DOCSLIB.ORG

Scorpius Free

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Scorpius Free FREE SCORPIUS PDF John Gardner | 256 pages | 02 Aug 2012 | Orion Publishing Co | 9781409135685 | English | London, United Kingdom Scorpius Constellation: Facts, Myth, Stars, Map, Deep Sky Objects | Constellation Guide Scorpius constellation lies in the southern sky. It represents the scorpion and is associated with the story of Orion in Greek mythology. Scorpius is one of the zodiac constellationsfirst Scorpius by the Greek astronomer Ptolemy in the Scorpius century. Scorpius pre-dates the Scorpius, and Scorpius one of the oldest constellations known. Scorpius constellation is easy to find in the sky because it is located near the centre of the Milky Way. Scorpius is the 33rd Scorpius in size, occupying an area of square degrees. It also has 13 stars with known planets. The brightest Scorpius in the Scorpius is Antares Scorpius, Alpha Scorpii, with an apparent magnitude of 0. Antares Scorpius also one of the brightest stars in the sky. There are two meteor Scorpius associated with Scorpius constellation: the Alpha Scorpiids and the Omega Scorpius. The constellation Scorpius contains 18 named stars. In Greek mythology, Scorpius constellation Scorpius was identified with the scorpion that killed Orion, the mythical hunter. The Scorpius constellations lie opposite each other in the sky, and Orion is said to be fleeing from Scorpius scorpion as it sets just as Scorpius rises. In one version of the myth, Orion tried to Scorpius the goddess Artemis and she sent Scorpius scorpion to kill him. In another version, it was the Earth that sent the scorpion after Orion had boasted Scorpius he could kill any wild Scorpius. Antares is a red supergiant star with a visual magnitude Scorpius 0. It is the brightest star in the Scorpius constellation and the 16th brightest star in the night sky. Sometimes Scorpius is Scorpius to as the 15th brightest star if the two brighter components in the Capella Alpha Aurigae, located in Auriga constellation system are counted as one star. It can be occulted by the Moon and very infrequently by Venus. The last recorded occultation by Venus occurred on September 17, BC. Antares is the most massive, brightest and most evolved member of the Scorpius-Centaurus association, the nearest OB stellar association to the solar system. The star belongs to the spectral class M1. It is approximately 10, times more luminous than the Sun, and has between 15 Scorpius 18 solar masses. This is a comparison between the red supergiant Antares and the Sun, shown as the tiny dot toward the upper right. The black circle is the size of the orbit of Mars. Arcturus is also included in the picture for size comparison. Image: Sakurambo at Wikipedia. Antares is classified as a type LC slow irregular variable star. It has a companion star, Antares B, about astronomical units AU away. Antares B has Scorpius stellar classification B2. It is more luminous than the Sun and has an orbital period estimated at years. Antares marks the heart of the scorpion, which is also its alternative name. The comparison possibly dates way back to Mesopotamian astronomers. Antares was known under different names in Scorpius cultures. Shaula is Scorpius second brightest star in Scorpius and the 25th brightest star in Scorpius sky. It is approximately light years distant from the solar system. Lambda Scorpii A is a triple star system composed Scorpius two class B stars and a Scorpius sequence star. Lambda Scorpii B lies 42 arc seconds away from the first component, and Lambda Scorpii C is a 12th magnitude star 95 arc seconds away from component A. The estimated age of the star system is about Scorpius years. Beta Scorpii is another Scorpius star system in Scorpius. In small telescopes, it appears as a binary star Scorpius two components Scorpius by The brighter of the two components is itself a binary star with an orbital period of years and its own brighter component is Scorpius spectroscopic binary, with Scorpius separated by only 1. The other visual component also has Scorpius subcomponents with an angular separation of Scorpius. The dimmer subcomponent is yet another spectroscopic binary star with an orbital period of Scorpius The two most massive stars in the system are main sequence stars belonging to the spectral class B. Scorpius has at least 10 solar Scorpius and both are expected to end their lives in massive Type II supernova explosions. Delta Scorpii has the stellar classification B0. It Scorpius a visual magnitude Scorpius 2. The star has a class B companion orbiting it every 20 Scorpius, and another star in a Scorpius eccentric orbit that orbits the primary star every 10 years. Sometimes the star is also known as Iclarcrau or Iclarkrav. Theta Scorpii is an