Benefits of Diversity

Total Page:16

File Type:pdf, Size:1020Kb

Benefits of Diversity commentary Benefits of diversity Abraham Loeb Discoveries in astronomy — or, in fact, any branch of science — can only happen when people are open-minded and willing to take risks. ccording to Mark Twain, “It ain’t used it to discover the expansion of the weak, as most of the X-ray sources would what you don’t know that gets you Universe. It was surpassed in 1948 by the be flaring stars. The launch of an X-ray Ainto trouble. It’s what you know for 200 inch telescope at the Mount Palomar telescope by NASA was therefore delayed sure that just ain’t so.” This illustrates a very Observatory in California, which played a by half a decade, after which astronomers common flaw astronomers have, which is to key role in the discovery of radio galaxies discovered X-ray emission from numerous believe that they know the truth even when and quasars and in studies of the other sources, such as accreting black holes data are scarce. This fault is the trademark intergalactic medium2. Clearly, bigger and neutron stars, supernova remnants and of a data-starved science. It occasionally telescopes continued to benefit astronomy galaxy clusters. leads to major blunders by the scientific as technology improved. community causing the wrong strategic Dark matter. In the early 1970s decisions, and bringing about unnecessary Composition of the Sun. While Jerry Ostriker gave a talk at the California delays in finding the truth. Let me illustrate working on her PhD thesis in 1925, Institute of Technology describing the this phenomenon with ten examples, in Cecilia Payne-Gaposchkin (who became case — developed by him in collaboration chronological order. the first to be awarded a PhD in Astronomy with Jim Peebles and Amos Yahil — for at Harvard-Radcliffe) interpreted the solar spiral galaxies having dark matter haloes Large telescopes. In 1909, spectrum based on the Saha equation that comprise most of their mass6. Members Edward Charles Pickering, who served and concluded that the Sun’s atmosphere of the audience were contemptuous as director of the Harvard College is made mostly of hydrogen. During the of the idea and dismissed it as wild Observatory from 1877 until 1919, argued review of her dissertation, the distinguished theoretical speculation. that telescopes had reached their optimal Princeton astronomer Henry Norris Russell size of 50–70 inches and there was no convinced her to avoid the conclusion that Gravitational lensing. Around 1980, advantage to be gained from seeking larger the composition of the Sun is different from shortly after the discovery7 of the first apertures. In December 1908, in an article that of the Earth, as it contradicted the gravitational lens (QSO 0957+561 A/B), titled ‘The Future of Astronomy’, he wrote1: conventional wisdom at the time3. Ed Turner at Princeton University was advised by a highly distinguished “It is more than doubtful, however, whether a Maser and complex molecules. When astronomer not to spend much time further increase in size is a great advantage. Charlie Townes worked on his experimental working on gravitational lenses because Much more depends on other conditions, demonstration of the maser in 1954, two they would turn out to be useless especially those of climate, the kind of work to Nobel laureates, Isidor Isaac Rabi and curiosities. For a few years, lenses were be done and, more than all, the man behind Polykarp Kusch, tried to stop him by widely regarded by astronomers as the gun. The case is not unlike that of a saying4: “Look, you should stop the work unimportant and it was almost impossible battleship. Would a ship a thousand feet long you are doing. It isn’t going to work. You to get observing time or grants to always sink one of five hundred feet? It seems know it’s not going to work, we know it’s study them. as if we had nearly reached the limit of size of not going to work. You’re wasting money. telescopes, and as if we must hope for the next Just stop!” Three months later, the maser Cosmology. Around 1990, during my improvement in some other direction.” worked. Similar circumstances repeated term as a postdoctoral fellow at Princeton, when Townes was determined to discover I asked a prominent astronomer from Pickering’s blunder led to a major blow for complex molecules in space and experienced another prestigious academic institution observational astronomy on the east coast of resistance from astronomers who argued whether they would consider hiring junior the USA. On the west coast, just before that the interstellar gas density is so low and faculty in the field of theoretical cosmology. Pickering’s article was published, the ultraviolet illumination so intense that He replied: “we might contemplate this George Ellery Hale obtained