Medical Research in Great Britain

Total Page:16

File Type:pdf, Size:1020Kb

Medical Research in Great Britain 840 NATURE MAy 20, 1939, VOL. 143 or three years old), small fields with a considerable To judge by the data at our disposal, the Sedov quantity of hummocky ice prevailing. In the is in the belt of hummocky ice situated between region of the North Pole, old comparatively level the main mass of Arctic ice and the ice carried fields were the most common. At least a year or comparatively recently into the central basin from more is necessary for the Sedov ice to be trans­ the seas of the Soviet Arctic. This would explain formed into fields of this kind. the constant movement and jamming of the ice When flying from Franz Josef Land to the observed by the Sedov expedition. North Pole, the Soviet airmen first saw a belt of Finally, it is possible that the belt of hummocked comparatively young ice. This was followed near ice stretches along the trough of low pressure lat. 86° N. by a peculiar belt of hummocky or created by the inrush of masses of Atlantic air jagged ice, the origin of which has not been into the Arctic. This is all the more probable since sufficiently studied. Level fields of old ice stretched the passage of this air is usually accompanied by beyond this belt to the Pole itself. powerful winds. Medical Research in Great Britain fOR those who desire to obtain some conception the Institute to Mill Hill has involved reconsidera­ of the progress of medical research in Great tion of the proposed memorial to the late Sir Britain, no better means can be suggested than a Walter Fletcher. The original intention was to perusal of the latest annual report of the Medical apply the balance of the fund, after providing the Research Council*. Subjects to which the Council personal memorial, towards a new laboratory for wishes to direct special attention are reviewed in research on nutrition at Mill Hill. With the the introduction ; the remainder of the report transference of the Institute, this laboratory, falls naturally into several sections describing work instead of being the chief building on the site, will carried out for different Government Departments, occupy only a relatively subordinate position. It at the National Institute for Medical Research has been decided, therefore, with the agreement (including the Department ofBiological Standards), of the subscribers to the fund, to devote it to the by members of the Council's external scientific provision of a hall for meetings and lectures as an staff, and in clinical research units and in hospitals addition to the new Institute. The Council will and other institutions by investigators aided by meet the whole cost of the nutrition laboratory. grants. The Council also awards research fellow­ The Council points out that, during the past ships in tropical medicine, Rockefeller medical twenty-five years, since the Medical Research fellowships and Dorothy Temple Cross research Committee was first set up, there has been a great fellowships in tuberculosis. During the year, Prof. increase in knowledge of the body in health and A. J. Clark and Sir John Ledingham retired from disease, greater even than that of the previous the Council and Prof. C. R. Harington and Prof. twenty-five years. This new knowledge has had W. W. C. Topley were appointed to succeed them. two influences which, in their effect on medical The report mentions that a beginning has been practice, are often opposed to each other. In the made with the work of construction of the new first place it has resulted in a great improvement National Institute for Medical Research at Mill in methods of diagnosis and treatment of disease, Hill, to which reference was made in last year's which has involved a vast increase in medical report. At least two years, however, will be services. Many patients suffering from diseases required for completion. The new Institute will which, twenty-five years ago, were incurable and provide accommodation for the central laboratory uncontrollable can now be restored to health and under the national scheme for research in chemo­ well-being. At the same time new knowledge of therapy, of which an account was also given last curative treatment may in itself also bring about year. At present, research work is being gradually reduction in incidence of disease ; for example, developed by selected investigators at different the more rapid and effective cure of gonorrhma by centres, the Council having assumed responsibility drugs of the sulphanilamide group should result in for supporting the chemical as well as the biological a reduction in its incidence by reducing the spread investigations : previously the former were sup­ of the infection. Recent results also give hope that ported by the Department of Scientific and these drugs may lead to reduction of the number Industrial Research. The policy of transferring of cases of middle ear disease, which is responsible • Committee of the Privy Council for Medical