A Critical Study of Various Theories on the References to Astrology and Cosmology in the Plays of Shakespeare
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The Tragedy of Hamlet
THE TRAGEDY OF HAMLET THE WORKS OF SHAKESPEARE THE TRAGEDY OF HAMLET EDITED BY EDWARD DOWDEN n METHUEN AND CO. 36 ESSEX STREET: STRAND LONDON 1899 9 5 7 7 95 —— CONTENTS PAGE Introduction ix The Tragedy of Hamlet i Appendix I. The "Travelling" of the Players. 229 Appendix II.— Some Passages from the Quarto of 1603 231 Appendix III. Addenda 235 INTRODUCTION This edition of Hamlet aims in the first place at giving a trustworthy text. Secondly, it attempts to exhibit the variations from that text which are found in the primary sources—the Quarto of 1604 and the Folio of 1623 — in so far as those variations are of importance towards the ascertainment of the text. Every variation is not recorded, but I have chosen to err on the side of excess rather than on that of defect. Readings from the Quarto of 1603 are occa- sionally given, and also from the later Quartos and Folios, but to record such readings is not a part of the design of this edition. 1 The letter Q means Quarto 604 ; F means Folio 1623. The dates of the later Quartos are as follows: —Q 3, 1605 161 1 undated 6, For ; Q 4, ; Q 5, ; Q 1637. my few references to these later Quartos I have trusted the Cambridge Shakespeare and Furness's edition of Hamlet. Thirdly, it gives explanatory notes. Here it is inevitable that my task should in the main be that of selection and condensation. But, gleaning after the gleaners, I have perhaps brought together a slender sheaf. -
Reinhold, Renee 24016 Thompson.Pdf (578.0Kb)
Renee J. Reinhold Capstone Abstract Technology In Education The Teacher Education Program at Northern Illinois University is typically divided into two sections: the methods courses/teacher preparation semesters, and the actual sixteen-week student teaching experience. This unintentional separation often leaves the students in the prepatory semesters apprehensive about what is actually going to ,happen when they are student teaching. The student teachers themselves also feel somewhat alienated from the program due to being off-campus. This research project presents a model of how to connect the two divided segments of the Elementary Education program through telecommunica~s. Students from CIEE 344 were used to complete the model. These pre~ semester students searched tools available on the internet to coincide with a thematic unit I was planning for my third grade student teaching experience. In the end, this model grew into not only using the information sent via electronic mail, but also evolved into a technological experience for the children. The third graders learned the basic searching mechanisms on the internet to complete cooperative reports on planets which were shared with the class. ~, HONORS 1HESIS ABSTRAcr nmsIS SUBMISSION FORM Aln1IOR:Renee Jean Reinhold THESISTITLE: "Technology in Education ADVISOR: Dr. Tom Thompson ADVISOR'SDEPT: Curriculum s Inst. DISCIP~: Science Curriculum and Instruction YEAR: 1996 PAGE LENGTH: BmLIOGRAPHY: yes ILLUSTRATED: no PUBUSHED (YES OR NO): no LIST PUBLICAnON: no COPIES AVAllABLE (HARD COPY. MICROFILM. DISKETIE): 4 ABSTRACf (100-200 WORDS): See Attached AlAY 10 19!6 Student name:.~R_e.u.n_e_e--W.J..•.,--Aolo"""''''''''~~-= _ Approved by: Department of: Curriculum and Instruction Date: April 29, 1996 / Technology In Education I. -
Uranus, Neptune and Pluto
