Lodewijk Woltjer (1930– 2019)
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Benjamin Apthorp Goulds
TWO BENJAMIN APTHORP GOULDS “NARRATIVE HISTORY” AMOUNTS TO FABULATION, THE REAL STUFF BEING MERE CHRONOLOGY “Stack of the Artist of Kouroo” Project Two Benjamin Apthorp Goulds HDT WHAT? INDEX BENJAMIN APTHORP GOULD, JR. BENJAMIN APTHORP GOULD 1787 June 15, Friday: Benjamin Apthorp Gould was born. Variant texts of the plan presented by William Patterson of New Jersey to the Federal Convention, Text A: READ THE FULL TEXT Text B: READ THE FULL TEXT Text C: READ THE FULL TEXT NOBODY COULD GUESS WHAT WOULD HAPPEN NEXT “Stack of the Artist of Kouroo” Project Two Benjamin Apthorp Goulds HDT WHAT? INDEX BENJAMIN APTHORP GOULD BENJAMIN APTHORP GOULD, JR. 1814 August 24, Wednesday: Viscount Castlereagh arrived at Paris, where he would be meeting with King Louis XVIII and Talleyrand before traveling on to Vienna. As part of a conflict that was essentially a continuation of the American Revolution by way of a dispute over the seas and over the border of Canada, on this day and the following one a British army defeated hastily assembled defenders of Washington DC at Bladensburg, Maryland, just north of the capital. The British would go on to burn Washington, including the White House and most of the 3,076 books and 53 maps, charts, and plans of the Library of Congress, along with paintings of Louis XVI and Marie Antoinette by Madame Vigee Lebruin. They would also put the chambers of the House and the Senate in Washington DC to the torch — but beware, it is sheer mythology that the books were used as kindling for the fire in the legislative chambers.1 Waldo Emerson would reminisce in his journal in about April or May of 1856 about a British-invasion-of- Boston scare that had occurred in about this period of his childhood:2 I have but one military recollection in all my life. -
December 2019
The Newsletter of Westchester Amateur Astronomers December 2019 M8-The Lagoon Nebula by Gary Miller A familiar object at summer star parties, M8 in Sagittarius was first glimpsed by John Flamsteed in 1680 and called “The Lagoon Nebula” by the Irish astronomer Agnes Clerke in The System of the Stars (1890). It is an emission nebula which re-radiates the energy of several hot young stars embedded within it, including 9 Sagittari (dead center). It also surrounds the open cluster NGC 6530, a system of 113 young stars. Although it’s low in the summer sky from Westchester, it’s a wonderful visual object in nearly any telescope. SERVING THE ASTRONOMY COMMUNITY SINCE 1986 Westchester Amateur Astronomers SkyWAAtch December 2019 WAA December Meeting WAA January Meeting Friday, December 6th at 7:30 pm Friday, January 10th at 7:30 pm Lienhard Hall, 3rd floor Lienhard Hall, 3rd floor Pace University, Pleasantville, NY Pace University, Pleasantville, NY The History of Glass: The Power Behind Why Go Back to the Moon? Discovery Andy Poniros Alan Witzgall NASA Solar System Ambassador Senior Optician, ESCO Optics Andy has been a NASA volunteer since 1997 and a Alan is an active member and officer of several ama- NASA/JPL Solar System Ambassador since 2004 . He teur astronomy societies in New Jersey. In his profes- has a degree in Electrical Engineering and has worked sional life, he is a Senior Optician for ESCO Optics of as a Medical Imaging Engineer for 45 years. He is Oak Ridge, NJ. His career in optics started with build- certified by NASA to handle Lunar samples, is a sci- ing telescopes in his basement during his high school ence correspondent for radio station WPKN in Con- and college years. -
T Vulpeculae
