April First Light Newsletter
Total Page:16
File Type:pdf, Size:1020Kb
 
											Load more
										Recommended publications
									
								- 
												  Mathématiques Et EspaceAtelier 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.
- 
												  Explore the Universe Observing Certificate Second EditionRASC Observing Committee Explore the Universe Observing Certificate Second Edition Explore the Universe Observing Certificate Welcome to the Explore the Universe Observing Certificate Program. This program is designed to provide the observer with a well-rounded introduction to the night sky visible from North America. Using this observing program is an excellent way to gain knowledge and experience in astronomy. Experienced observers find that a planned observing session results in a more satisfying and interesting experience. This program will help introduce you to amateur astronomy and prepare you for other more challenging certificate programs such as the Messier and Finest NGC. The program covers the full range of astronomical objects. Here is a summary: Observing Objective Requirement Available Constellations and Bright Stars 12 24 The Moon 16 32 Solar System 5 10 Deep Sky Objects 12 24 Double Stars 10 20 Total 55 110 In each category a choice of objects is provided so that you can begin the certificate at any time of the year. In order to receive your certificate you need to observe a total of 55 of the 110 objects available. Here is a summary of some of the abbreviations used in this program Instrument V – Visual (unaided eye) B – Binocular T – Telescope V/B - Visual/Binocular B/T - Binocular/Telescope Season Season when the object can be best seen in the evening sky between dusk. and midnight. Objects may also be seen in other seasons. Description Brief description of the target object, its common name and other details. Cons Constellation where object can be found (if applicable) BOG Ref Refers to corresponding references in the RASC’s The Beginner’s Observing Guide highlighting this object.
- 
												  The Heavens in August a Study of Short Period Variables100 SCIENTIFIC,AMERlCAN July 31, 1915 The Heavens in August A Study of Short Period Variables By Prof. Henry Norris Russell, Ph.D. HE warm clear nights of summer offer the amateur which is marked on our map, .and the second lies about and but 18 minutes of arc apart, while Neptune is only T the best chance for star-gazing in all the year, and, two fifths of the way from this to () Ophiuchi (also a degree away on the other side. This simultaneous fortunately, he has one of the finest portions of the shown on the map) and is the only bright star near conjunction of three planets is rather remarkable, but, heavens at his command in the splendid region of the this line. The character of the variation is in both as they rise less than an hour earlier than the Sun, Milky Way, which stretches from Cassiopeia and cases very similar to that of the stars previously de Neptune will be utterly invisible, though the other two Cygnus through Aquila to Sagittarius and Scorpio, and scribed. w Sagittarii varies from magnitude 4.3 to 5.1 planets may easily be seen with a telescope (provided forms a vast circle right across the summit of the vault in a period of 7.595 days, the ris� in brightness taking with suitable finding circles ) even in broad daylight, of heaven. about half as long as the fall, and the maximum being and in the same low-power field. The veriest novice can learn in an hour to identify a little more than twice the minimum light.