Modern Astronomy: Voyage to the Planets Lecture 8 The outer planets: Uranus, Neptune and Pluto University of Sydney Centre for Continuing Education Autumn 2005 Tonight: • Uranus • Neptune • Pluto and Chiron • The Voyager missions continue (or not?) The only mission to fly to the outer planets was Voyager 2. After leaving Saturn in August 1981, Voyager arrived at Uranus in January 1986, then flew on past Neptune in August 1989. It then swung down below the ecliptic and headed into interstellar space. Uranus Uranus was discovered in 1781 by William Herschel, musician and amateur astronomer. Herschel became the first person in recorded history to discover a new planet, at a stroke doubling the size of the known Solar System. In fact, Uranus had been detected, mistaken for a star, on 22 occasions during the preceding century, including by John Flamsteed, the first Astronomer Royal, who called it 34 Tauri. Basic facts Uranus Uranus/Earth Mass 86.83 x 1024 kg 14.536 Radius 25,559 km 4.007 Mean density 1.270 g/cm3 0.230 Gravity (eq., 1 bar) 8.87 m/s2 0.905 Semi-major axis 2872 x 106 km 19.20 Period 30 685.4 d 84.011 Orbital inclination 0.772o - Orbital eccentricity 0.0457 2.737 Axial tilt 97.8o 4.173 Rotation period –17.24 h 0.720 Length of day 17.24 h 0.718 Uranus shows an almost totally featureless disk. Even Voyager 2 at a distance of 80,000 km saw few distinguishable features. Uranus’ atmosphere is made up of 83% hydrogen, 15% helium, 2% methane and small amounts of acetylene and other hydrocarbons. -
Chapter Xii Individual Membership by Commission
Transactions IAU, Volume XXVIIB Proc. XXVII IAU General Assembly, August 2009 c 2010 International Astronomical Union Ian F. Corbett, ed. DOI: 00.0000/X000000000000000X CHAPTER XII INDIVIDUAL MEMBERSHIP BY COMMISSION 419 420 CHAPTER XII Division I Commission 4 Ephemerides President Kaplan, George Vice-President Hohenkerk, Catherine Organizing Committee Arlot, Jean-Eudes Folkner, William Urban, Sean Bangert, John Lara, Martin Vondr´ak,Jan Bell, Steven Pitjeva, Elena Members Abalakin, Viktor Hilton, James Olivier, Enrico Ahn, Youngsook Howard, Sethanne Reasenberg, Robert Aoki, Shinko Ilyas, Mohammad Rodin, Alexander Arakida, Hideyoshi Ivantsov, Anatoliy Rossello, Gaspar Bandyopadhyay, A. Janiczek, Paul Salazar, Antonio Capitaine, Nicole Johnston, Kenneth Schwan, Heiner Chapront, Jean Kinoshita, Hiroshi Seidelmann, P. Chapront-Touze, Michelle Klepczynski, William Shapiro, Irwin Coma, Juan Kolaczek, Barbara Shiryaev, Alexander Cooper, Nicholas Krasinsky, George Shuygina, Nadia de Greiff, J. Laskar, Jacques Simon, Jean-Louis Di, Xiaohua Lehmann, Marek S^oma,Mitsuru Dickey, Jean Lieske, Jay Standish, E. Duncombe, Raynor Lopez Moratalla, Teodoro Thuillot, William Dunham, David Lukashova, Marina Ting, Yeou-Tswen Eroshkin, Georgij Madsen, Claus Vilinga, Jaime Fiala, Alan Majid, Abdul Wang, Xiao-bin Fienga, Agn`es Mallamaci, Claudio Wielen, Roland Fominov, Aleksandr Emelyanenko, Yoshimitsu Wilkins, George Fu, Yanning Morrison, Leslie Williams, Carol Giorgini, Jon Mueller, Ivan Williams, James Glebova, Nina Newhall, X. Winkler, Gernot Harper, David -
Hamlet, Two of King Lear, Henry V, Romeo and Juliet, and Others
Folger Shakespeare Library https://shakespeare.folger.edu/ Get even more from the Folger You can get your own copy of this text to keep. Purchase a full copy to get the text, plus explanatory notes, illustrations, and more. Buy a copy Contents From the Director of the Folger Shakespeare Library Front Textual Introduction Matter Synopsis Characters in the Play Scene 1 Scene 2 ACT 1 Scene 3 Scene 4 Scene 5 Scene 1 ACT 2 Scene 2 Scene 1 Scene 2 ACT 3 Scene 3 Scene 4 Scene 1 Scene 2 Scene 3 ACT 4 Scene 4 Scene 5 Scene 6 Scene 7 Scene 1 ACT 5 Scene 2 From the Director of the Folger Shakespeare Library It is hard to imagine a world without Shakespeare. Since their composition four hundred years ago, Shakespeare’s plays and poems have traveled the globe, inviting those who see and read his works to make them their own. Readers of the New Folger Editions are part of this ongoing process of “taking up Shakespeare,” finding our own thoughts and feelings in language that strikes us as old or unusual and, for that very reason, new. We still struggle to keep up with a writer who could think a mile a minute, whose words paint pictures that shift like clouds. These expertly edited texts are presented to the public as a resource for study, artistic adaptation, and enjoyment. By making the classic texts of the New Folger Editions available in electronic form as The Folger Shakespeare (formerly Folger Digital Texts), we place a trusted resource in the hands of anyone who wants them. -
