Cielo Nocturno De Abril De 2021 Esta Carta Está Calculada Para Un Observador Situado En Una Latitud De 40º Norte

Total Page:16

File Type:pdf, Size:1020Kb

Cielo Nocturno De Abril De 2021 Esta Carta Está Calculada Para Un Observador Situado En Una Latitud De 40º Norte Cielo Nocturno de Abril de 2021 Esta carta está calculada para un observador situado en una latitud de 40º Norte. Representa el cielo que puede verse desde la ciudad de Valencia a mediados de abril, a las 21.00 hora local. LEYENDA 0 magnitud 1 magnitud 2 magnitud 3 magnitud 4 magnitud 5 magnitud Objeto cielo profundo Venus POSICIÓN DE LOS PLANETAS SOBRE EL HORIZONTE 90 º Mediados de abril, a las 21:00 90 Mediados de abril, a las 05:30 hora local hora local 60 º 60 Saturno 30 º 30 Venus Júpiter Venus se ve a escasa altura sobre el horizonte Oeste –Noroeste tras la puesta del Sol. Júpiter es visible horas antes del amanecer sobre el horizonte Sureste. Saturno se observa de madrugada, en Capricornio. *Para conocer los pasos de la ISS durante el mes de abril consulta la siguiente página web: https://goo.gl/hKkZDz LA ESTRELLA DEL MES: pos estelares que alberga este asterismo. Dentro de los cúmulos que se pueden ob- servar en la constelación de Vela, el cúmulo VELA Entre los más notorios por su belleza y/o relevancia se hallan la Nebulosa del Anillo abierto de Omicron Velorum (IC 2391 o La constelación Vela es la última de las sec- del Sur (NGC 3132). Es la nebulosa planeta- Caldwell 85) es de los fáciles de localizar y ciones en las que fue dividida la constela- ria más brillante de la constelación de Vela. ver, ya que es visible a simple vista. Forma- ción de Argos Navis. Localizada en el hemis- Se encuentra a unos 2.000 años luz de dis- do por algo más de 30 estrellas, se haya a ferio sur representa a las velas del mítico tancia del Sol, y se la considera la versión unos 500 años luz de la Tierra. Otro magni- navío Argos. austral de la Nebulosa del Anillo de la cons- fico cúmulo es, sin duda, NGC 3201 Al igual que la constelación de Puppis, sus telación de Lyra. Otra de las nebulosas a (Caldwell 79). Con una edad de alrededor estrellas más brillantes no están identifica- mencionar es la Nebulosa Gum (Gum 12). 10,24 miles de millones de años, este cú- das por las primeras letras del alfabeto grie- Se trata de una nebulosa de emisión que mulo globular está formado mayoritaria- go. De esta forma, la estrella principal es cubre una gran área del cielo, y dista de la mente por estrellas viejas, entre las cuales gamma Velorum, mientras que la segunda y Tierra unos 400 parsecs (1 parsec son 3,26 predominan las gigantes rojas. tercera estrellas en brillo son Alsephina años luz). En su interior nos encontramos Como curiosidad, mencionar que dos de las (delta Velorum) y Suhail (lambda Velorum) con otro extraordinario objeto, como es el estrellas de Vela - Alsephina (delta Ve- respectivamente. Remanente de supernova de Vela (Gum lorum), Markeb (kappa Velorum)- junto con En la constelación de Vela podemos hablar 16), que a su vez tiene asociados dos obje- otras dos estrellas de la constelación de sobre innumerables objetos de cielo pro- tos más: la Nebulosa del Lápiz (NGC 2736) y Carina -Aspidiske (iota Carinae) y Avior fundo, cada uno de los cuales destaca o el Pulsar de Vela (PSR B0833-45). Este pul- (epsilon Carinae) – forman el asterismo que presenta características y particularidades sar jugó un papel muy importante ya que, se conoce como la falsa Cruz, porque se extraordinarias, hermosas y fascinantes. gracias a su descubrimiento, quedó confir- suele confundir con la constelación de la Desde nebulosas planetarias, pulsares, cú- mado que las supernovas dan lugar a estre- Cruz del Sur. mulos abiertos y cerrados, hasta regiones llas de neutrones. de formación estelar, son los tipos de cuer- TABLA DE ORTOS Y OCASOS DEL SOL Y LA LUNA Lunes Martes Miércoles Jueves Viernes Sábado Domingo Cuarto menguante EFEMÉRIDES: La noche del 22 tendrá lugar el máximo de la lluvia de 1 2 3 4 estrellas de las Líridas. El 27 de abril será la primera superluna del año. Orto: 07:46 Ocaso: 10:11 Orto: 07:44 Orto: 01:12 Orto: 07:43 Orto: 02:24 Orto: 07:41 Orto: 03:28 Ocaso: 20:26 Ocaso: 20:27 Ocaso: 10:54 Ocaso: 20:28 Ocaso: 11:46 Ocaso: 20:29 Ocaso: 11:46 5 6 7 8 9 10 11 Orto: 07:39 Orto: 04:22 Orto: 07:38 Orto: 05:08 Orto: 07:36 Orto: 05:45 Orto: 07:35 Orto: 06:16 Orto: 07:33 Orto: 06:44 Orto: 07:32 Orto: 07:08 Orto: 07:30 Orto: 07:31 Ocaso: 20:30 Ocaso: 12:44 Ocaso: 20:30 Ocaso: 14:53 Ocaso: 20:31 Ocaso: 15:59 Ocaso: 20:32 Ocaso: 17:03 Ocaso: 20:33 Ocaso: 18:05 Ocaso: 20:34 Ocaso: 19:05 Ocaso: 20:35 Ocaso: 20:04 Luna nueva 12 13 14 15 16 17 18 Orto: 09:15 Orto: 07:29 Orto: 07:54 Orto: 07:27 Orto: 08:18 Orto: 07:26 Orto: 08:44 Orto: 07:24 Orto: 07:23 Orto: 05:04 Orto: 07:21 Ocaso: 00:01 Orto: 07:20 Ocaso: 01:57 Ocaso: 20:36 Ocaso: 21:03 Ocaso: 20:37 Ocaso: 22:02 Ocaso: 20:38 Ocaso: 23:02 Ocaso: 20:39 Ocaso: 20:40 Ocaso: 15:25 Ocaso: 20:41 Orto: 10:27 Ocaso: 20:42 Orto: 11:13 Cuarto creciente 19 20 21 22 23 24 25 Orto: 07:18 Ocaso: 02:49 Orto: 07:17 Ocaso: 03:36 Orto: 07:16 Ocaso: 04:18 Orto: 07:14 Ocaso: 04:54 Orto: 07:13 Ocaso: 05:27 Orto: 07:12 Ocaso: 05:57 Orto: 07:10 Ocaso: 06:26 Ocaso: 20:43 Orto: 12:06 Ocaso: 20:44 Orto: 13:06 Ocaso: 20:45 Orto: 14:11 Ocaso: 20:46 Orto: 15:19 Ocaso: 20:47 Orto: 16:30 Ocaso: 20:48 Orto: 17:42 Ocaso: 20:49 Orto: 18:56 Luna llena 26 27 28 29 30 Ocaso: 06:55 Ocaso: 07:27 Ocaso: 08:03 Ocaso: 08:45 Orto: 07:09 Orto: 07:08 Orto: 07:06 Orto: 07:05 Orto: 07:04 Orto: 00:06 Ocaso: 20:50 Orto: 20:12 Ocaso: 20:51 Orto: 21:30 Ocaso: 20:52 Orto: 22:49 Ocaso: 20:53 Orto: 03:50 Ocaso: 20:54 Ocaso: 09:34 ¿QUÉ OCURRIÓ EN MARZO? El hallazgo de materiales orgánicos en la superficie del asteroide Itokawa indica que los meteoritos de asteroides similares podrían haber proporcio- nado los precursores químicos para la aparición de la vida en la Tierra. En el planeta GJ 1132 b los gases producidos por volcanes activos están creando una segunda atmósfera, tras haber perdido la original al ser absor- bida por el manto de magma fundido que cubre el planeta. Un nuevo estudio afirma que entre el 30% y el 99% del agua que existía en Marte en el pasado está contenida en minerales dentro de la corteza del planeta, contradiciendo la teoría actual que sostiene que, debido a la baja gravedad del planeta rojo, su agua escapó al espacio. .
