STARLAB® Native American Mythology Cylinder
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Get Outside What to Look for in the Summer Sky Your Hosts of the Summer Sky Are Three Bright Stars — Vega, Altair and Deneb
Get Outside What to Look for in the Summer Sky Your hosts of the summer sky are three bright stars — Vega, Altair and Deneb. Together they make up the Summer Triangle. Look for the triangle in the east on a June evening, moving NORTH to overhead as the season progresses. Polaris The Big Dipper Deneb Cygnus Vega Lyra Hercules Arcturus EaST West Summer Triangle Altair Aquila Sagittarius Antares Turn the map so Scorpius the direction you are facing is at the Teapot the bottom. south facebook.com/KidsCanBooks @KidsCanPress GET OUTSIDE Text © 2013 Jane Drake & Ann Love Illustrations © 2013 Heather Collins www.kidscanpress.com Get Outside Vega The Keystone The brightest star in the Between Vega and Arcturus, Summer Triangle, Vega is look for four stars in a wedge or The summer bluish white. It is in the keystone shape. This is the body solstice constellation Lyra, the Harp. of Hercules, the Strongman. His feet are to the north and Every day from late Altair his arms to the south, making December to June, the The second-brightest star in his figure kneel Sun rises and sets a little the triangle, Altair is white. upside down farther north along the Altair is in the constellation in the sky. horizon. But about June Aquila, the Eagle. 21, the Sun seems to stop Keystone moving north. It rises in Deneb the northeast and sets in The dimmest star of the the northwest, seemingly Summer Triangle, Deneb would in the same spots for be the brightest if it were not so Hercules several days. -
Summer Constellations
Night Sky 101: Summer Constellations The Summer Triangle Photo Credit: Smoky Mountain Astronomical Society The Summer Triangle is made up of three bright stars—Altair, in the constellation Aquila (the eagle), Deneb in Cygnus (the swan), and Vega Lyra (the lyre, or harp). Also called “The Northern Cross” or “The Backbone of the Milky Way,” Cygnus is a horizontal cross of five bright stars. In very dark skies, Cygnus helps viewers find the Milky Way. Albireo, the last star in Cygnus’s tail, is actually made up of two stars (a binary star). The separate stars can be seen with a 30 power telescope. The Ring Nebula, part of the constellation Lyra, can also be seen with this magnification. In Japanese mythology, Vega, the celestial princess and goddess, fell in love Altair. Her father did not approve of Altair, since he was a mortal. They were forbidden from seeing each other. The two lovers were placed in the sky, where they were separated by the Celestial River, repre- sented by the Milky Way. According to the legend, once a year, a bridge of magpies form, rep- resented by Cygnus, to reunite the lovers. Photo credit: Unknown Scorpius Also called Scorpio, Scorpius is one of the 12 Zodiac constellations, which are used in reading horoscopes. Scorpius represents those born during October 23 to November 21. Scorpio is easy to spot in the summer sky. It is made up of a long string bright stars, which are visible in most lights, especially Antares, because of its distinctly red color. Antares is about 850 times bigger than our sun and is a red giant. -
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: -
CONSTELLATION VULPECULA, the (LITTLE) FOX Vulpecula Is a Faint Constellation in the Northern Sky
CONSTELLATION VULPECULA, THE (LITTLE) FOX Vulpecula is a faint constellation in the northern sky. Its name is Latin for "little fox", although it is commonly known simply as the fox. It was identified in the seventeenth century, and is located in the middle of the northern Summer Triangle (an asterism consisting of the bright stars Deneb in Cygnus (the Swan), Vega in Lyra (the Lyre) and Altair in Aquila (the Eagle). Vulpecula was introduced by the Polish astronomer Johannes Hevelius in the late 17th century. It is not associated with any figure in mythology. Hevelius originally named the constellation Vulpecula cum ansere, or Vulpecula et Anser, which means the little fox with the goose. The constellation was depicted as a fox holding a goose in its jaws. The stars were later separated to form two constellations, Anser and Vulpecula, and then merged back together into the present-day Vulpecula