Uranus' Moon Titania 6 July 2015, by Matt Williams
Uranus' moon Titania 6 July 2015, by Matt Williams than Herschel would observe them. In addition, Titania would be referred to as "the first satellite of Uranus" for many years – or by the designation Uranus I, which was given to it by William Lassell in 1848. By 1851, Lassell began to number all four known satellites in order of their distance from the planet by Roman numerals, at which point Titania's designation became Uranus III. By 1852, Herschel's son John, and at the behest of Lassell himself, suggested the moon's name be changed to Titania, the Queen of the Fairies in A Midsummer Night's Dream. This was consistent with all of Uranus' satellites, which were given names from the works of William Shakespeare and Alexander Pope. Voyager 2 image of Titania, Uranus’ largest moon. Credit: NASA Size, Mass and Orbit: With a diameter of 1,578 kilometers, a surface area of 7,820,000 km² and a mass of 3.527±0.09 × Like all of the Solar Systems' gas giants, Uranus 1021 kg, Titania is the largest of Uranus' moons has an extensive system of moons. In fact, and the eighth largest moon in the Solar System. At astronomers can now account for 27 moons in a distance of about 436,000 km (271,000 mi), orbit around Uranus. Of these, none are greater in Titania is also the second farthest from the planet size, mass, or surface area than Titania. One of of the five major moons. the first moon's to be discovered around Uranus, this heavily cratered and scarred moon was Titania's moon also has a small eccentricity and is appropriately named after the fictional Queen of inclined very little relative to the equator of Uranus. -
Reading Parenthood and the Pregnant Body in Shakespeare's a Midsummer Night's Dream and Titus Andronicus
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Supervised Undergraduate Student Research Chancellor’s Honors Program Projects and Creative Work 8-2013 Reading Parenthood and the Pregnant Body in Shakespeare’s A Midsummer Night’s Dream and Titus Andronicus Martha Elaine Goddard [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_chanhonoproj Part of the Literature in English, British Isles Commons Recommended Citation Goddard, Martha Elaine, "Reading Parenthood and the Pregnant Body in Shakespeare’s A Midsummer Night’s Dream and Titus Andronicus" (2013). Chancellor’s Honors Program Projects. https://trace.tennessee.edu/utk_chanhonoproj/1804 This Dissertation/Thesis is brought to you for free and open access by the Supervised Undergraduate Student Research and Creative Work at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Chancellor’s Honors Program Projects by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. Meg Goddard Advisor: Dr. Anthony Welch May 2013 Reading Parenthood and the Pregnant Body in Shakespeare’s A Midsummer Night’s Dream and Titus Andronicus In both A Midsummer Night’s Dream (1594-6) and Titus Andronicus (1592), Shakespeare explores themes related to parenthood, particularly in regard to sexual violence, pregnancy and fertility, maternity and paternity, and patriarchal control of the female body. The motifs of parenthood and pregnancy connect with themes that extend across both plays – for example, as a symbol of female mystery removed from male influence, as a metaphor for the “anxiety of influence” of a playwright painfully aware of his illustrious literary predecessors, as a metaphor for impending new beginnings of unknown potential, and, by its relation to birth and the cyclical pattern of life, a feature of human existence intimately linked with death. -
Appendix a Luna and Telescopes
