A Review of the Stable-Isotope Geochemistry of Sulfate Minerals in Selected Igneous Environments and Related Hydrothermal Systems
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An Introduction to Isotopic Calculations John M
An Introduction to Isotopic Calculations John M. Hayes ([email protected]) Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA, 30 September 2004 Abstract. These notes provide an introduction to: termed isotope effects. As a result of such effects, the • Methods for the expression of isotopic abundances, natural abundances of the stable isotopes of practically • Isotopic mass balances, and all elements involved in low-temperature geochemical • Isotope effects and their consequences in open and (< 200°C) and biological processes are not precisely con- closed systems. stant. Taking carbon as an example, the range of interest is roughly 0.00998 ≤ 13F ≤ 0.01121. Within that range, Notation. Absolute abundances of isotopes are com- differences as small as 0.00001 can provide information monly reported in terms of atom percent. For example, about the source of the carbon and about processes in 13 13 12 13 atom percent C = [ C/( C + C)]100 (1) which the carbon has participated. A closely related term is the fractional abundance The delta notation. Because the interesting isotopic 13 13 fractional abundance of C ≡ F differences between natural samples usually occur at and 13F = 13C/(12C + 13C) (2) beyond the third significant figure of the isotope ratio, it has become conventional to express isotopic abundances These variables deserve attention because they provide using a differential notation. To provide a concrete the only basis for perfectly accurate mass balances. example, it is far easier to say – and to remember – that Isotope ratios are also measures of the absolute abun- the isotope ratios of samples A and B differ by one part dance of isotopes; they are usually arranged so that the per thousand than to say that sample A has 0.3663 %15N more abundant isotope appears in the denominator and sample B has 0.3659 %15N. -
Isotopegeochemistry Chapter4
Isotope Geochemistry W. M. White Chapter 4 GEOCHRONOLOGY III: OTHER DATING METHODS 4.1 COSMOGENIC NUCLIDES 4.1.1 Cosmic Rays in the Atmosphere As the name implies, cosmogenic nuclides are produced by cosmic rays colliding with atoms in the atmosphere and the surface of the solid Earth. Nuclides so created may be stable or radioactive. Radio- active 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 produced. Assuming that the production rate is constant through time, then the abundance of a cosmogenic nuclide in a reservoir isolated from cos- mic ray production is simply given by: −λt N = N0e 4.1 Hence if we know N0 and measure N, we can calculate t. Table 4.1 lists the radioactive cosmogenic nu- clides of principal interest. As we shall, cosmic ray interactions can also produce rare stable nuclides, and their abundance can also be used to measure geologic time. A number of different nuclear reactions create cosmogenic nuclides. “Cosmic rays” are high-energy (several GeV up to 1019 eV!) atomic nuclei, mainly of H and He (because these constitute most of the matter in the universe), but nuclei of all the elements have been recognized. To put these kinds of ener- gies in perspective, the previous gen- eration of accelerators for physics ex- Table 4.1. Data on Cosmogenic Nuclides periments, such as the Cornell Elec- -1 tron Storage Ring produce energies in Nuclide Half-life, years Decay constant, yr the 10’s of GeV (1010 eV); while 14C 5730 1.209x 10-4 CERN’s Large Hadron Collider, 3H 12.33 5.62 x 10-2 mankind’s most powerful accelerator, 10Be 1.500 × 106 4.62 x 10-7 located on the Franco-Swiss border 26Al 7.16 × 105 9.68x 10-5 near Geneva produces energies of 36Cl 3.08 × 105 2.25x 10-6 ~10 TeV range (1013 eV). -
Ichtj Annual Report 2002
NUCLEAR TECHNOLOGIES AND METHODS 121 PROCESS ENGINEERING CERAMIC MEMBRANES APPLIED FOR RADIOACTIVE WASTES PROCESSING Grażyna Zakrzewska-Trznadel, Marian Harasimowicz, Bogdan Tymiński, Andrzej G. Chmielewski Ceramic membranes (MEMBRALOX® and CeRAM use of different complexing agents are shown in INSIDE®) were used for filtration of liquid radio- Fig.1. Best removal of cobalt, europium and am- active wastes. The experimental runs with samples ericium was observed when chelating polymers of original radioactive wastes were carried out. The NaPAA or PEI were applied. Complexing with poly- waste was characterized by a relatively low salinity acrylic acid of molecular weight 1200 and 8000 did (<1 g/dm3), however, the specific radioactivity not result in sufficient increase of decontamina- was in the medium-level liquid waste range (~150 