first light on any surviving molecules would be too scarce possibility if we could only convince the 60 inch telescope at Mount Wilson to be detectable5. ourselves that cosmology is a science”. Two Observatory in California, which became years later, in 1992, the COBE satellite one of the most productive telescopes in X-ray astronomy. In the early 1960s a reported the detection of microwave astronomical history. Around the same panel of experts was assembled by NASA background anisotropies8. time, Hale received funding from to evaluate the merits of a proposal to John Hooker and Andrew Carnegie to launch an X-ray telescope into space (as High-redshift galaxies. Piero Madau at create a larger telescope. The 100 inch the Earth’s atmosphere blocks X-rays). the University of California, Santa Cruz, telescope was completed in 1917; The panel concluded that the scientific once told me that he had great difficulties Edwin Hubble and Milton Humason later motivation for an X-ray space telescope was publishing a paper he wrote in the 616 NATURE PHYSICS | VOL 10 | SEPTEMBER 2014 | www.nature.com/naturephysics © 2014 Macmillan Publishers Limited. All rights reserved commentary mid-1990s on intergalactic absorption and the announcement of the discovery of agencies should dedicate a fixed fraction the colours of high-redshift galaxies because 51 Peg b in 199511 and after others had of their resources (say 10–20%) to risky the referee kept arguing: “we all know that found similar examples. As it turns out, explorations. This can be regarded as there are no normal galaxies above a redshift Otto Struve had already suggested12 in affirmative action to promote a diversity of of two”. 1952 that close-in planets may exist and ideas, which is as important for the progress would be easy to find through both radial of science as the promotion of gender and Kuiper Belt objects. David Jewitt at the velocity and transit observations, but his ethnic diversity. ❐ University of California, Los Angeles, paper was completely ignored because of could not get telescope time or funding theoretical priors. Abraham Loeb is in the Department of Astronomy, for attempts to detect the conjectured Harvard University, 60 Garden Street, Cambridge, population of Kuiper Belt objects9. He used These examples and many more like Massachusetts 02138, USA. observing time and funding he received for them (starting with the ancient view that e-mail: [email protected] other projects until he finally discovered the Earth is at the centre of the Universe the first of these objects in the outer Solar and that the Sun revolves around it), References 1. Pickering, E. C. Pop. Sci. Mon. 75, 105–116 (1909); System with Jane Luu in 1992, using the demonstrate that progress in astronomy can http://go.nature.com/SfXnMR 88 inch telescope at Mauna Kea, Hawaii. be delayed by the erroneous proposition 2. http://www.astro.caltech.edu/palomar/history.html that we know the truth even without 3. Padman, R. Cecilia Payne-Gaposchkin (1900–1979) (Needham College, 2010); http://go.nature.com/QPaUjS Close-in Jupiters. The first planets ever experimental evidence. Lapses of this type 4. Hora, H. & Miley, G. in Edward Teller Lectures: Laser discovered around a main sequence star can be avoided by an honest and open- and Inertial Fusion Energy (eds Hora, H. & Miley, G.) other than the Sun had masses similar to minded approach to scientific exploration, 4 (Imperial College Press, 2005). 5. Townes, C. H. in Revealing the Molecular Universe: One Jupiter but were orders of magnitude closer which I label as having a ‘non-informative Antenna is Never Enough (eds Backer, D., Moran, J. & Turner, J.) to their host star than Jupiter is to the Sun. prior’ (known as a Jeffreys prior in Bayesian 81 (ASPC, 2006). This can be simply understood as a selection statistics). This unbiased approach, which is 6. Ostriker, J. P., Peebles, P. J. E. & Yahil, A. Astrophys. J. effect, because the reflex motion of a star common among successful crime detectives, 193, L1–L4 (1974). 7. Walsh, D., Carswell, R. F. & Weymann, R. J. Nature due to a close-in planet is much easier to gives priority to evidence over imagination, 279, 381–384 (1979). detect than the motion induced by a distant and allows nature itself to guide us to 8. Smoot, G. F. et al. Astrophys. J 396, L1–L5 (1992). planet. But because Jupiter is considerably the correct answer. Its basic premise is 9. Jewitt, D. Astronomy Beat 48, 1 (2010). 10. Latham, D. W. et al. Nature 339, 38–40 (1989). farther out from the centre of the Solar humility — the recognition that nature is 11. Mayor, M. & Queloz, D. Nature 378, 355–359 (1995). System, time allocation committees on much richer than our imagination is able 12. Struve, O. The Observatory 72, 199–200 (1952). major telescopes declined proposals to to anticipate.
