Tremoring Transits: Railways, the Royal Observatory and the Capitalist Challenge to Victorian Astronomical Science
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Maxwell and the Rings of Saturn
newsletter OF THE James Clerk Maxwell Foundation Issue No.5 Spring 2 015 Maxwell a nd t he Rings of Saturn by Professor Andrew Whitaker, Emeritus Professor of Physics, Queen’s University, Belfast Le Verrier, or to be worthy of the credit bestowed on him by Britain and, in particular, Cambridge. The funds for the Adams Prize were A view of the rings of Saturn (from Gribbin, John and provided by alumni of Adams’ Cambridge Goodwin, Simon (1998). Empire of the Sun: Planets college, St. John’s, and the prize was in and Moons of the Solar System. Constable, London.) the gift of the University. Airy and Challis were heavily involved in choosing topics Maxwell considered the rings of Saturn Against this background, why was in the first few years of the prize, and in to be ‘ the most remarkable bodies in the Maxwell prepared to put in so much work Maxwell’s year William Thomson was heavens ’, second only, in his opinion, to over several years on the rings of Saturn? also an examiner. Thomson, later Lord the spiral nebulae. Yet it seems extremely Admittedly the prize was substantial – Kelvin, had, of course, been Professor of unlikely that he would have devoted £130, or perhaps £13,000 in today’s terms, Natural Philosophy at Glasgow University a substantial amount of time and and this was rather more than a third of since 1846, but retained very strong links effort to determining their structure his full year’s salary at Aberdeen. But it is with Cambridge throughout his career. mathematically had the topic not been more likely that the reasons for taking Thus the institution of the Adams Prize chosen in 1855 as the subject of the on the challenge were, firstly, personal and the quality of the prize-winning Adams Prize of 1856. -
Mister Mary Somerville: Husband and Secretary
Open Research Online The Open University’s repository of research publications and other research outputs Mister Mary Somerville: Husband and Secretary Journal Item How to cite: Stenhouse, Brigitte (2020). Mister Mary Somerville: Husband and Secretary. The Mathematical Intelligencer (Early Access). For guidance on citations see FAQs. c 2020 The Author https://creativecommons.org/licenses/by/4.0/ Version: Version of Record Link(s) to article on publisher’s website: http://dx.doi.org/doi:10.1007/s00283-020-09998-6 Copyright and Moral Rights for the articles on this site are retained by the individual authors and/or other copyright owners. For more information on Open Research Online’s data policy on reuse of materials please consult the policies page. oro.open.ac.uk Mister Mary Somerville: Husband and Secretary BRIGITTE STENHOUSE ary Somerville’s life as a mathematician and mathematician). Although no scientific learned society had a savant in nineteenth-century Great Britain was formal statute barring women during Somerville’s lifetime, MM heavily influenced by her gender; as a woman, there was nonetheless a great reluctance even toallow women her access to the ideas and resources developed and into the buildings, never mind to endow them with the rights circulated in universities and scientific societies was highly of members. Except for the visit of the prolific author Margaret restricted. However, her engagement with learned institu- Cavendish in 1667, the Royal Society of London did not invite tions was by no means nonexistent, and although she was women into their hallowed halls until 1876, with the com- 90 before being elected a full member of any society mencement of their second conversazione [15, 163], which (Societa` Geografica Italiana, 1870), Somerville (Figure 1) women were permitted to attend.1 As late as 1886, on the nevertheless benefited from the resources and social nomination of Isis Pogson as a fellow, the Council of the Royal networks cultivated by such institutions from as early as Astronomical Society chose to interpret their constitution as 1812. -
James Clerk Maxwell
James Clerk Maxwell JAMES CLERK MAXWELL Perspectives on his Life and Work Edited by raymond flood mark mccartney and andrew whitaker 3 3 Great Clarendon Street, Oxford, OX2 6DP, United Kingdom Oxford University Press is a department of the University of Oxford. It furthers the University’s objective of excellence in research, scholarship, and education by publishing worldwide. Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries c Oxford University Press 2014 The moral rights of the authors have been asserted First Edition published in 2014 Impression: 1 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, by licence or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this work in any other form and you must impose this same condition on any acquirer Published in the United States of America by Oxford University Press 198 Madison Avenue, New York, NY 10016, United States of America British Library Cataloguing in Publication Data Data available Library of Congress Control Number: 2013942195 ISBN 978–0–19–966437–5 Printed and bound by CPI Group (UK) Ltd, Croydon, CR0 4YY Links to third party websites are provided by Oxford in good faith and for information only. -
