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Soviet Steps Toward Permanent Human Presence in Space
SALYUT: Soviet Steps Toward Permanent Human Presence in Space December 1983 NTIS order #PB84-181437 Recommended Citation: SALYUT: Soviet Steps Toward Permanent Human Presence in Space–A Technical Mere- orandum (Washington, D. C.: U.S. Congress, Office of Technology Assessment, OTA- TM-STI-14, December 1983). Library of Congress Catalog Card Number 83-600624 For sale by the Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402 Foreword As the other major spacefaring nation, the Soviet Union is a subject of interest to the American people and Congress in their deliberations concerning the future of U.S. space activities. In the course of an assessment of Civilian Space Stations, the Office of Technology Assessment (OTA) has undertaken a study of the presence of Soviets in space and their Salyut space stations, in order to provide Congress with an informed view of Soviet capabilities and intentions. The major element in this technical memorandum was a workshop held at OTA in December 1982: it was the first occasion when a significant number of experts in this area of Soviet space activities had met for extended unclassified discussion. As a result of the workshop, OTA prepared this technical memorandum, “Salyut: Soviet Steps Toward Permanent Human Presence in Space. ” It has been reviewed extensively by workshop participants and others familiar with Soviet space activities. Also in December 1982, OTA wrote to the U. S. S. R.’s Ambassador to the United States Anatoliy Dobrynin, requesting any information concerning present and future Soviet space activities that the Soviet Union judged could be of value to the OTA assess- ment of civilian space stations. -
WHERE WAS MEAN SOLAR TIME FIRST ADOPTED? Simone Bianchi INAF-Osservatorio Astrofisico Di Arcetri, Largo E. Fermi, 5, 50125, Flor
WHERE WAS MEAN SOLAR TIME FIRST ADOPTED? Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: It is usually stated in the literature that Geneva was the first city to adopt mean solar time, in 1780, followed by London (or the whole of England) in 1792, Berlin in 1810 and Paris in 1816. In this short paper I will partially revise this statement, using primary references when available, and provide dates for a few other European cities. Although no exact date was found for the first public use of mean time, the primacy seems to belong to England, followed by Geneva in 1778–1779 (for horologists), Berlin in 1810, Geneva in 1821 (for public clocks), Vienna in 1823, Paris in 1826, Rome in 1847, Turin in 1849, and Milan, Bologna and Florence in 1860. Keywords: mean solar time 1 INTRODUCTION The inclination of the Earth’s axis with respect to the orbital plane and its non-uniform revolution around the Sun are reflected in the irregularity of the length of the day, when measured from two consecutive passages of the Sun on the meridian. Though known since ancient times, the uneven length of true solar days became of practical interest only after Christiaan Huygens (1629 –1695) invented the high-accuracy pendulum clock in the 1650s. For proper registration of regularly-paced clocks, it then became necessary to convert true solar time into mean solar time, obtained from the position of a fictitious mean Sun; mean solar days all having the same duration over the course of the year. -
Space Station” IMAX Film
“Space Station” IMAX Film Theme: Learning to Work, and Live, in Space The educational value of NASM Theater programming is that the stunning visual images displayed engage the interest and desire to learn in students of all ages. The programs do not substitute for an in-depth learning experience, but they do facilitate learning and provide a framework for additional study elaborations, both as part of the Museum visit and afterward. See the “Alignment with Standards” table for details regarding how “Space Station!” and its associated classroom extensions, meet specific national standards of learning. What you will see in the “Space Station” program: • How astronauts train • What it is like to live and work in Space aboard the International Space Station (ISS) Things to look for when watching “Space Station”: • Notice how quickly astronauts adapt to free fall conditions and life on the ISS • Reasons humans go to the cost, risk, and effort to work in Space • The importance of “the little things” in keeping astronauts productive so far from home Learning Elaboration While Visiting the National Air and Space Museum Perhaps the first stop to expand on your “Space Station” experience should be the Skylab Orbiting Laboratory, entered from the second floor overlooking the Space Race Gallery. Skylab was America’s first space station, launched in 1973 and visited by three different three-man crews. It fell back to Earth in 1979. The Skylab on display was the back-up for the Skylab that was launched; the Skylab program was cancelled before it was -
