Proquest Dissertations

Total Page:16

File Type:pdf, Size:1020Kb

Proquest Dissertations The sun, moon and stars of the southern Levant at Gezer and Megiddo: Cultural astronomy in Chalcolithic/Early and Middle Bronze Ages Item Type text; Dissertation-Reproduction (electronic) Authors Gardner, Sara Lee Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 25/09/2021 23:39:58 Link to Item http://hdl.handle.net/10150/280233 INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the text directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter face, while others may be from any type of computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand comer and continuing from left to right in equal sections with small overiaps. ProQuest Information and Leaming 300 North Zeeb Road. Ann Arbor, Ml 48106-1346 USA 800-521-0600 THE SL'N. MOON AND STARS OF THE SOUTHERN LEVANT AT GEZER AND MEGIDDO: CULTURAL ASTRONOMY IN CHALCOLITHIC/EARLY AND MIDDLE BRONZE AGES by Sara Lee Gardner A Dissertation Submitted to the Faculty of the DEPARTMENT OF NEAR EASTERN STUDIES In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 2002 UMI Number; 3073283 (g) UMI UMI Microform 3073283 Copyright 2003 by ProQuest Information and Learning Company. All rights reserved. This microform edition is protected against unauthorized copying under Title 17, United States Code. ProQuest Infomnation and Leaming Company 300 North Zeeb Road P.O. Box 1346 Ann Art)or, Ml 48106-1346 2 THE UNIVERSITY OF ARIZONA ® GRADUATE COLLEGE As members of the Final Examination Committee, ve certify that we have read the dissertation prepared by Sara Lee Gardner entitled THE SUN. MOON AND STARS OF THE SOUTHERN LEVANT ST PFZFR AMD MEGIDDO: CULTURAL ASTRONOMY IN CHALCOLITHIC/EARLY AND MIDDLE BRONZE AGES and recommend chat it be accepted as fulfilling the dissertation requirement for the Degree of Doctor of Philosophy 4/10/200^ Date //- 4/13/2002 J. Edward l-/ria Date 4/12/2002 H. >ii.]kinson Date 4/12/2002 r^ond E. White Date IL '^-co2, Date Final approval and acceptance of this dissertation is contingent upon the candidate's submission of the final copy of the dissertation to the Graduate College. I hereby certify that I have read this dissertation prepared under ny direction and recommend that it be accepted as fulfilling the dissertation requirement. Dissertation Director Date STATEMENT BY AUTHOR This dissertation has been submitted in panial fulfillment of requirements for an ad\ anced degree at the University of Arizona and is deposited in the University Librar\' to be made available to borrowers under the rules of the Librar>'. Brief quotations from this dissertation are allowable without special permission, provided that accurate acknowledgement of the source is made. Requests fro permission for extended quotation fi-om or reproduction of this manuscript in w hole or part may be granted by the head of the major depanment or the Dean of the College when in his or her judgment the proposed use of the material is in the interest of scholarship. In all other instances, however, permission must be obtained from the author. SIGN"ED^>^/^ Vy ^ 4 ACKNOWLEDGEMENTS The list of people who have innuenced m\ journey to the completion of the dissertation and believed in my ability to make a contribution to the "greater body of knowledge" is overly long—as it should be. LMtimately. the most important person is William G. Dever (Near Eastern Studies), who was willing to support the slightly less than mainstream subject I chose. His support, without which this dissertation would not have been written, has made the journey worthwhile. J. Edward Wright's (Near Eastern Studies) constant challenge that I could do more than I thought, pushed me forward in the textual materials, for w hich I am forever grateful. I thank Raymond E. White (Astronomy), who had the challenge of leaching and guiding me in the rudiments of astronomy, and then helped me to translate those rudiments into viable scholarly descriptions with practical applications. I also want to express my appreciation to Richard H. Wilkinson (Egyptology), who came to my committee at the last minute. His input and support were invaluable. In Israel I thank the W. F. .Albright Institution staff and visiting .scholars for their support and encouragement during my short stay. Particularly. I thank J. Rosenberg for his sur\eying expertise and his willingness to drive to the Negev and Gezer—more