Abscissas and Ordinates
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Exploding the Ellipse Arnold Good
Exploding the Ellipse Arnold Good Mathematics Teacher, March 1999, Volume 92, Number 3, pp. 186–188 Mathematics Teacher is a publication of the National Council of Teachers of Mathematics (NCTM). More than 200 books, videos, software, posters, and research reports are available through NCTM’S publication program. Individual members receive a 20% reduction off the list price. For more information on membership in the NCTM, please call or write: NCTM Headquarters Office 1906 Association Drive Reston, Virginia 20191-9988 Phone: (703) 620-9840 Fax: (703) 476-2970 Internet: http://www.nctm.org E-mail: [email protected] Article reprinted with permission from Mathematics Teacher, copyright May 1991 by the National Council of Teachers of Mathematics. All rights reserved. Arnold Good, Framingham State College, Framingham, MA 01701, is experimenting with a new approach to teaching second-year calculus that stresses sequences and series over integration techniques. eaders are advised to proceed with caution. Those with a weak heart may wish to consult a physician first. What we are about to do is explode an ellipse. This Rrisky business is not often undertaken by the professional mathematician, whose polytechnic endeavors are usually limited to encounters with administrators. Ellipses of the standard form of x2 y2 1 5 1, a2 b2 where a > b, are not suitable for exploding because they just move out of view as they explode. Hence, before the ellipse explodes, we must secure it in the neighborhood of the origin by translating the left vertex to the origin and anchoring the left focus to a point on the x-axis. -
2.3 Conic Sections: Ellipse
2.3 Conic Sections: Ellipse Ellipse: (locus definition) set of all points (x, y) in the plane such that the sum of each of the distances from F1 and F2 is d. Standard Form of an Ellipse: Horizontal Ellipse Vertical Ellipse 22 22 (xh−−) ( yk) (xh−−) ( yk) +=1 +=1 ab22 ba22 center = (hk, ) 2a = length of major axis 2b = length of minor axis c = distance from center to focus cab222=− c eccentricity e = ( 01<<e the closer to 0 the more circular) a 22 (xy+12) ( −) Ex. Graph +=1 925 Center: (−1, 2 ) Endpoints of Major Axis: (-1, 7) & ( -1, -3) Endpoints of Minor Axis: (-4, -2) & (2, 2) Foci: (-1, 6) & (-1, -2) Eccentricity: 4/5 Ex. Graph xyxy22+4224330−++= x2 + 4y2 − 2x + 24y + 33 = 0 x2 − 2x + 4y2 + 24y = −33 x2 − 2x + 4( y2 + 6y) = −33 x2 − 2x +12 + 4( y2 + 6y + 32 ) = −33+1+ 4(9) (x −1)2 + 4( y + 3)2 = 4 (x −1)2 + 4( y + 3)2 4 = 4 4 (x −1)2 ( y + 3)2 + = 1 4 1 Homework: In Exercises 1-8, graph the ellipse. Find the center, the lines that contain the major and minor axes, the vertices, the endpoints of the minor axis, the foci, and the eccentricity. x2 y2 x2 y2 1. + = 1 2. + = 1 225 16 36 49 (x − 4)2 ( y + 5)2 (x +11)2 ( y + 7)2 3. + = 1 4. + = 1 25 64 1 25 (x − 2)2 ( y − 7)2 (x +1)2 ( y + 9)2 5. + = 1 6. + = 1 14 7 16 81 (x + 8)2 ( y −1)2 (x − 6)2 ( y − 8)2 7. -
Deriving Kepler's Laws of Planetary Motion
DERIVING KEPLER’S LAWS OF PLANETARY MOTION By: Emily Davis WHO IS JOHANNES KEPLER? German mathematician, physicist, and astronomer Worked under Tycho Brahe Observation alone Founder of celestial mechanics WHAT ABOUT ISAAC NEWTON? “If I have seen further it is by standing on the shoulders of Giants.” Laws of Motion Universal Gravitation Explained Kepler’s laws The laws could be explained mathematically if his laws of motion and universal gravitation were true. Developed calculus KEPLER’S LAWS OF PLANETARY MOTION 1. Planets move around the Sun in ellipses, with the Sun at one focus. 2. The line connecting the Sun to a planet sweeps equal areas in equal times. 3. The square of the orbital period of a planet is proportional to the cube of the semimajor axis of the ellipse. INITIAL VALUES AND EQUATIONS Unit vectors of polar coordinates (1) INITIAL VALUES AND EQUATIONS From (1), (2) Differentiate with respect to time t (3) INITIAL VALUES AND EQUATIONS CONTINUED… Vectors follow the right-hand rule (8) INITIAL VALUES AND EQUATIONS CONTINUED… Force between the sun and a planet (9) F-force G-universal gravitational constant M-mass of sun Newton’s 2nd law of motion: F=ma m-mass of planet r-radius from sun to planet (10) INITIAL VALUES AND EQUATIONS CONTINUED… Planets accelerate toward the sun, and a is a scalar multiple of r. (11) INITIAL VALUES AND EQUATIONS CONTINUED… Derivative of (12) (11) and (12) together (13) INITIAL VALUES AND EQUATIONS CONTINUED… Integrates to a constant (14) INITIAL VALUES AND EQUATIONS CONTINUED… When t=0, 1. -
