Not to Worry
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Observing Protest from a Place
VISUAL AND MATERIAL CULTURE, 1300-1700 Knox Giles Knox Sense Knowledge and the Challenge of Italian Renaissance Art El Greco, Velázquez, Rembrandt of Italian Renaissance Art Challenge the Knowledge Sense and FOR PRIVATE AND NON-COMMERCIAL USE AMSTERDAM UNIVERSITY PRESS Sense Knowledge and the Challenge of Italian Renaissance Art FOR PRIVATE AND NON-COMMERCIAL USE AMSTERDAM UNIVERSITY PRESS Visual and Material Culture, 1300–1700 A forum for innovative research on the role of images and objects in the late medieval and early modern periods, Visual and Material Culture, 1300–1700 publishes monographs and essay collections that combine rigorous investigation with critical inquiry to present new narratives on a wide range of topics, from traditional arts to seemingly ordinary things. Recognizing the fluidity of images, objects, and ideas, this series fosters cross-cultural as well as multi-disciplinary exploration. We consider proposals from across the spectrum of analytic approaches and methodologies. Series Editor Dr. Allison Levy, an art historian, has written and/or edited three scholarly books, and she has been the recipient of numerous grants and awards, from the Nation- al Endowment for the Humanities, the American Association of University Wom- en, the Getty Research Institute, the Dumbarton Oaks Research Library of Harvard University, the Whiting Foundation and the Bogliasco Foundation, among others. www.allisonlevy.com. FOR PRIVATE AND NON-COMMERCIAL USE AMSTERDAM UNIVERSITY PRESS Sense Knowledge and the Challenge of Italian Renaissance Art El Greco, Velázquez, Rembrandt Giles Knox Amsterdam University Press FOR PRIVATE AND NON-COMMERCIAL USE AMSTERDAM UNIVERSITY PRESS This book was published with support from the Office of the Vice Provost for Research, Indiana University, and the Department of Art History, Indiana University. -
Modelling and the Transit of Venus
Modelling and the transit of Venus Dave Quinn University of Queensland <[email protected]> Ron Berry University of Queensland <[email protected]> Introduction enior secondary mathematics students could justifiably question the rele- Svance of subject matter they are being required to understand. One response to this is to place the learning experience within a context that clearly demonstrates a non-trivial application of the material, and which thereby provides a definite purpose for the mathematical tools under consid- eration. This neatly complements a requirement of mathematics syllabi (for example, Queensland Board of Senior Secondary School Studies, 2001), which are placing increasing emphasis on the ability of students to apply mathematical thinking to the task of modelling real situations. Success in this endeavour requires that a process for developing a mathematical model be taught explicitly (Galbraith & Clatworthy, 1991), and that sufficient opportu- nities are provided to students to engage them in that process so that when they are confronted by an apparently complex situation they have the think- ing and operational skills, as well as the disposition, to enable them to proceed. The modelling process can be seen as an iterative sequence of stages (not ) necessarily distinctly delineated) that convert a physical situation into a math- 1 ( ematical formulation that allows relationships to be defined, variables to be 0 2 l manipulated, and results to be obtained, which can then be interpreted and a n r verified as to their accuracy (Galbraith & Clatworthy, 1991; Mason & Davis, u o J 1991). The process is iterative because often, at this point, limitations, inac- s c i t curacies and/or invalid assumptions are identified which necessitate a m refinement of the model, or perhaps even a reassessment of the question for e h t which we are seeking an answer. -
Lomonosov, the Discovery of Venus's Atmosphere, and Eighteenth Century Transits of Venus
