Limestones. 22 Alteration of the Manning Canyon Formation 23 Alteration of the Quartzite. 23 Alteration of Volcanic Rocks. 23 Alteration of Dike Rocks. 23 Alteration of Quartz-Carbonate Veins . 23 OXIDATION OF ORES. 23 Oxidation of the Copper-Lead-Arsenic-Zinc Replacement Deposits 24 Oxidation of Tungsten and Molybdenum Deposits. 24 Oxidation of the Lead-Zinc Deposits 25 MINERALOGY. 25 CONTROLS OF MINERAL LOCALIZATION 25 ZONAL ARRANGEMENT OF ORE DEPOSITS. 25 GENESIS OF ORE DEPOSITS. 29 DESCRIPTION OF PROPERTIES. 29 The Alvarado Mine. 29 The Cane Spring Mine 30 The Bonnemort Mine 32 The Rube Gold Mine . 32 The Frankie Mine 32 The Yellow Hammer Mine 33 The Rube Lead Mine . 34 FUTURE OF THE DISTRICT AND RECOMMENDATIONS. .. 34 ACKNOWLEDGMENTS. .. 36 REFERENCES. • . .. 36 2 ILLUSTRATIONS Page Frontis piece Figure I. Index map showing location and accessibility to the Gold Hill mining district, Utah . 4 2. Geologic map of Rodenhouse Wash area, showing occurrence of berylliferous quartz-carbonate-adularia veins and sample locations. -
Radiogenic Isotope Geochemistry
W. M. White Geochemistry Chapter 8: Radiogenic Isotope Geochemistry CHAPTER 8: RADIOGENIC ISOTOPE GEOCHEMISTRY 8.1 INTRODUCTION adiogenic isotope geochemistry had an enormous influence on geologic thinking in the twentieth century. The story begins, however, in the late nineteenth century. At that time Lord Kelvin (born William Thomson, and who profoundly influenced the development of physics and ther- R th modynamics in the 19 century), estimated the age of the solar system to be about 100 million years, based on the assumption that the Sun’s energy was derived from gravitational collapse. In 1897 he re- vised this estimate downward to the range of 20 to 40 million years. A year earlier, another Eng- lishman, John Jolly, estimated the age of the Earth to be about 100 million years based on the assump- tion that salts in the ocean had built up through geologic time at a rate proportional their delivery by rivers. Geologists were particularly skeptical of Kelvin’s revised estimate, feeling the Earth must be older than this, but had no quantitative means of supporting their arguments. They did not realize it, but the key to the ultimate solution of the dilemma, radioactivity, had been discovered about the same time (1896) by Frenchman Henri Becquerel. Only eleven years elapsed before Bertram Boltwood, an American chemist, published the first ‘radiometric age’. He determined the lead concentrations in three samples of pitchblende, a uranium ore, and concluded they ranged in age from 410 to 535 million years. In the meantime, Jolly also had been busy exploring the uses of radioactivity in geology and published what we might call the first book on isotope geochemistry in 1908. -
Nucleosynthesis
Nucleosynthesis Nucleosynthesis is the process that creates new atomic nuclei from pre-existing nucleons, primarily protons and neutrons. The first nuclei were formed about three minutes after the Big Bang, through the process called Big Bang nucleosynthesis. Seventeen minutes later the universe had cooled to a point at which these processes ended, so only the fastest and simplest reactions occurred, leaving our universe containing about 75% hydrogen, 24% helium, and traces of other elements such aslithium and the hydrogen isotope deuterium. The universe still has approximately the same composition today. Heavier nuclei were created from these, by several processes. Stars formed, and began to fuse light elements to heavier ones in their cores, giving off energy in the process, known as stellar nucleosynthesis. Fusion processes create many of the lighter elements up to and including iron and nickel, and these elements are ejected into space (the interstellar medium) when smaller stars shed their outer envelopes and become smaller stars known as white dwarfs. The remains of their ejected mass form theplanetary nebulae observable throughout our galaxy. Supernova nucleosynthesis within exploding stars by fusing carbon and oxygen is responsible for the abundances of elements between magnesium (atomic number 12) and nickel (atomic number 28).[1] Supernova nucleosynthesis is also thought to be responsible for the creation of rarer elements heavier than iron and nickel, in the last few seconds of a type II supernova event. The synthesis of these heavier elements absorbs energy (endothermic process) as they are created, from the energy produced during the supernova explosion. Some of those elements are created from the absorption of multiple neutrons (the r-process) in the period of a few seconds during the explosion. -
