Harold Clayton Urey Papers

Total Page:16

File Type:pdf, Size:1020Kb

Harold Clayton Urey Papers http://oac.cdlib.org/findaid/ark:/13030/tf4c6006zq Online items available Harold Clayton Urey Papers Special Collections & Archives, UC San Diego Special Collections & Archives, UC San Diego Copyright 2005 9500 Gilman Drive La Jolla 92093-0175 [email protected] URL: http://libraries.ucsd.edu/collections/sca/index.html Harold Clayton Urey Papers MSS 0044 1 Descriptive Summary Languages: English Contributing Institution: Special Collections & Archives, UC San Diego 9500 Gilman Drive La Jolla 92093-0175 Title: Harold Clayton Urey Papers Identifier/Call Number: MSS 0044 Physical Description: 90.3 Linear feet(157 archives boxes, 34 flat boxes, 5 card file boxes, 1 carton, and 9 art bin items) Date (inclusive): 1924-1981 (bulk 1958-1978) Abstract: Papers of Harold Clayton Urey, Nobel Prize-winning chemist who contributed to significant advances in the fields of physical chemistry, geochemistry, lunar science, and astrochemistry. He received the Nobel Prize for Chemistry in 1934 for his discovery of deuterium, and made key scientific contributions to the development of the atomic bomb during World War II. The papers span the years 1929 to 1981 and contain significant correspondence with Urey's fellow scientists, including Albert Einstein, Enrico Fermi, J. Robert Oppenheimer, Leo Szilard, and Edward Teller. Scope and Content of Collection Papers of Harold Clayton Urey, Nobel Prize-winning chemist who contributed to significant advances in the fields of physical chemistry, geochemistry, lunar science, and astrochemistry. He received the Nobel Prize for Chemistry in 1934 for his discovery of deuterium, and made key scientific contributions to the development of the atomic bomb during World War II. The papers span the years 1929 to 1981 and contain significant correspondence with Urey's fellow scientists, including Albert Einstein, Enrico Fermi, J. Robert Oppenheimer, Leo Szilard, and Edward Teller, though the bulk of correspondence and writings date from the period 1958 to 1978, Urey's years at UC San Diego. The papers also contain a comprehensive collection of Urey's writings, including publications and speeches, and records of Urey's efforts in support of nuclear arms control and global cooperation. The collection does not contain significant materials relating to Urey's wartime work on the atomic bomb, records of his activities at Johns Hopkins and Columbia Universities, or documentation of his personal life. Arranged in ten series: 1) BIOGRAPHICAL MATERIALS, 2) CORRESPONDENCE, 3) SUBJECT FILES, 4) WRITINGS, 5) WRITINGS OF OTHERS, 6) PERSONAL EPHEMERA, 7) PHOTOGRAPHS, 8) AWARDS, 9) LUNAR ORBITER PHOTOS AND CHARTS, and 10) ORIGINALS OF PRESERVATION PHOTOCOPIES. Biography Harold Clayton Urey was a scientist of considerable scope whose discovery of deuterium helped him win the Nobel Prize for Chemistry in 1934. Urey also made fundamental contributions to the production of the atomic bomb through his development of the isotope separation processes for the Manhattan Project. In the period following World War II, Urey played an active part in advocating nuclear arms control, in promoting space exploration and in the development of the newly created campus of the University of California, San Diego. Born in Walkerton, Indiana, on April 29, 1893, Harold Urey was the son of Samuel Clayton and Cora Rebecca (Reinohl) Urey. His early schooling took place in rural Indiana. After graduating from high school he taught in country schools in Indiana and Montana for three years. In 1914 he entered Montana State University where he majored in zoology and minored in chemistry. He received a Bachelor of Science degree in 1917 and worked as an industrial chemist in Philadelphia until the end of World War I. He then returned to Montana as an instructor in the department of chemistry, where he remained for two years before pursuing a doctorate at the University of California, Berkeley. At Berkeley Urey studied thermodynamics and worked with Gilbert N. Lewis. Urey's doctoral research dealt with the rotational contributions to the heat capacities and entropies of gases, a subject not well understood at the time. He was able to form calculations which led directly to the present methods of calculating thermodynamic functions from spectroscopic data. In 1923 Urey attended the Institute for Theoretical Physics at the University of Copenhagen. There he studied under Niels Bohr, who was conducting seminal work in the theory of atomic structure. During this period Urey became involved in the international development of atomic and molecular physical science, and he made the acquaintance of prominent scientists of the time, including Werner Heisenberg, Wolfgang Pauli and Georg von Hevesy. Also in Europe Urey met Albert Einstein, who became a life-long friend. Dr. Urey returned to the United States in 1924, and for the next five years he served as Associate in Chemistry at Johns Hopkins University. From 1929 to 1934 he held the position of Associate Professor of Chemistry at Columbia University. His