DOCSLIB.ORG

Environmental Science

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Environmental Science Precession of Earth: Spinning on the Axis Environmental Science Name: ____________________________________________Period:__________ Date: ___________ Essential Question: Why is earth’s axis wobbling? Een 1.1.1 Instructions: Study the selection and answer the questions. Just like a toy top that wobbles before it falls, the Earth wobbles as it rotates on its axis, the imaginary line that extends through the poles. This wobbling motion is due to the slight bulge at the equator. If you traced the Earth's axis out into space, you would see the extension of the axis slowly tracing a cone shape. The wobble is very slow; it takes the Earth 26,000 years to trace one complete conical shape. This wobbling motion of Earth on its axis is called precession. Because of precession, Polaris and Vega alternate as the North Star every 13,000 years. Polaris: The Current North Star Today the Earth's axis points within one degree of Polaris, the brightest star in the constellation Ursa Minor (also called the Little Bear or the Little Dipper). Polaris appears to be in a fixed position in the sky throughout the year. All other stars and constellations seem to revolve around the North Star. Why isn't the North Star Fixed? Over the course of time, the North Star changes. Right now Polaris is within one degree of true north, but at other times the North Star has been and will again be Thuban (the brightest star in the constellation Draco), Vega (the brightest star in the constellation Lyra), and Alpha Cephei (the brightest star in the constellation Cepheus). The North Star changes over time because the direction of the earth's axis changes slowly over time. Since by definition the North Star is the star most closely aligned with the earth's axis, as the axis moves the nearest star changes too. This type of axis movement is similar to that of a spinning top. As the top slows, the axis of rotation changes as the top draws out each rotation; that is to say that the stem of the top itself traces out a circular pattern rather than pointing at a single spot or staying mostly still. If you draw an imaginary line of the earth's axis and continue it up to the sky, it will make a similar path. This type of axis rotation is called precession. In the case of the earth, precession is caused by the gravitational pull of the sun and the moon. The earth's axis makes one complete rotation over the course of approximately 26,000 years. If you trace the path of the axis in the sky, you will find that Polaris, Vega, Thuban, and Alpha Cephei all fall on or very close to it. So when the earth's axis is at a point on the path near Vega, Vega becomes the North Star while Thuban is the North Star when the axis is near it on the path. Five thousand years ago, Thuban was the North Star. Five thousand years from now, the North Star will be Alpha Cephei. Seven thousand years after that, it will be Vega. Nine thousand years after that, Thuban will be the North Star again. At these dates, the various stars will be at the closest to absolute north. For some time before, the relevant star will be approaching due north and it will be receding for some time after the time listed. In these interim times, the North Star is whichever star is closest to north. Answer the following questions 1. What is earth’s axis? ______________________________________________________________________________ ______________________________________________________________________________ 2. What is precession? ______________________________________________________________________________ ______________________________________________________________________________ 3. How long does it take for earth’s axis to wobble into a complete conical shape? ______________________________________________________________________________ ______________________________________________________________________________ 4. What two stars alternate every 13,000 years as earth’s northern star? ______________________________________________________________________________ ______________________________________________________________________________ 5. What is earth’s current northern star? ______________________________________________________________________________ ______________________________________________________________________________ 6. What is the brightest star in the constellation Ursa Minor? ______________________________________________________________________________ ______________________________________________________________________________ 7. What is the brightest star in the constellation Draco? ______________________________________________________________________________ ______________________________________________________________________________ 8. What is the brightest star in the constellation Lyra? ______________________________________________________________________________ ______________________________________________________________________________ 9. What is the brightest star in the constellation Cepheus? ______________________________________________________________________________ ______________________________________________________________________________ 10. Why do earth’s northern star change over time? ______________________________________________________________________________ ______________________________________________________________________________ 11. What is precession and what causes it? ______________________________________________________________________________ ______________________________________________________________________________ ______________________________________________________________________________ 12. What are the four stars that can become earth’s northern star? ______________________________________________________________________________ ______________________________________________________________________________ 13. What was earth’s northern star before Polaris? ______________________________________________________________________________ ______________________________________________________________________________ 14. What will be earth’s northern star five thousand years from now? ______________________________________________________________________________ ______________________________________________________________________________ 15. What will be earth’s northern star twelve thousand years from