Astrochallenge 2018 Multiple Choice Questions (Senior)
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The Fall of the Youngest Planetary Nebula, Hen3-1357
IOP Publishing Submitted in this form to ApJ 3 Sept 2020 Astrophysical Journal ApJ (XXXX) XXXXXX https://doi.org/XXXX/XXXX The Fall of the Youngest Planetary Nebula, Hen3-1357 Bruce Balick1*, Martín A. Guerrero2, Gerardo Ramos-Larios3 1 Department of Astronomy, University of Washington, Seattle, WA 98195-1580, USA 2 Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía S/N, 18008 Granada, Spain 3 Instituto de Astronomía y Meteorología, Universidad de Guadalajara, 44130 Guadalajara, Mexico *Corresponding author: [email protected] Received xxxxxx Accepted for publication xxxxxx Published xxxxxx Abstract The Stingray Nebula, aka Hen3-1357, went undetected until 1990 when bright nebular lines and radio emission were unexpectedly discovered. We report changes in shape and rapid and secular decreases in its nebular emission-line fluxes based on well calibrated images obtained by the Hubble Space Telescope in 1996, 2000, and 2016. Hen3-1357 is now a “recombination nebula”. Keywords: planetary nebulae: Planetary nebulae (1249), Post-asymptotic giant branch stars (2121), Ionization (2068) 1. Introduction Planetary nebulae (“PNe”) consist of stellar gas ejected in winds from the surfaces of post Asymptotic Branch Giant (“AGB”) stars. The winds systematically expose deeper and much hotter interior stellar layers until stellar energetic ultraviolet (“UV”) begins to ionize the ejected gas. The PN radiates a rich, luminous, and readily detectable set of emission lines (e.g., 6) as electron recombinations with H+ and He+ and optical forbidden lines of N+, O+, O++, S+, etc. These lines become increasingly visible by about a millennium after the winds begin as the central star shifts towards higher temperatures > 40 kK. -
Messier 58, 59, 60, 89, and 90, Galaxies in Virgo
Messier 58, 59, 60, 89, and 90, Galaxies in Virgo These are five of the many galaxies of the Coma-Virgo galaxy cluster, a prime hunting ground for galaxy observers every spring. Dozens of galaxies in this cluster are visible in medium to large amateur telescopes. This star hop includes elliptical galaxies M59, M60, and M89, and spiral galaxies M58 and M90. These galaxies are roughly 50 to 60 million light years away. All of them are around magnitude 10, and should be visible in even a small telescope. Start by finding the Spring Triangle, which consists of three widely- separated first magnitude stars-- Arcturus, Spica, and Regulus. The Spring Triangle is high in the southeast sky in early spring, and in the southwest sky by mid-Summer. (To get oriented, you can use the handle of the Big Dipper and "follow the arc to Arcturus"). For this star hop, look in the middle of the Spring Triangle for Denebola, the star representing the back end of Leo, the lion, and Vindemiatrix, a magnitude 2.8 star in Virgo. The galaxies of the Virgo cluster are found in the area between these two stars. From Vindemiatrix, look 5 degrees west and slightly south to find ρ (rho) Virginis, a magnitude 4.8 star that is easy to identify because it is paired with a slightly dimmer star just to its north. Center ρ in the telescope with a low-power eyepiece, and then just move 1.4 degrees north to arrive at the oval shape of M59. Continuing with a low-power eyepiece and using the chart below, you can take hops of less than 1 degree to find M60 to the east of M59, and M58, M89, and M90 to the west and north. -
Remote Video Astronomy Group MECATX Sky Tour May 2020
