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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. -
ESO Annual Report 2004 ESO Annual Report 2004 Presented to the Council by the Director General Dr
ESO Annual Report 2004 ESO Annual Report 2004 presented to the Council by the Director General Dr. Catherine Cesarsky View of La Silla from the 3.6-m telescope. ESO is the foremost intergovernmental European Science and Technology organi- sation in the field of ground-based as- trophysics. It is supported by eleven coun- tries: Belgium, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Sweden, Switzerland and the United Kingdom. Created in 1962, ESO provides state-of- the-art research facilities to European astronomers and astrophysicists. In pur- suit of this task, ESO’s activities cover a wide spectrum including the design and construction of world-class ground-based observational facilities for the member- state scientists, large telescope projects, design of innovative scientific instruments, developing new and advanced techno- logies, furthering European co-operation and carrying out European educational programmes. ESO operates at three sites in the Ataca- ma desert region of Chile. The first site The VLT is a most unusual telescope, is at La Silla, a mountain 600 km north of based on the latest technology. It is not Santiago de Chile, at 2 400 m altitude. just one, but an array of 4 telescopes, It is equipped with several optical tele- each with a main mirror of 8.2-m diame- scopes with mirror diameters of up to ter. With one such telescope, images 3.6-metres. The 3.5-m New Technology of celestial objects as faint as magnitude Telescope (NTT) was the first in the 30 have been obtained in a one-hour ex- world to have a computer-controlled main posure. -
Planetary Science Institute
PLANETARY SCIENCE INSTITUTE N7'6-3qo84 (NAS A'-CR:1'V7! 3 ) ASTEROIDAL AND PLANETARY ANALYSIS Final Report (Planetary Science Ariz.) 163 p HC $6.75 Inst., Tucson, CSCL 03A Unclas G3/89 15176 i-'' NSA tiFACIWj INP BRANC NASW 2718 ASTEROIDAL AND PLANETARY ANALYSIS Final Report 11 August 1975 Submitted by: Planetary Science Institute 252 W. Ina Road, Suite D Tucson, Arizona 85704 William K. Hartmann Manager TASK 1: ASTEROID SPECTROPHOTOMETRY AND INTERPRETATION (Principal Investigator: Clark R. Chapman) A.* INTRODUCTION The asteroid research program during 1974/5 has three major goals: (1) continued spectrophotometric reconnaissance of the asteroid belt to define compositional types; (2) detailed spectrophotometric observations of particular asteroids, especially to determine variations with rotational phase, if any; and (3) synthesis of these data with other physical studies of asteroids and interpretation of the implications of physical studies of the asteroids for meteoritics and solar system history. The program has been an especially fruitful one, yielding fundamental new insights to the nature of the asteroids and the implications for the early development of the terrestrial planets. In particular, it is believed that the level of understanding of the asteroids has been reached, and sufficiently fundamental questions raised about their nature, that serious consideration should be given to possible future spacecraft missions directed to study a sample of asteroids at close range. Anders (1971) has argued that serious consideration of asteroid missions should be postponed until ground-based techniques for studying asteroids had been sufficiently exploited so that we could intelligently select appropriate asteroids for spacecraft targeting. It is clear that that point has been reached, ,and now that relatively inexpensive fly-by missions have been discovered to be possible by utilizing Venus and Earth gravity assists (Bender and Friedlander, 1975), serious planning for such missions ought to begin. -
August 2014 BRAS Newsletter
