2 Anton Pannekoek's Astronomy in Relation to His Political Activities
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Telling the Truth About Class
TELLING THE TRUTH ABOUT CLASS G. M. TAMÁS ne of the central questions of social theory has been the relationship Obetween class and knowledge, and this has also been a crucial question in the history of socialism. Differences between people – acting and knowing subjects – may influence our view of the chances of valid cognition. If there are irreconcilable discrepancies between people’s positions, going perhaps as far as incommensurability, then unified and rational knowledge resulting from a reasoned dialogue among persons is patently impossible. The Humean notion of ‘passions’, the Nietzschean notions of ‘resentment’ and ‘genealogy’, allude to the possible influence of such an incommensurability upon our ability to discover truth. Class may be regarded as a problem either in epistemology or in the philosophy of history, but I think that this separation is unwarranted, since if we separate epistemology and the philosophy of history (which is parallel to other such separations characteristic of bourgeois society itself) we cannot possibly avoid the rigidly-posed conundrum known as relativism. In speak- ing about class (and truth, and class and truth) we are the heirs of two socialist intellectual traditions, profoundly at variance with one another, although often intertwined politically and emotionally. I hope to show that, up to a point, such fusion and confusion is inevitable. All versions of socialist endeavour can and should be classified into two principal kinds, one inaugurated by Rousseau, the other by Marx. The two have opposite visions of the social subject in need of liberation, and these visions have determined everything from rarefied epistemological posi- tions concerning language and consciousness to social and political attitudes concerning wealth, culture, equality, sexuality and much else. -
Byurakan Astrophysical Observatory Annual Report 2015
General News Byurakan Astrophysical Observatory Annual Report 2015 Introduction In 2015, Byurakan astronomers continued and developed scientific projects related to instability phenomena in the Universe resulted in a number of important discoveries, active international collaboration, a number of research grants by Byurakan astronomers, organization of a number of meetings, etc. BAO scientists had 2 ANSEF grants in 2015, as well as a French-Armenian (CNRS-SCS) joint project for 2014-2015. 5 BAO astronomers were listed among the most productive scientists in Armenia. There have been 17 publications in refereed journals, including most important international ones (ApJ, A&A, MNRAS), 3 electronic catalogs in VizieR, 2 books (Proceedings of meetings held in Byurakan), and 40 papers in Proceedings of meetings, including 18 in the Proceedings of Byurakan-Abastumani Colloquium “Instability and Evolution of Stars” held in 2013 and 19 in the Proceedings of the meeting “Relation of Astronomy to other Sciences, Culture and Society” held in 2014. There were 40 missions for research and participation in meetings and schools. Probably the most important event was the establishment in Armenia of the IAU South West Asian Regional Office of Astronomy for Development (SWA ROAD). The Inauguration Ceremony was held on Oct 13, and an attached Workshop was organized with participation of representatives from IAU and IAU OAD Officers and regional countries (Armenia, Georgia, Iran, Israel, Jordan, Russia and Turkey). The Office will operate until 2021 with further extension plans to 2030. A project of Digitization and Scientific Usage of BAO Plate Archive was conducted in April 2015. It is aimed at at compilation, accounting, digitization of BAO observational archive photographic plates and films, as well as their incorporation in databases with modern standards and methods, providing access for all observational material and development of new scientific programs based on this material. -
Henriette Roland Horst, Jacques Engels and the Influence of Class