than once. His photos are included in this dissertation, and his measurements are the foundation for the exposition on Gezer. Claire R. Farrer introduced me to the field of archao/ethnoastronomy. and when I faltered, gave me the courage to persevere. One group from which I received a copious amount of support, advice, and knowledge was the participants from the International Oxford Conference on Archaeoastronomy and Ethnoastronomy. Edwin C. Krupp (Griffith Observatiory) and Steven McCluskey (University of West Virgina) have provided me w ith articles, advice, and opinions on request. I want to thank Bradley E. Shaeffer (University of Texas. Austin) who helped me sort out astronomy, and Anthony F. Aveni (Colgate University) for taking their valuable time lo read my work and to send me comments. The members of the History of •Astronomy list (HASTRO-L) have al.so been extremely valuable to my research by answering questions and providing references; particularly. Gary D. Thompson, an engineer who has compiled an extensive bibliography on ancient western astronomy that he made readily available. Hermann Hunger (University of Vienna) who responded to an unknown student around the world and answered my questions on Mesopotamian astronomy via e-mail, also receives my appreciation for his time, patience, and support. Finally, I thank my children. J. Steven Gardner. H. Christine Lindblom. Leslie J. Christ, and J. Eric Lindblom, who have supported me from the inception to the completion of this journey. They have walked every step of the way with me, listened, encouraged, and believed. Without their love and belief that I could accomplish my goal, my journey would have more arduous and less satisfying. Dedicaled to my children, who are my best friends J. Steven Gardner H. Christine Lindblom Leslie J. Christ J. Eric Lindblom "And there are those who have little and give it all. These arc the believers in life and the bounty of life, and their coffer is never empty. There are those who give with joy. and that joy is their reward." The Prophet by Khalil Gibran 1923 6 TABLE OF CONTENTS LIST OF FIGURES II LIST OF TABLES 14 ABSTRACT 15 CHAPTER 1: INTRODUCTION 16 STATEMENT OF PURPOSE AND THESIS ORGANIZATION 17 CHAPTER 2: ARCHAEOASTRONOMICAL CONCEPTS 21 The Birth of Paradigm: Modem Methodological Origins 21 •"Green" and "Brown" Archaeoastronomy = Cultural Astronomy 22 Archaeo/Ethnoastronomy Now 32 Great Britain and Europe 34 Mesoamerica 34 Southwest United States 35 Egypt 36 Israel 38 CULTURAL ASTRONOMY 39 Observation. Perception, and Use 39 What is observ ed? What are the instruments of observation? 40 What are the perceptions"! 45 Lunar, solar, and lunisolar calendars in the ancient Near East 46 What is the use of the ohservaiions and perceptions'! 48 7 TABLE OF CONTENTS—continued... SUMMATION 49 ENDNOTES 52 C HAPTER 3; CONTACTS WITH EGYPT AND SYRIA 54 Introduciion 54 Late Chalcolithic/Eariy Bronze Age transition (3400-2900 BCE) and Egypt 54 Early Bronze Age I (EB I: 3300-3100 BCE) and Egypt 55 Early Bronze Age II (3100-2650 BCE) and Egypt 57 Late Chalcolithic/Eariy Bronze Age I (3400-2900 BCE) and Syria 58 ASTRONOMY AND THE LEVANT 59 Religion and Astral Images: Wall Paintings and Artifacts 60 Astral Images: Standing Stones. Sacred Poles, and Stars 64 STANDING STONES IN THE SOUTHERN LEVANT 67 RUJIM EL-HIRI: A CASE STUDY FROM EARLY AND MIDDLE BRONZE AGES 68 The site 68 Astronomical alignments 71 TEMPLE ORIENTATION 75 SUMMATION: PICKING THE TEST SITES 78 ENDNOTES 81 8 TABLE OF CONTENTS—(w/rmz/f J... C HAPTER 4: GEZER 83 Location and Excavation 83 Occupation History 85 THE ST.ANDLN'G STONES OF GEZER 87 The Stones of Gezer 87 Standing stones, public areas and astronomy at Gezer 89 Applying geocentric astronomy to the Standing Stones of Gezer 92 The Stones and Horizon in the draw ings of Cave 30/IV 98 SUMMATION 101 ENDNOTES 103 CHAPTER 5: MEGIDDO 104 Location and Excavation 104 Area BB; The Chalcolithic and Early Bronze cult areas and pavement 106 Occupation and specialization in the Chalcolithic period and the Early Bronze Age 108 ASTRONOMY AND CHALCOLITHIC RELIGION II1 Occurrence and Interpretation of the Lion in Near Eastern Iconography 111 Shoulder ornaments on animals 117 The Lion in the Sky 118 COMETS AND CULTURE RESPONSE 120 9 TABLE OF CONTENTS—cominuecl... How did conicts look to ancient observers? 125 ML L.APIN AND THE CONSTELLATION LEO 127 SUMMATION 133 ENDNOTES 137 CHAPTER 6; SUMMATION.
