DOCSLIB.ORG

Small Astronomy Calendar for Amateur Astronomers 2019

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Small Astronomy Calendar for Amateur Astronomers 2019 IGAEF Small Astronomy Calendar for Amateur Astronomers 2019 C A L E N D A R F O R 2019 January February March Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa 1 2 3 4 5 1 2 1 2 6 7 8 9 10 11 12 3 4 5 6 7 8 9 3 4 5 6 7 8 9 13 14 15 16 17 18 19 10 11 12 13 14 15 16 10 11 12 13 14 15 16 20 21 22 23 24 25 26 17 18 19 20 21 22 23 17 18 19 20 21 22 23 27 28 29 30 31 24 25 26 27 28 24 25 26 27 28 29 30 31 April May June Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa 1 2 3 4 5 6 1 2 3 4 1 7 8 9 10 11 12 13 5 6 7 8 9 10 11 2 3 4 5 6 7 8 14 15 16 17 18 19 20 12 13 14 15 16 17 18 9 10 11 12 13 14 15 21 22 23 24 25 26 27 19 20 21 22 23 24 25 16 17 18 19 20 21 22 28 29 30 26 27 28 29 30 31 23 24 25 26 27 28 29 30 July August September Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa 1 2 3 4 5 6 1 2 3 1 2 3 4 5 6 7 7 8 9 10 11 12 13 4 5 6 7 8 9 10 8 9 10 11 12 13 14 14 15 16 17 18 19 20 11 12 13 14 15 16 17 15 16 17 18 19 20 21 21 22 23 24 25 26 27 18 19 20 21 22 23 24 22 23 24 25 26 27 28 28 29 30 31 25 26 27 28 29 30 31 29 30 October November December Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa Su Mo Tu We Th Fr Sa 1 2 3 4 5 1 2 1 2 3 4 5 6 7 6 7 8 9 10 11 12 3 4 5 6 7 8 9 8 9 10 11 12 13 14 13 14 15 16 17 18 19 10 11 12 13 14 15 16 15 16 17 18 19 20 21 20 21 22 23 24 25 26 17 18 19 20 21 22 23 22 23 24 25 26 27 28 27 28 29 30 31 24 25 26 27 28 29 30 29 30 31 Easter Sunday: 2019 Apr 21 Phases of the Moon 2019 New Moon First Quarter Full Moon Last Quarter d h d h d h ⊕dist d h Jan 6 1.5 Jan 14 6.7 Jan 21 5.3 (56.09) Jan 27 21.2 Feb 4 21.1 Feb 12 22.5 Feb 19 15.9 (55.95) Feb 26 11.6 Mar 6 16.1 Mar 14 10.4 Mar 21 1.7 (56.57) Mar 28 4.2 Apr 5 8.8 Apr 12 19.1 Apr 19 11.3 (57.80) Apr 26 22.3 May 4 22.8 May 12 1.2 May 18 21.2 (59.40) May 26 16.6 Jun 3 10.0 Jun 10 6.0 Jun 17 8.6 (61.08) Jun 25 9.7 Jul 2 19.2 Jul 9 11.0 Jul 16 21.7 (62.54) Jul 25 1.3 Aug 1 3.2 Aug 7 17.6 Aug 15 12.6 (63.49) Aug 23 14.9 Aug 30 10.6 Sep 6 3.3 Sep 14 4.6 (63.69) Sep 22 2.7 Sep 28 18.5 Oct 5 16.9 Oct 13 21.2 (63.08) Oct 21 12.6 Oct 28 3.7 Nov 4 10.4 Nov 12 13.5 (61.76) Nov 19 21.2 Nov 26 15.2 Dec 4 7.0 Dec 12 5.2 (60.03) Dec 19 5.0 Dec 26 5.3 Moon at Perigee 2019 d h d h d h d h Jan 21 20 Feb 19 8 Mar 19 19 Apr 16 21 May 13 21 Jun 7 24 Jul 5 5 Aug 2 7 Aug 30 16 Sep 28 3 Oct 26 11 Nov 23 7 Dec 18 21 Moon at Apogee 2019 d h d h d h d h Jan 9 4 Feb 5 9 Mar 4 11 Apr 1 1 Apr 28 19 May 26 14 Jun 23 8 Jul 20 23 Aug 17 11 Sep 13 14 Oct 10 18 Nov 7 8 Dec 5 4 All data generated with Occult v4 Local Time of