August, 2014 Next Meeting Augustth, 7:00 PM at HRPO M27, The Dumbbell Nebula-Taken at HRPO by Ben Toman What's In This Issue? President's Message Final Outreach Message from Dr. Trevor McGuire Astro Short-Milky Way: Cosmic Cannibal Message from the HRPO Globe At Night Recent BRAS Forum Entries Observing Notes from John Nagle President's Message Summertime in Louisiana isn’t always the best time to observe the sky. Even on nights with no cloud cover, there always seems to be a haze of water vapor or dust that washes out the dimmer things we want to see. However, we often get those still nights that are great for viewing the planets. At least we have that. And we always have the Sun. Speaking of that, we are getting close to selling enough tickets to raffle the Lunt 35mm solar telescope. Once we have sold enough tickets we will make an announcement to draw for the winner at the next BRAS meeting. In the meantime, we have lots of new (actually inherited) books to raffle, a couple of Messier and Caldwell cards, and a few other odd items. So, until we raffle the solar scope, there will be plenty to choose from between now and then. On a happy/sad note, we are losing one of our more active BRAS members to his new career. Vice President Muralidar Chakravarthi will be moving to Florida in mid-August for a promotion with his company. The August meeting may be the last one we may see him for quite a while. -
The Observer's Handbook for 1918
T he O bse r v e r s H andbook FOR 1918 P ublished By The Royal Astron o m ic a l Society of Canada E d i t e d b y C. A . CHANT TENTH YEAR OF PUBLICATION TORONTO 198 C o l l e g e S t r e e t Pr i n t e d f o r t h e S o c i e t y 1918 CALENDAR 1918 JANUARY FEBRUARY MARCH APRIL MAY JUNE JULY AUGUST SEPTEMBER OCTOBER NOVEMBER DECEMBER T he O bservers H andbook FOR 1918 P ublished By T he R oyal As tronomical Society of Canada E d i t e d b y C. A. CHANT TENTH YEAR OF PUBLICATION T O R O N T O 198 C o l l e g e S t r e e t Pr i n t e d f o r t h e S o c i e t y 1918 CONTENTS Preface - - - 2 Anniversaries and Festivals - - - 3 Occultation of Fixed Stars by the Moon - - 3 Ephemeris of the Sun . - - 4 The Sky and Astronomical Phenomena for each Month - 6 Eclipses, etc., of Jupiter’s Satellites - - - 30 Eclipses of Sun and Moon in 1918 - - 32 PREFACE In order to lower the expense of publication the H a n d b o o k for this year has been reduced to its present size. This reduction has been accomplished by omitting those portions which are not much altered from year to year. They include the following :— Symbols and abbreviations. -
Occuthubn(Gnewstetter
Occuthubn(gNewstetter Volume I, Number 3 January, 1975 Edited and Published by X. F, DaBoli at 6 N 106 White Oak Lane, St, Charles, Illinois 60174 U. S. A. GRAZING OCCULTATION TRACKS IN THE 1975 OCCULTATIDNS OF STARS BY (433) EROS 94 Pierce Rd., Watertown, Mass. 02172, OBSERVER'S HANDBOOK phone 6}7, 926-2678 Or 864-7360. In David It Dunham order to catch the event, it will be flue to an unfortunate error at the necessary to have observers at roughly printer's, the maps of the grazing qc- A map showing Brian Marsden's predic- even intervals across the whole region cu1tation tracks for 1975 were not in- tion for the path of the occultation of uncertginty. Observers are there- cluded in the 1975 Obgeme7"8 Hand- of Kappa Geminorum by Eros across fore urged to contact the above to co- book; the maps which appear are actu- southern Quebec, the northern tip of ordinate plans. ally those for 1974. We hope to pub- New Hainpshlre, and southern Maine is lish the correct maps in the February shown on p. 9 of the January issue of flue to the relatively low a?titude and Journal of the Royal Astronomical So- Sky and Telescope. Another prediction brtght moonlight, naked-eye observa- cietjjof Canada, and to send the maps was conputecf recently by Paul Herget tions will not be sufficient; at least to a interested observers. These at the Minor Ptanet Center at Cimin- smait binoculars or opera g7asses maps will be available early in the natl Observatory, According to Herget. -
The Complete the Complete Guide to Guide to Guide to Observing Observing Lunar, Grazing and Lunar, Grazing and Asteroid Occulta