Popular Astronomy Lectures in Nineteenth Century Britain
Commercial and Sublime: Popular Astronomy Lectures in Nineteenth Century Britain Hsiang-Fu Huang UCL Department of Science and Technology Studies Thesis submitted for the degree of Doctor of Philosophy (PhD) in History and Philosophy of Science March 2015 2 I, Hsiang-Fu Huang, confirm that the work presented in this thesis is my own. Where information has been derived from other sources, I confirm that this has been indicated in the thesis. Date of signature: 9th March 2015 Supervisors: Joe Cain (UCL) Simon Werrett (UCL) Examiners: Frank A. J. L. James (UCL / Royal Institution of Great Britain) Richard Bellon (Michigan State University) Date of examination: 16th December 2014 3 4 Abstract This thesis discusses the practitioners, sites, curriculums, apparatus and audiences of popular astronomy lecturing in nineteenth-century Britain. Lecturers who were active approximately between 1820 and 1860 are the focus. This thesis emphasises popularisers who were not scientific elites, including C. H. Adams (1803-1871), George Bartley (c. 1782-1858), and D. F. Walker (1778-1865). Activities of private popularisers are compared with those in scientific establishments, such as the Royal Institution. Private entrepreneurs were not inferior to institutional competitors and enjoyed popularity among audiences. Until the 1860s, popular astronomy lecturing was a shared arena of institutional and private popularisers. A theatrical turn occurred in the popular astronomy lecturing trade before 1820. Popularisers moved lectures into theatres and adopted theatrical facilities in performance. They developed large onstage devices, such as the transparent orrery, for achieving scenic and dramatic effects. These onstage astronomical lectures were a phenomenon in the early nineteenth century and were usually performed during Lent. -
Autobiography of Sir George Biddell Airy by George Biddell Airy 1
Autobiography of Sir George Biddell Airy by George Biddell Airy 1 CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. CHAPTER I. CHAPTER II. CHAPTER III. CHAPTER IV. CHAPTER V. CHAPTER VI. CHAPTER VII. CHAPTER VIII. CHAPTER IX. CHAPTER X. Autobiography of Sir George Biddell Airy by George Biddell Airy The Project Gutenberg EBook of Autobiography of Sir George Biddell Airy by George Biddell Airy This eBook is for the use of anyone anywhere at no cost and with almost no restrictions whatsoever. You may copy it, give it away or re-use it under the terms of the Project Gutenberg Autobiography of Sir George Biddell Airy by George Biddell Airy 2 License included with this eBook or online at www.gutenberg.net Title: Autobiography of Sir George Biddell Airy Author: George Biddell Airy Release Date: January 9, 2004 [EBook #10655] Language: English Character set encoding: ISO-8859-1 *** START OF THIS PROJECT GUTENBERG EBOOK SIR GEORGE AIRY *** Produced by Joseph Myers and PG Distributed Proofreaders AUTOBIOGRAPHY OF SIR GEORGE BIDDELL AIRY, K.C.B., M.A., LL.D., D.C.L., F.R.S., F.R.A.S., HONORARY FELLOW OF TRINITY COLLEGE, CAMBRIDGE, ASTRONOMER ROYAL FROM 1836 TO 1881. EDITED BY WILFRID AIRY, B.A., M.Inst.C.E. 1896 PREFACE. The life of Airy was essentially that of a hard-working, business man, and differed from that of other hard-working people only in the quality and variety of his work. It was not an exciting life, but it was full of interest, and his work brought him into close relations with many scientific men, and with many men high in the State. -
Mchenry County Illinois Genealogical Society 1011 N
McHenry County Illinois Genealogical Society 1011 N. Green St., McHenry, IL 60050 15 June 1988 Office of the Clerk of the Circuit Court McHenry County Court House Woodstock, IL 60098 Dear Ruth, Thank you for all the help you gave us in the preparation of this, our latest publication. Enclosed is a complimentary copy of the McHENRY COUNTY DECLARATIONS OF INTENT, SEPTEMBER 1851 - SEPTEMBER 1906, with our thanks. Sincerely, Jv.A,saaJ Publications Comm. M.C.I.G.S. McHENRY COUNTY ILLINOIS DECLARATIONS OF INTENT SEPTEMBER 1851—SEPTEMBER 1906 Published by McHenry County Illinois Genealogical Society loll North Green Street McHenry, Illinois 60050 1988 All rights reserved. No part of this book may be reproduced or utilized in any form or by any means, electronic or mechanical, including photocopying, recording, or by any information storage and retrieval system, without permission in writing from the author. Copyright (D 1988 McHenry County Illinois Genealogical Society 10 11 North Green Street McHenry, Illinois 60050 Library of Congress Catalog Number: 88-61060 ISBN: 0-910741-08 PREFACE Early immigrants to the United States could apply for citizenship at any local court by filing a Declaration of Intent, often referred to as "First Papers". After a five-year residency the immigrant could submit his Citizenship Petition ("Final Papers") and become eligible for naturalization. The Declaration of Intent and the Citizenship Petition may not always be found in the same court. Often, after filing the Declaration, the applicant moved to another county or state and submitted his final petition there. Also, many immigrants made an initial Declaration of Intent in order to purchase land, but failed to have a final Citizenship Petition recorded by the court. -
