Messier 54 Globular Cluster in the Constellation Sagittarius Plus M55 - M69 - M70 and M75
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
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. -
Midwife of the Galactic Zoo
FOCUS 30 A miniature milky way: approximately 40 million light-years away, UGC 5340 is classified as a dwarf galaxy. Dwarf galaxies exist in a variety of forms – elliptical, spheroidal, spiral, or irregular – and originate in small halos of dark matter. Dwarf galaxies contain the oldest known stars. Max Planck Research · 4 | 2020 FOCUS MIDWIFE OF THE GALACTIC ZOO TEXT: THOMAS BÜHRKE 31 IMAGE: NASA, TEAM ESA & LEGUS Stars cluster in galaxies of dramatically different shapes and sizes: elliptical galaxies, spheroidal galaxies, lenticular galaxies, spiral galaxies, and occasionally even irregular galaxies. Nadine Neumayer at the Max Planck Institute for Astronomy in Heidelberg and Ralf Bender at the Max Planck Institute for Extraterrestrial Physics in Garching investigate the reasons for this diversity. They have already identified one crucial factor: dark matter. Max Planck Research · 4 | 2020 FOCUS Nature has bestowed an overwhelming diversity upon our planet. The sheer resourcefulness of the plant and animal world is seemingly inexhaustible. When scien- tists first started to explore this diversity, their first step was always to systematize it. Hence, the Swedish naturalist Carl von Linné established the principles of modern botany and zoology in the 18th century by clas- sifying organisms. In the last century, astronomers have likewise discovered that galaxies can come in an array of shapes and sizes. In this case, it was Edwin Hubble in the mid-1920s who systematized them. The “Hubble tuning fork dia- gram” classified elliptical galaxies according to their ellipticity. The series of elliptical galaxies along the di- PHOTO: PETER FRIEDRICH agram branches off into two arms: spiral galaxies with a compact bulge along the upper branch and galaxies with a central bar on the lower branch. -
VISTA Views a Vast Ball of Stars 9 May 2012
VISTA views a vast ball of stars 9 May 2012 sphere with a diameter of only about 25 times the distance between the Sun and the nearest star system, Alpha Centauri. About 160 globular clusters have been spotted encircling our galaxy, the Milky Way, mostly toward its bulging centre. The two latest discoveries, made using VISTA, were recently announced. The largest galaxies can have thousands of these rich collections of stars in orbit around them. Observations of globular clusters' stars reveal that they originated around the same time - more than 10 billion years ago - and from the same cloud of gas. As this formative period was just a few billion years after the Big Bang, nearly all of the gas on hand was the simplest, lightest and most common in the cosmos: hydrogen, along with some helium and much smaller amounts of heavier chemical elements such as oxygen and nitrogen. This striking view of the globular star cluster Messier 55 Being made mostly from hydrogen distinguishes in the constellation of Sagittarius (The Archer) was globular cluster residents from stars born in later obtained in infrared light with the VISTA survey eras, like our Sun, that are infused with heavier telescope at ESO's Paranal Observatory in Chile. This elements created in earlier generations of stars. vast ball of ancient stars is located at a distance of about The Sun lit up some 4.6 billion years ago, making it 17,000 light-years from Earth. Credit: ESO/J. only about half as old as the elderly stars in most Emerson/VISTA. -
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. -
Prime Focus (11-08)
Highlights of the November Sky. -- -- -- 1st -- -- -- Dusk: Thin crescent Moon appears 7º or 8º to the left PPrime Focuss of Venus. A Publication of the Kalamazoo Astronomical Society -- -- -- 2nd -- -- -- AM: Saturn 0.1º from 4.0 magnitude star Sigma November 2008 Leonis (use telescope). -- -- -- 3rd -- -- -- PM: Crescent Moon less than 3º to Jupiter’s lower ThisThis MonthsMonths KAS EventsEvents left.left. -- -- -- 5th -- -- -- First Quarter Moon General Meeting: Friday, November 7 @ 7:00 pm -- -- -- 13th -- -- -- Kalamazoo Math & Science Center - See Page 12 for Details Full Moon Field Trip: Saturday, November 8 @ 5:00 pm -- -- -- 17th -- -- -- Dusk: Venus appears 5′′ toto Abrams Planetarium & MSU Observatory - See Page 3 for Details 8′′ belowbelow 2.82.8 magnitudemagnitude Lambda Sagittarii. Board Meeting: Sunday, November 9 @ 5:00 pm -- -- -- 19th -- -- -- Sunnyside Church - 2800 Gull Road - All Members Welcome Last Quarter Moon -- -- -- 21st -- -- -- AM: Crescent Moon about 5º to Saturn’s right. Inside the Newsletter. -- -- -- 24th -- -- -- Inside the Newsletter. PM: Venus 1º to the upper right of 2.1 magnitude October Meeting Minutes.................... p. 2 Sigma Sagittarii. Board Meeting Minutes......................... p. 3 -- -- -- 27th -- -- -- New Moon Field Trip Itinerary................................. p. 3 Starbooks................................................. p. 4 -- -- -- 29th -- -- -- Dusk: Thin crescent Moon Great Lakes Star Gaze Report............ p. 5 very low in southwest, about 20º lower right of The Almost Perfect Night.................... p. 7 Venus and Jupiter. Sneak Peak Inside Comet Holmes...... p. 9 -- -- -- 30th -- -- -- November Night Sky............................. p. 10 PM: Jupiter only 2º from Venus. KAS Officers & Announcements........ p. 11 Crescent Moon about 8º to General Meeting Preview..................... p. 12 the planet’s lower right. www.kasonline.org OctoberOctober MeetingMeeting MinuteMinutess The general meeting of the Kalamazoo Astronomical Society Photographing the Sun and Moon were then covered. -
Astronomía Con Ordenador II, Crédito Variable De Ciencias Naturales De 1º De Bachillerato, Durante El Curso 2007/2008
Astronomía II [email protected] 1 ASTRONOMÍA con ORDENADOR II Fermí Vilà Astronomía II [email protected] 2 Índice Introducción................................................................................................................................3 1ª Parte: VIDA Y MUERTE DE LAS ESTRELLAS Nacimiento de una estrella: Etapa Nebulosa...............................................................................5 Nacimiento de una estrella: Etapa de Protoestrella...................................................................13 La Secuencia Principal..............................................................................................................19 Enanas Marrones: Estrellas Fallidas.........................................................................................27 Gigantes Rojas y Supergigantes................................................................................................29 La Muerte de la Tierra y los planetas interiores........................................................................31 ¿Un nuevo comienzo en Plutón?...............................................................................................35 Muerte de una Gigante Roja. Nebulosa Planetaria...................................................................36 Enanas Blancas.........................................................................................................................39 Enanas Negras...........................................................................................................................41 -
Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects
Juliana Crestani Ribeiro de Souza Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects Porto Alegre 2017 Juliana Crestani Ribeiro de Souza Spatial Distribution of Galactic Globular Clusters: Distance Uncertainties and Dynamical Effects Dissertação elaborada sob orientação do Prof. Dr. Eduardo Luis Damiani Bica, co- orientação do Prof. Dr. Charles José Bon- ato e apresentada ao Instituto de Física da Universidade Federal do Rio Grande do Sul em preenchimento do requisito par- cial para obtenção do título de Mestre em Física. Porto Alegre 2017 Acknowledgements To my parents, who supported me and made this possible, in a time and place where being in a university was just a distant dream. To my dearest friends Elisabeth, Robert, Augusto, and Natália - who so many times helped me go from "I give up" to "I’ll try once more". To my cats Kira, Fen, and Demi - who lazily join me in bed at the end of the day, and make everything worthwhile. "But, first of all, it will be necessary to explain what is our idea of a cluster of stars, and by what means we have obtained it. For an instance, I shall take the phenomenon which presents itself in many clusters: It is that of a number of lucid spots, of equal lustre, scattered over a circular space, in such a manner as to appear gradually more compressed towards the middle; and which compression, in the clusters to which I allude, is generally carried so far, as, by imperceptible degrees, to end in a luminous center, of a resolvable blaze of light." William Herschel, 1789 Abstract We provide a sample of 170 Galactic Globular Clusters (GCs) and analyse its spatial distribution properties. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
RASC Toronto Centre – the Sky This Month – Spring Galaxy Edition II April 29 to May 27, 2020 (Times in EDT, UT-4) by Chris Vaughan