Journal of Astronomical History and Heritage, 15(1), 3-14 (2012). LOMONOSOV, THE DISCOVERY OF VENUS'S ATMOSPHERE, AND EIGHTEENTH CENTURY TRANSITS OF VENUS Jay M. Pasachoff Hopkins Observatory, Williams College, Williamstown, Mass. 01267, USA. E-mail: [email protected] and William Sheehan 2105 SE 6th Avenue, Willmar, Minnesota 56201, USA. E-mail: [email protected] Abstract: The discovery of Venus's atmosphere has been widely attributed to the Russian academician M.V. Lomonosov from his observations of the 1761 transit of Venus from St. Petersburg. Other observers at the time also made observations that have been ascribed to the effects of the atmosphere of Venus. Though Venus does have an atmosphere one hundred times denser than the Earth’s and refracts sunlight so as to produce an ‘aureole’ around the planet’s disk when it is ingressing and egressing the solar limb, many eighteenth century observers also upheld the doctrine of cosmic pluralism: believing that the planets were inhabited, they had a preconceived bias for believing that the other planets must have atmospheres. A careful re-examination of several of the most important accounts of eighteenth century observers and comparisons with the observations of the nineteenth century and 2004 transits shows that Lomonosov inferred the existence of Venus’s atmosphere from observations related to the ‘black drop’, which has nothing to do with the atmosphere of Venus. Several observers of the eighteenth-century transits, includ- ing Chappe d’Auteroche, Bergman, and Wargentin in 1761 and Wales, Dymond, and Rittenhouse in 1769, may have made bona fide observations of the aureole produced by the atmosphere of Venus. -
Transit of Venus Presentation
http://sunearthday.nasa.gov/2012/transit/webcast.php Venus visible Venus with the unaided eye: "morning star" or the Earth "evening star. • Similar to Earth: – diameter: 12,103 km – 0.95 Earth’s – mass 0.89 of Earth's – few craters -- young surface – densities, chemical compositions are similar • rotation unusually slow (Venus day = 243 Earth days -- longer than Venus' year) • rotation retrograde • periods of Venus' rotation and of its orbit are synchronized -- always same face toward Earth when the two planets are at their closest approach • greenhouse effect -- surface temperature hot enough to melt lead M ikhail Lomonosov, june 5, 1761 discovered, during a transit, that V enus has an atmosphere The atmosphere is is composed mostly of carbon dioxide. There are several layers of clouds, many kilometers thick, composed of sulfuric acid. Mariner 10 Image of Venus V enera 13 Venus’ orbit is inclined (by 3.39 degrees) relative to the ecliptic If in the same plane we would have 5 transits in 8 years Venus: 13 years , Earth: 8 years Each time Earth completes 1.6 orbits, Venus catches up to it after 2.6 of its orbits Progress of the 2004 Transit of Venus pictured from NASA's Soho solar observatory. Credit: NASA Ascending (A) or Duration since last transit Date of transit Descending (D) node (years and months) 6 December 1631 A 4 December 1639 A 8 yrs 6 June 1761 D 121 yrs 6 months 3 June 1769 D 8 yrs 9 December 1874 A 105 yrs 6 months 6 December 1882 A 8 yrs 8 June 2004 D 121 yrs 6 months 5 June 2012 D 8 yrs 11 December 2117 A 105 yrs 6 months 8 December 2125 A 8 yrs In 6000 years 81 transits only Venus’ Role in History Copernican System vs Ptolemaic System http://astro.unl.edu/classaction/animations/renaissance/venusphases.html Venus’ Role in History Size of the Solar System - Revealed! • Kepler predicted the transit of December 1631 (though not observed!) and 120 year cycle. -
Venus Aerobot Multisonde Mission
w AIAA Balloon Technology Conference 1999 Venus Aerobot Multisonde Mission By: James A. Cutts ('), Viktor Kerzhanovich o_ j. (Bob) Balaram o), Bruce Campbell (2), Robert Gershman o), Ronald Greeley o), Jeffery L. Hall ('), Jonathan Cameron o), Kenneth Klaasen v) and David M. Hansen o) ABSTRACT requires an orbital relay system that significantly Robotic exploration of Venus presents many increases the overall mission cost. The Venus challenges because of the thick atmosphere and Aerobot Multisonde (VAMuS) Mission concept the high surface temperatures. The Venus (Fig 1 (b) provides many of the scientific Aerobot Multisonde mission concept addresses capabilities of the VGA, with existing these challenges by using a robotic balloon or technology and without requiring an orbital aerobot to deploy a number of short lifetime relay. It uses autonomous floating stations probes or sondes to acquire images of the (aerobots) to deploy multiple dropsondes capable surface. A Venus aerobot is not only a good of operating for less than an hour in the hot lower platform for precision