Geometry of Some Taxicab Curves
GEOMETRY OF SOME TAXICAB CURVES Maja Petrović 1 Branko Malešević 2 Bojan Banjac 3 Ratko Obradović 4 Abstract In this paper we present geometry of some curves in Taxicab metric. All curves of second order and trifocal ellipse in this metric are presented. Area and perimeter of some curves are also defined. Key words: Taxicab metric, Conics, Trifocal ellipse 1. INTRODUCTION In this paper, taxicab and standard Euclidean metrics for a visual representation of some planar curves are considered. Besides the term taxicab, also used are Manhattan, rectangular metric and city block distance [4], [5], [7]. This metric is a special case of the Minkowski 1 MSc Maja Petrović, assistant at Faculty of Transport and Traffic Engineering, University of Belgrade, Serbia, e-mail: [email protected] 2 PhD Branko Malešević, associate professor at Faculty of Electrical Engineering, Department of Applied Mathematics, University of Belgrade, Serbia, e-mail: [email protected] 3 MSc Bojan Banjac, student of doctoral studies of Software Engineering, Faculty of Electrical Engineering, University of Belgrade, Serbia, assistant at Faculty of Technical Sciences, Computer Graphics Chair, University of Novi Sad, Serbia, e-mail: [email protected] 4 PhD Ratko Obradović, full professor at Faculty of Technical Sciences, Computer Graphics Chair, University of Novi Sad, Serbia, e-mail: [email protected] 1 metrics of order 1, which is for distance between two points , and , determined by: , | | | | (1) Minkowski metrics contains taxicab metric for value 1 and Euclidean metric for 2. The term „taxicab geometry“ was first used by K. Menger in the book [9]. -
Mission to the Solar Gravity Lens Focus: Natural Highground for Imaging Earth-Like Exoplanets L
Planetary Science Vision 2050 Workshop 2017 (LPI Contrib. No. 1989) 8203.pdf MISSION TO THE SOLAR GRAVITY LENS FOCUS: NATURAL HIGHGROUND FOR IMAGING EARTH-LIKE EXOPLANETS L. Alkalai1, N. Arora1, M. Shao1, S. Turyshev1, L. Friedman8 ,P. C. Brandt3, R. McNutt3, G. Hallinan2, R. Mewaldt2, J. Bock2, M. Brown2, J. McGuire1, A. Biswas1, P. Liewer1, N. Murphy1, M. Desai4, D. McComas5, M. Opher6, E. Stone2, G. Zank7, 1Jet Propulsion Laboratory, Pasadena, CA 91109, USA, 2California Institute of Technology, Pasadena, CA 91125, USA, 3The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA,4Southwest Research Institute, San Antonio, TX 78238, USA, 5Princeton Plasma Physics Laboratory, Princeton, NJ 08543, USA, 6Boston University, Boston, MA 02215, USA, 7University of Alabama in Huntsville, Huntsville, AL 35899, USA, 8Emritus, The Planetary Society. Figure 1: A SGL Probe Mission is a first step in the goal to search and study potential habitable exoplanets. This figure was developed as a product of two Keck Institute for Space Studies (KISS) workshops on the topic of the “Science and Enabling Technologies for the Exploration of the Interstellar Medium” led by E. Stone, L. Alkalai and L. Friedman. Introduction: Recent data from Voyager 1, Kepler and New Horizons spacecraft have resulted in breath-taking discoveries that have excited the public and invigorated the space science community. Voyager 1, the first spacecraft to arrive at the Heliopause, discovered that Fig. 2. Imaging of an exo-Earth with solar gravitational Lens. The exo-Earth occupies (1km×1km) area at the image plane. Using a 1m the interstellar medium is far more complicated and telescope as a 1 pixel detector provides a (1000×1000) pixel image! turbulent than expected; the Kepler telescope According to Einstein’s general relativity, gravity discovered that exoplanets are not only ubiquitous but induces refractive properties of space-time causing a also diverse in our galaxy and that Earth-like exoplanets massive object to act as a lens by bending light. -