‘More freedom’ or ‘more harmony’? Henriette Roland Holst, Jacques Engels and the influence of class and gender on socialists’ sexual attitudes Paper submitted to the seminar on “Labour organizations and sexuality”, Université de Bourgogne, Dijon 5 October 2001 Peter Drucker1 Sheila Rowbotham once wrote, ‘A radical critical history ... requires a continuing movement between conscious criticism and evidence, a living relationship between questions coming from a radical political movement and the discovery of aspects of the past which would have been ignored within the dominant framework.’2 Her words may apply with particular force to the history of labour organizations and sexuality. Historians can find it easier to find criticisms and questions to raise about the past than to sustain the ‘continuing movement’ required to understand the past in its own terms. The temptation is great to compare positions on sexuality taken in labour organizations in the past with positions held by historians in the present. The result can be either an idealization of sex-radical forbears or a condemnation of those whose ideas fell short of twenty-first-century enlightenment — in either case a curiously old-fashioned sort of history, which benefits little from the advances made by social historians outside ‘the dominant framework’, particularly social historians of sexuality, since the 1970s. Analyzing positions on sexuality taken in labour organizations in the past in the light of knowledge that has been accumulating about social and sexual patterns of their specific periods seems likely to be a more fruitful approach. Four different angles of attack seem particularly likely to be useful. -
Review Section
CSIRO PUBLISHING www.publish.csiro.au/journals/hras Historical Records of Australian Science, 2004, 15, 121–138 Review Section Compiled by Libby Robin Centre for Resource and Environmental Studies (CRES), Australian National University, Canberra, ACT, 0200, Australia. Email: [email protected] Tom Frame and Don Faulkner: Stromlo: loss of what he described as a ‘national an Australian observatory. Allen & Unwin: icon’. Sydney, 2003. xix + 363 pp., illus., ISBN 1 Institutional histories are often suffused 86508 659 2 (PB), $35. with a sense of inevitability. Looking back from the security of a firmly grounded present, the road seems straight and well marked. The journey that is reconstructed is one where the end point is always known, where uncertainties and diversions are forgotten — a journey that lands neatly on the institution’s front doorstep. Institu- tional histories are often burdened, too, by the expectation that they will not merely tell a story, but provide a record of achieve- ment. Written for the institution’s staff, as well as broader public, they can become bogged down in the details of personnel and projects. In this case, the fires of January 2003 add an unexpected final act Few institutional histories could boast such to what is a fairly traditional story of a dramatic conclusion as Stromlo: an Aus- growth and success. The force of nature tralian observatory. The manuscript was intervenes to remind us of the limits of substantially complete when a savage fire- inevitability, to fashion from the end point storm swept through the pine plantations another beginning. flanking Mount Stromlo, destroying all the The book is roughly divided into halves. -
William Liller (1927–2021)
Bulletin of the AAS • Vol. 53, Issue 2 William Liller (1927–2021) Alan Hirshfeld1, Christine Jones2, William Forman2 1UMass Dartmouth, 2Center for Astrophysics | Harvard & Smithsonian Published on: Apr 07, 2021 DOI: 10.3847/25c2cfeb.97f3253d License: Creative Commons Attribution 4.0 International License (CC-BY 4.0) Bulletin of the AAS • Vol. 53, Issue 2 William Liller (1927–2021) William Liller died on Sunday the 28th of February 2021. William (“Bill”) Liller, research mentor and major contributor to the study of planetary nebulae, comets, asteroids, magnetic activity in cool stars, the optical identification of X-ray sources, and astro-archaeology, died peacefully in his sleep on 28 February 2021, after a brief illness. He was 93 years old. Born on 1 April 1927 in Philadelphia to Carroll Kalbaugh “Pete” Liller, an advertising executive, and his wife, Catherine Dellinger Liller, Bill noted in the book “Asteroids to Quasars” that he became “obsessed with astronomy” in Photo courtesy Clive Grainger. August 1932, when his uncle drove up from West Virginia in a Model A Ford to view a solar eclipse from New York, near where Bill’s family was living at the time. At age 13, Bill’s report on the Quadrantid meteor shower was cited in an article in Popular Astronomy from the American Meteor Society. In his letter to the society, Bill had misspelled the name of the society’s director, C. P. Olivier, which Bill believed led to an intentional misspelling of his own name in the published article as “Billy Lillier.” In the February 2018 issue of the alumni magazine of Harvard’s Adams House, Bill recalled the years leading up to his matriculation in 1944: “After attending public schools in my home town of Atlanta, I was shipped off ‘to finish,’ and I spent my last two high school years at Mercersburg Academy in Pennsylvania. -
