The Celestial Sphere

Total Page:16

File Type:pdf, Size:1020Kb

The Celestial Sphere 2/3/09 Mastering Astronomy Assignment 2 Constellations – the 88 semi-rectangular regions that make up the sky • Due Feb 10, 11 am • Northern constellations have Latinized • Read Chapter 1 Greek-mythology names: – Orion, Cygnus, Leo, Ursa Major, Canis Major, Canis Minor • Southern constellations have Latin names: – Telescopium, Sextans, Pyxsis What do you think? What do you think? • Do the stars stay in the same position in the • What causes the stars move? sky all day/night long? • Do the stars actually move in the way they • Do we see the same stars all year round appear from Earth? every night? • Is the daily motion of the Sun different from the stars? Earth’s daily rotation and yearly orbit The Celestial Sphere • The north celestial pole (NCP) • The south celestial pole (SCP) • The celestial equator • The ecliptic • Right ascension – like longitude • Declination – like latitude 1 2/3/09 The Celestial Sphere The Milky Way A band of light The 88 official making a circle constellations around the celestial cover the celestial sphere. sphere. What is it? Our view into the plane of our galaxy. Our view from Earth: The Local Sky • Stars near the north celestial pole are circumpolar and An object’s altitude (above horizon) and direction never set. (along horizon) specifies its location in your local • We cannot see stars near the south celestial pole. sky • All other stars (and Sun, Moon, planets) rise in east and set in west. A circumpolar star never sets Celesal Equator Your Horizon This star never rises Celestial Sphere In-class Activities: Position Rotation Star B 2 Star A 1 2 • Work with a partner! Celestial Celestial Sphere 3 Sphere • Read the instructions and questions carefully. 1 4 • Discuss the concepts and your answers with one 3 another. Take time to understand it now!!!! Horizon • Come to a consensus answer you both agree on. 4 • If you get stuck or are not sure of your answer, ask another group. Celestial Sphere • If you get really stuck or don’t understand what the Rotation question is asking, ask me. 2 2/3/09 Is the horizon shown a real physical horizon or an Celestial Sphere Rotation imaginary plane that extends In what direction Star B from your observing location 2 Star A and Earth out to the stars? Celestial Sphere is the observer 1 2 Rotation Star B Celestial Sphere Celestial Sphere facing? 3 Can the observer shown see a 2 Star A 1 star when it is located below 1 2 4 the horizon? Why or why not? Celestial Celestial 3 Sphere 3 Sphere 1 a) toward the South Horizon Is there a star that is in an unobservable position? 4 b) toward the North 4 3 Horizon c) toward the East When a star travels from a d) toward the West Celestial Sphere position below the observer’s Rotation 4 horizon to a position above the horizon, is that star rising or setting? Celestial Sphere Rotation Imagine that from your current location you Celestial Sphere observe a star rising directly in the east. When this Where would the Rotation Star B star reaches its highest position above the horizon, observer look to see 2 Star A where will it be? 1 2 the star indicated by Celestial Celestial Sphere 3 Sphere the arrow? 1 A. high in the northern sky 4 3 B. high in the southern sky Horizon C. high in the western sky D. directly overhead A. High in the Northeast 4 B. High in the Southeast Celestial C. High in the Northwest Sphere D. High in the Southwest Rotation Nightly Motion of the Stars Earth’s rotation • Imagine looking Celestial Sphere Rotation Star B causes the Sun, toward the East as 2 Star A Planets, Moon a star rises above 1 2 Celestial Celestial Sphere 3 Sphere and stars to your horizon - 1 appear to move what does it do 4 after that? 3 when viewed Horizon from Earth 4 Celestial Sphere Rotation 3 2/3/09 Nightly Motion of the Stars What direction • For stars (the Moon and planets) that is the observer appear in the southern sky: Stars first rise facing in this near the eastern horizon, move upward and toward the south, and then move down and picture? set near the western horizon. A. North B. South C. East D. West Nightly Motion of the Stars Nightly Motion of the Stars Celestial Sphere Rotation Star B 2 Star A • Imagine looking toward the North. What 1 2 Celestial Sphere Celestial Sphere do stars appear to do over the course of 3 1 an evening? 4 3 Horizon 4 Celestial Sphere Rotation Looking North: Circumpolar Stars Nightly Motion of the Stars • Looking North: Stars – Circumpolar stars seem to move counter-clockwise appear to move around the stationary North Star. counter-clockwise – These constellations and stars are visible any night of the around the stationary year in the NORTHERN sky because they never rise or North Star (Polaris) – set! we call these – Examples: Ursa Major, Ursa Minor, Draco, Cepheus, and Cassiopeia circumpolar stars. 4 2/3/09 What happens over time in the Northern Sky? How long did it take to get this picture? Take out a piece of paper and put your name on it along with your answer!! In-class Activities: Motion • Work with a partner! • Read the instructions and questions carefully. • Discuss the concepts and your answers with one another. Take time to understand it now!!!! • Come to a consensus answer you both agree on. • If you get stuck or are not sure of your answer, ask another group. • If you get really stuck or don’t understand what the question is asking, ask me. 5 .
