The First Four Asteroids: a History of Their Impact on English Astronomy in the Early Nineteenth Century
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Mathematics Is a Gentleman's Art: Analysis and Synthesis in American College Geometry Teaching, 1790-1840 Amy K
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 2000 Mathematics is a gentleman's art: Analysis and synthesis in American college geometry teaching, 1790-1840 Amy K. Ackerberg-Hastings Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Higher Education and Teaching Commons, History of Science, Technology, and Medicine Commons, and the Science and Mathematics Education Commons Recommended Citation Ackerberg-Hastings, Amy K., "Mathematics is a gentleman's art: Analysis and synthesis in American college geometry teaching, 1790-1840 " (2000). Retrospective Theses and Dissertations. 12669. https://lib.dr.iastate.edu/rtd/12669 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margwis, and improper alignment can adversely affect reproduction. in the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. -
Messier Objects
Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun. -
Chapter Two: the Astronomers and Extraterrestrials
Warning Concerning Copyright Restrictions The Copyright Law of the United States (Title 17, United States Code) governs the making of photocopies or other reproductions of copyrighted materials, Under certain conditions specified in the law, libraries and archives are authorized to furnish a photocopy or other reproduction, One of these specified conditions is that the photocopy or reproduction is not to be used for any purpose other than private study, scholarship, or research , If electronic transmission of reserve material is used for purposes in excess of what constitutes "fair use," that user may be liable for copyright infringement. • THE EXTRATERRESTRIAL LIFE DEBATE 1750-1900 The idea of a plurality of worlds from Kant to Lowell J MICHAEL]. CROWE University of Notre Dame TII~ right 0/ ,It, U,,;v"Jily 0/ Camb,idg4' to P'''''' a"d s,1I all MO""" of oooks WM grattlrd by H,rr,y Vlf(;ff I $J4. TM U,wNn;fyltas pritr"d and pu"fisllrd rOffti",.ously sincr J5U. Cambridge University Press Cambridge London New York New Rochelle Melbourne Sydney Published by the Press Syndicate of the University of Cambridge In lovi ng The Pirr Building, Trumpingron Srreer, Cambridge CB2. I RP Claire H 32. Easr 57th Streer, New York, NY 1002.2., U SA J 0 Sramford Road, Oakleigh, Melbourne 3166, Australia and Mi ha © Cambridge Univ ersiry Press 1986 firsr published 1986 Prinred in rh e Unired Srares of America Library of Congress Cataloging in Publication Data Crowe, Michael J. The exrrarerresrriallife debare '750-1900. Bibliography: p. Includes index. I. Pluraliry of worlds - Hisrory. -
Edgar Buckingham: Fluorescence of Quinine Salts
Bull. Hist. Chem., VOLUME 27, Number 1 (2002) 57 EDGAR BUCKINGHAM: FLUORESCENCE OF QUININE SALTS John T. Stock, University of Connecticut Malaria, an often-fatal disease, has been a worldwide factured from cinchona trees that are cultivated in South plague for several thousand years. The discovery of America and in the Far East. the efficacy of substances present in the bark of vari- It must have been known ous cinchona trees, native since ancient times that certain to the Andes, provided substances appear to have one some relief. A real anti- color when viewed by transmit- malarial drug was not ted light and another when available until 1820, when viewed obliquely. Mineralo- Joseph Baptiste Caventou gists recognize a type of fluor- (1795-1877) and Josephe spar, pale green when viewed Pelletier (1788-1842) iso- against the light, but appearing lated quinine from the blue when viewed at an angle bark (1). Eighty years af- to the light. Unrefined petro- ter their discovery, a statue leum shows the same kind of honoring these chemists effect, as do certain substances was erected in Paris (Fig. when in solution. Fluorescein, 1). used both in the laboratory as Other workers estab- an indicator and industrially for lished the formula for qui- the location of leaks in waste nine, showed that it acts as water systems, is a familiar ex- a diacid base, and that it ample. Another is quinine or, is a methoxy derivative of because of its low solubility in a companion alkaloid, cin- water, one of its salts. The so- chonine. The elucidation lution, colorless when viewed of the structure of these directly, appears blue when compounds, largely due to viewed at an angle to the inci- the work of Wilhelm dent light. -
Edwin Danson, UK: the Work of Charles Mason and Jeremiah Dixon