Recommended publications
  • Requirements of Timely Performance in Time and Voyage Charterparties
    Graduate School REQUIREMENTS OF TIMELY PERFORMANCE IN TIME AND VOYAGE CHARTERPARTIES - AN EXPLORATION OF THEIR IDENTITY, SCOPE AND LIMITATIONS UNDER ENGLISH LAW Thesis submitted for the degree of Doctor of Philosophy at the University of Leicester by Tamaraudoubra Tom Egbe School of Law University of Leicester 2019 Abstract REQUIREMENTS OF TIMELY PERFORMANCE IN TIME AND VOYAGE CHARTERPARTIES - AN EXPLORATION OF THEIR IDENTITY, SCOPE AND LIMITATIONS UNDER ENGLISH LAW By Tamaraudoubra Tom Egbe The importance of time in the performance of contractual obligations under sea carriage of goods arrangements are until now little explored. For the avoidance of breach, certain obligations and responsibilities of the parties to the contract need to be performed promptly. Ocean transport is an expensive venture and a shipowner could suffer considerable financial losses if an unnecessary but serious delay interrupt the vessel’s earning power in the course of the charterer’s performance of his contractual obligation. On the other hand, a charterer could also incur a substantial loss if arrangements for the shipment and receipt of cargo fail to go according to plan as a result of the shipowner’s failure to perform his charterparty obligation timely and with reasonable diligence. With these considerations in mind, this thesis critically explores the concept of timely performance in the discharge of the contractual obligations of parties to a contract of carriage. While the thesis is not an expository of the occurrence of time in all the obligations of parties to the carriage contract, it focusses particularly on the identity, scope, and limitations of timeliness in the context of timely payment of hire, laytime and reasonable despatch.
    [Show full text]
  • The Practice of Thresholds
    Chapter 1 The Practice of Thresholds Thresholds were important to the ancient Irish monks whose wis- dom guides us on this path. Thresholds are the space between, when we move from one time to another, as in the threshold of dawn to day or of dusk to dark; one space to another, as in times of inner or outer journeying or pilgrimage; and one awareness to another, as in times when our old structures start to fall away and we begin to build something new. The Celts describe thresholds as “thin times or places” where heaven and earth are closer together and the veil between worlds is thin. In the Celtic imagination, thresholds are potent places. We expe- rience the thresholds of the year unfolding, so that each new season beckons us into a renewed awareness of the nearness of the holy presence. In the Celtic wheel of the year there are eight portals in time that mark the equinoxes and solstices, as well as the midway points between them. Each of these festivals held the possibility of deeper connection to the divine. We will explore this further in chap- ter 10. We encounter thresholds each day through the movement across the hinges of time. The turning of early morning and evening were thought to be especially graced times of day when the otherworld was near. There are physical places that evoke a sense of wonder. My hus- band, John, wonders if “thin places” means they were worn thin by the many souls who have been drawn to these liminal landscapes 1 THE SOUL’S SLOW RIPENING and sought prayer there.