Recommended publications
  • I. I. Rabi Papers [Finding Aid]. Library of Congress. [PDF Rendered Tue Apr
    I. I. Rabi Papers A Finding Aid to the Collection in the Library of Congress Manuscript Division, Library of Congress Washington, D.C. 1992 Revised 2010 March Contact information: http://hdl.loc.gov/loc.mss/mss.contact Additional search options available at: http://hdl.loc.gov/loc.mss/eadmss.ms998009 LC Online Catalog record: http://lccn.loc.gov/mm89076467 Prepared by Joseph Sullivan with the assistance of Kathleen A. Kelly and John R. Monagle Collection Summary Title: I. I. Rabi Papers Span Dates: 1899-1989 Bulk Dates: (bulk 1945-1968) ID No.: MSS76467 Creator: Rabi, I. I. (Isador Isaac), 1898- Extent: 41,500 items ; 105 cartons plus 1 oversize plus 4 classified ; 42 linear feet Language: Collection material in English Location: Manuscript Division, Library of Congress, Washington, D.C. Summary: Physicist and educator. The collection documents Rabi's research in physics, particularly in the fields of radar and nuclear energy, leading to the development of lasers, atomic clocks, and magnetic resonance imaging (MRI) and to his 1944 Nobel Prize in physics; his work as a consultant to the atomic bomb project at Los Alamos Scientific Laboratory and as an advisor on science policy to the United States government, the United Nations, and the North Atlantic Treaty Organization during and after World War II; and his studies, research, and professorships in physics chiefly at Columbia University and also at Massachusetts Institute of Technology. Selected Search Terms The following terms have been used to index the description of this collection in the Library's online catalog. They are grouped by name of person or organization, by subject or location, and by occupation and listed alphabetically therein.
    [Show full text]
  • Physics Nobel 1997 Carl E. Wieman
    Julius Pluecker KLEIN TREE #1 c Dr. John Andraos, 2002 (Marburg, 1824) Klein bottle Carl L.F. Lindemann Max Born Richard Bornstein (Erlangen, 1873) (Goettingen, 1907) (Goettingen, 1872) proof that pi is transcendental (1882) Physics Nobel 1954 Sommerfeld model of the atom (1916) Hund's rules Born-Haber cycle (1919) Maria Goeppert-Mayer Born-Oppenheimer Victor Weisskopf (1925) Bigeleisen-Goeppert-Mayer (Goettingen, 1931) approximation (1927) heavy atom approximation (1947) discoveries relating to nuclear shell structure (1949) Max L.H. Delbrueck Physics Nobel 1963 Discoveries concerning Willis Eugene Lamb, Jr. Julian Schwinger Nicholas Kemmer Wendell H. Furry Murray Gell-Mann (ETH-Zurich, 1935) replication mechanism and (Illinois, 1932) Fine structure of H spectrum (Columbia, 1939; UC Berkeley) genetic material of viruses Physics Nobel 1955 Physics Nobel 1965 classification of elementary particles and their interactions Physiology & Medicine Moller-Plesset Abdus Salam Nobel 1969 eight-fold way, (1961), quark Jones effect single point calculation (1964) Physics Nobel 1969 Theory of unified weak (1948) (1934) Walter Kohn Sheldon L. Glashow and electromagnetic Development of DFT theory of unified weak Kenneth G. Wilson interaction between Chemistry Nobel 1998 and electromagnetic theory of critical phenomena elementary particles; Isidor I. Rabi Benjamin Mottelson forces between elementary in connection with phase weak neutral current (Columbia, 1927; Munich) Aage Bohr particles; prediction of transitions Physics Nobel 1979 Physics Nobel 1944 theory of structure of atomic weak neutral current Physics Nobel 1982 Physics Nobel 1979 Walter Gilbert nucleus Physics Nobel 1975 Maxam-Gilbert sequencing method Bernard T. Feld Norman F. Ramsey Martin L. Perl Julian Schwinger (1977) (Columbia, 1945) (Columbia, 1940) (Columbia, 1955) (Columbia, 1939) David J.