- 
												  LIST of PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research InstituteLIST OF PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute of Department of Science and Technology, Govt. of India) Manora Peak, Naini Tal - 263 129, India (1955−2020) ABBREVIATIONS AA: Astronomy and Astrophysics AASS: Astronomy and Astrophysics Supplement Series ACTA: Acta Astronomica AJ: Astronomical Journal ANG: Annals de Geophysique Ap. J.: Astrophysical Journal ASP: Astronomical Society of Pacific ASR: Advances in Space Research ASS: Astrophysics and Space Science AE: Atmospheric Environment ASL: Atmospheric Science Letters BA: Baltic Astronomy BAC: Bulletin Astronomical Institute of Czechoslovakia BASI: Bulletin of the Astronomical Society of India BIVS: Bulletin of the Indian Vacuum Society BNIS: Bulletin of National Institute of Sciences CJAA: Chinese Journal of Astronomy and Astrophysics CS: Current Science EPS: Earth Planets Space GRL : Geophysical Research Letters IAU: International Astronomical Union IBVS: Information Bulletin on Variable Stars IJHS: Indian Journal of History of Science IJPAP: Indian Journal of Pure and Applied Physics IJRSP: Indian Journal of Radio and Space Physics INSA: Indian National Science Academy JAA: Journal of Astrophysics and Astronomy JAMC: Journal of Applied Meterology and Climatology JATP: Journal of Atmospheric and Terrestrial Physics JBAA: Journal of British Astronomical Association JCAP: Journal of Cosmology and Astroparticle Physics JESS : Jr. of Earth System Science JGR : Journal of Geophysical Research JIGR: Journal of Indian
- 
												  Sky & TelescopeEclipse from the See Sirius B: The Nearest Spot the Other EDGE OF SPACE p. 66 WHITE DWARF p. 30 BLUE PLANETS p. 50 THE ESSENTIAL GUIDE TO ASTRONOMY What Put the Bang in the Big Bang p. 22 Telescope Alignment Made Easy p. 64 Explore the Nearby Milky Way p. 32 How to Draw the Moon p. 54 OCTOBER 2013 Cosmic Gold Rush Racing to fi nd exploding stars p. 16 Visit SkyandTelescope.com Download Our Free SkyWeek App FC Oct2013_J.indd 1 8/2/13 2:47 PM “I can’t say when I’ve ever enjoyed owning anything more than my Tele Vue products.” — R.C, TX Tele Vue-76 Why Are Tele Vue Products So Good? Because We Aim to Please! For over 30-years we’ve created eyepieces and telescopes focusing on a singular target; deliver a cus- tomer experience “...even better than you imagined.” Eyepieces with wider, sharper fields of view so you see more at any power, Rich-field refractors with APO performance so you can enjoy Andromeda as well as Jupiter in all their splendor. Tele Vue products complement each other to pro- vide an observing experience as exquisite in performance as it is enjoyable and effortless. And how do we score with our valued customers? Judging by superlatives like: “in- credible, truly amazing, awesome, fantastic, beautiful, work of art, exceeded expectations by a mile, best quality available, WOW, outstanding, uncom- NP101 f/5.4 APO refractor promised, perfect, gorgeous” etc., BULLSEYE! See these superlatives in with 110° Ethos-SX eye- piece shown on their original warranty card context at TeleVue.com/comments.
- 
												  School of Physics Publications 2007School of Physics Publications 2007 Books Karnutsch, C 2007, Low threshold organic thin-film laser devices, Göttingen, 1 Ostrikov, K, Xu, S 2007, Plasma-Aided Nanofabrication: From Plasma Sources to Nanoassembly, Weinheim, Germany Book Chapters Beck, R, Gaensler, B M, Feretti, L 2007, SKA and the Magnetic Universe, Exploring the Cosmic Frontier: Astrophysical Instruments for the 21st Century, Springer-Verlag Berlin Heidelberg, Berlin Heidelberg, 103-108 Bilek, M, Powles, R C, McKenzie, D R 2007, Treatment of polymeric biomaterials by ion implantation, Biomaterials and Surface Modification, Research Signpost, India, 205-248 Britton, S C, New, P B, Roberts, A L, Sharma, M D 2007, Investigating students' ability totransfer mathematics, Transforming a university: the scholarship of teaching and learning in practice, University of Sydney Press, NSW, Australia, 127-140 Dey, C J, Berger, C, Foran, B, Foran, M, Joske, R, Lenzen, M, Wood, R J 2007, Household environmental pressure from consumption: an Australian environmental atlas, Water Wind Art and Debate -How environmental concerns impacton disciplinary research, Sydney University Press, Sydney, 1, 280-314 Eggleton, B J, Slusher, R 2007, Nonlinear pulse propagation in one-dimensional photonic bandgap structures, Nonlinear photonic bandgap materials, Springer Khoukhi, M, Maruyama, S, Bosi, S G, Komiya, A 2007, A Simple Approach for Calculating the Optical Constants of a Clear Glass Window from 0.19 to 5 um, Recent Developments in Solar Energy, Nova Science Publishers, Inc, New York, 289-297
