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The Swinging Spring: Regular and Chaotic Motion
References The Swinging Spring: Regular and Chaotic Motion Leah Ganis May 30th, 2013 Leah Ganis The Swinging Spring: Regular and Chaotic Motion References Outline of Talk I Introduction to Problem I The Basics: Hamiltonian, Equations of Motion, Fixed Points, Stability I Linear Modes I The Progressing Ellipse and Other Regular Motions I Chaotic Motion I References Leah Ganis The Swinging Spring: Regular and Chaotic Motion References Introduction The swinging spring, or elastic pendulum, is a simple mechanical system in which many different types of motion can occur. The system is comprised of a heavy mass, attached to an essentially massless spring which does not deform. The system moves under the force of gravity and in accordance with Hooke's Law. z y r φ x k m Leah Ganis The Swinging Spring: Regular and Chaotic Motion References The Basics We can write down the equations of motion by finding the Lagrangian of the system and using the Euler-Lagrange equations. The Lagrangian, L is given by L = T − V where T is the kinetic energy of the system and V is the potential energy. Leah Ganis The Swinging Spring: Regular and Chaotic Motion References The Basics In Cartesian coordinates, the kinetic energy is given by the following: 1 T = m(_x2 +y _ 2 +z _2) 2 and the potential is given by the sum of gravitational potential and the spring potential: 1 V = mgz + k(r − l )2 2 0 where m is the mass, g is the gravitational constant, k the spring constant, r the stretched length of the spring (px2 + y 2 + z2), and l0 the unstretched length of the spring. -
Dynamics of the Elastic Pendulum Qisong Xiao; Shenghao Xia ; Corey Zammit; Nirantha Balagopal; Zijun Li Agenda
Dynamics of the Elastic Pendulum Qisong Xiao; Shenghao Xia ; Corey Zammit; Nirantha Balagopal; Zijun Li Agenda • Introduction to the elastic pendulum problem • Derivations of the equations of motion • Real-life examples of an elastic pendulum • Trivial cases & equilibrium states • MATLAB models The Elastic Problem (Simple Harmonic Motion) 푑2푥 푑2푥 푘 • 퐹 = 푚 = −푘푥 = − 푥 푛푒푡 푑푡2 푑푡2 푚 • Solve this differential equation to find 푥 푡 = 푐1 cos 휔푡 + 푐2 sin 휔푡 = 퐴푐표푠(휔푡 − 휑) • With velocity and acceleration 푣 푡 = −퐴휔 sin 휔푡 + 휑 푎 푡 = −퐴휔2cos(휔푡 + 휑) • Total energy of the system 퐸 = 퐾 푡 + 푈 푡 1 1 1 = 푚푣푡2 + 푘푥2 = 푘퐴2 2 2 2 The Pendulum Problem (with some assumptions) • With position vector of point mass 푥 = 푙 푠푖푛휃푖 − 푐표푠휃푗 , define 푟 such that 푥 = 푙푟 and 휃 = 푐표푠휃푖 + 푠푖푛휃푗 • Find the first and second derivatives of the position vector: 푑푥 푑휃 = 푙 휃 푑푡 푑푡 2 푑2푥 푑2휃 푑휃 = 푙 휃 − 푙 푟 푑푡2 푑푡2 푑푡 • From Newton’s Law, (neglecting frictional force) 푑2푥 푚 = 퐹 + 퐹 푑푡2 푔 푡 The Pendulum Problem (with some assumptions) Defining force of gravity as 퐹푔 = −푚푔푗 = 푚푔푐표푠휃푟 − 푚푔푠푖푛휃휃 and tension of the string as 퐹푡 = −푇푟 : 2 푑휃 −푚푙 = 푚푔푐표푠휃 − 푇 푑푡 푑2휃 푚푙 = −푚푔푠푖푛휃 푑푡2 Define 휔0 = 푔/푙 to find the solution: 푑2휃 푔 = − 푠푖푛휃 = −휔2푠푖푛휃 푑푡2 푙 0 Derivation of Equations of Motion • m = pendulum mass • mspring = spring mass • l = unstreatched spring length • k = spring constant • g = acceleration due to gravity • Ft = pre-tension of spring 푚푔−퐹 • r = static spring stretch, 푟 = 푡 s 푠 푘 • rd = dynamic spring stretch • r = total spring stretch 푟푠 + 푟푑 Derivation of Equations of Motion -
Vicious Circle”: Unscrambling A.-C
CORE Metadata, citation and similar papers at core.ac.uk Provided by Elsevier - Publisher Connector HISTORIA MATHEMATICA 15 t 19881, 228-239 Breaking a “Vicious Circle”: Unscrambling A.-C. Clairaut’s Iterative Method of 1743 JOHN L. GREENBERG Centre de Recherches Alexar~dre KoyrC, 12. rue Colherf. 75.002 Puris. FI.N~C.C In this paper 1 show how in 1743 A.-C. Clairaut applied an iterative method to calculate the ellipticity of an infinitesimally flattened, homogeneous ellipsoid of revolution in equilib- rium, taken to represent the earth. Clairaut did not make very clear what he was doing and, as a result, left certain readers in the dark. They could not understand the point of the calculation and erroneously thought that Clairaut was going around in circles. The paper ends with a discussion of Clairaut’s clarification of the calculation, published in 1760 in response to the criticisms of John Muller, and a brief comparison of Clairaut’s iterative method with the “Newton-Raphson Method.” 