research during these years was principally devoted to experimental and theoretical work in spectroscopy and quantum mechanics. At this time he collaborated with A.E. Ruark in writing Atoms, Molecules and Quanta, one of the earliest books on quantum mechanics. This work eventually became one of the standard texts on the subject. Harold Clayton Urey Papers MSS 0044 2 On a visit to Seattle, Dr. Urey met Frieda Daum, a bacteriologist working in a doctor's office. Ms. Daum's sister had been a friend of Urey's at Montana. Married in 1926, Frieda and Harold Urey had four children: Gertrude Elizabeth, Frieda Rebecca, Mary Alice, and John Clayton. In 1931 Dr. Urey announced that he, together with George M. Murphy and Ferdinand G. Brickwedde, had discovered the existence of heavy water, in which the molecules consist of an atom of oxygen and two atoms of heavy hydrogen or deuterium. The identification of deuterium has been called one of the foremost achievements of modern science and has had a significant effect on research in physics, chemistry, biology, and medicine. As the discoverer of this isotope, Urey was awarded the Nobel Prize for Chemistry in 1934. His Nobel Prize address, delivered on February 14, 1935, was entitled, "Some Thermodynamic Properties of Hydrogen and Deuterium." Urey became the first editor of the Journal of Chemical Physics in 1933. The American Institute of Physics published this journal in response to the developing interest in sub-atomic and molecular spectroscopy and structure. Urey remained editor until 1941, establishing the journal as a leader in the newly created field of chemical physics. For the next decade, Dr. Urey occupied himself with the experimental and theoretical aspects of isotopic chemistry, and he soon became the leading authority on the subject. In 1934 he was appointed to the position of Professor of Chemistry at Columbia University, and from 1939 to 1942 he was the executive officer of the Chemistry Department at Columbia. Urey's scientific work became increasingly concerned with the separation of isotopes. In 1940 the United States government recruited him to serve as director of the program, established at Columbia, for separation of uranium isotopes and deuterium oxide production. During World War II, Dr. Urey applied his work in uranium isotope separation to the development of the atomic bomb. The U.S. Army assumed responsibility for atomic weapons development -- eventually called the Manhattan Project -- and General Leslie Groves served as overall director of the effort. Dr. Urey was appointed to the position of Director of War Research for the Special Alloy Materials (SAM) Laboratories at Columbia, where he worked on the uranium separation problem. He also served as one of three program chiefs in the Manhattan Project. Although awarded the Congressional Medal of Merit for his contributions, Urey's concern for the destructive consequences of atomic weapons, and his aversion to secret work, prompted him to leave the project. In response to the U.S. use of atomic bombs against Japan, Dr. Urey joined Albert Einstein, Leo Szilard, and other scientists to form the Emergency Committee of Atomic Scientists. This organization dedicated itself to enunciating the ethical and moral problems involved in the use of atomic weapons. Urey also joined with physicist Leo Szilard to oppose the U.S. military's administration of atomic power and to advocate limitations in the use of the atomic bomb. In 1945 Urey joined the faculty of the University of Chicago and contributed his efforts to the establishment of the Institute of Nuclear Studies, together with Enrico Fermi, Edward Teller, Leo Szilard, Joseph Mayer, Maria Goeppert Mayer, and others. At Chicago, Urey focused his attention on geochemistry and the problems of the cosmos. His work on the measurement of the paleotemperatures of ancient oceans is considered one of the great developments of the earth sciences. This work involved a wide scope of disciplines ranging from Urey's early biological interests to his studies of isotopic fractionation and the history of the earth. While at Chicago, Urey wrote The Planets: Their Origin and Development, in which he constructed the first systematic and detailed chronology of the origin of the earth, the moon, the meteorites, and the solar system. Urey participated in Operation Crossroads in 1946. This was a major atomic bomb test carried out by the U.S. government at Bikini Atoll in the Pacific. As a scientific observer, Urey joined other prominent scientists, including Roger Revelle, future director of Scripps Institution of Oceanography. In 1952 the trials of Ethel and Julius Rosenberg and Morton Sobell attracted Dr. Urey's attention. The Rosenbergs, accused of atomic espionage and given a highly publicized and controversial trial, were eventually sentenced to death. Sobell, tried as a co-conspirator, was given a long prison sentence. These cases became causes celebres during in the Postwar era. Reading the trial documents, Dr. Urey seriously questioned whether the Rosenbergs and Sobell had received justice from the U.S.