Recommended publications
  • 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.
    [Show full text]
  • The Nearby Eclipsing Stellar System Delta Velorum - IV
    The nearby eclipsing stellar system delta Velorum - IV. Differential astrometry with VLT/NACO at the 100 microarcsecond level Pierre Kervella, Antoine Mérand, Monika Petr-Gotzens, Theo Pribulla, Frédéric Thévenin To cite this version: Pierre Kervella, Antoine Mérand, Monika Petr-Gotzens, Theo Pribulla, Frédéric Thévenin. The nearby eclipsing stellar system delta Velorum - IV. Differential astrometry with VLT/NACO at the 100 microarcsecond level. 2013. hal-00793521 HAL Id: hal-00793521 https://hal.archives-ouvertes.fr/hal-00793521 Preprint submitted on 22 Feb 2013 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Astronomy & Astrophysics manuscript no. DelVel4-Astrom-v3r1 c ESO 2013 February 23, 2013 The nearby eclipsing stellar system δ Velorum IV. Differential astrometry with VLT/NACO at the 100 microarcsecond level ? P. Kervella1, A. Mérand2, M. G. Petr-Gotzens3, T. Pribulla4, and F. Thévenin5 1 LESIA, Observatoire de Paris, CNRS UMR 8109, UPMC, Université Paris Diderot, 5 place Jules Janssen, 92195 Meudon, France 2 European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Santiago 19, Chile 3 European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany 4 Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia 5 Université de Nice-Sophia Antipolis, Lab.
    [Show full text]
  • CONFERENCE and REVIEW PUBLICATONS, and WHITE PAPERS: Reverse Chronological Harper, GM, 2013
    CONFERENCE AND REVIEW PUBLICATONS, AND WHITE PAPERS: Reverse Chronological Harper, G. M., 2013, [Invited Review] Atmospheric structure and dynamics: the spatial and temporal domains, EAS Publications Series, Vol 60, 2013, pp.59-68 Farzone, M., Ryde, N., Harper, G. M., Lambert, J., Josselin, E., Richter, M. J., & Eriksson, K., 2013, What is the Origin of the Water Vapour Signatures in Red Giant Stars?, EAS Publications Series, Vol 60, pp.155-159 Carpenter, K. G., Ayres, T., Brown, A., Harper, G. M., & Wahlgren, G. M., 2012. The Amazing COS FUV (1320 - 1460A)˚ Spectrum of λ Vel (K4Ib-II), 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. Eds. C. M. Johns-Krull, M. K. Browning, and A. A. West. San Francisco: ASP Conf Ser., Vol. 448, p.1083 Harper, G. M., Brown, A., & Redfield, S., 2012, Constraints on the Surface Magnetic Field Structure of Aldebaran (αTauri, K5 III), 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. Eds. C. M. Johns-Krull, M. K. Browning, and A. A. West. San Francisco: ASP Conf Ser., Vol. 448, p.1145 O’Gorman, E. & Harper, G. M., 2012, What is Heating Arcturus’ Wind?, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun. Eds. C. M. Johns-Krull, M. K. Browning, and A. A. West. San Francisco: ASP Conf Ser., Vol. 448, p.691 van Belle, G. T., Aufdenberg, J., Boyajian, T., Harper G. M., Hummel, C., Pedretti, E., Baines, E., White, R., Ravi, V., & Ridgway, S., 2012, Fundamental Stellar Properties from Optical Interferometry, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun.
    [Show full text]
  • 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!
