Using Stellarium by Dustin Angell Stellarium Stellarium Is a Computer Program That Can Help Make Astronomy and Stargazing Fun and Accessible
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THUBAN the Star Thuban in the Constellation Draco (The Dragon) Was the North Pole Star Some 5,000 Years Ago, When the Egyptians Were Building the Pyramids
STAR OF THE WEEK: THUBAN The star Thuban in the constellation Draco (the Dragon) was the North Pole Star some 5,000 years ago, when the Egyptians were building the pyramids. Thuban is not a particularly bright star. At magnitude 3.7 and known as alpha draconis it is not even the brightest star in its constellation. What is Thuban’s connection with the pyramids of Egypt? Among the many mysteries surrounding Egypt’s pyramids are the so-called “air shafts” in the Great Pyramid of Giza. These narrow passageways were once thought to serve for ventilation as the The Great Pyramid of Giza, an enduring monument of ancient pyramids were being built. In the 1960s, though, Egypt. Egyptologists believe that it was built as a tomb for fourth dynasty Egyptian Pharaoh Khufu around 2560 BC the air shafts were recognized as being aligned with stars or areas of sky as the sky appeared for the pyramids’ builders 5,000 years ago. To this day, the purpose of all these passageways inside the Great Pyramid isn’t clear, although some might have been connected to rituals associated with the king’s ascension to the heavens. Whatever their purpose, the Great Pyramid of Giza reveals that its builders knew the starry skies intimately. They surely knew Thuban was their Pole Star, the point around which the heavens appeared to turn. Various sources claim that Thuban almost exactly pinpointed the position of the north celestial pole in the This diagram shows the so-called air shafts in the Great year 2787 B.C. -
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. -
Dhruva the Ancient Indian Pole Star: Fixity, Rotation and Movement
Indian Journal of History of Science, 46.1 (2011) 23-39 DHRUVA THE ANCIENT INDIAN POLE STAR: FIXITY, ROTATION AND MOVEMENT R N IYENGAR* (Received 1 February 2010; revised 24 January 2011) Ancient historical layers of Hindu astronomy are explored in this paper with the help of the Purân.as and the Vedic texts. It is found that Dhruva as described in the Brahmân.d.a and the Vis.n.u purân.a was a star located at the tail of a celestial animal figure known as the Úiúumâra or the Dolphin. This constellation, which can be easily recognized as the modern Draco, is described vividly and accurately in the ancient texts. The body parts of the animal figure are made of fourteen stars, the last four of which including Dhruva on the tail are said to never set. The Taittirîya Âran.yaka text of the Kr.s.n.a-yajurveda school which is more ancient than the above Purân.as describes this constellation by the same name and lists fourteen stars the last among them being named Abhaya, equated with Dhruva, at the tail end of the figure. The accented Vedic text Ekâgni-kân.d.a of the same school recommends observation of Dhruva the fixed Pole Star during marriages. The above Vedic texts are more ancient than the Gr.hya-sûtra literature which was the basis for indologists to deny the existence of a fixed North Star during the Vedic period. However the various Purân.ic and Vedic textual evidence studied here for the first time, leads to the conclusion that in India for the Yajurvedic people Thuban (α-Draconis) was Dhruva the Pole Star c 2800 BC. -
PDF (Pbcameron Thesis.Pdf)
The Formation and Evolution of Neutron Stars: Astrometry, Timing, and Transients Thesis by P. Brian Cameron In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy California Institute of Technology Pasadena, California 2009 (Defended June 2, 2008) ii c 2009 P. Brian Cameron All Rights Reserved iii Acknowledgements I have been incredibly fortunate these last five years to work with and have the support of so many amazing people. Foremost, I would like to acknowledge my enormous debt to my advisor, Shri Kulkarni. His vision and tireless dedication to astronomy were inspiring, and led to the topics in this thesis being at the forefront of astrophysics. Our styles contrasted, but his energy, open advice, and support made for a very rewarding collaboration. In this same vein, I am grateful to