MOONRISE 2019 Date Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec 1 3.07 4.40 3.26 4.16 4.00 4.17 4.24 6.13 8.20 9.12 10.58 11.16 2 4.02 5.29 4.13 4.52 4.33 4.59 5.20 7.21 9.24 10.15 11.51 11.57 3 4.58 6.15 4.57 5.26 5.07 5.45 6.21 8.28 10.26 11.16 12.38 12.34 4 5.52 6.58 5.38 6.00 5.43 6.37 7.26 9.33 11.28 12.14 13.21 13.08 5 6.43 7.38 6.16 6.33 6.22 7.34 8.32 10.36 12.28 13.08 14.00 13.40 6 7.32 8.15 6.51 7.08 7.05 8.35 9.38 11.37 13.26 13.57 14.35 14.12 7 8.18 8.50 7.25 7.44 7.52 9.39 10.42 12.37 14.21 14.42 15.08 14.44 8 9.00 9.24 7.59 8.24 8.45 10.44 11.44 13.36 15.12 15.23 15.40 15.17 9 9.38 9.57 8.32 9.07 9.42 11.47 12.44 14.34 15.59 16.00 16.12 15.54 10 10.15 10.31 9.07 9.56 10.43 12.49 13.44 15.30 16.43 16.34 16.45 16.34 11 10.49 11.06 9.44 10.49 11.46 13.49 14.42 16.24 17.22 17.07 17.20 17.19 12 11.22 11.45 10.24 11.48 12.50 14.49 15.41 17.14 17.59 17.39 17.57 18.09 13 11.56 12.27 11.09 12.50 13.53 15.49 16.39 18.00 18.33 18.11 18.39 19.05 14 12.31 13.15 12.00 13.54 14.55 16.49 17.35 18.43 19.05 18.45 19.25 20.06 15 13.09 14.10 12.56 14.59 15.56 17.48 18.28 19.22 19.37 19.20 20.17 21.09 16 13.50 15.10 13.57 16.03 16.58 18.46 19.17 19.57 20.10 19.58 21.13 22.12 17 14.37 16.16 15.02 17.07 17.59 19.42 20.03 20.31 20.43 20.41 22.13 23.15 18 15.30 17.24 16.09 18.10 19.00 20.34 20.44 21.03 21.19 21.28 23.16 ..... 19 16.29 18.33 17.16 19.13 19.59 21.23 21.22 21.35 21.59 22.21 ..... 0.20 20 17.34 19.40 18.22 20.15 20.57 22.07 21.57 22.08 22.43 23.18 0.21 1.21 21 18.42 20.45 19.27 21.15 21.52 22.46 22.30 22.43 23.34 ..... 1.24 2.22 22 19.51 21.48 20.30 22.14 22.43 23.23 23.02 23.20 ..... 0.22 2.27 3.23 23 20.57 22.48 21.32 23.10 23.29 23.57 23.35 ..... 0.30 1.26 3.29 4.25 24 22.01 23.47 22.32 ..... ..... ..... ..... 0.03 1.31 2.31 4.32 5.27 25 23.02 ..... 23.30 0.02 0.11 0.30 0.08 0.51 2.36 3.36 5.36 6.28 26 ..... 0.45 ..... 0.50 0.49 1.04 0.46 1.45 3.43 4.41 6.40 7.26 27 0.02 1.43 0.27 1.35 1.25 1.37 1.26 2.45 4.50 5.46 7.42 8.20 28 1.02 2.36 1.21 2.15 1.59 2.13 2.12 3.50 5.57 6.51 8.43 9.08 29 1.58 ..... 2.10 2.51 2.32 2.51 3.04 4.58 7.03 7.55 9.39 9.52 30 2.53 ..... 2.56 3.26 3.05 3.35 4.02 6.06 8.08 8.59 10.30 10.31 31 3.48 ..... 3.37 ..... 3.40 ..... 5.06 7.14 ..... 10.00 ..... ..... ..... No phenomena occurs on this date ----- Moon continuously below the horizon ***** Moon continuously above the horizon All data generated with Occult v4 Local Time of MOONSET 2019 Date Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec 1 14.35 15.32 14.18 15.39 16.06 17.33 18.20 19.55 20.42 20.39 21.45 22.17 2 15.17 16.22 15.09 16.30 16.58 18.33 19.22 20.43 21.23 21.25 22.39 23.10 3 16.00 17.13 16.01 17.21 17.52 19.34 20.21 21.27 22.04 22.13 23.34 ....
