Measuring the Universe: a Brief History of Time
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
The Dunhuang Chinese Sky: a Comprehensive Study of the Oldest Known Star Atlas
25/02/09JAHH/v4 1 THE DUNHUANG CHINESE SKY: A COMPREHENSIVE STUDY OF THE OLDEST KNOWN STAR ATLAS JEAN-MARC BONNET-BIDAUD Commissariat à l’Energie Atomique ,Centre de Saclay, F-91191 Gif-sur-Yvette, France E-mail: [email protected] FRANÇOISE PRADERIE Observatoire de Paris, 61 Avenue de l’Observatoire, F- 75014 Paris, France E-mail: [email protected] and SUSAN WHITFIELD The British Library, 96 Euston Road, London NW1 2DB, UK E-mail: [email protected] Abstract: This paper presents an analysis of the star atlas included in the medieval Chinese manuscript (Or.8210/S.3326), discovered in 1907 by the archaeologist Aurel Stein at the Silk Road town of Dunhuang and now held in the British Library. Although partially studied by a few Chinese scholars, it has never been fully displayed and discussed in the Western world. This set of sky maps (12 hour angle maps in quasi-cylindrical projection and a circumpolar map in azimuthal projection), displaying the full sky visible from the Northern hemisphere, is up to now the oldest complete preserved star atlas from any civilisation. It is also the first known pictorial representation of the quasi-totality of the Chinese constellations. This paper describes the history of the physical object – a roll of thin paper drawn with ink. We analyse the stellar content of each map (1339 stars, 257 asterisms) and the texts associated with the maps. We establish the precision with which the maps are drawn (1.5 to 4° for the brightest stars) and examine the type of projections used. -
Geodesy Methods Over Time
Geodesy methods over time GISC3325 - Lecture 4 Astronomic Latitude/Longitude • Given knowledge of the positions of an astronomic body e.g. Sun or Polaris and our time we can determine our location in terms of astronomic latitude and longitude. US Meridian Triangulation This map shows the first project undertaken by the founding Superintendent of the Survey of the Coast Ferdinand Hassler. Triangulation • Method of indirect measurement. • Angles measured at all nodes. • Scaled provided by one or more precisely measured base lines. • First attributed to Gemma Frisius in the 16th century in the Netherlands. Early surveying instruments Left is a Quadrant for angle measurements, below is how baseline lengths were measured. A non-spherical Earth • Willebrod Snell van Royen (Snellius) did the first triangulation project for the purpose of determining the radius of the earth from measurement of a meridian arc. • Snellius was also credited with the law of refraction and incidence in optics. • He also devised the solution of the resection problem. At point P observations are made to known points A, B and C. We solve for P. Jean Picard’s Meridian Arc • Measured meridian arc through Paris between Malvoisine and Amiens using triangulation network. • First to use a telescope with cross hairs as part of the quadrant. • Value obtained used by Newton to verify his law of gravitation. Ellipsoid Earth Model • On an expedition J.D. Cassini discovered that a one-second pendulum regulated at Paris needed to be shortened to regain a one-second oscillation. • Pendulum measurements are effected by gravity! Newton • Newton used measurements of Picard and Halley and the laws of gravitation to postulate a rotational ellipsoid as the equilibrium figure for a homogeneous, fluid, rotating Earth. -
OF Versailles
THE CHÂTEAU DE VErSAILLES PrESENTS science & CUrIOSITIES AT THE COUrT OF versailles AN EXHIBITION FrOM 26 OCTOBEr 2010 TO 27 FEBrUArY 2011 3 Science and Curiosities at the Court of Versailles CONTENTS IT HAPPENED AT VErSAILLES... 5 FOrEWOrD BY JEAN-JACqUES AILLAGON 7 FOrEWOrD BY BÉATrIX SAULE 9 PrESS rELEASE 11 PArT I 1 THE EXHIBITION - Floor plan 3 - Th e exhibition route by Béatrix Saule 5 - Th e exhibition’s design 21 - Multimedia in the exhibition 22 PArT II 1 ArOUND THE EXHIBITION - Online: an Internet site, and TV web, a teachers’ blog platform 3 - Publications 4 - Educational activities 10 - Symposium 12 PArT III 1 THE EXHIBITION’S PArTNErS - Sponsors 3 - Th e royal foundations’ institutional heirs 7 - Partners 14 APPENDICES 1 USEFUL INFOrMATION 3 ILLUSTrATIONS AND AUDIOVISUAL rESOUrCES 5 5 Science and Curiosities at the Court of Versailles IT HAPPENED AT VErSAILLES... DISSECTION OF AN Since then he has had a glass globe made that ELEPHANT WITH LOUIS XIV is moved by a big heated wheel warmed by holding IN ATTENDANCE the said globe in his hand... He performed several experiments, all of which were successful, before Th e dissection took place at Versailles in January conducting one in the big gallery here... it was 1681 aft er the death of an elephant from highly successful and very easy to feel... we held the Congo that the king of Portugal had given hands on the parquet fl oor, just having to make Louis XIV as a gift : “Th e Academy was ordered sure our clothes did not touch each other.” to dissect an elephant from the Versailles Mémoires du duc de Luynes Menagerie that had died; Mr. -
