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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. -
Insidethisissue
Publications and Products of April / avril 2005 Volume/volume 99 Number/numéro 2 [711] The Royal Astronomical Society of Canada Observer’s Calendar — 2005 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 US 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. -
Messier Objects
Messier Objects From the Stocker Astroscience Center at Florida International University Miami Florida The Messier Project Main contributors: • Daniel Puentes • Steven Revesz • Bobby Martinez Charles Messier • Gabriel Salazar • Riya Gandhi • Dr. James Webb – Director, Stocker Astroscience center • All images reduced and combined using MIRA image processing software. (Mirametrics) What are Messier Objects? • Messier objects are a list of astronomical sources compiled by Charles Messier, an 18th and early 19th century astronomer. He created a list of distracting objects to avoid while comet hunting. This list now contains over 110 objects, many of which are the most famous astronomical bodies known. The list contains planetary nebula, star clusters, and other galaxies. - Bobby Martinez The Telescope The telescope used to take these images is an Astronomical Consultants and Equipment (ACE) 24- inch (0.61-meter) Ritchey-Chretien reflecting telescope. It has a focal ratio of F6.2 and is supported on a structure independent of the building that houses it. It is equipped with a Finger Lakes 1kx1k CCD camera cooled to -30o C at the Cassegrain focus. It is equipped with dual filter wheels, the first containing UBVRI scientific filters and the second RGBL color filters. Messier 1 Found 6,500 light years away in the constellation of Taurus, the Crab Nebula (known as M1) is a supernova remnant. The original supernova that formed the crab nebula was observed by Chinese, Japanese and Arab astronomers in 1054 AD as an incredibly bright “Guest star” which was visible for over twenty-two months. The supernova that produced the Crab Nebula is thought to have been an evolved star roughly ten times more massive than the Sun. -
April Constellations of the Month
April Constellations of the Month Leo Small Scope Objects: Name R.A. Decl. Details M65! A large, bright Sa/Sb spiral galaxy. 7.8 x 1.6 arc minutes, magnitude 10.2. Very 11hr 18.9m +13° 05’ (NGC 3623) high surface brighness showing good detail in medium sized ‘scopes. M66! Another bright Sb galaxy, only 21 arc minutes from M65. Slightly brighter at mag. 11hr 20.2m +12° 59’ (NGC 3627) 9.7, measuring 8.0 x 2.5 arc minutes. M95 An easy SBb barred spiral, 4 x 3 arc minutes in size. Magnitude 10.5, with 10hr 44.0m +11° 42’ a bright central core. The bar and outer ring of material will require larger (NGC 3351) aperature and dark skies. M96 Another bright Sb spiral, about 42 arc minutes east of M95, but larger and 10hr 46.8m +11° 49’ (NGC 3368) brighter. 6 x 4 arc minutes, magnitude 10.1. Located about 48 arc minutes NNE of M96. This small elliptical galaxy measures M105 only 2 x 2.1 arc minutes, but at mag. 10.3 has very high surface brightness. 10hr 47.8m +12° 35’ (NGC 3379) Look for NGC 3384! (110NGC) and NGC 3389 (mag 11.0 and 12.2) which form a small triangle with M105. NGC 3384! 10hr 48.3m +12° 38’ See comment for M105. The brightest galaxy in Leo, this Sb/Sc spiral galaxy shines at mag. 9.5. Look for NGC 2903!! 09hr 32.2m +21° 30’ a hazy patch 11 x 4.7 arc minutes in size 1.5° south of l Leonis. -
The Skyscraper 2009 04.Indd
