The Rectification of Quadratures As a Central Foundational Problem for The
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Chapter 1 Geometry of Plane Curves
Chapter 1 Geometry of Plane Curves Definition 1 A (parametrized) curve in Rn is a piece-wise differentiable func- tion α :(a, b) Rn. If I is any other subset of R, α : I Rn is a curve provided that α→extends to a piece-wise differentiable function→ on some open interval (a, b) I. The trace of a curve α is the set of points α ((a, b)) Rn. ⊃ ⊂ AsubsetS Rn is parametrized by α if and only if there exists set I R ⊂ ⊆ such that α : I Rn is a curve for which α (I)=S. A one-to-one parame- trization α assigns→ and orientation toacurveC thought of as the direction of increasing parameter, i.e., if s<t,the direction of increasing parameter runs from α (s) to α (t) . AsubsetS Rn may be parametrized in many ways. ⊂ Example 2 Consider the circle C : x2 + y2 =1and let ω>0. The curve 2π α : 0, R2 given by ω → ¡ ¤ α(t)=(cosωt, sin ωt) . is a parametrization of C for each choice of ω R. Recall that the velocity and acceleration are respectively given by ∈ α0 (t)=( ω sin ωt, ω cos ωt) − and α00 (t)= ω2 cos 2πωt, ω2 sin 2πωt = ω2α(t). − − − The speed is given by ¡ ¢ 2 2 v(t)= α0(t) = ( ω sin ωt) +(ω cos ωt) = ω. (1.1) k k − q 1 2 CHAPTER 1. GEOMETRY OF PLANE CURVES The various parametrizations obtained by varying ω change the velocity, ac- 2π celeration and speed but have the same trace, i.e., α 0, ω = C for each ω. -
Happy New Year! MEMBERSHIP? IT’S NEVER TOO LATE to JOIN!
Vol. 42, No. 1 January 2011 Great Work at Sleaford Renovations to the Sleaford Observatory warm-up shelter progressed rapidly last fall with Rick Huziak and Darrell Chatfield spending many days and evenings there. A wall was removed to the cold storage area to make more room, which meant extensive rewiring, insulating and refinishing. Other volunteers came to cut grass, paint, clean, do repairs, and provide food. Thank you to every one who helped to make Sleaford a more usable and pleasant site. Photo by Jeff Swick In This Issue: Membership Information / Bottle Drive / Officers of the Centre 2 U of S Observatory Hours / Light Pollution Abatement Website 2 Calendar of Events / Meeting Announcement 3 Solstice Eclipse – Tenho Tuomi, Norma Jensen plus others 4 ‘Tis the Night Before… 5 President’s Message – Jeff Swick 5 GOTO Telescopes are not for Beginners – Tenho Tuomi 6 Ask AstroNut 7 Saskatoon Centre Observers Group Notes – Larry Scott, Jeff Swick 8 The Royal Astronomical Society of Canada The Planets This Month – Murray Paulson 9 P.O. Box 317, RPO University The Messier, H-400 & H-400-II, FNGC, Bino, Lunar & EtU Club 10 Saskatoon, SK S7N 4J8 Editor’s Corner – Tenho Tuomi 10 WEBSITE: http://www.rasc.ca/saskatoon To view Saskatoon Skies in colour, see our Website: E •MAIL: [email protected] http://homepage.usask.ca/~ges125/rasc/newsletters.html TELEPHONE: (306) 373-3902 Happy New Year! MEMBERSHIP? IT’S NEVER TOO LATE TO JOIN! Regular: $80.00 /year Youth: $41.00 /year Associate: $33 /year The Saskatoon Centre operates on a one-year revolving membership. -
Tangent Lines
The Kabod Volume 5 Issue 1 Fall 2018 Article 1 September 2018 Tangent Lines Samuel Estep Liberty University, [email protected] Follow this and additional works at: https://digitalcommons.liberty.edu/kabod Part of the Mathematics Commons Recommended Citations MLA: Estep, Samuel "Tangent Lines," The Kabod 5. 