The Astrology of Space

Total Page:16

File Type:pdf, Size:1020Kb

The Astrology of Space The Astrology of Space 1 The Astrology of Space The Astrology Of Space By Michael Erlewine 2 The Astrology of Space An ebook from Startypes.com 315 Marion Avenue Big Rapids, Michigan 49307 Fist published 2006 © 2006 Michael Erlewine/StarTypes.com ISBN 978-0-9794970-8-7 All rights reserved. No part of the publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, electronic, mechanical, photocopying, recording, or otherwise, without the prior permission of the publisher. Graphics designed by Michael Erlewine Some graphic elements © 2007JupiterImages Corp. Some Photos Courtesy of NASA/JPL-Caltech 3 The Astrology of Space This book is dedicated to Charles A. Jayne And also to: Dr. Theodor Landscheidt John D. Kraus 4 The Astrology of Space Table of Contents Table of Contents ..................................................... 5 Chapter 1: Introduction .......................................... 15 Astrophysics for Astrologers .................................. 17 Astrophysics for Astrologers .................................. 22 Interpreting Deep Space Points ............................. 25 Part II: The Radio Sky ............................................ 34 The Earth's Aura .................................................... 38 The Kinds of Celestial Light ................................... 39 The Types of Light ................................................. 41 Radio Frequencies ................................................. 43 Higher Frequencies ................................................ 44 Part III: Astrophysical Directions ............................ 49 The Sacred Zodiac ................................................. 55 Chapter 2: The Solar System .................... 57 Solar System ......................................................... 57 The Planets of Our Solar System ........................... 59 The Sun ................................................................. 60 The Sun Data ......................................................... 61 The Moon ............................................................... 62 Mother Moon .......................................................... 63 Mercury .................................................................. 65 Venus ..................................................................... 66 Earth ...................................................................... 67 Mars ....................................................................... 68 Jupiter .................................................................... 69 Saturn .................................................................... 70 Uranus ................................................................... 71 Neptune ................................................................. 72 Pluto ....................................................................... 73 Invariable Plane of the Solar System ..................... 74 Invariable Plane ..................................................... 75 The Asteroids ......................................................... 76 5 The Astrology of Space The Trojan Asteroids .............................................. 78 Ceres ..................................................................... 80 Pallas ..................................................................... 81 Juno ....................................................................... 82 Vesta ...................................................................... 83 Chapter 3: Beyond the Solar System ....... 84 The Solar Wind ...................................................... 84 Meteors .................................................................. 87 Meteors Table ........................................................ 89 Famous Meteorite Craters ..................................... 90 Comets .................................................................. 91 The Head of the Comet .......................................... 92 Spectacular Comets ............................................... 93 Table of Comets..................................................... 95 Chapter 4: Local Star System ................... 97 The Nearest Stars .................................................. 97 Near Stars Table .................................................... 98 The Local System (Gould's Belt) ............................ 99 The Plane of the Local System ............................ 102 Via Combusta -- The Southern Stream ................ 104 Chapter 5: The Milky Way Galaxy ........... 106 Our Local Spiral Arm Region ............................... 106 Our Galaxy ........................................................... 108 The Galactic Sphere ............................................ 110 The Galactic disk ................................................. 111 The Location of Our Sun ...................................... 112 Chapter Four: The Galaxy ....................... 113 Spiral Arms .......................................................... 113 Differential Rotation ............................................. 115 How Differential Rotation Works .......................... 116 Interstellar Dust .................................................... 118 Windows to the Galaxy ........................................ 119 Dark Nebulae ....................................................... 120 Dark Clouds and Interstellar Dust ........................ 120 6 The Astrology of Space Dark Nebulae ....................................................... 121 Solar Apex ........................................................... 122 Star Streaming ..................................................... 