What's Nuclear Medicine?

Total Page:16

File Type:pdf, Size:1020Kb

Load more

What’s Nuclear Medicine? And its history The Atomic Age, one of history's most important events, took centuries to arrive, as events in science and international affairs evolved. The Atomic Theory, a cornerstone of modern science, was proposed by an early Greek thinker, Democritus. He suggested that everything in the universe was made up of particles so tiny that nothing smaller could exist. So… this is the known structure – currently! The Atomic Theory of Matter c.460 BCE - c.370 BCE The Atomic Theory, a cornerstone of modern science, was proposed by an early Greek thinker, Democritus. Atomic Weights 1808 John Dalton, an English chemist, stated that each atom of any given element is identical to every other atom of that element, including weight. The Periodic Table 1871 Dmitry Mendeleyev, a Russian chemist, revealed the basic importance of atomic weights and of nuclear structure. His work also showed the significance of structure in comprehending the behavior and properties of matter. Cathode Rays 1887 Sir William Crookes, an English chemist and physicist, pioneered work on cathode rays. X-Rays 1895 While studying cathode rays, German physicist Wilhelm Röentgen noticed some glowing barium platinocyanide across the room from his experiment. This led to the discovery of X-rays. His work helped found a major new medical technique and played an important role in revealing the secrets of the atom and its nucleus. Radioactivity 1896 French physicist Antoine Henri Becquerel discovered radioactivity. The Electron 1897 English physicist Sir J. J. Thomson explained the nature of the electron. Radium 1902 Marie Curie and her husband, Pierre, discovered the radioactive elements polonium and radium. Their work confirmed the existence of radioactivity. E=mc2 1905 For more than two centuries, scientists had unquestionably believed that the basic quantities of measurement -- mass, length, and time -- were absolute and unvarying. The German-born physicist Albert Einstein showed that in fact they depended very much on the relative motion between the observer and whatever was being observed. The Nuclear Model 1909 Sir Ernest Rutherford's great contribution to modern science was to show what happens to an element during radioactive decay. This enabled him to construct the first nuclear model of the atom, a cornerstone of present-day physics. The Electron Orbit 1913 Niels Bohr modified Rutherford's model of the atom to incorporate the ideas of quantum physics. This required a new mechanism for the way electrons emitted energy. Transformation of Atoms 1919 Rutherford's work, which he published in 1919, demonstrated that atoms could be transformed from those of one element into those of another by means of artificial tampering with the nucleus. Far more important, his experiment demonstrated that the nucleus of an atom could be breached. The Neutron 1932 British physicist Sir James Chadwick is best known for discovering the neutron, one of the fundamental particles making up the nucleus of atoms. The neutron differed from all other particles then known by having no electrical charge. The Atom is Split 1932 Sir John Douglas Cockroft and his colleague, Ernest T. S. Walton, developed the Cockroft-Walton particle accelerator. Using it in 1932, they managed to boost the speed of protons to the point where the voltage was high enough to energize each atom of lithium, their target metal, to form two atoms of helium. This was the first example of man-made nuclear transformation. Uranium and Fission 1938 German scientists Otto Hahn and Fritz Strassmann discovered that a tiny portion of the uranium atom's mass could be converted into an estimated 200 million electron volts of potentially usable energy. This process was to be called fission. Ernest O. Lawrence In 1929, Ernest O. Lawrence, working at the University of California at Berkeley, invented the cyclotron which could create a number of radioisotopes that are useful in biological and medical work. Glenn T. Seaborg and John J. Livingood Using an advanced cyclotron, scientists John Livingood, Fred Fairbrother, and Glenn T. Seaborg produced iron-59 (Fe-59) in 1937. Iron-59 was useful in the studies of the hemoglobin in human blood. In 1938, iodine-131 (I-131) was discovered by Livingood and Seaborg. Iodine-131 is used across the world to treat thyroid disease.Dr. Glenn Seaborg was considered one of the "founding fathers" of nuclear medicine. Dr. Seaborg was the most prolific discoverer of radioisotopes that are used today in diagnosis and treatment. Seaborg was active in the field up until the time of his death in 1999. Cyclotron In 1909, the prevailing theory of the atom's structure was that atoms were mushy, semi- permeable balls, with bits of charge strewn around them. This theory worked just fine for most experiments about the physical world. Physics, however, is not only interested in how the world appears to operate, but how it actually works. And so in 1909 a man named Ernest Rutherford set up