deployment of sondes but atmosphere of Venus. The dropsondes, hereafter is very effective at recovering high rate data. This described simply as sondes, acquire high paper describes the Venus Aerobot Multisonde resolution observations of the Venus surface concept and discusses a proposal to NASA's including imaging from a sufficiently close range Discovery program using the concept for a that atmospheric obscuration is not a major Venus Exploration of Volcanoes and concern and communicate these data to the Atmosphere (VEVA). The status of the balloon floating stations from where they are relayed to deployment and inflation, balloon envelope, Earth. -
Appendix 1: Venus Missions
Appendix 1: Venus Missions Sputnik 7 (USSR) Launch 02/04/1961 First attempted Venus atmosphere craft; upper stage failed to leave Earth orbit Venera 1 (USSR) Launch 02/12/1961 First attempted flyby; contact lost en route Mariner 1 (US) Launch 07/22/1961 Attempted flyby; launch failure Sputnik 19 (USSR) Launch 08/25/1962 Attempted flyby, stranded in Earth orbit Mariner 2 (US) Launch 08/27/1962 First successful Venus flyby Sputnik 20 (USSR) Launch 09/01/1962 Attempted flyby, upper stage failure Sputnik 21 (USSR) Launch 09/12/1962 Attempted flyby, upper stage failure Cosmos 21 (USSR) Launch 11/11/1963 Possible Venera engineering test flight or attempted flyby Venera 1964A (USSR) Launch 02/19/1964 Attempted flyby, launch failure Venera 1964B (USSR) Launch 03/01/1964 Attempted flyby, launch failure Cosmos 27 (USSR) Launch 03/27/1964 Attempted flyby, upper stage failure Zond 1 (USSR) Launch 04/02/1964 Venus flyby, contact lost May 14; flyby July 14 Venera 2 (USSR) Launch 11/12/1965 Venus flyby, contact lost en route Venera 3 (USSR) Launch 11/16/1965 Venus lander, contact lost en route, first Venus impact March 1, 1966 Cosmos 96 (USSR) Launch 11/23/1965 Possible attempted landing, craft fragmented in Earth orbit Venera 1965A (USSR) Launch 11/23/1965 Flyby attempt (launch failure) Venera 4 (USSR) Launch 06/12/1967 Successful atmospheric probe, arrived at Venus 10/18/1967 Mariner 5 (US) Launch 06/14/1967 Successful flyby 10/19/1967 Cosmos 167 (USSR) Launch 06/17/1967 Attempted atmospheric probe, stranded in Earth orbit Venera 5 (USSR) Launch 01/05/1969 Returned atmospheric data for 53 min on 05/16/1969 M. -
Estudios De Platería. San Eloy 2011
ESTUDIOS DE PLATERÍA. SAN ELOY 2011 Jesús Rivas Carmona (Coord.) ESTUDIOS DE PLATERÍA. SAN ELOY 2011 UNIVERSIDAD DE MURCIA 2011 Estudios de platería, San Eloy 2011 / Jesús Rivas Carmona (Coord.).– Murcia: Universidad de Murcia, Servicio de Publicaciones, 2011 568 p. ISBN: 978-84-8371-214-6 1. Platería – Estudios y conferencias. 2. Orfebrería – Estudios y conferencias. I. Rivas Carmona, Jesús.– II. Universidad de Murcia. Servicio de Publicaciones. III. Título 739.1 (082.2) 1ª Edición, 2011 Reservados todos los derechos. De acuerdo con la legislación vigente, y bajo las sanciones en ella previstas, queda totalmente prohibida la reproducción y/o transmisión parcial o total de este libro, por procedimientos mecánicos o electrónicos, incluyendo fotocopia, grabación magnética, óptica o cualesquiera otros procedimientos que la técnica permita o pueda permitir en el futuro, sin la expresa autorización por escrito de los propietarios del copyright. © Universidad de Murcia, Servicio de Publicaciones, 2011 ISBN: 978-84-8371-214-6 Depósito Legal MU-1.286-2011 Impreso en España −Printed in Spain Imprime: F.G. Graf, S.L. [email protected] A la ciudad de Lorca, centro y obrador de platería Índice PRÓLOGO........................................................................................................... 17 María Concepción García Gainza Fiel Contraste de Honor San Eloy 2010 ESTUDIOS Plateros de Guatemala. Don Juan de Barreneche y Aguirre y el legado de Lesaca ..................................................................................................................... 23 Javier Abad Viela Arquitecto Orefi ceria siciliana nei musei madrileni ............................................................. 43 Lucia Ajello Università degli Studi di Palermo La partición de la plata y las joyas de Isabel de Valois: la herencia de la infanta Catalina Micaela....................................................................................... 53 María Albaladejo Martínez Universidad de Murcia La joyería femenina del siglo XVIII en la Nueva España a través del retrato.. -
