HARLOW SHAPLEY November 2,1885-October 20,1972
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In This Issue (Dyed and Woven Cloth) and the Realm of Time and Space (Principles the Natural World)
No. 323 December 2004 Published monthly by Public Relations Center General Administration Div. Nippon Steel Corporation “A Pilgrimage: Colored Fibers Encounter Iron” More about Nippon Steel (A series of works by Kei Tsuji) —Contribution for December 2004— http://www.nsc.co.jp WWW (Works of art focused on “an alliance of iron—closely bound to both earth and man—with the arts of dyeing and weaving”) Born in Tokyo 1953, Kei Tsuji displays her installations, centered on dyeing and weaving, in deserts, woodlands and waterfronts the world over. Produced through a fieldwork approach, her installations represent a continuous pursuit of the connection between herself (dyed and woven cloth) and the realm of time and space (principles of the natural world). In this issue Regular Subscription Feature Story If you have received the web-version The Origin of Iron (Two-part series: 1) of Nippon Steel News, you are already —Birth of the Iron Star: Earth— a registered subscriber, thus no new registration is required. Associates who wish to become subscribers are requested to click on Operating Roundup the icon to complete and submit the registration form. Strategic Alliance between Nippon Steel and BHP Billiton WWW Nippon Steel and BHP Billiton have reached a basic agreement to mutually explore the possibility on strategic alliance for development of new mines and other fields. Operating Roundup Strategic Alliance between Nippon Steel and BHP Billiton WWW Back to Top Back Next No. 323 December 2004 Feature Story The Genesis of Product Making The Origin of Iron (Two-part Series: 1) From the Creation of the Universe to the Evolution of Life IRON formed the earth about 4.6 billion amount to about 232 billion tons, far great- years ago. -
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A&A 583, A85 (2015) Astronomy DOI: 10.1051/0004-6361/201526795 & c ESO 2015 Astrophysics Reaching the boundary between stellar kinematic groups and very wide binaries III. Sixteen new stars and eight new wide systems in the β Pictoris moving group F. J. Alonso-Floriano1, J. A. Caballero2, M. Cortés-Contreras1,E.Solano2,3, and D. Montes1 1 Departamento de Astrofísica y Ciencias de la Atmósfera, Facultad de Ciencias Físicas, Universidad Complutense de Madrid, 28040 Madrid, Spain e-mail: [email protected] 2 Centro de Astrobiología (CSIC-INTA), ESAC PO box 78, 28691 Villanueva de la Cañada, Madrid, Spain 3 Spanish Virtual Observatory, ESAC PO box 78, 28691 Villanueva de la Cañada, Madrid, Spain Received 19 June 2015 / Accepted 8 August 2015 ABSTRACT Aims. We look for common proper motion companions to stars of the nearby young β Pictoris moving group. Methods. First, we compiled a list of 185 β Pictoris members and candidate members from 35 representative works. Next, we used the Aladin and STILTS virtual observatory tools and the PPMXL proper motion and Washington Double Star catalogues to look for companion candidates. The resulting potential companions were subjects of a dedicated astro-photometric follow-up using public data from all-sky surveys. After discarding 67 sources by proper motion and 31 by colour-magnitude diagrams, we obtained a final list of 36 common proper motion systems. The binding energy of two of them is perhaps too small to be considered physically bound. Results. Of the 36 pairs and multiple systems, eight are new, 16 have only one stellar component previously classified as a β Pictoris member, and three have secondaries at or below the hydrogen-burning limit. -
The Birth of Stars and Planets