an experiment to test the validity of the prevailing theory. In doing so he established a way that for the first time physicists could "look into" tiny particles they couldn't see with microscopes. In Rutherford's expeirment, a radioactive source shot a stream of alpha particles at a sheet of very thin gold foil which stood in front of a screen. The alpha particles would make little flashes of light where they hit the screen. The alpha particles were expected pass right through the very thin gold foil and make their marks in a small cluster on the screen. Rutherford’s theory Particle Decays and Annihilations Radioactive Particles Scientists eventually identified several distinct types of radiation, the particles resulting from radioactive decays. The three types of radiation were named after the first three letters of the Greek alphabet: (alpha), (beta), and (gamma). Alpha particles are helium nuclei (2 p, 2 n) Beta particles are speedy electrons Gamma radiation is a high-energy photon These three forms of radiation can be distinguished by a magnetic field since the positively-charged alpha particles curve in one direction, the negatively-charged beta particles curve in the opposite direction, and the electrically-neutral gamma radiation doesn't curve at all. Alpha particles can be stopped by a sheet of paper, beta particles by aluminum, and gamma radiation by a block of lead. Gamma radiation can penetrate very far into a material, and so it is gamma radiation that poses the most danger when working with radioactive materials, although all types of radiation are very dangerous. Sadly, it took scientists many years to realize the perils of radioactivity. Radioactivity is measured in Curies and Becquerels, and the time it lasts, is expressed in half lives ie the time it takes to get to half the activity Carbon dating – the man in the Alps Carbon dating uses the radioactivity that occurs naturally in rocks and the environment A.H.Becquerel Henri Becquerel Over a hundred years ago, in early 1896, the French physicist, Henri Becquerel, discovered that a mysterious X-ray was produced by uranium. Becquerel's achievement was itself based on the work of the German scientist, Wilhelm Conrad Roentgen, who had discovered X-rays only a few months earlier in November 1895 First evidence of radioactivity Nuclear Fission This is used in a variety of processes •In nuclear bombs •In nuclear power stations •To produce radioactive products for medical uses Nuclear Reactor Nuclear Power Station Chernobyl Modern Nuclear Power Station Chernobyl Atomic Bomb Fat One Uncontrolled Fission Generator used in Nuclear Medicine Radioisotopes Used in Nuclear Medicine • For imaging Technetium is used extensively, as it has a short physical half life of 6 hours. However, as the body is continually eliminating products the biological half life may be shorter. Thus the amount of radioactive exposure is limited. • Technetium is a gamma emitter. This is important as the rays need to penetrate the body so the camera can detect them. • Because it has such a short half life, it cannot be stored for very long because it will have decayed. It is generated by a molybdenum source (parent host) which has a much greater half life and the Tc extracted on the day it is required. The molybdenum is obtained from a nuclear reactor and imported. For treatment of therapy, beta emitters are often used because they are absorbed locally. Hal Anger Hal Anger revolutionized the field of nuclear medicine with his development of the gamma camera in the late 1950s. He also developed the well counter, widely used in laboratory tests with small samples of radioactive materials. Modern Gamma camera, with patient undergoing heart imaging Gamma Camera – what is it? The following are the typical features of the scintillation crystal used in modern gamma cameras • most gamma cameras use thallium-activated NaI (NaI(Tl)) • NaI(Tl) emits blue-green light at about 415 nm • the spectral output of such a scintillation crystal matches well the response of standard bialkali photomultipliers (e.g SbK2Cs ) • the linear attenuation coefficient of NaI(Tl) at 150 KeV is about 2.2 1/cm . Therefore about 90% of all photons are absorbed within about 10 mm • NaI(Tl) is hyrdoscopic and therefore requires hermetic encapsulation • NaI(Tl) has a high refractive index ( ~ 1.85) and thus a light guide is used to couple the scintillation crystal to the photomultiplier tube • the scintillation crystal and associated electronics are surrounded by a lead shield to minimize the detection of unwanted radiation • digital and/or analog methods are used for image capture The Gamma Camera components- The modern gamma camera consists of: - multihole collimator - large area (e.g 5 cm ) NaI(Tl) (Sodium Iodide - Thallium activated) scintillation crystal - light guide for optical coupling array (commonly hexagonal) of photo- multiplier tubes - lead shield to minimize background radiation A crucial component of the modern gamma camera is the collimator.
Recommended publications
  • George De Hevesy in America