Educator's Guide: Orion
Legends of the Night Sky Orion Educator’s Guide Grades K - 8 Written By: Dr. Phil Wymer, Ph.D. & Art Klinger Legends of the Night Sky: Orion Educator’s Guide Table of Contents Introduction………………………………………………………………....3 Constellations; General Overview……………………………………..4 Orion…………………………………………………………………………..22 Scorpius……………………………………………………………………….36 Canis Major…………………………………………………………………..45 Canis Minor…………………………………………………………………..52 Lesson Plans………………………………………………………………….56 Coloring Book…………………………………………………………………….….57 Hand Angles……………………………………………………………………….…64 Constellation Research..…………………………………………………….……71 When and Where to View Orion…………………………………….……..…77 Angles For Locating Orion..…………………………………………...……….78 Overhead Projector Punch Out of Orion……………………………………82 Where on Earth is: Thrace, Lemnos, and Crete?.............................83 Appendix………………………………………………………………………86 Copyright©2003, Audio Visual Imagineering, Inc. 2 Legends of the Night Sky: Orion Educator’s Guide Introduction It is our belief that “Legends of the Night sky: Orion” is the best multi-grade (K – 8), multi-disciplinary education package on the market today. It consists of a humorous 24-minute show and educator’s package. The Orion Educator’s Guide is designed for Planetarians, Teachers, and parents. The information is researched, organized, and laid out so that the educator need not spend hours coming up with lesson plans or labs. This has already been accomplished by certified educators. The guide is written to alleviate the fear of space and the night sky (that many elementary and middle school teachers have) when it comes to that section of the science lesson plan. It is an excellent tool that allows the parents to be a part of the learning experience. The guide is devised in such a way that there are plenty of visuals to assist the educator and student in finding the Winter constellations. -
JUDITH MERRIL-PDF-Sep23-07.Pdf (368.7Kb)
JUDITH MERRIL: AN ANNOTATED BIBLIOGRAPHY AND GUIDE Compiled by Elizabeth Cummins Department of English and Technical Communication University of Missouri-Rolla Rolla, MO 65409-0560 College Station, TX The Center for the Bibliography of Science Fiction and Fantasy December 2006 Table of Contents Preface Judith Merril Chronology A. Books B. Short Fiction C. Nonfiction D. Poetry E. Other Media F. Editorial Credits G. Secondary Sources About Elizabeth Cummins PREFACE Scope and Purpose This Judith Merril bibliography includes both primary and secondary works, arranged in categories that are suitable for her career and that are, generally, common to the other bibliographies in the Center for Bibliographic Studies in Science Fiction. Works by Merril include a variety of types and modes—pieces she wrote at Morris High School in the Bronx, newsletters and fanzines she edited; sports, westerns, and detective fiction and non-fiction published in pulp magazines up to 1950; science fiction stories, novellas, and novels; book reviews; critical essays; edited anthologies; and both audio and video recordings of her fiction and non-fiction. Works about Merill cover over six decades, beginning shortly after her first science fiction story appeared (1948) and continuing after her death (1997), and in several modes— biography, news, critical commentary, tribute, visual and audio records. This new online bibliography updates and expands the primary bibliography I published in 2001 (Elizabeth Cummins, “Bibliography of Works by Judith Merril,” Extrapolation, vol. 42, 2001). It also adds a secondary bibliography. However, the reasons for producing a research- based Merril bibliography have been the same for both publications. Published bibliographies of Merril’s work have been incomplete and often inaccurate. -
Sirius - Wikipedia Coordinates: 06 H 4 5 M 08.9 1 7 3 S, −1 6 ° 4 2 ′ 5 8.01 7 ″