Recommended publications
  • Constructing a Galactic Coordinate System Based on Near-Infrared and Radio Catalogs
    A&A 536, A102 (2011) Astronomy DOI: 10.1051/0004-6361/201116947 & c ESO 2011 Astrophysics Constructing a Galactic coordinate system based on near-infrared and radio catalogs J.-C. Liu1,2,Z.Zhu1,2, and B. Hu3,4 1 Department of astronomy, Nanjing University, Nanjing 210093, PR China e-mail: [jcliu;zhuzi]@nju.edu.cn 2 key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing 210093, PR China 3 Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, PR China 4 Graduate School of Chinese Academy of Sciences, Beijing 100049, PR China e-mail: [email protected] Received 24 March 2011 / Accepted 13 October 2011 ABSTRACT Context. The definition of the Galactic coordinate system was announced by the IAU Sub-Commission 33b on behalf of the IAU in 1958. An unrigorous transformation was adopted by the Hipparcos group to transform the Galactic coordinate system from the FK4-based B1950.0 system to the FK5-based J2000.0 system or to the International Celestial Reference System (ICRS). For more than 50 years, the definition of the Galactic coordinate system has remained unchanged from this IAU1958 version. On the basis of deep and all-sky catalogs, the position of the Galactic plane can be revised and updated definitions of the Galactic coordinate systems can be proposed. Aims. We re-determine the position of the Galactic plane based on modern large catalogs, such as the Two-Micron All-Sky Survey (2MASS) and the SPECFIND v2.0. This paper also aims to propose a possible definition of the optimal Galactic coordinate system by adopting the ICRS position of the Sgr A* at the Galactic center.
    [Show full text]
  • Unit 2 Basic Concepts of Positional Astronomy
    Basic Concepts of UNIT 2 BASIC CONCEPTS OF POSITIONAL Positional Astronomy ASTRONOMY Structure 2.1 Introduction Objectives 2.2 Celestial Sphere Geometry of a Sphere Spherical Triangle 2.3 Astronomical Coordinate Systems Geographical Coordinates Horizon System Equatorial System Diurnal Motion of the Stars Conversion of Coordinates 2.4 Measurement of Time Sidereal Time Apparent Solar Time Mean Solar Time Equation of Time Calendar 2.5 Summary 2.6 Terminal Questions 2.7 Solutions and Answers 2.1 INTRODUCTION In Unit 1, you have studied about the physical parameters and measurements that are relevant in astronomy and astrophysics. You have learnt that astronomical scales are very different from the ones that we encounter in our day-to-day lives. In astronomy, we are also interested in the motion and structure of planets, stars, galaxies and other celestial objects. For this purpose, it is essential that the position of these objects is precisely defined. In this unit, we describe some coordinate systems (horizon , local equatorial and universal equatorial ) used to define the positions of these objects. We also discuss the effect of Earth’s daily and annual motion on the positions of these objects. Finally, we explain how time is measured in astronomy. In the next unit, you will learn about various techniques and instruments used to make astronomical measurements. Study Guide In this unit, you will encounter the coordinate systems used in astronomy for the first time. In order to understand them, it would do you good to draw each diagram yourself. Try to visualise the fundamental circles, reference points and coordinates as you make each drawing.
