The Astronomer Jules Janssen Astrophysics and Space Science Library
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Helium Mrs. Ahng the Second Lightest Element on Earth, Helium Is One Of
Helium Mrs. Ahng The second lightest element on Earth, Helium is one of the most important elements in our universe. It is the reason that we have sunlight, it makes balloons float, and used to cool down nuclear reactors. Although it is a simple noble gas with only two protons and two electrons, it is a powerful and essential resource. Discovered in1868 by astronomer Pierre Janssen while studying a solar eclipse; he noticed a yellow line around sun that had a wavelength that he had not seen before. English Astronomer Sir Norman Lockyer later named the element after the Greek word “Helios”, making the connection to how it was discovered. Helium only makes ups less than 1% of Earth’s atmosphere because of how light it is. It’s atomic mass is only 4.003, so the surrounding air is heavier than helium. An example of the difference in mass can be seen when comparing a helium filled balloon to a balloon filled with a mixture of atmospheric gases. The mass of the mixture is much heavier, and therefore is more effected by gravitational pull. Helium is found mostly in space in the core of stars, but it was also found on Earth in 1895 trapped underground. Scientists believe that the Helium that we harvest today was created during the creation of the universe, or the “Big Bang”. Only two electrons energize one orbital for this element, giving us the popular image for all atoms. With the outer orbital shell full, the element is referred to as inert and nonreactive. -
Arxiv:0906.0144V1 [Physics.Hist-Ph] 31 May 2009 Event
Solar physics at the Kodaikanal Observatory: A Historical Perspective S. S. Hasan, D.C.V. Mallik, S. P. Bagare & S. P. Rajaguru Indian Institute of Astrophysics, Bangalore, India 1 Background The Kodaikanal Observatory traces its origins to the East India Company which started an observatory in Madras \for promoting the knowledge of as- tronomy, geography and navigation in India". Observations began in 1787 at the initiative of William Petrie, an officer of the Company, with the use of two 3-in achromatic telescopes, two astronomical clocks with compound penduumns and a transit instrument. By the early 19th century the Madras Observatory had already established a reputation as a leading astronomical centre devoted to work on the fundamental positions of stars, and a principal source of stellar positions for most of the southern hemisphere stars. John Goldingham (1796 - 1805, 1812 - 1830), T. G. Taylor (1830 - 1848), W. S. Jacob (1849 - 1858) and Norman R. Pogson (1861 - 1891) were successive Government Astronomers who led the activities in Madras. Scientific high- lights of the work included a catalogue of 11,000 southern stars produced by the Madras Observatory in 1844 under Taylor's direction using the new 5-ft transit instrument. The observatory had recently acquired a transit circle by Troughton and Simms which was mounted and ready for use in 1862. Norman Pogson, a well known astronomer whose name is associated with the modern definition of the magnitude scale and who had considerable experience with transit instruments in England, put this instrument to good use. With the help of his Indian assistants, Pogson measured accurate positions of about 50,000 stars from 1861 until his death in 1891. -
In the Wake of the Compendia Science, Technology, and Medicine in Ancient Cultures
In the Wake of the Compendia Science, Technology, and Medicine in Ancient Cultures Edited by Markus Asper Philip van der Eijk Markham J. Geller Heinrich von Staden Liba Taub Volume 3 In the Wake of the Compendia Infrastructural Contexts and the Licensing of Empiricism in Ancient and Medieval Mesopotamia Edited by J. Cale Johnson DE GRUYTER ISBN 978-1-5015-1076-2 e-ISBN (PDF) 978-1-5015-0250-7 e-ISBN (EPUB) 978-1-5015-0252-1 ISSN 2194-976X Library of Congress Cataloging-in-Publication Data A CIP catalog record for this book has been applied for at the Library of Congress. Bibliographic information published by the Deutsche Nationalbibliothek The Deutsche Nationalbibliothek lists this publication in the Deutsche Nationalbibliografie; detailed bibliographic data are available on the Internet at http://dnb.dnb.de. © 2015 Walter de Gruyter Inc., Boston/Berlin Typesetting: Meta Systems Publishing & Printservices GmbH, Wustermark Printing and binding: Hubert & Co. GmbH & Co. KG, Göttingen ♾ Printed on acid-free paper Printed in Germany www.degruyter.com Notes on Contributors Florentina Badalanova Geller is Professor at the Topoi Excellence Cluster at the Freie Universität Berlin. She previously taught at the University of Sofia and University College London, and is currently on secondment from the Royal Anthropological Institute (London). She has published numerous papers and is also the author of ‘The Bible in the Making’ in Imagining Creation (2008), Qurʾān in Vernacular: Folk Islam in the Balkans (2008), and 2 (Slavonic Apocalypse of) Enoch: Text and Context (2010). Siam Bhayro was appointed Senior Lecturer in Early Jewish Studies in the Department of Theology and Religion, University of Exeter, in 2012, having previously been Lecturer in Early Jewish Studies since 2007. -