    George De Hevesy in America

    Journal of Nuclear Medicine, published on July 13, 2019 as doi:10.2967/jnumed.119.233254 George de Hevesy in America George de Hevesy was a Hungarian radiochemist who was awarded the Nobel Prize in Chemistry in 1943 for the discovery of the radiotracer principle (1). As the radiotracer principle is the foundation of all diagnostic and therapeutic nuclear medicine procedures, Hevesy is widely considered the father of nuclear medicine (1). Although it is well-known that he spent time at a number of European institutions, it is not widely known that he also spent six weeks at Cornell University in Ithaca, NY, in the fall of 1930 as that year’s Baker Lecturer in the Department of Chemistry (2-6). “[T]he Baker Lecturer gave two formal presentations per week, to a large and diverse audience and provided an informal seminar weekly for students and faculty members interested in the subject. The lecturer had an office in Baker Laboratory and was available to faculty and students for further discussion.” (7) There is also evidence that, “…Hevesy visited Harvard [University, Cambridge, MA] as a Baker Lecturer at Cornell in 1930…” (8). Neither of the authors of this Note/Letter was aware of Hevesy’s association with Cornell University despite our longstanding ties to Cornell until one of us (WCK) noticed the association in Hevesy’s biographical page on the official Nobel website (6). WCK obtained both his undergraduate degree and medical degree from Cornell in Ithaca and New York City, respectively, and spent his career in nuclear medicine. JRO did his nuclear medicine training at Columbia University and has subsequently been a faculty member of Weill Cornell Medical College for the last eleven years (with a brief tenure at Memorial Sloan Kettering Cancer Center (affiliated with Cornell)), and is now the program director of the Nuclear Medicine residency and Chief of the Molecular Imaging and Therapeutics Section.
  • A Brief History of Nuclear Astrophysics

    A Brief History of Nuclear Astrophysics

    A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J.
  • Europe's Biggest General Science Conference Concludes Successfully

    Europe's Biggest General Science Conference Concludes Successfully

    SCIENCEScience PagesPAGES Special Report - ESOF 2016 Europe’s biggest generalSpecial Report science conference concludes successfully ESOF 2016, Europe's biggest general science conference concludes successfully in Manchester,in Manchester,UK UK Theme: Science as Revolution Theme: Science as Revolution - Veena Patwardhan rom 23rd to 27th July, 2016, FManchester flaunted its City of Science status as the host city of the seventh edition of EuroScience Open Forum (ESOF 2016). A bi- ennial event held in a different European city every two years, this time it was Manchester's turn to host this globally reputed science conference. Around 4500 delegates – scien- tists, innovators, academics, young researchers, journalists, policy makers, industry representatives and others – converged on the world's first industrial city to dis- cover and have discussions about the latest advancements in scien- rd th Manchester Central, venue of ESOF 2016 tific and technological researchFrom 23 to 27 July, 2016, Manchester flaunted its City of Science status as the host city of the across Europe and beyond. The seventhmain theme edition this of EuroScienceyear Laureates Open Forumand distinguished (ESOF 2016). Ascientists biennial inevent the held packed in a different was 'Science as Revolution', indicatingEuropean that city the every focus two of years,Exchange this time Hall it wasof Manchester Manchester's Central, turn to hostthe venuethis globally of the reputed the conference would be on how sciencescience andconference. technology conference. could transform life on the planet, revolutionise econo- The proceedings began with a string quartet render- mies, and help in overcoming challenges faced by global ing a piece of specially composed music.
  • The Nobel Laureate George De Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine Niese S* Am Silberblick 9, 01723 Wilsdruff, Germany