124 Type of Solar Motion Table .................................. 125 The Galactic Center (GC) .................................... 126 The Galactic Nucleus ........................................... 128 Chapter 6: Star Lives ............................... 131 The Birthplace of Stars ........................................ 133 A Star is Born ....................................................... 134 Protostars ............................................................ 135 Stellar Equilibrium ................................................ 136 The Stellar Prime of Life ...................................... 137 A Red Giant ......................................................... 138 A Supernova ........................................................ 140 The End of Life for Stars ...................................... 141 A Neutron Star ..................................................... 143 The Black Hole..................................................... 144 Hertzsprung-Russell Diagram .............................. 146 Using Stars with your Natal Chart ........................ 148 Hertzsprung-Russell Diagram II ........................... 151 The Time Table for Our Sun in Years .................. 151 Chapter 7: The Kinds of Stars ................. 152 Double Stars ........................................................ 152 Double Stars: Equal Doubles ............................... 153 Double Stars: Unequal Doubles ........................... 154 Double Stars: Multiple Stars ................................ 155 Double Stars: Triple Stars .................................... 156 Rapid Binary ........................................................ 157 One star in very tight orbit around a larger star. ... 157 Physical Doubles or Binaries ............................... 158 Visual Binaries ..................................................... 159 Spectroscopic Binary Stars .................................. 160 Spectroscopic Binaries ........................................ 160 Binary System ...................................................... 162 Eclipsing Binaries ................................................. 163 7 The Astrology of Space Spectroscopic Binary Stars .................................. 163 Eclipsing Binaries ................................................. 163 Variable Stars ...................................................... 165 Pulsating Variables .............................................. 165 Explosive Variables .............................................. 166 Variable Star Naming ........................................... 166 The Two Types of Intrinsic Variables: .................. 167 Extrinsic Variables ............................................... 167 Intrinsic Variables ................................................. 167 Periodic Variables ................................................ 168 The Cepheid Variables ........................................ 168 The RR Lyrae Stars ............................................. 169 W. Virginis and RV Tauri Stars ............................ 169 Long-Period Variables ......................................... 170 Semi-Regular Variables ....................................... 171 Irregular Variables ................................................ 172 Flare Stars ........................................................... 173 Flare Star Table ................................................... 173 Magnetic Stars ..................................................... 174 Magnetic Stars Table ........................................... 174 Novae: Exploding Stars ....................................... 175 Dwarf Novae, Novae, and Recurrent Novae ........ 176 Dwarf Novae ........................................................ 177 Recurrent Novae .................................................. 177 Novae .................................................................
Recommended publications
  • Stsci Newsletter: 1997 Volume 014 Issue 01
    January 1997 • Volume 14, Number 1 SPACE TELESCOPE SCIENCE INSTITUTE Highlights of this issue: • AURA science and functional awards to Leitherer and Hanisch — pages 1 and 23 • Cycle 7 to be extended — page 5 • Cycle 7 approved Newsletter program listing — pages 7-13 Astronomy with HST Climbing the Starburst Distance Ladder C. Leitherer Massive stars are an important and powerful star formation events in sometimes dominant energy source for galaxies. Even the most luminous star- a galaxy. Their high luminosity, both in forming regions in our Galaxy are tiny light and mechanical energy, makes on a cosmic scale. They are not them detectable up to cosmological dominated by the properties of an distances. Stars ~100 times more entire population but by individual massive than the Sun are one million stars. Therefore stochastic effects times more luminous. Except for stars prevail. Extinction represents a severe of transient brightness, like novae and problem when a reliable census of the supernovae, hot, massive stars are Galactic high-mass star-formation the most luminous stellar objects in history is atempted, especially since the universe. massive stars belong to the extreme Massive stars are, however, Population I, with correspondingly extremely rare: The number of stars small vertical scale heights. Moreover, formed per unit mass interval is the proximity of Galactic regions — roughly proportional to the -2.35 although advantageous for detailed power of mass. We expect to find very studies of individual stars — makes it few massive stars compared to, say, difficult to obtain integrated properties, solar-type stars. This is consistent with such as total emission-line fluxes of observations in our solar neighbor- the ionized gas.