A Mathematician Reads Plutarch: Plato's Criticism of Geometers of His Time
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Scholarship@Claremont Journal of Humanistic Mathematics Volume 7 | Issue 2 July 2017 A Mathematician Reads Plutarch: Plato's Criticism of Geometers of His Time John B. Little College of the Holy Cross Follow this and additional works at: https://scholarship.claremont.edu/jhm Part of the Ancient History, Greek and Roman through Late Antiquity Commons, and the Mathematics Commons Recommended Citation Little, J. B. "A Mathematician Reads Plutarch: Plato's Criticism of Geometers of His Time," Journal of Humanistic Mathematics, Volume 7 Issue 2 (July 2017), pages 269-293. DOI: 10.5642/ jhummath.201702.13 . Available at: https://scholarship.claremont.edu/jhm/vol7/iss2/13 ©2017 by the authors. This work is licensed under a Creative Commons License. JHM is an open access bi-annual journal sponsored by the Claremont Center for the Mathematical Sciences and published by the Claremont Colleges Library | ISSN 2159-8118 | http://scholarship.claremont.edu/jhm/ The editorial staff of JHM works hard to make sure the scholarship disseminated in JHM is accurate and upholds professional ethical guidelines. However the views and opinions expressed in each published manuscript belong exclusively to the individual contributor(s). The publisher and the editors do not endorse or accept responsibility for them. See https://scholarship.claremont.edu/jhm/policies.html for more information. A Mathematician Reads Plutarch: Plato's Criticism of Geometers of His Time Cover Page Footnote This essay originated as an assignment for Professor Thomas Martin's Plutarch seminar at Holy Cross in Fall 2016. -
A Short History of Greek Mathematics
Cambridge Library Co ll e C t i o n Books of enduring scholarly value Classics From the Renaissance to the nineteenth century, Latin and Greek were compulsory subjects in almost all European universities, and most early modern scholars published their research and conducted international correspondence in Latin. Latin had continued in use in Western Europe long after the fall of the Roman empire as the lingua franca of the educated classes and of law, diplomacy, religion and university teaching. The flight of Greek scholars to the West after the fall of Constantinople in 1453 gave impetus to the study of ancient Greek literature and the Greek New Testament. Eventually, just as nineteenth-century reforms of university curricula were beginning to erode this ascendancy, developments in textual criticism and linguistic analysis, and new ways of studying ancient societies, especially archaeology, led to renewed enthusiasm for the Classics. This collection offers works of criticism, interpretation and synthesis by the outstanding scholars of the nineteenth century. A Short History of Greek Mathematics James Gow’s Short History of Greek Mathematics (1884) provided the first full account of the subject available in English, and it today remains a clear and thorough guide to early arithmetic and geometry. Beginning with the origins of the numerical system and proceeding through the theorems of Pythagoras, Euclid, Archimedes and many others, the Short History offers in-depth analysis and useful translations of individual texts as well as a broad historical overview of the development of mathematics. Parts I and II concern Greek arithmetic, including the origin of alphabetic numerals and the nomenclature for operations; Part III constitutes a complete history of Greek geometry, from its earliest precursors in Egypt and Babylon through to the innovations of the Ionic, Sophistic, and Academic schools and their followers. -
Orbital Mechanics Course Notes