    [Show full text]
  • Basic Principles of Celestial Navigation James A
    Basic principles of celestial navigation James A. Van Allena) Department of Physics and Astronomy, The University of Iowa, Iowa City, Iowa 52242 ͑Received 16 January 2004; accepted 10 June 2004͒ Celestial navigation is a technique for determining one’s geographic position by the observation of identified stars, identified planets, the Sun, and the Moon. This subject has a multitude of refinements which, although valuable to a professional navigator, tend to obscure the basic principles. I describe these principles, give an analytical solution of the classical two-star-sight problem without any dependence on prior knowledge of position, and include several examples. Some approximations and simplifications are made in the interest of clarity. © 2004 American Association of Physics Teachers. ͓DOI: 10.1119/1.1778391͔ I. INTRODUCTION longitude ⌳ is between 0° and 360°, although often it is convenient to take the longitude westward of the prime me- Celestial navigation is a technique for determining one’s ridian to be between 0° and Ϫ180°. The longitude of P also geographic position by the observation of identified stars, can be specified by the plane angle in the equatorial plane identified planets, the Sun, and the Moon. Its basic principles whose vertex is at O with one radial line through the point at are a combination of rudimentary astronomical knowledge 1–3 which the meridian through P intersects the equatorial plane and spherical trigonometry. and the other radial line through the point G at which the Anyone who has been on a ship that is remote from any prime meridian intersects the equatorial plane ͑see Fig.
    [Show full text]
  • The Lore of the Stars, for Amateur Campfire Sages
    obscure. Various claims have been made about Babylonian innovations and the similarity between the Greek zodiac and the stories, dating from the third millennium BCE, of Gilgamesh, a legendary Sumerian hero who encountered animals and characters similar to those of the zodiac. Some of the Babylonian constellations may have been popularized in the Greek world through the conquest of The Lore of the Stars, Alexander in the fourth century BCE. Alexander himself sent captured Babylonian texts back For Amateur Campfire Sages to Greece for his tutor Aristotle to interpret. Even earlier than this, Babylonian astronomy by Anders Hove would have been familiar to the Persians, who July 2002 occupied Greece several centuries before Alexander’s day. Although we may properly credit the Greeks with completing the Babylonian work, it is clear that the Babylonians did develop some of the symbols and constellations later adopted by the Greeks for their zodiac. Contrary to the story of the star-counter in Le Petit Prince, there aren’t unnumerable stars Cuneiform tablets using symbols similar to in the night sky, at least so far as we can see those used later for constellations may have with our own eyes. Only about a thousand are some relationship to astronomy, or they may visible. Almost all have names or Greek letter not. Far more tantalizing are the various designations as part of constellations that any- cuneiform tablets outlining astronomical one can learn to recognize. observations used by the Babylonians for Modern astronomers have divided the sky tracking the moon and developing a calendar. into 88 constellations, many of them fictitious— One of these is the MUL.APIN, which describes that is, they cover sky area, but contain no vis- the stars along the paths of the moon and ible stars.