Recommended publications
  • Aitken Basin
    Geological and geochemical analysis of units in the South Pole – Aitken Basin A.M. Borst¹,², F.S. Bexkens¹,², B. H. Foing², D. Koschny² ¹ Department of Petrology, VU University Amsterdam ² SCI-S. Research and Scientific Support Department, ESA – ESTEC Student Planetary Workshop 10-10-2008 ESA/ESTEC The Netherlands The South Pole – Aitken Basin Largest and oldest Lunar impact basin - Diameter > 2500 km - Depth > 12 km - Age 4.2 - 3.9 Ga Formed during Late heavy bombardment? Window into the interior and evolution of the Moon Priority target for future sample return missions Digital Elevation Model from Clementine altimetry data. Produced in ENVI, 50x vertical exaggeration, orthographic projection centered on the far side. Red +10 km, purple/black -10km. (A.M.Borst et.al. 2008) 1 The Moon and the SPA Basin Geochemistry Iron map South Pole – Aitken Basin mafic anomaly • High Fe, Th, Ti and Mg abundances • Excavation of mafic deep crustal / upper mantle material Thorium map Clementine 750 nm albedo map from USGS From Paul Lucey, J. Geophys. Res., 2000 Map-a-Planet What can we learn from the SPA Basin? • Large impacts; Implications and processes • Volcanism; Origin, age and difference with near side mare basalts • Cratering record; Age, frequency and size distribution • Late Heavy Bombardment; Intensity, duration and origin • Composition of the deeper crust and possibly upper mantle 2 Topics of SPA Basin study 1) Global structure of the basin (F.S. Bexkens et al, 2008) • Rims, rings, ejecta distribution, subsequent craters modifications, reconstructive
    [Show full text]
  • Monadnock Vol. 45 | June 1971
    THE MONADNOCK I - L. .RK UNIVERSITY Vol. XLV )GRAPHICAL SOCIETY June, 1971 THE MQNADNOCK Volume XIN Editor, Edwin T. Wei5e, Jr. Aaooite Editor5 James FOnSeOa Kirsten Haring David Seairøn Photoqzapher, Ernie Wight ypists Ronnie Mason Phyllis sczynski 323812 ii ‘7f THE MONADNOCK CONTENTs . 2 DIRECT0I MESSAGE THE JESUITS IN NORTH AMERICA: A STUDY . IN ENVIRONMENTAL COCEUALIZATI Eenry Aay 4 STRUCTURE IN TRANSACTION SYSTEMS. .Christopher Clayton 9 CULTURE AND AGRICULTURE ON THE ANEPJCAN NTIER Brad Baltensperger 22 THE PROBABILISTIC APPROACH TO SPATIAL THEORY Kang-tsung Chang 30 AROHITECTURE AND GEOGRAPHICAL STUDIES: A REVIEW Stephen Hobart 36 AN ESSAY ON GROWTH POLE THEORY B. David Miller 40 MIND, MEANING, AND MILIEU: PSYCHOLOGICAL NEED AND DESIGRED ENVIRONMENTS Ernest A. Wight Jr 43 SPATIAL DYNAMICS IN CLASSICAL LOCATION THEORY Alfred Hecht 52 THE GRADUATE SCHOOL OF GEOGRAPHY 56 ALUMNI NEWS 65 A N(YTE ON THE QUESTIONNAIRE 80 :1 DIRECTOR’S MESSAGE This academic year is very special for Geography at Clark, marking the fiftieth year of the founding of the Graduate School of Geography by Wallace W. Atwood. Dedication of the new Geography facilities — with special recognition to the memory of John K. Wright, Historical Geographer and Geosophist, an adopted son of Clark — is one appropriate mode of celebration. Another mark of the occasion is the honor accorded to two major figures in American Geography: Clark could not have chosen two more distinguished geographers than Richard Hartshorne and Samuel Van Valkenburg on whom were bestowed .1 . - Honorary Doctorates of Law at the anniversary ceremonies of April .17th. Very different in their contributions and their characters, Richard Hartshorne provided American geography with its philosophic and method ological rationale and Dr.