    [Show full text]
  • COMMISSION C4 WORLD HERITAGE and ASTRONOMY 1. Background
    Transactions IAU, Volume XXXA Reports on Astronomy 2015-2018 c 2018 International Astronomical Union Piero Benvenuti, ed. DOI: 00.0000/X000000000000000X COMMISSION C4 WORLD HERITAGE AND ASTRONOMY PATRIMOINE MONDIAL ET ASTRONOMIE PRESIDENT Clive Ruggles VICE-PRESIDENT Gudrun Wolfschmidt PAST PRESIDENT N/A ORGANIZING COMMITTEE Roger Ferlet, Siramas Komonjinda, Mikhail Marov, Malcolm Smith COMMISSION C4 WORKING GROUPS Div. C / Commission C4 WG1 Windows to the Universe: High-Mountain Observatories and other Astronomical Sites of the late 20th and early 21st Centuries (Joint with Commission B7) Div. C / Commission C4 WG2 Classical Observatories from the Renaissance to the 20th Century Div. C / Commission C4 WG3 Heritage of Space Exploration Div. C / Commission C4 WG4 Astronomical Heritage in Danger Div. C / Commission C4 WG5 Intangible Heritage (Joint with Commission C1) Div. C / Commission C4 WGAAC Archaeoastronomy and Astronomy in Culture (Joint with Commission C3) TRIENNIAL REPORT 2015-2018 1. Background UNESCO's Astronomy and World Heritage Initiative (AWHI) (whc.unesco.org/en/ astronomy) has existed since 2004 to identify, promote and protect heritage, and potential World Heritage, connected with astronomy. A Memorandum of Understanding (MoU) between UNESCO and the IAU, under which the IAU undertook to implement the AWHI jointly with UNESCO, was signed in 2008 ahead of the IYA 2009. This commitment now continues indefinitely, UNESCO and the IAU having entered into a wider global partnership. The Astronomy and World Heritage Working Group
    [Show full text]
  • The Skyscraper 2009 04.Indd
    A Better Galaxy Guide: Early Spring M67: One of the most ancient open clusters known and Craig Cortis is a great novelty in this regard. Located 1.7° due W of mag NGC 2419: 3.25° SE of mag 6.2 66 Aurigae. Hard to find 4.3 Alpha Cancri. and see; at E end of short row of two mag 7.5 stars. Highly NGC 2775: Located 3.7° ENE of mag 3.1 Zeta Hydrae. significant and worth the effort —may be approximately (Look for “Head of Hydra” first.) 300,000 light years distant and qualify as an extragalactic NGC 2903: Easily found at 1.5° due S of mag 4.3 Lambda cluster. Named the Intergalactic Wanderer. Leonis. NGC 2683: Marks NW “crook” of coathanger-type triangle M95: One of three bright galaxies forming a compact with easy double star mag 4.2 Iota Cancri (which is SSW by triangle, along with M96 and M105. All three can be seen 4.8°) and mag 3.1 Alpha Lyncis (at 6° to the ENE). together in a low power, wide field view. M105 is at the NE tip of triangle, midway between stars 52 and 53 Leonis, mag Object Type R.A. Dec. Mag. Size 5.5 and 5.3 respectively —M95 is at W tip. Lynx NGC 3521: Located 0.5° due E of mag 6.0 62 Leonis. M65: One of a pair of bright galaxies that can be seen in NGC 2419 GC 07h 38.1m +38° 53’ 10.3 4.2’ a wide field view along with M66, which lies just E.
    [Show full text]
  • Varro's Roman Seasons
    Varro’s Roman Seasons Amelia Carolina Sparavigna To cite this version: Amelia Carolina Sparavigna. Varro’s Roman Seasons. 2019. hal-02387848 HAL Id: hal-02387848 https://hal.archives-ouvertes.fr/hal-02387848 Submitted on 30 Nov 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. HAL, Submitted 30 November 2019 Varro's Roman Seasons A. C. Sparavigna1 1 Dipartimento di Scienza Applicata e Tecnologia, Politecnico di Torino, Torino, Italy The four seasons of the Roman calendar, as described by Marcus Terentius Varro, are different from our seasons, in the sense that they start on days which differ from those that we are using today. In his Books on Agriculture, Varro shows that the Roman seasons started on the Cross Quarter-days instead than on the Quarter-days of the year as it happens today. Besides the classic subdivision in four parts, in the Books on Agriculture we can also find the year divided into eight parts, that is eight seasons having quite different lengths. In our discussion of Varro's seasons we will compare the days he mentions for the separation of seasons to the Cross Quarter- and Quarter-days that we find in Celtic calendars.