A Better Galaxy Guide: Early Spring M67: One of the most ancient open clusters known and Craig Cortis is a great novelty in this regard. Located 1.7° due W of mag NGC 2419: 3.25° SE of mag 6.2 66 Aurigae. Hard to find 4.3 Alpha Cancri. and see; at E end of short row of two mag 7.5 stars. Highly NGC 2775: Located 3.7° ENE of mag 3.1 Zeta Hydrae. significant and worth the effort —may be approximately (Look for “Head of Hydra” first.) 300,000 light years distant and qualify as an extragalactic NGC 2903: Easily found at 1.5° due S of mag 4.3 Lambda cluster. Named the Intergalactic Wanderer. Leonis. NGC 2683: Marks NW “crook” of coathanger-type triangle M95: One of three bright galaxies forming a compact with easy double star mag 4.2 Iota Cancri (which is SSW by triangle, along with M96 and M105. All three can be seen 4.8°) and mag 3.1 Alpha Lyncis (at 6° to the ENE). together in a low power, wide field view. M105 is at the NE tip of triangle, midway between stars 52 and 53 Leonis, mag Object Type R.A. Dec. Mag. Size 5.5 and 5.3 respectively —M95 is at W tip. Lynx NGC 3521: Located 0.5° due E of mag 6.0 62 Leonis. M65: One of a pair of bright galaxies that can be seen in NGC 2419 GC 07h 38.1m +38° 53’ 10.3 4.2’ a wide field view along with M66, which lies just E. -
The SONG Prototype: Efficiency of a Robotic Telescope
To appear in “RevMexAA (Serie de Conferencias), 00, 14 (2015)” RevMexAA(SC) THE SONG PROTOTYPE: EFFICIENCY OF A ROBOTIC TELESCOPE M. F. Andersen,1 F. Grundahl,1 A. H. Beck,1 and P. Pall´e2 RESUMEN El telescopio prototipo del Grupo de la Red de Observaciones Estelares (SONG) ha operado en modo cient`ıfico desde marzo de 2014. El primer a˜no de observaciones se ha dedicado por completo al espectr`ografo. Varios objetos de inter`es astros`ısmico se han observado para verificaci`on cient`ıfica y t`ecnica. Algunas estrellas subgi- gantes brillantes y una gigante roja fueron elegidas para prueba ya que las oscilaciones en estas estrellas tienen grandes amplitudes y los periodos son lo suficientemente largos para ser detectados. Estos objetos ser`an usados para evaluar los instrumentos ya que las observaciones a largo plazo de los objetos de estudio podr`ıan presentar algunos problemas. En este art`ıculo describimos como opera el primero de los telescopios de la Red SONG para ilustrar la eficiencia y las capacidades de un telescopio robtico. ABSTRACT The Stellar Observations Network Group prototype telescope at the Teide Observatory has been operating in scientific mode since March 2014. The first year of observations has entirely been carried out using the high resolution echelle spectrograph. Several asteroseismic targets were selected for scientific and technical verification. A few bright subgiants and one red giant were chosen since the oscillations in these stars have large amplitudes and the periods long enough to easily be detected. These targets would also be used for evaluation of the instruments since long term observations of single targets would reveal potential problems. -
The Leo-I Group: New Dwarf Galaxy and UDG Candidates Oliver Müller1, Helmut Jerjen2, and Bruno Binggeli1
Astronomy & Astrophysics manuscript no. aanda c ESO 2018 February 26, 2018 The Leo-I group: new dwarf galaxy and UDG candidates Oliver Müller1, Helmut Jerjen2, and Bruno Binggeli1 1 Departement Physik, Universität Basel, Klingelbergstr. 82, CH-4056 Basel, Switzerland e-mail: [email protected] 2 Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 2611, Australia Received XX, 2018; accepted TBD ABSTRACT Context. The study of dwarf galaxies and their environments provides crucial testbeds for predictions of cosmological models and insights on the structure formation on small cosmological scales. In recent years, many problems on the scale of groups of galaxies challenged the current standard model of cosmology. Aims. We aim to increase the sample of known galaxies in the Leo-I group, containing the M 96 subgroup and the Leo Triplet. This galaxy aggregate is located at the edge of the Local Volume at a mean distance of 10.7 Mpc. Methods. We employ image enhancing techniques to search for low-surface brightness objects in publicly available gr images taken by the Sloan Digital Sky Survey within 500 square degrees around the Leo-I group. Once detected, we perform surface photometry and compare their structural parameters to other known dwarf galaxies in the nearby universe. Results. We found 36 new dwarf galaxy candidates within the search area. Their morphology and structural parameters resemble known dwarfs in other groups. Among the candidates 5 to 6 galaxies are considered as ultra diffuse galaxies candidates. If confirmed, they would be some of the closest examples of this galaxy type. -