    [Show full text]
  • Lurking in the Shadows: Wide-Separation Gas Giants As Tracers of Planet Formation
    Lurking in the Shadows: Wide-Separation Gas Giants as Tracers of Planet Formation Thesis by Marta Levesque Bryan In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy CALIFORNIA INSTITUTE OF TECHNOLOGY Pasadena, California 2018 Defended May 1, 2018 ii © 2018 Marta Levesque Bryan ORCID: [0000-0002-6076-5967] All rights reserved iii ACKNOWLEDGEMENTS First and foremost I would like to thank Heather Knutson, who I had the great privilege of working with as my thesis advisor. Her encouragement, guidance, and perspective helped me navigate many a challenging problem, and my conversations with her were a consistent source of positivity and learning throughout my time at Caltech. I leave graduate school a better scientist and person for having her as a role model. Heather fostered a wonderfully positive and supportive environment for her students, giving us the space to explore and grow - I could not have asked for a better advisor or research experience. I would also like to thank Konstantin Batygin for enthusiastic and illuminating discussions that always left me more excited to explore the result at hand. Thank you as well to Dimitri Mawet for providing both expertise and contagious optimism for some of my latest direct imaging endeavors. Thank you to the rest of my thesis committee, namely Geoff Blake, Evan Kirby, and Chuck Steidel for their support, helpful conversations, and insightful questions. I am grateful to have had the opportunity to collaborate with Brendan Bowler. His talk at Caltech my second year of graduate school introduced me to an unexpected population of massive wide-separation planetary-mass companions, and lead to a long-running collaboration from which several of my thesis projects were born.
    [Show full text]
  • Near and Mid-IR Photometry of the Pleiades, and a New List Of
    ApJS, in press; version with embedded figures can be obtained at http://spider.ipac.caltech.edu/staff/stauffer/ Near and Mid-IR Photometry of the Pleiades, and a New List of Substellar Candidate Members1,2 John R. Stauffer Spitzer Science Center, Caltech 314-6, Pasadena, CA 91125 [email protected] Lee W. Hartmann Astronomy Department, University of Michigan Giovanni G. Fazio, Lori E. Allen, Brian M. Patten Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 Patrick J. Lowrance, Robert L. Hurt, Luisa M. Rebull Spitzer Science Center, Caltech , Pasadena, CA 91125 Roc M. Cutri, Solange V. Ramirez Infrared Processing and Analysis Center, Caltech 220-6, Pasadena, CA 91125 Erick T. Young, George H. Rieke, Nadya I. Gorlova3, James C. Muzerolle Steward Observatory, University of Arizona, Tucson, AZ 85726 Cathy L. Slesnick Astronomy Department, Caltech, Pasadena, CA 91125 arXiv:0704.1832v1 [astro-ph] 13 Apr 2007 Michael F. Skrutskie Astronomy Department, University of Virginia, Charlottesville, VA 22903 1This work is based (in part) on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under NASA contract 1407. 2This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. 3Current address: University of Florida, 211 Bryant Space Center, Gainesville, FL 32611 –2– ABSTRACT We make use of new near and mid-IR photometry of the Pleiades cluster in order to help identify proposed cluster members.
    [Show full text]
  • Naming the Extrasolar Planets
    Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named.
    [Show full text]
  • AD ASTRA Pelo Preço Atual Devea Faze-Lo Logo, Pois Este Deverá Sofrer Majoraçáo Apáa L Do Setembro
    12 JULL T I í* # BOLETIM INFORMATIVO DA SOCIEDADE ASTRONÔMICA RIOGRANDENSE FUNDADA EM 16/09/79 ERRATA 0 editor pede desculpas pelos seguintes erros por ele cometidosv e que escaparam do revisão; pág._______ llmha____________ errado_________________cemroto__________ 1 33 CollsÕes de Cono as ColisÕes e Modelos Modelaram 12 título Planetários os Planetas 11 3 (e - 1) (e2 - i) 11 28 >0 E > 0 33 tabela 3 0** Oiih32nln 3^ diagrama saiu girado de 90° para a direita C í üL_J o mes passado a SARG procedeu una refomulaçao dos Estatutos desta Sociedade^ refomulaçao que já urgia, uma vez que o Ej3 U\i_J tatuto antigo nao se adequava mais à realidade da SARG. Cota cr^Jo crescimento da Sociedade, era necessário um Estatuto mais dinâmico, voltado aos novos interesses desta.^Por motivos, alguns normais e outros nem tanto, seguiu-se a eleição de uma nova Direto­ ria Executiva e de um novo Conselho^Fiscal, assim como uma reorgani^ zaçáo das coordenadorias das Comissões de Estudo (já existentes e novas) e Departamentos (recém-criados). Os novos titulares dos diver sos crgos estão relacionados á página 38. Todos que quiserem assinar o AD ASTRA pelo preço atual devea faze-lo logo, pois este deverá sofrer majoraçáo apáa l_do setembro. É conveniente lembrar que os artigos assinados são de respon sabilidade de seus autores, não necessitando estar em completo acor do cou o pensamento geral da Sociedade, que pode discordar de um ou outro ponto dos mesmos. Esta observação, no entanto, não possui re­ lação necessária com qualquer dos artigos publicados neste boletim, sendo somente um lembrete.