    [Show full text]
  • 407 a Abell Galaxy Cluster S 373 (AGC S 373) , 351–353 Achromat
    Index A Barnard 72 , 210–211 Abell Galaxy Cluster S 373 (AGC S 373) , Barnard, E.E. , 5, 389 351–353 Barnard’s loop , 5–8 Achromat , 365 Barred-ring spiral galaxy , 235 Adaptive optics (AO) , 377, 378 Barred spiral galaxy , 146, 263, 295, 345, 354 AGC S 373. See Abell Galaxy Cluster Bean Nebulae , 303–305 S 373 (AGC S 373) Bernes 145 , 132, 138, 139 Alnitak , 11 Bernes 157 , 224–226 Alpha Centauri , 129, 151 Beta Centauri , 134, 156 Angular diameter , 364 Beta Chamaeleontis , 269, 275 Antares , 129, 169, 195, 230 Beta Crucis , 137 Anteater Nebula , 184, 222–226 Beta Orionis , 18 Antennae galaxies , 114–115 Bias frames , 393, 398 Antlia , 104, 108, 116 Binning , 391, 392, 398, 404 Apochromat , 365 Black Arrow Cluster , 73, 93, 94 Apus , 240, 248 Blue Straggler Cluster , 169, 170 Aquarius , 339, 342 Bok, B. , 151 Ara , 163, 169, 181, 230 Bok Globules , 98, 216, 269 Arcminutes (arcmins) , 288, 383, 384 Box Nebula , 132, 147, 149 Arcseconds (arcsecs) , 364, 370, 371, 397 Bug Nebula , 184, 190, 192 Arditti, D. , 382 Butterfl y Cluster , 184, 204–205 Arp 245 , 105–106 Bypass (VSNR) , 34, 38, 42–44 AstroArt , 396, 406 Autoguider , 370, 371, 376, 377, 388, 389, 396 Autoguiding , 370, 376–378, 380, 388, 389 C Caldwell Catalogue , 241 Calibration frames , 392–394, 396, B 398–399 B 257 , 198 Camera cool down , 386–387 Barnard 33 , 11–14 Campbell, C.T. , 151 Barnard 47 , 195–197 Canes Venatici , 357 Barnard 51 , 195–197 Canis Major , 4, 17, 21 S. Chadwick and I. Cooper, Imaging the Southern Sky: An Amateur Astronomer’s Guide, 407 Patrick Moore’s Practical
    [Show full text]
  • Annual Report / Rapport Annuel / Jahresbericht 1996
    Annual Report / Rapport annuel / Jahresbericht 1996 ✦ ✦ ✦ E U R O P E A N S O U T H E R N O B S E R V A T O R Y ES O✦ 99 COVER COUVERTURE UMSCHLAG Beta Pictoris, as observed in scattered light Beta Pictoris, observée en lumière diffusée Beta Pictoris, im Streulicht bei 1,25 µm (J- at 1.25 microns (J band) with the ESO à 1,25 microns (bande J) avec le système Band) beobachtet mit dem adaptiven opti- ADONIS adaptive optics system at the 3.6-m d’optique adaptative de l’ESO, ADONIS, au schen System ADONIS am ESO-3,6-m-Tele- telescope and the Observatoire de Grenoble télescope de 3,60 m et le coronographe de skop und dem Koronographen des Obser- coronograph. l’observatoire de Grenoble. vatoriums von Grenoble. The combination of high angular resolution La combinaison de haute résolution angu- Die Kombination von hoher Winkelauflö- (0.12 arcsec) and high dynamical range laire (0,12 arcsec) et de gamme dynamique sung (0,12 Bogensekunden) und hohem dy- (105) allows to image the disk to only 24 AU élevée (105) permet de reproduire le disque namischen Bereich (105) erlaubt es, die from the star. Inside 50 AU, the main plane jusqu’à seulement 24 UA de l’étoile. A Scheibe bis zu einem Abstand von nur 24 AE of the disk is inclined with respect to the l’intérieur de 50 UA, le plan principal du vom Stern abzubilden. Innerhalb von 50 AE outer part. Observers: J.-L. Beuzit, A.-M.