    [Show full text]
  • Commission C4 Annual Report 2017
    Commission C4 annual report 2017 Report for the period January to December 2017 The Commission's main achievements during 2017 are as follows. 1 The publication of the second ICOMOS-IAU Thematic Study on astronomical heritage ("TS2"). Heritage Sites of Astronomy and Archaeoastronomy in the Context of the World Heritage Convention: Thematic Study no. 2 was published as an e-book in June, in time for the 2017 UNESCO World Heritage Committee meeting in Kraków, and as a paperback in November, in time for the ICOMOS General Assembly in Delhi. ICOMOS Thematic Studies (sometimes produced in co-operation with specialist partner organisations) aim to provide a synthesis of current research and knowledge on a specific theme and/or region, and are useful to State Parties wishing to nominate a heritage property for inscription on the World Heritage List. TS2 examines a number of key questions relating to astronomical heritage sites and their potential recognition as World Heritage, attempting to identify what might constitute “outstanding universal value” (OUV) in relation to astronomy. It represents the culmination of several years' work to address some of the most challenging issues raised in the first ICOMOS-IAU Thematic Study ("TS1"), published in 2010. A particularly complex issue is the recognition and protection of dark skies. Dark sky areas cannot in themselves be considered as potential World Heritage Sites, but TS2 includes a thematic chapter by Michel Cotte of ICOMOS considering a range of ways in which dark sky values can be interrelated with broader cultural or natural values of a place and thereby contribute to its overall cultural or natural value and potential OUV.
    [Show full text]
  • A Handbook of Double Stars, with a Catalogue of Twelve Hundred
    The original of this bool< is in the Cornell University Library. There are no known copyright restrictions in the United States on the use of the text. http://www.archive.org/details/cu31924064295326 3 1924 064 295 326 Production Note Cornell University Library pro- duced this volume to replace the irreparably deteriorated original. It was scanned using Xerox soft- ware and equipment at 600 dots per inch resolution and com- pressed prior to storage using CCITT Group 4 compression. The digital data were used to create Cornell's replacement volume on paper that meets the ANSI Stand- ard Z39. 48-1984. The production of this volume was supported in part by the Commission on Pres- ervation and Access and the Xerox Corporation. Digital file copy- right by Cornell University Library 1991. HANDBOOK DOUBLE STARS. <-v6f'. — A HANDBOOK OF DOUBLE STARS, WITH A CATALOGUE OF TWELVE HUNDRED DOUBLE STARS AND EXTENSIVE LISTS OF MEASURES. With additional Notes bringing the Measures up to 1879, FOR THE USE OF AMATEURS. EDWD. CROSSLEY, F.R.A.S.; JOSEPH GLEDHILL, F.R.A.S., AND^^iMES Mt^'^I^SON, M.A., F.R.A.S. "The subject has already proved so extensive, and still ptomises so rich a harvest to those who are inclined to be diligent in the pursuit, that I cannot help inviting every lover of astronomy to join with me in observations that must inevitably lead to new discoveries." Sir Wm. Herschel. *' Stellae fixac, quae in ccelo conspiciuntur, sunt aut soles simplices, qualis sol noster, aut systemata ex binis vel interdum pluribus solibus peculiari nexu physico inter se junccis composita.