Load more

Recommended publications
  • Ioptron AZ Mount Pro Altazimuth Mount Instruction
    ® iOptron® AZ Mount ProTM Altazimuth Mount Instruction Manual Product #8900, #8903 and #8920 This product is a precision instrument. Please read the included QSG before assembling the mount. Please read the entire Instruction Manual before operating the mount. If you have any questions please contact us at [email protected] WARNING! NEVER USE A TELESCOPE TO LOOK AT THE SUN WITHOUT A PROPER FILTER! Looking at or near the Sun will cause instant and irreversible damage to your eye. Children should always have adult supervision while observing. 2 Table of Content Table of Content ......................................................................................................................................... 3 1. AZ Mount ProTM Altazimuth Mount Overview...................................................................................... 5 2. AZ Mount ProTM Mount Assembly ........................................................................................................ 6 2.1. Parts List .......................................................................................................................................... 6 2.2. Identification of Parts ....................................................................................................................... 7 2.3. Go2Nova® 8407 Hand Controller .................................................................................................... 8 2.3.1. Key Description .......................................................................................................................
    [Show full text]
  • Occurrence and Core-Envelope Structure of 1–4× Earth-Size Planets Around Sun-Like Stars
    Occurrence and core-envelope structure of 1–4× SPECIAL FEATURE Earth-size planets around Sun-like stars Geoffrey W. Marcya,1, Lauren M. Weissa, Erik A. Petiguraa, Howard Isaacsona, Andrew W. Howardb, and Lars A. Buchhavec aDepartment of Astronomy, University of California, Berkeley, CA 94720; bInstitute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822; and cHarvard-Smithsonian Center for Astrophysics, Harvard University, Cambridge, MA 02138 Edited by Adam S. Burrows, Princeton University, Princeton, NJ, and accepted by the Editorial Board April 16, 2014 (received for review January 24, 2014) Small planets, 1–4× the size of Earth, are extremely common planets. The Doppler reflex velocity of an Earth-size planet − around Sun-like stars, and surprisingly so, as they are missing in orbiting at 0.3 AU is only 0.2 m s 1, difficult to detect with an − our solar system. Recent detections have yielded enough informa- observational precision of 1 m s 1. However, such Earth-size tion about this class of exoplanets to begin characterizing their planets show up as a ∼10-sigma dimming of the host star after occurrence rates, orbits, masses, densities, and internal structures. coadding the brightness measurements from each transit. The Kepler mission finds the smallest planets to be most common, The occurrence rate of Earth-size planets is a major goal of as 26% of Sun-like stars have small, 1–2 R⊕ planets with orbital exoplanet science. With three years of Kepler photometry in periods under 100 d, and 11% have 1–2 R⊕ planets that receive 1–4× hand, two groups worked to account for the detection biases in the incident stellar flux that warms our Earth.