    [Show full text]
  • Richard G. Hewlett and Jack M. Holl. Atoms
    ATOMS PEACE WAR Eisenhower and the Atomic Energy Commission Richard G. Hewlett and lack M. Roll With a Foreword by Richard S. Kirkendall and an Essay on Sources by Roger M. Anders University of California Press Berkeley Los Angeles London Published 1989 by the University of California Press Berkeley and Los Angeles, California University of California Press, Ltd. London, England Prepared by the Atomic Energy Commission; work made for hire. Library of Congress Cataloging-in-Publication Data Hewlett, Richard G. Atoms for peace and war, 1953-1961. (California studies in the history of science) Bibliography: p. Includes index. 1. Nuclear energy—United States—History. 2. U.S. Atomic Energy Commission—History. 3. Eisenhower, Dwight D. (Dwight David), 1890-1969. 4. United States—Politics and government-1953-1961. I. Holl, Jack M. II. Title. III. Series. QC792. 7. H48 1989 333.79'24'0973 88-29578 ISBN 0-520-06018-0 (alk. paper) Printed in the United States of America 1 2 3 4 5 6 7 8 9 CONTENTS List of Illustrations vii List of Figures and Tables ix Foreword by Richard S. Kirkendall xi Preface xix Acknowledgements xxvii 1. A Secret Mission 1 2. The Eisenhower Imprint 17 3. The President and the Bomb 34 4. The Oppenheimer Case 73 5. The Political Arena 113 6. Nuclear Weapons: A New Reality 144 7. Nuclear Power for the Marketplace 183 8. Atoms for Peace: Building American Policy 209 9. Pursuit of the Peaceful Atom 238 10. The Seeds of Anxiety 271 11. Safeguards, EURATOM, and the International Agency 305 12.
    [Show full text]
  • No. 40. the System of Lunar Craters, Quadrant Ii Alice P
    NO. 40. THE SYSTEM OF LUNAR CRATERS, QUADRANT II by D. W. G. ARTHUR, ALICE P. AGNIERAY, RUTH A. HORVATH ,tl l C.A. WOOD AND C. R. CHAPMAN \_9 (_ /_) March 14, 1964 ABSTRACT The designation, diameter, position, central-peak information, and state of completeness arc listed for each discernible crater in the second lunar quadrant with a diameter exceeding 3.5 km. The catalog contains more than 2,000 items and is illustrated by a map in 11 sections. his Communication is the second part of The However, since we also have suppressed many Greek System of Lunar Craters, which is a catalog in letters used by these authorities, there was need for four parts of all craters recognizable with reasonable some care in the incorporation of new letters to certainty on photographs and having diameters avoid confusion. Accordingly, the Greek letters greater than 3.5 kilometers. Thus it is a continua- added by us are always different from those that tion of Comm. LPL No. 30 of September 1963. The have been suppressed. Observers who wish may use format is the same except for some minor changes the omitted symbols of Blagg and Miiller without to improve clarity and legibility. The information in fear of ambiguity. the text of Comm. LPL No. 30 therefore applies to The photographic coverage of the second quad- this Communication also. rant is by no means uniform in quality, and certain Some of the minor changes mentioned above phases are not well represented. Thus for small cra- have been introduced because of the particular ters in certain longitudes there are no good determi- nature of the second lunar quadrant, most of which nations of the diameters, and our values are little is covered by the dark areas Mare Imbrium and better than rough estimates.
    [Show full text]
  • Glossary Glossary
    Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts.
    [Show full text]
  • Copyright by Paul Harold Rubinson 2008
    Copyright by Paul Harold Rubinson 2008 The Dissertation Committee for Paul Harold Rubinson certifies that this is the approved version of the following dissertation: Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War Committee: —————————————————— Mark A. Lawrence, Supervisor —————————————————— Francis J. Gavin —————————————————— Bruce J. Hunt —————————————————— David M. Oshinsky —————————————————— Michael B. Stoff Containing Science: The U.S. National Security State and Scientists’ Challenge to Nuclear Weapons during the Cold War by Paul Harold Rubinson, B.A.; M.A. Dissertation Presented to the Faculty of the Graduate School of The University of Texas at Austin in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy The University of Texas at Austin August 2008 Acknowledgements Thanks first and foremost to Mark Lawrence for his guidance, support, and enthusiasm throughout this project. It would be impossible to overstate how essential his insight and mentoring have been to this dissertation and my career in general. Just as important has been his camaraderie, which made the researching and writing of this dissertation infinitely more rewarding. Thanks as well to Bruce Hunt for his support. Especially helpful was his incisive feedback, which both encouraged me to think through my ideas more thoroughly, and reined me in when my writing overshot my argument. I offer my sincerest gratitude to the Smith Richardson Foundation and Yale University International Security Studies for the Predoctoral Fellowship that allowed me to do the bulk of the writing of this dissertation. Thanks also to the Brady-Johnson Program in Grand Strategy at Yale University, and John Gaddis and the incomparable Ann Carter-Drier at ISS.