Wynyard Planetarium & Observatory a Autumn Observing Notes
Wynyard Planetarium & Observatory A Autumn Observing Notes Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn Tour of the Sky with the Naked Eye CASSIOPEIA Look for the ‘W’ 4 shape 3 Polaris URSA MINOR Notice how the constellations swing around Polaris during the night Pherkad Kochab Is Kochab orange compared 2 to Polaris? Pointers Is Dubhe Dubhe yellowish compared to Merak? 1 Merak THE PLOUGH Figure 1: Sketch of the northern sky in autumn. © Rob Peeling, CaDAS, 2007 version 1.2 Wynyard Planetarium & Observatory PUBLIC OBSERVING – Autumn North 1. On leaving the planetarium, turn around and look northwards over the roof of the building. Close to the horizon is a group of stars like the outline of a saucepan with the handle stretching to your left. This is the Plough (also called the Big Dipper) and is part of the constellation Ursa Major, the Great Bear. The two right-hand stars are called the Pointers. Can you tell that the higher of the two, Dubhe is slightly yellowish compared to the lower, Merak? Check with binoculars. Not all stars are white. The colour shows that Dubhe is cooler than Merak in the same way that red-hot is cooler than white- hot. 2. Use the Pointers to guide you upwards to the next bright star. This is Polaris, the Pole (or North) Star. Note that it is not the brightest star in the sky, a common misconception. Below and to the left are two prominent but fainter stars. These are Kochab and Pherkad, the Guardians of the Pole. Look carefully and you will notice that Kochab is slightly orange when compared to Polaris. -
Variable Star Section Circular No
The British Astronomical Association Variable Star Section Circular No. 176 June 2018 Office: Burlington House, Piccadilly, London W1J 0DU Contents Joint BAA-AAVSO meeting 3 From the Director 4 V392 Per (Nova Per 2018) - Gary Poyner & Robin Leadbeater 7 High-Cadence measurements of the symbiotic star V648 Car using a CMOS camera - Steve Fleming, Terry Moon and David Hoxley 9 Analysis of two semi-regular variables in Draco – Shaun Albrighton 13 V720 Cas and its close companions – David Boyd 16 Introduction to AstroImageJ photometry software – Richard Lee 20 Project Melvyn, May 2018 update – Alex Pratt 25 Eclipsing Binary news – Des Loughney 27 Summer Eclipsing Binaries – Christopher Lloyd 29 68u Herculis – David Conner 36 The BAAVSS Eclipsing Binary Programme lists – Christopher Lloyd 39 Section Publications 42 Contributing to the VSSC 42 Section Officers 43 Cover image V392 Per (Nova Per 2018) May 6.129UT iTelescope T11 120s. Martin Mobberley 2 Back to contents Joint BAA/AAVSO Meeting on Variable Stars Warwick University Saturday 7th & Sunday 8th July 2018 Following the last very successful joint meeting between the BAAVSS and the AAVSO at Cambridge in 2008, we are holding another joint meeting at Warwick University in the UK on 7-8 July 2018. This two-day meeting will include talks by Prof Giovanna Tinetti (University College London) Chemical composition of planets in our Galaxy Prof Boris Gaensicke (University of Warwick) Gaia: Transforming Stellar Astronomy Prof Tom Marsh (University of Warwick) AR Scorpii: a remarkable highly variable -
ALBERT VAN HELDEN + HUYGENS’S RING CASSINI’S DIVISION O & O SATURN’S CHILDREN
_ ALBERT VAN HELDEN + HUYGENS’S RING CASSINI’S DIVISION o & o SATURN’S CHILDREN )0g-_ DIBNER LIBRARY LECTURE , HUYGENS’S RING, CASSINI’S DIVISION & SATURN’S CHILDREN c !@ _+++++++++ l ++++++++++ _) _) _) _) _)HUYGENS’S RING, _)CASSINI’S DIVISION _) _)& _)SATURN’S CHILDREN _) _) _)DDDDD _) _) _)Albert van Helden _) _) _) , _) _) _)_ _) _) _) _) _) · _) _) _) ; {(((((((((QW(((((((((} , 20013–7012 Text Copyright ©2006 Albert van Helden. All rights reserved. A H is Professor Emeritus at Rice University and the Univer- HUYGENS’S RING, CASSINI’S DIVISION sity of Utrecht, Netherlands, where he resides and teaches on a regular basis. He received his B.S and M.S. from Stevens Institute of Technology, M.A. from the AND SATURN’S CHILDREN University of Michigan and Ph.D. from Imperial College, University of London. Van Helden is a renowned author who has published respected books and arti- cles about the history of science, including the translation of Galileo’s “Sidereus Nuncius” into English. He has numerous periodical contributions to his credit and has served on the editorial boards of Air and Space, 1990-present; Journal for the History of Astronomy, 1988-present; Isis, 1989–1994; and Tractrix, 1989–1995. During his tenure at Rice University (1970–2001), van Helden was instrumental in establishing the “Galileo Project,”a Web-based source of information on the life and work of Galileo Galilei and the science of his time. A native of the Netherlands, Professor van Helden returned to his homeland in 2001 to join the faculty of Utrecht University. -