constellation. The goose was left out of the constellation’s name, but instead the brightest star, Alpha Vulpeculae, carries the name Anser. It is one of the seven constellations created by Hevelius. The fox and the goose shown as ‘Vulpec. & Anser’ on the Atlas Coelestis of John Flamsteed (1729). The Fox and Goose is a traditional pub name in Britain. STARS There are no stars brighter than 4th magnitude in this constellation. The brightest star is: Alpha Vulpeculae, a magnitude 4.44m red giant at a distance of 297 light-years. The star is an optical binary (separation of 413.7") that can be split using binoculars. The star also carries the traditional name Anser, which refers to the goose the little fox holds in its jaws. -
CCAS Newsletter-July 2021.Docx
Celestial Observer CCAS member Frank Widmann shot this image of Markarian’s Chain. Located in the constellation Virgo and visible during the Summer months, this string of galaxies forms part of the Virgo Cluster which contains over 1,300 galaxies. ____________________________________________________________ Next Star Gazing: ONLINE! Free Class: How to Use Saturday, July 10th at 7pm PDT Binoculars for Astronomy CCAS President Aurora Lipper, On Demand! and astronomers Kent Wallace Join Aurora and Brian as they go and Brian Cox will be taking you over what you need to know to get on a virtual tour of the July night started touring the night sky with a sky, so you can stargaze right from pair of binoculars! home! Connect here: More info here: CentralCoastAstronomy.org/stargaze CentralCoastAstronomy.org/binoculars_6-22-21 Next Stargazing: ONLINE! Invite friends!! Saturday, July 10th at 7pm PDT On July 10th, CCAS President Aurora Lipper, along with amateur astronomers Kent Wallace and Brian Cox will premier a tour of the July Summer sky. You’ll learn about objects visible naked-eye, through binoculars, and through a telescope. Then, using the tools you learn during the video, you’ll be able to stargaze from the comfort of your own home! Invite all your friends! Anyone with the link can view our free online stargazing session. All that’s needed is an internet connection. Join the stream using any tablet, personal computer, or YouTube enabled TV. After the premier, the video will be available on demand on our YouTube channel. Check our website for all the details: CentralCoastAstronomy.org/stargaze Central Coast Astronomy CentralCoastAstronomy.org Summer Triangle Corner: Vega, Deneb & Altair by NASA Night Sky Network nightsky.jpl.nasa.gov Can you spot Vega, Deneb & Altair? You may need to look straight up to find them, especially if observing late in the evening in the Summer months. -
Educator's Guide: Orion
Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations. -
JRASC-2007-04-Hr.Pdf
Publications and Products of April / avril 2007 Volume/volume 101 Number/numéro 2 [723] The Royal Astronomical Society of Canada Observer’s Calendar — 2007 The award-winning RASC Observer's Calendar is your annual guide Created by the Royal Astronomical Society of Canada and richly illustrated by photographs from leading amateur astronomers, the calendar pages are packed with detailed information including major lunar and planetary conjunctions, The Journal of the Royal Astronomical Society of Canada Le Journal de la Société royale d’astronomie du Canada meteor showers, eclipses, lunar phases, and daily Moonrise and Moonset times. Canadian and U.S. holidays are highlighted. Perfect for home, office, or observatory. Individual Order Prices: $16.95 Cdn/ $13.95 US RASC members receive a $3.00 discount Shipping and handling not included. The Beginner’s Observing Guide Extensively revised and now in its fifth edition, The Beginner’s Observing Guide is for a variety of observers, from the beginner with no experience to the intermediate who would appreciate the clear, helpful guidance here available on an expanded variety of topics: constellations, bright stars, the motions of the heavens, lunar features, the aurora, and the zodiacal light. New sections include: lunar and planetary data through 2010, variable-star observing, telescope information, beginning astrophotography, a non-technical glossary of astronomical terms, and directions for building a properly scaled model of the solar system. Written by astronomy author and educator, Leo Enright; 200 pages, 6 colour star maps, 16 photographs, otabinding. Price: $19.95 plus shipping & handling. Skyways: Astronomy Handbook for Teachers Teaching Astronomy? Skyways Makes it Easy! Written by a Canadian for Canadian teachers and astronomy educators, Skyways is Canadian curriculum-specific; pre-tested by Canadian teachers; hands-on; interactive; geared for upper elementary, middle school, and junior-high grades; fun and easy to use; cost-effective. -