    [Show full text]
  • Transactions 1905
    THE Royal Astronomical Society of Canada TRANSACTIONS FOR 1905 (INCLUDING SELECTED PAPERS AND PROCEEDINGS) EDITED BY C. A CHANT. TORONTO: ROYAL ASTRONOMICAL PRINT, 1906. The Royal Astronomical Society of Canada. THE Royal Astronomical Society of Canada TRANSACTIONS FOR 1905 (INCLUDING SELECTED PAPERS AND PROCEEDINGS) EDITED BY C. A CHANT. TORONTO: ROYAL ASTRONOMICAL PRINT, 1906. TABLE OF CONTENTS. The Dominion Observatory, Ottawa (Frontispiece) List of Officers, Fellows and A ssociates..................... - - 3 Treasurer’s R eport.....................--------- 12 President’s Address and Summary of Work ------ 13 List of Papers and Lectures, 1905 - - - - ..................... 26 The Dominion Observatory at Ottawa - - W. F. King 27 Solar Spots and Magnetic Storms for 1904 Arthur Harvey 35 Stellar Legends of American Indians - - J. C. Hamilton 47 Personal Profit from Astronomical Study - R. Atkinson 51 The Eclipse Expedition to Labrador, August, 1905 A. T. DeLury 57 Gravity Determinations in Labrador - - Louis B. Stewart 70 Magnetic and Meteorological Observations at North-West River, Labrador - - - - R. F. Stupart 97 Plates and Filters for Monochromatic and Three-Color Photography of the Corona J. S. Plaskett 89 Photographing the Sun and Moon with a 5-inch Refracting Telescope . .......................... D. B. Marsh 108 The Astronomy of Tennyson - - - - John A. Paterson 112 Achievements of Nineteenth Century Astronomy , L. H. Graham 125 A Lunar Tide on Lake Huron - - - - W. J. Loudon 131 Contributions...............................................J. Miller Barr I. New Variable Stars - - - - - - - - - - - 141 II. The Variable Star ξ Bootis -------- 143 III. The Colors of Helium Stars - - - ..................... 144 IV. A New Problem in Solar Physics ------ 146 Stellar Classification ------ W. Balfour Musson 151 On the Possibility of Fife in Other Worlds A.
    [Show full text]
  • Hardy 1 Williamina Fleming
    Hardy 1 Williamina Fleming: Breaking Barriers with A Universe of Glass Isabella L. Hardy Junior Division Individual Performance paper 500 words In the past, women in the sciences were often overlooked, so for National History Day, I chose to focus on an under-recognized female scientist. Early in my research, I found Williamina Paton Fleming. I was surprised I had never encountered her although I had heard of her colleagues, Annie Jump Cannon and Henrietta Leavitt. I have always loved studying the stars and am fascinated by the role of women in astronomy whose important contributions are sometimes forgotten. Williamina Fleming’s unique ability to interpret astronomical photographs changed astronomy in nineteenth- century America and beyond, breaking barriers for scientists and for women. In preliminary research, I located Harvard’s digital scans of Fleming's diary and excellent period photographs, as well as many academic articles about her and other women at the Harvard Observatory. I was also privileged to interview Dr. Lindsay Smith, current Curator of Astronomical Photographs at Harvard. She was extremely helpful in suggesting sources and later reviewed the performance script. Not much is known about Fleming’s early years in Scotland. After her husband abandoned her, she worked for Harvard Observatory Director Edward Pickering, who hired her for the new project to map the night sky. The process involved taking images though telescopes, then mapping all the stars in that small section of sky. Using this process, Fleming discovered stars, novae, and nebulae and encouraged the work of other astronomers, while facilitating many important discoveries. I chose performance to give a voice to a person who has been largely unnoticed.