Remote Video Astronomy Group MECATX Sky Tour May 2020 1) Boötes (bo-OH-teez), the Herdsman - May 2 2) Libra (LEE-bruh), the Scales - May 9 3) Lupus (LOOP-us), the Wolf - May 9 4) Ursa Minor (ER-suh MY-ner), the Little Bear - May 13 5) Corona Borealis (cuh-ROE-nuh bor-ee-AL-iss) the Northern Crown - May 19 6) Norma (NOR-muh), the Carpenter's Square - May 19 7) Apus (APE-us), the Bird of Paradise - May 21 8) Triangulum Australe (try-ANG-gyuh-lum aw-STRAL-ee), the Southern Triangle - May 23 9) Draco (DRAY-co), the Dragon - May 24 MECATX RVA May 2019 - www.mecatx.ning.com – YouTube – MECATX – www.ustream.tv – dfkott Revised: Alyssa Donnell 04.19.2020 May 2 Boötes (bo-OH-teez), the Herdsman Boo Boötis (bo-OH-tiss) MECATX RVA May 2019 - www.mecatx.ning.com – YouTube – MECATX – www.ustream.tv – dfkott 1 Boötes Meaning: The Bear Driver Pronunciation: bow owe' teez Abbreviation: Boo Possessive form: Boötis (bow owe' tiss) Asterisms: The Diamond [of Virgo], The Ice Cream Cone, The Kite, The Spring Triangle, The Trapezoid Bordering constellations: Canes Venatici, Coma Berenices, Corona Borealis, Draco, Hercules, Serpens, Ursa Major, Virgo Overall brightness: 5.845 (59) Central point: RA = 14h40m Dec.= +31° Directional extremes: N = +55° S = +7° E = 15h47m W = 13h33m Messier objects: none Meteor showers: Quadrantids (3 Jan),4 Boötids (1 May), a Boötids (28 Apr), June Bootids (28 Jun) Midnight culmination date: 2 May Bright stars: a (4), F, (78), i (106), y (175) Named stars: Arcturus (a), Hans (y), Izar (s), Merez (3), Merga (38), Mufrid (ii), Nekkar -
Asterism and Constellation: Terminological Dilemmas
www.ebscohost.com www.gi.sanu.ac.rs, www.doiserbia.nb.rs, J. Geogr. Inst. Cvijic. 67(1) (1–10) Original scientific paper UDC: 521/525 DOI: https://doi.org/10.2298/IJGI1701001P ASTERISM AND CONSTELLATION: TERMINOLOGICAL DILEMMAS Zorica Prnjat *1, Milutin Tadić * * University of Belgrade, Faculty of Geography, Belgrade, Serbia Received: March 14, 2017; Reviewed: March 23, 2017; Accepted: March 31, 2017 Abstract: In contemporary astronomical literature, there is no uniform definition of the term asterism. This inconsistency is the consequence of differences between the traditional understanding of the term constellation, from the standpoint of the naked eye astronomy, and its contemporary understanding from the standpoint of the International Astronomical Union. A traditional constellation is a recognizable star configuration with a well-established name, whereas the International Astronomical Union defines a constellation as an exactly defined sector of the cosmic space that belongs to a particular traditional constellation. Asterism is a lower rank term in comparison to constellation, and as such it may not denote a whole traditional constellation, as these terms would become synonymous and parts of constellations would become “asterisms of asterisms“. Similarly, asterism cannot define a macro configuration composed of the brightest stars in more constellations, thus, the Summer Triangle and other sky polygons are not asterisms. Therefore, asterisms are neither constellations nor sky polygons, but the third – easily recognizable parts of traditional constellations with historically well-established names, including separate groups of smaller stars that belong to star clusters (autonomous asterisms). Forms and names of asterisms may or may not be consistent with the parent constellation, and accordingly asterisms can be divided into compatible and incompatible. -
Indian Institute of Astrophysics Academic Report 1997-1998
INDIAN INSTITUTE OF ASTROPHYSICS ACADEMIC REPORT 1997-1998 ecf1ted by: P.Venkatakrishnan Editorial Assmance : Sandra Rajiva Front Cover Radioheliogram of active region obtained from Gauribidanur. Back Cover Lab simulation of optical interferometry. Interferogram produced with seven holes at High Angular Resolution Laboratory. Bangelore. Prned at Vykat Pmta Pvt. Ud.