T Vulpeculae: Maximum Times covering 120 years show a slight, continuous Period Decrease US astronomer Benjamin Apthorp Gould (1824...1896) studied in Germany, namely mathematics in Göttingen from Prof. Gauss and astronomy in Bonn from Prof. Argelander. Back home Gould started a visual sky survey to complete Argelander's Bonner Durchmusterung. After Gould had departed to observe in Argentina his assistant Seth Carlo Chandler jr. (1846...1913) in 1876 recruited the Boston bank clerk Edwin F. Sawyer to contribute with own visual observations. It seems, that Sawyer observed at least until about 1900. During these 25 years with the visual comparison methods of his time Sawyer discovered a remarkable number of variable stars, among them (Sawyer, 1885) the bright, classical cepheid T Vulpeculae. T Vul is about the 10th in apparent magnitude of all classical cepheids. A modern database (DDODB, ca. 1996) reports a mean magnitude of 5,75mag and an amplitude of 0,64mag. The period is 4,4 days. The lightcurve (figure 1) produces the typical smooth, asymmetric pattern of classical cepheids with periods between 3 and 6 days. Around 1900 the term "cepheid" had not yet been introduced. Researchers designated variables with asymmetric lightcurves and periods shorter than 50 days as short period variables. Karl Schwarzschild (1900) discovered, that brightness and brightness variation of a star on photographic plates can be much different from visual ones. In the following years scientists recognized, that short period variables show this phenomenon to an especially marked amount. Authors of the 1920ies and 1930ies continued to study this by comparing visual magnitudes or magnitudes on panchromatic, sensitised ("photovisual") plates on one with magnitudes on unsensitised, blue sensitive ("photographic") plates on the other side. -
On the Epistemic and Social Foundations of Mathematics As Tool and Instrument in Observatories, 1793–1846 David Aubin
On the Epistemic and Social Foundations of Mathematics as Tool and Instrument in Observatories, 1793–1846 David Aubin To cite this version: David Aubin. On the Epistemic and Social Foundations of Mathematics as Tool and Instrument in Observatories, 1793–1846. Johannes Lenhard & Martin Carrier,. Mathematics as a Tool: Tracing New Roles of Mathematics in the Sciences, 327, Springer, p. 177-196, 2017, Boston Studies in the Philosophy and History of Science. hal-01269674 HAL Id: hal-01269674 https://hal.sorbonne-universite.fr/hal-01269674 Submitted on 5 Feb 2016 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. On the Epistemic and Social Foundations of Mathematics as Tool and Instrument in Observatories, 1793–1846 David Aubin* May 2015, revised February 2016 The astronomer is dependent on his tools; the observatory is but the receptacle of his tools, his tool-chest so to speak (Harrington 1883–1884, 249). One night, in June 1782, the Astronomer Royal Nevil Maskelyne suddenly felt “much out of love with his instrument.”1 William Herschel had come to Greenwich to stargaze in his company and Maskelyne had welcomed him. But to realize that all telescopes in the Royal Observatory were so much inferior to Herschel’s new reflector was disheartening to the Astronomer Royal. -
Vera Rubin Finding
Vera C. Rubin Photograph Collection, circa 1942-2012 Carnegie Institution of Washington Department of Terrestrial Magnetism Archives Washington, DC Finding aid written by: Mary Ferranti and Shaun Hardy March 2018 Revised July 2019 Vera C. Rubin Photograph Collection, circa 1942-2012 TABLE OF CONTENTS Page Introduction 1 Biographical Sketch 1 Scope and Content 2 Image Listing 3 Subject Terms 26 Bibliography 26 Related Collections 27 Vera C. Rubin Photograph Collection, circa 1942-2012 Table of Contents Vera C. Rubin Photograph Collection, circa 1942-2012 DTM-2016-03 Introduction Abstract: This collection consists of photographs documenting the professional and personal life of astronomer Vera C. Rubin. Extent: 3 linear feet: 5 three-ring album boxes, 1 flat print box. Acquisition: The collection was donated by Vera Rubin in 2012 and formally deeded to the archives by her son, Allan M. Rubin, in 2018. Access Restrictions: There are no access restrictions. Copyright: Copyright is held by the Department of Terrestrial Magnetism, Carnegie Institution of Washington. For permission to