Enhancing Conceptual Understanding of Trigonometry Using Earth Geometry and the Great Circle
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Assignment: 14 Subject: - Social Science Class: - VI Teacher: - Mrs
Assignment: 14 Subject: - Social Science Class: - VI Teacher: - Mrs. Shilpa Grover Name: ______________ Class & Sec: _______________ Roll No. ______ Date: 23.05.2020 GEOGRAPHY QUESTIONS CHAPTER-2 A. Define the following terms: 1. Equator: It is an imaginary line drawn midway between the North and South Poles. It divides the Earth into two equal parts, the North Hemisphere and the South Hemisphere. 2. Earth’s grid: The network of parallels or latitudes and meridians or longitudes that divide the Earth’s surface into a grid-like pattern is called the Earth’s grid or geographic grid. 3. Heat zones: The Earth is divided into three heat zones based on the amount of heat each part receives from the Sun. These three heat zones are the Torrid Zone, the Temperate Zone and the Frigid Zone. 4. Great circle: The Equator is known as the great circle, as it is the largest circle that can be drawn on the globe. This is because the equatorial diameter of the Earth is the largest. 5. Prime Meridian: It is the longitude that passes through Greenwich, a place near London in the UK. It is treated as the reference point. Places to the east and west of the Prime Meridian are measured in degrees. 6. Time zones: A time zone is a narrow belt of the Earth’s surface, which has an east‒west extent of 15 degrees of longitude. The world has been divided into 24 standard time zones. B. Answer the following Questions: 1. What is the true shape of the Earth? The Earth looks spherical in shape, but it is slightly flattened at the North and South Poles and bulges at the equator due to the outward force caused by the rotation of the Earth. -
And Are Lines on Sphere B That Contain Point Q
11-5 Spherical Geometry Name each of the following on sphere B. 3. a triangle SOLUTION: are examples of triangles on sphere B. 1. two lines containing point Q SOLUTION: and are lines on sphere B that contain point Q. ANSWER: 4. two segments on the same great circle SOLUTION: are segments on the same great circle. ANSWER: and 2. a segment containing point L SOLUTION: is a segment on sphere B that contains point L. ANSWER: SPORTS Determine whether figure X on each of the spheres shown is a line in spherical geometry. 5. Refer to the image on Page 829. SOLUTION: Notice that figure X does not go through the pole of ANSWER: the sphere. Therefore, figure X is not a great circle and so not a line in spherical geometry. ANSWER: no eSolutions Manual - Powered by Cognero Page 1 11-5 Spherical Geometry 6. Refer to the image on Page 829. 8. Perpendicular lines intersect at one point. SOLUTION: SOLUTION: Notice that the figure X passes through the center of Perpendicular great circles intersect at two points. the ball and is a great circle, so it is a line in spherical geometry. ANSWER: yes ANSWER: PERSEVERANC Determine whether the Perpendicular great circles intersect at two points. following postulate or property of plane Euclidean geometry has a corresponding Name two lines containing point M, a segment statement in spherical geometry. If so, write the containing point S, and a triangle in each of the corresponding statement. If not, explain your following spheres. reasoning. 7. The points on any line or line segment can be put into one-to-one correspondence with real numbers. -
Chapter Outline Thinking Ahead 4 EARTH, MOON, AND