• Aiport Road Cross, Banga/ore 560017 CONTENTS Page Page Governing Council 1 Library 48 Highlights of the year 1997-98 3 Official Language Implementation 48 Sun and the solar system 7 Personnel 49 Stars and stellar systems 17 Appendixes 51 Theoretical Astrophysics 27 A: Publications 5:1 Physics 35 B: HRD Activities 65 Facilities 39 C: Sky Conditions at VBO and Kodaikanal Observatory 67 GOVERNING COUNCIL 1 Prof. B. V. Sreekantan Chairman Prof. Yash Pal Member S. Radhakrishnan Professor Chairman, Steering Committee National Institute of Advanced Studies Inter-University Consortium for Indian Inst.itute of Science Campus Educational Communication Bangalore 560012 New Delhi 110067 Prof. V.S. Ramamurthy Member Prof. 1. B. S. Passil Member Secretary Professor, Department of Science and Technology Centre for Advanced Study in Mathematics New Delhi 110016 Panjab University Chandigarh 160014 Sri Rahul Sarin, lAS Member Joint Secretary and Financial Advisor Prof. H. S. Mani2 Membpr Department. of Science and Technology Director New Delhi 110016 Mehta Research Institute of Mathematirs & Mathematical Physics Prof. J. C. Bhattacharyya2 Member Chhatnag Road, Jhusi 215, Trinity Enclave Allahabad 221506 Old Madras Road Bangalore 560008 Dr. S.K. Sikka Associate Director, Prof. Ramanath Cowsik Member Solid St.ate & Spectroscopy Group, and Director Head, High Pressure Physics Division Indian Institute of Astrophysics BARC, Trombay, Mumbai 400085 Bangalore 560034 Prof. -
Messier 61, Oriani's Galaxy
Messier 61, Oriani’s Galaxy This beautiful face-on barred spiral galaxy was discovered in 1779 by Barnabas Oriani, a Catholic priest and accomplished astronomer, and it became the 61st entry in Messier's catalog. It is on the southern outskirts of the Virgo galaxy cluster. Through small scopes, it appears as a circular glow with a brighter center. Large scopes will show its two large spiral arms. Start by finding the Spring Triangle, which consists of three widely- separated first magnitude stars-- Arcturus, Spica, and Regulus. The Spring Triangle is high in the southeast sky in early spring, and in the southwest sky by mid-Summer. (To get oriented, you can use the handle of the Big Dipper and "follow the arc to Arcturus"). For this star hop, look in the middle of the Spring Triangle for Denebola, the star representing the back end of Leo, the lion, and Vindemiatrix, a magnitude 2.8 star in Virgo. The galaxies of the Virgo cluster are found in the area between these two stars. From Vindemiatrix, trace the curving arc of stars that form part of the constellation Virgo to reach Zaniah, as shown below. All of these stars should be easy to see with the naked eye under a clear sky. From Zaniah, move 4 degrees north to a 5th magnitude star that will be easily visible in binoculars or a finderscope. Center this star in your telescope with a low-power eyepiece, then move a little more than 1 degree to the north- northeast to reach M61. Star hop from www.skyledge.net by Jim Mazur. -
Observing the Way It Was Meant to Be Nothing Is Better Than Observing Under a Dark, Clear, Steady Sky
THE CIGaR GALAXY (M82) in Ursa deep-sky observing Major is a great object for 6-inch or larger telescopes. Through a 30-inch What we saw through a 30-inch telescope under an inky black sky scope at 736x, however, it ranks as a blew our minds. ⁄ ⁄ ⁄ BY michael e. Bakich spectacular sight. Tony and daphne hallas Observing the way it was meant to be Nothing is better than observing under a dark, clear, steady sky. Wait, one thing’s better — observing that sky through a large scope. In February, I had the opportunity to do just that under the pristine conditions at Arizona Sky Village (ASV), located in Portal, Arizona. As a guest of real-estate developer Eugene more detail you’ll see. If you double the Turner, I had 2 nights with Turner’s superb aperture, you capture 4 times as much 30-inch Starmaster telescope. light. So, an 8-inch telescope gathers 4 The 30-inch is a high-quality Newto- times as much light as a 4-inch. nian reflector on a Dobsonian mount. I’d But there’s another advantage to all the THE GhOsT OF JUPiTeR (NGC 3242) is a used this telescope one year earlier, with light a large scope collects. The object may small object. Its bright inner sphere mea- Astronomy’s editor, David J. Eicher. We appear bright enough to trigger your eyes’ sures only 25" across. Seeing the 40"-wide observed many celestial wonders in Orion color receptors. A planetary nebula that outer halo and fine details requires a large and the rest of the winter sky. -