Researeh. Report of for a large proportion of the cases of disabling the Medical Research Council for the Year 1937-38. (Cmd. 5939.) Pp. 221. (London : H.M. Stationery Office, 1939.) S.. 6d. net. deafness in Great Britain. ©1939 Nature Publishing Group No. 3629, MAY 20, 1939 NATURE 841 On the other hand, medical research has brought part of the work helped by the Council by means another kind of knowledge which, properly used, of personal and expenses grants, the initiative in leads directly to the prevention and elimination of choice of subject and method of investigation lies disease. The effect on medical practice is clearly with the head of the laboratory in respect of some opposed to the first-mentioned effect, since, by individual worker, or with the worker himself. eliminating disease, it tends to reduce the needs The Council considers that at the present time there for curative aids. The report points out that there is a relatively great dearth of work in clinical is often great delay in bringing about the applica­ science and in experimental pathology, so that tion of new discoveries to preventive ends. Fresh it is offering scholarships and fellowships to means of curative treatment, on the other hand, attract young investigators into these particular are generally applied within a short period of their fields of inquiry. discovery. This delay is considered to be due to An important duty of the Council is to help the fact that there is no means of educating the Government departments confronted with immedi­ public in the established advances in preventive ate problems of health and disease in the course medicine. It is responsible for much unnecessary of their work. The report describes briefly some suffering. The report illustrates this point by of the main investigations now being made. reference to the prevention of diphtheria and to Important research on nutrition in the Colonial the value of improved nutrition. Where preventive Empire has been carried out in association with inoculation with diphtheria toxoid has been the Colonial Office. In Nyasaland, the dietetic and generally adopted, diphtheria as a clinical entity nutritional conditions of the people are being has practically disappeared: yet in 1937 there accurately assessed and related to other surveys were more than 61,000 cases in England and of the agricultural and social conditions. It is Wales, with almost 3,000 deaths. The report urges hoped thereby to determine methods of producing parents to demand this prophylactic inoculation those agricultural products which will cause a for their children, and considers that there is no great improvement in the physical condition of doubt that its general adoption would lead to the the population. It is also hoped that this survey virtual disappearance of the disease from Great may form a model for many similar studies else­ Britain. where in the Colonial territories. Other investiga­ The need for improved nutrition has been tions made for Government departments relate to discussed in previous reports, but the adop­ the nature and causes of chronic lung disease in tion of modern teaching in the subject is still coal miners, and to the dangers to health which depressingly slow: a much greater consumption may follow the use of certain organic substances of milk and other dairy products, of eggs, vege­ as solvents in industry. Research has been made tables and fruit and of fat fish at the expense of into the best methods of ridding houses of the bread, biscuits, sugar and sweets, will improve the bed-bug; it is hoped by this work to discover new physique of the people, reduce the amount of insecticides for the purpose which are rapid in dental decay and greatly raise the standard of action, safe and cheap ; good results have already health. An increased consumption of the 'pro­ been reported from fumigation with heavy naphtha. tective' foods would also be of great economic The report describes results obtained in the value to the country. treatment of cancer of the mouth, tongue, pharynx The Council is sometimes asked what is its and larynx by radium beam therapy; most of policy in promoting research : whether it favours the patients have been in an advanced and research on disease itself rather than on more inoperable stage of cancer, but the results appear academic problems of physiology and biochemistry. to compare favourably with those to be expected The general answer is that it welcomes both kinds from surgery. Of even greater importance than of investigation. Promotion of specific research by the actual therapeutic results are the new technical the Council is usually done by appointment of methods which have been elaborated as the result individuals to its permanent staff, the choice of close co-operation between physicists and depending on the subject which seems to require clinicians : they are already being widely used as special attention and the merits of the person models to be followed in researches in radiotherapy chosen.