    [Show full text]
  • List of Easy Double Stars for Winter and Spring  = Easy  = Not Too Difficult  = Difficult but Possible
    List of Easy Double Stars for Winter and Spring = easy = not too difficult = difficult but possible 1. Sigma Cassiopeiae (STF 3049). 23 hr 59.0 min +55 deg 45 min This system is tight but very beautiful. Use a high magnification (150x or more). Primary: 5.2, yellow or white Seconary: 7.2 (3.0″), blue 2. Eta Cassiopeiae (Achird, STF 60). 00 hr 49.1 min +57 deg 49 min This is a multiple system with many stars, but I will restrict myself to the brightest one here. Primary: 3.5, yellow. Secondary: 7.4 (13.2″), purple or brown 3. 65 Piscium (STF 61). 00 hr 49.9 min +27 deg 43 min Primary: 6.3, yellow Secondary: 6.3 (4.1″), yellow 4. Psi-1 Piscium (STF 88). 01 hr 05.7 min +21 deg 28 min This double forms a T-shaped asterism with Psi-2, Psi-3 and Chi Piscium. Psi-1 is the uppermost of the four. Primary: 5.3, yellow or white Secondary: 5.5 (29.7), yellow or white 5. Zeta Piscium (STF 100). 01 hr 13.7 min +07 deg 35 min Primary: 5.2, white or yellow Secondary: 6.3, white or lilac (or blue) 6. Gamma Arietis (Mesarthim, STF 180). 01 hr 53.5 min +19 deg 18 min “The Ram’s Eyes” Primary: 4.5, white Secondary: 4.6 (7.5″), white 7. Lambda Arietis (H 5 12). 01 hr 57.9 min +23 deg 36 min Primary: 4.8, white or yellow Secondary: 6.7 (37.1″), silver-white or blue 8.
    [Show full text]
  • Varro's Roman Seasons
    HAL, Submitted 30 November 2019 Varro's Roman Seasons A. C. Sparavigna1 1 Dipartimento di Scienza Applicata e Tecnologia, Politecnico di Torino, Torino, Italy The four seasons of the Roman calendar, as described by Marcus Terentius Varro, are different from our seasons, in the sense that they start on days which differ from those that we are using today. In his Books on Agriculture, Varro shows that the Roman seasons started on the Cross Quarter-days instead than on the Quarter-days of the year as it happens today. Besides the classic subdivision in four parts, in the Books on Agriculture we can also find the year divided into eight parts, that is eight seasons having quite different lengths. In our discussion of Varro's seasons we will compare the days he mentions for the separation of seasons to the Cross Quarter- and Quarter-days that we find in Celtic calendars. Keywords: Chronology, Roman Chronology, Julian Calendar, Celtic festivals. DOI:10.5281/zenodo.3559524 Marcus Terentius Varro (116 - 27 BC) was a Roman scholar and writer. In his political career, he became tribune of the people, quaestor and curule aedile. Supporting Pompey, Varro reached the office of praetor [1,2]. He was also one of the members of the commission that carried out the agrarian plan of Julius Caesar for the resettlement of Capua and Campania (59 BC) [2]. During the civil war, Varro commanded one of Pompey's armies in Spain. After the battle of Pharsalus, he reconciled with Julius Caesar, and Caesar appointed him to oversee the public library of Rome [1].
    [Show full text]
  • April 14 2018 7:00Pm at the April 2018 Herrett Center for Arts & Science College of Southern Idaho
    Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting President’s Message Tim Frazier Saturday, April 14th 2018 April 2018 7:00pm at the Herrett Center for Arts & Science College of Southern Idaho. It really is beginning to feel like spring. The weather is more moderate and there will be, hopefully, clearer skies. (I write this with some trepidation as I don’t want to jinx Public Star Party Follows at the it in a manner similar to buying new equipment will ensure at least two weeks of Centennial Observatory cloudy weather.) Along with the season comes some great spring viewing. Leo is high overhead in the early evening with its compliment of galaxies as is Coma Club Officers Berenices and Virgo with that dense cluster of extragalactic objects. Tim Frazier, President One of my first forays into the Coma-Virgo cluster was in the early 1960’s with my [email protected] new 4 ¼ inch f/10 reflector and my first star chart, the epoch 1960 version of Norton’s Star Atlas. I figured from the maps I couldn’t miss seeing something since Robert Mayer, Vice President there were so many so closely packed. That became the real problem as they all [email protected] appeared as fuzzy spots and the maps were not detailed enough to distinguish one galaxy from another. I still have that atlas as it was a precious Christmas gift from Gary Leavitt, Secretary my grandparents but now I use better maps, larger scopes and GOTO to make sure [email protected] it is M84 or M86.