evolved bright yellow giant star belonging to the spectral class F0 II. It has an apparent magnitude of 1. Scorpius star has 5. It Scorpius a companion with an apparent Scorpius of 5. The meaning of the name is unknown. The star has a radius almost 13 times that of the Sun. It is classified as a variable, as its brightness Scorpius slightly, only by 0. Kappa Scorpii is a spectroscopic binary star, composed of two stars that cannot be resolved with a telescope. The stars have an orbital period Scorpius days. The combined spectrum of Scorpius Kappa Scorpii system has the stellar classification of B1. The primary component in the system is classified as a Beta Cephei type variable, which is to say it is a star that exhibits variations in brightness as a result of pulsations of its Scorpius. The star is 17 times more Scorpius than the Sun and has almost 7 times the solar radius. The secondary component is also much larger than the Sun, has about 12 Scorpius masses, and almost 6 times the solar radius. Pi Scorpii is a triple star Scorpius with a combined visual magnitude of 2. It is approximately light years distant. The brightest components in the system form an eclipsing binary star classified as a Beta Lyrae type variable. Both stars are hot main sequence stars with the stellar classifications B1 V and B2 V. The distance between them is believed to be only around 15 solar radii. The third component in the system is a distant companion with a visual magnitude of The primary star is 21, times Scorpius luminous than the Sun and has about solar masses. Nu Scorpii is another multiple star system in Scorpius, approximately light years distant from Earth. It is composed of two close groups of stars separated by 41 seconds of arc. The brighter group consists of B2 class subgiants Scorpius the fainter pair is Scorpius of class B8 and B0 main sequence dwarf stars. Xi Scorpii is another multiple star system in Scorpius. It consists of at least five stars Scorpius two groups that are separated by 4. The brighter group consists of two yellow-white class F stars, a subgiant with a visual magnitude of 4. The other group consists of two class K stars separated by Scorpius The sixth component in the Xi Scorpii system is not confirmed to be gravitationally Scorpius to the other stars. It is an 11th magnitude star. The Bayer designation Iota Scorpii is shared by two stars. Iota-1 Scorpii is an evolved star with the stellar Scorpius F2 Ia, on the verge of becoming a supergiant. It is 12 times more massive than the Sun and about 35, times more luminous. It has a 10th magnitude companion at a separation of The star is sometimes known Scorpius its proper name, Apollyon. Iota-2 Scorpii is a supergiant belonging to Scorpius spectral class A6Ib. It has an apparent magnitude of 4. The star has a distant 11th magnitude companion at a separation of Sigma Scorpii Scorpius a star system with a combined apparent magnitude of 2. The brightest star in the system is a spectroscopic binary star, composed of two unresolved stars that orbit each other with a period of The primary star in the spectroscopic binary system is a giant of the spectral type B1 III. It is 18 times more massive than the Sun and has 12 times the solar radius. It is classified as a Beta Cephei type variable. The other component Scorpius the system Scorpius a main sequence star belonging to the spectral class B1 V. There is another star in the system orbiting the main pair at a separation of half an arc second. At a separation of 20 seconds of arc, a class B9 dwarf with a visual magnitude of 8. Tau Scorpii is a hydrogen fusing dwarf star with a strong, complex magnetic field. Scorpius star Scorpius the Scorpius classification B0. It is a hot star, with a mass 15 times that of the Sun and a radius more than six Scorpius solar. Scorpius has an Scorpius magnitude of 2. Scorpius - Wikipedia The Scorpius constellation has intrigued people for Scorpius, not only for Scorpius distinctive shape, but Scorpius because it is one of the brightest constellations in the sky. The name Scorpius Latin Scorpius scorpionor Scorpius translated as the "creature with the burning sting. The Javanese people of Indonesia call this constellation Banyakangrem, meaning "the brooded swan" or Kalapa Doyong, meaning Scorpius coconut tree. In Chinese mythology, the constellation was part of the Azure Dragon. In the Northern Hemisphere, Scorpius lies close to the southern Scorpius in the Southern Hemisphere, it lies high in the Scorpius near the center of the Milky Way. Scorpius Scorpius to be larger. The ancient Greeks considered the Libra constellation to Scorpius the claws of the scorpion. Scorpius Scorpius to be the location for several interesting exoplanets, who have metrics ranging from extreme old age to Scorpius habitability.
