The 28-Xiu Constellations in East Asian Calendars and Analysis of Their Observation Dates
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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. -
Poison King: the Life and Legend of Mithradates the Great, Rome's
Copyrighted Material Kill em All, and Let the Gods Sort em Out IN SPRING of 88 BC, in dozens of cities across Anatolia (Asia Minor, modern Turkey), sworn enemies of Rome joined a secret plot. On an appointed day in one month’s time, they vowed to kill every Roman man, woman, and child in their territories. e conspiracy was masterminded by King Mithradates the Great, who communicated secretly with numerous local leaders in Rome’s new Province of Asia. (“Asia” at this time referred to lands from the eastern Aegean to India; Rome’s Province of Asia encompassed western Turkey.) How Mithradates kept the plot secret remains one of the great intelli- gence mysteries of antiquity. e conspirators promised to round up and slay all the Romans and Italians living in their towns, including women and children and slaves of Italian descent. ey agreed to confiscate the Romans’ property and throw the bodies out to the dogs and crows. Any- one who tried to warn or protect Romans or bury their bodies was to be harshly punished. Slaves who spoke languages other than Latin would be spared, and those who joined in the killing of their masters would be rewarded. People who murdered Roman moneylenders would have their debts canceled. Bounties were offered to informers and killers of Romans in hiding.1 e deadly plot worked perfectly. According to several ancient histo- rians, at least 80,000—perhaps as many as 150,000—Roman and Italian residents of Anatolia and Aegean islands were massacred on that day. e figures are shocking—perhaps exaggerated—but not unrealistic. -
Constraining the Masses of Microlensing Black Holes and the Mass Gap with Gaia DR2 Łukasz Wyrzykowski1 and Ilya Mandel2,3,4
A&A 636, A20 (2020) Astronomy https://doi.org/10.1051/0004-6361/201935842 & c ESO 2020 Astrophysics Constraining the masses of microlensing black holes and the mass gap with Gaia DR2 Łukasz Wyrzykowski1 and Ilya Mandel2,3,4 1 Warsaw University Astronomical Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland e-mail: [email protected] 2 Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University, Clayton, Victoria 3800, Australia 3 OzGrav: The ARC Center of Excellence for Gravitational Wave Discovery, Australia 4 Institute of Gravitational Wave Astronomy and School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK Received 6 May 2019 / Accepted 27 January 2020 ABSTRACT Context. Gravitational microlensing is sensitive to compact-object lenses in the Milky Way, including white dwarfs, neutron stars, or black holes, and could potentially probe a wide range of stellar-remnant masses. However, the mass of the lens can be determined only in very limited cases, due to missing information on both source and lens distances and their proper motions. Aims. Our aim is to improve the mass estimates in the annual parallax microlensing events found in the eight years of OGLE-III observations towards the Galactic Bulge with the use of Gaia Data Release 2 (DR2). Methods. We use Gaia DR2 data on distances and proper motions of non-blended sources and recompute the masses of lenses in parallax events. We also identify new events in that sample which are likely to have dark lenses; the total number of such events is now 18. Results. -
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. -
The Late Republic in 5 Timelines (Teacher Guide and Notes)
1 180 BC: lex Villia Annalis – a law regulating the minimum ages at which a individual could how political office at each stage of the cursus honorum (career path). This was a step to regularising a political career and enforcing limits. 146 BC: The fall of Carthage in North Africa and Corinth in Greece effectively brought an end to Rome’s large overseas campaigns for control of the Mediterranean. This is the point that the historian Sallust sees as the beginning of the decline of the Republic, as Rome had no rivals to compete with and so turn inwards, corrupted by greed. 139 BC: lex Gabinia tabelleria– the first of several laws introduced by tribunes to ensure secret ballots for for voting within the assembliess (this one applied to elections of magistrates). 