    The Nobel Laureate George De Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine Niese S* Am Silberblick 9, 01723 Wilsdruff, Germany

    Open Access SAJ Biotechnology LETTER ISSN: 2375-6713 The Nobel Laureate George de Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine Niese S* Am Silberblick 9, 01723 Wilsdruff, Germany *Corresponding author: Niese S, Am Silberblick 9, 01723 Wilsdruff, Germany, Tel: +49 35209 22849, E-mail: [email protected] Citation: Niese S, The Nobel Laureate George de Hevesy (1885-1966) - Universal Genius and Father of Nuclear Medicine. SAJ Biotechnol 5: 102 Article history: Received: 20 March 2018, Accepted: 29 March 2018, Published: 03 April 2018 Abstract The scientific work of the universal genius the Nobel Laureate George de Hevesy who has discovered and developed news in physics, chemistry, geology, biology and medicine is described. Special attention is given to his work in life science which he had done in the second half of his scientific career and was the base of the development of nuclear medicine. Keywords: George de Hevesy; Radionuclides; Nuclear Medicine Introduction George de Hevesy has founded Radioanalytical Chemistry and Nuclear Medicine, discovered the element hafnium and first separated stable isotopes. He was an inventor in many disciplines and his interest was not only focused on the development and refinement of methods, but also on the structure of matter and its changes: atoms, molecules, cells, organs, plants, animals, men and cosmic objects. He was working under complicated political situation in Europe in the 20th century. During his stay in Germany, Austria, Hungary, Switzerland, Denmark, and Sweden he wrote a lot papers in German. In 1962 he edited a large part of his articles in a collection where German papers are translated in English [1].
  • Appendix E Nobel Prizes in Nuclear Science

    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
  • ARIE SKLODOWSKA CURIE Opened up the Science of Radioactivity

    ARIE SKLODOWSKA CURIE Opened up the Science of Radioactivity

    ARIE SKLODOWSKA CURIE opened up the science of radioactivity. She is best known as the discoverer of the radioactive elements polonium and radium and as the first person to win two Nobel prizes. For scientists and the public, her radium was a key to a basic change in our understanding of matter and energy. Her work not only influenced the development of fundamental science but also ushered in a new era in medical research and treatment. This file contains most of the text of the Web exhibit “Marie Curie and the Science of Radioactivity” at http://www.aip.org/history/curie/contents.htm. You must visit the Web exhibit to explore hyperlinks within the exhibit and to other exhibits. Material in this document is copyright © American Institute of Physics and Naomi Pasachoff and is based on the book Marie Curie and the Science of Radioactivity by Naomi Pasachoff, Oxford University Press, copyright © 1996 by Naomi Pasachoff. Site created 2000, revised May 2005 http://www.aip.org/history/curie/contents.htm Page 1 of 79 Table of Contents Polish Girlhood (1867-1891) 3 Nation and Family 3 The Floating University 6 The Governess 6 The Periodic Table of Elements 10 Dmitri Ivanovich Mendeleev (1834-1907) 10 Elements and Their Properties 10 Classifying the Elements 12 A Student in Paris (1891-1897) 13 Years of Study 13 Love and Marriage 15 Working Wife and Mother 18 Work and Family 20 Pierre Curie (1859-1906) 21 Radioactivity: The Unstable Nucleus and its Uses 23 Uses of Radioactivity 25 Radium and Radioactivity 26 On a New, Strongly Radio-active Substance
  • Cambridge's 92 Nobel Prize Winners Part 4 - 1996 to 2015: from Stem Cell Breakthrough to IVF