    [Show full text]
  • METEOR CSILLAGÁSZATI ÉVKÖNYV 2019 Meteor Csillagászati Évkönyv 2019
    METEOR CSILLAGÁSZATI ÉVKÖNYV 2019 meteor csillagászati évkönyv 2019 Szerkesztette: Benkő József Mizser Attila Magyar Csillagászati Egyesület www.mcse.hu Budapest, 2018 Az évkönyv kalendárium részének összeállításában közreműködött: Tartalom Bagó Balázs Görgei Zoltán Kaposvári Zoltán Kiss Áron Keve Kovács József Bevezető ....................................................................................................... 7 Molnár Péter Sánta Gábor Kalendárium .............................................................................................. 13 Sárneczky Krisztián Szabadi Péter Cikkek Szabó Sándor Szőllősi Attila Zsoldos Endre: 100 éves a Nemzetközi Csillagászati Unió ........................191 Zsoldos Endre Maria Lugaro – Kereszturi Ákos: Elemkeletkezés a csillagokban.............. 203 Szabó Róbert: Az OGLE égboltfelmérés 25 éve ........................................218 A kalendárium csillagtérképei az Ursa Minor szoftverrel készültek. www.ursaminor.hu Beszámolók Mizser Attila: A Magyar Csillagászati Egyesület Szakmailag ellenőrizte: 2017. évi tevékenysége .........................................................................242 Szabados László Kiss László – Szabó Róbert: Az MTA CSFK Csillagászati Intézetének 2017. évi tevékenysége .........................................................................248 Petrovay Kristóf: Az ELTE Csillagászati Tanszékének működése 2017-ben ............................................................................ 262 Szabó M. Gyula: Az ELTE Gothard Asztrofi zikai Obszervatórium
    [Show full text]
  • The Maunder Minimum and the Variable Sun-Earth Connection
    The Maunder Minimum and the Variable Sun-Earth Connection (Front illustration: the Sun without spots, July 27, 1954) By Willie Wei-Hock Soon and Steven H. Yaskell To Soon Gim-Chuan, Chua Chiew-See, Pham Than (Lien+Van’s mother) and Ulla and Anna In Memory of Miriam Fuchs (baba Gil’s mother)---W.H.S. In Memory of Andrew Hoff---S.H.Y. To interrupt His Yellow Plan The Sun does not allow Caprices of the Atmosphere – And even when the Snow Heaves Balls of Specks, like Vicious Boy Directly in His Eye – Does not so much as turn His Head Busy with Majesty – ‘Tis His to stimulate the Earth And magnetize the Sea - And bind Astronomy, in place, Yet Any passing by Would deem Ourselves – the busier As the Minutest Bee That rides – emits a Thunder – A Bomb – to justify Emily Dickinson (poem 224. c. 1862) Since people are by nature poorly equipped to register any but short-term changes, it is not surprising that we fail to notice slower changes in either climate or the sun. John A. Eddy, The New Solar Physics (1977-78) Foreword By E. N. Parker In this time of global warming we are impelled by both the anticipated dire consequences and by scientific curiosity to investigate the factors that drive the climate. Climate has fluctuated strongly and abruptly in the past, with ice ages and interglacial warming as the long term extremes. Historical research in the last decades has shown short term climatic transients to be a frequent occurrence, often imposing disastrous hardship on the afflicted human populations.