- 
												  134, December 2007British Astronomical Association VARIABLE STAR SECTION CIRCULAR No 134, December 2007 Contents AB Andromedae Primary Minima ......................................... inside front cover From the Director ............................................................................................. 1 Recurrent Objects Programme and Long Term Polar Programme News............4 Eclipsing Binary News ..................................................................................... 5 Chart News ...................................................................................................... 7 CE Lyncis ......................................................................................................... 9 New Chart for CE and SV Lyncis ........................................................ 10 SV Lyncis Light Curves 1971-2007 ............................................................... 11 An Introduction to Measuring Variable Stars using a CCD Camera..............13 Cataclysmic Variables-Some Recent Experiences ........................................... 16 The UK Virtual Observatory ......................................................................... 18 A New Infrared Variable in Scutum ................................................................ 22 The Life and Times of Charles Frederick Butterworth, FRAS........................24 A Hard Day’s Night: Day-to-Day Photometry of Vega and Beta Lyrae.........28 Delta Cephei, 2007 ......................................................................................... 33
- 
												  JRASC August 2021 Lo-ResThe Journal of The Royal Astronomical Society of Canada PROMOTING ASTRONOMY IN CANADA August/août 2021 Volume/volume 115 Le Journal de la Société royale d’astronomie du Canada Number/numéro 4 [809] Inside this issue: A Pas de Deux with Aurora and Steve Detection Threshold of Noctilucent Clouds The Sun, Moon, Waves, and Cityscape The Best of Monochrome Colour Special colour edition. This great series of images was taken by Raymond Kwong from his balcony in Toronto. He used a Canon EOS 500D, with a Sigma 70–300 ƒ/4–5.6 Macro Super lens (shot at 300 mm), a Kenko Teleplus HD 2× DGX teleconverter and a Thousand Oaks solar filter. The series of photos was shot at ISO 100, 0.1s, 600 mm at ƒ/11. August/ août 2021 | Vol. 115, No. 4 | Whole Number 809 contents / table des matières Feature Articles / Articles de fond 182 Binary Universe: Watch the Planets Wheel Overhead 152 A Pas de Deux with Aurora and Steve by Blake Nancarrow by Jay and Judy Anderson 184 Dish on the Cosmos: FYSTing on a 160 Detection Threshold of Noctilucent Clouds New Opportunity and its Effect on Season Sighting Totals by Erik Rosolowsky by Mark Zalcik 186 John Percy’s Universe: Everything Spins 166 Pen and Pixel: June 10 Partial Eclipse (all) by John R. Percy by Nicole Mortillaro / Allendria Brunjes / Shelly Jackson / Randy Attwood Departments / Départements Columns / Rubriques 146 President’s Corner by Robyn Foret 168 Your Monthly Guide to Variable Stars by Jim Fox, AAVSO 147 News Notes / En manchettes Compiled by Jay Anderson 170 Skyward: Faint Fuzzies and Gravity by David Levy 159 Great Images by Michael Gatto 172 Astronomical Art & Artifact: Exploring the History of Colonialism and Astronomy in 188 Astrocryptic and Previous Answers Canada II: The Cases of the Slave-Owning by Curt Nason Astronomer and the Black Astronomer Knighted by Queen Victoria iii Great Images by Randall Rosenfeld by Carl Jorgensen 179 CFHT Chronicles: Times They Are A-Changing by Mary Beth Laychak Bleary-eyed astronomers across most of the country woke up early to catch what they could of the June 10 annular eclipse.