Orders of Magnitude (Length) - Wikipedia
03/08/2018 Orders of magnitude (length) - Wikipedia Orders of magnitude (length) The following are examples of orders of magnitude for different lengths. Contents Overview Detailed list Subatomic Atomic to cellular Cellular to human scale Human to astronomical scale Astronomical less than 10 yoctometres 10 yoctometres 100 yoctometres 1 zeptometre 10 zeptometres 100 zeptometres 1 attometre 10 attometres 100 attometres 1 femtometre 10 femtometres 100 femtometres 1 picometre 10 picometres 100 picometres 1 nanometre 10 nanometres 100 nanometres 1 micrometre 10 micrometres 100 micrometres 1 millimetre 1 centimetre 1 decimetre Conversions Wavelengths Human-defined scales and structures Nature Astronomical 1 metre Conversions https://en.wikipedia.org/wiki/Orders_of_magnitude_(length) 1/44 03/08/2018 Orders of magnitude (length) - Wikipedia Human-defined scales and structures Sports Nature Astronomical 1 decametre Conversions Human-defined scales and structures Sports Nature Astronomical 1 hectometre Conversions Human-defined scales and structures Sports Nature Astronomical 1 kilometre Conversions Human-defined scales and structures Geographical Astronomical 10 kilometres Conversions Sports Human-defined scales and structures Geographical Astronomical 100 kilometres Conversions Human-defined scales and structures Geographical Astronomical 1 megametre Conversions Human-defined scales and structures Sports Geographical Astronomical 10 megametres Conversions Human-defined scales and structures Geographical Astronomical 100 megametres 1 gigametre -
Astronomers Observe Star Reborn in a Flash 13 September 2016
Astronomers observe star reborn in a flash 13 September 2016 astronomers have observed an exception to this rule. "SAO 244567 is one of the rare examples of a star that allows us to witness stellar evolution in real time", explains Nicole Reindl from the University of Leicester, UK, lead author of the study. "Over only twenty years the star has doubled its temperature and it was possible to watch the star ionising its previously ejected envelope, which is now known as the Stingray Nebula." SAO 244567, 2700 light-years from Earth, is the central star of the Stingray Nebula and has been visibly evolving between observations made over the last 45 years. Between 1971 and 2002 the surface temperature of the star skyrocketed by almost 40 000 degrees Celsius. Now new observations made with the Cosmic Origins Spectrograph (COS) on the NASA/ESA Hubble Space Telescope have revealed that SAO 244567 has started to cool and expand. This image of the Stingray nebula, a planetary nebula This is unusual, though not unheard-of, and the 2400 light-years from Earth, was taken with the Wide rapid heating could easily be explained if one Field and Planetary Camera 2 (WFPC2) in 1998. In the assumed that SAO 244567 had an initial mass of 3 centre of the nebula the fast evolving star SAO 244567 to 4 times the mass of the Sun. However, the data is located. Observations made within the last 45 years show that SAO 244567 must have had an original showed that the surface temperature of the star mass similar to that of our Sun. -
The Agb Newsletter
THE AGB NEWSLETTER An electronic publication dedicated to Asymptotic Giant Branch stars and related phenomena Official publication of the IAU Working Group on Red Giants and Supergiants No. 279 — 2 October 2020 https://www.astro.keele.ac.uk/AGBnews Editors: Jacco van Loon, Ambra Nanni and Albert Zijlstra Editorial Board (Working Group Organising Committee): Marcelo Miguel Miller Bertolami, Carolyn Doherty, JJ Eldridge, Anibal Garc´ıa-Hern´andez, Josef Hron, Biwei Jiang, Tomasz Kami´nski, John Lattanzio, Emily Levesque, Maria Lugaro, Keiichi Ohnaka, Gioia Rau, Jacco van Loon (Chair) Figure 1: The Rapid Fading of the Youngest Planetary Nebula, Hen 3-1357. Two composite Hubble images of the Sting Ray Nebula taken in 1996 and 2016 in (R:G:B) = (F658N,F656N,F502N) = the emission lines of ([N ii], Hα, [O iii]). Both images are shown with the