1 (2018) Article 1. Liberty University Digital Commons. Web. [xx Month xxxx]. APA: Estep, Samuel (2018) "Tangent Lines" The Kabod 5( 1 (2018)), Article 1. Retrieved from https://digitalcommons.liberty.edu/kabod/vol5/iss1/1 Turabian: Estep, Samuel "Tangent Lines" The Kabod 5 , no. 1 2018 (2018) Accessed [Month x, xxxx]. Liberty University Digital Commons. This Individual Article is brought to you for free and open access by Scholars Crossing. It has been accepted for inclusion in The Kabod by an authorized editor of Scholars Crossing. For more information, please contact [email protected]. Estep: Tangent Lines Tangent Lines Sam Estep 2018-05-06 In [1] Leibniz published the first treatment of the subject of calculus. An English translation can be found in [2]; he says that to find a tangent is to draw a right line, which joins two points of the curve having an infinitely small difference, or the side of an infinite angled polygon produced, which is equivalent to the curve for us. Today, according to [3], a straight line is said to be a tangent line of a curve y = f(x) at a point x = c on the curve if the line passes through the point (c; f(c)) on the curve and has slope f 0(c) where f 0 is the derivative of f. -
Culpeper Astronomy Club Meeting February 26, 2018 Overview
The Moon: Our Neighbor Culpeper Astronomy Club Meeting February 26, 2018 Overview • Introductions • Radio Astronomy: The Basics • The Moon • Constellations: Monoceros, Canis Major, Puppis • Observing Session (Tentative) Radio Astronomy • Stars, galaxies and gas clouds emit visible light as well as emissions from other parts of the electromagnetic spectrum • Includes radio waves, gamma rays, X- rays, and infrared radiation • Radio astronomy is the study of the universe through analysis of celestial objects' radio emission • the longest-wavelength, least energetic form of radiation on the electromagnetic spectrum • The first detection of radio waves from an astronomical object was in 1932 • Karl Jansky at Bell Telephone Laboratories observed radiation coming from the Milky Way Radio Astronomy • A radio telescope has three basic components: • One or more antennas pointed to the sky, to collect the radio waves • A receiver and amplifier to boost the very weak radio signal to a measurable level, and • A recorder to keep a record of the signal Radio Astronomy • Subsequent observations have identified a number of different sources of radio emission • Include stars and galaxies, as well as entirely new classes of objects, such as: • Radio galaxies: nuclei emit jets of high- velocity gas (near the speed of light) above and below the galaxy -- the jets interact with magnetic fields and emit radio signals • Quasars: distant objects powered by black holes a billion times as massive as our sun • Pulsars: the rapidly spinning remnants of supernova explosions -
Det.,Class.,Lunar Rilles 1
UNIVERSITÀ DEGLI STUDI DI PERUGIA DIPARTIMENTO DI FISICA E GEOLOGIA Corso di Laurea Magistrale in Scienze e Tecnologie Geologiche TESI DI LAUREA DETECTION, CLASSIFICATION, AND ANALYSIS OF SINUOUS RILLES ON THE NEAR-SIDE OF THE MOON Laureando: Relatore: SOFIA FIORUCCI LAURA MELELLI Correlatore: MARIA TERESA BRUNETTI Anno Accademico 2019/2020 “I have not failed. I've just found 10,000 ways that won't work.” ― Thomas A. Edison Table of Contents 1 Chapter 1: Introduction .................................................................................. 1 1.1 The Moon Mapping Project ..................................................................................... 1 1.2 Chang’E missions ...................................................................................................... 4 1.3 Moon Mapping Topics ............................................................................................. 9 1.3.1 Topic 1 –Map of the solar wind .............................................................................................. 10 1.3.2 Topic 2 – Geomorphologic map of the Moon ....................................................................... 11 1.3.3 Topic 3 – Data processing of Chang’E-1 mission ................................................................. 13 1.3.4 Topic 4 –Map of element distribution ................................................................................... 14 1.3.5 Topic 5 – 3D Visualization system ......................................................................................... 14 -