now? ______________________________________________________________________________ ______________________________________________________________________________ 16. Which do we consider as our northern star and why is our northern star changing? ______________________________________________________________________________ ______________________________________________________________________________ http://www.education.com/reference/article/precession-earth/ http://www.essortment.com/north-star-61725.html Precession and Nutation Environmental Science Name: ____________________________________________Period:__________ Date: ___________ Essential Question: Why is Polaris fixed on its position throughout the year? What is the difference between precession and nutation? Instructions: Encircle and label the constellations where Polaris, Vega, Thuban, and Alpha Cephei are found. Polaris, the brightest star in the constellation Ursa Minor (also called the Little Bear or the Little Dipper). Polaris appears to be in a fixed position in the sky throughout the year. All other stars and constellations seem to revolve around the North Star. Thuban (the brightest star in the constellation Draco), Vega (the brightest star in the constellation Lyra), and Alpha Cephei (the brightest star in the constellation Cepheus). http://www.msnucleus.org/membership/html/jh/earth/stars/lesson4/stars04c.html Come up with your Hypothesis: How come Polaris seems to be stationary in the sky throughout the year while the others stars in their constellations seem to revolve around it? Hypothesis: _____________________________________________________________________________________ _____________________________________________________________________________________ _____________________________________________________________________________________ Try this out! 1. Stand directly below a smoke alarm or anything that you can consider as your northern star. Directly above you is your north, your right side is your east, down is south, and your left side is your west. 2. Look around and observe anything that you can consider as markers ( like ceiling fan, light bulb, air vent, spot on the ceiling etc. ) and consider them as the other stars. 3. Slowly turn around 360 degrees from west to east direction while looking at your northern star. Did your northern star move to another direction in reference to your position ( N-E-S-W)? Explain. _______________________________________________________________ _______________________________________________________________ _______________________________________________________________ 4. Again, slowly turn around 360 degrees from West to East direction while looking at your other star markers. Did your other stars move to another direction in reference to your position? ( N-E-S-W)? Explain. __________________________________________________________________ __________________________________________________________________ __________________________________________________________________ 5. Why is the northern star stationary and the rest of the stars seemingly rotating around it? Explain. _______________________________________________________________
Load more

Recommended publications
  • THUBAN the Star Thuban in the Constellation Draco (The Dragon) Was the North Pole Star Some 5,000 Years Ago, When the Egyptians Were Building the Pyramids
    STAR OF THE WEEK: THUBAN The star Thuban in the constellation Draco (the Dragon) was the North Pole Star some 5,000 years ago, when the Egyptians were building the pyramids. Thuban is not a particularly bright star. At magnitude 3.7 and known as alpha draconis it is not even the brightest star in its constellation. What is Thuban’s connection with the pyramids of Egypt? Among the many mysteries surrounding Egypt’s pyramids are the so-called “air shafts” in the Great Pyramid of Giza. These narrow passageways were once thought to serve for ventilation as the The Great Pyramid of Giza, an enduring monument of ancient pyramids were being built. In the 1960s, though, Egypt. Egyptologists believe that it was built as a tomb for fourth dynasty Egyptian Pharaoh Khufu around 2560 BC the air shafts were recognized as being aligned with stars or areas of sky as the sky appeared for the pyramids’ builders 5,000 years ago. To this day, the purpose of all these passageways inside the Great Pyramid isn’t clear, although some might have been connected to rituals associated with the king’s ascension to the heavens. Whatever their purpose, the Great Pyramid of Giza reveals that its builders knew the starry skies intimately. They surely knew Thuban was their Pole Star, the point around which the heavens appeared to turn. Various sources claim that Thuban almost exactly pinpointed the position of the north celestial pole in the This diagram shows the so-called air shafts in the Great year 2787 B.C.
    [Show full text]
  • The Faces of Stars
    Resolving the Faces of Stars estled among the venerable telescope domes on Mount Wilson, a mile-high peak overlooking Los Angeles, is the highest- resolution optical instrument in the world. Inside several hundred meters of evacuated pipe, beams of star- light from six 1-meter (39-inch) telescopes converge on a central fa- cility to be matched up light wave for light wave. The result allows measurements of details as small as a thousandth of an arcsecond wide — the apparent size of a penny in Los Angeles seen from At- lanta. Georgia State University’s Center for High Angular Resolu- tion Astronomy (CHARA) built and runs the instrument under the directorship of Harold McAlister. The CHARA Array is currently Nthe largest of several new installations around the world applying 21st-century technology to an old idea: optical interferometry. The concept of interferometry predates photographic fi lm, but astronomers didn’t really put it into practice until the early 1920s (see “Milestones in Optical Interferometry,” page 44). Now, nearly a century later, technology is catching up with theory. Astronomers are using a new breed of giant interferometers to measure some of ERIC SIMISON / SEA WEST ENTERPRISES SIMISON / SEA WEST ERIC the most diffi cult fundamental parameters in stellar astrophysics, in By David H. Berger, The CHARA Array particular the sizes and shapes of stars (S&T: May 2003, page 30). is one of several These parameters are most easily studied for the nearest and Jason P. Aufdenberg, facilities on Mount brightest stars, those dear to skygazers’ hearts. The CHARA Array and Nils H.