    [Show full text]
  • Atlas Menor Was Objects to Slowly Change Over Time
    C h a r t Atlas Charts s O b by j Objects e c t Constellation s Objects by Number 64 Objects by Type 71 Objects by Name 76 Messier Objects 78 Caldwell Objects 81 Orion & Stars by Name 84 Lepus, circa , Brightest Stars 86 1720 , Closest Stars 87 Mythology 88 Bimonthly Sky Charts 92 Meteor Showers 105 Sun, Moon and Planets 106 Observing Considerations 113 Expanded Glossary 115 Th e 88 Constellations, plus 126 Chart Reference BACK PAGE Introduction he night sky was charted by western civilization a few thou - N 1,370 deep sky objects and 360 double stars (two stars—one sands years ago to bring order to the random splatter of stars, often orbits the other) plotted with observing information for T and in the hopes, as a piece of the puzzle, to help “understand” every object. the forces of nature. The stars and their constellations were imbued with N Inclusion of many “famous” celestial objects, even though the beliefs of those times, which have become mythology. they are beyond the reach of a 6 to 8-inch diameter telescope. The oldest known celestial atlas is in the book, Almagest , by N Expanded glossary to define and/or explain terms and Claudius Ptolemy, a Greco-Egyptian with Roman citizenship who lived concepts. in Alexandria from 90 to 160 AD. The Almagest is the earliest surviving astronomical treatise—a 600-page tome. The star charts are in tabular N Black stars on a white background, a preferred format for star form, by constellation, and the locations of the stars are described by charts.
    [Show full text]
  • 00E the Construction of the Universe Symphony
    The basic construction of the Universe Symphony. There are 30 asterisms (Suites) in the Universe Symphony. I divided the asterisms into 15 groups. The asterisms in the same group, lay close to each other. Asterisms!! in Constellation!Stars!Objects nearby 01 The W!!!Cassiopeia!!Segin !!!!!!!Ruchbah !!!!!!!Marj !!!!!!!Schedar !!!!!!!Caph !!!!!!!!!Sailboat Cluster !!!!!!!!!Gamma Cassiopeia Nebula !!!!!!!!!NGC 129 !!!!!!!!!M 103 !!!!!!!!!NGC 637 !!!!!!!!!NGC 654 !!!!!!!!!NGC 659 !!!!!!!!!PacMan Nebula !!!!!!!!!Owl Cluster !!!!!!!!!NGC 663 Asterisms!! in Constellation!Stars!!Objects nearby 02 Northern Fly!!Aries!!!41 Arietis !!!!!!!39 Arietis!!! !!!!!!!35 Arietis !!!!!!!!!!NGC 1056 02 Whale’s Head!!Cetus!! ! Menkar !!!!!!!Lambda Ceti! !!!!!!!Mu Ceti !!!!!!!Xi2 Ceti !!!!!!!Kaffalijidhma !!!!!!!!!!IC 302 !!!!!!!!!!NGC 990 !!!!!!!!!!NGC 1024 !!!!!!!!!!NGC 1026 !!!!!!!!!!NGC 1070 !!!!!!!!!!NGC 1085 !!!!!!!!!!NGC 1107 !!!!!!!!!!NGC 1137 !!!!!!!!!!NGC 1143 !!!!!!!!!!NGC 1144 !!!!!!!!!!NGC 1153 Asterisms!! in Constellation Stars!!Objects nearby 