Hydra's Arrow-Head
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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. -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
Cr> Γ- ΟΟ [ Publications of the Astronomical Society of the Pacific
cr> - ΟΟΓ [ Publications of the Astronomical Society of the Pacific cs] 102:379-411, April 1990 \—I0 ωCu 1 PUBLICATIONS OF THE 2 ASTRONOMICAL SOCIETY OF THE PACIFIC Vol. 102 April 1990 No. 650 CONTEMPORARY OPTICAL SPECTRAL CLASSIFICATION OF THE OB STARS: A DIGITAL ATLAS* NOLAN R. WALBORNt Space Telescope Science Institute, φ 3700 San Martin Drive, Baltimore, Maryland 21218 AND EDWARD L. FITZPATRICKf Princeton University Observatory, Peyton Hall, Princeton, New Jersey 08544 Received 1990 ABSTRACT Some recent developments in the optical classification of OB spectra are reviewed in terms of a comprehensive atlas of new blue-violet digital data from the CTIO 1-meter photon-counting system. These developments include the OS spectral type; luminosity criteria for the O stars; OBN/OBC anomalies; and refined, interpolated late-O/early-B types. Examples of these phenom- ena are included among extensive spectral- and luminosity-class sequences, comprising 75 standard objects arranged into 27 montages and covering the wavelength range 3950 Â-4750 A for types OS-BS (-B8 at Iö). It is intended that this atlas serve a reference function analogous to that of the printed MK atlases, for morphological investigations of OB spectra based on digital data, which will supersede photographic techniques in most future applications. Key words: spectral atlas-OB stars 1. Introduction and Background The Μ Κ classification was based on blue-violet The system of spectral classification provided one (3900 Â-4900 A) photographic spectrograms of disper- Μ Κ -1 of the foundations of stellar astrophysics. Far from being sion ~ 100 A mm (resolution ~ 2 A) and widening at rendered obsolete by the development of the latter, how- least 0.5 mm. -
The Brightest Stars Seite 1 Von 9
The Brightest Stars Seite 1 von 9 The Brightest Stars This is a list of the 300 brightest stars made using data from the Hipparcos catalogue. The stellar distances are only fairly accurate for stars well within 1000 light years. 1 2 3 4 5 6 7 8 9 10 11 12 13 No. Star Names Equatorial Galactic Spectral Vis Abs Prllx Err Dist Coordinates Coordinates Type Mag Mag ly RA Dec l° b° 1. Alpha Canis Majoris Sirius 06 45 -16.7 227.2 -8.9 A1V -1.44 1.45 379.21 1.58 9 2. Alpha Carinae Canopus 06 24 -52.7 261.2 -25.3 F0Ib -0.62 -5.53 10.43 0.53 310 3. Alpha Centauri Rigil Kentaurus 14 40 -60.8 315.8 -0.7 G2V+K1V -0.27 4.08 742.12 1.40 4 4. Alpha Boötis Arcturus 14 16 +19.2 15.2 +69.0 K2III -0.05 -0.31 88.85 0.74 37 5. Alpha Lyrae Vega 18 37 +38.8 67.5 +19.2 A0V 0.03 0.58 128.93 0.55 25 6. Alpha Aurigae Capella 05 17 +46.0 162.6 +4.6 G5III+G0III 0.08 -0.48 77.29 0.89 42 7. Beta Orionis Rigel 05 15 -8.2 209.3 -25.1 B8Ia 0.18 -6.69 4.22 0.81 770 8. Alpha Canis Minoris Procyon 07 39 +5.2 213.7 +13.0 F5IV-V 0.40 2.68 285.93 0.88 11 9. Alpha Eridani Achernar 01 38 -57.2 290.7 -58.8 B3V 0.45 -2.77 22.68 0.57 144 10. -
Stars and Their Spectra: an Introduction to the Spectral Sequence Second Edition James B
Cambridge University Press 978-0-521-89954-3 - Stars and Their Spectra: An Introduction to the Spectral Sequence Second Edition James B. Kaler Index More information Star index Stars are arranged by the Latin genitive of their constellation of residence, with other star names interspersed alphabetically. Within a constellation, Bayer Greek letters are given first, followed by Roman letters, Flamsteed numbers, variable stars arranged in traditional order (see Section 1.11), and then other names that take on genitive form. Stellar spectra are indicated by an asterisk. The best-known proper names have priority over their Greek-letter names. Spectra of the Sun and of nebulae are included as well. Abell 21 nucleus, see a Aurigae, see Capella Abell 78 nucleus, 327* ε Aurigae, 178, 186 Achernar, 9, 243, 264, 274 z Aurigae, 177, 186 Acrux, see Alpha Crucis Z Aurigae, 186, 269* Adhara, see Epsilon Canis Majoris AB Aurigae, 255 Albireo, 26 Alcor, 26, 177, 241, 243, 272* Barnard’s Star, 129–130, 131 Aldebaran, 9, 27, 80*, 163, 165 Betelgeuse, 2, 9, 16, 18, 20, 73, 74*, 79, Algol, 20, 26, 176–177, 271*, 333, 366 80*, 88, 104–105, 106*, 110*, 113, Altair, 9, 236, 241, 250 115, 118, 122, 187, 216, 264 a Andromedae, 273, 273* image of, 114 b Andromedae, 164 BDþ284211, 285* g Andromedae, 26 Bl 253* u Andromedae A, 218* a Boo¨tis, see Arcturus u Andromedae B, 109* g Boo¨tis, 243 Z Andromedae, 337 Z Boo¨tis, 185 Antares, 10, 73, 104–105, 113, 115, 118, l Boo¨tis, 254, 280, 314 122, 174* s Boo¨tis, 218* 53 Aquarii A, 195 53 Aquarii B, 195 T Camelopardalis, -