same absolute intensities in each filter. Nebular emission from Hen3-1357, the youngest planetary nebula (Bobrowsky, 1994, ApJ, 426, L47), unexpectedly appeared sometime during the 1980s (Parthasarathy et al. 1993, A&A, 267, 19). Since then the central star has rapidly faded (e.g., Schaefer & Edwards, 2015, ApJ, 812, 133). The integrated emission fluxes of these three lines in the images above decreased by factors of 0.20, 0.37, and 0.6, respectively, over 20 years. As expected, the rates of fading are much higher in regions of highest emission measure as N+, H+, and O++ recombine. See Balick et al. in this issue. 1 Editorial Dear Colleagues, It is a pleasure to present you the 279th issue of the AGB Newsletter. -
Popular Names of Deep Sky (Galaxies,Nebulae and Clusters) Viciana’S List
POPULAR NAMES OF DEEP SKY (GALAXIES,NEBULAE AND CLUSTERS) VICIANA’S LIST 2ª version August 2014 There isn’t any astronomical guide or star chart without a list of popular names of deep sky objects. Given the huge amount of celestial bodies labeled only with a number, the popular names given to them serve as a friendly anchor in a broad and complicated science such as Astronomy The origin of these names is varied. Some of them come from mythology (Pleiades); others from their discoverer; some describe their shape or singularities; (for instance, a rotten egg, because of its odor); and others belong to a constellation (Great Orion Nebula); etc. The real popular names of celestial bodies are those that for some special characteristic, have been inspired by the imagination of astronomers and amateurs. The most complete list is proposed by SEDS (Students for the Exploration and Development of Space). Other sources that have been used to produce this illustrated dictionary are AstroSurf, Wikipedia, Astronomy Picture of the Day, Skymap computer program, Cartes du ciel and a large bibliography of THE NAMES OF THE UNIVERSE. If you know other name of popular deep sky objects and you think it is important to include them in the popular names’ list, please send it to [email protected] with at least three references from different websites. If you have a good photo of some of the deep sky objects, please send it with standard technical specifications and an optional comment. It will be published in the names of the Universe blog. It could also be included in the ILLUSTRATED DICTIONARY OF POPULAR NAMES OF DEEP SKY. -
The Complete Idiot's Guide to Astronomy
00 1981 FM 6/11/01 9:55 AM Page i Astronomy Second Edition by Christopher De Pree and Alan Axelrod A Pearson Education Company 00 1981 FM 6/11/01 9:55 AM Page ii To my girls, Julia, Claire, and Madeleine (CGD) For my stars, Anita and Ian (AA) Copyright © 2001 by The Ian Samuel Group, Inc. All rights reserved. No part of this book shall be reproduced, stored in a retrieval sys- tem, or transmitted by any means, electronic, mechanical, photocopying, recording, or otherwise, without written permission from the publisher. No patent liability is as- sumed with respect to the use of the information contained herein. Although every precaution has been taken in the preparation of this book, the publisher and authors assume no responsibility for errors or omissions. Neither is any liability assumed for damages resulting from the use of information contained herein. For information, ad- dress Alpha Books, 201 West 103rd Street, Indianapolis, IN 46290. THE COMPLETE IDIOT’S GUIDE TO and Design are registered trademarks of Pearson Education, Inc. International Standard Book Number:1-5925-7003-8 Library of Congress Catalog Card Number: 2001091092 03020187654321 Interpretation of the printing code: The rightmost number of the first series of num- bers is the year of the book’s printing; the rightmost number of the second series of numbers is the number of the book’s printing. For example, a printing code of 01-1 shows that the first printing occurred in 2001. Printed in the United States of America Note:This publication contains the opinions and ideas of its authors.