Unit 6: The Birth of Stars and Planets This material was developed by the Friends of the Dominion Astrophysical Observatory with the assistance of a Natural Science and Engineering Research Council PromoScience grant and the NRC. It is a part of a larger project to present grade-appropriate material that matches 2020 curriculum requirements to help students understand planets, with a focus on exoplanets. This material is aimed at BC Grade 6 students. French versions are available. Instructions for teachers ● For questions and to give feedback contact: Calvin Schmidt [email protected], ● All units build towards the Big Idea in the curriculum showing our solar system in the context of the Milky Way and the Universe, and provide background for understanding exoplanets. ● Look for Ideas for extending this section, Resources, and Review and discussion questions at the end of each topic in this Unit. These should give more background on each subject and spark further classroom ideas. We would be happy to help you expand on each topic and develop your own ideas for your students. Contact us at the [email protected]. Instructions for students ● If there are parts of this unit that you find confusing, please contact us at [email protected] for help. ● We recommend you do a few sections at a time. We have provided links to learn more about each topic. ● You don’t have to do the sections in order, but we recommend that. Do sections you find interesting first and come back and do more at another time. ● It is helpful to try the activities rather than just read them. -
A Basic Requirement for Studying the Heavens Is Determining Where In
Abasic requirement for studying the heavens is determining where in the sky things are. To specify sky positions, astronomers have developed several coordinate systems. Each uses a coordinate grid projected on to the celestial sphere, in analogy to the geographic coordinate system used on the surface of the Earth. The coordinate systems differ only in their choice of the fundamental plane, which divides the sky into two equal hemispheres along a great circle (the fundamental plane of the geographic system is the Earth's equator) . Each coordinate system is named for its choice of fundamental plane. The equatorial coordinate system is probably the most widely used celestial coordinate system. It is also the one most closely related to the geographic coordinate system, because they use the same fun damental plane and the same poles. The projection of the Earth's equator onto the celestial sphere is called the celestial equator. Similarly, projecting the geographic poles on to the celest ial sphere defines the north and south celestial poles. However, there is an important difference between the equatorial and geographic coordinate systems: the geographic system is fixed to the Earth; it rotates as the Earth does . The equatorial system is fixed to the stars, so it appears to rotate across the sky with the stars, but of course it's really the Earth rotating under the fixed sky. The latitudinal (latitude-like) angle of the equatorial system is called declination (Dec for short) . It measures the angle of an object above or below the celestial equator. The longitud inal angle is called the right ascension (RA for short). -
Effemeridi Astronomiche Di Milano Per L'anno
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. -
Chapter I Review Papers Harlow Shapley
Chapter I Review Papers Harlow Shapley Downloaded from https://www.cambridge.org/core. IP address: 170.106.40.40, on 25 Sep 2021 at 08:30:59, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900042340 Helen Sawyer Hogg and Willis Shapley remembering Willis Shapley fielding questions on his father Downloaded from https://www.cambridge.org/core. IP address: 170.106.40.40, on 25 Sep 2021 at 08:30:59, subject to the Cambridge Core terms of use, available at https://www.cambridge.org/core/terms. https://doi.org/10.1017/S0074180900042340 SHAPLEY'S DEBATE Michael Hoskin Cambridge University The attempt to make three-dimensional sense of the Milky Way goes back to a most unlikely origin: the English antiquary of the early eighteenth century, William Stukeley, remembered today for associating the Druids with Stonehenge. Stukeley came from Lincolnshire and so was a fellow-countryman of Isaac Newton, and as a result he was privileged to talk with the great man from time to time. In his Memoirs of Newton Stukeley records one conversation they had in about 1720, in which Stukeley proposed that the Sun and the brightest stars of the night sky make up what we today would term a globular cluster, and this cluster is surrounded by a gap, outside of which lie the small stars of the Milky Way in the form of a flattened ring. Stukeley's remarkable suggestion was recorded only in his manuscript memoirs, and had no effect on the subsequent history of astronomy. -
Our Milky Way.Key