Recommended publications
  • Eclipse Science Results: Past and Present
    The Last Total Solar Eclipse of the Mil lennium in Turkey ASP Conference Series Vol W Livingston and A Ozgu c eds Eclipse Science Results Past and Present W Livingston National Solar Observatory NOAO PO Box Tucson AZ USA S Koutchmy Institut dAstrophysique de ParisCNRS Bis Boulevard Arago F Paris France Abstract We review the signicant advances that havebeenachieved by eclipse exp eriments First we note the anomaly that the corona was not even seen until relatively mo dern times Beginning in whitelight WL photographs suggested structures that must have b een dominated by magnetic elds This led to the disco very of surface magnetism in sunsp ots by Hale in the rst detection of cosmic magnetism Deli cate direct photographic observations conrmed the b ending of starlight near the eclipsed Sun as predicted by Einsteins General Theory of Rela tivity Chromospheric ash sp ectra indicated that the outer layer of the Sun was much hotter than the underlying photosphere leading to non lo cal thermo dynamic equilibrium concepts and the idea of various me chanical and wave pro cesses to maintain it Decades have been devoted to understanding the corona Discovery of its million degree plus tem p erature and guring howto heat it how co ol prominences can coexist within it all are topics to which eclipse observations havecontributed Totality without a Corona Eclipses have b een chronicled for o ver years but the corona escap ed b eing noticed until mo dern times The single exception Leonis Deaconis in AD mentions a certain dull and feeble glow
    [Show full text]
  • EPSC2015-913, 2015 European Planetary Science Congress 2015 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2015
    EPSC Abstracts Vol. 10, EPSC2015-913, 2015 European Planetary Science Congress 2015 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2015 The “Station de Planétologie des Pyrénées” (S2P), a collaborative science program in the course of a long history at Pic du Midi observatory. F. Colas (1), A. Klotz (2), F. Vachier (1), M. Birlan (1), B. Sicardy (3), J. Lecacheux (3), M. Antuna (6), R. Behrend (4), C. Birnbaum (6), G. Blanchard (6), C. Buil (4,5), J. Caquel (6), M. Castets (5), C. Cavadore (4), B. Christophe (6), F. Cochard (4), J.L. Dauvergne (6), F. Deladerriere (6), M. Delcroix (6), V. Denoux (4), J.B. DeVanssay (6), P. Devechere (6), P. Dupouy (5), E. Frappa (6), S. Fauvaud (5), B. Gaillard (6), F. Jabet (6), M. Lavayssiere (6), T. Legault (6), A. Leroy (5), A. Maury (6), M. Meunier (6), C. Pellier (6), C. Rinner (4), E. Rolland (6), O. Stenuit (6), I. Testar (6), P. Thierry (4), O. Thizy (4), B. Tregon (5), F. Vaissiere (4), S. Vauclair (6), C. Viladrich (6), C. Angeli (6), J.E. Arlot (1), M. Assafin (28), D. Bancelin (1), D. Baratoux (29), N. Barrado-Izagirre (8), M.A. Barucci (3), L. Beauvalet (9), P. Bendjoya (13), J. Berthier (1), N. Biver (3), D. Bockelee-Morvan (3), D. Berard (3), S. Bouley (10), S. Bouquillon (9), P. Bourget (11), F. Bragas- Ribas (7), J. Camargo (7), B. Carry (1), S. Chevrel (2), M; Chevreton, (3), P. Colom (3), J. Crovisier (3), J. Demars (1), R. Despiau (2), P. Descamps (1), N. Dolez (2), A.
    [Show full text]
  • February 2014 the Newsletter of the Barnard-Seyfert Astronomical Society
    February TheECLIPSE 2014 The Newsletter of the Barnard-Seyfert Astronomical Society From the President Next Membership Meeting: February 19, 2014, 7:30 pm Cumberland Valley Professionals vs. amateurs… the distinctions have Girl Scout Council Building blurred over the years in different ways. There was 4522 Granny White Pike a time when mere money could get you the gear to have a professional observatory. Many large Program Topic: telescopes were built with private funds by Joshua Emery - interested individuals… think of William Hershel and the “Don Quixote” object (details on page 5) Percival Lowell. Then amateurs were pushed aside by large scale photography and the truly large telescopes that needed institutions to care for and run them… like the Mt. Wilson and Mt. Palomar observatories. Expensive ccd cameras, exotic cooling, the computing power needed even after In this Issue: glass plates were replaced put meaningful observations out of reach of amateurs. Then with President’s Message 1 the advent of the personal computer and digital Observing Highlights 2 cameras, the playing field was leveled by computers that anyone could own, low noise digital Happy Birthday, cameras and powerful software. Bernard Ferdinand Lyot by Robin Byrne 3Today, you can take the hobby or second life in astronomy as far as you wish, in partnership with Board Meeting Minutes January 8, 2014 6professionals. On any given clear night, enthusiasts around the world are recording not just pretty Membership Meeting Minutes pictures, but data. Our sheer numbers allow us to January 15, 2013 9look at things in depth and at a frequency not possible if we depended just on the large research Membership Information 10 telescopes.