Janson. History of Art. Chapter 16: The
16_CH16_P556-589.qxp 12/10/09 09:16 Page 556 16_CH16_P556-589.qxp 12/10/09 09:16 Page 557 CHAPTER 16 CHAPTER The High Renaissance in Italy, 1495 1520 OOKINGBACKATTHEARTISTSOFTHEFIFTEENTHCENTURY , THE artist and art historian Giorgio Vasari wrote in 1550, Truly great was the advancement conferred on the arts of architecture, painting, and L sculpture by those excellent masters. From Vasari s perspective, the earlier generation had provided the groundwork that enabled sixteenth-century artists to surpass the age of the ancients. Later artists and critics agreed Leonardo, Bramante, Michelangelo, Raphael, Giorgione, and with Vasari s judgment that the artists who worked in the decades Titian were all sought after in early sixteenth-century Italy, and just before and after 1500 attained a perfection in their art worthy the two who lived beyond 1520, Michelangelo and Titian, were of admiration and emulation. internationally celebrated during their lifetimes. This fame was For Vasari, the artists of this generation were paragons of their part of a wholesale change in the status of artists that had been profession. Following Vasari, artists and art teachers of subse- occurring gradually during the course of the fifteenth century and quent centuries have used the works of this 25-year period which gained strength with these artists. Despite the qualities of between 1495 and 1520, known as the High Renaissance, as a their births, or the differences in their styles and personalities, benchmark against which to measure their own. Yet the idea of a these artists were given the respect due to intellectuals and High Renaissance presupposes that it follows something humanists. -
Download This Article (Pdf)
244 Trimble, JAAVSO Volume 43, 2015 As International as They Would Let Us Be Virginia Trimble Department of Physics and Astronomy, University of California, Irvine, CA 92697-4575; [email protected] Received July 15, 2015; accepted August 28, 2015 Abstract Astronomy has always crossed borders, continents, and oceans. AAVSO itself has roughly half its membership residing outside the USA. In this excessively long paper, I look briefly at ancient and medieval beginnings and more extensively at the 18th and 19th centuries, plunge into the tragedies associated with World War I, and then try to say something relatively cheerful about subsequent events. Most of the people mentioned here you will have heard of before (Eratosthenes, Copernicus, Kepler, Olbers, Lockyer, Eddington…), others, just as important, perhaps not (von Zach, Gould, Argelander, Freundlich…). Division into heroes and villains is neither necessary nor possible, though some of the stories are tragic. In the end, all one can really say about astronomers’ efforts to keep open channels of communication that others wanted to choke off is, “the best we can do is the best we can do.” 1. Introduction astronomy (though some of the practitioners were actually Christian and Jewish) coincided with the largest extents of Astronomy has always been among the most international of regions governed by caliphates and other Moslem empire-like sciences. Some of the reasons are obvious. You cannot observe structures. In addition, Arabic astronomy also drew on earlier the whole sky continuously from any one place. Attempts to Greek, Persian, and Indian writings. measure geocentric parallax and to observe solar eclipses have In contrast, the Europe of the 16th century, across which required going to the ends (or anyhow the middles) of the earth. -
Norman Lockyer Resources Information Sheet
Norman Lockyer resources information sheet Sir Joseph Lockyer was born in Rugby in 1836, the only son of a surgeon-apothecary, Joseph Hooley Lockyer and was educated privately in England and he also studied languages on the Continent. At the age of twenty-one he became a clerk in the War Office, and married Winifred James in the following year. He developed an interest in astronomy and journalism, and in 1863 began to give scientific papers to the Royal Astronomical Society. It is his discovery of helium which he has become most well known for. In 1869 Lockyer founded the journal 'Nature', which he edited until a few months before his death, and which remains to this day a major resource for international scientific knowledge. In 1870 he was appointed secretary to the Royal Commission on Scientific Instruction, which over the next five years reported on scientific education and resulted in the government setting up a laboratory of solar physics at South Kensington. To further this work Lockyer was transferred from the War Office to the Science and Art Department at South Kensington in 1875. Here he organised an international exhibition of scientific apparatus, as well as establishing the loan collection which eventually formed the nucleus of the collections of the Science Museum. Throughout this period, Lockyer continued to be active in astronomical observations and in spectroscopic studies in the laboratory of the College of Chemistry; he also wrote several books on astronomy and spectral analysis. Lockyer also studied the correlations between solar activity and weather, and developed interests in meteorology. -