The Fifth Level of Learning: the Vedic Gods
The Wes Penre Papers || The Fifth Level of Learning The Vedic Texts The Wes Penre Papers: The Vedic Texts The Fifth Level of Learning Part 2 by Wes Penre The Wes Penre Papers || The Fifth Level of Learning The Vedic Texts Copyright © 2014-2015 Wes Penre All rights reserved. This is an electronic paper free of charge, which can be downloaded, quoted from, and copied to be shared with other people, as long as nothing in this paper is altered or quoted out of context. Not for commercial use. Editing provided by Bob Stannard: www.twilocity.com 1st Edition, February 27, 2015 Wes Penre Productions Oregon, USA The Wes Penre Papers || The Fifth Level of Learning The Vedic Texts Table of Contents PAPER 10: THE NAKSHATRAS—THE GOD AND THEIR STAR SYSTEMS ...... 6 I. The Nakshatras or Lunar Mansions ...................................................................... 6 II. Star Systems and Constellations in Domain of the Orion Empire ...................... 9 ii.i. The Orion Empire in the Vedas ....................................................................... 17 III. Domains Conquered by the AIF with Marduk in Charge ................................ 20 IV. Star Systems and Constellations under En.ki’s Control .................................. 40 V. Asterism Ruled by Queen Ereškigal ................................................................. 61 PAPER 11: DISCUSSING STAR SYSTEMS NOT MENTIONED IN THE NAKSHATRAS ........................................................................................................... 65 I. Introduction -
Adventuring with Books: a Booklist for Pre-K-Grade 6. the NCTE Booklist
DOCUMENT RESUME ED 311 453 CS 212 097 AUTHOR Jett-Simpson, Mary, Ed. TITLE Adventuring with Books: A Booklist for Pre-K-Grade 6. Ninth Edition. The NCTE Booklist Series. INSTITUTION National Council of Teachers of English, Urbana, Ill. REPORT NO ISBN-0-8141-0078-3 PUB DATE 89 NOTE 570p.; Prepared by the Committee on the Elementary School Booklist of the National Council of Teachers of English. For earlier edition, see ED 264 588. AVAILABLE FROMNational Council of Teachers of English, 1111 Kenyon Rd., Urbana, IL 61801 (Stock No. 00783-3020; $12.95 member, $16.50 nonmember). PUB TYPE Books (010) -- Reference Materials - Bibliographies (131) EDRS PRICE MF02/PC23 Plus Postage. DESCRIPTORS Annotated Bibliographies; Art; Athletics; Biographies; *Books; *Childress Literature; Elementary Education; Fantasy; Fiction; Nonfiction; Poetry; Preschool Education; *Reading Materials; Recreational Reading; Sciences; Social Studies IDENTIFIERS Historical Fiction; *Trade Books ABSTRACT Intended to provide teachers with a list of recently published books recommended for children, this annotated booklist cites titles of children's trade books selected for their literary and artistic quality. The annotations in the booklist include a critical statement about each book as well as a brief description of the content, and--where appropriate--information about quality and composition of illustrations. Some 1,800 titles are included in this publication; they were selected from approximately 8,000 children's books published in the United States between 1985 and 1989 and are divided into the following categories: (1) books for babies and toddlers, (2) basic concept books, (3) wordless picture books, (4) language and reading, (5) poetry. (6) classics, (7) traditional literature, (8) fantasy,(9) science fiction, (10) contemporary realistic fiction, (11) historical fiction, (12) biography, (13) social studies, (14) science and mathematics, (15) fine arts, (16) crafts and hobbies, (17) sports and games, and (18) holidays. -
THE CONSTELLATION HYDRA, WATER SNAKE Hydra Is the Largest of the 88 Modern Constellations, Measuring 1303 Square Degrees
