Vannevar Bush and Ernest Lawrence – Two Key Individuals
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Building 9731 – Secret City Festival’S Y-12 Public Tour Or: Building 9731 to Be Featured in Secret City Festival's Public Tour (Title Provided by the Oak Ridger)
Building 9731 – Secret City Festival’s Y-12 public tour Or: Building 9731 to be featured in Secret City Festival's public tour (title provided by The Oak Ridger) In March 1943 the very first structure to be completed at the newly emerging Y-12 Electromagnetic Separation Plant was Building 9731. It was only a little over a month earlier that ground had been broken for the first of nine major buildings designed to hold cautrons (CALifornia University Cyclotron). But the real push had been to complete the construction of a smaller building, one with a high bay and especially designed to house four very special units of newly designed equipment using huge magnets. The Alpha Calutron magnets stand well over 20 feet tall and are still standing there today―the only ones in the world! For the first time ever, the public will have a chance to see these huge magnets and will also be able to tour inside historic Building 9731. This historic event is a part of the Secret City Festival this year. On Saturday, June 19, 2010, from 9:00 AM to 4:00 PM, a major part of the Y-12 public tour will include Building 9731. The public will be allowed to see inside the historic structure and view the magnets of both the two Alpha and two Beta calutrons. These calutron magnets have been designated as Manhattan Project Signature Artifacts by the Depart- ment of Energy’s Federal Preservation Officer in the DOE Office of History and Heritage Resources. The building is being submitted for Historical Landmark status on the National Register of Historic Places. -
Chapter 4. CLASSIFICATION UNDER the ATOMIC ENERGY
Chapter 4 CLASSIFICATION UNDER THE ATOMIC ENERGY ACT INTRODUCTION The Atomic Energy Act of 1946 was the first and, other than its successor, the Atomic Energy Act of 1954, to date the only U.S. statute to establish a program to restrict the dissemination of information. This Act transferred control of all aspects of atomic (nuclear) energy from the Army, which had managed the government’s World War II Manhattan Project to produce atomic bombs, to a five-member civilian Atomic Energy Commission (AEC). These new types of bombs, of awesome power, had been developed under stringent secrecy and security conditions. Congress, in enacting the 1946 Atomic Energy Act, continued the Manhattan Project’s comprehensive, rigid controls on U.S. information about atomic bombs and other aspects of atomic energy. That Atomic Energy Act designated the atomic energy information to be protected as “Restricted Data” and defined that data. Two types of atomic energy information were defined by the Atomic Energy Act of 1954, Restricted Data (RD) and a type that was subsequently termed Formerly Restricted Data (FRD). Before discussing further the Atomic Energy Act of 1946 and its unique requirements for controlling atomic energy information, some of the special information-control activities that accompanied the research, development, and production efforts that led to the first atomic bomb will be mentioned. Realization that an atomic bomb was possible had a profound impact on the scientists who first became aware of that possibility. The implications of such a weapon were so tremendous that the U.S. scientists conducting the initial, basic research related to nuclear fission voluntarily restricted the publication of their scientific work in this area. -
Harry Truman, the Atomic Bomb and the Apocalyptic Narrative
Volume 5 | Issue 7 | Article ID 2479 | Jul 12, 2007 The Asia-Pacific Journal | Japan Focus The Decision to Risk the Future: Harry Truman, the Atomic Bomb and the Apocalyptic Narrative Peter J. Kuznick The Decision to Risk the Future: Harry stressed that the future of mankind would be Truman, the Atomic Bomb and theshaped by how such bombs were used and Apocalyptic Narrative subsequently controlled or shared.[3] Truman recalled Stimson “gravely” expressing his Peter J. Kuznick uncertainty about whether the U.S. should ever use the bomb, “because he was afraid it was so I powerful that it could end up destroying the whole world.” Truman admitted that, listening In his personal narrative Atomic Quest, Nobel to Stimson and Groves and reading Groves’s Prize-winning physicist Arthur Holly Compton, accompanying memo, he “felt the same who directed atomic research at the University fear.”[4] of Chicago’s Metallurgical Laboratory during the Second World War, tells of receiving an urgent visit from J. Robert Oppenheimer while vacationing in Michigan during the summer of 1942. Oppenheimer and the brain trust he assembled had just calculated the possibility that an atomic explosion could ignite all the hydrogen in the oceans or the nitrogen in the atmosphere. If such a possibility existed, Compton concluded, “these bombs must never be made.” As Compton said, “Better to accept the slavery of the Nazis than to run a chance of drawing the final curtain on mankind.”[1] Certainly, any reasonable human being could be expected to respond similarly. Three years later, with Hitler dead and the Nazis defeated, President Harry Truman faced Truman and Byrnes en route to Potsdam, July a comparably weighty decision. -