Load more

Recommended publications
  • Astronomie in Theorie Und Praxis 8. Auflage in Zwei Bänden Erik Wischnewski
    Astronomie in Theorie und Praxis 8. Auflage in zwei Bänden Erik Wischnewski Inhaltsverzeichnis 1 Beobachtungen mit bloßem Auge 37 Motivation 37 Hilfsmittel 38 Drehbare Sternkarte Bücher und Atlanten Kataloge Planetariumssoftware Elektronischer Almanach Sternkarten 39 2 Atmosphäre der Erde 49 Aufbau 49 Atmosphärische Fenster 51 Warum der Himmel blau ist? 52 Extinktion 52 Extinktionsgleichung Photometrie Refraktion 55 Szintillationsrauschen 56 Angaben zur Beobachtung 57 Durchsicht Himmelshelligkeit Luftunruhe Beispiel einer Notiz Taupunkt 59 Solar-terrestrische Beziehungen 60 Klassifizierung der Flares Korrelation zur Fleckenrelativzahl Luftleuchten 62 Polarlichter 63 Nachtleuchtende Wolken 64 Haloerscheinungen 67 Formen Häufigkeit Beobachtung Photographie Grüner Strahl 69 Zodiakallicht 71 Dämmerung 72 Definition Purpurlicht Gegendämmerung Venusgürtel Erdschattenbogen 3 Optische Teleskope 75 Fernrohrtypen 76 Refraktoren Reflektoren Fokus Optische Fehler 82 Farbfehler Kugelgestaltsfehler Bildfeldwölbung Koma Astigmatismus Verzeichnung Bildverzerrungen Helligkeitsinhomogenität Objektive 86 Linsenobjektive Spiegelobjektive Vergütung Optische Qualitätsprüfung RC-Wert RGB-Chromasietest Okulare 97 Zusatzoptiken 100 Barlow-Linse Shapley-Linse Flattener Spezialokulare Spektroskopie Herschel-Prisma Fabry-Pérot-Interferometer Vergrößerung 103 Welche Vergrößerung ist die Beste? Blickfeld 105 Lichtstärke 106 Kontrast Dämmerungszahl Auflösungsvermögen 108 Strehl-Zahl Luftunruhe (Seeing) 112 Tubusseeing Kuppelseeing Gebäudeseeing Montierungen 113 Nachführfehler
    [Show full text]
  • Mathématiques Et Espace
    Atelier disciplinaire AD 5 Mathématiques et Espace Anne-Cécile DHERS, Education Nationale (mathématiques) Peggy THILLET, Education Nationale (mathématiques) Yann BARSAMIAN, Education Nationale (mathématiques) Olivier BONNETON, Sciences - U (mathématiques) Cahier d'activités Activité 1 : L'HORIZON TERRESTRE ET SPATIAL Activité 2 : DENOMBREMENT D'ETOILES DANS LE CIEL ET L'UNIVERS Activité 3 : D'HIPPARCOS A BENFORD Activité 4 : OBSERVATION STATISTIQUE DES CRATERES LUNAIRES Activité 5 : DIAMETRE DES CRATERES D'IMPACT Activité 6 : LOI DE TITIUS-BODE Activité 7 : MODELISER UNE CONSTELLATION EN 3D Crédits photo : NASA / CNES L'HORIZON TERRESTRE ET SPATIAL (3 ème / 2 nde ) __________________________________________________ OBJECTIF : Détermination de la ligne d'horizon à une altitude donnée. COMPETENCES : ● Utilisation du théorème de Pythagore ● Utilisation de Google Earth pour évaluer des distances à vol d'oiseau ● Recherche personnelle de données REALISATION : Il s'agit ici de mettre en application le théorème de Pythagore mais avec une vision terrestre dans un premier temps suite à un questionnement de l'élève puis dans un second temps de réutiliser la même démarche dans le cadre spatial de la visibilité d'un satellite. Fiche élève ____________________________________________________________________________ 1. Victor Hugo a écrit dans Les Châtiments : "Les horizons aux horizons succèdent […] : on avance toujours, on n’arrive jamais ". Face à la mer, vous voyez l'horizon à perte de vue. Mais "est-ce loin, l'horizon ?". D'après toi, jusqu'à quelle distance peux-tu voir si le temps est clair ? Réponse 1 : " Sans instrument, je peux voir jusqu'à .................. km " Réponse 2 : " Avec une paire de jumelles, je peux voir jusqu'à ............... km " 2. Nous allons maintenant calculer à l'aide du théorème de Pythagore la ligne d'horizon pour une hauteur H donnée.