    [Show full text]
  • CIRCULAR No. 163 (OCTOBER 2007)
    INTERNATIONAL ASTRONOMICAL UNION COMMISSION 26 (DOUBLE STARS) INFORMATION CIRCULAR No. 163 (OCTOBER 2007) NEW ORBITS ADS Name P T e ­(2000) 2007 Author(s) ®2000± n a i ! Last ob. 2008 450 A 111 AB 21y38 1947.17 0.020 104±5 156±7 000156 BRENDLEY 00321-0511 16.8382 000172 150±0 18±7 1994.7083 139.5 0.161 & HARTKOPF 504 A 914 467. 1905.32 0.107 35.3 24.2 0.436 LING 00366+5609 0.7709 0.468 118.2 291.9 2005.034 23.8 0.435 865 MLR 87 55.97 2020.45 0.513 139.7 29.0 0.240 BRENDLEY 01036+6341 6.4320 0.238 145.1 246.4 2003.9517 24.4 0.233 & MASON 1538 STF 186 165.72 1892.28 0.726 219.7 65.0 0.906 BRENDLEY 01559+0151 2.1723 0.986 72.4 40.2 2006.9180 65.6 0.888 & MASON 3032 A 469 124.87 1968.61 0.885 236.8 320.3 1.723 BRENDLEY 04093-0756 2.8830 2.435 65.5 277.0 1996.8984 321.4 1.736 & MASON - CHR 17 13.93 1995.87 0.600 125.3 290.7 0.168 CVETKOVIC 04340+1510 25.8455 0.150 45.4 297.9 2001.7531 304.7 0.135 3389 A 1014 74.83 1969.67 0.465 111.9 10.2 0.349 BRENDLEY 04430+5712 4.8109 0.244 13.0 78.8 1999.8859 12.3 0.348 & HARTKOPF - BTZ 1Aa 18.75 1992.57 0.297 120.9 265.0 0.040 CVETKOVIC 06290+2013 19.1992 0.081 72.9 228.4 1997.1366 281.9 0.053 5625 A 2681 208.33 1938.47 0.793 118.2 329.9 0.442 BRENDLEY 06575+0253 1.7280 0.273 119.4 339.1 1997.2000 329.6 0.445 & MASON 6796 HU 856 80.35 1949.90 0.589 185.5 299.7 0.231 BRENDLEY 08254+3723 4.4804 0.201 36.2 263.6 2004.2017 302.0 0.228 & HARTKOPF 7555 AC 5 AB 77.82 1957.65 0.736 194.7 53.1 0.585 BRENDLEY 09525-0806 4.6261 0.397 141.1 303.3 2006.3199 51.9 0.582 & HARTKOPF 1 NEW ORBITS (continuation) ADS Name P T e ­(2000) 2007 Author(s) ®2000± n a i ! Last ob.