Chapter 4 Earth, Moon, and Sky 103 4 EARTH, MOON, AND SKY Figure 4.1 Southern Summer. As captured with a fish-eye lens aboard the Atlantis Space Shuttle on December 9, 1993, Earth hangs above the Hubble Space Telescope as it is repaired. The reddish continent is Australia, its size and shape distorted by the special lens. Because the seasons in the Southern Hemisphere are opposite those in the Northern Hemisphere, it is summer in Australia on this December day. (credit: modification of work by NASA) Chapter Outline 4.1 Earth and Sky 4.2 The Seasons 4.3 Keeping Time 4.4 The Calendar 4.5 Phases and Motions of the Moon 4.6 Ocean Tides and the Moon 4.7 Eclipses of the Sun and Moon Thinking Ahead If Earth’s orbit is nearly a perfect circle (as we saw in earlier chapters), why is it hotter in summer and colder in winter in many places around the globe? And why are the seasons in Australia or Peru the opposite of those in the United States or Europe? The story is told that Galileo, as he left the Hall of the Inquisition following his retraction of the doctrine that Earth rotates and revolves about the Sun, said under his breath, “But nevertheless it moves.” Historians are not sure whether the story is true, but certainly Galileo knew that Earth was in motion, whatever church authorities said. It is the motions of Earth that produce the seasons and give us our measures of time and date. The Moon’s motions around us provide the concept of the month and the cycle of lunar phases. -
Reference Systems for Surveying and Mapping Lecture Notes
Delft University of Technology Reference Systems for Surveying and Mapping Lecture notes Hans van der Marel ii The front cover shows the NAP (Amsterdam Ordnance Datum) ”datum point” at the Stopera, Amsterdam (picture M.M.Minderhoud, Wikipedia/Michiel1972). H. van der Marel Lecture notes on Reference Systems for Surveying and Mapping: CTB3310 Surveying and Mapping CTB3425 Monitoring and Stability of Dikes and Embankments CIE4606 Geodesy and Remote Sensing CIE4614 Land Surveying and Civil Infrastructure February 2020 Publisher: Faculty of Civil Engineering and Geosciences Delft University of Technology P.O. Box 5048 Stevinweg 1 2628 CN Delft The Netherlands Copyright ©20142020 by H. van der Marel The content in these lecture notes, except for material credited to third parties, is licensed under a Creative Commons AttributionsNonCommercialSharedAlike 4.0 International License (CC BYNCSA). Third party material is shared under its own license and attribution. The text has been type set using the MikTex 2.9 implementation of LATEX. Graphs and diagrams were produced, if not mentioned otherwise, with Matlab and Inkscape. Preface This reader on reference systems for surveying and mapping has been initially compiled for the course Surveying and Mapping (CTB3310) in the 3rd year of the BScprogram for Civil Engineering. The reader is aimed at students at the end of their BSc program or at the start of their MSc program, and is used in several courses at Delft University of Technology. With the advent of the Global Positioning System (GPS) technology in mobile (smart) phones and other navigational devices almost anyone, anywhere on Earth, and at any time, can determine a three–dimensional position accurate to a few meters. -
Educator Guide
E DUCATOR GUIDE This guide, and its contents, are Copyrighted and are the sole Intellectual Property of Science North. E DUCATOR GUIDE The Arctic has always been a place of mystery, myth and fascination. The Inuit and their predecessors adapted and thrived for thousands of years in what is arguably the harshest environment on earth. Today, the Arctic is the focus of intense research. Instead of seeking to conquer the north, scientist pioneers are searching for answers to some troubling questions about the impacts of human activities around the world on this fragile and largely uninhabited frontier. The giant screen film, Wonders of the Arctic, centers on our ongoing mission to explore and come to terms with the Arctic, and the compelling stories of our many forays into this captivating place will be interwoven to create a unifying message about the state of the Arctic today. Underlying all these tales is the crucial role that ice plays in the northern environment and the changes that are quickly overtaking the people and animals who have adapted to this land of ice and snow. This Education Guide to the Wonders of the Arctic film is a tool for educators to explore the many fascinating aspects of the Arctic. This guide provides background information on Arctic geography, wildlife and the ice, descriptions of participatory activities, as well as references and other resources. The guide may be used to prepare the students for the film, as a follow up to the viewing, or to simply stimulate exploration of themes not covered within the film. -