    [Show full text]
  • Materiały Sekcji Obserwacji Pozycji I Zakryć Polskiego Towarzystwa Miłośników Astronomii
    Materiały Sekcji Obserwacji Pozycji i Zakryć Polskiego Towarzystwa Miłośników Astronomii Nr 81 (1/2007) Brzegówkowy początek roku Uczestnicy wypraw obserwacyjnych 21 kwietnia Wydawnictwo dofinansowane ze środków Ministerstwa Nauki i Szkolnictwa Wyższego Sekcja Obserwacji Pozycji i Zakryć Polskiego Towarzystwa Miłośników Astronomii (SOPiZ PTMA) członek Międzynarodowego Towarzystwa Rejestracji Momentów Zakryć / Sekcja Europejska (International Occultation Timing Association / European Section) Sekcja istnieje od roku 1979 jako organizacja wewnętrzna Polskiego Towarzystwa Miłośników Astronomii. Sekcja zajmuje się prowadzeniem prac obserwacyjnych, obliczeniowych i analitycznych w dziedzinie zakryć - zaćmień oraz obserwacji pozycyjnych. Raz do roku SOPiZ organizuje konferencję poświęconą tematyce zakryć, zagadnień astrometrycznych i innych pokrewnych. Sekcja wydaje własny biuletyn „Materiały". Każdy członek Towarzystwa może przystąpić do aktywnej pracy w SOPiZ, stając się jej pełnoprawnym członkiem poprzez wykonywanie cennych obserwacji czy prac obliczeniowo - analitycznych. Bogate doświadczenie SOPiZ, jej zaangażowanie w prace techniczne, aktywna współpraca analityczna i koordynacyjna z innymi grupami z całego świata spowodowały, że od wielu lat Sekcja cieszy się uznaniem w międzynarodowym środowisku zajmującym się jej dziedziną działalności. Siedziba SOPiZ PTMA mieści się w Łodzi. Korespondencję należy kierować na adres: Sekcja Obserwacji Pozycji i Zakryć PTMA Planetarium i Obserwatorium Astronomiczne im. Arego Sternfelda ul. Pomorska 16
    [Show full text]
  • Arxiv:2006.10868V2 [Astro-Ph.SR] 9 Apr 2021 Spain and Institut D’Estudis Espacials De Catalunya (IEEC), C/Gran Capit`A2-4, E-08034 2 Serenelli, Weiss, Aerts Et Al
    Noname manuscript No. (will be inserted by the editor) Weighing stars from birth to death: mass determination methods across the HRD Aldo Serenelli · Achim Weiss · Conny Aerts · George C. Angelou · David Baroch · Nate Bastian · Paul G. Beck · Maria Bergemann · Joachim M. Bestenlehner · Ian Czekala · Nancy Elias-Rosa · Ana Escorza · Vincent Van Eylen · Diane K. Feuillet · Davide Gandolfi · Mark Gieles · L´eoGirardi · Yveline Lebreton · Nicolas Lodieu · Marie Martig · Marcelo M. Miller Bertolami · Joey S.G. Mombarg · Juan Carlos Morales · Andr´esMoya · Benard Nsamba · KreˇsimirPavlovski · May G. Pedersen · Ignasi Ribas · Fabian R.N. Schneider · Victor Silva Aguirre · Keivan G. Stassun · Eline Tolstoy · Pier-Emmanuel Tremblay · Konstanze Zwintz Received: date / Accepted: date A. Serenelli Institute of Space Sciences (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E- 08193, Spain and Institut d'Estudis Espacials de Catalunya (IEEC), Carrer Gran Capita 2, Barcelona, E-08034, Spain E-mail: [email protected] A. Weiss Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany C. Aerts Institute of Astronomy, Department of Physics & Astronomy, KU Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium and Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ Nijmegen, the Netherlands G.C. Angelou Max Planck Institute for Astrophysics, Karl Schwarzschild Str. 1, Garching bei M¨unchen, D-85741, Germany D. Baroch J. C. Morales I. Ribas Institute of· Space Sciences· (ICE, CSIC), Carrer de Can Magrans S/N, Bellaterra, E-08193, arXiv:2006.10868v2 [astro-ph.SR] 9 Apr 2021 Spain and Institut d'Estudis Espacials de Catalunya (IEEC), C/Gran Capit`a2-4, E-08034 2 Serenelli, Weiss, Aerts et al.
    [Show full text]