How the Saha Ionization Equation Was Discovered
How the Saha Ionization Equation Was Discovered Arnab Rai Choudhuri Department of Physics, Indian Institute of Science, Bangalore – 560012 Introduction Most youngsters aspiring for a career in physics research would be learning the basic research tools under the guidance of a supervisor at the age of 26. It was at this tender age of 26 that Meghnad Saha, who was working at Calcutta University far away from the world’s major centres of physics research and who never had a formal training from any research supervisor, formulated the celebrated Saha ionization equation and revolutionized astrophysics by applying it to solve some long-standing astrophysical problems. The Saha ionization equation is a standard topic in statistical mechanics and is covered in many well-known textbooks of thermodynamics and statistical mechanics [1–3]. Professional physicists are expected to be familiar with it and to know how it can be derived from the fundamental principles of statistical mechanics. But most professional physicists probably would not know the exact nature of Saha’s contributions in the field. Was he the first person who derived and arrived at this equation? It may come as a surprise to many to know that Saha did not derive the equation named after him! He was not even the first person to write down this equation! The equation now called the Saha ionization equation appeared in at least two papers (by J. Eggert [4] and by F.A. Lindemann [5]) published before the first paper by Saha on this subject. The story of how the theory of thermal ionization came into being is full of many dramatic twists and turns. -
Book Reviews Biman Nath, the Story of Helium and the Birth of Astrophysics
Phys. Perspect. 15 (2013) 361–370 Ó 2013 Springer Basel 1422-6944/13/030361-10 DOI 10.1007/s00016-013-0121-5 Physics in Perspective Book Reviews Biman Nath, The Story of Helium and the Birth of Astrophysics. Heidelberg: Springer, 2012, 285 pages. $39.95 (cloth). Helium is the only chemical element ever to be first found anyplace except on earth, despite transitory claims for nebulium, coronium, aldebarium, asterium, cassiopeum, and more. Because the periodic table is now filled at least as far as Z = 112 (Copernicium, with a very short half-life) this will remain true at least as long as the only chemists and physicists we know are confined to terrestrial labs. Biman Nath’s history of the discovery of helium involves astronomy, chemistry, and physics, and so is particularly appropriate for 2013, which is the centenary both of the Bohr atom and of the first of two short papers by Henry Moseley (1887–1915) that established the primacy of Z (atomic number) over A (atomic weight) for constructing periodic tables and, in due course, for understanding the synthesis of the elements in stars. The crucial observations in the helium story were made from Guntur and Masulipam, India, during a long total solar eclipse in August 1868 by expeditions under the leadership of Jules Janssen (for France) and James Tennant and Norman Pogson (for England). John Herschel, son of the one most astronomers know, Captain Haig, and Professor Kero Laxuman also observed from other sites in India, and George Rayet (fresh from his 1867 triumph in codiscovering stars with emission-line spectra) from the Malay Peninsula. -
Lick Observatory Records: Correspondence UA.036.Ser.01
http://oac.cdlib.org/findaid/ark:/13030/c8dj5m3f No online items Guide to the Lick Observatory Records: Correspondence UA.036.Ser.01 Alix Norton University of California, Santa Cruz 2015 1156 High Street Santa Cruz 95064 [email protected] URL: http://guides.library.ucsc.edu/speccoll Guide to the Lick Observatory UA.036.Ser.01 1 Records: Correspondence UA.036.Ser.01 Language of Material: English Contributing Institution: University of California, Santa Cruz Title: Lick Observatory Records: Correspondence Creator: Lick Observatory Identifier/Call Number: UA.036.Ser.01 Physical Description: 148.5 Linear Feet257 boxes and 54 microfilm reels Date (inclusive): 1833-2009 Date (bulk): 1870-1960 Access Collection is open for research. The physical copybooks are restricted due to the fragile nature of the material. All use is directed to the microfilm of these volumes. The microfilm reels can be accessed by requesting them from Special Collections via the Library Catalog. Historical note The Lick Observatory was completed in 1888 and continues to be an active astronomy research facility at the summit of Mount Hamilton, near San Jose, California. It is named after James Lick (1796-1876), who left $700,000 in 1875 to purchase land and build a facility that would be home to "a powerful telescope, superior to and more powerful than any telescope yet made". The completion of the Great Lick Refractor in 1888 made the observatory home to the largest refracting telescope in the world for 9 years, until the completion of the 40-inch refractor at Yerkes Observatory in 1897. Since its founding in 1887, the Lick Observatory facility has provided on-site housing on Mount Hamilton for researchers, their families, and staff, making it the world's oldest residential observatory. -
Johannes Vermeer's Mistress and Maid