Orbital Mechanics Course Notes David J. Westpfahl Professor of Astrophysics, New Mexico Institute of Mining and Technology March 31, 2011 2 These are notes for a course in orbital mechanics catalogued as Aerospace Engineering 313 at New Mexico Tech and Aerospace Engineering 362 at New Mexico State University. This course uses the text “Fundamentals of Astrodynamics” by R.R. Bate, D. D. Muller, and J. E. White, published by Dover Publications, New York, copyright 1971. The notes do not follow the book exclusively. Additional material is included when I believe that it is needed for clarity, understanding, historical perspective, or personal whim. We will cover the material recommended by the authors for a one-semester course: all of Chapter 1, sections 2.1 to 2.7 and 2.13 to 2.15 of Chapter 2, all of Chapter 3, sections 4.1 to 4.5 of Chapter 4, and as much of Chapters 6, 7, and 8 as time allows. Purpose The purpose of this course is to provide an introduction to orbital me- chanics. Students who complete the course successfully will be prepared to participate in basic space mission planning. By basic mission planning I mean the planning done with closed-form calculations and a calculator. Stu- dents will have to master additional material on numerical orbit calculation before they will be able to participate in detailed mission planning. There is a lot of unfamiliar material to be mastered in this course. This is one field of human endeavor where engineering meets astronomy and ce- lestial mechanics, two fields not usually included in an engineering curricu- lum. -
Big Astronomy Educator Guide
Show Summary 2 EDUCATOR GUIDE National Science Standards Supported 4 Main Questions and Answers 5 TABLE OF CONTENTS Glossary of Terms 9 Related Activities 10 Additional Resources 17 Credits 17 SHOW SUMMARY Big Astronomy: People, Places, Discoveries explores three observatories located in Chile, at extreme and remote places. It gives examples of the multitude of STEM careers needed to keep the great observatories working. The show is narrated by Barbara Rojas-Ayala, a Chilean astronomer. A great deal of astronomy is done in the nation of Energy Camera. Here we meet Marco Bonati, who is Chile, due to its special climate and location, which an Electronics Detector Engineer. He is responsible creates stable, dry air. With its high, dry, and dark for what happens inside the instrument. Marco tells sites, Chile is one of the best places in the world for us about this job, and needing to keep the instrument observational astronomy. The show takes you to three very clean. We also meet Jacoline Seron, who is a of the many telescopes along Chile’s mountains. Night Assistant at CTIO. Her job is to take care of the instrument, calibrate the telescope, and operate The first site we visit is the Cerro Tololo Inter-American the telescope at night. Finally, we meet Kathy Vivas, Observatory (CTIO), which is home to many who is part of the support team for the Dark Energy telescopes. The largest is the Victor M. Blanco Camera. She makes sure the camera is producing Telescope, which has a 4-meter primary mirror. The science-quality data. -
Boethius the Demiurge
BOETHIUS THE DEMIURGE: TIMAEAN DOUBLE-CIRCLE SPIRAL STRUCTURE IN THE CONSOLATIO by Cristalle N. Watson Submitted in partial fulfilment of the requirements for the degree of Master of Arts at Dalhousie University Halifax, Nova Scotia April 2020 © Copyright by Cristalle N. Watson, 2020 For my Opa, Karl Heinz Hiob 1926-1999 Vir doctissimus & lover of words, who first introduced me to Latin Ars longa, vita brevis ii TABLE OF CONTENTS LIST OF TABLES..............................................................................................................vi LIST OF FIGURES...........................................................................................................vii ABSTRACT.....................................................................................................................viii ACKNOWLEDGEMENTS................................................................................................ix CHAPTER 1: INTRODUCTION........................................................................................1 CHAPTER 2: POETRY AND THE CIRCLE IN THE CONSOLATIO: AN OVERVIEW….............................................................................................................3 2.1 A "MULTIFACETED" CONSOLATIO AND AUTHOR.............................................3 2.2 THE METERS OF THE CONSOLATIO: A NEGLECTED STUDY............................11 2.3 IIIM9: CENTRAL PIVOT, TIMAEAN PARAPHRASE, PRAYER...........................17 2.4 THE CIRCLE IN THE CONSOLATIO AND IN IIIM9.............................................22 -