What's Hot on the Moon Tonight?: the Ultimate Guide to Lunar Observing
What’s Hot on the Moon Tonight: The Ultimate Guide to Lunar Observing Copyright © 2015 Andrew Planck All rights reserved. No part of this book may be reproduced in any written, electronic, recording, or photocopying without written permission of the publisher or author. The exception would be in the case of brief quotations embodied in the critical articles or reviews and pages where permission is specifically granted by the publisher or author. Although every precaution has been taken to verify the accuracy of the information contained herein, the publisher and author assume no responsibility for any errors or omissions. No liability is assumed for damages that may result from the use of information contained within. Books may be purchased by contacting the publisher or author through the website below: AndrewPlanck.com Cover and Interior Design: Nick Zelinger (NZ Graphics) Publisher: MoonScape Publishing, LLC Editor: John Maling (Editing By John) Manuscript Consultant: Judith Briles (The Book Shepherd) ISBN: 978-0-9908769-0-8 Library of Congress Catalog Number: 2014918951 1) Science 2) Astronomy 3) Moon Dedicated to my wife, Susan and to my two daughters, Sarah and Stefanie Contents Foreword Acknowledgments How to Use this Guide Map of Major Seas Nightly Guide to Lunar Features DAYS 1 & 2 (T=79°-68° E) DAY 3 (T=59° E) Day 4 (T=45° E) Day 5 (T=24° E.) Day 6 (T=10° E) Day 7 (T=0°) Day 8 (T=12° W) Day 9 (T=21° W) Day 10 (T= 28° W) Day 11 (T=39° W) Day 12 (T=54° W) Day 13 (T=67° W) Day 14 (T=81° W) Day 15 and beyond Day 16 (T=72°) Day 17 (T=60°) FINAL THOUGHTS GLOSSARY Appendix A: Historical Notes Appendix B: Pronunciation Guide About the Author Foreword Andrew Planck first came to my attention when he submitted to Lunar Photo of the Day an image of the lunar crater Pitatus and a photo of a pie he had made. -
Sources and Studies in the History of Mathematics and Physical Sciences
Sources and Studies in the History of Mathematics and Physical Sciences Editorial Board J.Z. Buchwald J. Lützen G.J. Toomer Advisory Board P.J. Davis T. Hawkins A.E. Shapiro D. Whiteside Springer Science+Business Media, LLC Sources and Studies in the History of Mathematics and Physical Seiences K. Andersen Brook Taylor's Work on Linear Perspective H.l.M. Bos Redefining Geometrical Exactness: Descartes' Transformation of the Early Modern Concept of Construction 1. Cannon/S. Dostrovsky The Evolution of Dynamics: Vibration Theory from 1687 to 1742 B. ChandIerlW. Magnus The History of Combinatorial Group Theory A.I. Dale AHistory of Inverse Probability: From Thomas Bayes to Karl Pearson, Second Edition A.I. Dale Most Honourable Remembrance: The Life and Work of Thomas Bayes A.I. Dale Pierre-Simon Laplace, Philosophical Essay on Probabilities, Translated from the fifth French edition of 1825, with Notes by the Translator P. Damerow/G. FreudenthallP. McLaugWin/l. Renn Exploring the Limits of Preclassical Mechanics: A Study of Conceptual Development in Early Modem Science: Free Fall and Compounded Motion in the Work of Descartes, Galileo, and Beeckman, Second Edition P.l. Federico Descartes on Polyhedra: A Study of the De Solworum Elementis B.R. Goldstein The Astronomy of Levi ben Gerson (1288-1344) H.H. Goldstine A History of Numerical Analysis from the 16th Through the 19th Century H.H. Goldstine A History of the Calculus of Variations from the 17th Through the 19th Century G. Graßhoff The History of Ptolemy's Star Catalogue A.W. Grootendorst Jan de Witt's Eiementa Curvarum Linearum, über Primus Continued after Index The Arithmetic of Infinitesimals John Wallis 1656 Translated from Latin to English with an Introduction by Jacqueline A. -
Build Your Own Model Planet