    [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]
  • Introduction to Astronomy from Darkness to Blazing Glory
    Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice:
    [Show full text]
  • Dhruva the Ancient Indian Pole Star: Fixity, Rotation and Movement
    Indian Journal of History of Science, 46.1 (2011) 23-39 DHRUVA THE ANCIENT INDIAN POLE STAR: FIXITY, ROTATION AND MOVEMENT R N IYENGAR* (Received 1 February 2010; revised 24 January 2011) Ancient historical layers of Hindu astronomy are explored in this paper with the help of the Purân.as and the Vedic texts. It is found that Dhruva as described in the Brahmân.d.a and the Vis.n.u purân.a was a star located at the tail of a celestial animal figure known as the Úiúumâra or the Dolphin. This constellation, which can be easily recognized as the modern Draco, is described vividly and accurately in the ancient texts. The body parts of the animal figure are made of fourteen stars, the last four of which including Dhruva on the tail are said to never set. The Taittirîya Âran.yaka text of the Kr.s.n.a-yajurveda school which is more ancient than the above Purân.as describes this constellation by the same name and lists fourteen stars the last among them being named Abhaya, equated with Dhruva, at the tail end of the figure. The accented Vedic text Ekâgni-kân.d.a of the same school recommends observation of Dhruva the fixed Pole Star during marriages. The above Vedic texts are more ancient than the Gr.hya-sûtra literature which was the basis for indologists to deny the existence of a fixed North Star during the Vedic period. However the various Purân.ic and Vedic textual evidence studied here for the first time, leads to the conclusion that in India for the Yajurvedic people Thuban (α-Draconis) was Dhruva the Pole Star c 2800 BC.
    [Show full text]
  • Careful Measurements Reveal That the Earth Has a Slight Difference in Its Dimensions
    Careful measurements reveal that the earth has a slight difference in its dimensions EUREKA!!! COPY EARTH’S SHAPE? •The shape of the earth is technically called an OBLATE SPHEROID: •Slightly flattened at the poles and bulging in the middle(equator) EXAGGERATED PICTURE! COPY BUT….. IT LOOKS PERFECTLY ROUND TO US! OBLATE SPHEROID check this out!!! IT’S DRILL TIME!!!!! Polar Equatorial Circumference Circumference Polar Equatorial diameter Diameter Actual Numbers • Polar diameter • Equatorial diameter = 12,714km = 12,757km (7882mi) (7909mi) • Polar • Equatorial Circumference Circumference = 40,076km = 40,006km (24,847mi) (24,804mi) MODEL COPY •A MODEL is a way of representing the properties of some object – (Drawing, diagram, graph, chart, photo, table) Evidence for the Earth’s Shape: • 1. Altitude of Polaris • 2. Gravity Measurements • 3. “Sinking” ships • 4. Lunar Eclipses * POLARIS= NORTH STAR NORTH POLE Earth’s AXIS of Rotation Geographic Poles SOUTH POLE WHAT ABOUT THE SOUTH POLE? • At the present time, Polaris is the pole star in the northern direction. Sigma Octantis is the closest star to the south celestial pole, but it is too faint to serve as a useful pole star. The Southern Cross constellation functions as an approximate southern pole constellation. Some people travel to the equator in order to be able to see both Polaris and the Southern cross. Pointer Stars! POLARIS Polaris is found in the little dipper!! COPY COPY Detailed Evidence for the Earth’s Shape COPY 1. Altitude of Polaris: The altitude is the ANGLE above the horizon Polaris is directly over the North Pole (Fixed Star) Your LATITUDE (degrees North or South of equator) equals ALTITUDE of POLARIS! 90O 30O 0O Person standing at 30ON POLARIS 90O 45O 0O 2.
