Iau Commission 3 Science Meetings
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OF Versailles
THE CHÂTEAU DE VErSAILLES PrESENTS science & CUrIOSITIES AT THE COUrT OF versailles AN EXHIBITION FrOM 26 OCTOBEr 2010 TO 27 FEBrUArY 2011 3 Science and Curiosities at the Court of Versailles CONTENTS IT HAPPENED AT VErSAILLES... 5 FOrEWOrD BY JEAN-JACqUES AILLAGON 7 FOrEWOrD BY BÉATrIX SAULE 9 PrESS rELEASE 11 PArT I 1 THE EXHIBITION - Floor plan 3 - Th e exhibition route by Béatrix Saule 5 - Th e exhibition’s design 21 - Multimedia in the exhibition 22 PArT II 1 ArOUND THE EXHIBITION - Online: an Internet site, and TV web, a teachers’ blog platform 3 - Publications 4 - Educational activities 10 - Symposium 12 PArT III 1 THE EXHIBITION’S PArTNErS - Sponsors 3 - Th e royal foundations’ institutional heirs 7 - Partners 14 APPENDICES 1 USEFUL INFOrMATION 3 ILLUSTrATIONS AND AUDIOVISUAL rESOUrCES 5 5 Science and Curiosities at the Court of Versailles IT HAPPENED AT VErSAILLES... DISSECTION OF AN Since then he has had a glass globe made that ELEPHANT WITH LOUIS XIV is moved by a big heated wheel warmed by holding IN ATTENDANCE the said globe in his hand... He performed several experiments, all of which were successful, before Th e dissection took place at Versailles in January conducting one in the big gallery here... it was 1681 aft er the death of an elephant from highly successful and very easy to feel... we held the Congo that the king of Portugal had given hands on the parquet fl oor, just having to make Louis XIV as a gift : “Th e Academy was ordered sure our clothes did not touch each other.” to dissect an elephant from the Versailles Mémoires du duc de Luynes Menagerie that had died; Mr. -
The Genesis of the Essai D'une Carte Géologique
From sketches to publication : the genesis of the Essai d’une carte géologique by Omalius d’Halloy and Coquebert de Montbret (1810-1823) Isabelle Laboulais To cite this version: Isabelle Laboulais. From sketches to publication : the genesis of the Essai d’une carte géologique by Omalius d’Halloy and Coquebert de Montbret (1810-1823). Earth Sciences History. Journal of the History of the Earth Sciences Society, 2007, 26 (1), pp.31-53. hal-02932788 HAL Id: hal-02932788 https://hal.archives-ouvertes.fr/hal-02932788 Submitted on 7 Sep 2020 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. From sketches to publication : the genesis of the Essai d’une carte géologique by Omalius d’Halloy and Coquebert de Montbret (1810-1823) Isabelle Laboulais (Université Marc Bloch – Strasbourg 2) In December 1822, the Essai d’une carte géologique de la France, des Pays-Bas et de quelques contrées voisines dressée par J.-J. d’Omalius d’Halloy d’après des matériaux recueillis de concert avec Mr. le baron Coquebert de Montbret 1 left the workshop of the Parisian engraver Berthe. 2 While it is probably an exaggeration to say that this map was awaited in academic circles, its appearance had nevertheless been widely announced by the two collaborators, who multiplied initiatives to make their work known even before its publication. -
Recent Publications 1984 — 2017 Issues 1 — 100
RECENT PUBLICATIONS 1984 — 2017 ISSUES 1 — 100 Recent Publications is a compendium of books and articles on cartography and cartographic subjects that is included in almost every issue of The Portolan. It was compiled by the dedi- cated work of Eric Wolf from 1984-2007 and Joel Kovarsky from 2007-2017. The worldwide cartographic community thanks them greatly. Recent Publications is a resource for anyone interested in the subject matter. Given the dates of original publication, some of the materi- als cited may or may not be currently available. The information provided in this document starts with Portolan issue number 100 and pro- gresses to issue number 1 (in backwards order of publication, i.e. most recent first). To search for a name or a topic or a specific issue, type Ctrl-F for a Windows based device (Command-F for an Apple based device) which will open a small window. Then type in your search query. For a specific issue, type in the symbol # before the number, and for issues 1— 9, insert a zero before the digit. For a specific year, instead of typing in that year, type in a Portolan issue in that year (a more efficient approach). The next page provides a listing of the Portolan issues and their dates of publication. PORTOLAN ISSUE NUMBERS AND PUBLICATIONS DATES Issue # Publication Date Issue # Publication Date 100 Winter 2017 050 Spring 2001 099 Fall 2017 049 Winter 2000-2001 098 Spring 2017 048 Fall 2000 097 Winter 2016 047 Srping 2000 096 Fall 2016 046 Winter 1999-2000 095 Spring 2016 045 Fall 1999 094 Winter 2015 044 Spring -
WHERE WAS MEAN SOLAR TIME FIRST ADOPTED? Simone Bianchi INAF-Osservatorio Astrofisico Di Arcetri, Largo E. Fermi, 5, 50125, Flor