THE EARTH. MERIDIANS and PARALLELS 2=Meridian (Geography)
THE EARTH. MERIDIANS AND PARALLELS 1=Circle of latitude 2=Meridian (geography) A circle of latitude , on the Earth , is an imaginary east -west circle connecting all locations (not taking into account elevation) that share a given latitude . A location's position along a circle of latitude is given by its longitude . Circles of latitude are often called parallels because they are parallel to each other. On some map projections, including the Equirectangular projection , they are drawn at equidistant intervals. Circles of latitude become smaller the farther they are from the equator and the closer they are to the poles . A circle of latitude is perpendicular to all meridians at the points of intersection, and is hence a special case of a loxodrome . Contrary to what might be assumed from their straight-line representation on some map projections, a circle of latitude is not, with the sole exception of the Equator, the shortest distance between two points lying on the Earth. In other words, circles of latitude (except for the Equator) are not great circles (see also great-circle distance ). It is for this reason that an airplane traveling between a European and North American city that share the same latitude will fly farther north, over Greenland for example. Arcs of circles of latitude are sometimes used as boundaries between countries or regions where distinctive natural borders are lacking (such as in deserts), or when an artificial border is drawn as a "line on a map", as happened in Korea . Longitude (λ) Lines of longitude appear vertical with varying curvature in this projection; but are actually halves of great ellipses, with identical radii at a given latitude. -
List of Boundary Lines
A M K RESOURCE WORLD GENERAL KNOWLEDGE www.amkresourceinfo.com List of Boundary Lines The line which demarcates the two countries is termed as Boundary Line List of important boundary lines Durand Line is the line demarcating the boundaries of Pakistan and Afghanistan. It was drawn up in 1896 by Sir Mortimer Durand. Hindenburg Line is the boundary dividing Germany and Poland. The Germans retreated to this line in 1917 during World War I Mason-Dixon Line is a line of demarcation between four states in the United State. Marginal Line was the 320-km line of fortification on the Russia-Finland border. Drawn up by General Mannerheim. Macmahon Line was drawn up by Sir Henry MacMahon, demarcating the frontier of India and China. China did not recognize the MacMahon line and crossed it in 1962. Medicine Line is the border between Canada and the United States. Radcliffe Line was drawn up by Sir Cyril Radcliffe, demarcating the boundary between India and Pakistan. Siegfried Line is the line of fortification drawn up by Germany on its border with France.Order-Neisse Line is the border between Poland and Germany, running along the Order and Neisse rivers, adopted at the Poland Conference (Aug 1945) after World War II. 17th Parallel defined the boundary between North Vietnam and South Vietnam before two were united. 24th Parallel is the line which Pakistan claims for demarcation between India and Pakistan. This, however, is not recognized by India 26th Parallel south is a circle of latitude which crosses through Africa, Australia and South America. 30th Parallel north is a line of latitude that stands one-third of the way between the equator and the North Pole. -
Positional Astronomy Coordinate Systems