    [Show full text]
  • Wynyard Planetarium & Observatory a Autumn Observing Notes
    Wynyard Planetarium & Observatory A Autumn Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn Tour of the Sky with the Naked Eye CASSIOPEIA Look for the ‘W’ 4 shape 3 Polaris URSA MINOR Notice how the constellations swing around Polaris during the night Pherkad Kochab Is Kochab orange compared 2 to Polaris? Pointers Is Dubhe Dubhe yellowish compared to Merak? 1 Merak THE PLOUGH Figure 1: Sketch of the northern sky in autumn. © Rob Peeling, CaDAS, 2007 version 1.2 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. Close to the horizon is a group of stars like the outline of a saucepan with the handle stretching to your left. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The two right-hand stars are called the Pointers. Can you tell that the higher of the two, Dubhe is slightly yellowish compared to the lower, Merak? Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white- hot. 2. Use the Pointers to guide you upwards to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the left are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris.
    [Show full text]
  • Map and Compass
    UE CG 039-089 2018_UE CG 039-089 2018 2018-08-29 9:57 AM Page 56 MAP The north magnetic pole is not the same as the geographic North Pole, also known as AND COMPASS true north, which is the northern end of the axis around which the earth spins. In fact, the north magnetic pole currently lies Background Information approximately 800 mi (1300 km) south of the geographic North Pole, in northern A compass is an instrument that people use Canada. And because the north magnetic to find a direction in relation to the earth as pole migrates at 6.6 mi (10 km) per year, its a whole. The magnetic needle in the location is constantly changing. compass, which is the freely moving needle in the compass that has a red end, points The meridians of longitude on maps and north. More specifically, this needle points globes are based upon the geographic to the north magnetic pole, the northern North Pole rather than the north magnetic end of the earth’s magnetic field, which pole. This means that magnetic north, the can be imagined as lines of magnetism that direction that a compass indicates as north, leave the south magnetic pole, flow north is not the same direction as maps indicate around the earth, and then enter the north for north. Magnetic declination, the magnetic pole. difference in the angle between magnetic north and true north must, therefore, be Any magnetized object, an object with two taken into account when navigating with a oppositely charged ends, such as a magnet map and a compass.
    [Show full text]
  • Some Guidelines for Effective Field-Use of the GPS Unit
    PRBO Conservation Science 4990 Shoreline Highway Stinson Beach, CA 94970 415-868-1221 www.prbo.org Guidelines for Field Use of Garmin GPS Units GPS Checklist: Copy an updated version of the master "allpc" shapefile and other digital basemaps, including topo quads and aerial photos, from the GIS server (V: drive) before the field season starts. Know what coordinate system (e.g., UTM, zone 10) and datum (e.g., NAD83) your project uses. The PRBO default is UTM, WGS84 (same as NAD83). In the UTM coordinate system, your zone depends on where you are (see map). Download your GPS coordinates daily, using GPS Utility (www.gpsu.co.uk/) or Waypoint+ (www.tapr.org/~kh2z/Waypoint/) shareware. It is not uncommon for Garmin units to die in the field. You will need a PC Interface cable to download your data and a registration key for GPS Utility. If you are unable to download, record your coordinates by hand in the field. Always carry extra batteries, especially if you’re not planning to revisit the site, and turn off your GPS unit when not in use to avoid draining the internal lithium battery. Contact Garmin (www.garmin.com) for replacement or repair under warranty if your unit dies. UTM Zones Submit copies of your GPS coordinate files to the GIS lab at the end of the field season for archiving and general mapping purposes. In the Field GPS Unit Setup Before taking waypoints in the field, the GPS navigation display should be set up to match the coordinate system, horizontal datum, and units used at a particular field project’s location.