    [Show full text]
  • Polykarp Kusch 1 9 1 1 — 1 9 9 3
    NATIONAL ACADEMY OF SCIENCES POLYKARP KUSCH 1 9 1 1 — 1 9 9 3 A Biographical Memoir by NORMAN F. RAMSEY Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2008 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. POLYKARP KUSCH January 26, 1911–March 20, 1993 BY NORMAN F . RAMSEY OLYKARP KUSCH, A GREAT physicist, teacher, and Nobel laure- Pate, died in Dallas, Texas, at age 82 on March 20, 1993. Kusch was a pioneer in molecular beam magnetic resonance experiments; he and his associates, with unprecedented high accuracy, measured many atomic and nuclear spins, magnetic dipole moments, electric quadrupole moments, and atomic hyperfine structure separations. Kusch and his associates also made the first direct measurement of the magnetic moment of the electron, which showed that it was consistent with the previously observed anomalous hyperfine separation in atomic hydrogen and with J. Schwinger’s then-new relativistic quantum electrodynamics (QED). Polykarp Kusch was born in Blankenburg, Germany, on January 26, 1911, the son of John Mathias Kusch, a Lutheran missionary, and Henrietta van der Haas. The family emigrated to the United States in 1912, and Kusch became a naturalized U.S. citizen in 1922. He attended grade school in the Mid- west, and started his college education as a chemistry major at Case Institute of Technology in Cleveland, Ohio, shifting to physics before receiving his bachelor of science degree in 1931. He then moved to the University of Illinois, where in 1933 he received an M.S.
    [Show full text]
  • Spectroscopy: History 1885-1927
    SPECTROSCOPY: HISTORY 1885-1927 Harvard Observatory director Edward Charles Pickering hired over 80 women as technicians to perform scientific and mathematical calculations by hand. They became known as the “Harvard Computers”. This was more than 40 years before women gained the right to vote. They received global recognition for their contributions that changed the science of astronomy. Due to their accomplishments, they paved the way for other women to work in scientific and engineering careers. WHAT DID THEY DO: They studied glass photographic plates of stellar spectra created by using a spectroscope. Using a simple magnifying glass, they compared Credit: Secrets of the Universe: Space Pioneer, card 48 positions of stars between plates, calculating the temperature and motion of the stars. WHO WERE THEY: They measured the relative brightness of stars and analyzed spectra Some had college degrees, others received on-the job-training. to determine the properties of celestial objects. A few were permitted to receive graduate degrees for their accomplishments. These plates were gathered from observatories in Peru, South Africa, New Zealand, Chile and throughout the USA They worked for 25 cents an hour, six days a week in a small cramped library. Many of these women received numerous awards and honors for Harvard University Plates Stacks Digitization Project their contributions. Noteable among them were: Harvard College Observatory’s Plate Collection (also known as the Plate Stacks) is the world’s largest archive of stellar glass plate negatives. Taken between the mid 1880s and 1989 (with a gap 1953-68) the WILLIAMINA FLEMING (1857-1911) - developed the Pickering- collection grew to 500,000 and is currently being digitized.
    [Show full text]
  • From the Executive Director Kathryn Sullivan to Receive Sigma Xi's Mcgovern Award
    May-June 2011 · Volume 20, Number 3 Kathryn Sullivan to From the Executive Director Receive Sigma Xi’s McGovern Award Annual Report In my report last year I challenged the membership to consider ormer astronaut the characteristics of successful associations. I suggested that we Kathryn D. emulate what successful associations do that others do not. This FSullivan, the first year as I reflect back on the previous fiscal year, I suggest that we need to go even further. U.S. woman to walk We have intangible assets that could, if converted to tangible outcomes, add to the in space, will receive value of active membership in Sigma Xi. I believe that standing up for high ethical Sigma Xi’s 2011 John standards, encouraging the earlier career scientist and networking with colleagues of diverse disciplines is still very relevant to our professional lives. Membership in Sigma P. McGovern Science Xi still represents recognition for scientific achievements, but the value comes from and Society Award. sharing with companions in zealous research. Since 1984, a highlight of Sigma Xi’s Stronger retention of members through better local programs would benefit the annual meeting has been the McGovern Society in many ways. It appears that we have continued to initiate new members in Lecture, which is made by the recipient of numbers similar to past years but retention has declined significantly. In addition, the the McGovern Medal. Recent recipients source of the new members is moving more and more to the “At-large” category and less and less through the Research/Doctoral chapters. have included oceanographer Sylvia Earle and Nobel laureates Norman Borlaug, Mario While Sigma Xi calls itself a “chapter-based” Society, we have found that only about half of our “active” members are affiliated with chapters in “good standing.” As long Molina and Roald Hoffmann.