Our Milky Way Learning Objectives ! What is the Milky Way? The Herschels thought we were at the center of our Galaxy...why were they wrong? ! How did Shapley prove we aren’t at the center? What are globular clusters? Cepheid Variable stars? ! How do we use Cepheid Variables to measure distance? ! What are the components of our Galaxy? What color are old stars? Young stars? Does our Galaxy get older or younger as you move out (i.e. from the disk to the halo)? ! How do we know our Galaxy is a spiral galaxy? ! Do stars in our Galaxy’s disk orbit as Kepler’s Laws would predict? What is a rotation curve? Why does our Galaxy’s rotation curve suggest dark matter exists? The Milky Way ! Our Galaxy is a collection of stars, nebulae, molecular clouds, and stellar remnants ! All bound together by gravity ! Connected by the stellar evolution cycle Determining the Shape of our Galaxy ! The number of 6400 ly stars were counted in all directions from 1300 ly the Sun by Sun Caroline Herschel and her brother William ! They assumed that all stars have the same brightness and that space contains no dust – these are incorrect assumptions ! They thus concluded that the Sun is at the center of the Universe - which is not true The Importance of Dust ! Dust dims and reddens starlight ! There is more dust toward the center of the Galaxy ! Consequence: We underestimate the number of stars in one direction ! We appear to be near the center, but we’re not Us Star Sun Can’t see stars here (if we’re looking for blue light from them) How Do We Find the Galactic Center? -
How Supernovae Became the Basis of Observational Cosmology
Journal of Astronomical History and Heritage, 19(2), 203–215 (2016). HOW SUPERNOVAE BECAME THE BASIS OF OBSERVATIONAL COSMOLOGY Maria Victorovna Pruzhinskaya Laboratoire de Physique Corpusculaire, Université Clermont Auvergne, Université Blaise Pascal, CNRS/IN2P3, Clermont-Ferrand, France; and Sternberg Astronomical Institute of Lomonosov Moscow State University, 119991, Moscow, Universitetsky prospect 13, Russia. Email: [email protected] and Sergey Mikhailovich Lisakov Laboratoire Lagrange, UMR7293, Université Nice Sophia-Antipolis, Observatoire de la Côte d’Azur, Boulevard de l'Observatoire, CS 34229, Nice, France. Email: [email protected] Abstract: This paper is dedicated to the discovery of one of the most important relationships in supernova cosmology—the relation between the peak luminosity of Type Ia supernovae and their luminosity decline rate after maximum light. The history of this relationship is quite long and interesting. The relationship was independently discovered by the American statistician and astronomer Bert Woodard Rust and the Soviet astronomer Yury Pavlovich Pskovskii in the 1970s. Using a limited sample of Type I supernovae they were able to show that the brighter the supernova is, the slower its luminosity declines after maximum. Only with the appearance of CCD cameras could Mark Phillips re-inspect this relationship on a new level of accuracy using a better sample of supernovae. His investigations confirmed the idea proposed earlier by Rust and Pskovskii. Keywords: supernovae, Pskovskii, Rust 1 INTRODUCTION However, from the moment that Albert Einstein (1879–1955; Whittaker, 1955) introduced into the In 1998–1999 astronomers discovered the accel- equations of the General Theory of Relativity a erating expansion of the Universe through the cosmological constant until the discovery of the observations of very far standard candles (for accelerating expansion of the Universe, nearly a review see Lipunov and Chernin, 2012). -
121012-AAS-221 Program-14-ALL, Page 253 @ Preflight
221ST MEETING OF THE AMERICAN ASTRONOMICAL SOCIETY 6-10 January 2013 LONG BEACH, CALIFORNIA Scientific sessions will be held at the: Long Beach Convention Center 300 E. Ocean Blvd. COUNCIL.......................... 2 Long Beach, CA 90802 AAS Paper Sorters EXHIBITORS..................... 4 Aubra Anthony ATTENDEE Alan Boss SERVICES.......................... 9 Blaise Canzian Joanna Corby SCHEDULE.....................12 Rupert Croft Shantanu Desai SATURDAY.....................28 Rick Fienberg Bernhard Fleck SUNDAY..........................30 Erika Grundstrom Nimish P. Hathi MONDAY........................37 Ann Hornschemeier Suzanne H. Jacoby TUESDAY........................98 Bethany Johns Sebastien Lepine WEDNESDAY.............. 158 Katharina Lodders Kevin Marvel THURSDAY.................. 