tion factor. For the membrane of 15 nm pore size, kBq/dm3). The main activity came from radioac- which was used in experiments, the proper molecu- tive cobalt and caesium, but also a significant lar weight of NaPAA was 15 000 or 30 000. In most amount of lanthanides and actinides was present. of experiments the removal of Eu-154 and Am-241 To enhance the separation, membrane filtration was complete (specific activity below the detection was combined with complexation (sole ultrafiltra- limit). Binding the caesium ions with all tested poly- tion gave decontamination factors in the range of mers gave rather poor results. The best complexing 1.1-1.7). Soluble polymers like polyacrylic acid agent for caesium was cobalt hexacyanoferrate, (PAA) derivatives of different average molecular which gave decontamination factors higher than weight, polyethylenimine (PEI) and cyanoferrates 100. -
Arizona Radiocarbon Dates X
[RADIOCARBON, VOL 23, No. 2, 1981, P 191-217] ARIZONA RADIOCARBON DATES X AUSTIN LONG and A B MULLER* Laboratory of Isotope Geochemistry, Department of Geosciences University of Arizona, Tucson, Arizona 85721 INTRODUCTION Routine radiocarbon analyses were last reported for the Laboratory of Isotope Geochemistry at the University of Arizona in 1971 (Haynes, Grey, and Long, 1971), and a special date list on packrat middens appeared in 1978 (Mead, Thompson, and Long, 1978). This list presents results obtained from our gas proportional counting facility before its major renovation and before the addition of a liquid scintillation counting system. The characteristics of these new systems will be de- scribed in the next date list. The majority of the results presented here are for extramural samples (submitted by researchers not associated with this laboratory) and were analyzed in conjunction with the service aspects of our facility. Results obtained from the radiocarbon analysis of bristlecone pine tree rings, which is the main thrust of our intramural research' on radio- carbon fluctuations in atmospheric CO2 and their relationship to climate, will be presented elsewhere. '4C All the ages reported here are based on the half-life of 5568 years, using 95% of the activity of NBS Oxalic Acid I as the modern value. The activities of samples of terrestrial organic material have been. normalized to account for the difference between the measured 613C and -25% PDB, as recommended by Stuiver and Polach (1977). Errors, based on counting statistics, are expressed as ± lo-; samples counting within'C 20- of background are reported as non-finite. -
Oxygen Isotope Geochemistry of Laurentide Ice-Sheet Meltwater Across Termination I
Quaternary Science Reviews 178 (2017) 102e117 Contents lists available at ScienceDirect Quaternary Science Reviews journal homepage: www.elsevier.com/locate/quascirev Oxygen isotope geochemistry of Laurentide ice-sheet meltwater across Termination I * Lael Vetter a, , Howard J. Spero a, Stephen M. Eggins b, Carlie Williams c, Benjamin P. Flower c a Department of Earth and Planetary Sciences, University of California Davis, Davis, CA 95616, USA b Research School of Earth Sciences, The Australian National University, Canberra 0200, ACT, Australia c College of Marine Sciences, University of South Florida, St. Petersburg, FL 33701, USA article info abstract Article history: We present a new method that quantifies the oxygen isotope geochemistry of Laurentide ice-sheet (LIS) Received 3 April 2017 meltwater across the last deglaciation, and reconstruct decadal-scale variations in the d18O of LIS Received in revised form meltwater entering the Gulf of Mexico between ~18 and 11 ka. We employ a technique that combines 1 October 2017 laser ablation ICP-MS (LA-ICP-MS) and oxygen isotope analyses on individual shells of the planktic Accepted 4 October 2017 18 foraminifer Orbulina universa to quantify the instantaneous d Owater value of Mississippi River outflow, which was dominated by meltwater from the LIS. For each individual O. universa shell, we measure Mg/ Ca (a proxy for temperature) and Ba/Ca (a proxy for salinity) with LA-ICP-MS, and then analyze the same 18 18 O. universa for d O using the remaining material from the shell. From these proxies, we obtain d Owater and salinity estimates for each individual foraminifer. Regressions through data obtained from discrete 18 18 core intervals yield d Ow vs. -
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. -
Planktonic Foraminiferal Mg/Ca As a Proxy for Past Oceanic Temperatures: a Methodological Overview and Data Compilation for the Last Glacial Maximum