WHERE WAS MEAN SOLAR TIME FIRST ADOPTED? Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: It is usually stated in the literature that Geneva was the first city to adopt mean solar time, in 1780, followed by London (or the whole of England) in 1792, Berlin in 1810 and Paris in 1816. In this short paper I will partially revise this statement, using primary references when available, and provide dates for a few other European cities. Although no exact date was found for the first public use of mean time, the primacy seems to belong to England, followed by Geneva in 1778–1779 (for horologists), Berlin in 1810, Geneva in 1821 (for public clocks), Vienna in 1823, Paris in 1826, Rome in 1847, Turin in 1849, and Milan, Bologna and Florence in 1860. Keywords: mean solar time 1 INTRODUCTION The inclination of the Earth’s axis with respect to the orbital plane and its non-uniform revolution around the Sun are reflected in the irregularity of the length of the day, when measured from two consecutive passages of the Sun on the meridian. Though known since ancient times, the uneven length of true solar days became of practical interest only after Christiaan Huygens (1629 –1695) invented the high-accuracy pendulum clock in the 1650s. For proper registration of regularly-paced clocks, it then became necessary to convert true solar time into mean solar time, obtained from the position of a fictitious mean Sun; mean solar days all having the same duration over the course of the year. -
13 Astronomical Molecular Spectroscopy Timothy W
j377 13 Astronomical Molecular Spectroscopy Timothy W. Schmidt 13.1 The Giants Shoulders Stargazing, in its most primitive form, has entertained our species for hundreds of thousands of years. The ancients used knowledge of the positions of fixed stars as navigational aids and also recognized wandering stars (planets), comets, and novae. The astrolabe, an instrument for fixing the positions of stars, was invented in Greece some 2200 years ago. In medieval times, the positions of stars were of great importance to the Islamic world to indicate the correct times for prayer and the direction of Mecca, and the astrolabe was an important tool. Indeed, one of the 1) greatest observational astronomers, Tycho Brahe, performed his measurements without a telescope. He used a great mural quadrant, whereby stars were sighted through a slot in a wall with a tool attached to a 90 arc. Accurate measurements of the positions of stars and planets were made in this way, and they remained the most accurate until the introduction of well-built telescopes. Brahe died in 1601, passing 2) his legacy to Johannes Kepler, who had joined him as an assistant only a year before. Kepler continued to work with Brahes observations for a decade, during which he developed the laws of planetary motion for which he is most famous, and advanced 3) theories on geometric optics. Kepler was a contemporary of Galileo, who is credited with the development and improvement of the refractive telescope. Galileo observed the four largest moons of Jupiter and described the phases of Venus as being similar 4) to the Earths moon. -
Testo Completo
Università degli Studi di Ferrara DOTTORATO DI RICERCA IN "MATEMATICA E INFORMATICA" CICLO XXVI COORDINATORE Prof. Mella Massimiliano L’INTERNAZIONALIZZAZIONE DEGLI STUDI MATEMATICI IN ITALIA A METÀ OTTOCENTO Settore Scientifico Disciplinare MAT / 04 Dottorando Tutore Dott. Nagliati Iolanda Prof. Borgato Maria Teresa ________________________ ___________________________ (firma) (firma) Anni 2011/2013 1 1 L’internazionalizzazione degli studi matematici in Italia a metà Ottocento Introduction p. 3 Introduzione 17 L’internazionalizzazione degli studi 21 I rapporti di Betti con studiosi stranieri: temi delle lettere Corrispondenti stranieri di Brioschi Corrispondenti stranieri di Tardy La situazione degli esuli: Mossotti da Corfù a Pisa 43 Il ritorno dall’esilio I primi anni dell’attività a Pisa e i rapporti con Betti Vicende politiche, organizzazione degli studi e della ricerca nella corrispondenza tra Brioschi e Tardy 59 L’organizzazione degli studi superiori Gli “Annali” Le equazioni algebriche di quinto grado 73 La teoria degli invarianti 81 Ricerche sui differenziali ad indice fratto 99 Le riviste scientifiche toscane nell’Ottocento 109 Documenti: Lettere di Giorgini a Mossotti 127 Lettere di Mossotti a Tardy 135 Lettere di Mossotti a Betti 139 Carteggio Brioschi-Tardy 191 Lettere a Betti di studiosi stranieri 285 Lettere a Tardy di studiosi stranieri 342 Lettere a Brioschi di studiosi stranieri 369 Bibliografia 371 1 2 Introduction The past few decades have seen several studies carried out by historians of mathematics on mathematics in the post unification period in Italy, further interest being recently stimulated by the celebration of 150 years since the Unification of Italy; this moment brought about a period of renewal of structures and infrastructures suitable for the new state, a sort of modernisation of the economy, which, at the same time, required a new institutional organisation on a national level for the scientific community, to carry on the work already started in the previous decades by single states, like Piedmont and the Grand Duchy of Tuscany. -