    [Show full text]
  • The Transfiguration in the Theology of Gregory Palamas And
    Duquesne University Duquesne Scholarship Collection Electronic Theses and Dissertations Spring 2015 Deus in se et Deus pro nobis: The rT ansfiguration in the Theology of Gregory Palamas and Its Importance for Catholic Theology Cory Hayes Follow this and additional works at: https://dsc.duq.edu/etd Recommended Citation Hayes, C. (2015). Deus in se et Deus pro nobis: The rT ansfiguration in the Theology of Gregory Palamas and Its Importance for Catholic Theology (Doctoral dissertation, Duquesne University). Retrieved from https://dsc.duq.edu/etd/640 This Immediate Access is brought to you for free and open access by Duquesne Scholarship Collection. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of Duquesne Scholarship Collection. For more information, please contact [email protected]. DEUS IN SE ET DEUS PRO NOBIS: THE TRANSFIGURATION IN THE THEOLOGY OF GREGORY PALAMAS AND ITS IMPORTANCE FOR CATHOLIC THEOLOGY A Dissertation Submitted to the McAnulty Graduate School of Liberal Arts Duquesne University In partial fulfillment of the requirements for the degree of Doctor of Philosophy By Cory J. Hayes May 2015 Copyright by Cory J. Hayes 2015 DEUS IN SE ET DEUS PRO NOBIS: THE TRANSFIGURATION IN THE THEOLOGY OF GREGORY PALAMAS AND ITS IMPORTANCE FOR CATHOLIC THEOLOGY By Cory J. Hayes Approved March 31, 2015 _______________________________ ______________________________ Dr. Bogdan Bucur Dr. Radu Bordeianu Associate Professor of Theology Associate Professor of Theology (Committee Chair) (Committee Member) _______________________________ Dr. Christiaan Kappes Professor of Liturgy and Patristics Saints Cyril and Methodius Byzantine Catholic Seminary (Committee Member) ________________________________ ______________________________ Dr. James Swindal Dr.
    [Show full text]
  • LIST of PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute
    LIST OF PUBLICATIONS Aryabhatta Research Institute of Observational Sciences ARIES (An Autonomous Scientific Research Institute of Department of Science and Technology, Govt. of India) Manora Peak, Naini Tal - 263 129, India (1955−2020) ABBREVIATIONS AA: Astronomy and Astrophysics AASS: Astronomy and Astrophysics Supplement Series ACTA: Acta Astronomica AJ: Astronomical Journal ANG: Annals de Geophysique Ap. J.: Astrophysical Journal ASP: Astronomical Society of Pacific ASR: Advances in Space Research ASS: Astrophysics and Space Science AE: Atmospheric Environment ASL: Atmospheric Science Letters BA: Baltic Astronomy BAC: Bulletin Astronomical Institute of Czechoslovakia BASI: Bulletin of the Astronomical Society of India BIVS: Bulletin of the Indian Vacuum Society BNIS: Bulletin of National Institute of Sciences CJAA: Chinese Journal of Astronomy and Astrophysics CS: Current Science EPS: Earth Planets Space GRL : Geophysical Research Letters IAU: International Astronomical Union IBVS: Information Bulletin on Variable Stars IJHS: Indian Journal of History of Science IJPAP: Indian Journal of Pure and Applied Physics IJRSP: Indian Journal of Radio and Space Physics INSA: Indian National Science Academy JAA: Journal of Astrophysics and Astronomy JAMC: Journal of Applied Meterology and Climatology JATP: Journal of Atmospheric and Terrestrial Physics JBAA: Journal of British Astronomical Association JCAP: Journal of Cosmology and Astroparticle Physics JESS : Jr. of Earth System Science JGR : Journal of Geophysical Research JIGR: Journal of Indian
    [Show full text]
  • Numerical Treatment of Radiation Processes in the Internal Shocks of Magnetized Relativistic Outflows