    [Show full text]
  • 10. Scientific Programme 10.1
    10. SCIENTIFIC PROGRAMME 10.1. OVERVIEW (a) Invited Discourses Plenary Hall B 18:00-19:30 ID1 “The Zoo of Galaxies” Karen Masters, University of Portsmouth, UK Monday, 20 August ID2 “Supernovae, the Accelerating Cosmos, and Dark Energy” Brian Schmidt, ANU, Australia Wednesday, 22 August ID3 “The Herschel View of Star Formation” Philippe André, CEA Saclay, France Wednesday, 29 August ID4 “Past, Present and Future of Chinese Astronomy” Cheng Fang, Nanjing University, China Nanjing Thursday, 30 August (b) Plenary Symposium Review Talks Plenary Hall B (B) 8:30-10:00 Or Rooms 309A+B (3) IAUS 288 Astrophysics from Antarctica John Storey (3) Mon. 20 IAUS 289 The Cosmic Distance Scale: Past, Present and Future Wendy Freedman (3) Mon. 27 IAUS 290 Probing General Relativity using Accreting Black Holes Andy Fabian (B) Wed. 22 IAUS 291 Pulsars are Cool – seriously Scott Ransom (3) Thu. 23 Magnetars: neutron stars with magnetic storms Nanda Rea (3) Thu. 23 Probing Gravitation with Pulsars Michael Kremer (3) Thu. 23 IAUS 292 From Gas to Stars over Cosmic Time Mordacai-Mark Mac Low (B) Tue. 21 IAUS 293 The Kepler Mission: NASA’s ExoEarth Census Natalie Batalha (3) Tue. 28 IAUS 294 The Origin and Evolution of Cosmic Magnetism Bryan Gaensler (B) Wed. 29 IAUS 295 Black Holes in Galaxies John Kormendy (B) Thu. 30 (c) Symposia - Week 1 IAUS 288 Astrophysics from Antartica IAUS 290 Accretion on all scales IAUS 291 Neutron Stars and Pulsars IAUS 292 Molecular gas, Dust, and Star Formation in Galaxies (d) Symposia –Week 2 IAUS 289 Advancing the Physics of Cosmic
    [Show full text]
  • Variable Star Classification and Light Curves Manual
    Variable Star Classification and Light Curves An AAVSO course for the Carolyn Hurless Online Institute for Continuing Education in Astronomy (CHOICE) This is copyrighted material meant only for official enrollees in this online course. Do not share this document with others. Please do not quote from it without prior permission from the AAVSO. Table of Contents Course Description and Requirements for Completion Chapter One- 1. Introduction . What are variable stars? . The first known variable stars 2. Variable Star Names . Constellation names . Greek letters (Bayer letters) . GCVS naming scheme . Other naming conventions . Naming variable star types 3. The Main Types of variability Extrinsic . Eclipsing . Rotating . Microlensing Intrinsic . Pulsating . Eruptive . Cataclysmic . X-Ray 4. The Variability Tree Chapter Two- 1. Rotating Variables . The Sun . BY Dra stars . RS CVn stars . Rotating ellipsoidal variables 2. Eclipsing Variables . EA . EB . EW . EP . Roche Lobes 1 Chapter Three- 1. Pulsating Variables . Classical Cepheids . Type II Cepheids . RV Tau stars . Delta Sct stars . RR Lyr stars . Miras . Semi-regular stars 2. Eruptive Variables . Young Stellar Objects . T Tau stars . FUOrs . EXOrs . UXOrs . UV Cet stars . Gamma Cas stars . S Dor stars . R CrB stars Chapter Four- 1. Cataclysmic Variables . Dwarf Novae . Novae . Recurrent Novae . Magnetic CVs . Symbiotic Variables . Supernovae 2. Other Variables . Gamma-Ray Bursters . Active Galactic Nuclei 2 Course Description and Requirements for Completion This course is an overview of the types of variable stars most commonly observed by AAVSO observers. We discuss the physical processes behind what makes each type variable and how this is demonstrated in their light curves. Variable star names and nomenclature are placed in a historical context to aid in understanding today’s classification scheme.