Positional Astronomy Observational Astronomy 2019 Part 2 Prof. S.C. Trager Coordinate systems We need to know where the astronomical objects we want to study are located in order to study them! We need a system (well, many systems!) to describe the positions of astronomical objects. The Celestial Sphere First we need the concept of the celestial sphere. It would be nice if we knew the distance to every object we’re interested in — but we don’t. And it’s actually unnecessary in order to observe them! The Celestial Sphere Instead, we assume that all astronomical sources are infinitely far away and live on the surface of a sphere at infinite distance. This is the celestial sphere. If we define a coordinate system on this sphere, we know where to point! Furthermore, stars (and galaxies) move with respect to each other. The motion normal to the line of sight — i.e., on the celestial sphere — is called proper motion (which we’ll return to shortly) Astronomical coordinate systems A bit of terminology: great circle: a circle on the surface of a sphere intercepting a plane that intersects the origin of the sphere i.e., any circle on the surface of a sphere that divides that sphere into two equal hemispheres Horizon coordinates A natural coordinate system for an Earth- bound observer is the “horizon” or “Alt-Az” coordinate system The great circle of the horizon projected on the celestial sphere is the equator of this system. Horizon coordinates Altitude (or elevation) is the angle from the horizon up to our object — the zenith, the point directly above the observer, is at +90º Horizon coordinates We need another coordinate: define a great circle perpendicular to the equator (horizon) passing through the zenith and, for convenience, due north This line of constant longitude is called a meridian Horizon coordinates The azimuth is the angle measured along the horizon from north towards east to the great circle that intercepts our object (star) and the zenith. -
Spherical Geometry
987023 2473 < % 52873 52 59 3 1273 ¼4 14 578 2 49873 3 4 7∆��≌ ≠ 3 δ � 2 1 2 7 5 8 4 3 23 5 1 ⅓β ⅝Υ � VCAA-AMSI maths modules 5 1 85 34 5 45 83 8 8 3 12 5 = 2 38 95 123 7 3 7 8 x 3 309 �Υβ⅓⅝ 2 8 13 2 3 3 4 1 8 2 0 9 756 73 < 1 348 2 5 1 0 7 4 9 9 38 5 8 7 1 5 812 2 8 8 ХФУШ 7 δ 4 x ≠ 9 3 ЩЫ � Ѕ � Ђ 4 � ≌ = ⅙ Ё ∆ ⊚ ϟϝ 7 0 Ϛ ό ¼ 2 ύҖ 3 3 Ҧδ 2 4 Ѽ 3 5 ᴂԅ 3 3 Ӡ ⍰1 ⋓ ӓ 2 7 ӕ 7 ⟼ ⍬ 9 3 8 Ӂ 0 ⤍ 8 9 Ҷ 5 2 ⋟ ҵ 4 8 ⤮ 9 ӛ 5 ₴ 9 4 5 € 4 ₦ € 9 7 3 ⅘ 3 ⅔ 8 2 2 0 3 1 ℨ 3 ℶ 3 0 ℜ 9 2 ⅈ 9 ↄ 7 ⅞ 7 8 5 2 ∭ 8 1 8 2 4 5 6 3 3 9 8 3 8 1 3 2 4 1 85 5 4 3 Ӡ 7 5 ԅ 5 1 ᴂ - 4 �Υβ⅓⅝ 0 Ѽ 8 3 7 Ҧ 6 2 3 Җ 3 ύ 4 4 0 Ω 2 = - Å 8 € ℭ 6 9 x ℗ 0 2 1 7 ℋ 8 ℤ 0 ∬ - √ 1 ∜ ∱ 5 ≄ 7 A guide for teachers – Years 11 and 12 ∾ 3 ⋞ 4 ⋃ 8 6 ⑦ 9 ∭ ⋟ 5 ⤍ ⅞ Geometry ↄ ⟼ ⅈ ⤮ ℜ ℶ ⍬ ₦ ⍰ ℨ Spherical Geometry ₴ € ⋓ ⊚ ⅙ ӛ ⋟ ⑦ ⋃ Ϛ ό ⋞ 5 ∾ 8 ≄ ∱ 3 ∜ 8 7 √ 3 6 ∬ ℤ ҵ 4 Ҷ Ӂ ύ ӕ Җ ӓ Ӡ Ҧ ԅ Ѽ ᴂ 8 7 5 6 Years DRAFT 11&12 DRAFT Spherical Geometry – A guide for teachers (Years 11–12) Andrew Stewart, Presbyterian Ladies’ College, Melbourne Illustrations and web design: Catherine Tan © VCAA and The University of Melbourne on behalf of AMSI 2015. -
08. Non-Euclidean Geometry 1
Topics: 08. Non-Euclidean Geometry 1. Euclidean Geometry 2. Non-Euclidean Geometry 1. Euclidean Geometry • The Elements. ~300 B.C. ~100 A.D. Earliest existing copy 1570 A.D. 1956 First English translation Dover Edition • 13 books of propositions, based on 5 postulates. 1 Euclid's 5 Postulates 1. A straight line can be drawn from any point to any point. • • A B 2. A finite straight line can be produced continuously in a straight line. • • A B 3. A circle may be described with any center and distance. • 4. All right angles are equal to one another. 2 5. If a straight line falling on two straight lines makes the interior angles on the same side together less than two right angles, then the two straight lines, if produced indefinitely, meet on that side on which the angles are together less than two right angles. � � • � + � < 180∘ • Euclid's Accomplishment: showed that all geometric claims then known follow from these 5 postulates. • Is 5th Postulate necessary? (1st cent.