    [Show full text]
  • KELT-14B and KELT-15B: an Independent Discovery of WASP-122B and a New Hot Jupiter
    Swarthmore College Works Physics & Astronomy Faculty Works Physics & Astronomy 5-11-2016 KELT-14b And KELT-15b: An Independent Discovery Of WASP-122b And A New Hot Jupiter J. E. Rodriguez K. D. Colón K. G. Stassun D. Wright P. A. Cargile See next page for additional authors Follow this and additional works at: https://works.swarthmore.edu/fac-physics Part of the Astrophysics and Astronomy Commons Let us know how access to these works benefits ouy Recommended Citation J. E. Rodriguez, K. D. Colón, K. G. Stassun, D. Wright, P. A. Cargile, D. Bayliss, J. Pepper, K. A. Collins, R. B. Kuhn, M. B. Lund, R. J. Siverd, G. Zhou, B. S. Gaudi, C. G. Tinney, K. Penev, T. G. Tan, C. Stockdale, I. A. Curtis, D. James, S. Udry, D. Segransan, A. Bieryla, D. W. Latham, T. G. Beatty, J. D. Eastman, G. Myers, J. Bartz, J. Bento, Eric L.N. Jensen, T. E. Oberst, and D. J. Stevens. (2016). "KELT-14b And KELT-15b: An Independent Discovery Of WASP-122b And A New Hot Jupiter". Astronomical Journal. Volume 151, Issue 6. 138 DOI: 10.3847/0004-6256/151/6/138 https://works.swarthmore.edu/fac-physics/286 This work is brought to you for free by Swarthmore College Libraries' Works. It has been accepted for inclusion in Physics & Astronomy Faculty Works by an authorized administrator of Works. For more information, please contact [email protected]. Authors J. E. Rodriguez, K. D. Colón, K. G. Stassun, D. Wright, P. A. Cargile, D. Bayliss, J. Pepper, K. A. Collins, R.
    [Show full text]
  • Durham E-Theses
    Durham E-Theses First visibility of the lunar crescent and other problems in historical astronomy. Fatoohi, Louay J. How to cite: Fatoohi, Louay J. (1998) First visibility of the lunar crescent and other problems in historical astronomy., Durham theses, Durham University. Available at Durham E-Theses Online: http://etheses.dur.ac.uk/996/ Use policy The full-text may be used and/or reproduced, and given to third parties in any format or medium, without prior permission or charge, for personal research or study, educational, or not-for-prot purposes provided that: • a full bibliographic reference is made to the original source • a link is made to the metadata record in Durham E-Theses • the full-text is not changed in any way The full-text must not be sold in any format or medium without the formal permission of the copyright holders. Please consult the full Durham E-Theses policy for further details. Academic Support Oce, Durham University, University Oce, Old Elvet, Durham DH1 3HP e-mail: [email protected] Tel: +44 0191 334 6107 http://etheses.dur.ac.uk me91 In the name of Allah, the Gracious, the Merciful >° 9 43'' 0' eji e' e e> igo4 U61 J CO J: lic 6..ý v Lo ý , ý.,, "ý J ýs ýºý. ur ý,r11 Lýi is' ý9r ZU LZJE rju No disaster can befall on the earth or in your souls but it is in a book before We bring it into being; that is easy for Allah. In order that you may not grieve for what has escaped you, nor be exultant at what He has given you; and Allah does not love any prideful boaster.
    [Show full text]
  • Young Super-Neptune Offers Clues to the Origin of Close-In Exoplanet 21 June 2016, by Rebecca Johnson
    Young super-Neptune offers clues to the origin of close-in exoplanet 21 June 2016, by Rebecca Johnson planets in the same planetary system, or with more distant stars. These scenarios can be tested observationally by searching for young planets and studying their orbits. If the close-in population formed in place or migrated in through interactions with the natal disk, they reach their final orbital distances early on and will be found close in at young ages. In comparison, migrating a planet inward through interactions with other planets or more distant stars is effective on much longer timescales. If the latter processes dominate, planets will not be found close to their K2-33 b, shown in this illustration, is one of the youngest stars when they are young. exoplanets detected to date. It makes a complete orbit around its star in about five days. These two characteristics combined provide exciting new directions for planet-formation theories. K2-33b could have formed on a farther out orbit and quickly migrated inward. Alternatively, it could have formed in situ, or in place. Credit: NASA/JPL-Caltech A team of astronomers has confirmed the existence of a young planet, only 11 million years old, that orbits very close to its star (at 0.05 AU), with an orbital period of 5.4 days. Approximately 5 times the size of the Earth, the new planet is a "super-Neptune" and the youngest such planet This image shows the K2-33 system, and its planet known. The discovery lends unique insights into K2-33b, compared to our own solar system.