1 1988.4cademlc Pres\. Inc. Dans cet article je montre la methode d’approximation d’A.-C. Clairaut pour trouver I’ellipticite d’un ellipsoi’de homogene de revolution en equilibre dont l’ellipticitt est infinite- simale et qui reprtsente la terre. Certains lecteurs ont mal compris Clairaut. Ceux-ci ont cru Clairaut pris au piege dans un “cercle vicieux en logique.” Clairaut a repondu a son critique John Muller en 1760, et j’explique cette reponse. Mon article se termine par une breve comparaison de la methode de Clairaut et de celle dite “Newton-Raphson.” Cette com- paraison peut eclairer la cause du malentendu. -
Geodesy Methods Over Time
Geodesy methods over time GISC3325 - Lecture 4 Astronomic Latitude/Longitude • Given knowledge of the positions of an astronomic body e.g. Sun or Polaris and our time we can determine our location in terms of astronomic latitude and longitude. US Meridian Triangulation This map shows the first project undertaken by the founding Superintendent of the Survey of the Coast Ferdinand Hassler. Triangulation • Method of indirect measurement. • Angles measured at all nodes. • Scaled provided by one or more precisely measured base lines. • First attributed to Gemma Frisius in the 16th century in the Netherlands. Early surveying instruments Left is a Quadrant for angle measurements, below is how baseline lengths were measured. A non-spherical Earth • Willebrod Snell van Royen (Snellius) did the first triangulation project for the purpose of determining the radius of the earth from measurement of a meridian arc. • Snellius was also credited with the law of refraction and incidence in optics. • He also devised the solution of the resection problem. At point P observations are made to known points A, B and C. We solve for P. Jean Picard’s Meridian Arc • Measured meridian arc through Paris between Malvoisine and Amiens using triangulation network. • First to use a telescope with cross hairs as part of the quadrant. • Value obtained used by Newton to verify his law of gravitation. Ellipsoid Earth Model • On an expedition J.D. Cassini discovered that a one-second pendulum regulated at Paris needed to be shortened to regain a one-second oscillation. • Pendulum measurements are effected by gravity! Newton • Newton used measurements of Picard and Halley and the laws of gravitation to postulate a rotational ellipsoid as the equilibrium figure for a homogeneous, fluid, rotating Earth. -
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. -
Measuring the Universe: a Brief History of Time
Measuring the Universe A Brief History of Time & Distance from Summer Solstice to the Big Bang Michael W. Masters Outline • Seasons and Calendars • Greece Invents Astronomy Part I • Navigation and Timekeeping • Measuring the Solar System Part II • The Expanding Universe Nov 2010 Measuring the Universe 2 Origins of Astronomy • Astronomy is the oldest natural science – Early cultures identified celestial events with spirits • Over time, humans began to correlate events in the sky with phenomena on earth – Phases of the Moon and cycles of the Sun & stars • Stone Age cave paintings show Moon phases! – Related sky events to weather patterns, seasons and tides • Neolithic humans began to grow crops (8000-5500 BC) – Agriculture made timing the seasons vital – Artifacts were built to fix the dates of the Vernal Equinox and the Summer Solstice A 16,500 year old night • Astronomy’s originators sky map has been found include early Chinese, on the walls of the famous Lascaux painted Babylonians, Greeks, caves in central France. Egyptians, Indians, and The map shows three bright stars known today Mesoamericans as the Summer Triangle. Source: http://ephemeris.com/history/prehistoric.html Nov 2010 Measuring the Universe 3 Astronomy in Early History • Sky surveys were developed as long ago as 3000 BC – The Chinese & Babylonians and the Greek astronomer, Meton of Athens (632 BC), discovered that eclipses follow an 18.61-year cycle, now known as the Metonic cycle – First known written star catalog was developed by Gan De in China in 4 th Century BC – Chinese -
Pioneers in Optics: Christiaan Huygens