5. Hipparchus 6. Ptolemy
introduction | 15 catalogue included into his oeuvre? Our answer is in Hipparchus. The catalogue itself has not survived. the positive. We have developed a method to serve However, it is believed that the ecliptic longitude and this end, tested it on several veraciously dated cata- latitude of each star was indicated there, as well as the logues, and then applied it to the Almagest. The reader magnitude. It is believed that Hipparchus localised the shall find out about our results in the present book. stars using the same terms as the Almagest: “the star Let us now cite some brief biographical data con- on the right shoulder of Perseus”,“the star over the cerning the astronomers whose activities are imme- head of Aquarius” etc ([395], page 52). diately associated with the problem as described above. One invariably ponders the extreme vagueness of These data are published in Scaligerian textbooks. One this star localization method. Not only does it imply must treat them critically, seeing as how the Scaligerian a canonical system of drawing the constellations and version of history is based on an erroneous chronol- indicating the stars they include – another stipulation ogy (see Chron1 and Chron2). We shall consider is that there are enough identical copies of a single star other facts that confirm it in the present book. chart in existence. This is the only way to make the verbal descriptions of stars such as the above work 5. and help a researcher with the actual identification of HIPPARCHUS stars. However, in this case the epoch of the cata- logue’s propagation must postdate the invention of Scaligerian history is of the opinion that astron- the printing press and the engraving technique, since omy became a natural science owing to the works of no multiple identical copies of a single work could be Hipparchus, an astronomer from the “ancient” Greece manufactured earlier. -
Lecture 11. Apollonius and Conic Sections
Lecture 11. Apollonius and Conic Sections Figure 11.1 Apollonius of Perga Apollonius of Perga Apollonius (262 B.C.-190 B.C.) was born in the Greek city of Perga, close to the southeast coast of Asia Minor. He was a Greek geometer and astronomer. His major mathematical work on the theory of conic sections had a very great influence on the development of mathematics and his famous book Conics introduced the terms parabola, ellipse and hyperbola. Apollonius' theory of conics was so admired that it was he, rather than Euclid, who in antiquity earned the title the Great Geometer. He also made contribution to the study of the Moon. The Apollonius crater on the Moon was named in his honor. Apollonius came to Alexandria in his youth and learned mathematics from Euclid's successors. As far as we know he remained in Alexandria and became an associate among the great mathematicians who worked there. We do not know much details about his life. His chief work was on the conic sections but he also wrote on other subjects. His mathematical powers were so extraordinary that he became known in his time. His reputation as an astronomer was also great. Apollonius' mathematical works Apollonius is famous for his work, the Conic, which was spread out over eight books and contained 389 propositions. The first four books were 69 in the original Greek language, the next three are preserved in Arabic translations, while the last one is lost. Even though seven of the eight books of the Conics have survived, most of his mathematical work is known today only by titles and summaries in works of later authors.