    [Show full text]
  • Gaia Data Release 2 Special Issue
    A&A 623, A110 (2019) Astronomy https://doi.org/10.1051/0004-6361/201833304 & © ESO 2019 Astrophysics Gaia Data Release 2 Special issue Gaia Data Release 2 Variable stars in the colour-absolute magnitude diagram?,?? Gaia Collaboration, L. Eyer1, L. Rimoldini2, M. Audard1, R. I. Anderson3,1, K. Nienartowicz2, F. Glass1, O. Marchal4, M. Grenon1, N. Mowlavi1, B. Holl1, G. Clementini5, C. Aerts6,7, T. Mazeh8, D. W. Evans9, L. Szabados10, A. G. A. Brown11, A. Vallenari12, T. Prusti13, J. H. J. de Bruijne13, C. Babusiaux4,14, C. A. L. Bailer-Jones15, M. Biermann16, F. Jansen17, C. Jordi18, S. A. Klioner19, U. Lammers20, L. Lindegren21, X. Luri18, F. Mignard22, C. Panem23, D. Pourbaix24,25, S. Randich26, P. Sartoretti4, H. I. Siddiqui27, C. Soubiran28, F. van Leeuwen9, N. A. Walton9, F. Arenou4, U. Bastian16, M. Cropper29, R. Drimmel30, D. Katz4, M. G. Lattanzi30, J. Bakker20, C. Cacciari5, J. Castañeda18, L. Chaoul23, N. Cheek31, F. De Angeli9, C. Fabricius18, R. Guerra20, E. Masana18, R. Messineo32, P. Panuzzo4, J. Portell18, M. Riello9, G. M. Seabroke29, P. Tanga22, F. Thévenin22, G. Gracia-Abril33,16, G. Comoretto27, M. Garcia-Reinaldos20, D. Teyssier27, M. Altmann16,34, R. Andrae15, I. Bellas-Velidis35, K. Benson29, J. Berthier36, R. Blomme37, P. Burgess9, G. Busso9, B. Carry22,36, A. Cellino30, M. Clotet18, O. Creevey22, M. Davidson38, J. De Ridder6, L. Delchambre39, A. Dell’Oro26, C. Ducourant28, J. Fernández-Hernández40, M. Fouesneau15, Y. Frémat37, L. Galluccio22, M. García-Torres41, J. González-Núñez31,42, J. J. González-Vidal18, E. Gosset39,25, L. P. Guy2,43, J.-L. Halbwachs44, N. C. Hambly38, D.
    [Show full text]
  • Sodium and Potassium Signatures Of
    Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets Apurva Oza, Robert Johnson, Emmanuel Lellouch, Carl Schmidt, Nick Schneider, Chenliang Huang, Diana Gamborino, Andrea Gebek, Aurelien Wyttenbach, Brice-Olivier Demory, et al. To cite this version: Apurva Oza, Robert Johnson, Emmanuel Lellouch, Carl Schmidt, Nick Schneider, et al.. Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets. The Astro- physical Journal, American Astronomical Society, 2019, 885 (2), pp.168. 10.3847/1538-4357/ab40cc. hal-02417964 HAL Id: hal-02417964 https://hal.sorbonne-universite.fr/hal-02417964 Submitted on 18 Dec 2019 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. The Astrophysical Journal, 885:168 (19pp), 2019 November 10 https://doi.org/10.3847/1538-4357/ab40cc © 2019. The American Astronomical Society. Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets Apurva V. Oza1 , Robert E. Johnson2,3 , Emmanuel Lellouch4 , Carl Schmidt5 , Nick Schneider6 , Chenliang Huang7 , Diana Gamborino1 , Andrea Gebek1,8 , Aurelien Wyttenbach9 , Brice-Olivier Demory10 , Christoph Mordasini1 , Prabal Saxena11, David Dubois12 , Arielle Moullet12, and Nicolas Thomas1 1 Physikalisches Institut, Universität Bern, Bern, Switzerland; [email protected] 2 Engineering Physics, University of Virginia, Charlottesville, VA 22903, USA 3 Physics, New York University, 4 Washington Place, New York, NY 10003, USA 4 LESIA–Observatoire de Paris, CNRS, UPMC Univ.