Lecture 12: Cosmogenic Isotopes In
Geol. 655 Isotope Geochemistry Lecture 12 Spring 2007 GEOCHRONOLOGY VIII: COSMOGENIC NUCLIDES INTRODUCTION As the name implies, cosmogenic nuclides are produced by cosmic rays, specifically by collisions with atoms in the atmosphere (and to a much lesser extent, the surface of the solid Earth). Nuclides so created may be stable or radioactive. Radioactive cosmogenic nuclides, like the U decay series nuclides, have half-lives sufficiently short that they would not exist in the Earth if they were not continually pro- duced. Assuming that the production rate is constant through time, then the abundance of a cos- mogenic nuclide in a reservoir isolated from cosmic ray production is simply given by: !"t N = N0e 12.1 Hence if we know N0 and measure N, we can calculate t. Table 12.1 lists the radioactive cosmogenic nuclides of principal interest. As we shall see in the next lecture, cosmic ray interactions can also produce TABLE 12.1. COSMOGENIC NUCLIDES OF GEOLOGICAL INTEREST rare stable nuclides, and their abun- Nuclide Half-life, years Decay constant, y-1 dance can also be used to measure 14C 5730 1.209x 10-3 geologic time. 3H 12.33 5.62 x 10-2 Cosmogenic nuclides are created 10Be 1.500 × 106 4.62 x 10-5 by a number of nuclear reactions 26Al 7.16 × 105 9.68x 10-5 with cosmic rays and by-products of 36Cl 3.08 × 105 2.25x 10-6 cosmic rays. “Cosmic rays” are high 32Si 276 2.51x 10-2 energy (several GeV up to 1019 eV!!) charged particles, mainly protons, or H nuclei (since, after all, H constitutes most of the matter in the universe), but nuclei of all the elements have been recognized. -
ADA Fluoridation Facts 2018
Fluoridation Facts Dedication This 2018 edition of Fluoridation Facts is dedicated to Dr. Ernest Newbrun, respected researcher, esteemed educator, inspiring mentor and tireless advocate for community water fluoridation. About Fluoridation Facts Fluoridation Facts contains answers to frequently asked questions regarding community water fluoridation. A number of these questions are responses to myths and misconceptions advanced by a small faction opposed to water fluoridation. The answers to the questions that appear in Fluoridation Facts are based on generally accepted, peer-reviewed, scientific evidence. They are offered to assist policy makers and the general public in making informed decisions. The answers are supported by over 400 credible scientific articles, as referenced within the document. It is hoped that decision makers will make sound choices based on this body of generally accepted, peer-reviewed science. Acknowledgments This publication was developed by the National Fluoridation Advisory Committee (NFAC) of the American Dental Association (ADA) Council on Advocacy for Access and Prevention (CAAP). NFAC members participating in the development of the publication included Valerie Peckosh, DMD, chair; Robert Crawford, DDS; Jay Kumar, DDS, MPH; Steven Levy, DDS, MPH; E. Angeles Martinez Mier, DDS, MSD, PhD; Howard Pollick, BDS, MPH; Brittany Seymour, DDS, MPH and Leon Stanislav, DDS. Principal CAAP staff contributions to this edition of Fluoridation Facts were made by: Jane S. McGinley, RDH, MBA, Manager, Fluoridation and Preventive Health Activities; Sharon (Sharee) R. Clough, RDH, MS Ed Manager, Preventive Health Activities and Carlos Jones, Coordinator, Action for Dental Health. Other significant staff contributors included Paul O’Connor, Senior Legislative Liaison, Department of State Government Affairs. -
Cosmogenic and Nucleogenic 21Ne in Quartz in a 28-Meter Sandstone Core from the Mcmurdo Dry Valleys, Antarctica