-19th cent.) • Basic strategy: Attempt to show that replacing 5th Postulate with alternative leads to contradiction. 3 • Equivalent to 5th Postulate (Playfair 1795): 5'. Through a given point, exactly one line can be drawn parallel to a given John Playfair (1748-1819) line (that does not contain the point). • Parallel straight lines are straight lines which, being in the same plane and being • Only two logically possible alternatives: produced indefinitely in either direction, do not meet one 5none. Through a given point, no lines can another in either direction. (The Elements: Book I, Def. -
The Celestial Sphere
The Celestial Sphere Useful References: • Smart, “Text-Book on Spherical Astronomy” (or similar) • “Astronomical Almanac” and “Astronomical Almanac’s Explanatory Supplement” (always definitive) • Lang, “Astrophysical Formulae” (for quick reference) • Allen “Astrophysical Quantities” (for quick reference) • Karttunen, “Fundamental Astronomy” (e-book version accessible from Penn State at http://www.springerlink.com/content/j5658r/ Numbers to Keep in Mind • 4 π (180 / π)2 = 41,253 deg2 on the sky • ~ 23.5° = obliquity of the ecliptic • 17h 45m, -29° = coordinates of Galactic Center • 12h 51m, +27° = coordinates of North Galactic Pole • 18h, +66°33’ = coordinates of North Ecliptic Pole Spherical Astronomy Geocentrically speaking, the Earth sits inside a celestial sphere containing fixed stars. We are therefore driven towards equations based on spherical coordinates. Rules for Spherical Astronomy • The shortest distance between two points on a sphere is a great circle. • The length of a (great circle) arc is proportional to the angle created by the two radial vectors defining the points. • The great-circle arc length between two points on a sphere is given by cos a = (cos b cos c) + (sin b sin c cos A) where the small letters are angles, and the capital letters are the arcs. (This is the fundamental equation of spherical trigonometry.) • Two other spherical triangle relations which can be derived from the fundamental equation are sin A sinB = and sin a cos B = cos b sin c – sin b cos c cos A sina sinb € Proof of Fundamental Equation • O is -
Appendix a Glossary
BASICS OF RADIO ASTRONOMY Appendix A Glossary Absolute magnitude Apparent magnitude a star would have at a distance of 10 parsecs (32.6 LY). Absorption lines Dark lines superimposed on a continuous electromagnetic spectrum due to absorption of certain frequencies by the medium through which the radiation has passed. AM Amplitude modulation. Imposing a signal on transmitted energy by varying the intensity of the wave. Amplitude The maximum variation in strength of an electromagnetic wave in one wavelength. Ångstrom Unit of length equal to 10-10 m. Sometimes used to measure wavelengths of visible light. Now largely superseded by the nanometer (10-9 m). Aphelion The point in a body’s orbit (Earth’s, for example) around the sun where the orbiting body is farthest from the sun. Apogee The point in a body’s orbit (the moon’s, for example) around Earth where the orbiting body is farthest from Earth. Apparent magnitude Measure of the observed brightness received from a source. Astrometry Technique of precisely measuring any wobble in a star’s position that might be caused by planets orbiting the star and thus exerting a slight gravitational tug on it. Astronomical horizon The hypothetical interface between Earth and sky, as would be seen by the observer if the surrounding terrain were perfectly flat. Astronomical unit Mean Earth-to-sun distance, approximately 150,000,000 km. Atmospheric window Property of Earth’s atmosphere that allows only certain wave- lengths of electromagnetic energy to pass through, absorbing all other wavelengths. AU Abbreviation for astronomical unit. Azimuth In the horizon coordinate system, the horizontal angle from some arbitrary reference direction (north, usually) clockwise to the object circle.