Matthew Britton whose ideas and open door made the last 2 years incredibly enjoyable. I have also had the privilege of working with a number talented people on a wide variety of topics. I am grateful to Bryan Jacoby, David Kaplan, Bob Rutledge, and Dale Frail for their insights and patience. I would also like to thank the NGAO crowd that got me thinking hard about astrometry: Rich Dekany, Claire Max, Jessica Lu, and Andrea Ghez. No observer could ever function with out people working tirelessly at the telescope and when you return from it. I am grateful for the patience and dedication of the Keck astronomers, especially Al Conrad, Randy Campbell and Jim Lyke, as well as those at Palomar: Jean Mueller, and Karl Dunscombe. I am indebted to the excellent staff here at Caltech for putting up with my endless questions and requests: Patrick Shopbell, Anu Mahabal, and Cheryl Southard. -
Star Clusters Or Asterisms? 2MASS CMD and Structural Analyses of 15 Challenging Targets
A&A 530, A32 (2011) Astronomy DOI: 10.1051/0004-6361/201116452 & c ESO 2011 Astrophysics Star clusters or asterisms? 2MASS CMD and structural analyses of 15 challenging targets E. Bica and C. Bonatto Universidade Federal do Rio Grande do Sul, Departamento de Astronomia, CP 15051, RS, Porto Alegre 91501-970, Brazil e-mail: [charles;bica]@if.ufrgs.br Received 7 January 2011 / Accepted 29 March 2011 ABSTRACT Context. Poorly-populated star clusters may have photometric and structural properties not much different from asterisms, to the point that, in some cases, widely-used databases present conflicting classifications. Aims. We investigate the nature of a sample of challenging targets that have been classified either as star clusters or asterisms in different studies. A few objects are studied for the first time. Methods. The analysis employs 2MASS photometry, field-star decontamination, to enhance the intrinsic colour–magnitude diagram (CMD) morphology, and colour-magnitude filters, for high contrast stellar radial density profiles (RDPs). Results. Based on properties derived from field-star decontaminated CMDs, and structural parameters from RDPs, we find that Pismis 12, IC 1434, Juchert 10, Ruprecht 30, NGC 3519, Herschel 1, Mayer 1, and Muzzio 1 are open clusters with ages within 5Myr−1.3 Gyr. Ruprecht 129, 130, 140, and 146 are borderline cases, being rather poorly-populated, with evolutionary sequences and RDPs suggesting star clusters. Dolidze 39, BH 79, and Ruprecht 103, have CMDs and RDPs typical of asterisms. Conclusions. When a low stellar population is associated with a dense field contamination and/or important differential reddening, only a thin line separates star clusters and asterisms. -
STUDENT PAGE CONSTELLATION/STAR Big Dipper/Polaris CROW the Seven Bulls BLACKFEET Fixed Star GREEK Ursa Minor JAPANESE the One S
STUDENT PAGE Astronomy Lesson 1: One Sky, Many Stories CONSTELLATION/STAR JAPANESE GREEK BLACKFEET CROW Big Dipper/Polaris The One Star Ursa Fixed The Seven & Big Dipper Minor Star Bulls 48 constellations in his famous book “Almagest”. These CONSTELLATIONS are called the “Ptolemaic constellations,” and most of them survive to this day. The history of the constellations is ancient; many were likely created by the Babylonian, Egyptian and Assyrian There are 88 official constellations recognized by the peoples. These constellations would have moved through International Astronomical Union. Only the official the regions via trade, and eventually they made their way boundaries of these constellations are determined; there into Greece, where they were assimilated into the culture is no official line drawing that makes up the shape of any and mythology. In the second century, Ptolemy organized constellation. Image courtesy wikihow ONE SKY, MANY STORIES 46 | ASTRONOMY STUDENT PAGE Astronomy Lesson 1: One Sky, Many Stories Image courtesy Wikipedia Star chart, Kitora Tomb, Asuka, Japan (7th century) In 1998, a star map was discovered in the Kitora Tomb Cultures all over the world have created star stories in the Asuka village in Japan. Dating back to the late based on constellations to pass traditions and knowledge seventh, early eighth century, this star chart is the oldest on to the next generation. Each culture had different existing map of its kind in the world. It features 68 names and stories for the Sun and Moon, visible planets, constellations and the movement of celestial objects is stars, and star groups. These stories are told at night and represented by the three concentric circles in the chart. -