Downloaded from Microscopy Pioneers https://www.cambridge.org/core Pioneers in Optics: Christiaan Huygens Eric Clark From the website Molecular Expressions created by the late Michael Davidson and now maintained by Eric Clark, National Magnetic Field Laboratory, Florida State University, Tallahassee, FL 32306 . IP address: [email protected] 170.106.33.22 Christiaan Huygens reliability and accuracy. The first watch using this principle (1629–1695) was finished in 1675, whereupon it was promptly presented , on Christiaan Huygens was a to his sponsor, King Louis XIV. 29 Sep 2021 at 16:11:10 brilliant Dutch mathematician, In 1681, Huygens returned to Holland where he began physicist, and astronomer who lived to construct optical lenses with extremely large focal lengths, during the seventeenth century, a which were eventually presented to the Royal Society of period sometimes referred to as the London, where they remain today. Continuing along this line Scientific Revolution. Huygens, a of work, Huygens perfected his skills in lens grinding and highly gifted theoretical and experi- subsequently invented the achromatic eyepiece that bears his , subject to the Cambridge Core terms of use, available at mental scientist, is best known name and is still in widespread use today. for his work on the theories of Huygens left Holland in 1689, and ventured to London centrifugal force, the wave theory of where he became acquainted with Sir Isaac Newton and began light, and the pendulum clock. to study Newton’s theories on classical physics. Although it At an early age, Huygens began seems Huygens was duly impressed with Newton’s work, he work in advanced mathematics was still very skeptical about any theory that did not explain by attempting to disprove several theories established by gravitation by mechanical means. -
Redalyc.The International Pendulum Project
Revista Electrónica de Investigación en Educación en Ciencias E-ISSN: 1850-6666 [email protected] Universidad Nacional del Centro de la Provincia de Buenos Aires Argentina Matthews, Michael R. The International Pendulum Project Revista Electrónica de Investigación en Educación en Ciencias, vol. 1, núm. 1, octubre, 2006, pp. 1-5 Universidad Nacional del Centro de la Provincia de Buenos Aires Buenos Aires, Argentina Available in: http://www.redalyc.org/articulo.oa?id=273320433002 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative Año 1 – Número 1 – Octubre de 2006 ISSN: en trámite The International Pendulum Project Michael R. Matthews [email protected] School of Education, University of New South Wales, Sydney 2052, Australia The Pendulum in Modern Science Galileo in his final great work, The Two New Sciences , written during the period of house arrest after the trial that, for many, marked the beginning of the Modern Age, wrote: We come now to the other questions, relating to pendulums, a subject which may appear to many exceedingly arid, especially to those philosophers who are continually occupied with the more profound questions of nature. Nevertheless, the problem is one which I do not scorn. I am encouraged by the example of Aristotle whom I admire especially because he did not fail to discuss every subject which he thought in any degree worthy of consideration. (Galileo 1638/1954, pp.94-95) This was the pendulum’s low-key introduction to the stage of modern science and modern society. -
A Phenomenology of Galileo's Experiments with Pendulums
BJHS, Page 1 of 35. f British Society for the History of Science 2009 doi:10.1017/S0007087409990033 A phenomenology of Galileo’s experiments with pendulums PAOLO PALMIERI* Abstract. The paper reports new findings about Galileo’s experiments with pendulums and discusses their significance in the context of Galileo’s writings. The methodology is based on a phenomenological approach to Galileo’s experiments, supported by computer modelling and close analysis of extant textual evidence. This methodology has allowed the author to shed light on some puzzles that Galileo’s experiments have created for scholars. The pendulum was crucial throughout Galileo’s career. Its properties, with which he was fascinated from very early in his career, especially concern time. A 1602 letter is the earliest surviving document in which