    Cambridge's 92 Nobel Prize Winners Part 4 - 1996 to 2015: from Stem Cell Breakthrough to IVF

    Cambridge's 92 Nobel Prize winners part 4 - 1996 to 2015: from stem cell breakthrough to IVF By Cambridge News | Posted: February 01, 2016 Some of Cambridge's most recent Nobel winners Over the last four weeks the News has been rounding up all of Cambridge's 92 Nobel Laureates, which this week comes right up to the present day. From the early giants of physics like JJ Thomson and Ernest Rutherford to the modern-day biochemists unlocking the secrets of our genome, we've covered the length and breadth of scientific discovery, as well as hugely influential figures in economics, literature and politics. What has stood out is the importance of collaboration; while outstanding individuals have always shone, Cambridge has consistently achieved where experts have come together to bounce their ideas off each other. Key figures like Max Perutz, Alan Hodgkin and Fred Sanger have not only won their own Nobels, but are regularly cited by future winners as their inspiration, as their students went on to push at the boundaries they established. In the final part of our feature we cover the last 20 years, when Cambridge has won an average of a Nobel Prize a year, and shows no sign of slowing down, with ground-breaking research still taking place in our midst today. The Gender Pay Gap Sale! Shop Online to get 13.9% off From 8 - 11 March, get 13.9% off 1,000s of items, it highlights the pay gap between men & women in the UK. Shop the Gender Pay Gap Sale – now. Promoted by Oxfam 1.1996 James Mirrlees, Trinity College: Prize in Economics, for studying behaviour in the absence of complete information As a schoolboy in Galloway, Scotland, Mirrlees was in line for a Cambridge scholarship, but was forced to change his plans when on the weekend of his interview he was rushed to hospital with peritonitis.
  • Guides to the Royal Institution of Great Britain: 1 HISTORY

    Guides to the Royal Institution of Great Britain: 1 HISTORY

    Guides to the Royal Institution of Great Britain: 1 HISTORY Theo James presenting a bouquet to HM The Queen on the occasion of her bicentenary visit, 7 December 1999. by Frank A.J.L. James The Director, Susan Greenfield, looks on Front page: Façade of the Royal Institution added in 1837. Watercolour by T.H. Shepherd or more than two hundred years the Royal Institution of Great The Royal Institution was founded at a meeting on 7 March 1799 at FBritain has been at the centre of scientific research and the the Soho Square house of the President of the Royal Society, Joseph popularisation of science in this country. Within its walls some of the Banks (1743-1820). A list of fifty-eight names was read of gentlemen major scientific discoveries of the last two centuries have been made. who had agreed to contribute fifty guineas each to be a Proprietor of Chemists and physicists - such as Humphry Davy, Michael Faraday, a new John Tyndall, James Dewar, Lord Rayleigh, William Henry Bragg, INSTITUTION FOR DIFFUSING THE KNOWLEDGE, AND FACILITATING Henry Dale, Eric Rideal, William Lawrence Bragg and George Porter THE GENERAL INTRODUCTION, OF USEFUL MECHANICAL - carried out much of their major research here. The technological INVENTIONS AND IMPROVEMENTS; AND FOR TEACHING, BY COURSES applications of some of this research has transformed the way we OF PHILOSOPHICAL LECTURES AND EXPERIMENTS, THE APPLICATION live. Furthermore, most of these scientists were first rate OF SCIENCE TO THE COMMON PURPOSES OF LIFE. communicators who were able to inspire their audiences with an appreciation of science.
  • Back Matter (PDF)