    Departament d’Astronom´ıa i Astrof´ısica Programa de Doctorat en F´ısica Numerical treatment of radiation processes in the internal shocks of magnetized relativistic outflows Tesi Doctoral feta per Jesus´ Misrayim´ Rueda Becerril dirigida per Dr. Miguel Angel´ Aloy Toras´ Dr. Petar Mimica Juliol de 2017 Miguel A´ ngel Aloy Toras´ , Profesor Titular del Departamento de Astronom´ıa y Astrof´ısica de la Universitat de Valencia` y Petar Mimica, Investigador Asociado al Departamento de Astronom´ıa y Astrof´ısica de la Universitat de Valencia` CERTIFICAN: Que la presente memoria, titulada: Numerical treatment of radiation processes in the internal shocks of magnetized relativistic outflows, ha sido realizada bajo su direccion´ en el Departamento de Astronom´ıa y Astrof´ısica de la Universitat de Valencia` por Jesus´ Misrayim´ Rueda Becerril, y constituye su Tesis Doctoral para optar al grado de Doctor en F´ısica. Y para que conste firman el presente certificado en Burjassot, a 29 de mayo de 2017 Fdo: Miguel Angel´ Aloy Toras´ Fdo: Petar Mimica Abstract Blazars are a type of active galactic nuclei (AGNs) which are among the most en- ergetic and violent astrophysical objects, alongside γ-ray bursts (GRBs). The phys- ical processes, and, in particular, the relativistic jet itself in which the high energy radiation detected by the terrestrial and space observatories is generated, has been attracting the attention and interest of astronomers and astrophysicists since their dis- covery. In the present thesis, we investigate the internal shock (IS) model in which two magnetized shells of plasma, with cylindrical geometry, collide forming shock waves, which propagate throughout the plasma accelerating electrons (thermal and nonthermal) in their wake.
    [Show full text]
  • 1991Apj. . .370. . .78H the Astrophysical Journal
    The Astrophysical Journal, 370:78-101,1991 March 20 .78H . © 1991. The American Astronomical Society. All rights reserved. Printed in U.S.A. .370. SPATIALLY RESOLVED OPTICAL IMAGES OF HIGH-REDSHIFT QUASI-STELLAR OBJECTS 1991ApJ. Timothy M. Heckman,12,3 Matthew D. Lehnert,1,2,4 Wil van Breugel,3,5 and George K. Miley2,3,6 Received 1990 June 21 ; accepted 1990 August 29 ABSTRACT We present and discuss the results of a program of deep optical imaging of 19 high-redshift (z > 2) radio- loud QSOs. These data represent the first large body of nonradio detections of spatially resolved structure surrounding high-redshift QSOs. _1 In 15 of 18 cases, the Lya emission is spatially resolved, with a typical size of 100 kpc (for H0 = 75 km s 1 44 _1 Mpc“ ; q0 = 0). The luminosity of the resolved Lya is «10 ergs s («10% of the total Lya luminosity). The nebulae are usually asymmetric and/or elongated with a morphological axis that aligns with the radio source axis to better than « 30°. These properties are quite similar to those of the Lya nebulae associated with high-z radio galaxies. The brighter side of the nebula is generally on the same side as the brighter radio emis- sion and/or one-sided, jetlike radio structure. There is no strong correlation between the Lya isophotal and radio sizes (the Lya nebulae range from several times larger than the radio source to several times smaller). None of the properties of the nebulae correlate with the presence or strength of C iv “associated” absorption C^abs ^ ^em)* It is likely that the nebulae are the interstellar or circumgalactic medium of young or even protogalaxies being photoionized by QSO radiation that escapes anisotropically along the radio axis.