Molecular Gas Content of Galaxies in the Hydra-Centaurus Supercluster
MOLECULAR GAS CONTENT OF GALAXIES IN THE HYDRA-CENTAURUS SUPERCLUSTER W.K. Huchtmeier ™ ** <$ '"" & ^ O Max-Planck-Institut fiir Radioastronomie Auf dem Hugel 69 , 5300 Bonn 1 , W. Germany • Abstract A survey of bright spiral galaxies in the Hydra-Centaurus supercluster for the CO(l-O) transition at 115 GHz was performed with the 15m Swedish-ESO submillimeter telescope (SEST). A total of 30 galaxies have been detected in the CO(l-O) transition out of 47 observed, which is a detection rate over 60%. Global physical parameters of these galaxies derived from optical, CO, HI, and IR measurements compare very well with properties of galaxies in the Virgo cluster. The Hydra I cluster (Abell 1060) is one of the nearest clusters and very similar to the Virgo cluster in many global parameters like type, population, size, and shape. Both clusters have comparable velocity dispersions (i.e. total mass) and are spiral rich. Hydra is well isolated in velocity space and appears more circular (Kwast 1966), and might be dynamically more relaxed, although the center may contain significant substructures (Fitchett and Meritt 1988) or projected foreground groups. Both clusters contain low luminosity central X-ray sources. We assume a distance of 68.4 Mpc for Hydra I in order to allow direct comparison with some (nearly) complete galaxy samples. The Centaurus cluster provides a valuable contrast to Virgo and Coma. It is intermediate in distance and in galaxy population type with a relatively well defined SO-dominated core and an extensive S-rich halo. Its richness class in the Abell scale is 1 or 2 which is richer than Virgo and poorer than Coma. -
Sky & Telescope
Eclipse from the See Sirius B: The Nearest Spot the Other EDGE OF SPACE p. 66 WHITE DWARF p. 30 BLUE PLANETS p. 50 THE ESSENTIAL GUIDE TO ASTRONOMY What Put the Bang in the Big Bang p. 22 Telescope Alignment Made Easy p. 64 Explore the Nearby Milky Way p. 32 How to Draw the Moon p. 54 OCTOBER 2013 Cosmic Gold Rush Racing to fi nd exploding stars p. 16 Visit SkyandTelescope.com Download Our Free SkyWeek App FC Oct2013_J.indd 1 8/2/13 2:47 PM “I can’t say when I’ve ever enjoyed owning anything more than my Tele Vue products.” — R.C, TX Tele Vue-76 Why Are Tele Vue Products So Good? Because We Aim to Please! For over 30-years we’ve created eyepieces and telescopes focusing on a singular target; deliver a cus- tomer experience “...even better than you imagined.” Eyepieces with wider, sharper fields of view so you see more at any power, Rich-field refractors with APO performance so you can enjoy Andromeda as well as Jupiter in all their splendor. Tele Vue products complement each other to pro- vide an observing experience as exquisite in performance as it is enjoyable and effortless. And how do we score with our valued customers? Judging by superlatives like: “in- credible, truly amazing, awesome, fantastic, beautiful, work of art, exceeded expectations by a mile, best quality available, WOW, outstanding, uncom- NP101 f/5.4 APO refractor promised, perfect, gorgeous” etc., BULLSEYE! See these superlatives in with 110° Ethos-SX eye- piece shown on their original warranty card context at TeleVue.com/comments. -
A Collection of Curricula for the STARLAB Greek Mythology Cylinder