    Back Matter (PDF)

    V ll INDEX to VOL. CXXIV. (A) Adsorbed gas and emission of soft X-rays (Nakaya), 61G. Adsorption of electrolytes, influence of (Phelps and Peters), 554. Alpha particles, radioactive decay and nuclear penetration (Fowler and Wilson), 493. Analysis by X-ray spectroscopy (Eddy and others), 249. Asundi (R. K.) The Third Positive Carbon and Associated Bands, 277. Asundi (R. K.) See also Johnson and Asundi. Atom, many-electron, relativistic theory (Gaunt), 163. Bhagavantam (S.) The Magnetic Anisotropy of Naphthalene Crystals, 545. Bickley (W. G.) Hydrodynamic Forces acting on a Cylinder in Motion, and the idea of a “ Hydrodynamic Centre,” 296. Brunt (D.) The Transfer of Heat by Radiation and Turbulence in the Lower Atmosphere, 201. Catalysis by silver of the union of hydrogen and oxygen (Chapman and Hall), 478. Cawood (W.) See Patterson and others. Chapman (D. L.) and Hall (W. K.) A Study of the Catalysis by Silver of the Union of Hydrogen and Oxygen, 478. Clark (R. J.) On the Direct Determination of the Electrostatic Moments of Molecules, 689. Combination of hydrogen and oxygen (Thompson and Hinshelwood), 219. Curie point and magnetostriction (Fowler and Kapitza), 1. Darwin (G. C.) A Collision Problem in the Wave Mechanics, 375. Davidson (P. M.) See Richardson and Davidson. Davies (L. P.) The Soft X-Ray Emission from Various Elements after Oxidation, 268. Dispersion in metals, quantum theory (Kronig), 409. Duncan (W. J.) See Frazer and Duncan. Eddy (C. E.), Laby (T. H.) and Turner (A. H.) Analysis by X-Ray Spectroscopy, 249. Einstein’s unified field theory (McVittie), 366. Electrical condition of hot surfaces during adsorption (Finch and Stimson), 356.
  • The World Around Is Physics

    The World Around Is Physics

    The world around is physics Life in science is hard What we see is engineering Chemistry is harder There is no money in chemistry Future is uncertain There is no need of chemistry Therefore, it is not my option I don’t have to learn chemistry Chemistry is life Chemistry is chemicals Chemistry is memorizing things Chemistry is smell Chemistry is this and that- not sure Chemistry is fumes Chemistry is boring Chemistry is pollution Chemistry does not excite Chemistry is poison Chemistry is a finished subject Chemistry is dirty Chemistry - stands on the legacy of giants Antoine-Laurent Lavoisier (1743-1794) Marie Skłodowska Curie (1867- 1934) John Dalton (1766- 1844) Sir Humphrey Davy (1778 – 1829) Michael Faraday (1791 – 1867) Chemistry – our legacy Mendeleev's Periodic Table Modern Periodic Table Dmitri Ivanovich Mendeleev (1834-1907) Joseph John Thomson (1856 –1940) Great experimentalists Ernest Rutherford (1871-1937) Jagadish Chandra Bose (1858 –1937) Chandrasekhara Venkata Raman (1888-1970) Chemistry and chemical bond Gilbert Newton Lewis (1875 –1946) Harold Clayton Urey (1893- 1981) Glenn Theodore Seaborg (1912- 1999) Linus Carl Pauling (1901– 1994) Master craftsmen Robert Burns Woodward (1917 – 1979) Chemistry and the world Fritz Haber (1868 – 1934) Machines in science R. E. Smalley Great teachers Graduate students : Other students : 1. Werner Heisenberg 1. Herbert Kroemer 2. Wolfgang Pauli 2. Linus Pauling 3. Peter Debye 3. Walter Heitler 4. Paul Sophus Epstein 4. Walter Romberg 5. Hans Bethe 6. Ernst Guillemin 7. Karl Bechert 8. Paul Peter Ewald 9. Herbert Fröhlich 10. Erwin Fues 11. Helmut Hönl 12. Ludwig Hopf 13. Walther Kossel 14.
  • Ernest Rutherford