JRASC August 2021 Lo-Res
The 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. -
Introduction to Astronomical Photometry, Second Edition
This page intentionally left blank Introduction to Astronomical Photometry, Second Edition Completely updated, this Second Edition gives a broad review of astronomical photometry to provide an understanding of astrophysics from a data-based perspective. It explains the underlying principles of the instruments used, and the applications and inferences derived from measurements. Each chapter has been fully revised to account for the latest developments, including the use of CCDs. Highly illustrated, this book provides an overview and historical background of the subject before reviewing the main themes within astronomical photometry. The central chapters focus on the practical design of the instruments and methodology used. The book concludes by discussing specialized topics in stellar astronomy, concentrating on the information that can be derived from the analysis of the light curves of variable stars and close binary systems. This new edition includes numerous bibliographic notes and a glossary of terms. It is ideal for graduate students, academic researchers and advanced amateurs interested in practical and observational astronomy. Edwin Budding is a research fellow at the Carter Observatory, New Zealand, and a visiting professor at the Çanakkale University, Turkey. Osman Demircan is Director of the Ulupınar Observatory of Çanakkale University, Turkey. Cambridge Observing Handbooks for Research Astronomers Today’s professional astronomers must be able to adapt to use telescopes and interpret data at all wavelengths. This series is designed to provide them with a collection of concise, self-contained handbooks, which covers the basic principles peculiar to observing in a particular spectral region, or to using a special technique or type of instrument. The books can be used as an introduction to the subject and as a handy reference for use at the telescope, or in the office. -
Back Matter (PDF)
[ 395 ] INDEX TO THE PHILOSOPHICAL TRANSACTIONS, S e r ie s A, V o l . 193. A. Abney (W. de W.). The Colour Sensations in Terms of Luminosity, 259. Atmospheric electricity—experiments in connection with precipitation (Wilson), 289. Bakebian Lectube. See Ewing and Kosenhain. C. Colour-blind, neutral points in spectra found by (Abney), 259. Colour sensations in terms of luminosity (Abney), 259. Condensation nuclei, positively and negatively charged ions as (W ilson), 289. Crystalline aggregates, plasticity in (Ewing and Rosenhain), 353. D. Dawson (H. M.). See Smithells, Dawson, and Wilson VOL. CXCIII.— Ao : S F 396 INDEX. Electric spark, constitution of (Schuster and Hemsalech), 189; potential—variation with pressure (Strutt), 377. Electrical conductivity of flames containing vaporised salts (Smithells, Dawson, and Wilson), 89. Electrocapillary phenomena, relation to potential differences between‘solutions (Smith), 47. Electrometer, capillary, theory of (Smith), 47. Ewing (J. A.) and Rosenhain (W.). The Crystalline Structure of Metals.—Bakerian Lecture, 353. F. Filon (L. N. G ). On the Resistance to Torsion of certain Forms of Shafting, with special Reference to the Effect of Keyways, 309. Flames, electrical conductivity of, and luminosity of salt vapours in (Smithells, Dawson, and Wilson), 89. G. Gravity balance, quartz thread (Threlfall and Pollock), 215. H. Hemsalech (Gustav). See Schuster and Hemsalech. Hertzian oscillator, vibrations in field of (Pearson and Lee), 159. Hysteresis in the relation of extension to stress exhibited by overstrained iron (Muir), 1. I. Ions, diffusion into gases, determination of coefficient (Townsend), 129. Ions positively and negatively charged, as condensation nuclei (Wilson), 289. Iron, recovery of, from overstrain (Muir), 1. -
The French Savants, and the Earth–Sun Distance: a R´Esum´E