    [Show full text]
  • The Sky Tonight
    MARCH POUTŪ-TE-RANGI HIGHLIGHTS Conjunction of Saturn and the Moon A conjunction is when two astronomical objects appear close in the sky as seen THE- SKY TONIGHT- - from Earth. The planets, along with the TE AHUA O TE RAKI I TENEI PO Sun and the Moon, appear to travel across Brightest Stars our sky roughly following a path called the At this time of the year, we can see the ecliptic. Each body travels at its own speed, three brightest stars in the night sky. sometimes entering ‘retrograde’ where they The brightness of a star, as seen from seem to move backwards for a period of time Earth, is measured as its apparent (though the backwards motion is only from magnitude. Pictured on the cover is our vantage point, and in fact the planets Sirius, the brightest star in our night sky, are still orbiting the Sun normally). which is 8.6 light-years away. Sometimes these celestial bodies will cross With an apparent magnitude of −1.46, paths along the ecliptic line and occupy the this star can be found in the constellation same space in our sky, though they are still Canis Major, high in the northern sky. millions of kilometres away from each other. Sirius is actually a binary star system, consisting of Sirius A which is twice the On March 19, the Moon and Saturn will be size of the Sun, and a faint white dwarf in conjunction. While the unaided eye will companion named Sirius B. only see Saturn as a bright star-like object (Saturn is the eighth brightest object in our Sirius is almost twice as bright as the night sky), a telescope can offer a spectacular second brightest star in the night sky, view of the ringed planet close to our Moon.
    [Show full text]
  • Review for Astronomy 5 Midterm and Final Midterm Covers First 70 Questions, Final Covers All 105
    Review for Astronomy 5 Midterm and Final Midterm covers first 70 questions, Final covers all 105. MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. Chapter 1 is covered by Q1-4; Ch. 2 Q5-13; Ch. 3 Q14-21; Ch. 4 Q22-28; Ch. 5 Q29-38; Ch. 6 Q39-43; Ch. 14 Q44-49; Ch. 15 Q50-60; Ch. 16 Q61-65; Ch. 17 Q66-73; Ch. 18 Q74-82; Ch. 19 Q83-87; Ch. 20 Q88-94; Ch. 21 Q95-96; Ch. 22 Q97-100; Ch. 23 Q101-105 1) Which of the following has your "address" in the correct order? A) you, Earth, solar system, Milky Way, Local Group, Local Supercluster B) you, Earth, solar system, Local Group, Milky Way, Local Supercluster C) you, Earth, solar system, Local Group, Local Supercluster, Milky Way D) you, Earth, Local Group, Local Supercluster, solar system, Milky Way E) you, Earth, solar system, Milky Way, Local Supercluster, Local Group 2) Roughly how many stars are in the Milky Way Galaxy? A) 10 billion B) 1 billion C) 100 million D) 100 trillion E) 100 billion 3) Which scientists played a major role in overturning the ancient idea of an Earth-centered universe, and about when? A) Aristotle and Copernicus; about 400 years ago B) Huygens and Newton; about 300 years ago C) Copernicus, Kepler, and Galileo; about 400 years ago D) Newton and Einstein; about 100 years ago E) Aristotle and Plato; about 2,000 years ago 4) What is an astronomical unit? A) the average distance from Earth to the Sun B) any basic unit used in astronomy C) the length of time it takes Earth to revolve around the Sun D) the average speed of Earth around the Sun E) the diameter of Earth's orbit around the Sun 5) Which of the following statements about the celestial sphere is not true? A) The celestial sphere does not exist physically.
    [Show full text]
  • Celestial Sphere, Solar Motion, Coordinates
    Celestial Sphere, Solar Motion, Coordinates Lecture Outline -- 1 Reading: Astronomy Notes sections 3.1 through 3.5 Vocabulary terms used: celestial poles⎯points on celestial sphere directly above geographic poles. celestial equator⎯circle around the sky directly above the Earth’s equator. zenith⎯point on the celestial sphere that is always straight overhead. meridian⎯circle around the sky that goes through celestial poles and the zenith point. Separates the daytime motions of the Sun into “a.m.” and “p.m.”. solar day⎯time between successive meridian crossings of the Sun. Our clocks are based on this. ecliptic⎯the apparent yearly path of the Sun through the stars on the celestial sphere. It is the projection of the Earth’s orbit around the Sun onto the celestial sphere. vernal equinox⎯specific moment in the year (on March 21) when the Sun is directly on the celestial equator, moving north of the celestial equator. autumnal equinox⎯specific moment in the year (on September 22) when the Sun is directly on the celestial equator, moving south of the celestial equator. season⎯approximately three-month period bounded by an equinox and a solstice. solstice⎯specific moment in the year when the Sun is farthest away from the celestial equator. The summer solstice is when the Sun gets closest to zenith at noon (on June 21 for U.S.). The winter solstice is when the Sun gets closest to the horizon at noon (on December 21 for U.S.). latitude⎯used to specify position on the Earth, it is the number of degrees north or south of the Earth’s equator.