ALABAMA University Libraries
THE UNIVERSITY OF ALABAMA University Libraries Hot Diffuse Emission in the Nuclear Starburst Region of NGC 2903 Jimmy A. Irwin – University of Alabama et al. Deposited 09/12/2018 Citation of published version: Yukita, M., et al. (2012): Hot Diffuse Emission in the Nuclear Starburst Region of NGC 2903. The Astrophysical Journal, 758(2). http://dx.doi.org/10.1088/0004-637X/758/2/105 © 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. The Astrophysical Journal, 758:105 (17pp), 2012 October 20 doi:10.1088/0004-637X/758/2/105 C 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A. HOT DIFFUSE EMISSION IN THE NUCLEAR STARBURST REGION OF NGC 2903 Mihoko Yukita1, Douglas A. Swartz2, Allyn F. Tennant3, Roberto Soria4, and Jimmy A. Irwin1 1 Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487, USA 2 Universities Space Research Association, NASA Marshall Space Flight Center, ZP12, Huntsville, AL 35812, USA 3 Space Science Office, NASA Marshall Space Flight Center, ZP12, Huntsville, AL 35812, USA 4 International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, WA 6845, Australia Received 2012 June 14; accepted 2012 August 30; published 2012 October 5 ABSTRACT We present a deep Chandra observation of the central regions of the late-type barred spiral galaxy NGC 2903. The Chandra data reveal soft (kTe ∼ 0.2–0.5 keV) diffuse emission in the nuclear starburst region and extending ∼2 (∼5 kpc) to the north and west of the nucleus. Much of this soft hot gas is likely to be from local active star-forming regions; however, besides the nuclear region, the morphology of hot gas does not strongly correlate with the bar or other known sites of active star formation. -
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%2/(7Ì1 '( /$ $*583$&,Ð1 $67521Ð0,&$ 9,=&$,1$ %,=.$,.2 $6752120, (/.$57($ GALILEO 1998 2º TRIMESTRE AÑO II Nº 5 (Q HVWH Q~PHUR 0RQWDMHV SUiFWLFRV (IHPpULGHV 3ODQHWDULDV 2EVHUYDFLRQHV GH OD $$9 /RV FDPLQRV GHO FLHOR $VWURIRWRJUDItD 1RWLFLDV EUHYHV 0DSDV GHO &LHOR GALILEO ,1',&( '( $57Ì&8/26 Boletín de la Pág. AGRUPACIÓN ASTRONÓMICA VIZCAINA Cómo poner un telescopio en estación........... 3 BIZKAIKO ASTRONOMI ELKARTEA Cálculos horarios........................................... 4 Sede: Locales del Departamento de Cultura de la Di- Taller: Una máscara de enfoque .................... 6 putación Foral de Vizcaya - Bizkaiko Foru Al- dundia. c/ Iparragirre 46, 5º - 4. Bilbao Los caminos del cielo: Leo y C. Berenices...... 7 Apertura de locales: Martes y Miércoles de 19:30 a Informes de observación de la AAV ............... 9 21:00 Depósito legal: BI-420-92 Las extraordinarias dobles de Boötes ...........11 Este ejemplar se distribuye de forma gratuita a los so- El Cielo este trimestre...................................14 cios y colaboradores de la A.A.V. - B.A.E. Cámaras de vídeo en astronomía.................17 La A.A.V. - B.A.E. no se hace responsable del conteni- do de los artículos ni de las opiniones vertidas en ellos Previ-observación. Climatología ....................20 por sus autores. Ráfagas de Rayos Gamma...........................21 Prohibida la reproducción total o parcial de los conte- nidos de cualquier información gráfica o escrita por Observando el Sol........................................22 cualquier medio, sin permiso escrito de la AAV. Efemérides planetarias .................................24 BREVES * INTERNET * ASTRONOMIA * BREVES * INTERNET * ASTRONOMIA * BREVES * INTERNET * ASTRONOMIA EL HUBBLE DESCUBRE QUE HASTA LAS ESTRELLAS MASIVAS DESAPARECEN POCO A POCO (9-4-98) Apuntando al rápido oscurecimiento de una estrella recientemente apagada, el Telescopio Espacial Hubble está dando a los astrónomos una mejor estimación sobre como solamente una gran estrella puede ser antes una estrella antes de que explote como una supernova. -