Fleming Vs. Florey: It All Comes Down to the Mold Kristin Hess La Salle University
The Histories Volume 2 | Issue 1 Article 3 Fleming vs. Florey: It All Comes Down to the Mold Kristin Hess La Salle University Follow this and additional works at: https://digitalcommons.lasalle.edu/the_histories Part of the History Commons Recommended Citation Hess, Kristin () "Fleming vs. Florey: It All Comes Down to the Mold," The Histories: Vol. 2 : Iss. 1 , Article 3. Available at: https://digitalcommons.lasalle.edu/the_histories/vol2/iss1/3 This Paper is brought to you for free and open access by the Scholarship at La Salle University Digital Commons. It has been accepted for inclusion in The iH stories by an authorized editor of La Salle University Digital Commons. For more information, please contact [email protected]. The Histories, Vol 2, No. 1 Page 3 Fleming vs. Florey: It All Comes Down to the Mold Kristen Hess Without penicillin, the world as it is known today would not exist. Simple infections, earaches, menial operations, and diseases, like syphilis and pneumonia, would possibly all end fatally, shortening the life expectancy of the population, affecting everything from family-size and marriage to retirement plans and insurance policies. So how did this “wonder drug” come into existence and who is behind the development of penicillin? The majority of the population has heard the “Eureka!” story of Alexander Fleming and his famous petri dish with the unusual mold growth, Penicillium notatum. Very few realize that there are not only different variations of the Fleming discovery but that there are also other people who were vitally important to the development of penicillin as an effective drug. -
Ira Sprague Bowen Papers, 1940-1973
http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington. -
Atomic Physics & Quantum Effects
KEY CONCEPTS ATOMIC PHYSICS & QUANTUM EFFECTS 1. PHOTONS & THE PHOTOELECTRIC EFFECT Max Planck explained blackbody radiation with his quantum hypothesis, which states that the energy of a thermal oscillator, Eosc, is not continuous, but instead is a discrete quantity given by the equation: Eosc = nhf n = 1, 2, 3,... where f is the frequency and h is a constant now known as Planck’s constant. Albert Einstein extended the idea by adding that all emitted radiation is quantized. He suggested that light is composed of discrete quanta, rather than of waves. According to his theory, each particle of light, known as a photon, has an energy E given by: E = hf Einstein’s theory helped him explain a phenomenon known as the photoelectric effect, in which a photon of light strikes a photosensitive material and causes an electron to be ejected from the material. A photocell constructed from photosensitive material can produce an electrical current when light shines on it. The kinetic energy, K, of a photoelectron displaced by a photon of energy, hf, is given by: K = hf - φ where the work function, φ, is the minimum energy needed to free the electron from the photosensitive material. No photoemission occurs if the frequency of the incident light falls below a certain cutoff frequency – or threshold frequency – given by: φ f0 = h Einstein's theory explained several aspects of the photoelectric effect that could not be explained by classical theory: • The kinetic energy of photoelectrons is dependent on the light’s frequency. • No photoemission occurs for light below a certain threshold frequency. -
Cave Archaeology and the NSS: 1941–2006
George Crothers, P. Willey, and Patty Jo Watson – Cave archaeology and the NSS: 1941–2006. Journal of Cave and Karst Studies, v. 69, no. 1, p. 27–34. CAVE ARCHAEOLOGY AND THE NSS: 1941–2006 GEORGE CROTHERS1,P.WILLEY2, AND PATTY JO WATSON3 Abstract: Like most other branches of speleology, cave archaeology in the U.S. grew and developed significantly during the mid to late twentieth century. Originally viewed as marginal to mainstream Americanist archaeology, pursuit of prehistoric and historic archaeology underground is now widely accepted as making valuable contributions to knowledge of human past. The National Speleological Society played a central role in that development and continues to do so. We outline the establishment and growth of cave archaeology in North America, with special emphasis on relations between the NSS and archaeology performed in dark zone, deep cave interiors. INTRODUCTION 1920s and 1930s by ‘‘the Caveman,’’ as Neville was often called. The NSS has directly participated in cave archaeology Despite interest in cave archaeology within the NSS through cooperation, education, and conservation. Mem- governance and some portion of the membership during bers of the Society have made notable contributions to the the first few decades after the organization was formed, science by reporting the location of archaeological sites, systematic, long-term archaeological research by pro- participating in their investigation, and by equipping fessional archaeologists in the dark zones of big caves in scientists with the techniques and technology needed to the Americas did not get underway until the 1960s. There work safely in the cave environment (Damon, 1991, p. -
The Development of Military Nuclear Strategy And