Appendix A Luna and Telescopes Exploring Luna’s surface is one of the easiest things to do in this book. You have a few options when you do this. It has the advan- tage of being the only moon visible to the naked eyes. (You might be able to just see the Galilean moons, but you would hardly be able to do anything beyond just see them.) So the next step is to consider an instrument. Be aware, this is not a general purpose guide. If you want one, look at the local library or bookseller for a copy of “NightWatch” as the book is excellent, has a sturdy plastic spiral for easy hands- free use and will serve you in more ways than just binoculars for many years to come. That being said all my recommendations in this chapter are for viewing ONLY OUR MOON. Most other moons will be pinpricks, so if you can see them at all you did the best you could. If you also wish to view nebula, galaxies, birds, be rude to your neighbors, and so forth, do your homework. Binoculars The first option is to go with binoculars. These come in a variety of sizes, which is listed as two numbers. The first is magnification and the second is aperture size (in mm). Common sizes include 7 × 35, 7 × 42, 8 × 40, 9 × 50 or even 10 × 50. For dim object you will want the bigger sizes, but the moon is not a dim object. Even a 7 × 35 will produce some pretty spectacular views. -
The Science Case for Spacecraft Exploration of the Uranian Satellites
The Science Case for Spacecraft Exploration of the Uranian Satellites A Science White Paper for the Planetary Science and Astrobiology Decadal Survey 2023-2032 Richard Cartwright, Chloe Beddingfield, T Nordheim, C. Elder, W. Grundy, B. Buratti, A. Bramson, M. Sori, R. Pappalardo, M. Neveu, et al. To cite this version: Richard Cartwright, Chloe Beddingfield, T Nordheim, C. Elder, W. Grundy, et al.. The Science Case for Spacecraft Exploration of the Uranian Satellites A Science White Paper for the Planetary Science and Astrobiology Decadal Survey 2023-2032. 2020. hal-03017585 HAL Id: hal-03017585 https://hal.archives-ouvertes.fr/hal-03017585 Preprint submitted on 1 Dec 2020 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. The Science Case for Spacecraft Exploration of the Uranian Satellites Lead Authors: Richard J. Cartwright1 & Chloe B. Beddingfield1,2 1 2 SETI Institute, NASA Ames Research Center [email protected] [email protected] Uranian satellites imaged by Voyager 2, not shown to scale (NASA/JPL-Caltech/USGS, [55]). Puck (top left), Miranda (top middle), Ariel (top right), Umbriel (bottom left), Titania (bottom middle), and Oberon (bottom right). Co-Authors: T. -
Data Mining by Grid Computing in the Search for Extrasolar Planets
Technological University Dublin ARROW@TU Dublin Doctoral Theses&Dissertations 2017 Data Mining by Grid Computing in the Search for Extrasolar Planets Oisin Creaner [Thesis] Dublin Institute for Advanced Studies, [email protected] Follow this and additional works at: https://arrow.tudublin.ie/ittthedoc Part of the Databases and Information Systems Commons, External Galaxies Commons, Instrumentation Commons, Numerical Analysis and Scientific Computing Commons, Other Astrophysics and Astronomy Commons, Other Computer Sciences Commons, Software Engineering Commons, Stars, Interstellar Medium and the Galaxy Commons, and the Theory and Algorithms Commons Recommended Citation Creaner, O. (2017) Data Mining by Grid Computing in the Search for Extrasolar Planets, Doctoral Thesis, Institute of Technology, Tallaght, Dublin. DOI:10.21427/7w45-6018 This Theses, Ph.D is brought to you for free and open access by the Theses&Dissertations at ARROW@TU Dublin. It has been accepted for inclusion in Doctoral by an authorized administrator of ARROW@TU Dublin. For more information, please contact [email protected], [email protected]. This work is licensed under a Creative Commons Attribution-Noncommercial-Share Alike 4.0 License Data Mining by Grid Computing in the Search for Extrasolar Planets Oisín Oliver Creaner B.A. (mod) Being a Thesis presented for the award of Doctor of Philosophy Dr. Eugene Hickey CPhys, MInstP, DEA, PhD Kevin Nolan BSc MSc, Dr. Niall Smith Ph.D School of Science and Computing Institute of Technology, Tallaght, Dublin Old Belgard Road, Tallaght, Dublin 24 Submitted to Quality and Qualifications Ireland (QQI) July 2016 i i. Declaration Statement I hereby certify that the material, which I now submit for assessment on the programmes of study leading to the award of PhD, is entirely my own work and has not been taken from the work of others except to the extent that such work has been cited and acknowledged within the text of my own work. -