MESSIER 15 RA(2000) : 21H 29M 58S DEC(2000): +12° 10'
MESSIER 15 RA(2000) : 21h 29m 58s DEC(2000): +12° 10’ 01” BASIC INFORMATION OBJECT TYPE: Globular Cluster CONSTELLATION: Pegasus BEST VIEW: Late October DISCOVERY: Jean-Dominique Maraldi, 1746 DISTANCE: 33,600 ly DIAMETER: 175 ly APPARENT MAGNITUDE: +6.2 APPARENT DIMENSIONS: 18’ FOV:Starry 1.00Night FOV: 60.00 Vulpecula Sagitta Pegasus NGC 7009 (THE SATURN NEBULA) Delphinus NGC 7009 RA(2000) : 21h 04m 10.8s DEC(2000): -11° 21’ 48.6” Equuleus Pisces Aquila NGC 7009 FOV: 5.00 Aquarius Telrad Capricornus Sagittarius Cetus Piscis Austrinus NGC 7009 Microscopium BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Aquarius Sculptor BEST VIEW: Early November DISCOVERY: William Herschel, 1782 DISTANCE: 2000 - 4000 ly DIAMETER: 0.4 - 0.8 ly Grus APPARENT MAGNITUDE: +8.0 APPARENT DIMENSIONS: 41” x 35” Telescopium Telrad Indus NGC 7662 (THE BLUE SNOWBALL) RA(2000) : 23h 25m 53.6s DEC(2000): +42° 32’ 06” BASIC INFORMATION OBJECT TYPE: Planetary Nebula CONSTELLATION: Andromeda BEST VIEW: Late November DISCOVERY: William Herschel, 1784 DISTANCE: 1800 – 6400 ly DIAMETER: 0.3 – 1.1 ly APPARENT MAGNITUDE: +8.6 APPARENT DIMENSIONS: 37” MESSIER 52 RA(2000) : 23h 24m 48s DEC(2000): +61° 35’ 36” BASIC INFORMATION OBJECT TYPE: Open Cluster CONSTELLATION: Cassiopeia BEST VIEW: December DISCOVERY: Charles Messier, 1774 DISTANCE: ~5000 ly DIAMETER: 19 ly APPARENT MAGNITUDE: +7.3 APPARENT DIMENSIONS: 13’ AGE: 50 million years FOV:Starry 1.00Night FOV: 60.00 Auriga Cepheus Andromeda MESSIER 31 (THE ANDROMEDA GALAXY) M 31 RA(2000) : 00h 42m 44.3Cassiopeias DEC(2000): +41° 16’ 07.5” Perseus Lacerta AndromedaM 31 FOV: 5.00 Telrad Triangulum Taurus Orion Aries Andromeda M 31 Pegasus Pisces BASIC INFORMATION OBJECT TYPE: Galaxy CONSTELLATION: Andromeda Telrad BEST VIEW: December DISCOVERY: Abd al-Rahman al-Sufi, 964 Eridanus CetusDISTANCE: 2.5 million ly DIAMETER: ~250,000 ly* APPARENT MAGNITUDE: +3.4 APPARENT DIMENSIONS: 178’ x 63’ (3° x 1°) *This value represents the total diameter of the disk, based on multi-wavelength measurements. -
April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86. -
GTO Keypad Manual, V5.001
ASTRO-PHYSICS GTO KEYPAD Version v5.xxx Please read the manual even if you are familiar with previous keypad versions Flash RAM Updates Keypad Java updates can be accomplished through the Internet. Check our web site www.astro-physics.com/software-updates/ November 11, 2020 ASTRO-PHYSICS KEYPAD MANUAL FOR MACH2GTO Version 5.xxx November 11, 2020 ABOUT THIS MANUAL 4 REQUIREMENTS 5 What Mount Control Box Do I Need? 5 Can I Upgrade My Present Keypad? 5 GTO KEYPAD 6 Layout and Buttons of the Keypad 6 Vacuum Fluorescent Display 6 N-S-E-W Directional Buttons 6 STOP Button 6 <PREV and NEXT> Buttons 7 Number Buttons 7 GOTO Button 7 ± Button 7 MENU / ESC Button 7 RECAL and NEXT> Buttons Pressed Simultaneously 7 ENT Button 7 Retractable Hanger 7 Keypad Protector 8 Keypad Care and Warranty 8 Warranty 8 Keypad Battery for 512K Memory Boards 8 Cleaning Red Keypad Display 8 Temperature Ratings 8 Environmental Recommendation 8 GETTING STARTED – DO THIS AT HOME, IF POSSIBLE 9 Set Up your Mount and Cable Connections 9 Gather Basic Information 9 Enter Your Location, Time and Date 9 Set Up Your Mount in the Field 10 Polar Alignment 10 Mach2GTO Daytime Alignment Routine 10 KEYPAD START UP SEQUENCE FOR NEW SETUPS OR SETUP IN NEW LOCATION 11 Assemble Your Mount 11 Startup Sequence 11 Location 11 Select Existing Location 11 Set Up New Location 11 Date and Time 12 Additional Information 12 KEYPAD START UP SEQUENCE FOR MOUNTS USED AT THE SAME LOCATION WITHOUT A COMPUTER 13 KEYPAD START UP SEQUENCE FOR COMPUTER CONTROLLED MOUNTS 14 1 OBJECTS MENU – HAVE SOME FUN!