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. -
Skywatchers of Africa and Follow The
A Teacher Resource Guide for For Grades 3 to 8 Children’s Museum of Virginia Lesson Overview The education resource was developed using the 5E model of learning and involves pre-visit activities to ENGAGE student interest, planetarium presentations using simulation software along with hands on activities to EXPLORE and EXPAIN about the nature of constellations and related the constellations to the lore from African societies, an EXTEND/ELABORATE section where they further develop the concepts of their visit as well as the EVALUATE section to allow a check of student mastery. The delivery of the EXPLORE and EXPLAIN sections can be tailored to your particular needs and may include one of two possible planetarium shows as well as a mini lesson on selected constellations. Standards of Learning Virginia Standards History 3.1, 3.4, 8.3, 8.4 Science Various point 1 bullets for grades 3 - 6 National Standards Geography How to use maps and other geographic representations, tools and technologies to acquire, process and report information. How to use mental maps to organize information about people, place and environments. Science As a result of their activities in grades k – 4, all students should develop an understanding of: o Objects in the sky o Changes in Earth and sky Essential Questions What are constellations and what methods are best to observe them? How do the constellations you can see vary from one spot to another on Earth? How do the accepted constellations of today differ from those created by early African civilizations? Instructional Objectives Students will observe the planetarium sky using familiar patters to navigate other constellations; view the southern skies above Africa to illustrate how the groups of constellations varies with latitude; learn about several of the dominant cultures of native Africa and about the names for the constellations; and recognize that the constellations which they invent can be just as useful as the ancient Greek, Roman or African constellations. -
Polaris — Vega — Centauri
PLEASE READ CAREFULLY AND KEEP THIS MANUAL FOR FUTURE REFERENCE Instruction Manual Product # 10-000 POLARIS — VEGA — CENTAURI Certified and tested according to CAN/ULC S627-00 UL 1482-2011 2020 U.S. Environmental Protection Agency's crib wood emission standard 490, rue de l'Argon Québec, CANADA G2N 2C9 Tél.: 418-849-8095 Fax : 418-849-0077 www.jaroby.com August 15 2017 Printed in Canada TABLE OF CONTENTS INTRODUCTION ...................................................................... 3 EXTERNAL COMBUSTION AIR SOURCE ............................ 22 LISTING AND CODE APPROVALS ......................................... 3 Exterior Air Intake pipe ....................................................... 22 Appliance certification .......................................................... 3 Installation of Air Intake Pipe ......................................... 22 Mobile home approved......................................................... 3 Air Inlet Obstruction ....................................................... 22 BTU & Efficiency Specifications ........................................... 3 STAINLESS STEEL TUBES REPLACEMENT ...................... 23 WARNING ................................................................................ 3 Stainless steel tubes Installation ........................................ 23 RATING PLATE ....................................................................... 4 How to install tubes ....................................................... 23 APPLIANCE DIMENSION ....................................................... -
(NASA/Chandra X-Ray Image) Type Ia Supernova Remnant – Thermonuclear Explosion of a White Dwarf