The Science Case for Spacecraft Exploration of the Uranian Satellites
The Science Case for Spacecraft Exploration of the Uranian Satellites Lead Authors: Richard J. Cartwright1 & Chloe B. Beddingfield1,2 1 2 SETI Institute, NASA Ames Research Center [email protected] [email protected] Uranian satellites imaged by Voyager 2, not shown to scale (NASA/JPL-Caltech/USGS, [55]). Puck (top left), Miranda (top middle), Ariel (top right), Umbriel (bottom left), Titania (bottom middle), and Oberon (bottom right). Co-Authors: T. Nordheim, Jet Propulsion Laboratory D. Burr, Northern Arizona University C. Elder, Jet Propulsion Laboratory A. Ermakov, University of CA Berkeley W. Grundy, Lowell Observatory J. Roser, SETI Institute & NASA Ames B. Buratti, Jet Propulsion Laboratory J. Castillo-Rogez, Jet Propulsion Laboratory A. Bramson, Purdue University M. Showalter, SETI Institute M. Sori, Purdue University I. Cohen, John Hopkins University, APL R. Pappalardo, Jet Propulsion Laboratory E. Turtle, John Hopkins University, APL M. Neveu, Goddard Space Flight Center M. Hofstadter, Jet Propulsion Laboratory Additional Co-Authors and Endorsers: A full list of co-authors and endorsers is included at the end of this document. 1. Introduction and Motivation A spacecraft mission to the Uranian satellites would address the following ‘Big Questions’ identified in the Scientific Goals for Exploration of the Outer Solar System document, outlined by the OPAG community (https://www.lpi.usra.edu/opag/goals-08-28-19.pdf) [Table 1]: (1) What is the distribution and history of life in the Solar System? (2) What is the origin, evolution, and structure of planetary systems? (3) What present-day processes shape planetary systems, and how do these processes create diverse outcomes within and across different worlds? The large moons of Uranus are possible ocean worlds [1] that exhibit a variety of surface features , hinting at endogenic geologic activity in the recent past (e.g., [2]). -
Issue #88 of Lunar and Planetary
Lunar and Planetary Information BULLETIN Spring 2000/NUMBER 88 • LUNAR AND PLANETARY INSTITUTE • UNIVERSITIES SPACE RESEARCH ASSOCIATION CONTENTS G ALILEO GALIEO REDISCOVERS IO NEAR AT EROS NEWS FROM SPACE NEW IN PRINT AT IO NAMING THE PLANETS CALENDAR PREVIOUSPREVIOUS ISSUESISSUES Galileo rediscovers Io (Top) This mosaic of images collected by NASA’s Galileo spacecraft on November 25, 1999, shows a fountain of lava spewing above the surface of Jupiter’s moon Io. The active lava was bright enough to cause what the camera team describes as “bleeding” in Galileo’s camera, caused when the camera’s detector is so overloaded by the brightness of the target that elec- trons spill down across the detector. This shows up as a white blur in the image. This is the first time an active lava flow has been imaged on an- other planet. There also appear to be additional hot areas below this line, suggesting that hot lava is flowing away from the fissure. Initial estimates of the lava temperature indicate that it is well above 1000 K (1300°C) and might even be hotter than 1600 K (2400°C). Also of interest is the flat-topped mesa on the right. The scalloped margins are typical of a pro- cess geologists call “sapping,” which occurs when erosion is caused by a fluid escaping from the base of a cliff. (Above) This image taken by NASA’s Galileo spacecraft during its close flyby of Jupiter’s moon Io on November 25, 1999, shows some of the curi- ous mountains found there. The Sun illuminates the scene from the left, and because it is setting, the Sun exaggerates the shadows cast by the moun- tains.