THE CONSTELLATION HYDRA, WATER SNAKE Hydra is the largest of the 88 modern constellations, measuring 1303 square degrees. Also one of the longest at over 100 degrees, its southern end abuts Libra and Centaurus and its northern end borders Cancer. It has a long history, having been included among the 48 constellations listed by the 2nd century astronomer Ptolemy. It is commonly represented as a water snake. It should not be confused with the similarly named constellation of Hydrus. The neighboring constellations are Antlia, Cancer, Canis Minor, Centaurus, Corvus, Crater, Leo, Libra, Lupus, Monoceros, Puppis, Pyxis, Sextans and Virgo. Despite its size, Hydra contains only one reasonably bright star, Alphard, designated Alpha Hydrae. It is an orange giant of magnitude 2.0, 177 light-years from Earth. Its traditional name means "the solitary one". Beta Hydrae is a blue-white star of magnitude 4.3, 365 light-years from Earth. Gamma Hydrae is a yellow giant of magnitude 3.0, 132 light-years from Earth. Hydra has one bright binary star, Epsilon Hydrae, which is difficult to split in amateur telescopes; it has a period of 1000 years and is 135 light-years from Earth. The other main named star in Hydra is Sigma Hydrae, which has the name of Minaruja, from the Arabic for snake's nose. At magnitude 4.54, it is rather dim. The head of the snake corresponds to the Ashlesha nakshatra, a lunar zodiacal constellation in Indian astronomy. Hydra is also home to several variable stars. R Hydrae is a Mira variable star 2000 light-years from Earth; it is one of the brightest Mira variables at its maximum of magnitude 3.5. -
Planetarische Nebel Zeigt Eine Polypolare 2015 Und Auf Dessen Rückseite Den Von „Sterne Und Weltraum“ Zusammenge- Struktur
www.vds-astro.de ISSN 1615-0880 I/2015 Nr. 52 Zeitschrift der Vereinigung der Sternfreunde e.V. Schwerpunktthema Planetarische Universal-Newton Sternbedeckungen Beobachterforum Seite 70 Seite 117 Seite 134 Nebel Editorial 1 Liebe Mitglieder, liebe Sternfreunde, das neue Jahr hat begonnen, und es ist nicht übertrieben, wenn wir es als astro- nomisch besonders spannend ankündigen. Doch vor den Freuden der Himmels- beobachtung erlauben wir uns, Sie mit einer jährlichen Pflicht zu belästigen: Diesem Heft liegt die Beitragsrechnung für das Jahr 2015 bei. Bitte kommen Sie Ihrer Zahlungspflicht so bald wie möglich nach, denn die unbezahlten Mit- Unser Titelbild: gliedsbeiträge haben sich mittlerweile zu einem stattlichen Betrag summiert. Am Skinakas-Observatorium auf Kreta/ Lesen Sie dazu auch die Informationen auf Seite 4. Griechenland entstand im August 2012 in verschiedenen Nächten diese tiefe Auf- Doch zurück zum Himmelsgeschehen: Die wichtigsten Ereignisse haben wir für nahme des Helixnebels NGC 7293. Was Sie wieder in der beiliegenden Broschüre „Astronomie 2015“ zusammenge- den meisten Lesern neu sein dürfte: Der fasst. Als weitere Beilage enthält diese Sendung das Plakat zum Astronomietag Planetarische Nebel zeigt eine polypolare 2015 und auf dessen Rückseite den von „Sterne und Weltraum“ zusammenge- Struktur. Bipolare Auswürfe unterlagen im stellten „Astro-Planer“. Nur für den wolkenlosen Himmel war in der Versand- Laufe der Zeit einer Rotation wie bei KjPn 8 tasche leider kein Platz mehr. Wir bitten, das zu entschuldigen. (siehe Bericht von Hartmut Bornemann in dieser Ausgabe). Teleskop war eine Das erste Quartal 2015 bietet uns einen echten „Hingucker“: die partielle Son- 300-mm-Flatfieldkamera (Lichtenknecker) nenfinsternis am 20. März. Auch aus diesem Grund lautet das Motto zum dies- mit 940 mm Brennweite, als Kamera wur- jährigen Astronomietag „Schattenspiele im All“. -
Binocular Certificate Handbook
Irish Federation of Astronomical Societies Binocular Certificate Handbook How to see 110 extraordinary celestial sights with an ordinary pair of binoculars © John Flannery, South Dublin Astronomical Society, August 2004 No ordinary binoculars! This photograph by the author is of the delightfully whimsical frontage of the Chiat/Day advertising agency building on Main Street, Venice, California. Binocular Certificate Handbook page 1 IFAS — www.irishastronomy.org Introduction HETHER NEW to the hobby or advanced am- Wateur astronomer you probably already own Binocular Certificate Handbook a pair of a binoculars, the ideal instrument to casu- ally explore the wonders of the Universe at any time. Name _____________________________ Address _____________________________ The handbook you hold in your hands is an intro- duction to the realm far beyond the Solar System — _____________________________ what amateur astronomers call the “deep sky”. This is