The Complete Guide to Observing Lunar, Grazing and Asteroid Occultations Published by the International Occultation Timing Association Richard Nugent, Editor Copyright 2007 International Occultation Timing Association, Richard Nugent, Editor. All rights reserved. No part of this publication may be reproduced, distributed or copied in any manner without the written permission from the Editor in Chief. No part of this publication may be reproduced, stored in any retrieval system, or transmitted in any form or by any means, electronic, mechanical, photocopying, recording, scanning, or otherwise, except as permitted under the 1976 United States Copyright Act and with the written permission of the Editor and Publisher. Request to the Editor should be sent via email: [email protected]. While the Editor, Authors and Publisher have made their best efforts in preparing the IOTA Occultation Manual, they make no representation or warranties with respect to the accuracy and completeness regard to its contents. The Publisher, Editor and Authors specifically disclaim any implied warranties of merchantability or fitness of the material presented herein for any purpose. The advice and strategies contained herein may not be suitable for your situation and the reader and/or user assumes full responsibility for using and attempting the methods and techniques presented. Neither the publisher nor the authors shall be liable for any loss of profit or any damages, including but not limited to special, incidental, consequential, or other damages and any loss or injury. Persons are advised that occultation observations involve substantial risk and are advised to take the necessary precautions before attempting such observations. Editor in Chief: Richard Nugent Assistant Editor: Lydia Lousteaux Contributors: Trudy E. -
Adrian Zielonka's June 2021 Astronomy and Space News
Astronomy News Night Sky 2021 - June Sunrise Sunset Mercury Sets / Venus Sets Rises 1st – 5:02am 1st – 9:17pm 1st – 10:08pm 1st – 10:40pm 10th – 4:57am 10th – 9:25pm 11th – Inf 10th – 10:52pm 20th – 4:56am 20th – 9:29pm Conjunction 20th – 10:57pm 30th – 5:00am 30th – 9:29pm 26th – 4:18am 30th – 10:54pm 30th – 4:05am Moon Rise Moon Set Moon Rise Moon Set 1st - 2:05am 1st - 11:25am 20th – 4:05pm 21st – 2:40am 2nd – 2:26am (ESE) (WSW) 21st – 5:32pm (WSW) 3rd – 2:43am 2nd – 12:40pm (ESE) 22nd – 3:04am 4th – 2:57am 3rd – 1:52pm 22nd – 7:01pm 23rd – 3:34am 5th – 3:11am (E) 4th – 3:01pm (W) 23rd – 8:28pm 24th – 4:15am 6th – 3:25am 5th – 4:09pm 24th – 9:45pm 25th – 5:11am 7th – 3:41am 6th – 5:17pm 25th – 10:47pm 26th – 6:21am (ENE) 7th – 6:26pm 26th – 11:33pm 27th – 7:41am 8th – 3:58 am (WNW) 28th – 12:05am 28th – 9:02am 9th – 4:20am 8th – 7:34pm 29th – 12:29am 29th – 10:21am 10th – 4:48am 9th – 8:42pm (ESE) (WSW) 11th – 5:25am 10th – 9:47pm 30th – 12:48am 30th – 11:36am 12th – 6:11am 11th – 10:46pm 13th – 7:09am 12th – 11:35pm - - - - - - - - - - - - - - 14th – 8:16am 14th – 12:15am 15th – 9:29am 15th – 12:45am All times Moon Phases 16th – 10:44am 16th – 1:10am in notes are set Last Quarter – 2nd (ENE) 17th – 1:30am for New Moon – 10th 17th – 12:02pm (WNW) Somerton First Quarter – 18th – 1:20pm 18th – 1:48am unless stated 18th 19th – 2:41pm (E) 19th – 2:04am (W) Full Moon – 24th 20th – 2:21am A useful site: www.heavens-above.com A S Zielonka From the 30th May – 1st June Mars passes close to the star Kappa Geminorum (3.5 mag). -
Clusters Nebulae & Galaxies
CLUSTERS, NEBULAE & GALAXIES A NOVICE OBSERVER’S HANDBOOK By: Prof. P. N. Shankar PREFACE In the normal course of events, an amateur who builds or acquires a telescope will use it initially to observe the Moon and the planets. After the thrill of seeing the craters of the Moon, the Galilean moons of Jupiter and its bands, and the rings of Saturn he(*) is usually at a loss as to what to do next; Mars and Venus are usually disappointing as are the stars (they don’t look any bigger!). If the telescope had good resolution one could observe binaries, but alas, this is often not the case. Moreover, at this stage, the amateur is unlikely to be willing to do serious work on variable stars or on planetary observations. What can he do with his telescope that will rekindle his interest and prepare him for serious work? I believe that there is little better for him to do than hunt for the Messier objects; this book is meant as a guide in this exciting adventure. While this book is primarily a guide to the Messier objects, a few other easy clusters and nebulae have also been included. I have tried, while writing this handbook, to keep in mind the difficulties faced by a beginner. Even if one has good star maps, such as those in Norton’s Star Atlas, a beginner often has difficulty in locating some of the Messier objects because he does not know what he is expected to see! A cluster like M29 is a little difficult because it is a sparse cluster in a rich field; M97 is nominally brighter than M76, another planetary, but is more difficult to see; M33 is an approximately 6th magnitude galaxy but is far more difficult than many 9th magnitude galaxies. -