    [Show full text]
  • Observation of Venus and Mercury Transits from the Pic-Du-Midi Observatory
    MEETING VENUS C. Sterken, P. P. Aspaas (Eds.) The Journal of Astronomical Data 19, 1, 2013 Observation of Venus and Mercury Transits from the Pic-du-Midi Observatory Guy Ratier 43 rue des Longues All´ees, F-45800 Saint-Jean-de-Braye, France Sylvain Rondi Soci´et´eAstronomique de France, 3 rue Beethoven, F-75016 Paris France Abstract. The Pic-du-Midi, on the French side of the Pyr´en´ees, became a state observatory in the summer of 1882. The first major astronomical event to be observed was the Venus transit of 6 December 1882. Unfortunately this attempt by the well-known Henry brothers was unsuccessful due to bad weather conditions. During the twentieth century, the Pic-du-Midi became famous for the quality of its solar and planetary observations. In the sixties, Jean R¨osch decided to use this experience to monitor the transits of Mercury. The objective was not to measure the parallax, but to determine the diameter of the planet in order to confirm its high density. Observations were made using a photometric method – the Hertzsprung method – during the transits of 1960, 1970 and 1973. The pioneer work of Ch. Boyer on the rotation of the Venus atmosphere as well as some experiments involving Lyot coronographs are also noteworthy. A Venus transit was finally observed on 8 June 2004 with a new CCD camera, providing a significant contribution to the model of the Venus mesosphere. This opened the field for new observations in 2012. 1. Early days of the Pic-du-Midi Observatory The site of the “Pic-du-Midi de Bigorre”, on the forefront of the Pyr´en´ees, has been known since ages as an ideal location to carry out astronomical observations.
    [Show full text]
  • Istros 2013 Proceedings Download Link
    Proceedings of the ISTROS 2013 International Conference Editors: M. Veselský and M. Venhart INSTITUTE OF PHYSICS, SLOVAK ACADEMY OF SCIENCES Bratislava 2015 ISBN 978-80-971975-0-6 Dear participants, we bring to you the proceedings of the conference ISTROS (Isospin, STructure, Reactions and energy Of Symmetry), which took place in the period between Sept 23 – - for meeting of Sept 27 2013 in Častá withPapiernička. experimental The declared and theoretical aim of theaspects conference of physics was of to exotic provide nuclei platform and states of nuclear international and Slovak scientists, active in the field of nuclear physics, specifically dealing matter, and we hope that this aim was fulfilled. presentationDuring the conference, is represented 36 invited in this and proceedings contributed in talks the formwere ofpresented, short artic coveringles, while the otheropen participantsproblems in decidedthe physics to abstain of exotic from nuclei this and thusof the their states presentations of nuclear matter.are represented Part of these only by their abstracts. In general, present time appears to modify traditional procedures and one of the victims are the conference proceedings in their habitual form. We are still convinced complementthat publication the of proceedi proceedingsngs iswith a part a briefof our summaryduties as organizersof history as of a servicenatural to sciences participants and and with this in mind we bring to you these proceedings. Besides the contributed articles, we technology in the territory of Slovakia, which bring some interesting facts about the progress of scientific and technical knowledge in Slovakia. - discussing interesting physics, and thus we aim to bring the second edition of the ISTROS As far as we can judge, you had a productive time at Častá Papiernička, spent meaningfully conference in the near future.
    [Show full text]
  • 1 Accepted for Publication in the Journal of the British
    1 David Elijah Packer: cluster variables, meteors and the solar corona Jeremy Shears Abstract David Elijah Packer (1862-1936), a librarian by profession, was an enthusiastic amateur astronomer who observed from London and Birmingham. He first came to the attention of the astronomical community in 1890 when he discovered a variable star in the globular cluster M5, only the second periodic variable to be discovered in a globular cluster. He also observed meteors and nebulae, on one occasion reporting a brightening in the nucleus of the galaxy M77. However, his remarkable claims in 1896 that he had photographed the solar corona in daylight were soon shown to be flawed. Biographical sketch David Elijah Packer was born in Bermondsey, London, in 1862 April (1) the eldest child of Edward Packer (1820-1896) and Emma (Bidmead) Packer (1831-1918) (2). David attended the Free Grammar School of Saint Olave and Saint John at Southwark, where he performed well, especially in arithmetic, algebra and general mathematics (3). Edward Packer was a basket maker, as was his father and grandfather before him, the Packer family originally coming to London from Thanet, in Kent. The English basket-making industry was in decline during the second half of the nineteenth century due to the availability of cheaper imports from the continent. In spite of this, Edward was still in business in 1881, but the prospects for his son continuing in a trade that had made a living for generations of his ancestors were probably limited (4). Thus at the age of 18 we find David Elijah Packer working as an Oilman’s Assistant, supplying fuel for the oil lamps of London (5).