    [Show full text]
  • Women of Astronomy
    WOMEN OF ASTRONOMY AND A TIMELINE OF EVENTS… Time line of Astronomy • 2350 B.C. – EnHeduanna (ornament of heaven) – • Chief Astronomer Priestess of the Moon Goddess of the City in Babylonia. • Movement of the Stars were used to create Calendars • 2000 B.C. - According to legend, two Chinese astronomers are executed for not predicting an eclipse. • 129 B.C. - Hipparchos completes the first catalog of the stars, and invented stellar magnitude (still in use today!) • 150 A.D. - Claudius Ptolemy publishes his theory of the Earth- centered universe. • 350 A.D – Hypatia of Alexandria – First woman Astronomer • Hypatia of Alexandria Born approximately in 350 A.D. • Accomplished mathematician, inventor, & philosopher of Plato and Aristotle • Designed astronomical instruments, such as the astrolabe and the planesphere. The first star chart to have the name An early astrolabe was invented in "planisphere" was made in 1624 by 150 BC and is often attributed to Jacob Bartsch. Son of Johannes Hipparchus Kepler, who solved planetary motion. Time line of Astronomy • 970 - al-Sufi, a Persian Astronomer prepares catalog of over 1,000 stars. • 1420 Ulugh-Beg, prince of Turkestan, builds a great observatory and prepares tables of planet and stars • 1543 While on his deathbed, Copernicus publishes his theory that planets orbit around the sun. • 1609 Galileo discovers craters on Earth’s moon, the moons of Jupiter, the turning of the sun, and the presence of innumerable stars in the Milky Way with a telescope that he built. • 1666 Isaac Newton begins his work on the theory of universal gravitation. • 1671 Newton demonstrates his invention, the reflecting telescope.
    [Show full text]
  • Otto Stern Annalen 22.9.11
    September 22, 2011 Otto Stern (1888-1969): The founding father of experimental atomic physics J. Peter Toennies,1 Horst Schmidt-Böcking,2 Bretislav Friedrich,3 Julian C.A. Lower2 1Max-Planck-Institut für Dynamik und Selbstorganisation Bunsenstrasse 10, 37073 Göttingen 2Institut für Kernphysik, Goethe Universität Frankfurt Max-von-Laue-Strasse 1, 60438 Frankfurt 3Fritz-Haber-Institut der Max-Planck-Gesellschaft Faradayweg 4-6, 14195 Berlin Keywords History of Science, Atomic Physics, Quantum Physics, Stern- Gerlach experiment, molecular beams, space quantization, magnetic dipole moments of nucleons, diffraction of matter waves, Nobel Prizes, University of Zurich, University of Frankfurt, University of Rostock, University of Hamburg, Carnegie Institute. We review the work and life of Otto Stern who developed the molecular beam technique and with its aid laid the foundations of experimental atomic physics. Among the key results of his research are: the experimental determination of the Maxwell-Boltzmann distribution of molecular velocities (1920), experimental demonstration of space quantization of angular momentum (1922), diffraction of matter waves comprised of atoms and molecules by crystals (1931) and the determination of the magnetic dipole moments of the proton and deuteron (1933). 1 Introduction Short lists of the pioneers of quantum mechanics featured in textbooks and historical accounts alike typically include the names of Max Planck, Albert Einstein, Arnold Sommerfeld, Niels Bohr, Werner Heisenberg, Erwin Schrödinger, Paul Dirac, Max Born, and Wolfgang Pauli on the theory side, and of Konrad Röntgen, Ernest Rutherford, Max von Laue, Arthur Compton, and James Franck on the experimental side. However, the records in the Archive of the Nobel Foundation as well as scientific correspondence, oral-history accounts and scientometric evidence suggest that at least one more name should be added to the list: that of the “experimenting theorist” Otto Stern.