The Kew Photoheliograph
THE KEW PHOTOHELIOGRAPH PEDRO RÉ http://pedroreastrophotography.com/ The Kew Photoheliograph (Figure 1) was the first telescope specifically designed for solar photography. It was commissioned in 1854 and named after the Kew Observatory where it has housed. The Photoheliograph was designed by Warren De la Rue (1815-1889) (Figure 2) for the London Royal Society in 1857 and made by Andrew Ross (1798-1859). It was mainly used for daily photography of the Sun at the Kew Observatory and the Royal Observatory of Greenwich. It was also transported to Rivabellosa in Northern Spain where it was used to photograph the Total eclipse of the Sun on July 18th, 1860. Figure 1- The Kew Photoheliograph. The first solar photographs were obtained by Hippolyte Fizeau and Leon Focault in 1844. The first photographs of the partial phase of a total solar eclipse and of the solar spectrum were also obtained in the 1840s. In 1849 Hervé Faye made an important communication to the Frech Academy of Sciences proposing the continuous photographic survey of the Sun: If a solar image is formed in the daguerrotype plate ... the same measurements can be repeated later on and compared with contemporaneous ones ... The same procedure may be applied to the determination of the heliocentric sunspot co-ordinates ... On April 24, 1854 John Herschel wrote to Edward Sabine: I consider it an object of very considerable importance to secure at some observatory, and indeed at more than one, in different localities, daily photographic representations of the sun, with a view to keep up a consecutive and perfectly faithful record of the history of the spots. -
New Force at Large Distances
New force at large distances Daniel Grumiller Institute for Theoretical Physics Vienna University of Technology TEDx Vienna, November 2010 I What are the fundamental forces in Nature? I What is the nature of space, time and matter? Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? (picture by NASA) D. Grumiller | New force 2/11 I What is the nature of space, time and matter? Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? (picture by lifesbalancebeam) D. Grumiller | New force 2/11 Some questions physics cannot address: We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? I What is the nature of space, time and matter? (picture by spacescan.org) D. Grumiller | New force 2/11 We live in the golden age of fundamental physics Goal: want to understand how the Universe works Some questions physics can address: I What is the Universe made of? I What are the fundamental forces in Nature? I What is the nature of space, time and matter? Some questions physics cannot address: D. Grumiller | New force 2/11 What is the Universe made of? D. -
The Maunder Minimum and the Variable Sun-Earth Connection
The Maunder Minimum and the Variable Sun-Earth Connection (Front illustration: the Sun without spots, July 27, 1954) By Willie Wei-Hock Soon and Steven H. Yaskell To Soon Gim-Chuan, Chua Chiew-See, Pham Than (Lien+Van’s mother) and Ulla and Anna In Memory of Miriam Fuchs (baba Gil’s mother)---W.H.S. In Memory of Andrew Hoff---S.H.Y. To interrupt His Yellow Plan The Sun does not allow Caprices of the Atmosphere – And even when the Snow Heaves Balls of Specks, like Vicious Boy Directly in His Eye – Does not so much as turn His Head Busy with Majesty – ‘Tis His to stimulate the Earth And magnetize the Sea - And bind Astronomy, in place, Yet Any passing by Would deem Ourselves – the busier As the Minutest Bee That rides – emits a Thunder – A Bomb – to justify Emily Dickinson (poem 224. c. 1862) Since people are by nature poorly equipped to register any but short-term changes, it is not surprising that we fail to notice slower changes in either climate or the sun. John A. Eddy, The New Solar Physics (1977-78) Foreword By E. N. Parker In this time of global warming we are impelled by both the anticipated dire consequences and by scientific curiosity to investigate the factors that drive the climate. Climate has fluctuated strongly and abruptly in the past, with ice ages and interglacial warming as the long term extremes. Historical research in the last decades has shown short term climatic transients to be a frequent occurrence, often imposing disastrous hardship on the afflicted human populations. -
1 AA Issue 4 Final Print Version 10 Dec 07.Pub