Ira Sprague Bowen Papers, 1940-1973
http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington. -
Pos(Westerbork)002 Historical Introduction Historical S 4.0 International License (CC BY-NC-ND 4.0)
Historical Introduction PoS(Westerbork)002 Richard Strom ASTRON Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands E-mail: [email protected] 50 Years Westerbork Radio Observatory, A Continuing Journey to Discoveries and Innovations Richard Strom, Arnold van Ardenne, Steve Torchinsky (eds) Published with permission of the Netherlands Institute for Radio Astronomy (ASTRON) under the terms of the Creative CommonsAttribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). Chapter 1 Historical introduction Richard Strom* rom the English longbows at the battle of Crécy (1346) to Winston Chur- chill’s world war I mobilized cannon (its true identity hidden behind the Fpseudonym “[water] tank”), warfare has always pushed technological innovation to new fronts. The second world war (WWII) was no exception. It gave us technology ranging from the dynamo-powered flashlight (a Philips invention) to jet engines, and space-capable rockets (Germany’s V2), not to mention (in a completely different realm) the mass production of Penicillin. In fact, it could be argued that WWII inventions marked the inception of the modern technological era1. In the field of electronics, the war led to innovations such as radio navigation, aircraft landing systems, and radar. It was these developments which were to * ASTRON, Univer- sity of Amsterdam, have a revolutionary impact on astronomy, initially in Britain, Australia and the The Netherlands United States. But the story begins in the US, with the electronics of the 1920s and ‘30s. Figure 1. Karl G. Jansky (c. 1933) Around 1930, there was increasing interest in the use of radio frequencies for communication. One of the main players, the Bell Telephone Laboratories in New Jersey, asked their research engineer, Karl Jansky (Figure 1), to investigate the inter- ference environment in the “short-wave” band around 20 MHz. -
German Politics and the 'Jewish Question', 1914-1919
German Politics and the 'Jewish Question', 1914-1919 Lucia Juliette Linares Darwin College Dissertation submitted for the degree of Doctor of Philosophy August 2019 PREFACE I hereby declare that this dissertation is the result of my own work and includes nothing which is the outcome of work done in collaboration except as declared in the preface and specified in the text. It is not substantially the same as any other work that I have submitted, or, is being concurrently submitted for a degree or diploma or other qualification at the University of Cambridge or any other university or similar institution except as declared in the preface and specified in the text. I further state that no substantial part of my dissertation has already been submitted, or, is being concurrently submitted for any such degree, diploma or other qualification at the University of Cambridge or any other university or similar institution except as declared in the preface and specified in the text. It does not exceed the prescribed word limit for the Faculty of History. All translations are my own unless specified in the text. i ABSTRACT German Politics and the 'Jewish Question', 1914-1919 Lucia Juliette Linares The First World War confronted German politicians with a range of unprecedented, vital questions in the spheres of domestic as well as foreign policy. As the fortunes of war shifted, so did borders, populations and national allegiances. In a period of acute and almost constant political crisis, the German government faced issues concerning citizenship, minority rights, religious identity, nationhood and statehood. My dissertation analyses these issues through the prism of the so-called 'Jewish Question'. -
Marcel Minnaert, Astrofysicus 1893-1970