Part 2 Almaz, Salyut, And
Part 2 Almaz/Salyut/Mir largely concerned with assembly in 12, 1964, Chelomei called upon his Part 2 Earth orbit of a vehicle for circumlu- staff to develop a military station for Almaz, Salyut, nar flight, but also described a small two to three cosmonauts, with a station made up of independently design life of 1 to 2 years. They and Mir launched modules. Three cosmo- designed an integrated system: a nauts were to reach the station single-launch space station dubbed aboard a manned transport spacecraft Almaz (“diamond”) and a Transport called Siber (or Sever) (“north”), Logistics Spacecraft (Russian 2.1 Overview shown in figure 2-2. They would acronym TKS) for reaching it (see live in a habitation module and section 3.3). Chelomei’s three-stage Figure 2-1 is a space station family observe Earth from a “science- Proton booster would launch them tree depicting the evolutionary package” module. Korolev’s Vostok both. Almaz was to be equipped relationships described in this rocket (a converted ICBM) was with a crew capsule, radar remote- section. tapped to launch both Siber and the sensing apparatus for imaging the station modules. In 1965, Korolev Earth’s surface, cameras, two reentry 2.1.1 Early Concepts (1903, proposed a 90-ton space station to be capsules for returning data to Earth, 1962) launched by the N-1 rocket. It was and an antiaircraft cannon to defend to have had a docking module with against American attack.5 An ports for four Soyuz spacecraft.2, 3 interdepartmental commission The space station concept is very old approved the system in 1967. -
Outlook for Rapid Expansion of Soviet Space Programs Through 1986
----~t---------------------------------- COS183190 SECRET ~ Directorate of -Seeret ii' "1-) Intelligence \lcr_J l· Withheld under statutory authority of the ~ Central Intelligence Agency Act of1!'4!) (SO U.S.C., section 3507) DECLASSIFIED UNDER AUTHORITY OF THE INTERAGENCY SECURITY CLASSIFICATION APPEALS PANEL, E.O. 13526, SECTION 5.~.(b)(3) ISCAP APPEAL NO. 2012-064, document no. 1 DECLASSIFICATION DATE: September 6, 2019 J Outlook for Rapid Expansion, of Soviet Space .Programs Through 1986 (u) An Intelligence Assessment .. f J Secret \ SOY82-l01SS Octo~r 1982 . ' C0~183190 SECRET Warning Notice Intelligence Sources or Methods Involved (WNINTEL) National Security Unauthorized Disclosure Information Subject to Criminal Sanctions ,I Dissemination Control NOFORN (NF) . Not releasable to foreign nationals Abbmiations NOCONTRACT (NC) Nol releasable to contractors or contractor/cpnsultants PROPIN(PR) Caution-proprietary information involved ORCON(OC) Dissemination and extraction of information controlled by originator REL...:...__________Th_i_s_infi_o_r_m_a_ti_o_n_h_as_b_c_c_n_a_ut_h_o_ri_zc_d_fi_o_r_re_le_as_c_to_.•_.____ FGI Foreign government information· WN WNINTEL-lntelligencesources or methods involved A microfiche copy of this docu ment is available from OCR/ DLI, I CZ printed copies ·fromCPAS/IM, ·ff -----------~ Regular receipt of DDI_ Withheld under stotutory authority ortho Centrnl lntelllgenco Agency Act or 1949 (SO reports in either microfiche u.s.c.,sectlon 3507) or printed form can also be arranged Lbrough CPAS/IMC. '-·------- All material on this page is Unclassified. I SECRET Directorate of Seeret Intelligence WithbeJd under H~lutOJ')' a1dhority ofthe "'''"Ctatr.:.1 lnttW:en« Age,u:, Act Gf 1949 (SO u.s.c. mt!oa JSO'I) Outlook for Rapid Expansion of Soviet ·Space Programs Through 1986 (u) An Intelligence Assessment The author of this paper is of the Aerospace Industries Branch, Office of Soviet Will1hold under statutory aull,oril)' or tltc Analysis. -
13 Astronomical Molecular Spectroscopy Timothy W
j377 13 Astronomical Molecular Spectroscopy Timothy W. Schmidt 13.1 The Giants Shoulders Stargazing, in its most primitive form, has entertained our species for hundreds of thousands of years. The ancients used knowledge of the positions of fixed stars as navigational aids and also recognized wandering stars (planets), comets, and novae. The astrolabe, an instrument for fixing the positions of stars, was invented in Greece some 2200 years ago. In medieval times, the positions of stars were of great importance to the Islamic world to indicate the correct times for prayer and the direction of Mecca, and the astrolabe was an important tool. Indeed, one of the 1) greatest observational astronomers, Tycho Brahe, performed his measurements without a telescope. He used a great mural quadrant, whereby stars were sighted through a slot in a wall with a tool attached to a 90 arc. Accurate measurements of the positions of stars and planets were made in this way, and they remained the most accurate until the introduction of well-built telescopes. Brahe died in 1601, passing 2) his legacy to Johannes Kepler, who had joined him as an assistant only a year before. Kepler continued to work with Brahes observations for a decade, during which he developed the laws of planetary motion for which he is most famous, and advanced 3) theories on geometric optics. Kepler was a contemporary of Galileo, who is credited with the development and improvement of the refractive telescope. Galileo observed the four largest moons of Jupiter and described the phases of Venus as being similar 4) to the Earths moon. -