    [Show full text]
  • The Canadian Astronomical Handbook for 1908
    T h e Ca n a d i a n A stronomical H a n d b o o k FOR 1908 PUBLISHED BY THE ROYAL ASTRONOMICAL SOCIETY OF CANADA E d i t e d b y C. A. CHANT SECOND YEAR OF PUBLICATION TORONTO 198 C o l l e g e S t r e e t P r i n t e d f o r t h e S o c i e t y 1907 T h e Ca n a d i a n A stronomical H a n d b o o k FOR 1908 T h e Ca n a d ia n A stronomical H a n d b o o k FOR 1908 PUBLISHED BY THE ROYAL ASTRONOMICAL SOCIETY OF CANADA E d i t e d b y C. A. CHANT SECOND YEAR OF PUBLICATION TORONTO 198 C o l l e g e S t r e e t P r i n t e d f o r t h e S o c i e t y 1907 CONTENTS Page Preface.......................................................................... 5 Symbols and Abbreviations ....................................... 7 Chronological Eras and Cycles.................................... 8 Fixed and Movable Festivals, Etc.............................. 8 Standard Time..................................................... 9 Calendar for the Year . 9 to 33 Geographical Positions of Points in Canada............. 34 Magnetic Elements for Toronto, 1901-1906............... 36 The Solar System : Eclipses of Sun and Moon................................... 37 Principal Elements of the Solar System............ 39 Satellites of the Solar System............................. 40 The Planets in 1908, with Maps......................... 41 Meridian Passage of Five Planets..............................
    [Show full text]
  • Nobel Prize 1965
    Modern Trends in Basic and Applied Laser Spectroscopy Lund 6-7 April, 2010 Once upon a time there was no laser … How Science changed the course of World History How World History changed the course of Science Ingvar Lindgren: After-dinner speech Isaac Rabi (1898-1988) Inventor of ABMR – first radio- frequency-resonance method 1937 Nobel Prize 1944 Radio-frequency induced transitions The demonstration of induced transitions by Rabi represents the start of a new epoch in physics New resonance metods followed rapidly Nuclear Magnetic Resonance NMR discovered 1945 Felix Bloch Edward Purcell 1905-1983 1912-1997 Nobel Prize 1952 "for their development of new methods for nuclear magnetic precision measurements and discoveries in connection therewith" Nuclear Magnetic Resonance Imaging MRI Electron Spin (Paramagnetic) Resonance ESR/EPR Discovered in 1944 by E.K. Zavoisky, USSR, and B. Bleaney, Oxford Norman Ramsey 1915- Nobel Prize 1989 Separate oscillatory fields 1949 Led to the caesium clock and new def. of time 1967 NBS 1955:1sec/300y METAS/Switzerland 2004:1sec/30 000 000y 10-5 10-10 10-15 Accuracy of the Rydberg constant basis for next time standard? Willis Lamb (1913-2008) Nobel Prize 1955 "for his discoveries concerning the fine structure of the hydrogen spectrum" Lamb shift 1947 2s1/2 and 2p1/2 NOT degenerate Bengt Edlén, Lund, observed in early 1930’s significant deviation from Dirac theory in the fs for H-like ions. Existence of the shift known for some time The origin quite mysterious Oppenheimer suggested it was of quantum-el. dyn. origin Lamb thought it was of different origin Hyperfine separations differ from theory by 0.26 and 0.31 % Well outside the limits of error Rabi suspected erroneous fine-structure constant was used G.
    [Show full text]
  • Harvard's Computers
    Prior to the nineteenth-century, little is written of women’s contributions in astronomy. In most astronomy texts, you will find no mention of Hypatia of Alexandria, considered the first woman astronomer. Most historians consider her brutal death in the early fifth-century to be the beginning of the “Dark Ages.” There is no mention of Hildegard von Bingen (1099-1179) whose ideas on “universal gravitation” predate Isaac Newton’s, nor Sophia Brahe, Tycho’s younger sister. It was not until the director of Harvard Observatory became disgruntled with the sloppy work of his male assistant, saying his housekeeper could do better, that women were readily accepted into the study of astronomy. 1 Harvard College Observatory was founded in 1839, a time when astronomy was beginning to be taught as a science subject in its own right, instead of as an extension of philosophy. This was also a time when universities were receiving funds for astronomical research, an endeavor previously pursued by learned men of means. Astronomy is a science requiring observations and exact calculations, particularly of positions of celestial objects. This was tedious work completed by “computers.” Originally, young men performed these tasks. This changed when Edward Charles Pickering became director of the observatory in 1877 and opened the doors of astronomy to women. 2 Pickering was sympathetic to the women’s suffrage movement and recognized that there was a new breed of women, women that were educated. He also realized that with the new technologies of the time, telescopes that were readily available and astrophotography, that the data collection was happening faster than could be catalogued so as to be useful.
    [Show full text]