    [Show full text]
  • AD Leonis: Flares Observed by XMM-Newton and Chandra
    A&A 411, 587–593 (2003) Astronomy DOI: 10.1051/0004-6361:20031398 & c ESO 2003 Astrophysics AD Leonis: Flares observed by XMM-Newton and Chandra E. J. M. van den Besselaar1;2, A. J. J. Raassen1;3,R.Mewe1,R.L.J.vanderMeer1,M.G¨udel4, and M. Audard5 1 SRON National Institute for Space Research, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands e-mail: [email protected];[email protected];[email protected] 2 Department of Astrophysics, University of Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands 3 Astronomical Institute “Anton Pannekoek”, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands 4 Paul Scherrer Institut, W¨urenlingen & Villigen, 5232 Villigen PSI, Switzerland e-mail: [email protected] 5 Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA e-mail: [email protected] Received 3 February 2003 / Accepted 2 September 2003 Abstract. The M-dwarf AD Leonis has been observed with the Reflection Grating Spectrometers and the European Photon Imaging Camera aboard XMM-Newton and also with the Low Energy Transmission Grating Spectrometer aboard the Chandra X-ray Observatory. In the observation taken with XMM-Newton five large flares produced by AD Leo were identified and only one in the observation taken with Chandra. A quiescent level to the lightcurves is difficult to define, since several smaller flares mutually overlap each other. However, we defined a quasi-steady state outside of obvious flares or flare decays. The spectra from the flare state and the quasi-steady state are analysed separately.
    [Show full text]
  • A Search for Transiting Extrasolar Planets in the Open Cluster NGC 4755
    ResearchOnline@JCU This file is part of the following reference: Jayawardene, Bandupriya S. (2015) A search for transiting extrasolar planets in the open cluster NGC 4755. DAstron thesis, James Cook University. Access to this file is available from: http://researchonline.jcu.edu.au/41511/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://researchonline.jcu.edu.au/41511/ A SEARCH FOR TRANSITING EXTRASOLAR PLANETS IN THE OPEN CLUSTER NGC 4755 by Bandupriya S. Jayawardene A thesis submitted in satisfaction of the requirements for the degree of Doctor of Astronomy in the Faculty of Science, Technology and Engineering June 2015 James Cook University Townsville - Australia i STATEMENT OF ACCESS I the undersigned, author of this work, understand that James Cook University will make this thesis available for use within the University Library and, via the Australian Digital Thesis network, for use elsewhere. I understand that, as an unpublished work, a thesis has significant protection under the Copyright Act and; I do not wish to place any further restriction on access to this work. 2 STATEMENT OF SOURCES DECLARATION I declare that this thesis is my own work and has not been submitted in any form for another degree or diploma at any University or other institution of tertiary education. Information derived from the published or unpublished work of others has been acknowledged in the text and list of references is given.
    [Show full text]
  • The Observer, November
    The OBSERVER The Newsletter of the Twin City Amateur Astronomers, Inc. November 2001 Volume 26, Number 11 Adventures in Meteor Hunting — Duane Yockey In This Issue: REETINGS to my brother and and binoculars just in case the meteors sister sky watchers, didn't live up to their billing. Saturday G was clear here in central Illinois, and • Meteor Hunting Adventures ...1 when I got back from a Duane shows that he has the The long awaited day play at Illinois State right stuff as he tears after the of the Leonid meteor University around Leonids and finds them! shower arrived Satur- 10:30 p.m. the sky was day. I was really still showing lots of • TCAA Calendar ........................1 looking forward to stars. I called Laura Use our calendar to mark going out to the (my oldest daughter), your calendar. observatory with who said the skies were other Twin City clear down in southern • TCAA Annual Holiday Bash....3 Amateur Indiana and I could Party like it’s, um, 2001, at Astronomers and see- drive down there, if the Vic & Cindy’s! ............................ ing the "show" from clouds rolled in (ha, 2:00 a.m. to 6:00 a.m. ha). I assured her that • Club Notes................................4 early Sunday morn- the sky would cooper- Wow, it’s been a busy month! ing. So I packed my ate, and it was looking car early with a lawn good then, and I wished • Software Review: DSE ...........5 chair and threw in my her good luck (if she And just think, if you never telescope, star charts turn to page 5, you’ll never know continued on next page what DSE stands for..
    [Show full text]