    [Show full text]
  • The 1994 Arctic Ocean Section the First Major Scientific Crossing of the Arctic Ocean 1994 Arctic Ocean Section
    The 1994 Arctic Ocean Section The First Major Scientific Crossing of the Arctic Ocean 1994 Arctic Ocean Section — Historic Firsts — • First U.S. and Canadian surface ships to reach the North Pole • First surface ship crossing of the Arctic Ocean via the North Pole • First circumnavigation of North America and Greenland by surface ships • Northernmost rendezvous of three surface ships from the largest Arctic nations—Russia, the U.S. and Canada—at 89°41′N, 011°24′E on August 23, 1994 — Significant Scientific Findings — • Uncharted seamount discovered near 85°50′N, 166°00′E • Atlantic layer of the Arctic Ocean found to be 0.5–1°C warmer than prior to 1993 • Large eddy of cold fresh shelf water found centered at 1000 m on the periphery of the Makarov Basin • Sediment observed on the ice from the Chukchi Sea to the North Pole • Biological productivity estimated to be ten times greater than previous estimates • Active microbial community found, indicating that bacteria and protists are significant con- sumers of plant production • Mesozooplankton biomass found to increase with latitude • Benthic macrofauna found to be abundant, with populations higher in the Amerasia Basin than in the Eurasian Basin • Furthest north polar bear on record captured and tagged (84°15′N) • Demonstrated the presence of polar bears and ringed seals across the Arctic Basin • Sources of ice-rafted detritus in seafloor cores traced, suggesting that ocean–ice circulation in the western Canada Basin was toward Fram Strait during glacial intervals, contrary to the present
    [Show full text]
  • 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.
    [Show full text]
  • The Distant Early Warning (DEW) Line: a Bibliography and Documentary Resource List
    The Distant Early Warning (DEW) Line: A Bibliography and Documentary Resource List Prepared for the Arctic Institute of North America By: P. Whitney Lackenbauer, Ph.D. Matthew J. Farish, Ph.D. Jennifer Arthur-Lackenbauer, M.Sc. October 2005 © 2005 The Arctic Institute of North America ISBN 1-894788-01-X The DEW Line: Bibliography and Documentary Resource List 1 TABLE OF CONTENTS 1.0 PREFACE 2 2.0 BACKGROUND DOCUMENTS 3 2.1 Exchange of Notes (May 5, 1955) Between Canada and the United States Of America Governing the Establishment of a Distant Early Warning System in Canadian Territory.......................................................................................................... 3 2.2 The DEW Line Story in Brief (Western Electric Corporation, c.1960) ……………… 9 2.3 List of DEW Line Sites ……………………………………….…………………….... 16 3.0 ARCHIVAL COLLECTIONS 23 3.1 Rt. Hon. John George Diefenbaker Centre ……………………………………….…... 23 3.2 Library and Archives Canada …………………………………….…………………... 26 3.3 Department of National Defence, Directorate of History and Heritage ………………. 46 3.4 NWT Archives Council, Prince of Wales Northern Heritage Centre ……………….... 63 3.5 Yukon Territorial Archives, Whitehorse, YT ………………………………………… 79 3.6 Hudson Bay Company Archives ……………………………………………………... 88 3.7 Archives in the United States ……………………………………………………….… 89 4.0 PUBLISHED SOURCES 90 4.1 The Globe and Mail …………………………………………………………………………… 90 4.2 The Financial Post ………………………………………………………………………….…. 99 4.3 Other Print Media …………………………………………………………………..… 99 4.4 Contemporary Journal Articles ……………………………………………………..… 100 4.5 Government Publications …………………………………………………………….. 101 4.6 Corporate Histories ………………………………………………………………...... 103 4.7 Professional Journal Articles ………………………………………………………..… 104 4.8 Books ………………………………………………………………………………..… 106 4.9 Scholarly and Popular Articles ………………………………………………….……. 113 4.10 Environmental Issues and Cleanup: Technical Reports and Articles …………….…. 117 5.0 OTHER SOURCES 120 5.1 Theses and Dissertations ……………………………………………………………...