213 Karen Masters Bryan Miller AUTHOR INDEX ........ 245 Nancy Morrison Judit Ries Michael Rutkowski Allyn Smith Joe Tenn Session Numbering Key 100’s Monday 200’s Tuesday 300’s Wednesday 400’s Thursday Sessions are numbered in the Program Book by day and time. Changes after 27 November 2012 are included only in the online program materials. 1 AAS Officers & Councilors Officers Councilors President (2012-2014) (2009-2012) David J. Helfand Quest Univ. Canada Edward F. Guinan Villanova Univ. [email protected] [email protected] PAST President (2012-2013) Patricia Knezek NOAO/WIYN Observatory Debra Elmegreen Vassar College [email protected] [email protected] Robert Mathieu Univ. of Wisconsin Vice President (2009-2015) [email protected] Paula Szkody University of Washington [email protected] (2011-2014) Bruce Balick Univ. of Washington Vice-President (2010-2013) [email protected] Nicholas B. Suntzeff Texas A&M Univ. suntzeff@aas.org Eileen D. Friel Boston Univ. [email protected] Vice President (2011-2014) Edward B. Churchwell Univ. of Wisconsin Angela Speck Univ. of Missouri [email protected] [email protected] Treasurer (2011-2014) (2012-2015) Hervey (Peter) Stockman STScI Nancy S. -
Divinus Lux Observatory Bulletin: Report # 27
Vol. 9 No. 1 January 1, 2013 Journal of Double Star Observations Page 10 Divinus Lux Observatory Bulletin: Report # 27 Dave Arnold Program Manager for Double Star Research 2728 North Fox Run Drive Flagstaff, AZ 86004 Email: [email protected] Abstract: This report contains theta/rho measurements from 120 different double star systems. The time period spans from 2012.189 to 2012.443. Measurements were obtained using a 20-cm Schmidt-Cassegrain telescope and an illuminated reticle micrometer. This report represents a portion of the work that is currently being conducted in double star astronomy at Divinus Lux Observatory in Flagstaff, Arizona. This article contains a listing of double star the theta value. Perhaps AC warrants further scru- measurements that are part of a series, which have tiny by others in order to determine, more accu- been continuously reported at Divinus Lux Observa- rately, what these parameters actually are. tory, since the spring of 2001. The selected double Some other apparent discrepancies in the star systems, which appear in the table below, have catalog involve the STF 2319 (18277+1918) star sys- been taken exclusively from the 2006.5 version of the tem. To begin with, the measurements for the AC Washington Double Star Catalog, with published components appear to more nearly match the pa- measurements that are no more recent than ten rameters for BC, while the BC measurements appear years ago. There are also some noteworthy items to match the AC parameters. In addition, the theta that are discussed, which pertain to a few of the measurements for AD appear to reflect a quadrant measured systems. -
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. -
Crystal Reports Activex Designer
Quiz List—Reading Practice Page 1 Printed Wednesday, March 18, 2009 2:36:33PM School: Churchland Academy Elementary School Reading Practice Quizzes Quiz Word Number Lang. Title Author IL ATOS BL Points Count F/NF 9318 EN Ice Is...Whee! Greene, Carol LG 0.3 0.5 59 F 9340 EN Snow Joe Greene, Carol LG 0.3 0.5 59 F 36573 EN Big Egg Coxe, Molly LG 0.4 0.5 99 F 9306 EN Bugs! McKissack, Patricia C. LG 0.4 0.5 69 F 86010 EN Cat Traps Coxe, Molly LG 0.4 0.5 95 F 9329 EN Oh No, Otis! Frankel, Julie LG 0.4 0.5 97 F 9333 EN Pet for Pat, A Snow, Pegeen LG 0.4 0.5 71 F 9334 EN Please, Wind? Greene, Carol LG 0.4 0.5 55 F 9336 EN Rain! Rain! Greene, Carol LG 0.4 0.5 63 F 9338 EN Shine, Sun! Greene, Carol LG 0.4 0.5 66 F 9353 EN Birthday Car, The Hillert, Margaret LG 0.5 0.5 171 F 9305 EN Bonk! Goes the Ball Stevens, Philippa LG 0.5 0.5 100 F 7255 EN Can You Play? Ziefert, Harriet LG 0.5 0.5 144 F 9314 EN Hi, Clouds Greene, Carol LG 0.5 0.5 58 F 9382 EN Little Runaway, The Hillert, Margaret LG 0.5 0.5 196 F 7282 EN Lucky Bear Phillips, Joan LG 0.5 0.5 150 F 31542 EN Mine's the Best Bonsall, Crosby LG 0.5 0.5 106 F 901618 EN Night Watch (SF Edition) Fear, Sharon LG 0.5 0.5 51 F 9349 EN Whisper Is Quiet, A Lunn, Carolyn LG 0.5 0.5 63 NF 74854 EN Cooking with the Cat Worth, Bonnie LG 0.6 0.5 135 F 42150 EN Don't Cut My Hair! Wilhelm, Hans LG 0.6 0.5 74 F 9018 EN Foot Book, The Seuss, Dr.