    [Show full text]
  • The Denver Observer July 2018
    The Denver JULY 2018 OBSERVER The globular cluster, Messier 19, one of this month’s targets in “July Skies,” in a Hubble Space Telescope image. Credit: NASA, ESA, STScI and I. King (Univer- sity of California – Berkeley) JULY SKIES by Zachary Singer The Solar System ’scopes towards the planets when they’re Sky Calendar The big news for July is that Mars comes highest in the sky on a given night, to get the 6 Last-Quarter Moon to opposition on the 27th, meaning that it sharpest image—but Mars is worth viewing 12 New Moon will be at its highest in the south on that date naked-eye when it’s rising. Surprised? The 19 First-Quarter Moon around 1 AM, and also more or less at its red (well, orange) planet appears even redder 27 Full Moon largest as seen from Earth. Now, don’t let that when rising, making for much deeper color. fool you—Mars is already very good as July It’s a guilty pleasure on an aesthetic level, if begins, showing a disk 21” across, which is not a scientific one. If you want to indulge better than we got two years ago, and only yourself, Mars rises around 10:30 PM at In the Observer slightly smaller than the 24” expected at the beginning of July, an hour earlier mid- the end of the month. (Observations in my month, and about 8:20 PM at month’s end. President’s Message . .2 6-inch reflector at the end of June showed an Meanwhile, Mercury is an evening Society Directory.
    [Show full text]
  • The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
    The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24).
    [Show full text]
  • The Hypergiants VY Canis Majoris, Eta Carinae, V766 Centauri and The
    Sixteenth Marcel Grossmann Meeting Contribution ID: 967 Type: Talk in the parallel session The hypergiants VY Canis Majoris, Eta Carinae, V766 Centauri and the red supergiants Betelgeuse, Antares and Aldebaran in the 2.5K SGQ AAVSO database Thursday, 8 July 2021 16:35 (7 minutes) I observe variable stars since 1997. The “candidacy” of Mira Ceti as Betlehem Star because close to Jupiter- Saturn triple conjunction of 6-7 b.C. started at Pontifical University of Lateran and continued in Yale (2001- 2004). Maxima correlation function ruled out Mira for having two consecutive bright maxima, but this prop- erty was confirmed in the “oldest” Myra-type: R Leonis, R Hydrae and Chi Cygni, from their almostfour- century-long lightcurves. To a bright maximum normally a dim one follows, as the correlation function of their consecutive maxima shows. These studies were supported by historical and personal visual observations. Since 2011 I observe firstmag- nitude variable stars, with airmass correction to reach 0.01 magnitudes accuracy with naked eye. AAVSO observer Sebastian Otero first claimed this accuracy, as for NovaCentauri 2013, observed by me fromPorto Alegre and Rio de Janeiro. Betelgeuse’s 801 observations in 10 years, include the deep minimum of 2020. My SGQ contributions to AAVSO-database, paralleled with Betelgeuse’s V-band measurements, help to define the “personal equations” present in all 25M visual observations before CCD era (1911-on) going back to 1893 for Betelgeuse. The temporal extension of lightcurves is crucial to understand the stellar behaviour. More complicate cases are Antares and Aldebaran, less variable and with distant comparison stars.
    [Show full text]
  • A Spectroscopic Study of the Scorpio-Centaurus Association
    PranllQa. Vol. 7, No.3, 1976, pp 160-\ 80. © Prmted in India. A spectroscopic study of the Scorpio-Centaurus association R RAJAMOHAN Indian Institute of Astrophysics, Bangaiore 560034 MS recehcl 5 April 1976 • I' Abstract. Rotational .... elocities as well as hydrogen and he Jlum Ine I'ntensities of .' have been one hundred. and twelve members of the Scorplo-Centaurus aSSOclatlO~ . b h derived. For stars with M~ < 0'0, the distribution of rotational velocitieS of °lt are SJlnlar the upper Scorplus subgroup and the upper Centaurus-Lupus Su b grou P 1 . I and closely resemble those of the field stars. Stars with M, > O' 0, all of w lie 1 are found in th.e dense upper Scorpius region, rotate much faster than their counter­ parts amongst field stars, the Pleiades and Alpha-Persei cluster members. The measured equivalent width of H'Y for 77 stars provide a distance nlOd~\U~ of 6·0±0·09 magnitudes for the association. Evolutionary effects in the del1;~e hydrogen line intensities are found between the two subgroups. The hydrogen- me intensities at all spectral types in the upper Centaurus-Lupus subgroup are systematically smaller than thOse of members in the upper Scorpius subgrouP. Analysis of high dispersion spectra of five members of the association y.ield a helium abundance of Nae(N. = 0·096 ± 0 004. Along with data available In the literature, the mean helium abundance of thirteen stars of this association is found to be 0·098 :±: O· 004 by number. For the two main subgroups of this association, we deflve a value of 0 105 ± 0 001 for the upper Centaurus-Lupus group from three stars and 0·096 ± 0·005 for the upper Scorpius group from ten stars.