    Ernest Rutherford

    Ernest Rutherford (1) On August 30th, 1871 in Spring Grove, New Zealand, Ernest Rutherford was born to James Rutherford, a Scottish wheelwright and engineer, and Martha Rutherford, an English school teacher. Ernest Rutherford grew up in a large family; he was the fourth child in a family with 12 children (2). Education Ernest Rutherford spent his early education in the schools provided by the government (3). In 1887, at the age of 16, he won a scholarship to attend Nelson Collegiate School now know as Nelson College; Rutherford won this scholarship on his second attempt (2). Two years later, again on his second attempt, Rutherford won another scholarship this time to attend Canterbury College which was administered by the University of New Zealand (2). At Canterbury College, Rutherford received his BA in Pure Mathematics and Latin, Applied Mathematics, English, French, and Physics in 1892. Rutherford also won a scholarship that allowed him to continue at Canterbury to achieve his Masters. A year later, Rutherford obtained his Masters of Arts with double first class honors, first in Mathematics and Mathematical Physics then in Physical Sciences (2). After obtaining his Masters Rutherford failed three times at finding a job as a school- teacher and remained as a tutor (2). The Royal Commissioners for the Exhibit of 1851 initiated a scholarship that allowed graduates of universities of the British Empire to go anywhere in the world and work on research of importance to their home country’s industry. With this news Rutherford returned to Canterbury College in 1894 since it was a requirement to be enrolled at a university (2).
  • Nobel Laureates

    Nobel Laureates

    Nobel Laureates Over the centuries, the Academy has had a number of Nobel Prize winners amongst its members, many of whom were appointed Academicians before they received this prestigious international award. Pieter Zeeman (Physics, 1902) Lord Ernest Rutherford of Nelson (Chemistry, 1908) Guglielmo Marconi (Physics, 1909) Alexis Carrel (Physiology, 1912) Max von Laue (Physics, 1914) Max Planck (Physics, 1918) Niels Bohr (Physics, 1922) Sir Chandrasekhara Venkata Raman (Physics, 1930) Werner Heisenberg (Physics, 1932) Charles Scott Sherrington (Physiology or Medicine, 1932) Paul Dirac and Erwin Schrödinger (Physics, 1933) Thomas Hunt Morgan (Physiology or Medicine, 1933) Sir James Chadwick (Physics, 1935) Peter J.W. Debye (Chemistry, 1936) Victor Francis Hess (Physics, 1936) Corneille Jean François Heymans (Physiology or Medicine, 1938) Leopold Ruzicka (Chemistry, 1939) Edward Adelbert Doisy (Physiology or Medicine, 1943) George Charles de Hevesy (Chemistry, 1943) Otto Hahn (Chemistry, 1944) Sir Alexander Fleming (Physiology, 1945) Artturi Ilmari Virtanen (Chemistry, 1945) Sir Edward Victor Appleton (Physics, 1947) Bernardo Alberto Houssay (Physiology or Medicine, 1947) Arne Wilhelm Kaurin Tiselius (Chemistry, 1948) - 1 - Walter Rudolf Hess (Physiology or Medicine, 1949) Hideki Yukawa (Physics, 1949) Sir Cyril Norman Hinshelwood (Chemistry, 1956) Chen Ning Yang and Tsung-Dao Lee (Physics, 1957) Joshua Lederberg (Physiology, 1958) Severo Ochoa (Physiology or Medicine, 1959) Rudolf Mössbauer (Physics, 1961) Max F. Perutz (Chemistry, 1962)