reproduce or publish please contact the archivist. Preferred Citation: Vera C. Rubin Photograph Collection, circa 1942-2012, Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, D.C. Processing: Maria V. Lobanova processed the collection in December 2016-April 2017 and identified as many individuals, places, and events as possible. Shaun Hardy and Mary Ferranti prepared the finding aid in 2018. Biographical Sketch Vera Rubin was born the younger daughter of Philip and Rose Cooper on July 23, 1928, in Philadelphia, PA. At the age of 10, she and her family moved to Washington, DC, when her father accepted a job offer there. -
The Pre-Embryonic State of the AAVSO
154 Saladyga, JAAVSO Volume 27, 1999 THE “PRE-EMBRYONIC” STATE OF THE AAVSO: AMATEUR OBSERVERS OF VARIABLE STARS IN THE UNITED STATES FROM 1875 TO 1911 Michael Saladyga AAVSO Headquarters 25 Birch Street Cambridge, MA 02138 Presented at the 87th Annual Meeting of the AAVSO, October 31, 1998 Abstract For 35 years before the formation of the AAVSO, independent amateur variable star astronomers in the United States were making significant contributions to the field. Skilled, dedicated individuals like S. C. Chandler, E. F. Sawyer, and P. S. Yendell laid the foundation in variable star work that was expanded upon by Harvard College Observatory Director E. C. Pickering, under whose direction a new generation of enthusiastic amateur and professional astronomers continued to further the cause of variable star research. This paper is a survey of the contributions made by several independent amateur variable star astronomers, and it is also a chronology of the growth of a broader, more popularized, amateur involvement in variable star astronomy which led to the organization of the AAVSO in 1911. 1. Introduction The German astronomer Friedrich Argelander is well-known in variable star histories as the “father of variable star observing.” The professional astronomer Argelander in 1844 first brought to the attention of the astronomical community the phenomena of variable stars and the need for observations of them. His Uranometria Nova catalogue of the magnitudes of over 3,500 northern stars was a great boost to the involvement of amateur observers of variable stars in Europe. This catalogue was not widely available in America, hence the late start here in amateur variable star work. -
But It Was Fun
But it was Fun The First Forty years of Radio Astronomy at Green Bank Second Printing, with corrections. Edited by Felix J. Lockman, Frank D. Ghigo, and Dana S. Balser Second printing published by the Green Bank Observatory, 2016. i Front cover: The 140 Foot Telescope and admirers at its dedication, October 1965. Title Page: The Tatel telescope under construction, 1958. Back cover, clockwise from lower left: Grote Reber in the Bean Patch in Green Bank, 1959; Employee group photo, 1960; site view of 300 Foot and Interferometer, 1971; the 140 Foot in September 1965; the 140 Foot at night; the Tatel Telescope under construction, 1958; the Tatel telescope, ca. 1980, view towards the west; the 300 Foot Telescope, 1964; aerial view of the 100 Meter Green Bank Telescope and the 140 Foot Telescope when the GBT was nearing completion, summer 2000. Cover design by Bill Saxton Copyright °c 2007, by National Radio Astronomy Observatory Second printing copyright °c 2016, by the Green Bank Observatory ISBN 0-9700411-2-8 Printed by The West Virginia Book Company, Charleston WV. The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. ii Table of Contents Preface ............................................................ v Acknowledgements ................................................. vii Historical Introduction ............................................. viii Part I. Building an Observatory ................................ 1 1. Need for a National Observatory -
Report Annexes