Stellar Evolution Card Set Description and Links 1. Tycho’s SNR (NASA/Chandra X-ray image) Type Ia supernova remnant – thermonuclear explosion of a white dwarf http://chandra.harvard.edu/photo/2011/tycho2/ 2. Protostar formation (NASA/JPL/Caltech/Spitzer/R. Hurt illustration) A young star/protostar forming within a cloud of gas and dust http://www.spitzer.caltech.edu/images/1852-ssc2007-14d-Planet-Forming-Disk- Around-a-Baby-Star 3. The Crab Nebula (NASA/Chandra X-ray/Hubble optical/Spitzer IR composite image) A type II supernova remnant with a millisecond pulsar stellar core http://chandra.harvard.edu/photo/2009/crab/ 4. Cygnus X-1 (NASA/Chandra/M Weiss illustration) A stellar mass black hole in an X-ray binary system with a main sequence companion star http://chandra.harvard.edu/photo/2011/cygx1/ 5. White dwarf with red giant companion star (ESO/M. Kornmesser illustration/video) A white dwarf accreting material from a red giant companion could result in a Type Ia supernova http://www.eso.org/public/videos/eso0943b/ 6. Eight Burst Nebula (NASA/Hubble optical image) A planetary nebula with a white dwarf and companion star binary system in its center http://apod.nasa.gov/apod/ap150607.html 7. The Carina Nebula star-formation complex (NASA/Hubble optical image) A massive and active star formation region with newly forming protostars and stars http://www.spacetelescope.org/images/heic0707b/ 8. NGC 6826 (Chandra X-ray/Hubble optical composite image) A planetary nebula with a white dwarf stellar core in its center http://chandra.harvard.edu/photo/2012/pne/ 9. -
Asterism: Volume 2
ASTERISM: VOLUME 2 2018 Asterism: An Undergraduate Literary Journal Staff is published anually by The Ohio State Uni- versity at Lima. Senior Editors *** All poems and stories in the magazine are Jenna Bush works of imagination. Ashley Meihls Address all correspondence to: Galvin Hall 401A Editors 4240 Campus Dr. *** Lima, OH 45804 Katie Marshall Victoria Sullivan Visit our website: Mattea Rolsten lima.osu.edu/asterism Andrea Morales Jacob Short Published 2018 Cover Art: Faculty Advisors “Raindrops” by Jessy Gilcher *** Beth Sutton-Ramspeck Doug Sutton-Ramspeck Asterism - I Table of Contents A Note to Our Readers V -273.15 °C ............................................................. Emma DePanise Poetry 8 Holy Man ............................................................. Deon Robinson Poetry 9 Starry Eyes ................................................... Hannah Schotborgh Poetry 10 Untitled ....................................................................... Riley Klaus Art 12 Bones ..................................................................... Angela Kramer Poetry 13 Blinker ....................................................................... Bryan Miller Fiction 15 Still Water ............................................................ Trevor Bashaw Poetry 19 Hearsay .................................................................... Noah Corbett Poetry 21 Para Mi Alma ........................................................... Asalia Arauz Poetry 26 Amaryllis ................................................................ -
The Relative Sizes of the Sun and Stars 25
The relative sizes of the sun and stars 25 Stars come in many sizes, but their true appearances are impossible to see without special telescopes. The image to the left was taken by the Hubble Space telescope and resolves the red supergiant star Betelgeuse so that its surface can be just barely seen. Follow the number clues below to compare the sizes of some other familiar stars! Problem 1 - The sun's diameter if 10 times the diameter of Jupiter. If Jupiter is 11 times larger than Earth, how much larger than Earth is the Sun? Problem 2 - Capella is three times larger than Regulus, and Regulus is twice as large as Sirius. How much larger is Capella than Sirius? Problem 3 - Vega is 3/2 the size of Sirius, and Sirius is 1/12 the size of Polaris. How much larger is Polaris than Vega? Problem 4 - Nunki is 1/10 the size of Rigel, and Rigel is 1/5 the size of Deneb. How large is Nunki compared to Deneb? Problem 5 - Deneb is 1/8 the size of VY Canis Majoris, and VY Canis Majoris is 504 times the size of Regulus. How large is Deneb compared to Regulus? Problem 6 - Aldebaran is 3 times the size of Capella, and Capella is twice the size of Polaris. How large is Aldebaran compared to Polaris? Problem 7 - Antares is half the size of Mu Cephi. If Mu Cephi is 28 times as large as Rigel, and Rigel is 50 times as large as Alpha Centauri, how large is Antares compared to Alpha Centauri? Problem 8 - The Sun is 1/4 the diameter of Regulus.