    [Show full text]
  • Communications in Observations
    ISSN 0917-7388 COMMUNICATIONS IN CMO Since 1986 MARS No.378 25 November 2010 OBSERVATIONS No.04 PublishedbytheInternational Society of the Mars Observers Audouin Charles DOLLFUS, 1924-2010 By Richard McKIM ith the death of Audouin Dollfus W(Figure 1), a few weeks prior to his 86th birthday, planetary astronomy has lost one of its greatest exponents. He was born in Paris on 1924 November 12, son of famous balloonist and airship pilot Charles Dollfus. Later, Audouin would set several world records for balloon flights. At age 14 he made himself a small refractor, and by 1943 a 20 cm Newtonian reflector. Despite few meters stood Gabrielle Flammarion, E‐M. wartime restrictions he was also able to ob‐ Antoniadi, F. Baldet, A. Danjon, G. de serve with the instruments of the observatory Vaucouleurs and many other planetary ob‐ of the Société astronomique de France at the servers whose names have passed into histo‐ Sorbonne, where his mentor was Romanian ry. Within a year the German occupation amateur and fellow University student Jean would be over. Fifty years later I stood in the Dragesco. same spot with Dollfus and Juvisy’s curator One day in the summer of 1943 there as‐ Jacques Pernet when we inspected the prepa‐ sembled a galaxy of French astronomers at rations being made to preserve this famous the graveside of SAF founder Camille butbythenrun‐down estate. During his Flammarion, for the annual celebration of the Presidency of the SAF in the 1980s, Dollfus life of that great populariser. Dollfus was in had started the restoration ball rolling, and goodcompanyatJuvisythatday:withina this year Flammarion’s famous telescope will Ser3-0049 CMO No.
    [Show full text]
  • Encke's Minima and Encke's Division in Saturn's A-Ring
    ENCKE’S MINIMA AND ENCKE’S DIVISION IN SATURN’S A-RING Pedro Ré http://astrosurf.com/re When viewed with the aid of a good quality telescope Saturn is undoubtedly one of the most spectacular objects in the sky. Many amateur astronomers (including the author) say that their first observation of Saturn turned them on to astronomy. Saturn’s rings are easily visible with a good 60 mm refractor at 50x. The 3D appearance of this planet is what makes it so interesting. Details in the rings can be seen during moments of good seeing. The Cassini division (between ring A and B) is easily visible with moderate apertures. The Encke minima and Encke division are more difficult to observe and require large apertures and telescopes of excellent optical quality. These two features can be observed in Saturn’s A-Ring. The Encke minima consists of a broad, low contrast feature located about halfway out in the middle of the A-Ring. The Encke division is a narrow, high contrast feature located near the outer edge of the A-Ring. Unlike the Encke minima, the Encke division is an actual division of the ring (Figure 1). Figure 1- Saturn near Opposition on June 11, 2017. D. Peach, E. Kraaikamp, F. Colas, M. Delcroix, R. Hueso, G. Thérin, C. Sprianu, S2P, IMCCE, OMP. The Encke division is visible around the entire outer A ring. Astronomy Picture of the Day (20170617) https://apod.nasa.gov/apod/ap170617.html 1 Galileo Galilei observed the disk Saturn for the first time using one of his largest refractor.