International Astronomical Union XXVth General Assembly July 13-26 2003 Sydney, Australia Contents Annex 1 Timeline of Events Annex 2 National Organizing Committee Members Annex 3 Opening Ceremony Annex 4 Student-Volunteer Program Annex 5 Tours Program Annex 6 The Australian Festival of Astronomy Annex 7 Associated Public Events Annex 8 “Astronomy on the Go” Annex 9 Room Allocations Annex 10 Astro Expo Exhibitor listing Annex 11 Industry Day Annex 12 Delegate List Annex 13 The Australian Festival of Astronomy - Marketing Report ANNEX 1 INTERNATIONAL ASTRONOMY UNION 25TH GENERAL ASSEMBLY Timeline of Events 1994 At Don Mathewson’s invitation, IAU Executive Committee members visit Australia Jeremy Mould heads move to bid for 2003 GA in Sydney 1995 Bid for 2003 GA in Sydney submitted to IAU 1997 Aug Sydney awarded 2003 GA during Kyoto GA Jeremy Mould calls for expressions of interest to form LOC (NOC) 1998 Apr John Norris convenes 1st meeting of NOC NOC decide on SCEC for GA venue Convention Centre booked for period July 13-26, 2003? Sep Lawrence Cram takes over Chair for 5th NOC meeting Sep NOC call for tenders for provision of PCO services Dec 7th NOC meeting spent visiting two candidate PCO companies 1999 Mar Raymond Haynes takes over NOC Chair for 8th NOC meeting Jun ICMS chosen as GA PCO at the 9th NOC meeting Jun Use of Sydney Opera House for Opening Ceremony considered Oct Preliminary budget tabled at 11th NOC meeting 2000 May Logo design selected at 14th NOC meeting Aug Sydney GA display and David Malin presentation at Manchester -
URSI Commission J – Radio Astronomy
1 URSI Commission J – Radio Astronomy Jacob W.M. Baars Max-Planck-Institut für Radioastronomie Bonn, Germany Preface The organisation and operation of URSI can be seen as a sailing trip around the world by ten boats, each representing one of the ten Commissions of URSI, that gather at three year intervals in a place on earth decided by the central overseers, the Council. At these General Assemblies the captains of the Commission ships meet with the Council to discuss the experiences of the recent period and make plans for the next. The crews of the ten boats set up their individual meetings to present the scientific discoveries of the last three years to their colleagues who could not fit on the ship and travelled to the harbour to hear the news. Occasionally, crews from more than one boat find common interest in holding joint meetings. Also, individual captains may make landfall by invitation at a suitable place for a conference on a special subject of interest. This procedure has been in place for a hundred years to great satisfaction of the URSI community and with considerable success. It is not unusual to accompany such a centennial with the publication of a book on the history of the organisation. The URSI Centenary Book, of which this chapter is a part, will do just that. But how to write a history of a journey with short highlights every three years and intermediate years of calm? In addition, the highlights, the General Assemblies, tend to be rather similar in structure and there is a danger that the story will become repetitive and rather boring. -
From Radar to Radio Astronomy
John Bolton and the Nature of Discrete Radio Sources Thesis submitted by Peter Robertson BSc (Hons) Melbourne, MSc Melbourne 2015 for the degree of Doctor of Philosophy in the School of Agricultural, Computational and Environmental Sciences University of Southern Queensland ii Peter Robertson: ‘John Bolton and the Nature of Discrete Radio Sources’ Abstract John Bolton is regarded by many to be the pre-eminent Australian astronomer of his generation. In the late 1940s he and his colleagues discovered the first discrete sources of radio emission. Born in Sheffield in 1922 and educated at Cambridge University, in 1946 Bolton joined the Radiophysics Laboratory in Sydney, part of Australia’s Council for Scientific and Industrial Research. Radio astronomy was then in its infancy. Radio waves from space had been discovered by the American physicist Karl Jansky in 1932, followed by Grote Reber who mapped the emission