03 Hyades!!!Taurus! Aldebaran !!!!!! Theta 2 Tauri !!!!!! Gamma Tauri !!!!!! Delta 1 Tauri !!!!!! Epsilon Tauri !!!!!!!!!Struve’s Lost Nebula !!!!!!!!!Hind’s Variable Nebula !!!!!!!!!IC 374 03 Kids!!!Auriga! Almaaz !!!!!! Hoedus II !!!!!! Hoedus I !!!!!!!!!The Kite Cluster !!!!!!!!!IC 397 03 Pleiades!! ! Taurus! Pleione (Seven Sisters)!! ! ! Atlas !!!!!! Alcyone !!!!!! Merope !!!!!! Electra !!!!!! Celaeno !!!!!! Taygeta !!!!!! Asterope !!!!!! Maia !!!!!!!!!Maia Nebula !!!!!!!!!Merope Nebula !!!!!!!!!Merope
    [Show full text]
  • The Evening Sky
    I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O o l P l u & x r , o w t O N s e a r e C Z , c y o I C g n o s l R I i o d R e h O t r C e y H d m L p E k E a e t e H ( r r o T F G n O f s D o R NORTH a N i s M n E n A t i X O s w A H t o C M T f e . I s h P e t N L S a E , E f s Z P a e r “ e E SOUTHERN HEMISPHERE m A N r i H s O t . M T R t n T Y N e H E i c ” K E ) n W S . a . T Capella T n E U I W B R N The Evening Sky Map W D LYNX E T T FEBRUARY 2011 WH T A h E C FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY e O S L n K a Y E m R M e A A AURIGA SKY MAP SHOWS HOW A Get Sky Calendar on Twitter S P T l p .
    [Show full text]
  • The Evening Sky
    I N E D R I A C A S T N E O D I T A C L E O R N I G D S T S H A E P H M O O R C I . Z N O e d b l A a r , a l n e O , g N i C R a , Z p s e u I l i C l r a i , R I S C f R a O o s C t p H o L u r E e E & d H P a ( o T F m l O l s u i D R NORTH x ” , N M n E a A o n O X g d A H a x C P M T e r . I o P Polaris H N c S L r y E E e o P Z t n “ n E . EQUATORIAL EDITION i A N H O W T M “ R e T Y N H h E T ” K E ) W S . T T E U W B R N The Evening Sky Map W D E T T . FEBRUARY 2011 WH r A e E C t M82 FREE* EACH MONTH FOR YOU TO EXPLORE, LEARN & ENJOY THE NIGHT SKY O s S L u K l T Y c E CASSIOPEIA h R e r M a A S t A SKY MAP SHOWS HOW i s η M81 Get Sky Calendar on Twitter S P c T s k C A l e e E CAMELOPARDALIS R d J Sky Calendar – February 2011 a O http://twitter.com/skymaps i THE NIGHT SKY LOOKS s B y U O a H N L s D e t A h NE a I t I EARLY FEB 9 PM r T T f S p 1 Moon near Mercury (16° from Sun, morning sky) at 17h UT.
    [Show full text]
  • Culmination of a Constellation
    Culmination of a Constellation Over any night, stars and constellations in the sky will appear to move from east to west due to the Earth’s rotation on its axis. A constellation will culminate (reach its highest point in the sky for your location) when it centres on the meridian - an imaginary line that runs across the sky from north to south and also passes through the zenith (the point high in the sky directly above your head). For example: When to Observe Constellations The taBle shows the