    [Show full text]
  • Field Astronomy Circumpolar Star at Elongation ➢ at Elongation a Circumpolar Star Is at the Farthest Position from the Pole Either in the East Or West
    Field Astronomy Circumpolar Star at Elongation ➢ At elongation a circumpolar star is at the farthest position from the pole either in the east or west. ➢ When the star is at elongation (East or West), which is perpendicular to the N-S line. ➢ Thus the ZMP is 90° as shown in the figure below. Distances between two points on the Earth’s surface ➢ Direct distance From the fig. above, in the spherical triangle APB P = Difference between longitudes of A and B BP = a = co-latitude of B = 90 – latitude of B AP = b = co-latitude of A = 90 – latitude of A Apply the cosine rule: cosp− cos a cos b CosP = sinab sin Find the value of p = AB Then the distance AB = arc length AB = ‘p’ in radians × radius of the earth ➢ Distance between two points on a parallel of latitude Let A and B be the two points on the parallel latitude θ. Let A’ and B’ be the corresponding points on the equator having the same longitudes (ФB, ФA). Thus from the ∆ O’AB AB = O’B(ФB - ФA) From the ∆ O’BO o O’B = OB’ sin (90- θ) Since =BOO ' 90 = R cos θ where R=Radius of the Earth. AB= (ФB - ФA) R cos θ where ФB , ФA are longitudes of B and A in radians. Practice Problems 1. Find the shortest distance between two places A and B on the earth for the data given below: Latitude of A = 14° N Longitude of A = 60°30‘E Latitude of B = 12° N Longitude of A = 65° E Find also direction of B from A.
    [Show full text]
  • Introduction to Astronomy Introduction
    IDP HOME CONTENTS NEXT: Introduction to Astronomy Introduction For many thousands of years, man has attempted to make sense of the sky by naming and grouping stars into recognisable patterns. At the turn of the twentieth century, Marc Aurel Stein, a Hungarian- born, British archaeologist uncovered the world’s oldest existing star chart in a Buddhist cave complex in Dunhuang, China. The chart, now known as the Dunhuang Star Atlas and probably dating from before AD 700, was just one of a large number of important manuscripts, printed documents and paintings which were found at the site, and which tell us much about social, religious and political issues in medieval China and Central Asia. But the Star Atlas – now held at the British Library in London – is also proving important for our current understanding of astronomical history due to the accuracy and detail it provides about the sky seen from China from such an early period. This resource aims to: Introduce the Dunhuang Star Atlas and explain its importance as a historical and scientific document Offer an introduction to astronomy and explain the place it has occupied in Chinese history and culture. Introduce the most important Chinese constellations and the myths associated with them. Look at the links between Chinese astronomy and astrology and explore the Chinese ‘zodiac’. Offer ideas for classroom activities and downloadable resources for teachers. Link to related websites and other sources of information. IDP HOME CONTENTS NEXT: Introduction to Astronomy file:///Users/bobi/PC/Documents_PC/wintext/chine/dunhuang/BLib... 1 sur 1 IDP HOME CONTENTS PREVIOUS: Introduction to this Resource NEXT: History of Astronomy in China Introduction to Astronomy For thousands of years, man has used the sky to help him find his way, tell the change of season and the time of day.
    [Show full text]