A Collection of Curricula for the STARLAB Greek Mythology Cylinder Including: A Look at the Greek Mythology Cylinder Three Activities: Constellation Creations, Create a Myth, I'm Getting Dizzy by Gary D. Kratzer ©2008 by Science First/STARLAB, 95 Botsford Place, Buffalo, NY 14216. www.starlab.com. All rights reserved. Curriculum Guide Contents A Look at the Greek Mythology Cylinder ...................3 Leo, the Lion .....................................................9 Introduction ......................................................3 Lepus, the Hare .................................................9 Andromeda ......................................................3 Libra, the Scales ................................................9 Aquarius ..........................................................3 Lyra, the Lyre ...................................................10 Aquila, the Eagle ..............................................3 Ophuichus, Serpent Holder ..............................10 Aries, the Ram ..................................................3 Orion, the Hunter ............................................10 Auriga .............................................................4 Pegasus, the Winged Horse..............................11 Bootes ..............................................................4 Perseus, the Champion .....................................11 Cancer, the Crab ..............................................4 Phoenix ..........................................................11 Canis Major, the Big Dog -
SUMMER SPECTACLE? Take in Wyoming’S Ultimate Drive-In Theater
WANT TO VIEW A GREAT SUMMER SPECTACLE? Take in Wyoming’s ultimate drive-in theater Travis Laurence You might notice dark regions ow is a wonderful time to stay within the band of light of the Milky Nup late, go outside, and see Way. These are called dark nebula some of the amazing summer stars and are clouds of interstellar dust. and constellations. Astronomers use the term “interstel- Something that might catch your lar dust” to describe tiny particles wonder is the bright band of light we of matter found throughout space. call the Milky Way. The farther you These dust clouds may be light-years can get from city lights, the more in size and contain material that obvious this pale, diffuse band be- some day may be formed into stars comes. You are looking at part of the and planets. They absorb light from galaxy in which we live. those millions of unseen stars behind Our galaxy is a massive collec- them. tion of 200 billion to 400 billion stars. In effect, you can get a sense of All of the stars you see in the night depth if you see a star within a dark sky are part of the Milky Way. About nebula. The star is in front of the 3,000 of these stars can be seen on a cloud, and behind the cloud is light clear night. That is a lot of stars! from the Milky Way. Stars within the But what we see with our eyes is constellation Cygnus (described be- only a tiny fraction of the stars within low) are a great example of this. -
Large Peculiar Velocities in the Hydra Centaurus Supercluster
LARGE PECULIAR VELOCITIES IN THE HYDRA CENTAURUS SUPERCLUSTER M. Aaronson1*, G.D. Bothun2, K.G. Budge3, JA. Dawe4, R.J. Dickens5, RJ. Hall6, J.R. Lucey7, J.R. Mould3, J.D. Murray6, R.A. Schommer8, A.E. Wright6. 1 Steward Observatory, University of Arizona 2 University of Michigan 3 California Institute of Technology 4 Australian National University 5Rutherford Appleton Laboratory 6 Australian National Radio Astronomy Observatory 7Anglo Australian Observatory 8 Rutgers University ABSTRACT Six clusters forming part of the Hydra-Cen Supercluster and its ex- tension on the opposite side of the galactic plane are under study at 21 cm with the Parkes radiotélescope. The infrared Tully-Fisher relation is used to determine the relative distances of the clusters. These clusters exhibit significant and generally positive peculiar velocities ranging from essentially zero for the Hydra cluster to as much as 1000 km/sec for the Pavo and Centaurus clusters. An upper limit of 500 km/sec was previously found in the study of clusters accessible from Arecibo. Data collection is not yet complete, however, and is further subject to unstud- ied systematic errors due to present reliance on photographic galaxy diameters. Nevertheless, these preliminary results support the notion of a large scale (and pre- sumably gravit at ionally) disturbed velocity field in the second and third quadrants of the supergalactic plane. 1. INTRODUCTION Comparison of the ratios of distances of galaxies with the ratios of their recession velocities allows one to learn something about the "noise" in the Hubble flow on various scales. One is subject to the limitation, however, that distance indicators are imprecise, and the 0.4 mag scatter in the infrared Tully-Fisher (IRTF) relation translates to an uncertainty of 1000 km/sec in an individual galaxy at cz = 5000 km/sec.