    [Show full text]
  • Annual Report 2013.Pdf
    ATOMIC HERITAGE FOUNDATION Preserving & Interpreting Manhattan Project History & Legacy preserving history ANNUAL REPORT 2013 WHY WE SHOULD PRESERVE THE MANHATTAN PROJECT “The factories and bombs that Manhattan Project scientists, engineers, and workers built were physical objects that depended for their operation on physics, chemistry, metallurgy, and other nat- ural sciences, but their social reality - their meaning, if you will - was human, social, political....We preserve what we value of the physical past because it specifically embodies our social past....When we lose parts of our physical past, we lose parts of our common social past as well.” “The new knowledge of nuclear energy has undoubtedly limited national sovereignty and scaled down the destructiveness of war. If that’s not a good enough reason to work for and contribute to the Manhattan Project’s historic preservation, what would be? It’s certainly good enough for me.” ~Richard Rhodes, “Why We Should Preserve the Manhattan Project,” Bulletin of the Atomic Scientists, May/June 2006 Photographs clockwise from top: J. Robert Oppenheimer, General Leslie R. Groves pinning an award on Enrico Fermi, Leona Woods Marshall, the Alpha Racetrack at the Y-12 Plant, and the Bethe House on Bathtub Row. Front cover: A Bruggeman Ranch property. Back cover: Bronze statues by Susanne Vertel of J. Robert Oppenheimer and General Leslie Groves at Los Alamos. Table of Contents BOARD MEMBERS & ADVISORY COMMITTEE........3 Cindy Kelly, Dorothy and Clay Per- Letter from the President..........................................4
    [Show full text]
  • U.S. Government Printing Office Style Manual, 2008
    U.S. Government Printing Offi ce Style Manual An official guide to the form and style of Federal Government printing 2008 PPreliminary-CD.inddreliminary-CD.indd i 33/4/09/4/09 110:18:040:18:04 AAMM Production and Distribution Notes Th is publication was typeset electronically using Helvetica and Minion Pro typefaces. It was printed using vegetable oil-based ink on recycled paper containing 30% post consumer waste. Th e GPO Style Manual will be distributed to libraries in the Federal Depository Library Program. To fi nd a depository library near you, please go to the Federal depository library directory at http://catalog.gpo.gov/fdlpdir/public.jsp. Th e electronic text of this publication is available for public use free of charge at http://www.gpoaccess.gov/stylemanual/index.html. Use of ISBN Prefi x Th is is the offi cial U.S. Government edition of this publication and is herein identifi ed to certify its authenticity. ISBN 978–0–16–081813–4 is for U.S. Government Printing Offi ce offi cial editions only. Th e Superintendent of Documents of the U.S. Government Printing Offi ce requests that any re- printed edition be labeled clearly as a copy of the authentic work, and that a new ISBN be assigned. For sale by the Superintendent of Documents, U.S. Government Printing Office Internet: bookstore.gpo.gov Phone: toll free (866) 512-1800; DC area (202) 512-1800 Fax: (202) 512-2104 Mail: Stop IDCC, Washington, DC 20402-0001 ISBN 978-0-16-081813-4 (CD) II PPreliminary-CD.inddreliminary-CD.indd iiii 33/4/09/4/09 110:18:050:18:05 AAMM THE UNITED STATES GOVERNMENT PRINTING OFFICE STYLE MANUAL IS PUBLISHED UNDER THE DIRECTION AND AUTHORITY OF THE PUBLIC PRINTER OF THE UNITED STATES Robert C.
