Jean-Sylvain Bailly's History of Indian Astronomy
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Jacques-Louis David's 'Oath of the Tennis Court'
EXTENSION ACTIVITIES – Jacques-Louis David’s ‘Oath of the Tennis Court’, 1791 Read the discussion of Jacques-Louis-David’s ‘Oath of the Tennis Court’ (1791) on p. 3-8 of this handout. Then complete the following extension activities: 1. One of the big problems which faced David as the Revolution progressed was that many of the figures to whom he had given prominence in the 1791 drawing fell from favour as political conditions changed. Using Liberating France (including the Who’s Who) and other sources, find out what happened to Mounier, Mirabeau, Bailly, Barère, Barnave, and Robespierre. Then research the clergymen, Abbé Grégoire and Abbé Sieyès. 2. David alludes to the popular movement which became known as the sans-culottes through the strong and robust figure in the red bonnet of liberty in the lower left hand corner. Referring to Liberating France (including the Section B Timeline), write a paragraph to outline the role played by the sans-culottes movement from 10 August 1792 until the days of Germinal and Prairial Year III, (1 April and 20-23 May 1795). 3. Using Liberating France (including the Who’s Who) and other sources, outline David’s revolutionary career – both as a painter and as a politician. In your answer consider the importance his paintings and drawings 1789-1795, and his role in organising public ceremonies. Then investigate his political activities as a deputy in the National Convention. 4. David uses at least eight revolutionary ideas in his 1791 study of the Tennis Court Oath. Locate them and any other revolutionary ideas not mentioned in the summary above. -
The Democratic Sphere Communications with the French National Assembly's Committee of Research,1789-1791
The Democratic Sphere Communications with the French National Assembly's Committee of Research,1789-1791 Maia Kirby Queen Mary, University of London Submitted in partial fulfilment of the requirements of the degree of Doctor of Philosophy 1 I, Maia Olive Claire Kirby, confirm that the research included within this thesis is my own work or that where it has been carried out in collaboration with, or supported by others, that this is duly acknowledged below and my contribution indicated. Previously published material is also acknowledged below. I attest that I have exercised reasonable care to ensure that the work is original, and does not to the best of my knowledge break any UK law, infringe any third party’s copyright or other Intellectual Property Right, or contain any confidential material. I accept that the College has the right to use plagiarism detection software to check the electronic version of the thesis. I confirm that this thesis has not been previously submitted for the award of a degree by this or any other university. The copyright of this thesis rests with the author and no quotation from it or information derived from it may be published without the prior written consent of the author. Signature: Maia Kirby Date: 24.08.16 2 Abstract On 28 July 1789 the National Assembly established the Committee of Research as a mechanism through which it could identify threats to its existence from amongst its large correspondence. In the time it was active, the committee received thousands of letters from across France. In the early 1990s the archivist Pierre Caillet wrote a thorough inventory and a general synthesis of the communications which further opened them up as a resource that could provide insight into popular reponses to various themes. -
BABYLONIAN ASTRONOMY* by W.M. O'neil Though the Modern Western
o BABYLONIAN ASTRONOMY* By W.M. O'Neil Though the modern western world had heard of the Chaldaeans in the Old Testament as soothsayers and astrologers and students of Hellenistic astronomy knew of references to Babylonian observations of eclipses and the like, it is only during the last three quarters of a century but especially during the last half century that modern scholars, following the decipherment of the cuneiform writing on clay tablets, have begun to reveal the richness of Babylonian astronomy. They have, however, a long way yet to go. First, only a fraction of the materials scattered throughout the western world have been studied and interpreted. Fragments of the one tablet are sometimes in different museums; this adds to the difficulty. Second, the materials are usually fragmentary: a few pages torn from a book as it were or even only a few parts of pages (See Plate 1). Otto Neugebauer, perhaps the greatest scholar recently working on Babylonian astronomy, says that it is impossible yet to write an adequate history of Babylonian astronomy and suggests that it may never be possible. How many of the needed basic texts have crumbled into dust after acquisition by small museums unable to give them the needed care? , how many are lying unstudied in the multitudinous collections in the Middle East, in Europe and in North America? or are still lying in the ground?, are questions to which the answers are unknown. Nevertheless, through the work of Neugebauer, his predecessors and younger scholars taking over from him, some outlines of the history and the methods of Babylonian astronomy are becoming clearer. -
Introduction
© Copyright, Princeton University Press. No part of this book may be distributed, posted, or reproduced in any form by digital or mechanical means without prior written permission of the publisher. CHAPTER 1 Introduction French Society in 1789 Historians working on the French Revolution have a problem. All of our attempts to find an explanation in terms of social groups or classes, or particular segments of society becoming powerfully activated, have fallen short. As one expert aptly expressed it: “the truth is we have no agreed general theory of why the French Revolution came about and what it was— and no prospect of one.”1 This gaping, causal void is cer- tainly not due to lack of investigation into the Revolution’s background and origins. If class conflict in the Marxist sense has been jettisoned, other ways of attributing the Revolution to social change have been ex- plored with unrelenting rigor. Of course, every historian agrees society was slowly changing and that along with the steady expansion of trade and the cities, and the apparatus of the state and armed forces, more (and more professional) lawyers, engineers, administrators, officers, medical staff, architects, and naval personnel were increasingly infusing and diversifying the existing order.2 Yet, no major, new socioeconomic pressures of a kind apt to cause sudden, dramatic change have been identified. The result, even some keen revisionists admit, is a “somewhat painful void.”3 Most historians today claim there was not one big cause but instead numerous small contributory impulses. One historian, stressing the absence of any identifiable overriding cause, likened the Revolution’s origins to a “multi- coloured tapestry of interwoven causal factors.”4 So- cial and economic historians embracing the “new social interpretation” identify a variety of difficulties that might have rendered eighteenth- century French society, at least in some respects, more fraught and vulnerable than earlier. -
The Roots of Astronomy
The Roots of Astronomy • Already in the stone and bronze ages, human cultures realized the cyclic nature of motions in the sky. • Monuments dating back to ~ 3000 B.C. show alignments with astronomical significance. • Those monuments were probably used as calendars or even to predict eclipses. Stonehenge • Constructed: 3000 – 1800 B.C. Summer solstice Heelstone • Alignments with locations of sunset, sunrise, moonset and moonrise at summer and winter solstices • Probably used as calendar. Other Examples All Over the World Big Horn Medicine Wheel (Wyoming) Other Examples All Over the World (2) Caracol (Maya culture, approx. A.D. 1000) Ancient Greek Astronomers (1) • Unfortunately, there are no written documents about the significance of stone and bronze age monuments. • First preserved written documents about ancient astronomy are from ancient Greek philosophy. • Greeks tried to understand the motions of the sky and describe them in terms of mathematical (not physical!) models. Ancient Greek Astronomers (2) Models were generally wrong because they were based on wrong “first principles”, believed to be “obvious” and not questioned: 1. Geocentric Universe: Earth at the Center of the Universe. 2. “Perfect Heavens”: Motions of all celestial bodies described by motions involving objects of “perfect” shape, i.e., spheres or circles. Ancient Greek Astronomers (3) • Eudoxus (409 – 356 B.C.): Model of 27 nested spheres • Aristotle (384 – 322 B.C.), major authority of philosophy until the late middle ages: Universe can be divided in 2 parts: 1. Imperfect, -
Ligo-India Proposal for an Interferometric Gravitational-Wave Observatory
LIGO-INDIA PROPOSAL FOR AN INTERFEROMETRIC GRAVITATIONAL-WAVE OBSERVATORY IndIGO Indian Initiative in Gravitational-wave Observations PROPOSAL FOR LIGO-INDIA !"#!$ Indian Initiative in Gravitational wave Observations http://www.gw-indigo.org II Title of the Project LIGO-INDIA Proposal of the Consortium for INDIAN INITIATIVE IN GRAVITATIONAL WAVE OBSERVATIONS IndIGO to Department of Atomic Energy & Department of Science and Technology Government of India IndIGO Consortium Institutions Chennai Mathematical Institute IISER, Kolkata IISER, Pune IISER, Thiruvananthapuram IIT Madras, Chennai IIT, Kanpur IPR, Bhatt IUCAA, Pune RRCAT, Indore University of Delhi (UD), Delhi Principal Leads Bala Iyer (RRI), Chair, IndIGO Consortium Council Tarun Souradeep (IUCAA), Spokesperson, IndIGO Consortium Council C.S. Unnikrishnan (TIFR), Coordinator Experiments, IndIGO Consortium Council Sanjeev Dhurandhar (IUCAA), Science Advisor, IndIGO Consortium Council Sendhil Raja (RRCAT) Ajai Kumar (IPR) Anand Sengupta(UD) 10 November 2011 PROPOSAL FOR LIGO-INDIA II PROPOSAL FOR LIGO-INDIA LIGO-India EXECUTIVE SUMMARY III PROPOSAL FOR LIGO-INDIA IV PROPOSAL FOR LIGO-INDIA This proposal by the IndIGO consortium is for the construction and subsequent 10- year operation of an advanced interferometric gravitational wave detector in India called LIGO-India under an international collaboration with Laser Interferometer Gravitational–wave Observatory (LIGO) Laboratory, USA. The detector is a 4-km arm-length Michelson Interferometer with Fabry-Perot enhancement arms, and aims to detect fractional changes in the arm-length smaller than 10-23 Hz-1/2 . The task of constructing this very sophisticated detector at the limits of present day technology is facilitated by the amazing opportunity offered by the LIGO Laboratory and its international partners to provide the complete design and all the key components required to build the detector as part of the collaboration. -
Geminos and Babylonian Astronomy
Geminos and Babylonian astronomy J. M. Steele Introduction Geminos’ Introduction to the Phenomena is one of several introductions to astronomy written by Greek and Latin authors during the last couple of centuries bc and the first few centuries ad.1 Geminos’ work is unusual, however, in including some fairly detailed—and accurate—technical information about Babylonian astronomy, some of which is explicitly attributed to the “Chal- deans.” Indeed, before the rediscovery of cuneiform sources in the nineteenth century, Gem- inos provided the most detailed information on Babylonian astronomy available, aside from the reports of several eclipse and planetary observations quoted by Ptolemy in the Almagest. Early-modern histories of astronomy, those that did not simply quote fantastical accounts of pre-Greek astronomy based upon the Bible and Josephus, relied heavily upon Geminos for their discussion of Babylonian (or “Chaldean”) astronomy.2 What can be learnt of Babylonian astron- omy from Geminos is, of course, extremely limited and restricted to those topics which have a place in an introduction to astronomy as this discipline was understood in the Greek world. Thus, aspects of Babylonian astronomy which relate to the celestial sphere (e.g. the zodiac and the ris- ing times of the ecliptic), the luni-solar calendar (e.g. intercalation and the 19-year (“Metonic”) cycle), and lunar motion, are included, but Geminos tells us nothing about Babylonian planetary theory (the planets are only touched upon briefly by Geminos), predictive astronomy that uses planetary and lunar periods, observational astronomy, or the problem of lunar visibility, which formed major parts of Babylonian astronomical practice. -
The Persian-Toledan Astronomical Connection and the European Renaissance
Academia Europaea 19th Annual Conference in cooperation with: Sociedad Estatal de Conmemoraciones Culturales, Ministerio de Cultura (Spain) “The Dialogue of Three Cultures and our European Heritage” (Toledo Crucible of the Culture and the Dawn of the Renaissance) 2 - 5 September 2007, Toledo, Spain Chair, Organizing Committee: Prof. Manuel G. Velarde The Persian-Toledan Astronomical Connection and the European Renaissance M. Heydari-Malayeri Paris Observatory Summary This paper aims at presenting a brief overview of astronomical exchanges between the Eastern and Western parts of the Islamic world from the 8th to 14th century. These cultural interactions were in fact vaster involving Persian, Indian, Greek, and Chinese traditions. I will particularly focus on some interesting relations between the Persian astronomical heritage and the Andalusian (Spanish) achievements in that period. After a brief introduction dealing mainly with a couple of terminological remarks, I will present a glimpse of the historical context in which Muslim science developed. In Section 3, the origins of Muslim astronomy will be briefly examined. Section 4 will be concerned with Khwârizmi, the Persian astronomer/mathematician who wrote the first major astronomical work in the Muslim world. His influence on later Andalusian astronomy will be looked into in Section 5. Andalusian astronomy flourished in the 11th century, as will be studied in Section 6. Among its major achievements were the Toledan Tables and the Alfonsine Tables, which will be presented in Section 7. The Tables had a major position in European astronomy until the advent of Copernicus in the 16th century. Since Ptolemy’s models were not satisfactory, Muslim astronomers tried to improve them, as we will see in Section 8. -
The GREAT ARC 1-23.Qxd 6/24/03 5:27 PM Page 2
1-23.qxd 6/24/03 5:27 PM Page 1 The GREAT ARC 1-23.qxd 6/24/03 5:27 PM Page 2 SURVEY of INDIA AN INTRODUCTION Dr. Prithvish Nag, Surveyor General of India he Survey of lndia has played an invaluable respite, whether on the slopes of the Western Ghats, role in the saga of India’s nation building. the swampy areas of the Sundarbans, ponds and TIt has seldom been realized that the founding tanks, oxbow lakes or the meandering rivers of of modern India coincides with the early activities of Bengal, Madurai or the Ganga basin. Neither were this department, and the contribution of the Survey the deserts spared, nor the soaring peaks of the has received little emphasis - not even by the Himalayas, the marshlands of the Rann of Kutch, department itself. Scientific and development rivers such as the Chambal in the north and Gandak initiatives in the country could not have taken place to the east, the terai or the dooars.With purpose and without the anticipatory actions taken by the dedication the intrepid men of the Survey confronted department, which played an indispensable the waves of the Arabian Sea and Bay of Bengal, dust pioneering role in understanding the country’s storms of Rajasthan, cyclones of the eastern coast, the priorities in growth and defense. cold waves of the north and the widespread The path-breaking activities of the Survey came, monsoons and enervating heat. of course, at a price and with immense effort. The It was against this price, and with the scientific measurement of the country, which was the determination and missionary zeal of the Survey’s Survey’s primary task, had several ramifications. -
A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair
ASTRONOMY AND ASTROPHYSICS - A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair A HISTORY OF ASTRONOMY, ASTROPHYSICS AND COSMOLOGY Malcolm Longair Cavendish Laboratory, University of Cambridge, JJ Thomson Avenue, Cambridge CB3 0HE Keywords: History, Astronomy, Astrophysics, Cosmology, Telescopes, Astronomical Technology, Electromagnetic Spectrum, Ancient Astronomy, Copernican Revolution, Stars and Stellar Evolution, Interstellar Medium, Galaxies, Clusters of Galaxies, Large- scale Structure of the Universe, Active Galaxies, General Relativity, Black Holes, Classical Cosmology, Cosmological Models, Cosmological Evolution, Origin of Galaxies, Very Early Universe Contents 1. Introduction 2. Prehistoric, Ancient and Mediaeval Astronomy up to the Time of Copernicus 3. The Copernican, Galilean and Newtonian Revolutions 4. From Astronomy to Astrophysics – the Development of Astronomical Techniques in the 19th Century 5. The Classification of the Stars – the Harvard Spectral Sequence 6. Stellar Structure and Evolution to 1939 7. The Galaxy and the Nature of the Spiral Nebulae 8. The Origins of Astrophysical Cosmology – Einstein, Friedman, Hubble, Lemaître, Eddington 9. The Opening Up of the Electromagnetic Spectrum and the New Astronomies 10. Stellar Evolution after 1945 11. The Interstellar Medium 12. Galaxies, Clusters Of Galaxies and the Large Scale Structure of the Universe 13. Active Galaxies, General Relativity and Black Holes 14. Classical Cosmology since 1945 15. The Evolution of Galaxies and Active Galaxies with Cosmic Epoch 16. The Origin of Galaxies and the Large-Scale Structure of The Universe 17. The VeryUNESCO Early Universe – EOLSS Acknowledgements Glossary Bibliography Biographical SketchSAMPLE CHAPTERS Summary This chapter describes the history of the development of astronomy, astrophysics and cosmology from the earliest times to the first decade of the 21st century. -
Historical Astronomy
Historical Astronomy (Neolithic record of Moon Phases) Introduction Arguably the history of astronomy IS the history of science. Many cultures carried out astronomical observations. However, very few formed mathematical or physical models based on their observations. It is those that did that we will focus on here, primarily the Babylonians and Greeks. Other Examples At the same time, that focus should not cause us to forget the impressive accomplishments of other cultures. Other Examples ∼ 2300 year old Chankillo Big Horn Medicine Wheel, Observatory, near Lima, Wyoming Peru Other Examples Chinese Star Map - Chinese records go back over 4000 Stonehenge, England years Babylonian Astronomy The story we will follow in more detail begins with the Babylonians / Mesopotamians / Sumerians, the cultures that inhabited the “fertile crescent.” Babylonian Astronomy Their observations and mathematics was instrumental to the development of Greek astronomy and continues to influence science today. They were the first to provide a mathematical description of astronomical events, recognize that astronomical events were periodic, and to devise a theory of the planets. Babylonian Astronomy Some accomplishments: • The accurate prediction of solar and lunar eclipses. • They developed mathematical models to predict the motions of the planets. • Accurate star charts. • Recognized the changing apparent speed of the Sun’s motion. • Developed models to account for the changing speed of the Sun and Moon. • Gave us the idea of 360◦ in a circle, 600 in a degree, 6000 in a minute. Alas, only very fragmentary records of their work survives. Early Greek The conquests of Alexander the Great are oen credited with bringing knowl- edge of the Babylonians science and mathematics to the Greeks. -
Jean-Sylvain Bailly (BUY-Yee) Member of the National Assembly
ROUSSEAU, BURKE AND REVOLUTION IN FRANCE, 1791 FEUILLANT FACTION Jean-Sylvain Bailly (BUY-yee) Member of the National Assembly ou are cultured and influential. You were born 55 years ago in Paris and raised in its environs and in Versailles. Your family has always been deeply involved in court life. Both your father and grandfather were court painters and you originally intended Y to follow in their footsteps. You became attracted in the course of your studies to astronomical science, however, and prepared a career in that path instead, building an observatory in the Louvre and promoting the new science everywhere. You were elected to the French Academy in 1783, and by the time the Revolution began, you were a renowned astronomer and a bril- liant philosophe. Your Essay on the Theory of the Satellites of Jupiter added to Galileo and Kepler’s vision of the universe, and your literary reputation was not far below that of your scientific one. Everyone knows who you are and admires you. This is France, after all, and to be a brilliant philosopher is to be influential. It is not surprising, then, that when you wished to take part in revolutionary politics, you found the path wide open. You presided over your district’s elections for delegates to the Estates General, and you yourself were elected. The Third Estate contingent was thrilled to have such a brilliant mind as yours; it brought prestige and honor to the delegates (who were, after all, mere commoners). When the Third Estate fol- lowed Sieyès and declared itself to be the National Assembly, it chose you as its president.