ARTICLE IN PRESS Quaternary Science Reviews ] (]]]]) ]]]–]]] Planktonic foraminiferal Mg/Ca as a proxy for past oceanic temperatures: a methodological overview and data compilation for the Last Glacial Maximum Stephen Barkera,Ã, Isabel Cachob, Heather Benwayc, Kazuyo Tachikawad aDepartment of Earth Sciences, University of Cambridge, Downing Street, Cambridge CB2 3EQ, UK bCRG Marine Geosciences, Department of Stratigraphy, Paleontology and Marine Geosciences, University of Barcelona, C/Martı´ i Franque´s, s/n, E-08028 Barcelona, Spain cCollege of Oceanic and Atmospheric Sciences, 104 COAS, Administration Bldg., Oregon State University, Corvallis, OR 97331, USA dCEREGE, Europole de l’Arbois BP 80, 13545 Aix en Provence, France Abstract As part of the Multi-proxy Approach for the Reconstruction of the Glacial Ocean (MARGO) incentive, published and unpublished temperature reconstructions for the Last Glacial Maximum (LGM) based on planktonic foraminiferal Mg/Ca ratios have been synthesised and made available in an online database. Development and applications of Mg/Ca thermometry are described in order to illustrate the current state of the method. Various attempts to calibrate foraminiferal Mg/Ca ratios with temperature, including culture, trap and core-top approaches have given very consistent results although differences in methodological techniques can produce offsets between laboratories which need to be assessed and accounted for where possible. Dissolution of foraminiferal calcite at the sea-floor generally causes a lowering of Mg/Ca ratios. This effect requires further study in order to account and potentially correct for it if dissolution has occurred. Mg/Ca thermometry has advantages over other paleotemperature proxies including its use to investigate changes in the oxygen isotopic composition of seawater and the ability to reconstruct changes in the thermal structure of the water column by use of multiple species from different depth and or seasonal habitats. -
Formation of the Ice Core Isotopic Composition
Title Formation of the Ice Core Isotopic Composition Author(s) Ekaykin, Alexey A.; Lipenkov, Vladimir Ya. 低温科学, 68(Supplement), 299-314 Citation Physics of Ice Core Records II : Papers collected after the 2nd International Workshop on Physics of Ice Core Records, held in Sapporo, Japan, 2-6 February 2007. Edited by Takeo Hondoh Issue Date 2009-12 Doc URL http://hdl.handle.net/2115/45456 Type bulletin (article) Note IV. Chemical properties and isotopes File Information LTS68suppl_022.pdf Instructions for use Hokkaido University Collection of Scholarly and Academic Papers : HUSCAP Formation of the Ice Core Isotopic Composition Alcxcy A. Ekaykin·· •• , Vladimir Va. Lipcnkov" '" Hokkaido Ulliversily, Sapporo, Japan, ekaykill@aari,lIl1'.ru •• Arctic and All/arctic Research Instilule, SI. Petersburg. Russia. [email protected] Abstract: Main processes of the ice core isotopic In this work we overview the processes leading to the composition formation are overviewed. Theory of formation of the vertical profile of isotopic composition isotope-temperature relationship is discussed and of an ice core. using the extensive data set obtained at confirmed by a number of experimental data. The the Russian Vostok Station, central Antarctica. At first , factors related to wind-driven spatial snow we present the theoretical background of the redistribution and post-depositional isotopic changes relationship between the stable water isotope content in that may aller or weaken this relationship, are also precipitation and air temperature (Section 2). In Section considered. For high-resolution isotopic time-series 3 we consider the limitations of isotopic method due to obtatned at sites wilh low accumulation of snow, Ihe the fonnation of non-climatic noise as a result of signal-to-noise ratio is shown to be as low as 0.25, depositional and post-depositional processes in the which means that noise accounts for about 80 % of the upper snow thickness. -
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. -
Isotope Geochemistry I Lectures & Exercises
Tools and methods Geochronology Methods relying on the decay of naturally occurring radiogenic isotopes: Parent isotope Daughter isotope 1. Potassium-40 -> Argon-40 2. Rubidium-87 -> Strontium-87 3. Uranium-235 -> Lead-207 4. Uranium-238 -> Lead-206 5. Thorium-232 -> Lead-208 Radioactivity Natural and artificial radioactivity Natural radioactivity Isotopes that have been here since the earth formed: 238U, 235U, 232Th, 40K Isotopes produced by cosmic rays from the sun, i.e cosmogenic radionuclides: 14C, 10Be, 36Cl Synthetic radioisotopes Made in nuclear reactors when atoms are split (fission). Produced usinc cyclotrons, linear accererators... 