    [Show full text]
  • Solar Surveillance with CLIMSO: Instrumentation, Database and On-Going Developments
    J. Space Weather Space Clim. 2020, 10,47 Ó F. Pitout et al., Published by EDP Sciences 2020 https://doi.org/10.1051/swsc/2020039 Available online at: www.swsc-journal.org Topical Issue - Space Weather Instrumentation TECHNICAL ARTICLE OPEN ACCESS Solar surveillance with CLIMSO: instrumentation, database and on-going developments Frédéric Pitout1,*, Laurent Koechlin1, Arturo López Ariste1, Luc Dettwiller2, and Jean-Michel Glorian1 1 IRAP, Université Toulouse 3, CNRS, CNES, 9 Avenue du Colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France 2 Higher Education Section of Lycée Blaise Pascal, 36 Avenue Carnot, 63037 Clermont-Ferrand Cedex, France Received 1 May 2020 / Accepted 27 July 2020 Abstract – CLIMSO is a suite of solar telescopes installed at Pic du Midi observatory in the southwest of France. It consists of two refractors that image the full solar disk in Ha and CaII K, and two coronagraphs that capture the prominences and ejections of chromospheric matter in Ha and HeI. Synoptic observations are carried out since 2007 and they follow those of previous instruments. CLIMSO, together with its predecessors, offer a temporal coverage of several solar cycles. With a direct access to its images, CLIMSO contributes to real time monitoring of the Sun. For that matter, the national research council for astrophysics (CNRS/INSU) has labelled CLIMSO as a national observation service for “surveillance of the Sun and the terrestrial space environment”. Products, under the form of images, movies or data files, are available via the CLIMSO DataBase. In this paper, we present the current instrumental configuration; we detail the available products and show how to access them; we mention some possible applications for solar and space weather; and finally, we evoke developments underway, both numerical to valorise our data, and instrumental to offer more and better capabilities.
    [Show full text]
  • Gerard Peter Kuiper
    NATIONAL ACADEMY OF SCIENCES G ERARD PETER K UIPER 1905—1973 A Biographical Memoir by D A L E P . CRUIKSHANK Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1993 NATIONAL ACADEMY OF SCIENCES WASHINGTON D.C. GERARD PETER KUIPER December 7, 1905-December 24, 1973 BY DALE P.CRUIKSHANK OW DID THE SUN and planets form in the cloud of gas H and dust called the solar nebula, and how does this genesis relate to the formation of other star systems? What is the nature of the atmospheres and the surfaces of the planets in the contemporary solar system, and what have been their evolutionary histories? These were the driv- ing intellectual questions that inspired Gerard Kuiper's life of observational study of stellar evolution, the properties of star systems, and the physics and chemistry of the Sun's family of planets. Gerard Peter Kuiper (originally Gerrit Pieter Kuiper) was born in The Netherlands in the municipality of Haringcarspel, now Harenkarspel, on December 7, 1905, son of Gerrit and Antje (de Vries) Kuiper. He died in Mexico City on December 24, 1973, while on a trip with his wife and his long-time friend and colleague, Fred Whipple. He was the first of four children; his sister, Augusta, was a teacher before marriage, and his brothers, Pieter and Nicolaas, were trained as engineers. Kuiper's father was a tailor. Young Kuiper was an outstanding grade school student, but for a high school education he was obliged to leave his small town and go to Haarlem to a special institution that would lead him to a career as a primary school teacher.
    [Show full text]
  • French Astronomers, Visual Double Stars and the Double Stars Working Group of the Société Astronomique De France Edgar J
    French astronomers, visual double stars and the double stars working group of the Société Astronomique de France Edgar J. Soulié Société Astronomique de France 3, rue Beethoven 75016 PARIS France 1. A long tradition : The discovery of the orbital motion of visual double stars by William Herschel aroused the interest of French astronomers for the observation of double stars and the computation of their orbits at the beginning of the XIX-th century. Thus, the first orbit determination, pertaining to the binary ksi Ursae Majoris, was made by Félix Savary in 1827 (1). About twenty years later, Antoine Yvon Villarceau, whose career was surprisingly varied (see his biography in ref. 2), proposed an elegant method for the determination of the apparent orbit and an algorithm to deduce the real orbit (3). Camille Flammarion, the founder of the Société Astronomique de France whose biography was published in 1994 (4), observed visual double stars, calculated orbits and published in 1878 a book entitled "Catalogue des étoiles doubles et multiples en mouvement relatif certain..." (5). Guillaume Bigourdan, inventor of a method for setting an equatorial instrument into an appropriate position which bears his name, observed them between 1880 and 1895, and analyzed the personal factor in the measurement process (6). In the second volume of his treatise on stellar astronomy (7), Charles André devoted seven chapters to binary stars, in which the knowledge of the time on the various categories of double stars are gathered. In particular, methods for orbit determination are given for each category. In this treatise, he published among other things the list of binaries, the orbits of which were known in 1900.
    [Show full text]