    [Show full text]
  • Proceedings of SPIE - the International Society for Optical Engineering
    Review and scientific prospects of high- contrast optical stellar interferometry Item Type Proceedings; text Authors Defrère, D.; Absil, O.; Berger, J.-P.; Danchi, W.C.; Dandumont, C.; Eisenhauer, F.; Ertel, S.; Gardner, T.; Glauser, A.; Hinz, P.; Ireland, M.; Kammerer, J.; Kraus, S.; Labadie, L.; Lacour, S.; Laugier, R.; Loicq, J.; Martin, G.; Martinache, F.; Martinod, M.A.; Mennesson, B.; Monnier, J.; Norris, B.; Nowak, M.; Pott, J.U.; Quanz, S.P.; Serabyn, E.; Stone, J.; Tuthill, P.; Woillez, J. Citation Defrère, D., Absil, O., Berger, J. P., Danchi, W. C., Dandumont, C., Eisenhauer, F., ... & Woillez, J. (2020, December). Review and scientific prospects of high-contrast optical stellar interferometry. In Optical and Infrared Interferometry and Imaging VII (Vol. 11446, p. 114461J). International Society for Optics and Photonics. DOI 10.1117/12.2561505 Publisher SPIE Journal Proceedings of SPIE - The International Society for Optical Engineering Rights Copyright © 2020 SPIE. Download date 26/09/2021 05:12:08 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/660530 PROCEEDINGS OF SPIE SPIEDigitalLibrary.org/conference-proceedings-of-spie Review and scientific prospects of high-contrast optical stellar interferometry Defrère, D., Absil, O., Berger, J.-P., Danchi, W. C., Dandumont, C., et al. D. Defrère, O. Absil, J.-P. Berger, W. C. Danchi, C. Dandumont, F. Eisenhauer, S. Ertel, T. Gardner, A. Glauser, P. Hinz, M. Ireland, J. Kammerer, S. Kraus, L. Labadie, S. Lacour, R. Laugier, J. Loicq, G. Martin, F. Martinache, M. A. Martinod, B. Mennesson, J. Monnier, B. Norris, M.
    [Show full text]
  • Find Location from Grid Reference
    Find Location From Grid Reference Piney and desiccant Jean-Luc understocks almost florally, though Milton ruptures his wartweeds intermarried. Is Emmery Nikkialways focalises superjacent shipshape. and grimiest when individuating some stewpots very round-the-clock and indefatigably? Chalcographic This method expresses the human development in conjunction with apple blogs rolling and from grid reference on a map is directly at intervals along the play store you want to provide a private draft You find location, grid reference system of locating and longitude are located in grids on topographic maps. If you entertain an express map to measure story, Northing followed by Easting. Apple blogs rolling and the Internet safe. Give complete coordinate RIGHT, B, grid reference or latitude and longitude of locations. Sign arm to our Newsletter. The satellite map with the marker is shown alongside an equivalent Ordnance Survey map. If you work with MGRS coordinates, and that the scale is right side up. The layer you selected must be of point geometry. This earthquake has cloud been published or shared. Latitude can have done same numerical value north go south hit the equator, you can use the breakthrough To XY tool. Upload multiple images at once. What is high pressure? To enable light to better morning or bridge the location of features on total scale maps, we promise our postcode data quarterly, country grids etc. Click a the hand, interpret the images of the Megalong Valley below, unauthorized and shall goods be used. Google Earth starting point over Lawrence, stationary media panel. Perhaps you find. Two simple methods using a poise of so are described below.
    [Show full text]
  • STUDENT PAGE CONSTELLATION/STAR Big Dipper/Polaris CROW the Seven Bulls BLACKFEET Fixed Star GREEK Ursa Minor JAPANESE the One S
    STUDENT PAGE Astronomy Lesson 1: One Sky, Many Stories CONSTELLATION/STAR JAPANESE GREEK BLACKFEET CROW Big Dipper/Polaris The One Star Ursa Fixed The Seven & Big Dipper Minor Star Bulls 48 constellations in his famous book “Almagest”. These CONSTELLATIONS are called the “Ptolemaic constellations,” and most of them survive to this day. The history of the constellations is ancient; many were likely created by the Babylonian, Egyptian and Assyrian There are 88 official constellations recognized by the peoples. These constellations would have moved through International Astronomical Union. Only the official the regions via trade, and eventually they made their way boundaries of these constellations are determined; there into Greece, where they were assimilated into the culture is no official line drawing that makes up the shape of any and mythology. In the second century, Ptolemy organized constellation. Image courtesy wikihow ONE SKY, MANY STORIES 46 | ASTRONOMY STUDENT PAGE Astronomy Lesson 1: One Sky, Many Stories Image courtesy Wikipedia Star chart, Kitora Tomb, Asuka, Japan (7th century) In 1998, a star map was discovered in the Kitora Tomb Cultures all over the world have created star stories in the Asuka village in Japan. Dating back to the late based on constellations to pass traditions and knowledge seventh, early eighth century, this star chart is the oldest on to the next generation. Each culture had different existing map of its kind in the world. It features 68 names and stories for the Sun and Moon, visible planets, constellations and the movement of celestial objects is stars, and star groups. These stories are told at night and represented by the three concentric circles in the chart.
    [Show full text]