    [Show full text]
  • To Trappist-1 RAIR Golaith Ship
    Mission Profile Navigator 10:07 AM - 12/2/2018 page 1 of 10 Interstellar Mission Profile for SGC Navigator - Report - Printable ver 4.3 Start: omicron 2 40 Eri (Star Trek Vulcan home star) (HD Dest: Trappist-1 2Mass J23062928-0502285 in Aquarii [X -9.150] [Y - 26965) (Keid) (HIP 19849) in Eridani [X 14.437] [Y - 38.296] [Z -3.452] 7.102] [Z -2.167] Rendezvous Earth date arrival: Tuesday, December 8, 2420 Ship Type: RAIR Golaith Ship date arrival: Tuesday, January 8, 2419 Type 2: Rendezvous with a coasting leg ( Top speed is reached before mid-point ) Start Position: Start Date: 2-December-2018 Star System omicron 2 40 Eri (Star Trek Vulcan home star) (HD 26965) (Keid) Earth Polar Primary Star: (HIP 19849) RA hours: inactive Type: K0 V Planets: 1e RA min: inactive Binary: B, C, b RA sec: inactive Type: M4.5V, DA2.9 dec. degrees inactive Rank from Earth: 69 Abs Mag.: 5.915956445 dec. minutes inactive dec. seconds inactive Galactic SGC Stats Distance l/y Sector X Y Z Earth to Start Position: 16.2346953 Kappa 14.43696547 -7.10221947 -2.16744969 Destination Arrival Date (Earth time): 8-December-2420 Star System Earth Polar Trappist-1 2Mass J23062928-0502285 Primary Star: RA hours: inactive Type: M8V Planets 4, 3e RA min: inactive Binary: B C RA sec: inactive Type: 0 dec. degrees inactive Rank from Earth 679 Abs Mag.: 18.4 dec. minutes inactive Course Headings SGC decimal dec. seconds inactive RA: (0 <360) 232.905748 dec: (0-180) 91.8817176 Galactic SGC Sector X Y Z Destination: Apparent position | Start of Mission Omega -9.09279603 -38.2336637 -3.46695345 Destination: Real position | Start of Mission Omega -9.09548281 -38.2366036 -3.46626331 Destination: Real position | End of Mission Omega -9.14988933 -38.2961361 -3.45228825 Shifts in distances of Destination Distance l/y X Y Z Change in Apparent vs.
    [Show full text]
  • 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,
    [Show full text]
  • Downloads/ Astero2007.Pdf) and by Aerts Et Al (2010)
    This work is protected by copyright and other intellectual property rights and duplication or sale of all or part is not permitted, except that material may be duplicated by you for research, private study, criticism/review or educational purposes. Electronic or print copies are for your own personal, non- commercial use and shall not be passed to any other individual. No quotation may be published without proper acknowledgement. For any other use, or to quote extensively from the work, permission must be obtained from the copyright holder/s. i Fundamental Properties of Solar-Type Eclipsing Binary Stars, and Kinematic Biases of Exoplanet Host Stars Richard J. Hutcheon Submitted in accordance with the requirements for the degree of Doctor of Philosophy. Research Institute: School of Environmental and Physical Sciences and Applied Mathematics. University of Keele June 2015 ii iii Abstract This thesis is in three parts: 1) a kinematical study of exoplanet host stars, 2) a study of the detached eclipsing binary V1094 Tau and 3) and observations of other eclipsing binaries. Part I investigates kinematical biases between two methods of detecting exoplanets; the ground based transit and radial velocity methods. Distances of the host stars from each method lie in almost non-overlapping groups. Samples of host stars from each group are selected. They are compared by means of matching comparison samples of stars not known to have exoplanets. The detection methods are found to introduce a negligible bias into the metallicities of the host stars but the ground based transit method introduces a median age bias of about -2 Gyr.
    [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]