12/2/2018 Sirius - Wikipedia Coordinates: 06 h 4 5 m 08.9 1 7 3 s, −1 6 ° 4 2 ′ 5 8.01 7 ″ Sirius Sirius (/ˈsɪriəs/, a romanization of Greek Σείριος, Seirios, lit. "glowing" or "scorching") is a star system Sirius A and B and the brightest star in the Earth's night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The system has the Bayer designation Alpha Canis Majoris (α CMa). What the naked eye perceives as a single star is a binary star system, consisting of a white main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, called Sirius B. The distance separating Sirius A from its companion varies between 8.2 and 31.5 AU.[24] Sirius appears bright because of its intrinsic luminosity and its proximity to Earth. At a distance of 2.6 parsecs (8.6 ly), as determined by the Hipparcos astrometry satellite,[2][25][26] the Sirius system is one of Earth's near neighbours. Sirius is gradually moving closer to the Solar System, so it will slightly increase in brightness over the next 60,000 years. After that time its distance will begin to increase and it will become fainter, but it will continue to be the brightest star in the Earth's night sky for the next 210,000 years.[27] The position of Sirius (circled). Sirius A is about twice as massive as the Sun (M☉) and has an absolute visual magnitude of 1.42. -
Transit of Venus M
National Aeronautics and Space Administration The Transit of Venus June 5/6, 2012 HD209458b (HST) The Transit of Venus June 5/6, 2012 Transit of Venus Mathof Venus Transit Top Row – Left image - Photo taken at the US Naval Math Puzzler 3 - The duration of the transit depends Observatory of the 1882 transit of Venus. Middle on the relative speeds between the fast-moving image - The cover of Harpers Weekly for 1882 Venus in its orbit and the slower-moving Earth in its showing children watching the transit of Venus. orbit. This speed difference is known to be 5.24 km/sec. If the June 5, 2012, transit lasts 24,000 Right image – Image from NASA's TRACE satellite seconds, during which time the planet moves an of the transit of Venus, June 8, 2004. angular distance of 0.17 degrees across the sun as Middle - Geometric sketches of the transit of Venus viewed from Earth, what distance between Earth and by James Ferguson on June 6, 1761 showing the Venus allows the distance traveled by Venus along its shift in the transit chords depending on the orbit to subtend the observed angle? observer's location on Earth. The parallax angle is related to the distance between Earth and Venus. Determining the Astronomical Unit Bottom – Left image - NOAA GOES-12 satellite x-ray image showing the Transit of Venus 2004. Middle Based on the calculations of Nicolas Copernicus and image – An observer of the 2004 transit of Venus Johannes Kepler, the distances of the known planets wearing NASA’s Sun-Earth Day solar glasses for from the sun could be given rather precisely in terms safe viewing. -
Title Spons Agency Bureau No Pub Date Contract Note
DOCUMENT LIZSUME ED 071' C87 82 015 524 TITLE Project Musics Reader 2,Motion in the Heavens. .INSTITUTION Harvard Univ., Cambridge,Mass. Harvard Project _Physics. SPONS AGENCY Office of Education (DREW), Washington, D.C.,Bureau of Research. BUREAU NO BK-5-1038 PUB DATE 68 CONTRACT 08C-5-10-058 NOTE 233p.; Authorized InterimVersion EDRS PRICE MF -$0.65 HC-89.87 _DESCRIPTORS Astronomy; Instructional Materials;.*Motion; *Physics; Science, Fiction;. Science Materials; _Secondary Grades; *Secondary School Science; *Space; *Supplementary Reading Materials IDENTIFIER'S Harvard Project Physics ABSTRACT As a supplement to.Projpct Physics Unit 2, specially, selected articles are presented in this reader for student browsing. _Eight excerpts are given under headings:,the starry messenger, Newton_. And the principia, an appreciation of the earth, space the unconquerable, Is there intelligent life beyond the earth3,11 the life story of a galaxy, expansion of the universe, and Dyson sphere. Seven book passages. are included under. the, headings of the black cloud, roll call, a night at the observatory, Repler's celestial music, universal gravitation, a table of stars within twenty-two light years that could have habitable planets, and three poetic _fragments about astronomy. The remaining articles includea preface to the books of the ,revolutions, Kepler, Kepler on. Mars, laws of ..motion and proposition one,, garden of Epicurus, a search for life on earth at Kilometer resolution, the. boy who redeemed his father's _name, great comet of 1965, gravity experiments, unidentified flying objects, and negative mass. Illustrations for explanationpurposes . are provided. The work of Harvard. Project Physics has been .financially supported by: the Carnegie Corporation of New York, the Ford.