Cosmogenic and nucleogenic 21Ne in quartz in a 28-meter sandstone core from the McMurdo Dry Valleys, Antarctica Greg Balco∗,a, Pierre-Henri Blardb, David L. Shusterd,a, John O.H. Stonec, Laurent Zimmermannb a Berkeley Geochronology Center, 2455 Ridge Road, Berkeley CA 94709 USA b CRPG, CNRS-Universit´ede Lorraine, UMR 7358, 15 rue Notre Dame des Pauvres, 54501 Vandoeuvre-l`es-Nancy, France c Earth and Space Sciences, University of Washington, Seattle WA USA d Department of Earth and Planetary Science, 479 McCone Hall, University of California, Berkeley CA 94720, USA Abstract We measured concentrations of Ne isotopes in quartz in a 27.6-meter sandstone core from a low-erosion-rate site at 2183 m elevation at Beacon Heights in the Antarc- tic Dry Valleys. Surface concentrations of cosmogenic 21Ne indicate a surface exposure age of at least 4.1 Ma and an erosion rate no higher than ca. 14 cm Myr−1. 21Ne con- centrations in the upper few centimeters of the core show evidence for secondary spal- logenic neutron escape effects at the rock surface, which is predicted by first-principles models of cosmogenic-nuclide production but is not commonly observed in natural examples. We used a model for 21Ne production by various mechanisms fit to the ob- servations to distinguish cosmic-ray-produced 21Ne from nucleogenic 21Ne produced by decay of trace U and Th present in quartz, and also constrain rates of subsurface 21Ne production by cosmic-ray muons. Core samples have a quartz (U-Th)/Ne closure age, reflecting cooling below approximately 95°C, near 160 Ma, which is consistent with existing apatite fission-track data and the 183 Ma emplacement of nearby Ferrar dolerite intrusions. -
Tungsten Minerals and Deposits
DEPARTMENT OF THE INTERIOR FRANKLIN K. LANE, Secretary UNITED STATES GEOLOGICAL SURVEY GEORGE OTIS SMITH, Director Bulletin 652 4"^ TUNGSTEN MINERALS AND DEPOSITS BY FRANK L. HESS WASHINGTON GOVERNMENT PRINTING OFFICE 1917 ADDITIONAL COPIES OF THIS PUBLICATION MAY BE PROCURED FROM THE SUPERINTENDENT OF DOCUMENTS GOVERNMENT PRINTING OFFICE WASHINGTON, D. C. AT 25 CENTS PER COPY CONTENTS. Page. Introduction.............................................................. , 7 Inquiries concerning tungsten......................................... 7 Survey publications on tungsten........................................ 7 Scope of this report.................................................... 9 Technical terms...................................................... 9 Tungsten................................................................. H Characteristics and properties........................................... n Uses................................................................. 15 Forms in which tungsten is found...................................... 18 Tungsten minerals........................................................ 19 Chemical and physical features......................................... 19 The wolframites...................................................... 21 Composition...................................................... 21 Ferberite......................................................... 22 Physical features.............................................. 22 Minerals of similar appearance................................. -
Preparation and Solubility of Hydroxyapatite
JOURNAL O F RESEARC H of the National Bureau of Standards - A. Ph ys ics a nd Chemistry Vol. 72A, No. 6, N ovember- December 1968 Preparation and Solubility of Hydroxyapatite E. C. Moreno,* T. M. Gregory,* and W. E. Brown* Institute for Basic Standards, National Bureau of Standards, Washington, D.C. 20234 (August 2, 1968) Two portions of a syntheti c hydroxyapatite (HA), Ca" OH(PO'}J, full y characterized by x-ray, infrared, petrographi c, and chemi cal anal yses, were heated at 1,000 °C in air and steam atmospheres, respectively. Solubility isotherms for these two samples in the syste m Ca(OH}2 -H3PO,-H20 were determined in the pH range 5 to 7 by equilibrating the solids with dilute H3 PO. solutions. Both sam ples of HA disso lved stoichiometrically. The activity products (Ca + +)'( OH - ) (pO~f' and their standard errors-obtained by a least squares adjustment of the measurements (Ca and P concentrations and pH of the saturated solutions) subject to the conditions of electroneutralit y, constancy of the activity product, and stoichiometric dissolution - were 3.73 ± 0.5 x 10- 58 for the steam-h eated HA and 2_5, ± 0.4 x 10- 55 for the air-heated HA. Allowance was made in the calculations for the presence of the ion pairs [CaHPO. lo and [CaH2P04 1+ The hi gher solubility product for the air-heated HA is as cribed either to a change in the heat of formation brought about by partial dehydration or to a state of fine subdivision resulting from a disproportionation reacti on_ The solubility product constant s were used to cal culate the points of intersection (i.e_, sin gular points) of the two HA solubility isot herms with the isotherms of CaHPO.