- 
												  David Levy's Guide to the Night Sky DaCambridge University Press 0521797535 - David Levy’s Guide to the Night Sky David H. Levy Index More information INDEX AAVSO, 200–201, 331, 332 binoculars, 57–59 absolute magnitudes, 36 Bobrovnikoff method, estimating comet Adams, John Couch, 156 brightness, 178 aetheria darkening, 138 Bode, Johann, 163 Alcock, George, 44, 185 Bode’s Law, 163–165 Algol, 325 Brahe, Tycho, 81 aligning, 67 Brasch, Klaus, 126 Alpha Capricornids, 47 Brashear, John, 60 altazimuth, 62, 65 bright nebulae, 232–233 altitude, 67 Brooks, William, 182 Amalthea, 111 Burnham, Sherbourne Wesley, 193 amateur astronomy, introduced, xvii, xviii Andromedids, 48, 49, 68 Callisto, 111, 119, 121 Antoniadi, Eugenios, 112 Carrington, Christopher, 103 aphelic oppositions, 134 Cassini spacecraft, 130 aphelion, 134 Cassini, Giovanni, 81, 124 apochromat, 60 Cassini’s Division, 124, 125 apparent magnitude, 36 CCD technology, 275–280 apparitions, of comets, 134, 135 CCDs, for astrometry, 283 Arago, Francois, 156 Celestial Police, 163–164 Ariel, 159 celestial equator, 8 ashen light, Venus, 152 Central Bureau for Astronomical Association of Lunar and Planetary Telegrams,120, 121, 186–187, 280 Observers, 331, 332 Challis, James, 156 Asteroids, 163–172 Chapman, Clark, 170 naming of, 165–166 Chaucer, Geoffrey, 318 Astronomical League, 333 chromosphere, 293 astrophotography, 262 Clark, Alvin, 60 Aurigids, 46 Clavius, Christopher, 82 Aurora, 28–33 Collins, Peter, 158, 217 Auroral Data Center in the US, 29 Coma Berenicids, 50 averted vision, 41 comets, 172–189, 294 azimuth, 67 Arend–Roland, 43 Biela, 49, 68 Baker, Lonny, xxii Bradfield, 69 Barnard, E. E. 111, 181–182 Denning–Fujikawa, 181 Beyer method, estimating comet brightness, Encke, 49, 175 179 Giacobini–Zinner, 48 Beyond the Observatory (Shapley), 35 Halley, 44, 46, 48, 55, 78, 175, 225 big bang, 65 Hartley–IRAS, 175 339 © Cambridge University Press www.cambridge.org Cambridge University Press 0521797535 - David Levy’s Guide to the Night Sky David H.
- 
												  Getting Started with Variable Star ObservingGetting Started with Variable Star Observing The primary types of variable stars you will be observing are: Cepheids - Named after Delta Cephei, these luminous stars brighten and fade with clockwork regularity. There are several types of Cepheids ranging from Beta Cepheids with 0.1 magnitude fluctuations and short periods from 3 to 7 hours to W Virginis Stars with fluctuation of about one magnitude over a period of up to 20 days. In 1910, Henrietta Leavitt learned that the longer a Cepheids period was, the brighter the absolute magnitude was. This led to Harlow Shapely developing the method of using Cepheids to determine the distance to globular clusters and nearby galaxies. Mira Stars - These long period variables are very large red pulsating stars having brightness magnitude ranges of up to 11 magnitudes and a time period from 24 days to 5.7 years. These stars can be regular, semiregular, or irregular. Some examples are Mira 2.0-9.3 332 days, R Leo 5.9 -10.1 313 days, Chi Cygni 3.3-14.2 408 days, Betelgeuse .4- 1.3 5.7 years. Estimates should be done at least twice per month. Eruptive Stars - This group contains Novae and Nova like stars with a great range of types. Recurrent Nova such as T Coronae Borealis may have outbursts that are decades apart. Stars like U Geminorum and SS Cygni repeat their outbursts every few months. One type, R Coronae Borealis, instead of erupting drops by as much as eight magnitudes. UV Ceti stars may flare several magnitudes in a matter of minutes.