Adrian Zielonka's December 2020 Astronomy and Space News
Astronomy News Night Sky 2020 - December Sunrise Sunset Mercury Venus Rises 1st – 7:53am 1st – 4:07pm 1st – 5:19am 10th – 8:04am 10th – 4:04pm Not Visible 10th – 5:46am 20th – 8:12am 20th – 4:06pm this month. 20th – 6:16am 30th – 8:15am 30th – 4:13pm 30th – 6:43am Moon Rise Moon Set Moon Rise Moon Set - - - - - - - 1st – 8:54am 20th – 12:16pm (ESE) 20th – 10:46pm 1st – 4:52pm 2nd – 9:56am 21st – 12:33pm 21st – 11:55pm 2nd – 5:36pm 3rd – 10:50am 22nd – 12:48pm (E) 23rd – 1:02am (W) 3rd – 6:31pm 4th – 11:35am 23rd – 1:03pm 24th – 2:09am 4th – 7:37pm 5th – 12:10pm 24th – 1:18pm 25th – 3:16am 5th – 8:50pm 6th – 12:38pm 25th – 1:35pm (ENE) 26th – 4:24am (WNW) 6th – 10:07pm (ENE) 7th – 1:01pm (WNW) 26th – 1:55pm 27th – 5:33am 7th – 11:26pm 8th – 1:21pm 27th – 2:19pm 28th – 6:41am 9th – 12:46am 9th – 1:39pm (W) 28th – 2:50pm 29th – 7:46am 10th – 2:08am (E) 10th – 1:58pm 29th – 3:31pm 30th – 8:44am 11th – 3:32am 11th – 2:18pm 30th – 4:23pm 31st – 9:33am 12th – 4:58am (ESE) 12th – 2:42pm (WSW) 31st – 5:27pm - - - - - - - 13th – 6:26am 13th – 3:13pm - - - - - - - Moon Phases 14th – 7:51am 14th – 3:53pm All times Last Quarter – 8th 15th – 9:07am 15th – 4:45pm in notes are set New Moon – 14th 16th – 10:09am 16th – 5:50pm for First Quarter – 21st 17th – 10:56am 17th – 7:03pm Somerton Full Moon – 30th 18th – 11:30am 18th – 8:19pm unless stated 19th – 11:56am +4.5 19th – 9:34pm (WSW) A useful site: www.heavens- A S Zielonka above.com There is a planned launch (no earlier than December) of SpaceX CRS-21 Cargo mission to the International Space Station (ISS). -
Observing List
day month year Epoch 2000 local clock time: 2.00 Observing List for 17 11 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 58 286 Andromeda Gamma Andromedae (*266) 2.3 5.5 9.8 yellow & blue green double star 2 3.9 42 19 40 283 Andromeda Pi Andromedae 4.4 8.6 35.9 bright white & faint blue 0 36.9 33 43 48 295 Andromeda STF 79 (Struve) 6 7 7.8 bluish pair 1 0.1 44 42 59 279 Andromeda 59 Andromedae 6.5 7 16.6 neat pair, both greenish blue 2 10.9 39 2 32 301 Andromeda NGC 7662 (The Blue Snowball) planetary nebula, fairly bright & slightly elongated 23 25.9 42 32.1 44 292 Andromeda M31 (Andromeda Galaxy) large sprial arm galaxy like the Milky Way 0 42.7 41 16 44 291 Andromeda M32 satellite galaxy of Andromeda Galaxy 0 42.7 40 52 44 293 Andromeda M110 (NGC205) satellite galaxy of Andromeda Galaxy 0 40.4 41 41 56 279 Andromeda NGC752 large open cluster of 60 stars 1 57.8 37 41 62 285 Andromeda NGC891 edge on galaxy, needle-like in appearance 2 22.6 42 21 30 300 Andromeda NGC7640 elongated galaxy with mottled halo 23 22.1 40 51 35 308 Andromeda NGC7686 open cluster of 20 stars 23 30.2 49 8 47 258 Aries 1 Arietis 6.2 7.2 2.8 fine yellow & pale blue pair 1 50.1 22 17 57 250 Aries 30 Arietis 6.6 7.4 38.6 pleasing yellow pair 2 37 24 39 59 253 Aries 33 Arietis 5.5 8.4 28.6 yellowish-white & blue pair 2 40.7 27 4 59 239 Aries 48, Epsilon Arietis 5.2 5.5 1.5 white pair, splittable @ 150x 2 59.2 21 20 46 254 Aries 5, Gamma Arietis (*262) 4.8 4.8 7.8 nice bluish-white pair 1 53.5 19 18 49 258 Aries 9, Lambda Arietis -
Ephemerides Astronomicae ... Ad Meridianum Medioalanensum
Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. Linee guide per l’utilizzo Google è orgoglioso di essere il partner delle biblioteche per digitalizzare i materiali di pubblico dominio e renderli universalmente disponibili. I libri di pubblico dominio appartengono al pubblico e noi ne siamo solamente i custodi. Tuttavia questo lavoro è oneroso, pertanto, per poter continuare ad offrire questo servizio abbiamo preso alcune iniziative per impedire l’utilizzo illecito da parte di soggetti commerciali, compresa l’imposizione di restrizioni sull’invio di query automatizzate. Inoltre ti chiediamo di: + Non fare un uso commerciale di questi file Abbiamo concepito Google Ricerca Libri per l’uso da parte dei singoli utenti privati e ti chiediamo di utilizzare questi file per uso personale e non a fini commerciali.