RASC Toronto Centre – www.rascto.ca The Sky This Month – Spring Galaxy Edition II April 29 to May 27, 2020 (times in EDT, UT-4) by Chris Vaughan NEWS Space Exploration – Public and Private Ref. http://spaceflightnow.com/launch-schedule/ Launches Most launches by multiple countries are TBD May 27 tbd - SpaceX Falcon 9 rocket from Cape Canaveral Air Force Station, Florida, SpaceX Crew Dragon Capsule test flight to/from ISS with “Bob and Doug” (Douglas Hurley and Robert Behnken). NASA says no in-person public viewing May 5 tbd - Long March 5b rocket from Wenchang, China, new Chinese Crew Capsule test flight and high- speed re-entry without crew of 20 metric ton version designed for deep space (beyond LEO). Capsule can launch 6 persons or 3 persons with 500 kg of cargo This Month in History (a sampling) Ref. http://www2.jpl.nasa.gov/calendar/, http://www.planetary.org/multimedia/space-images/charts/whats- up-in-the-solar-system-frohn.html, http://www.lunar-occultations.com/rlo/calendar.pdf Astro-Birthdays and Milestones May 1, 1825 – Swiss mathematician Johann Jakob Balmer, formulated formula for spectral emission lines of Hydrogen. May 10, 1900 – Pioneering female British-American astronomer Cecilia Payne-Gaposchkin, earned the first PhD from Harvard’s Radcliffe College, on stellar composition. She surveyed all stars brighter than 10th mag. and millions of variable stars, setting the foundations of stellar evolution studies. Also supervised Helen Sawyer-Hogg and others. May 15, 1857 - Scottish astronomer, Williamina Fleming. In nine years, she catalogued more than 10,000 stars. During her work, she discovered 59 gaseous nebulae (including the Horsehead Nebula), over 310 variable stars, and 10 novae. -
CALENDARIO ASTRONOMICO Per L'anno Bisestile
CALENDARIO ASTRONOMICO per l’anno bisestile 2016 (Anno Internazionale delle Leguminose) con tabelle di Cronologia comparata con i Calendari Ortodosso, Copto, Israelita, Musulmano e Cinese Elaborato da LUCIANO UGOLINI Astrofilo di PRATO (Toscana) Componente dell’ASSOCIAZIONE ASTRONOMICA QUASAR presso CENTRO DI SCIENZE NATURALI di GALCETI – PRATO La pubblicazione di questo Calendario è sostenuta dal C.A.A.T. - Coordinamento delle Associazioni Astrofile della Toscana – www.astrocaat.it – [email protected] Il C.A.A.T. è: ollaoazioe ta gli astofili tosai, attività ossevativa, poozioe dell’astooia aatoiale ella osta egioe, incontri e seminari di aggiornamento, sensibilizzazione sul polea dell’iuiaeto luioso. Differenza ET-UT adottata per l’ao 16 = +68 secondi. Gli orari delle congiunzioni fra Luna, Pianeti e Stelle e la loro separazione angolare, si riferiscono all’istate della loro iia distaza e sono indicati per il centro della Terra. Gli orari del sorgere, culminare e tramontare del Sole e della Luna soo espressi per l’orizzote astrooio di Prato Piazza del Coue - Latitudine: ° ’ 8” Nord - Logitudie: ° ’ ” Est da Greeih. Le correzioni da apportare unicamente agli istanti del sorgere, culminare e tramontare degli astri, rispetto a quelle indicate, per altre città della Toscana, sono minime e riconducibili, al massimo, a pochi minuti in più o in meno. Gli altri orari indicati nel presete Caledario o eessitao di alua orrezioe e algoo per tutta l’Italia. Tutti i tepi soo espressi i T.M.E.C. Tepo Medio dell’Europa Cetrale he è il Tepo Ciile segato dai ostri orologi. Non viene tenuto conto dell’aueto di iuti douto all’ora estia, attualete i igore i Italia dall’ultia Doeia di Marzo all’ultia Doeia di Ottore. -
121012-AAS-221 Program-14-ALL, Page 253 @ Preflight
221ST MEETING OF THE AMERICAN ASTRONOMICAL SOCIETY 6-10 January 2013 LONG BEACH, CALIFORNIA Scientific sessions will be held at the: Long Beach Convention Center 300 E. Ocean Blvd. COUNCIL.......................... 2 Long Beach, CA 90802 AAS Paper Sorters EXHIBITORS..................... 4 Aubra Anthony ATTENDEE Alan Boss SERVICES.......................... 9 Blaise Canzian Joanna Corby SCHEDULE.....................12 Rupert Croft Shantanu Desai SATURDAY.....................28 Rick Fienberg Bernhard Fleck SUNDAY..........................30 Erika Grundstrom Nimish P. Hathi MONDAY........................37 Ann Hornschemeier Suzanne H. Jacoby TUESDAY........................98 Bethany Johns Sebastien Lepine WEDNESDAY.............. 158 Katharina Lodders Kevin Marvel THURSDAY.................. 213 Karen Masters Bryan Miller AUTHOR INDEX ........ 245 Nancy Morrison Judit Ries Michael Rutkowski Allyn Smith Joe Tenn Session Numbering Key 100’s Monday 200’s Tuesday 300’s Wednesday 400’s Thursday Sessions are numbered in the Program Book by day and time. Changes after 27 November 2012 are included only in the online program materials. 1 AAS Officers & Councilors Officers Councilors President (2012-2014) (2009-2012) David J. Helfand Quest Univ. Canada Edward F. Guinan Villanova Univ. [email protected] [email protected] PAST President (2012-2013) Patricia Knezek NOAO/WIYN Observatory Debra Elmegreen Vassar College [email protected] [email protected] Robert Mathieu Univ. of Wisconsin Vice President (2009-2015) [email protected] Paula Szkody University of Washington [email protected] (2011-2014) Bruce Balick Univ. of Washington Vice-President (2010-2013) [email protected] Nicholas B. Suntzeff Texas A&M Univ. suntzeff@aas.org Eileen D. Friel Boston Univ. [email protected] Vice President (2011-2014) Edward B. Churchwell Univ. of Wisconsin Angela Speck Univ. of Missouri [email protected] [email protected] Treasurer (2011-2014) (2012-2015) Hervey (Peter) Stockman STScI Nancy S.