Testo Completo
Università degli Studi di Ferrara DOTTORATO DI RICERCA IN "MATEMATICA E INFORMATICA" CICLO XXVI COORDINATORE Prof. Mella Massimiliano L’INTERNAZIONALIZZAZIONE DEGLI STUDI MATEMATICI IN ITALIA A METÀ OTTOCENTO Settore Scientifico Disciplinare MAT / 04 Dottorando Tutore Dott. Nagliati Iolanda Prof. Borgato Maria Teresa ________________________ ___________________________ (firma) (firma) Anni 2011/2013 1 1 L’internazionalizzazione degli studi matematici in Italia a metà Ottocento Introduction p. 3 Introduzione 17 L’internazionalizzazione degli studi 21 I rapporti di Betti con studiosi stranieri: temi delle lettere Corrispondenti stranieri di Brioschi Corrispondenti stranieri di Tardy La situazione degli esuli: Mossotti da Corfù a Pisa 43 Il ritorno dall’esilio I primi anni dell’attività a Pisa e i rapporti con Betti Vicende politiche, organizzazione degli studi e della ricerca nella corrispondenza tra Brioschi e Tardy 59 L’organizzazione degli studi superiori Gli “Annali” Le equazioni algebriche di quinto grado 73 La teoria degli invarianti 81 Ricerche sui differenziali ad indice fratto 99 Le riviste scientifiche toscane nell’Ottocento 109 Documenti: Lettere di Giorgini a Mossotti 127 Lettere di Mossotti a Tardy 135 Lettere di Mossotti a Betti 139 Carteggio Brioschi-Tardy 191 Lettere a Betti di studiosi stranieri 285 Lettere a Tardy di studiosi stranieri 342 Lettere a Brioschi di studiosi stranieri 369 Bibliografia 371 1 2 Introduction The past few decades have seen several studies carried out by historians of mathematics on mathematics in the post unification period in Italy, further interest being recently stimulated by the celebration of 150 years since the Unification of Italy; this moment brought about a period of renewal of structures and infrastructures suitable for the new state, a sort of modernisation of the economy, which, at the same time, required a new institutional organisation on a national level for the scientific community, to carry on the work already started in the previous decades by single states, like Piedmont and the Grand Duchy of Tuscany. -
1 the Founding of Arcetri Observatory in Florence
THE FOUNDING OF ARCETRI OBSERVATORY IN FLORENCE Simone Bianchi INAF-Osservatorio Astrofisico di Arcetri, Largo E. Fermi, 5, 50125, Florence, Italy [email protected] Abstract: The first idea of establishing a public astronomical observatory in Florence, Capital of the Grand Duchy of Tuscany, dates to the mid of the 18th century. Initially, the use of a low building on a high ground was proposed, and the hill of Arcetri suggested as a proper location. At the end of the century, the Florence Observatory - or Specola - was built instead on a tower at the same level as the city’s centre. As soon as astronomers started to use this observatory, they recognized all its flaws and struggled to search for a better location. Giovanni Battista Donati, director of the Specola of Florence from the eve of the Italian Unification in 1859, finally succeeded in creating a new observatory: first, he obtained funds from the Parliament of the Kingdom of Italy to build an equatorial mount for the Amici 28-cm refractor, which could not be installed conveniently in the tower of the Specola; then, he went through the process of selecting a proper site, seeking funds and finally building Arcetri Observatory. Although Donati was a pioneer of spectroscopy and astrophysics, his intent was to establish a modern observatory for classical astronomy, as the Italian peninsula did not have a national observatory like those located in many foreign capitals – Florence was the capital of the Kingdom of Italy from 1865 to 1871. To promote the project, Donati made use of writings by one of the most authoritative European astronomers, Otto Wilhelm Struve. -
Jjmonl 1606.Pmd