The Book of Roger Brady Hibbs Ouachita Baptist University
Ouachita Baptist University Scholarly Commons @ Ouachita History Class Publications Department of History 3-31-2015 The Book of Roger Brady Hibbs Ouachita Baptist University Follow this and additional works at: https://scholarlycommons.obu.edu/history Part of the Medieval History Commons Recommended Citation Hibbs, Brady, "The Book of Roger" (2015). History Class Publications. 22. https://scholarlycommons.obu.edu/history/22 This Class Paper is brought to you for free and open access by the Department of History at Scholarly Commons @ Ouachita. It has been accepted for inclusion in History Class Publications by an authorized administrator of Scholarly Commons @ Ouachita. For more information, please contact [email protected]. Brady Hibbs 31 March 2015 Medieval Europe The Book of Roger Tabula Rogeriana (Latin for “Book of Roger) is the name of a publication created by Arab cartographer Muhammad al-Idrisi in 1154 under the guidance of King Roger II of Sicily. The book is recognized for its groundbreaking world map and its accompanying descriptions and information regarding the areas shown in the map. The world map is divided into 70 regional maps, with these divisions dictated by the seven climate zones (originally proposed by Ptolemy) al-Idrisi used for the map along with ten geographical sections (Glick, 2014). The book begins with the southwestern most section, which includes the Canary Islands, to the easternmost section, then proceeds northward until each section has been represented. With each section, al-Idrisi gives textual descriptions of the land in the maps and described the people who were indigenous to those regions. The whole map includes lands from Spain in the east to China in the west, and Scandinavia in the north, down to Africa in the south. -
1 the Founding of Arcetri Observatory in Florence
THE FOUNDING OF ARCETRI OBSERVATORY IN FLORENCE Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: The first idea of establishing a public astronomical observatory in Florence, Capital of the Grand Duchy of Tuscany, dates to the mid of the 18th century. Initially, the use of a low building on a high ground was proposed, and the hill of Arcetri suggested as a proper location. At the end of the century, the Florence Observatory - or Specola - was built instead on a tower at the same level as the city’s centre. As soon as astronomers started to use this observatory, they recognized all its flaws and struggled to search for a better location. Giovanni Battista Donati, director of the Specola of Florence from the eve of the Italian Unification in 1859, finally succeeded in creating a new observatory: first, he obtained funds from the Parliament of the Kingdom of Italy to build an equatorial mount for the Amici 28-cm refractor, which could not be installed conveniently in the tower of the Specola; then, he went through the process of selecting a proper site, seeking funds and finally building Arcetri Observatory. Although Donati was a pioneer of spectroscopy and astrophysics, his intent was to establish a modern observatory for classical astronomy, as the Italian peninsula did not have a national observatory like those located in many foreign capitals – Florence was the capital of the Kingdom of Italy from 1865 to 1871. To promote the project, Donati made use of writings by one of the most authoritative European astronomers, Otto Wilhelm Struve. -
Jjmonl 1606.Pmd
alactic Observer GJohn J. McCarthy Observatory Volume 9, No. 6 June 2016 Dead End? Conventional wisdom has long held that galaxies regenerate from the gas and debris of their own dead stars. Find out why that isn't always true - inside, page 15 http://www.mccarthyobservatory.org June 2016 • 1 The John J. McCarthy Observatory Galactic Observvvererer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky It is through their efforts that the McCarthy Observatory Technical Support has established itself as a significant educational and Bob Lambert recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Mike Chiarella Roger Moore Route Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Cecilia Dietrich Marc Polansky Dirk Feather Joe Privitera Randy Fender Monty Robson Randy Finden Don Ross John Gebauer Gene Schilling Elaine Green Katie Shusdock Tina Hartzell Paul Woodell Tom Heydenburg Amy Ziffer In This Issue OUT THE WINDOW ON YOUR LEFT .................................... 4 ASTRONOMICAL AND HISTORICAL EVENTS ......................... 12 SURVEYOR 1 LANDING SITE .............................................. 4 COMMONLY USED TERMS ............................................... 14 2016 MERCURY TRANSIT -
Assessing the Reliability of the 1760 British Geographical Survey of the St