E WILL R YO E U H R W C ? U U R O I O Y S E I T K Y A T SCIENCE@HOME You may have seen photos of Earth from space where it looks like it is You will need: round, like a blue marble as it is A stick described by astronauts. (provided) Some card Planet Earth is not, in fact, perfectly (provided) round! Instead it is an oblate spheroid — Glue a sphere that is squashed at its poles (provided) (top and bottom) and swollen at the Access to scissors (if you do not have scissors at equator (middle). home ask if you can use some at school or at your We are going to look at why... local library). The bigger the planet, the bigger the squashed effect. Planets are shaped this way because they spin, and this experiment will show you how. We are going to build a model planet! A B 1 Cut out the three discs from the card, the larger two are A and B. The smaller one is C. C 2 Cut the central holes in discs A and C so they are a tight fit on the stick (so they do not move). Cut the larger hole into B so that it can slide up and down the stick easily. 3 Now cut out the strips of card. Glue one end of each strip around the edge of disc A then put it on the stick. 4 Next fix C halfway up the stick as a reference point. -
January 2018
The StarGazer http://www.raclub.org/ Newsletter of the Rappahannock Astronomy Club No. 3, Vol. 6 November 2017–January 2018 Field Trip to Randolph-Macon College Keeble Observatory By Jerry Hubbell and Linda Billard On December 2, Matt Scott, Jean Benson, Bart and Linda Billard, Jerry Hubbell, and Peter Orlowski joined Scott Lansdale to tour the new Keeble Observatory at his alma mater, Randolph-Macon College in Ashland, VA. The Observatory is a cornerstone instrument in the College's academic minor program in astrophysics and is also used for student and faculty research projects. At the kind invitation of Physics Professor George Spagna— Scott’s advisor during his college days and now the director of the new facility—we received a private group tour. We stayed until after dark to see some of its capabilities. Keeble Observatory at Randolph-Macon College Credit: Jerry Hubbell The observatory, constructed in summer 2017, is connected to the northeast corner of the Copley Science Center on campus. It houses a state-of-the-art $30,000 Astro Systeme Austria (ASA) Ritchey-Chretien telescope with a 16-inch (40-cm) primary mirror. Instrumentation will eventually include CCD cameras for astrophotography and scientific imaging, and automation for the 12-foot (3.6-m) dome. The mount is a $50,000 ASA DDM 160 Direct Drive system placed on an interesting offset pier system that allows the mount to track well past the meridian without having to do the pier-flip that standard German equatorial mounts (GEMs) perform when approaching the meridian. All told, the fully outfitted observatory will be equipped with about $100,000 of instrumentation and equipment. -
ED164303.Pdf
DOCUMENT RESUME -.. a ED 164.303 E 025. 458 AUTHOR Beck, A.; And Others ,TITLE Calculus, Part 3,'Studentl'Text, Unit No. 70. Revised Edition. , INSTITUTION Stanford Univ.,'CaliY. School Mathematics Study 't.-Group. SPONS AGENCY -National Science Foundation, Washington, D.C. PUB DATE ,65: NOTE 36bp.; For related documents, see SE 025 456-4:59; Contains light and braken'type EDRS PRICE MF-$0.83 HC-$19.41 Plus Postage. DESCRIPTORS *Calculus; *Cuiriculum; *Instructional Materials; *Mathematical Applications; Mathematics .Educatioi; S4Condary Education; *Secondary School Mathematics; *Textbooks IDENTIFIERS *School Mathematics Study Group ABSTRACT. This is part three of a'three-part SMSG calculuS text for high sahool students. One of the goals of the text is to present -calculus as a mathematical discipline -as yell, as presenting its practical uses. The authbrs emphasize the importance of being able to ipterpret the conceptS and theory interms of models to which they .apply. The text demonstrates the origins of the ideas of the calculus in pradtical problems; attempts to express these ideas precisely and_ ` develop them logically; and finally, returns to the