approximate time (AEST) constellations will culminate around the middle (15th day) of each month. Constellations will culminate 2 hours earlier for each successive month. Note: add an hour to the given time when daylight saving time is in effect. The time “12” is midnight. Sunrise/sunset times are rounded off to the nearest half an hour. Sun- Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Rise 5am 5:30 6am 6am 7am 7am 7am 6:30 6am 5am 4:30 4:30 Set 7pm 6:30 6pm 5:30 5pm 5pm 5pm 5:30 6pm 6pm 6:30 7pm And 5am 3am 1am 11pm 9pm Aqr 5am 3am 1am 11pm 9pm Aql 4am 2am 12 10pm 8pm Ara 4am 2am 12 10pm 8pm Ari 5am 3am 1am 11pm 9pm Aur 10pm 8pm 4am 2am 12 Boo 3am 1am 11pm 9pm 7pm Cnc 1am 11pm 9pm 7pm 3am CVn 3am 1am 11pm 9pm 7pm CMa 11pm 9pm 7pm 3am 1am Cap 5am 3am 1am 11pm 9pm 7pm Car 2am 12 10pm 8pm 6pm Cen 4am 2am 12 10pm 8pm 6pm Cet 4am 2am 12 10pm 8pm Cha 3am 1am 11pm 9pm 7pm Col 10pm 8pm 4am 2am 12 Com 3am 1am 11pm 9pm 7pm CrA 3am 1am 11pm 9pm 7pm CrB 4am 2am 12 10pm 8pm Crv 3am 1am 11pm 9pm 7pm Cru 3am 1am 11pm 9pm 7pm Cyg 5am 3am 1am 11pm 9pm 7pm Del
    [Show full text]
  • 6<10 JULY 2015
    ()!""#$*+%&* ,$'&()*( *+!,"'-,.#//,0,+12+,.#//,)'%%!)*1'% #,34567849,:4;<7=>?,4>,@8A,54BA,4:,CD77,B477,=>,@8A,BD@A, 7@D?A7,4:,7@ABBD5,AE4B<@=4>,4:,7@D57,4:,DBB,CD77A7 (62*$5&+,1* ;<=>*?@AB*C>=D -.'$/%&$*(0.12''2"#*34%562#4 !"#"$%&'(")*+,"! 6FLHQWLƄF2UJDQLVLQJ&RPPLWWHH 7#82$45*(94%:4/'*7#&6054 -../"0.1'/"234"-.56./7"8.(9'5:; -HDQ3KLOOLSH%HUJHUs+HQUL%RIĺQ <5=>//."[email protected]/.&"24B"4%%=>(>7"<C.D./; U>(./M'/"85W>&&>L>("X"J&>F>:"?>&%.& -'E"?5:%F&.G="2H<I7"J.&:>/G; <5=>//."[email protected]/.&"X"K@L.&M>"?5:%F&.G= K@L.&M>"?5:%F&.G="24B"N'//.=@M>7"4<$; S@.("3>=M/.&"X"P&>/E"3.&=1FL>5: H&'1"->9>D.1"2IO$7"P&>/1.; $9/.="-.L&."X"I&=@(>"D."N>&1@ Q>@(>"N>&'9@"24B"Q>D@6>7"RM>(G; N'V>V@"N>M=55&>"X"R>'/"N10@/>(D S@F/"N@//'.&"24B"N'1F'9>/7"4<$; J.@&9.="N.G/.M"X"8./@'M"N@==.& $/'M>"K'1F>&D="2S8O$7"4B"N>/1F.=M.&7"43; ?>/="I(@A==@/"X"O(>5D'>"Q>(>D'/' T@5M.&"U(.::'/9="2OF>(:.&=7"<C.D./; 6RĺD5DPVWHGWs$QLWD5LFKDUGV S.&.:G"T>(=F"2H<I7"J.&:>/G; ->5&./1."<>L'/"X"Y>MF>/"<:'MF N>&V5="T'MMV@C=V'"2H<I7"J.&:>/G; -.@/>&D@"Z.=M'"X"$(L.&M"['W(=M&> /RFDO2UJDQLVLQJ&RPPLWWHH <M.((>"OF>='@M'=\3('/9/.&"X"S>=@/"J&5/F5M -'E"?5:%F&.G="X"3>M."N>95'&. S.&.:G"T>(=F"X"N>&V5="T'MMV@C=V' !"#$%&$' !"#$!%#!&'&() *""$+,,---'#!&'&(),!./,0##"/1)! ,2345,678962345'*"0: ! ! STELLAR END PRODUCTS – THE LOW MASS – HIGH MASS CONNECTION ! 6-10 July, 2015 in Garching, Germany Programme Overview 13:00 Registration 14:00 Tim De Zeeuw Welcome and Opening 14:10 SOC/LOC Announcements Session 1: Overview (Chair: Liz Humphreys) 14:20 Albert Zijlstra (invited) Grand Overview 15:00 Eric Lagadec Summary of the Recent Physics
    [Show full text]