The Work of Charles Mason and Jeremiah Dixon Edwin DANSON, United Kingdom Key words: Mason, Charles; Dixon, Jeremiah; Mason-Dixon Line; Pre-revolutionary History; Surveying; Geodesy; US History; Pennsylvania; Maryland. ABSTRACT The geodetic activities of Charles Mason and Jeremiah Dixon in America between 1763-68 were, for the period, without precedent. Their famous boundary dividing Maryland from Pennsylvania, the Mason-Dixon Line, today remains a fitting monument to these two brave, resourceful and extremely talented scientists. Tutored by Astronomer Royal Dr James Bradley, Charles Mason was aware of the contemporary theories and experiments to establish the true shape of the Earth. He was also cognisant of what was being termed “the attraction of mountains” (deviation of the vertical). However, at the time it was no more than a theory, a possibility, and it was by no means certain whether the Earth was solid or hollow. The Mason-Dixon Line, a line of constant latitude fifteen miles south of Philadelphia, although the most arduous of their tasks, was only part of their work for the proprietors of Maryland and Pennsylvania. For the Royal Society of London, they also measured the first degree of latitude in America. In recent years, the Mason-Dixon Line Preservation Partnership has located many of the original markers and surveyed them using GPS. The paper reviews the work of Mason and Dixon covering the period 1756-1786. In particular, their methods and results for the American boundary lines are discussed together with comments on the accuracy they achieved compared with GPS observations. CONTACT Edwin Danson 14 Sword Gardens Swindon, SN5 8ZE UNITED KINGDOM Tel. -
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. -
Volta, the Istituto Nazionale and Scientific Communication in Early Nineteenth-Century Italy*
Luigi Pepe Volta, the Istituto Nazionale and Scientific Communication in Early Nineteenth-Century Italy* In a famous paper published in Isis in 1969, Maurice Crosland posed the question as to which was the first international scientific congress. Historians of science commonly established it as the Karlsruhe Congress of 1860 whose subject was chemical notation and atomic weights. Crosland suggested that the first international scientific congress could be considered the meeting convened in Paris on January 20, 1798 for the definition of the metric system.1 In September 1798 there arrived in Paris Bugge from Denmark, van Swinden and Aeneae from Germany, Trallès from Switzerland, Ciscar and Pedrayes from Spain, Balbo, Mascheroni, Multedo, Franchini and Fabbroni from Italy. These scientists joined the several scientists already living in Paris and engaged in the definition of the metric system: Coulomb, Mechain, Delambre, Laplace, Legendre, Lagrange, etc. English and American scientists, however, did not take part in the meeting. The same question could be asked regarding the first national congress in England, in Germany, in Switzerland, in Italy, etc. As far as Italy is concerned, many historians of science would date the first meeting of Italian scientists (Prima Riunione degli Scienziati Italiani) as the one held in Pisa in 1839. This meeting was organised by Carlo Luciano Bonaparte, Napoleon’s nephew, with the co-operation of the mathematician Gaetano Giorgini under the sanction of the Grand Duke of Tuscany Leopold II (Leopold was a member of the Royal Society).2 Participation in the meetings of the Italian scientists, held annually from 1839 for nine years, was high: * This research was made possible by support from C.N.R. -
Literary Branding in the Romantic Period
Literary Branding in the Romantic Period by Christopher Laxer A thesis submitted in conformity with the requirements for the degree of Doctor of Philosophy Graduate Department of English University of Toronto © Copyright by Christopher Laxer 2013 Literary Branding in the Romantic Period Christopher Laxer Doctor of Philosophy Department of English University of Toronto 2013 Abstract This thesis argues that, unlike the study of commodity branding, the study of literary branding should not focus solely upon book advertising, but rather investigate all of the processes of attribution that connect conceptual domains with literary labels, enabling their common use in the perception and navigation of the cultural world. Such processes should not be understood exclusively by analogy with the forms of commodity branding that originated in the consumer revolutions of the eighteenth or nineteenth centuries, but rather as the inherent consequences of more ancient and fundamental practices of naming and poetry. Rather than interpret the reactions of historical readers to Byron, for instance, largely in terms of the author as subject – as has been the tendency with earlier approaches to the question – this thesis seeks to explore historical readers’ reactions to the author’s name as label. The readers of Don Juan in 1819 knew Byron, not as we do after two centuries of biographical research, scholarly inquiry, and literary criticism, but as a literary label with relatively few associations. Arguing that the recent vogue for celebrity studies risks reifying elements of what Jerome McGann has called the Romantic Ideology, this thesis attempts to begin to redress this critical imbalance by examining the deployment of a number of interconnected literary labels in a series of case studies. -
Hamilton College Library "Home Notes"