39 39 K (n, p) Ar 19 18 The dawn of radiometric dating “U-Pb” method • Boltwood studied radioactive elements and found that Pb was always present in uranium and thorium ores. Pb must be the final product of the radioactive decay. • In 1907, he reasoned that since he knew the rate at which uranium breaks down (its half-life), he could use the proportion of lead in the uranium ores (chemical dating, isotopes not discovered yet) as a meter or clock. • His observations and calculations put Earth's age at 2.2 billion years. He accumulation method • Based on the fact that 235U, 238U and 232Th emit 7, 8 and 6 α-particles, resp. in their decay to Pb • U and Th concentration can be determined chemically and the current rate of He production can be calculated • The sample is heated to release He and the helium-retention age is calculated Radioactive decay half-lifes, T1/2 • if it is possible to determine the -
Sulfur and Lead Isotope Characteristics of the Greens Creek Polymetallic Massive Sulfide Deposit, Admiralty Island, Southeastern Alaska
Sulfur and Lead Isotope Characteristics of the Greens Creek Polymetallic Massive Sulfide Deposit, Admiralty Island, Southeastern Alaska By Cliff D. Taylor, Wayne R. Premo, and Craig A. Johnson Chapter 10 of Geology, Geochemistry, and Genesis of the Greens Creek Massive Sulfide Deposit, Admiralty Island, Southeastern Alaska Edited by Cliff D. Taylor and Craig A. Johnson Professional Paper 1763 U.S. Department of the Interior U.S. Geological Survey Contents Abstract .......................................................................................................................................................241 Introduction.................................................................................................................................................241 Regional and District Setting ...................................................................................................................242 Terrane Relationships ......................................................................................................................242 District Geology ..........................................................................................................................................242 Deposit Geology .........................................................................................................................................243 Mine Sequence Nomenclature and Stratigraphy .......................................................................243 Ore Types and Ore Mineralogy ................................................................................................................244 -
Pathways for Neoarchean Pyrite Formation Constrained by Mass
Pathways for Neoarchean pyrite formation constrained SPECIAL FEATURE by mass-independent sulfur isotopes James Farquhara,b,1, John Cliffb, Aubrey L. Zerklec, Alexey Kamyshnyd, Simon W. Poultone, Mark Clairef, David Adamsb, and Brian Harmsa aDepartment of Geology and Earth System Science Interdisciplinary Center, University of Maryland, College Park, MD 20742; bCentre for Microscopy and Microanalysis, University of Western Australia, Perth, WA 6009, Australia; cSchool of Civil Engineering and Geosciences, Newcastle University, Newcastle upon Tyne NE1 7RU, United Kingdom; dDepartment of Geological and Environmental Sciences, Faculty of Natural Sciences, Ben-Gurion University of the Negev, Beer Sheva 84105, Israel; eSchool of Earth and Environment, University of Leeds, Leeds LS2 9JT, United Kingdom; and fSchool of Environmental Sciences, University of East Anglia, Norwich NR4 7TJ, United Kingdom Edited by Mark H. Thiemens, University of California at San Diego, La Jolla, CA, and approved December 28, 2012 (received for review November 1, 2012) It is generally thought that the sulfate reduction metabolism is range of variability for Δ33S is significantly greater in samples older ancient and would have been established well before the Neo- than ∼2.4 Ga than in younger samples (e.g., compilation in refs. archean. It is puzzling, therefore, that the sulfur isotope record of 4 and 5). This observation has been linked to the production, the Neoarchean is characterized by a signal of atmospheric mass- transfer, and preservation of mass-independent sulfur isotope independent chemistry rather than a strong overprint by sulfate signals (presumably of atmospheric origin) early in Earth history. reducers. Here, we present a study of the four sulfur isotopes The production of this signal in the atmosphere and its subsequent obtained using secondary ion MS that seeks to reconcile a number transfer to the Earth surface is sensitive to atmospheric O2 levels of features seen in the Neoarchean sulfur isotope record.