- 
												![Arxiv:2003.03982V3 [Astro-Ph.HE] 7 May 2020](https://docslib.b-cdn.net/cover/0452/arxiv-2003-03982v3-astro-ph-he-7-may-2020-2900452.webp)  Arxiv:2003.03982V3 [Astro-Ph.HE] 7 May 2020Prospects for Pre-supernova Neutrino Observation in Future Large Liquid-scintillator Detectors Hui-Ling Li,1, ∗ Yu-Feng Li,1, 2, y Liang-Jian Wen,1, z and Shun Zhou1, 2, x 1Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 2School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, China Abstract Before massive stars heavier than (8 ··· 10) solar masses evolve to the phase of a gravitational core collapse, they will emit a huge number of MeV-energy neutrinos that are mainly produced in the thermal processes and nuclear weak interactions. The detection of such pre-supernova (pre-SN) neutrinos could provide an important and independent early warning for the optical observations of core-collapse SNe. In this paper, we investigate the prospects of future large liquid-scintillator + − − detectors for the observation of pre-SN neutrinos in both νe +p ! e +n and ν(ν)+e ! ν(ν)+e reaction channels, where ν (ν) denotes neutrinos (antineutrinos) of all three flavors. We propose a quantitative assessment of the capability in terms of three working criteria, namely, how far the SN distance can be covered, how long the early warning before the core collapse can be sent out, and how well the direction pointing to the SN can be determined. The dependence of the final results on the different models of progenitor stars, neutrino flavor conversions and the relevant backgrounds is also discussed. arXiv:2003.03982v3 [astro-ph.HE] 7 May 2020 ∗Electronic address: [email protected] yElectronic address: [email protected] (corresponding author) zElectronic address: [email protected] (corresponding author) xElectronic address: [email protected] 1 I.
- 
												  Review of Small-Angle Coronagraphic Techniques in the Wake of Ground-Based Second-Generation Adaptive Optics SystemsInvited Paper Review of small-angle coronagraphic techniques in the wake of ground-based second-generation adaptive optics systems Dimitri Maweta,b, Laurent Pueyoc, Peter Lawsonb, Laurent Mugnierd, Wesley Traubb, Anthony Boccalettie, John Traugerb, Szymon Gladyszf, Eugene Serabynb, Julien Millia,g, Ruslan Belikovh, Markus Kasperi, Pierre Baudoze, Bruce Macintoshj, Christian Maroisk, Ben Oppenheimerl, Harrisson Barrettm, Jean-Luc Beuzitg, Nicolas Devaneyn, Julien Girarda, Olivier Guyono, John Kristb, Bertrand Mennessonb, David Mouilletg, Naoshi Murakamip, Lisa Poyneerj, Dmitri Savranskyj, Christophe V´erinaudg, and James K. Wallaceb aEuropean Southern Observatory, Alonso de C´ordova 3107, Vitacura, Casilla 19001, Chile; bJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA; cJHU Department of Physics and Astronomy, 3400 N. Charles St, Baltimore, MD 21218, USA; dONERA, Division Optique Theorique et Appliqu´ee, BP 72, 92322 Chatillon Cedex, France; eLESIA, Observatoire de Paris, CNRS, 5 place Jules Janssen, 92195 Meudon, France; fFraunhofer Institute, Gutleuthausstrasse 1, 76275 Ettlingen, Germany; gIPAG, 414 rue de la Piscine, Domaine Univ., BP 53, 38041 Grenoble Cedex 09, France; hNASA Ames Research Center, Moffett Field, CA 94035, USA; iEuropean Southern Observatory, Karl-Schwarzschild-Straße 2, 85748 Garching, Germany; jLawrence Livermore National Laboratory, 7000 East Ave, Livermore, CA 94550, USA; kNRC, Herzberg Institute of Astrophysics, Victoria, BC V9E 2E7, Canada; lAmerican Museum of Natural History,