American Communal Societies Quarterly Volume 3 Number 4 Pages 232-236 October 2009 Hamilton College Library "Home Notes" Follow this and additional works at: https://digitalcommons.hamilton.edu/acsq This work is made available by Hamilton College for educational and research purposes under a Creative Commons BY-NC-ND 4.0 license. For more information, visit http://digitalcommons.hamilton.edu/about.html or contact [email protected]. et al.: Hamilton College Library "Home Notes" Hamilton College Library “Home Notes” Communal Societies Collection New Acquisitions SEAL OF JOANNA SOUTHCOTT FIRST MEssENGER OF THE CHRISTIAN ISRAELITES Hamilton College Library recently acquired a remarkable collection of documents relating to Joanna Southcott (1750-1814) for its Communal Societies Collection. Southcott is considered to have been the first messenger of the Christian Israelite faith.1 In 1792 Southcott realized she was the woman spoken of in Revelation 12: 1And there appeared a great wonder in heaven; a woman clothed with the sun, and the moon under her feet, and upon her head a crown of twelve stars: 2And she being with child cried, travailing in birth, and pained to be delivered. Southcott gained an increasing number of followers throughout the late 1790s. Many adherents of contemporary messenger Richard Brothers, considered second in the lineage by the followers of Benjamin and Mary Purnell (House of David and Mary’s City of David), defected to Southcott upon Brothers’ imprisonment in 1795. Among these was the engraver William Sharp who brought Southcott to London to begin the process of “sealing” the elect, or the 144,000 who would be saved at the Day of Judgment. -
The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24). -
Articles Articles
Articles Articles ALEXI BAKER “Precision,” “Perfection,” and the Reality of British Scientific Instruments on the Move During the 18th Century Résumé Abstract On représente souvent les instruments scientifiques Early modern British “scientific” instruments, including du 18e siècle, y compris les chronomètres de précision, precision timekeepers, are often represented as static, comme des objets statiques, à l’état neuf et complets en pristine, and self-contained in 18th-century depictions eux-mêmes dans les descriptions des débuts de l’époque and in many modern museum displays. In reality, they moderne et dans de nombreuses expositions muséales were almost constantly in physical flux. Movement and d’aujourd’hui. En réalité, ces instruments se trouvaient changing and challenging environmental conditions presque constamment soumis à des courants physiques. frequently impaired their usage and maintenance, Le mouvement et les conditions environnementales especially at sea and on expeditions of “science” and difficiles et changeantes perturbaient souvent leur exploration. As a result, individuals’ experiences with utilisation et leur entretien, en particulier en mer et mending and adapting instruments greatly defined the lors d’expéditions scientifiques et d’exploration. Ce culture of technology and its use as well as later efforts sont donc les expériences individuelles de réparation at standardization. et d’adaptation des instruments qui ont grandement contribué à définir la culture de la technologie. In 1769, the astronomer John Bradley finally the calculation of the distance between the Earth reached the Lizard peninsula in Cornwall and the Sun. Bradley had not needed to travel with his men, instruments, and portable tent as far as many of his Transit counterparts, but observatory after a stressful journey. -
Downloading Material Is Agreeing to Abide by the Terms of the Repository Licence
Cronfa - Swansea University Open Access Repository _____________________________________________________________ This is an author produced version of a paper published in: Transactions of the Honourable Society of Cymmrodorion Cronfa URL for this paper: http://cronfa.swan.ac.uk/Record/cronfa40899 _____________________________________________________________ Paper: Tucker, J. Richard Price and the History of Science. Transactions of the Honourable Society of Cymmrodorion, 23, 69- 86. _____________________________________________________________ This item is brought to you by Swansea University. Any person downloading material is agreeing to abide by the terms of the repository licence. Copies of full text items may be used or reproduced in any format or medium, without prior permission for personal research or study, educational or non-commercial purposes only. The copyright for any work remains with the original author unless otherwise specified. The full-text must not be sold in any format or medium without the formal permission of the copyright holder. Permission for multiple reproductions should be obtained from the original author. Authors are personally responsible for adhering to copyright and publisher restrictions when uploading content to the repository. http://www.swansea.ac.uk/library/researchsupport/ris-support/ 69 RICHARD PRICE AND THE HISTORY OF SCIENCE John V. Tucker Abstract Richard Price (1723–1791) was born in south Wales and practised as a minister of religion in London. He was also a keen scientist who wrote extensively about mathematics, astronomy, and electricity, and was elected a Fellow of the Royal Society. Written in support of a national history of science for Wales, this article explores the legacy of Richard Price and his considerable contribution to science and the intellectual history of Wales.