the abode of galaxies, nebulae, and stars in many _____________________________ guises. It is here that we set sail from Earth and are Telephone _____________________________ transported across many light years of space to the wonderful and the exotic; dense glowing clouds of E-mail _____________________________ gas where new suns are being born, star-studded sec- tions of the Milky Way, and the ghostly light of far- Observing beginner/intermediate/advanced flung galaxies — all are within the grasp of an ordi- experience (please circle one of the above) nary pair of binoculars. Equipment __________________________________ True, the fixed magnification of (most) binocu- IFAS club __________________________________ lars will not allow you get the detail provided by telescopes but their wide field of view is perfect for NOTES: Details will be treated in strictest confidence. -
Uranometría Argentina Bicentenario
URANOMETRÍA ARGENTINA BICENTENARIO Reedición electrónica ampliada, ilustrada y actualizada de la URANOMETRÍA ARGENTINA Brillantez y posición de las estrellas fijas, hasta la séptima magnitud, comprendidas dentro de cien grados del polo austral. Resultados del Observatorio Nacional Argentino, Volumen I. Publicados por el observatorio 1879. Con Atlas (1877) 1 Observatorio Nacional Argentino Dirección: Benjamin Apthorp Gould Observadores: John M. Thome - William M. Davis - Miles Rock - Clarence L. Hathaway Walter G. Davis - Frank Hagar Bigelow Mapas del Atlas dibujados por: Albert K. Mansfield Tomado de Paolantonio S. y Minniti E. (2001) Uranometría Argentina 2001, Historia del Observatorio Nacional Argentino. SECyT-OA Universidad Nacional de Córdoba, Córdoba. Santiago Paolantonio 2010 La importancia de la Uranometría1 Argentina descansa en las sólidas bases científicas sobre la cual fue realizada. Esta obra, cuidada en los más pequeños detalles, se debe sin dudas a la genialidad del entonces director del Observatorio Nacional Argentino, Dr. Benjamin A. Gould. Pero nada de esto se habría hecho realidad sin la gran habilidad, el esfuerzo y la dedicación brindada por los cuatro primeros ayudantes del Observatorio, John M. Thome, William M. Davis, Miles Rock y Clarence L. Hathaway, así como de Walter G. Davis y Frank Hagar Bigelow que se integraron más tarde a la institución. Entre éstos, J. M. Thome, merece un lugar destacado por la esmerada revisión, control de las posiciones y determinaciones de brillos, tal como el mismo Director lo reconoce en el prólogo de la publicación. Por otro lado, Albert K. Mansfield tuvo un papel clave en la difícil confección de los mapas del Atlas. La Uranometría Argentina sobresale entre los trabajos realizados hasta ese momento, por múltiples razones: Por la profundidad en magnitud, ya que llega por vez primera en este tipo de empresa a la séptima. -
Cycle 25 Approved Programs
Cycle 25 Approved Programs Phase II First Name Last Name Institution Country Type Resources Title 15328 Jessica Agarwal Max Planck Institute for Solar DEU GO 5 Orbital period and formation process of the exceptional binary asteroid System Research system 288P 15090 Marcel Agueros Columbia University in the City of USA GO 35 A UV spectroscopic survey of periodic M dwarfs in the Hyades New York 15091 Marcel Agueros Columbia University in the City of USA SNAP 86 A UV spectroscopic snapshot survey of low-mass stars in the Hyades New York 15092 Monique Aller Georgia Southern University Res. USA GO 6 Testing Dust Models at Moderate Redshift: Is the z=0.437 DLA toward 3C & Svc. Foundation, Inc 196 Rich in Carbonaceous Dust? 15193 Alessandra Aloisi Space Telescope Science Institute USA GO 22 Addressing Ionization and Depletion in the ISM of Nearby Star-Forming Galaxies 15194 Alessandra Aloisi Space Telescope Science Institute USA GO 18 The Epoch of the First Star Formation in the Closest Metal-Poor Blue Compact Dwarf Galaxy UGC 4483 15299 Julian Alvarado GomeZ Smithsonian Institution USA GO 13 Weaving the history of the solar wind with magnetic field lines Astrophysical Observatory 15093 Jennifer Andrews University of Arizona USA GO 18 Dwarfs and Giants: Massive Stars in Little Dwarf Galaxies 15222 Iair Arcavi University of California - Santa USA GO 1 What Type of Star Made the One-of-a-kind Supernova iPTF14hls? Barbara 15223 Matthew Auger University of Cambridge GBR GO 1 The Brightest Galaxy-Scale Lens 15300 Thomas Ayres University of Colorado