strength across the sky, but very little was known about the origin or properties of the emission. This thesis will examine how the next major step forward was made by Bolton and colleagues Gordon Stanley and Bruce Slee. In June 1947, observing at the Dover Heights field station, they were able to show that strong radio emission from the Cygnus constellation came from a compact point-like source. By the end of 1947 the group had discovered a further five of these discrete radio sources, or ‘radio stars’ as they were known, revealing a new class of previously-unknown astronomical objects. By early 1949 the Dover Heights group had measured celestial positions for the sources accurately enough to identify three of them with known optical objects. -
PART II. OTHER PUBLICATIONS of the ACADEMY MEMOIRS of the NATIONAL ACADEMY of SCIENCES -The Memoirs Are Monographs Published at Irregular Intervals
PART II. OTHER PUBLICATIONS OF THE ACADEMY MEMOIRS OF THE NATIONAL ACADEMY OF SCIENCES -The Memoirs are monographs published at irregular intervals. Some volumes are comprised of a single monograph, while others consist of several separate papers relating to different branches of science. The Memoirs listed as "out of print" qare no longer available from the Academy,' but it is possible that some of these might still be obtained from the Superintendent of Documents, Government Printing Office, Washington, D. C., who sometimes has additional copies which are sold at cost. The Academy edition of the Memoirs is distributed free. CONTENTS VoLums I. 1866. Out of print 1. Reduction of the observations of fixed stars made by Joseph LePaute D'Agelet, at Paris, in 1783-1785, with a catalogue of the corresponding mean places, referred to the Equinox of 1800.0. BENJAMIN APTHORP GOULD. Read January 8, 1864. Pp. 1-261. 2. The Saturnian system. BZNJAMIN Pumcu. Read January 8, 1864. Pp. 263-86. 3. On the distribution of certain diseases in reference to hygienic choice of location for the cure of invalid soldiers. AUGUSTrUS A. GouLD. Read August 5, 1864. Pp. 287-90. 4. On shooting stars. H. A. NEWTON.- Read August 6, 1864. Pp. 291-312. 5. Rifled guns. W. H. C. BARTL*rT. Read August 25, 1865. Pp. 313-43. VoLums II. 1884 1. Report of the eclipse expedition to Caroline Island, May, 1883. Pp. 5-146. 2. Experimental determination of wave-lengths in the invisible prismatic spectrum. S. P. LANGIXY. April, 1883. 4 plates. Pp. 147-2. -
C.H.F. Peters
NATIONAL ACADEMY OF SCIENCES Ch RISTIAN HEINRIC H F RIEDRIC H PETERS A Biographical Memoir by W I L L I A M ShEE H AN 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 1999 NATIONAL ACADEMIES PRESS WASHINGTON D.C. CHRISTIAN HEINRICH FRIEDRICH PETERS September 19, 1813–July 18, 1890 BY WILLIAM SHEEHAN N THE MID-NINETEENTH century the discovery of new aster- Ioids was still far from routine. These objects had not yet grown so numerous as to earn for themselves the contemp- tuous label later applied, “vermin of the skies,” and those who excelled in claiming the starlike wanderers from the camouflage of background stars were honored with renown. Hind, de Gasparis, Goldschmidt, Chacornac, Pogson, and Peters were foremost among the early discoverers. Even on this short list C. H. F. Peters stood out. On May 29, 1861—just weeks after the American Civil War began at Fort Sumter—Peters discovered his first aster- oid (72 Feronia). It was the fifth asteroid discovered in North America (others had been found by Ferguson and Searle). Feronia was the first of forty-eight such discoveries that made Peters the most prolific finder of minor planets of his generation, and even today he remains second only to Johann Palisa among visual discoverers of asteroids. Dur- ing his colorful career, he also compiled meticulous star charts of the zodiac, collated observations from manuscripts of Ptolemy, and embroiled himself in a series of often bitter controversies with other astronomers, notably over the ex- istence of an intra-Mercurial planet.