g{x TÇà|ÖâtÜ|tÇ TáàÜÉÇÉÅxÜ Journal of the Society for the History of Astronomy Issue 4 January 2008 ISSN 1740-3677 The cover illustration The Oxford heliometer ontinuing the anniversary theme of previous covers of The Antiquarian Astronomer, this issue shows an engraving of the Oxford heliometer1. Ordered from the instrument maker A & G Repsold, C Hamburg, Germany, in 1841, the heliometer began work 160 years ago, in 1848. It was the only large example of this type of instrument installed at an observatory in Britain. The heliometer (more correctly a divided-objective-lens micrometer) was conceived by Ole Römer (1644-1710), and improved by the optician, John Dollond (1706-1761). His design used an objective lens bisected across the diameter, each part having the same focal length, and served by one eyepiece. Mounted in a frame, each semi-lens could be moved along its diameter using a fine screw-thread. The displacement between the two images gives a very precise measure of the angular separation of the stars under observa- tion, or the apparent diameter of the Sun or planet. Significant work using a heliometer was not achieved until a 6-inch instrument was delivered to the Königsberg Observatory in 1829. Designed by Joseph Fraun- hofer (1787-1826), this heliometer was used by Friedrich Bessel (1784-1846) to measure the parallax of the star 61 Cygni - the first accurate measure of the distance to the stars. Against this background of German success in using the heliometer, the trustees of the Radcliffe Observatory, Oxford, England, opted to acquire an example with a 7½-inch diameter objective lens. -
A Newly-Discovered Accurate Early Drawing of M51, the Whirlpool Nebula
Journal of Astronomical History and Heritage , 11(2), 107-115 (2008). A NEWLY-DISCOVERED ACCURATE EARLY DRAWING OF M51, THE WHIRLPOOL NEBULA William Tobin 6 rue Saint Louis, 56000 Vannes, France. E-mail: [email protected] and J.B. Holberg Lunar and Planetary Laboratory, University of Arizona, 1541 East University Boulevard, Tucson, AZ 85721, U.S.A. E-mail: [email protected] Abstract: We have discovered a lost drawing of M51, the nebula in which spiral structure was first discovered by Lord Rosse. The drawing was made in April 1862 by Jean Chacornac at the Paris Observatory using Léon Foucault’s newly-completed 80-cm silvered-glass reflecting telescope. Comparison with modern images shows that Chacornac’s drawing was more accurate with respect to gross structure and showed fainter details than any other nineteenth century drawing, although its superiority would not have been apparent at the time without nebular photography to provide a standard against which to judge drawing quality. M51 is now known as the Whirlpool Nebula, but the astronomical appropriation of ‘whirlpool’ predates Rosse’s discovery. Keywords: reflecting telescopes, nebulae, spiral structure, Léon Foucault, Lord Rosse, M51, Whirlpool Nebula 1 REFLECTING TELESCOPES AND SPIRAL STRUCTURE The French physicist Léon Foucault (1819–1868) is the father of the reflecting telescope in its modern form, with large, optically-perfect, metallized glass or ceramic mirrors. Foucault achieved this breakthrough while working as ‘physicist’ at the Paris Observatory in the late 1850s. The largest telescope that he built (Foucault, 1862) had a silvered-glass, f/5.6 primary mirror of 80-cm diameter in a Newtonian configura- tion (see Figure 1). -
Kew Observatory and the Evolution of Victorian Science, 1840–1910
introduction Kew Observatory, Victorian Science, and the “Observatory Sciences” One more recent instance of the operations of this Society in this respect I may mention, in addition to those I have slightly enumerated. I mean the important accession to the means of this Society of a fixed position, a place for deposit, regula- tion, and comparison of instruments, and for many more purposes than I could name, perhaps even more than are yet contemplated, in the Observatory at Kew. Address by Lord Francis Egerton to British Association for the Advancement of Science, June 1842 When in 1842 Lord Egerton, president of the British Association for the Advancement of Science (BAAS), announced the association’s acquisition of Kew Observatory (figure I.1), he heralded the inaugura- tion of what would become one of the major institutions of nineteenth- century British—indeed international—science. Originally built as a pri- vate observatory for King George III and long in a moribund state, after 1842 the Kew building would, as Egerton predicted, become a multi- functional observatory, put to more purposes than were even imagined in 1842. It became distinguished in several sciences: geomagnetism, me- teorology, solar astronomy, and standardization—the latter term being used in this book to refer to testing scientific instruments and develop- ing prototypes of instruments to be used elsewhere, as well as establish- ing and refining constants and standards of measurement. Many of the major figures in the physical sciences of the nineteenth century were in some way involved with Kew Observatory. For the first twenty months of the twentieth century, Kew was the site of the National Physical Labora- 3 © 2018 University of Pittsburgh Press.