Marcel Minnaert, astrofysicus 1893-1970 De rok van het universum Leo Molenaar bron Leo Molenaar, Marcel Minnaert, astrofysicus 1893-1970. De rok van het universum. Balans, Amsterdam / Van Halewyck, Leuven 2003 Zie voor verantwoording: http://www.dbnl.org/tekst/mole016marc01_01/colofon.htm © 2007 dbnl / Leo Molenaar 4 In deze tijd heeft wat men altijd noemde Schoonheid, schoonheid haar gezicht verbrand Zij troost niet meer de mensen Zij troost de larven de reptielen de ratten Maar de mens verschrikt zij En treft hem met het besef Een broodkruimel te zijn op de rok van het universum (Uit Lucebert, ik tracht op poëtische wijze, Verzamelde gedichten, Amsterdam 2002, pag. 52) Leo Molenaar, Marcel Minnaert, astrofysicus 1893-1970 7 Proloog Marcel Minnaert (1893-1970): Erflater van de Groot-Nederlandse beschaving Er zijn heel wat mensen voor wie de naam van Minnaert nog een dierbare klank heeft. Dat geldt in ieder geval voor leraren in de natuurwetenschap die houden van waarnemingen in de vrije natuur. Mijn eerste kennismaking met hem had dan ook plaats via de Minnaert: zo heten de drie delen van De Natuurkunde van 't Vrije Veld die ik omstreeks 1970 heb aangeschaft. De eerste druk van dit boek verscheen eind jaren dertig. In de jaren negentig kwamen van het eerste deel van Minnaerts trilogie, Licht en kleur in het landschap, nieuw geïllustreerde uitgaven in het Engels en Duits op de markt naast de herdruk van de Minnaert in het Nederlands. Het is dan ook een uniek boek. Minnaert had vijfentwintig jaar lang natuurverschijnselen geobserveerd, daar aantekeningen van gemaakt en onderzoek gedaan naar de fysische verklaringen. -
Appendix A: Scientific Notation
Appendix A: Scientific Notation Since in astronomy we often have to deal with large numbers, writing a lot of zeros is not only cumbersome, but also inefficient and difficult to count. Scientists use the system of scientific notation, where the number of zeros is short handed to a superscript. For example, 10 has one zero and is written as 101 in scientific notation. Similarly, 100 is 102, 100 is 103. So we have: 103 equals a thousand, 106 equals a million, 109 is called a billion (U.S. usage), and 1012 a trillion. Now the U.S. federal government budget is in the trillions of dollars, ordinary people really cannot grasp the magnitude of the number. In the metric system, the prefix kilo- stands for 1,000, e.g., a kilogram. For a million, the prefix mega- is used, e.g. megaton (1,000,000 or 106 ton). A billion hertz (a unit of frequency) is gigahertz, although I have not heard of the use of a giga-meter. More rarely still is the use of tera (1012). For small numbers, the practice is similar. 0.1 is 10À1, 0.01 is 10À2, and 0.001 is 10À3. The prefix of milli- refers to 10À3, e.g. as in millimeter, whereas a micro- second is 10À6 ¼ 0.000001 s. It is now trendy to talk about nano-technology, which refers to solid-state device with sizes on the scale of 10À9 m, or about 10 times the size of an atom. With this kind of shorthand convenience, one can really go overboard. -
Astrometry and Optics During the Past 2000 Years
1 Astrometry and optics during the past 2000 years Erik Høg Niels Bohr Institute, Copenhagen, Denmark 2011.05.03: Collection of reports from November 2008 ABSTRACT: The satellite missions Hipparcos and Gaia by the European Space Agency will together bring a decrease of astrometric errors by a factor 10000, four orders of magnitude, more than was achieved during the preceding 500 years. This modern development of astrometry was at first obtained by photoelectric astrometry. An experiment with this technique in 1925 led to the Hipparcos satellite mission in the years 1989-93 as described in the following reports Nos. 1 and 10. The report No. 11 is about the subsequent period of space astrometry with CCDs in a scanning satellite. This period began in 1992 with my proposal of a mission called Roemer, which led to the Gaia mission due for launch in 2013. My contributions to the history of astrometry and optics are based on 50 years of work in the field of astrometry but the reports cover spans of time within the past 2000 years, e.g., 400 years of astrometry, 650 years of optics, and the “miraculous” approval of the Hipparcos satellite mission during a few months of 1980. 2011.05.03: Collection of reports from November 2008. The following contains overview with summary and link to the reports Nos. 1-9 from 2008 and Nos. 10-13 from 2011. The reports are collected in two big file, see details on p.8. CONTENTS of Nos. 1-9 from 2008 No. Title Overview with links to all reports 2 1 Bengt Strömgren and modern astrometry: 5 Development of photoelectric astrometry including the Hipparcos mission 1A Bengt Strömgren and modern astrometry .. -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis,