1 Early Life
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Cultural Gap: an International Physicist’S Experience
Bridging the Socio- Cultural Gap: An International Physicist’s Experience J. Pedro Ochoa Berkeley Lab APS March Meeting: Experiences and Issues of Young Physicist’s on the International Arena Dallas, TX – March 2011 1 Wednesday, July 20, 2011 Let’s start with an example… Some quick facts about the academic career of Isaac Newton, arguably the best physicist of all times: Born in Lincolnshire Educated at King’s School, Grantham Attended Trinity College in Cambridge His advisors were Isaac Barrow and Benjamin Pulleyn He was appointed the Lucasian Professor of Mathematics at Cambridge Mentored notable students such as Roger Cotes and William Whiston. Died in Kensington at age 67 2 Wednesday, July 20, 2011 Let’s start with an example… Some quick facts about the academic career of Isaac Newton, arguably the best physicist of all times: England Born in Lincolnshire Educated at King’s School, Grantham Attended Trinity College in Cambridge His advisors were Isaac Barrow and Benjamin Pulleyn He was appointed the Lucasian Professor of Mathematics at Cambridge Mentored notable students such as Roger Cotes and William Whiston. Died in Kensington at age 67 2 Wednesday, July 20, 2011 Let’s start with an example… Some quick facts about the academic career of Isaac Newton, arguably the best physicist of all times: England Born in Lincolnshire England Educated at King’s School, Grantham Attended Trinity College in Cambridge His advisors were Isaac Barrow and Benjamin Pulleyn He was appointed the Lucasian Professor of Mathematics -
Newton.Indd | Sander Pinkse Boekproductie | 16-11-12 / 14:45 | Pag
omslag Newton.indd | Sander Pinkse Boekproductie | 16-11-12 / 14:45 | Pag. 1 e Dutch Republic proved ‘A new light on several to be extremely receptive to major gures involved in the groundbreaking ideas of Newton Isaac Newton (–). the reception of Newton’s Dutch scholars such as Willem work.’ and the Netherlands Jacob ’s Gravesande and Petrus Prof. Bert Theunissen, Newton the Netherlands and van Musschenbroek played a Utrecht University crucial role in the adaption and How Isaac Newton was Fashioned dissemination of Newton’s work, ‘is book provides an in the Dutch Republic not only in the Netherlands important contribution to but also in the rest of Europe. EDITED BY ERIC JORINK In the course of the eighteenth the study of the European AND AD MAAS century, Newton’s ideas (in Enlightenment with new dierent guises and interpre- insights in the circulation tations) became a veritable hype in Dutch society. In Newton of knowledge.’ and the Netherlands Newton’s Prof. Frans van Lunteren, sudden success is analyzed in Leiden University great depth and put into a new perspective. Ad Maas is curator at the Museum Boerhaave, Leiden, the Netherlands. Eric Jorink is researcher at the Huygens Institute for Netherlands History (Royal Dutch Academy of Arts and Sciences). / www.lup.nl LUP Newton and the Netherlands.indd | Sander Pinkse Boekproductie | 16-11-12 / 16:47 | Pag. 1 Newton and the Netherlands Newton and the Netherlands.indd | Sander Pinkse Boekproductie | 16-11-12 / 16:47 | Pag. 2 Newton and the Netherlands.indd | Sander Pinkse Boekproductie | 16-11-12 / 16:47 | Pag. -
The First Measurement of the Deflection of the Vertical in Longitude
Eur. Phys. J. H. DOI: 10.1140/epjh/e2014-40055-2 The first measurement of the deflection of the vertical in longitude The figure of the earth in the early 19th century Andreas Schrimpfa Philipps-Universit¨atMarburg, Fachbereich Physik, Renthof 5, D-35032 Marburg, Germany Abstract. During the summer of 1837 Christian Ludwig Gerling, a for- mer student of Carl Friedrich Gauß’s, organized the world wide first de- termination of the deflection of the vertical in longitude. From a mobile observatory at the Frauenberg near Marburg (Hesse) he measured the astronomical longitude difference between C.F. Gauß’s observatory at G¨ottingenand F.G.B. Nicolai's observatory at Mannheim within an er- ror of 000: 4. To achieve this precision he first used a series of light signals for synchronizing the observatory clocks and, second, he very carefully corrected for the varying reaction time of the observers. By comparing these astronomical results with the geodetic{determined longitude dif- ferences he had recently measured for the triangulation of Kurhessen, he was able to extract a combined value of the deflection of the vertical in longitude of G¨ottingenand Mannheim. His results closely agree with modern vertical deflection data. 1 Introduction The discussion about the figure of the earth and its determination was an open ques- tion for almost two thousand years, the sciences involved were geodesy, geography and astronomy. Without precise instruments the everyday experience suggested a flat, plane world, although ideas of a spherically shaped earth were known and ac- cepted even in the ancient world. Assuming that the easily observable daily motion of the stars is due to the rotation of the earth, the rotational axis can be used to define a celestial sphere; a coordinate system, where the stars' position is given by two angles. -
Maty's Biography of Abraham De Moivre, Translated
Statistical Science 2007, Vol. 22, No. 1, 109–136 DOI: 10.1214/088342306000000268 c Institute of Mathematical Statistics, 2007 Maty’s Biography of Abraham De Moivre, Translated, Annotated and Augmented David R. Bellhouse and Christian Genest Abstract. November 27, 2004, marked the 250th anniversary of the death of Abraham De Moivre, best known in statistical circles for his famous large-sample approximation to the binomial distribution, whose generalization is now referred to as the Central Limit Theorem. De Moivre was one of the great pioneers of classical probability the- ory. He also made seminal contributions in analytic geometry, complex analysis and the theory of annuities. The first biography of De Moivre, on which almost all subsequent ones have since relied, was written in French by Matthew Maty. It was published in 1755 in the Journal britannique. The authors provide here, for the first time, a complete translation into English of Maty’s biography of De Moivre. New mate- rial, much of it taken from modern sources, is given in footnotes, along with numerous annotations designed to provide additional clarity to Maty’s biography for contemporary readers. INTRODUCTION ´emigr´es that both of them are known to have fre- Matthew Maty (1718–1776) was born of Huguenot quented. In the weeks prior to De Moivre’s death, parentage in the city of Utrecht, in Holland. He stud- Maty began to interview him in order to write his ied medicine and philosophy at the University of biography. De Moivre died shortly after giving his Leiden before immigrating to England in 1740. Af- reminiscences up to the late 1680s and Maty com- ter a decade in London, he edited for six years the pleted the task using only his own knowledge of the Journal britannique, a French-language publication man and De Moivre’s published work. -
The Meridian Arc Measurement in Peru 1735 – 1745
The Meridian Arc Measurement in Peru 1735 – 1745 Jim R. SMITH, United Kingdom Key words: Peru. Meridian. Arc. Triangulation. ABSTRACT: In the early 18th century the earth was recognised as having some ellipsoidal shape rather than a true sphere. Experts differed as to whether the ellipsoid was flattened at the Poles or the Equator. The French Academy of Sciences decided to settle the argument once and for all by sending one expedition to Lapland- as near to the Pole as possible; and another to Peru- as near to the Equator as possible. The result supported the view held by Newton in England rather than that of the Cassinis in Paris. CONTACT Jim R. Smith, Secretary to International Institution for History of Surveying & Measurement 24 Woodbury Ave, Petersfield Hants GU32 2EE UNITED KINGDOM Tel. & fax + 44 1730 262 619 E-mail: [email protected] Website: http://www.ddl.org/figtree/hsm/index.htm HS4 Surveying and Mapping the Americas – In the Andes of South America 1/12 Jim R. Smith The Meridian Arc Measurement in Peru 1735-1745 FIG XXII International Congress Washington, D.C. USA, April 19-26 2002 THE MERIDIAN ARC MEASUREMENT IN PERU 1735 – 1745 Jim R SMITH, United Kingdom 1. BACKGROUND The story might be said to begin just after the mid 17th century when Jean Richer was sent to Cayenne, S. America, to carry out a range of scientific experiments that included the determination of the length of a seconds pendulum. He returned to Paris convinced that in Cayenne the pendulum needed to be 11 lines (2.8 mm) shorter there than in Paris to keep the same time. -
Calculation and Controversy
calculation and controversy The young Newton owed his greatest intellectual debt to the French mathematician and natural philosopher, René Descartes. He was influ- enced by both English and Continental commentators on Descartes’ work. Problems derived from the writings of the Oxford mathematician, John Wallis, also featured strongly in Newton’s development as a mathe- matician capable of handling infinite series and the complexities of calcula- tions involving curved lines. The ‘Waste Book’ that Newton used for much of his mathematical working in the 1660s demonstrates how quickly his talents surpassed those of most of his contemporaries. Nevertheless, the evolution of Newton’s thought was only possible through consideration of what his immediate predecessors had already achieved. Once Newton had become a public figure, however, he became increasingly concerned to ensure proper recognition for his own ideas. In the quarrels that resulted with mathematicians like Gottfried Wilhelm Leibniz (1646–1716) or Johann Bernoulli (1667–1748), Newton supervised his disciples in the reconstruction of the historical record of his discoveries. One of those followers was William Jones, tutor to the future Earl of Macclesfield, who acquired or copied many letters and papers relating to Newton’s early career. These formed the heart of the Macclesfield Collection, which has recently been purchased by Cambridge University Library. 31 rené descartes, Geometria ed. and trans. frans van schooten 2 parts (Amsterdam, 1659–61) 4o: -2 4, a-3t4, g-3g4; π2, -2 4, a-f4 Trinity* * College, Cambridge,* shelfmark* nq 16/203 Newton acquired this book ‘a little before Christmas’ 1664, having read an earlier edition of Descartes’ Geometry by van Schooten earlier in the year. -
Graphical Evidence for the Solar Coronal Structure During the Maunder Minimum: Comparative Study of the Total Eclipse Drawings in 1706 and 1715
J. Space Weather Space Clim. 2021, 11,1 Ó H. Hayakawa et al., Published by EDP Sciences 2021 https://doi.org/10.1051/swsc/2020035 Available online at: www.swsc-journal.org Topical Issue - Space climate: The past and future of solar activity RESEARCH ARTICLE OPEN ACCESS Graphical evidence for the solar coronal structure during the Maunder minimum: comparative study of the total eclipse drawings in 1706 and 1715 Hisashi Hayakawa1,2,3,4,*, Mike Lockwood5,*, Matthew J. Owens5, Mitsuru Sôma6, Bruno P. Besser7, and Lidia van Driel – Gesztelyi8,9,10 1 Institute for Space-Earth Environmental Research, Nagoya University, 4648601 Nagoya, Japan 2 Institute for Advanced Researches, Nagoya University, 4648601 Nagoya, Japan 3 Science and Technology Facilities Council, RAL Space, Rutherford Appleton Laboratory, Harwell Campus, OX11 0QX Didcot, UK 4 Nishina Centre, Riken, 3510198 Wako, Japan 5 Department of Meteorology, University of Reading, RG6 6BB Reading, UK 6 National Astronomical Observatory of Japan, 1818588 Mitaka, Japan 7 Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria 8 Mullard Space Science Laboratory, University College London, RH5 6NT Dorking, UK 9 LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, 92195 Meudon, France 10 Konkoly Observatory, Hungarian Academy of Sciences, 1121 Budapest, Hungary Received 18 October 2019 / Accepted 29 June 2020 Abstract – We discuss the significant implications of three eye-witness drawings of the total solar eclipse on 1706 May 12 in comparison with two on 1715 May 3, for our understanding of space climate change. These events took place just after what has been termed the “deep Maunder Minimum” but fall within the “extended Maunder Minimum” being in an interval when the sunspot numbers start to recover. -
Alfonsi-Article Marine V5
1 Liliane ALFONSI Groupe d’Histoire et de Diffusion des Sciences d’Orsay (GHDSO ) Bât. 407. Université Paris Sud 11 91405 ORSAY Cédex [email protected] Un successeur de Bouguer : Étienne Bézout (1730–1783) commissaire et expert pour la marine Résumé : Entré à l’Académie Royale des Sciences dès 1758, Étienne Bézout, compte parmi ses tâches, l’obligation d’étudier différents ouvrages et outils présentés à l’Académie. Si dès le début il se voit confier l’étude d’instruments relatifs à la navigation, cela s’amplifiera à partir de 1764, date à laquelle Choiseul, ministre de la Marine, charge Bézout de réorganiser la formation des officiers de ce corps. Ses visites dans les ports pour faire passer les examens de la Marine, l‘amènent à appréhender concrètement les problèmes de la navigation. Cela lui vaudra d’être désigné pour juger la validité des critiques que l’hydrographe Blondeau énonce à l’encontre du traité de Pilotage de Bouguer. Par ailleurs cette situation amène Bézout à être membre de l’Académie de Marine de Brest et à être un des responsables de son association avec l’Académie des Sciences. Nous étudierons ces divers points. Enfin, Bézout écrit en 1769 un Traité de navigation que nous pourrons comparer à l’ouvrage de Bouguer sur le même sujet. Mots clés : Académie des Sciences, Marine, Académie de Marine, Traité de Navigation, Bézout, Bouguer. Abstract : Étienne Bézout, member of the Académie Royale des Sciences, have to study some works and books sended to this institution. In this article, we will look at his responsibility for Navy, before and after 1764, which is the year of Bézout’s nomination at the charge of Examinateur des Gardes du Pavillon et de la Marine. -
Newton As Philosopher
This page intentionally left blank NEWTON AS PHILOSOPHER Newton’s philosophical views are unique and uniquely difficult to categorize. In the course of a long career from the early 1670s until his death in 1727, he articulated profound responses to Cartesian natural philosophy and to the prevailing mechanical philosophy of his day. Newton as Philosopher presents Newton as an original and sophisti- cated contributor to natural philosophy, one who engaged with the principal ideas of his most important predecessor, René Descartes, and of his most influential critic, G. W. Leibniz. Unlike Descartes and Leibniz, Newton was systematic and philosophical without presenting a philosophical system, but, over the course of his life, he developed a novel picture of nature, our place within it, and its relation to the creator. This rich treatment of his philosophical ideas, the first in English for thirty years, will be of wide interest to historians of philosophy, science, and ideas. ANDREW JANIAK is Assistant Professor in the Department of Philosophy, Duke University. He is editor of Newton: Philosophical Writings (2004). NEWTON AS PHILOSOPHER ANDREW JANIAK Duke University CAMBRIDGE UNIVERSITY PRESS Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore, São Paulo Cambridge University Press The Edinburgh Building, Cambridge CB2 8RU, UK Published in the United States of America by Cambridge University Press, New York www.cambridge.org Information on this title: www.cambridge.org/9780521862868 © Andrew Janiak 2008 This publication is in copyright. Subject to statutory exception and to the provision of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. -
Newton on the Beach: the Information Order of Principia Mathematica
Hist. Sci., xlvii (2009) NEWTON ON THE BEACH: THE INFORMATION ORDER OF PRINCIPIA MATHEMATICA Simon Schaffer Cambridge University WHAT I MAY SEEM TO THE WORLD I know not what I may seem to the world, but as to myself, I seem to have been only like a boy playing on the sea-shore and diverting myself in now and then finding a smoother pebble or a prettier shell than ordinary, whilst the great ocean of truth lay all undiscovered before me.1 It is one of the most celebrated of Isaac Newton’s obiter dicta. Like many such, its provenance is hazy. The literary reference may well be to a passage from John Milton’s great redemptive poem Paradise regained (1671) where, in dialogue with Satan, Christ praises divine illumination above pagan learning: “who reads / Inces- santly, and to his reading brings not / A spirit and judgment equal or superior, / … Uncertain and unsettled still remains, / Deep verst in books, and shallow in himself, / Crude or intoxicate, collecting toys / And trifles for choice matters, worth a spunge, / As children gath’ring pebbles on the shore”.2 But the remark’s immediate relation with Newton is more ambiguous. The earliest version is found in a conversation of April 1730, three years after Newton’s death, between the gossipy man of letters Joseph Spence and the Jacobite, freemason and court tutor Andrew Ramsay. While chatting about Newton’s debt to ancient theology and his strange attitudes towards the doctrine of the Trinity, Ramsay quoted Newton’s phrase, adding it was “as great as all” of Principia mathematica.3 Never one to let a nice epigram slip, Ramsay then incorporated the expression in his 1732 Plan of education for a young prince, composed to help tutor the heirs of a noble French clan. -
The Important Role of the Two French Astronomers J.-N. Delisle and J.-J. Lalande in the Choice of Observing Places During the Transits of Venus in 1761 and 1769
MEETING VENUS C. Sterken, P. P. Aspaas (Eds.) The Journal of Astronomical Data 19, 1, 2013 The Important Role of the Two French Astronomers J.-N. Delisle and J.-J. Lalande in the Choice of Observing Places during the Transits of Venus in 1761 and 1769 Simone Dumont1 and Monique Gros2 1Observatoire de Paris, 61 Avenue de l’Observatoire, 75014, Paris, France 2Observatoire de Paris, Institut d’Astrophysique de Paris – Universit´e Pierre et Marie Curie, 98 bis Boulevard Arago, 75014, Paris, France Abstract. Joseph-Nicolas Delisle, as a member of the Acad´emie Royale des Sci- ences of Paris and professor at the Coll`ege Royal de France, went to England in 1724 to visit Newton and Halley. The latter suggested observations of the transits of Mercury and of Venus in order to obtain the solar parallax. Delisle was also in- terested in the Mercury transits. After a stay of 22 years in Saint Petersburg, on his return to Paris, he distributed avertissements (information bulletins) encouraging all astronomers to observe the same phenomena, like the solar eclipse of 1748. Later, in 1760, Delisle presented an Adresse to the King and to the Acad´emie in which he detailed his method to observe the 1761 transit of Venus. This was accompanied by a mappemonde showing the best places for observations. Copies of the text, together with 200 maps, were sent to his numerous correspondents in France and abroad. Following the advanced age and finally death of Delisle, his assistant and successor Joseph-J´erˆome Lalande presented a m´emoire related to the 1769 transit of Venus and an improved map of the best observing places. -
The Napoleon Series
The Napoleon Series Maps and Mapmakers of the Napoleonic Wars Part II: French Mapmakers – the Cassinis and Maraldis By: Richard Tennant The Cassini Dynasty Giovanni Domenico Cassini (8 June 1625 – 14 September 1712)1 He was an Italian mathematician, astronomer, astrologer and engineer. Cassini was born in Perinaldo, near Imperia, at that time in the County of Nice, part of the Duchy of Savoy. Cassini is known for his work in the fields of astronomy and engineering. Cassini discovered four satellites of the planet Saturn and noted the division of the rings of Saturn; the Cassini Division was named after him. In 1669 Cassini moved to France and through a grant from Louis XIV of France helped to set up the Paris Observatory, which opened in 1671; Cassini would remain the director of the observatory for the rest of his career until his death in 1712. For the remaining forty-one years of his life Cassini served as astronomer/astrologer to Louis XIV ("The Sun King"); serving the expected dual role yet focusing the overwhelming majority of his time on astronomy rather than the astrology he had studied so much in his youth. During this time, Cassini's method of determining longitude was used to measure the size of France accurately for the first time. The country turned out to be considerably smaller than expected, and the king quipped that Cassini had taken more of his kingdom from him than he had won in all his wars. Cassini had two sons; the younger, Jacques Cassini, succeeded him as astronomer and geodesist under the name of Cassini II.