MEETING VENUS C. Sterken, P. P. Aspaas (Eds.) The Journal of Astronomical Data 19, 1, 2013 The French Savants, and the Earth–Sun Distance: a R´esum´e Suzanne D´ebarbat SYRTE, Observatoire de Paris, Bureau des longitudes 61, avenue de l’Observatoire, 75014 Paris, France Abstract. Transits of Venus have played an important rˆole during more than two centuries in determining the Earth–Sun distance. In 2012, three centuries after Cassini’s death, the issue has been finally settled by the latest Resolution formulated by the International Astronomical Union. 1. Prologue From Antiquity up to the sixteenth century, values of the Earth–Sun distance were considered as being 10 to 20 times smaller than nowadays. Then came the Coper- nican revolution that brought new ideas about the solar system, followed by Jo- hannes Kepler (1571–1630) and Galileo Galilei (1564–1642) and, later in the seven- teenth century, Christiaan Huygens (1629–1695), Jean Picard (1620–1682), Gian- Domenico Cassini (1625–1712) and Isaac Newton (1643–1727) with his Principia. Powerful instruments were built, new pluridisciplinary groups formed, and novel con- cepts were presented. In France, Louis XIV created in 1666 the Acad´emie Royale des Sciences and the following year, 1667, the Observatoire Royal on the southern outskirts of the capital. Soon after, he demanded, from his academicians, a new geographical map of his kingdom. Picard presented ideas and new instruments to be built, and he performed a careful determination of the dimension of the Earth, along a meridian line represented by the symmetry axis of the observatory under construction. -
GEODETIC SURVEYS in the UNITED STATES the BEGINNING and the NEXT ONE HUNDRED YEARS 1807Ана1940 Joseph F. Drac
5/28/2017 Geodetic Surveys GEODETIC SURVEYS IN THE UNITED STATES THE BEGINNING AND THE NEXT ONE HUNDRED YEARS 1807 1940 Joseph F. Dracup Coast and Geodetic Survey (Retired) 12934 Desert Glen Drive Sun City West, AZ 853754825 ABSTRACT The United States began geodetic surveys later than most of the world's major countries, yet its achievements in this scientific area are immense and unequaled elsewhere. Most of the work was done by a single agency that began as the Survey of the Coast in 1807, identified as the Coast Survey in 1836,renamed the Coast and Geodetic Survey in 1878 and since about 1970 the National Geodetic Survey, presently an office in the National Ocean Service, NOAA. An introduction containing a brief history of geodetic surveying to 1800 is followed by accounts of the American experience to 1940. Broadly speaking the 18071940 period is divided into three sections: The Early Years 18071843, Laying the Foundations of the Networks 18431900 and Building the Networks 19001940. The scientific accomplishments, technology developments, major and other interesting events, anecdotes and the contributions made by the people of each period are summarized. PROLOGUE Early Geodetic Surveys And The BritishFrench Controversy The first geodetic survey of note was observed in France during the latter part of the 17th and early 18th centuries and immediately created a major controversy. Jean Picard began an arc of triangulation near Paris in 166970 and continued the work southward until his death about 1683. His work was resumed by the Cassini family in 1700 and completed to the Pyrenees on the Spanish border prior to 1718 when the northern extension to Dunkirk on the English Channel was undertaken. -
Storia Della Misurazione Del Grado Di Meridiano Terrestre Di Maristella Galeazzi
Storia della misurazione del grado di meridiano terrestre di Maristella Galeazzi Alcuni filosofi greci presocratici ritenevano che la Terra fosse piatta, ma questa non era certo l’opinione della maggioranza di essi, infatti già Aristotele (384-322 a.C.) sosteneva la sfericità della Terra e confermava la sua ipotesi mediante la circolarità dell’ombra della Terra sulla Luna osservabile durante le eclissi del nostro satellite e tramite il fatto che la configurazione del cielo mutava con la latitudine. Già Eratostene (275-195 a.C.) calcolò la prima misura del meridiano terrestre, ottenendo un valore di circa 44000 km. I geografi dell’antichità e del Medioevo non ottennero nuove misure significative, bisogna attendere la fine del XVII secolo per avere una nuova misura. Il problema della figura e della misura della Terra fu, insieme a quello della misurazione della longitudine, uno dei grandi problemi che preoccupò il mondo scientifico nel XVII e XVIII secolo e fu oggetto di una forte rivalità tra gli scienziati francesi e quelli inglesi. Tappe fondamentali della cartografia antica 580 a.C. Talete di Mileto immagina la terra piatta circondata dall’oceano. 570 a.C. Pitagora pensa che la Terra sia sferica in quanto la sfera è una forma “perfetta”. 335 a.C. Aristotele fornisce le prove della sfericità della Terra. 230 a.C. Eratostene ad Alessandria misura un arco di meridiano e calcola con una buona approssimazione, per quel tempo, il valore del raggio terrestre. 400 d.C. Sant’Agostino rifiuta la sfericità della Terra. IX – XI sec. Gli astronomi e i geografi arabi perfezionano gli strumenti di misura e sono dunque in grado di proseguire la tradizione greca.