Assessing the Reliability of the 1760 British Geographical Survey of the St. Lawrence River Valley by Nicholas Gliserman A Thesis Presented to the Faculty of the USC Graduate School University of Southern California In Partial Fulfillment of the Requirements for the Degree Master of Science (Geographic Information Science and Technology) May 2018 Copyright © 2018 by Nicholas Gliserman ii To my loving wife, Christina Copland iii Table of Contents List of Figures ................................................................................................................................. vi List of Tables ................................................................................................................................... x Acknowledgements ........................................................................................................................ xi List of Abbreviations .................................................................................................................... xii Abstract ........................................................................................................................................ xiii Chapter 1: Introduction .................................................................................................................... 1 Chapter 2: Towards a Historiographical Synthesis of Archival and Digital Methods .................... 7 2.1. The Underwhelming Presence of Historical Maps in the Spatial Humanities ................... 8 2.2. Scholarship on the Murray -
The Worldwide Impact of Donati's Comet on Art and Society in the Mid
The Rˆole of Astronomy in Society and Culture Proceedings IAU Symposium No. 260, 2011 c 2011 International Astronomical Union D. Valls-Gabaud & A. Boksenberg, eds. DOI: 00.0000/X000000000000000X The worldwide impact of Donati’s comet on art and society in the mid-19th century Antonella Gasperini1, Daniele Galli1 and Laura Nenzi2 1 INAF–Osservatorio Astrofisico di Arcetri, Firenze, Italy email: gasperi,[email protected] 2 University of Tennessee, Knoxville, USA email: [email protected] Abstract. Donati’s comet was one of the most impressive astronomical events of the nineteenth century. Its extended sword-like tail was a spectacular sight that inspired several literary and artistic representations. Traces of Donati’s comet are found in popular magazines, children’s books, collection cards, and household objects through the beginning of the twentieth century. Keywords. Donati’s comet, 19th century literature and art 1. Introduction Donati’s comet was discovered in Florence on June 2, 1858. It became visible to the naked eye in the northern and southern hemispheres between September 1858 and March 1859. Its gracefully curved tail, which extended almost 40 degrees in the southwestern sky, made a great visual impact and inspired several pictorial (paintings, watercolours, sketches) and poetic (lyrical and satirical) representations, especially in Great Britain and France. In the Eastern world, the influence of Donati’s comet on contemporary society is particularly significant in Siam and Japan. This contribution outlines the relations and interconnections between a scientific discovery, the artistic movements of the period, and the different social environments in a worldwide context. 2. The discoverer, Giovanni Battista Donati Giovanni Battista Donati was born in Pisa in 1826 and studied physics and mathemat- ics at the local University under the guidance of O. -
Introduction
Cambridge University Press 978-1-107-00229-6 - Unravelling Starlight: William and Margaret Huggins and the Rise of the New Astronomy Barbara J. Becker Excerpt More information 1 Introduction where in the murky depths of mind do idea-seeds sleep? what seasons do they know that make them wont to wake and grow in spasms – madly now, dormant then – entangling all within their ken: synaptic vines to clamber to the very stars. My interest in the life and work of English astronomer William Huggins (1824–1910) began over twenty years ago in a graduate seminar on conceptual transfer within and among specialised scientific communities. The exchange of cultural baggage is a subtle dynamic that practitioners, particularly those working in long-established disciplines, usually take care to shield from public view. Our little group spent the semester analysing the far more transparent machinery of newer, still-developing hybrid disciplines like geophysics, bio- chemistry and astrobiology. The topic meshed well with my own research interests at the time. I wanted to learn more about how the boundaries of scientific disciplines are established, policed and altered: What are the rules members must follow in investigating the natural world? What questions are deemed appropriate to ask? What do good answers to such questions look like and how can they be recognised? What constitutes an acceptable way of finding those answers? Who is allowed to participate in the search? Who says? How better to find answers to these questions than to watch a scientific discipline during a period of change? I chose to explore the origins of astrophysics, a mature hybrid science that blends the methods, instruments and theories of chemistry and physics, as well as those of both mathematical and descriptive astronomy.