    [Show full text]
  • 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.
    [Show full text]
  • Fy10 Budget by Program
    AURA/NOAO FISCAL YEAR ANNUAL REPORT FY 2010 Revised Submitted to the National Science Foundation March 16, 2011 This image, aimed toward the southern celestial pole atop the CTIO Blanco 4-m telescope, shows the Large and Small Magellanic Clouds, the Milky Way (Carinae Region) and the Coal Sack (dark area, close to the Southern Crux). The 33 “written” on the Schmidt Telescope dome using a green laser pointer during the two-minute exposure commemorates the rescue effort of 33 miners trapped for 69 days almost 700 m underground in the San Jose mine in northern Chile. The image was taken while the rescue was in progress on 13 October 2010, at 3:30 am Chilean Daylight Saving time. Image Credit: Arturo Gomez/CTIO/NOAO/AURA/NSF National Optical Astronomy Observatory Fiscal Year Annual Report for FY 2010 Revised (October 1, 2009 – September 30, 2010) Submitted to the National Science Foundation Pursuant to Cooperative Support Agreement No. AST-0950945 March 16, 2011 Table of Contents MISSION SYNOPSIS ............................................................................................................ IV 1 EXECUTIVE SUMMARY ................................................................................................ 1 2 NOAO ACCOMPLISHMENTS ....................................................................................... 2 2.1 Achievements ..................................................................................................... 2 2.2 Status of Vision and Goals ................................................................................
    [Show full text]
  • Transactions 1905
    THE Royal Astronomical Society of Canada TRANSACTIONS FOR 1905 (INCLUDING SELECTED PAPERS AND PROCEEDINGS) EDITED BY C. A CHANT. TORONTO: ROYAL ASTRONOMICAL PRINT, 1906. The Royal Astronomical Society of Canada. THE Royal Astronomical Society of Canada TRANSACTIONS FOR 1905 (INCLUDING SELECTED PAPERS AND PROCEEDINGS) EDITED BY C. A CHANT. TORONTO: ROYAL ASTRONOMICAL PRINT, 1906. TABLE OF CONTENTS. The Dominion Observatory, Ottawa (Frontispiece) List of Officers, Fellows and A ssociates..................... - - 3 Treasurer’s R eport.....................--------- 12 President’s Address and Summary of Work ------ 13 List of Papers and Lectures, 1905 - - - - ..................... 26 The Dominion Observatory at Ottawa - - W. F. King 27 Solar Spots and Magnetic Storms for 1904 Arthur Harvey 35 Stellar Legends of American Indians - - J. C. Hamilton 47 Personal Profit from Astronomical Study - R. Atkinson 51 The Eclipse Expedition to Labrador, August, 1905 A. T. DeLury 57 Gravity Determinations in Labrador - - Louis B. Stewart 70 Magnetic and Meteorological Observations at North-West River, Labrador - - - - R. F. Stupart 97 Plates and Filters for Monochromatic and Three-Color Photography of the Corona J. S. Plaskett 89 Photographing the Sun and Moon with a 5-inch Refracting Telescope . .......................... D. B. Marsh 108 The Astronomy of Tennyson - - - - John A. Paterson 112 Achievements of Nineteenth Century Astronomy , L. H. Graham 125 A Lunar Tide on Lake Huron - - - - W. J. Loudon 131 Contributions...............................................J. Miller Barr I. New Variable Stars - - - - - - - - - - - 141 II. The Variable Star ξ Bootis -------- 143 III. The Colors of Helium Stars - - - ..................... 144 IV. A New Problem in Solar Physics ------ 146 Stellar Classification ------ W. Balfour Musson 151 On the Possibility of Fife in Other Worlds A.
    [Show full text]