problems and applies the theorems resulting from that development. Chapter topics include: (1)vectors and curves; (2) mechanics; (3) numerical analysis; (4) sequences and series; and (5) geometricl optics and waves. (MP) 1 - ********************************45*******************************/ * Reproductions supplied by EDRS are the best that can' be made ,* + ) - * from the original doCumente ../ * *****************************************************#*****,J U S DEPARTMENT lEDUCATIOPtilmi AI id NATIONALINS1 i I EDUCAT . THiSDOCUMENTHA! DUCEDEXACTLYAS TAE PERSONOR ORGAP ATIkr;T POINTSOF V STATEDDO NOT NECE SENTiOFFifiALNATION EDUCATIONPOSITION Calculus Part 3 Student's Text REVISED EDITION ' The following is a list of all thosewho.participiated in the preparation of this volume: A. -
SS1718 Example Exam
SOLAR SYSTEM EXAMPLE EXAM B DIVISION 2017-2018 TEAM NUMBER:_____ TEAM NAME:_______________________________________ STUDENT NAMES:___________________________________ ___________________________________ Do not open the test packet until instructed by the event supervisor. Ensure that you have all 6 pages of the test, 3 image sheets, and 2 answer sheets. You are encouraged to use the backs of the test sheets as scratch paper. Only answers recorded on the answer sheet will be graded. All questions are of equal value. Good luck! IMAGE SHEET A IMAGE SHEET B IMAGE SHEET C SECTION A Questions 1-34 in Section A refer to Image Sheet A. 1. Which image shows one full hemisphere of the planet closest to the Sun? 2. Which image shows this planet’s largest crater? 3. What is the name of the crater indicated in Question #2? 4. Which image shows Phobos? 5. Phobos has one large crater, named for the wife of the astronomer who discovered Phobos. What is the name of this crater? 6. What is the name of Mars’s other moon? 7. Does Phobos orbit closer to Mars or further from Mars than Mars’s other moon? 8. Scientists have long believed that Mars’s moons are gravitationally captured asteroids, but recent evidence suggests that they may be another type of solar system object that originated beyond the Asteroid Belt. What kind of objects may Mars’s moons be? 9. Which images show the object closest to Earth? 10. Which image shows the object furthest from Earth? 11. Who discovered the object indicated in Question #10? 12. -
A Concise History of Mathematics the Beginnings 3
A CONCISE HISTORY OF A CONCISE HISTORY MATHEMATICS STRUIK OF MATHEMATICS DIRK J. STRUIK Professor Mathematics, BELL of Massachussetts Institute of Technology i Professor Struik has achieved the seemingly impossible task of compress- ing the history of mathematics into less than three hundred pages. By stressing the unfolding of a few main ideas and by minimizing references to other develop- ments, the author has been able to fol- low Egyptian, Babylonian, Chinese, Indian, Greek, Arabian, and Western mathematics from the earliest records to the beginning of the present century. He has based his account of nineteenth cen- tury advances on persons and schools rather than on subjects as the treatment by subjects has already been used in existing books. Important mathema- ticians whose work is analysed in detail are Euclid, Archimedes, Diophantos, Hammurabi, Bernoulli, Fermat, Euler, Newton, Leibniz, Laplace, Lagrange, Gauss, Jacobi, Riemann, Cremona, Betti, and others. Among the 47 illustra- tions arc portraits of many of these great figures. Each chapter is followed by a select bibliography. CHARLES WILSON A CONCISE HISTORY OF MATHEMATICS by DIRK. J. STRUIK Professor of Mathematics at the Massachusetts Institute of Technology LONDON G. BELL AND SONS LTD '954 Copyright by Dover Publications, Inc., U.S.A. FOR RUTH Printed in Great Britain by Butler & Tanner Ltd., Frame and London CONTENTS Introduction xi The Beginnings 1 The Ancient Orient 13 Greece 39 The Orient after the Decline of Greek Society 83 The Beginnings in Western Europe 98 The