Mahon et al. Herit Sci (2020) 8:30 https://doi.org/10.1186/s40494-020-00375-2 RESEARCH ARTICLE Open Access Johannes Vermeer’s Mistress and Maid: new discoveries cast light on changes to the composition and the discoloration of some paint passages Dorothy Mahon1, Silvia A. Centeno2* , Margaret Iacono3, Federico Carό2, Heike Stege4 and Andrea Obermeier4 Abstract Among the thirty-six paintings ascribed to the Dutch seventeenth century artist Johannes Vermeer (1632–1675), Mistress and Maid, in The Frick Collection, stands out for the large-scale fgures set against a rather plain background depicting a barely discernible curtain. Although generally accepted as among the late works of the artist and dated to 1667–1668, for decades scholars have continued to puzzle over aspects of this portrayal. When the painting was cleaned and restored in 1952, attempts to understand the seeming lack of fnish and simplifed composition were hampered by the limited technical means available at that time. In 1968, Hermann Kühn included Mistress and Maid in his groundbreaking technical investigation ‘A Study of the Pigments and the Grounds Used by Jan Vermeer.’ In the present study, imaging by infrared refectography and macro-X-ray fuorescence (MA-XRF) revealed signifcant com- positional changes and drew focus to areas of suspected color change. Three of the samples taken by Hermann Kühn, and now in the archive of the Doerner Institut in Munich, were re-analyzed, along with a few paint samples taken from areas not examined in the 1968 study, using scanning electron microscopy–energy dispersive X-ray spectros- copy (SEM–EDS) and Raman spectroscopy. -
Alfred Fowler, F.R.S
JOURNAL OF THE TRANSACTIONS OF ·@hr t8ittl1ria Jnstitut~, OR, j gilosopbintl ,Sotietu of ®nat ~ritain. SECRI,'TARY: E. WALTER MAUNDER, F.R.A.S. VOL. XLVII. LONDON: (:\8ullliJSl)rlJ ll!) tl)e inJStitutr, 1, <tmtral 3Suill:riugJS, ErJStminJSter, j,,E.) ALL RIGHTS RESBRVER . 1915. 565TH ORDINARY GENERAL MEETING, HELD IN THE CONFERENCE HALL, CENTRAL HALL, WESTMINSTER, ON MONDAY, MARCH lsT, 1915, AT 4.30 P.M. Sm FRANK W. DYSON, F.R.S., ASTRONOMER ROYAL, TOOK THE OHAIR. The Minutes of the preceding Meeting were read and confirmed. The SECRETARY announced the election of the Rev. Martin Anstey and the Rev. G. Campbell Morgan as Members of the Institute. The Rev. Prebendary H. E. Fox, M.A., opened the Meeting and introduced the Lecturer, Professor Alfred Fowler, F.R.S. THE SPECTRA OF STARS AND NEBUL.JE. By Professor A. FOWLER, F.R.S. [ABSTRACT.] HE purpose of this lecture is to give some indication of the T way in which the wonderful power of the spectroscope has been utilised in investigations of the chemistry of stars and nebula\ and of the bearing of such knowledge upon the great question of celestial evolution. The only intelligible message that a star sends to the earth is borne on its rays of light, and it is only by the analysis of such light that we can learn anything at all as to the chemical composition and physical condition of the star. Such an analysis has been rendered possible by the invention of the spectroscope in its various forms. Each element, and some com pounds, has its own distinctive family of spectrum lines or bands, by which it can be identified wherever it occurs in the luminous condition. -
George Ellery Hale Papers 10142-MS
http://oac.cdlib.org/findaid/ark:/13030/kt067nb6q6 Online items available Guide to the George Ellery Hale Papers 10142-MS Daniel J. Kevles, Charlotte E. Erwin, Peter Sachs Collopy Carnegie Institution of Washington, California Institute of Technology, American Institute of Physics Center for the History of Physics Revised to accompany the web publication of the George Ellery Hale Papers. California Institute of Technology Archives and Special Collections 2018 1200 East California Blvd. MC B215-74 Pasadena, California 91125 [email protected] URL: http://archives.caltech.edu/ Guide to the George Ellery Hale 10142-MS 1 Papers 10142-MS Language of Material: English Contributing Institution: California Institute of Technology Archives and Special Collections Title: George Ellery Hale Papers creator: Hale, George Ellery, 1868-1938 Identifier/Call Number: 10142-MS Physical Description: 73 linear feet Date (inclusive): 1863-1950 Date (bulk): 1882-1938 Abstract: George Ellery Hale (1868–1938) was an influential astrophysicist and science administrator. This collection of Hale's scientific, professional, and personal papers documents his roles in inventing the spectrohelioscope; promoting international cooperation among scientists; and founding major observatories, as well as the California Institute of Technology, Huntington Library, Astrophysical Journal, and National Research Council. https://hale.archives.caltech.edu/ Conditions Governing Access Most of this collection is available on the web, linked from individual folder records in this finding aid. If you would like to examine the original paper copies of materials in series 1 through 9, please email [email protected] to apply for an appointment. The original Director's Files of the Mount Wilson Observatory are located at the Huntington Library and available to qualified researchers by application through their Reader Services Department.