The Development of Military Nuclear Strategy and Anglo-American Relations, 1939 – 1958 Submitted by: Geoffrey Charles Mallett Skinner to the University of Exeter as a thesis for the degree of Doctor of Philosophy in History, July 2018 This thesis is available for Library use on the understanding that it is copyright material and that no quotation from the thesis may be published without proper acknowledgement. I certify that all material in this thesis which is not my own work has been identified and that no material has previously been submitted and approved for the award of a degree by this or any other University. (Signature) ……………………………………………………………………………… 1 Abstract There was no special governmental partnership between Britain and America during the Second World War in atomic affairs. A recalibration is required that updates and amends the existing historiography in this respect. The wartime atomic relations of those countries were cooperative at the level of science and resources, but rarely that of the state. As soon as it became apparent that fission weaponry would be the main basis of future military power, America decided to gain exclusive control over the weapon. Britain could not replicate American resources and no assistance was offered to it by its conventional ally. America then created its own, closed, nuclear system and well before the 1946 Atomic Energy Act, the event which is typically seen by historians as the explanation of the fracturing of wartime atomic relations. Immediately after 1945 there was insufficient systemic force to create change in the consistent American policy of atomic monopoly. As fusion bombs introduced a new magnitude of risk, and as the nuclear world expanded and deepened, the systemic pressures grew. -
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. -
Arthur Holly Compton
Arthur Holly Compton ALSO LISTED IN Physicists ALSO KNOWN AS Arthur Holly Compton FAMOUS AS Nobel Prize Laureate in Physics NATIONALITY American Famous American Men RELIGION Baptist BORN ON 10 September 1892 AD Famous 10th September Birthdays ZODIAC SIGN Virgo Virgo Men BORN IN Wooster, Ohio, USA DIED ON 15 March 1962 AD PLACE OF DEATH Berkeley, California, USA FATHER Elias Compton MOTHER Otelia Catherine SIBLINGS Karl Taylor Compton, Wilson Martindale Compton SPOUSE: Betty Charity McCloskey CHILDREN Arthur Allen Compton, John Joseph Compton EDUCATION University of Cambridge, The College of Wooster, Princeton University DISCOVERIES / INVENTIONS Compton Effect AWARDS: Nobel Prize for Physics (1927) Matteucci Medal (1930) Franklin Medal (1940) Hughes Medal (1940) Arthur Holly Compton was a renowned American physicist who first rose to fame with his famous revolutionary discovery of the Compton Effect for which he also won the Nobel Prize in Physics. This discovery confirmed the dual nature of electromagnetic radiation as both a wave and a particle. Thomson was initially interested in astronomy before he shifted his focus to the study of quantum physics. He started his research in Cavendish Laboratory of Cambridge University and this research led to the discovery of Compton Effect. Later on, during the Second World War, Compton became head of the Manhattan Project’s Metallurgical Laboratory. Manhattan Project developed the first nuclear weapons of the world and Compton played a key role in it. He also served as Chancellor of Washington University in St. Louis. Under his leadership, the University made remarkable academic progress; the university formally desegregated its undergraduate divisions, named its first female full professor, and enrolled a record number of students. -
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 -
Bob Farquhar
1 2 Created by Bob Farquhar For and dedicated to my grandchildren, their children, and all humanity. This is Copyright material 3 Table of Contents Preface 4 Conclusions 6 Gadget 8 Making Bombs Tick 15 ‘Little Boy’ 25 ‘Fat Man’ 40 Effectiveness 49 Death By Radiation 52 Crossroads 55 Atomic Bomb Targets 66 Acheson–Lilienthal Report & Baruch Plan 68 The Tests 71 Guinea Pigs 92 Atomic Animals 96 Downwinders 100 The H-Bomb 109 Nukes in Space 119 Going Underground 124 Leaks and Vents 132 Turning Swords Into Plowshares 135 Nuclear Detonations by Other Countries 147 Cessation of Testing 159 Building Bombs 161 Delivering Bombs 178 Strategic Bombers 181 Nuclear Capable Tactical Aircraft 188 Missiles and MIRV’s 193 Naval Delivery 211 Stand-Off & Cruise Missiles 219 U.S. Nuclear Arsenal 229 Enduring Stockpile 246 Nuclear Treaties 251 Duck and Cover 255 Let’s Nuke Des Moines! 265 Conclusion 270 Lest We Forget 274 The Beginning or The End? 280 Update: 7/1/12 Copyright © 2012 rbf 4 Preface 5 Hey there, I’m Ralph. That’s my dog Spot over there. Welcome to the not-so-wonderful world of nuclear weaponry. This book is a journey from 1945 when the first atomic bomb was detonated in the New Mexico desert to where we are today. It’s an interesting and sometimes bizarre journey. It can also be horribly frightening. Today, there are enough nuclear weapons to destroy the civilized world several times over. Over 23,000. “Enough to make the rubble bounce,” Winston Churchill said. The United States alone has over 10,000 warheads in what’s called the ‘enduring stockpile.’ In my time, we took care of things Mano-a-Mano.