    [Show full text]
  • March 21–25, 2016
    FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk,
    [Show full text]
  • Appendix E Nobel Prizes in Nuclear Science
    Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2018 Contemporary Physics Education Project (CPEP) Appendix E Nobel Prizes in Nuclear Science Many Nobel Prizes have been awarded for nuclear research and instrumentation. The field has spun off: particle physics, nuclear astrophysics, nuclear power reactors, nuclear medicine, and nuclear weapons. Understanding how the nucleus works and applying that knowledge to technology has been one of the most significant accomplishments of twentieth century scientific research. Each prize was awarded for physics unless otherwise noted. Name(s) Discovery Year Henri Becquerel, Pierre Discovered spontaneous radioactivity 1903 Curie, and Marie Curie Ernest Rutherford Work on the disintegration of the elements and 1908 chemistry of radioactive elements (chem) Marie Curie Discovery of radium and polonium 1911 (chem) Frederick Soddy Work on chemistry of radioactive substances 1921 including the origin and nature of radioactive (chem) isotopes Francis Aston Discovery of isotopes in many non-radioactive 1922 elements, also enunciated the whole-number rule of (chem) atomic masses Charles Wilson Development of the cloud chamber for detecting 1927 charged particles Harold Urey Discovery of heavy hydrogen (deuterium) 1934 (chem) Frederic Joliot and Synthesis of several new radioactive elements 1935 Irene Joliot-Curie (chem) James Chadwick Discovery of the neutron 1935 Carl David Anderson Discovery of the positron 1936 Enrico Fermi New radioactive elements produced by neutron 1938 irradiation Ernest Lawrence
    [Show full text]
  • UC San Diego UC San Diego Electronic Theses and Dissertations
    UC San Diego UC San Diego Electronic Theses and Dissertations Title The new prophet : Harold C. Urey, scientist, atheist, and defender of religion Permalink https://escholarship.org/uc/item/3j80v92j Author Shindell, Matthew Benjamin Publication Date 2011 Peer reviewed|Thesis/dissertation eScholarship.org Powered by the California Digital Library University of California UNIVERSITY OF CALIFORNIA, SAN DIEGO The New Prophet: Harold C. Urey, Scientist, Atheist, and Defender of Religion A dissertation submitted in partial satisfaction of the requirements for the degree Doctor of Philosophy in History (Science Studies) by Matthew Benjamin Shindell Committee in charge: Professor Naomi Oreskes, Chair Professor Robert Edelman Professor Martha Lampland Professor Charles Thorpe Professor Robert Westman 2011 Copyright Matthew Benjamin Shindell, 2011 All rights reserved. The Dissertation of Matthew Benjamin Shindell is approved, and it is acceptable in quality and form for publication on microfilm and electronically: ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ Chair University of California, San Diego 2011 iii TABLE OF CONTENTS Signature Page……………………………………………………………………...... iii Table of Contents……………………………………………………………………. iv Acknowledgements………………………………………………………………….
    [Show full text]
  • Scientific References for Nobel Physics Prizes
    1 Scientific References for Nobel Physics Prizes © Dr. John Andraos, 2004 Department of Chemistry, York University 4700 Keele Street, Toronto, ONTARIO M3J 1P3, CANADA For suggestions, corrections, additional information, and comments please send e-mails to [email protected] http://www.chem.yorku.ca/NAMED/ 1901 - Wilhelm Conrad Roentgen "in recognition of the extraordinary services he has rendered by the discovery of the remarkable rays subsequently named after him." Roentgen X-ray Roentgen, W.C. Ann. Physik 1898, 64 , 1 Stanton, A. Science 1896, 3 , 227; 726 (translation) 1902 - Hendrik Antoon Lorentz and Pieter Zeeman "in recognition of the extraordinary service they rendered by their researches into the influence of magnetism upon radiation phenomena." Zeeman effect Zeeman, P., Verhandlungen der Physikalischen Gesellschaft zu Berlin 1896, 7 , 128 Zeeman, P., Nature 1897, 55 , 347 (translation by A. Stanton) 1903 - Antoine Henri Becquerel "in recognition of the extraordinary service he has rendered by his discovery of spontaneous radioactivity." Becquerel, A.H. Compt. Rend. 1896, 122 , 420; 501; 559; 689; 1086 Becquerel, A.H. Compt. Rend. 1896, 123 , 855 Becquerel, A.H. Compt. Rend. 1897, 124 , 444; 800 Becquerel, A.H. Compt. Rend. 1899, 129 , 996; 1205 Becquerel, A.H. Compt. Rend. 1900, 130 , 327; 809; 1583 Becquerel, A.H. Compt. Rend. 1900, 131 , 137 Becquerel, A.H. Compt. Rend. 1901, 133 , 977 1903 - Pierre Curie and Marie Curie, nee Sklodowska "in recognition of the extraordinary services they have rendered by their joint researches on the radiation phenomena discovered by Professor Henri Becquerel." Curie unit of radiation Curie, P; Desains, P., Compt. Rend.
    [Show full text]