Galileo discusses the hypothesis of pendulum isochronism.1 In this letter Galileo claims that all pendulums are isochronous, and that he has long been trying to demonstrate isochronism mechanically, but that so far he has been unable to succeed. From 1602 onwards Galileo referred to pendulum isochronism as an admirable property but failed to demonstrate it. The pendulum is the most open-ended of Galileo’s artefacts. After working on my reconstructed pendulums for some time, I became convinced that the pendulum had the potential to allow Galileo to break new ground. But I also realized that its elusive nature sometimes threatened to undermine the progress Galileo was making on other fronts. It is this ambivalent nature that, I thought, might prove invaluable in trying to understand crucial aspects of Galileo’s innovative methodology. -
Sarlette Et Al
COMPARISON OF THE HUYGENS MISSION AND THE SM2 TEST FLIGHT FOR HUYGENS ATTITUDE RECONSTRUCTION(*) A. Sarlette(1), M. Pérez-Ayúcar, O. Witasse, J.-P. Lebreton Planetary Missions Division, Research and Scientific Support Department, ESTEC-ESA, Noordwijk, The Netherlands. Email: [email protected], [email protected], [email protected] (1) Stagiaire from February 1 to April 29; student at Liège University, Belgium. Email: [email protected] ABSTRACT 1. The SM2 probe characteristics The Huygens probe is the ESA’s main contribution to In agreement with its main purpose – performing a the Cassini/Huygens mission, carried out jointly by full system check of the Huygens descent sequence – NASA, ESA and ASI. It was designed to descend into the SM2 probe was a full scale model of the Huygens the atmosphere of Titan on January 14, 2005, probe, having the same inner and outer structure providing surface images and scientific data to study (except that the deploying booms of the HASI the ground and the atmosphere of Saturn’s largest instrument were not mounted on SM2), the same mass moon. and a similar balance. A complete description of the Huygens flight model system can be found in [1]. In the framework of the reconstruction of the probe’s motions during the descent based on the engineering All Descent Control SubSystem items (parachute data, additional information was needed to investigate system, mechanisms, pyro and command devices) were the attitude and an anomaly in the spin direction. provided according to expected flight standard; as the test flight was successful, only few differences actually Two years before the launch of the Cassini/Huygens exist at this level with respect to the Huygens probe. -
ALBERT VAN HELDEN + HUYGENS’S RING CASSINI’S DIVISION O & O SATURN’S CHILDREN
_ ALBERT VAN HELDEN + HUYGENS’S RING CASSINI’S DIVISION o & o SATURN’S CHILDREN )0g-_ DIBNER LIBRARY LECTURE , HUYGENS’S RING, CASSINI’S DIVISION & SATURN’S CHILDREN c !@ _+++++++++ l ++++++++++ _) _) _) _) _)HUYGENS’S RING, _)CASSINI’S DIVISION _) _)& _)SATURN’S CHILDREN _) _) _)DDDDD _) _) _)Albert van Helden _) _) _) , _) _) _)_ _) _) _) _) _) · _) _) _) ; {(((((((((QW(((((((((} , 20013–7012 Text Copyright ©2006 Albert van Helden. All rights reserved. A H is Professor Emeritus at Rice University and the Univer- HUYGENS’S RING, CASSINI’S DIVISION sity of Utrecht, Netherlands, where he resides and teaches on a regular basis. He received his B.S and M.S. from Stevens Institute of Technology, M.A. from the AND SATURN’S CHILDREN University of Michigan and Ph.D. from Imperial College, University of London. Van Helden is a renowned author who has published respected books and arti- cles about the history of science, including the translation of Galileo’s “Sidereus Nuncius” into English. He has numerous periodical contributions to his credit and has served on the editorial boards of Air and Space, 1990-present; Journal for the History of Astronomy, 1988-present; Isis, 1989–1994; and Tractrix, 1989–1995. During his tenure at Rice University (1970–2001), van Helden was instrumental in establishing the “Galileo Project,”a Web-based source of information on the life and work of Galileo Galilei and the science of his time. A native of the Netherlands, Professor van Helden returned to his homeland in 2001 to join the faculty of Utrecht University. -
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.