133 BC – the tribunate of Tiberius Gracchus, who along with his younger brother, is seen as either a social reformer or a demagogue. He introduced an agrarian land that aimed to distribute Roman public land to the poorer elements within Roman society (although this act quite likely increased tensions between the Italian allies and Rome, because it was land on which the Italians lived that was be redistributed). He was killed in 132 BC by a band of senators led by the pontifex maximus (chief priest), because they saw have as a political threat, who was allegedly aiming at kingship. 2 123-121 BC – the younger brother of Tiberius Gracchus, Gaius Gracchus was tribune in 123 and 122 BC, passing a number of laws, which apparent to have aimed to address a number of socio-economic issues and inequalities. -
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. -
(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. -
New Wide Common Proper Motion Binaries
Vol. 6 No. 1 January 1, 2010 Journal of Double Star Observations Page 30 New Wide Common Proper Motion Binaries Rafael Benavides1,2, Francisco Rica2,3, Esteban Reina4, Julio Castellanos5, Ramón Naves6, Luis Lahuerta7, Salvador Lahuerta7 1. Astronomical Society of Córdoba, Observatory of Posadas, MPC-IAU Code J53, C/.Gaitán nº 20, 1º, 14730 Posadas (Spain) 2. Double Star Section of Liga Iberoamericana de Astronomía (LIADA), Avda. Almirante Guillermo Brown No. 4998, 3000 Santa Fe (Argentina) 3. Astronomical Society of Mérida, C/José Ruíz Azorín, 14, 4º D, 06800 Mérida (Spain) 4. Plza. Mare de Dèu de Montserrat, 1 Etlo 2ªB, 08901 L'Hospitalet de Llobregat (Spain) 5. 0bservatory with MPC-IAU Code 939, Av. Primado Reig 183, 46020 Valencia (Spain) 6. Observatory of Montcabrer, MPC-IAU Code 213, C/Jaume Balmes, 24, 08348 Cabrils (Spain) 7. G.E.O.D.A., Observatorio Manises, MPC-IAU Code J98, C/ Mayor, 111-4, 46940 Manises (Spain) Abstract: In this work we report the discovery of 150 new double stars of which 142 are wide common proper motion stellar systems. In addition to this, we report the study of 23 recently catalogued wide common proper motion binaries discovered by other observers. Spectral types, photometric distances, kinematics and ages were determined from data ob- tained consulting the literature. Several criteria were used to determine the nature of each double star. Orbital periods and the semimajor axes were calculated. they are good sensors to detect unknown mass concen- 1. Introduction trations that they may encounter along their galactic For several years double-star amateurs have con- trajectories. -
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 ................................................................ -
Lecture 8: Stellar Motions Reading: Box 19-1
Lecture 8: Stellar Motions Reading: Box 19-1 Key Ideas The stars are in constant motion. Observed Motions Proper motions (motion against the background, measured in angular motion/time) Radial velocities (motion towards or away, measured from the Doppler shift) True Space Motion Combination of radial velocity, proper motion, and distance (important for proper motion!) The “Fixed” Stars Although the stars are moving, their motions across the sky are so small that to the naked eye, the stars appear “fixed” to the sky. Great distances make the amount of motion small on human lifetimes. (Of course, stars moving directly away or towards us will not to appear to move across the sky) Proper Motions Apparent angular motion across the sky of nearby stars with respect to distant objects. (Distant stars are used because we assume that even though they are moving through space they are so far away that from our perspective they are fixed). It is the projection of the star’s true motion through space relative to the Sun. Typical proper motion for stars in the solar neighborhood is about 0.1 arcsec/year Largest proper motion measured is 10.25 arcsec/year Barnard’s Star) Proper motions are cumulative. Effects build up over time. The longer you wait, the greater apparent angular motion is. Measuring proper motions: Compare photos of the sky taken 20 to 50 years apart Measure how much stars have moved compared to more distant background objects (galaxies, quasars). Example: if a star has a proper motion of 0.1 arcsec/year: In one year, it moves 0.1 arcsec In 10 years, it moves 10x0.1= 1 arcsec In 100 years, it moves 100x0.1 =10 arcsec It can take a long time for the constellations to noticeably change shape.