alactic Observer GJohn J. McCarthy Observatory Volume 9, No. 6 June 2016 Dead End? Conventional wisdom has long held that galaxies regenerate from the gas and debris of their own dead stars. Find out why that isn't always true - inside, page 15 http://www.mccarthyobservatory.org June 2016 • 1 The John J. McCarthy Observatory Galactic Observvvererer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky It is through their efforts that the McCarthy Observatory Technical Support has established itself as a significant educational and Bob Lambert recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Mike Chiarella Roger Moore Route Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Cecilia Dietrich Marc Polansky Dirk Feather Joe Privitera Randy Fender Monty Robson Randy Finden Don Ross John Gebauer Gene Schilling Elaine Green Katie Shusdock Tina Hartzell Paul Woodell Tom Heydenburg Amy Ziffer In This Issue OUT THE WINDOW ON YOUR LEFT .................................... 4 ASTRONOMICAL AND HISTORICAL EVENTS ......................... 12 SURVEYOR 1 LANDING SITE .............................................. 4 COMMONLY USED TERMS ............................................... 14 2016 MERCURY TRANSIT -
Icons on the International Space Station
religions Article Eternity in Low Earth Orbit: Icons on the International Space Station Wendy Salmond 1, Justin Walsh 1 and Alice Gorman 2,* 1 Department of Art, Chapman University, Orange, CA 92866, USA; [email protected] (W.S.); [email protected] (J.W.) 2 Department of Archaeology, Flinders University, Bedford Park, SA 5042, Australia * Correspondence: alice.gorman@flinders.edu.au Received: 15 October 2020; Accepted: 10 November 2020; Published: 17 November 2020 Abstract: This paper investigates the material culture of icons on the International Space Station as part of a complex web of interactions between cosmonauts and the Russian Orthodox Church, reflecting contemporary terrestrial political and social affairs. An analysis of photographs from the International Space Station (ISS) demonstrated that a particular area of the Zvezda module is used for the display of icons, both Orthodox and secular, including the Mother of God of Kazan and Yuri Gagarin. The Orthodox icons are frequently sent to space and returned to Earth at the request of church clerics. In this process, the icons become part of an economy of belief that spans Earth and space. This practice stands in contrast to the prohibition against displaying political/religious imagery in the U.S.-controlled modules of ISS. The icons mark certain areas of ISS as bounded sacred spaces or hierotopies, separated from the limitless outer space beyond the space station walls. Keywords: International Space Station; iconography; hierotopy; material culture; sacred space; cosmonaut 1. Introduction How the perspective of being outside the world—that is, in space—changes personal approaches to spirituality among space travelers has been the subject of numerous studies (e.g., Suedfeld 2006; Weibel 2016, 2020; Weibel and Swanson 2006). -
The Worldwide Impact of Donati's Comet on Art and Society in the Mid
The Rˆole of Astronomy in Society and Culture Proceedings IAU Symposium No. 260, 2011 c 2011 International Astronomical Union D. Valls-Gabaud & A. Boksenberg, eds. DOI: 00.0000/X000000000000000X The worldwide impact of Donati’s comet on art and society in the mid-19th century Antonella Gasperini1, Daniele Galli1 and Laura Nenzi2 1 INAF–Osservatorio Astrofisico di Arcetri, Firenze, Italy email: gasperi,[email protected] 2 University of Tennessee, Knoxville, USA email: [email protected] Abstract. Donati’s comet was one of the most impressive astronomical events of the nineteenth century. Its extended sword-like tail was a spectacular sight that inspired several literary and artistic representations. Traces of Donati’s comet are found in popular magazines, children’s books, collection cards, and household objects through the beginning of the twentieth century. Keywords. Donati’s comet, 19th century literature and art 1. Introduction Donati’s comet was discovered in Florence on June 2, 1858. It became visible to the naked eye in the northern and southern hemispheres between September 1858 and March 1859. Its gracefully curved tail, which extended almost 40 degrees in the southwestern sky, made a great visual impact and inspired several pictorial (paintings, watercolours, sketches) and poetic (lyrical and satirical) representations, especially in Great Britain and France. In the Eastern world, the influence of Donati’s comet on contemporary society is particularly significant in Siam and Japan. This contribution outlines the relations and interconnections between a scientific discovery, the artistic movements of the period, and the different social environments in a worldwide context. 2. The discoverer, Giovanni Battista Donati Giovanni Battista Donati was born in Pisa in 1826 and studied physics and mathemat- ics at the local University under the guidance of O. -
Introduction
Cambridge University Press 978-1-107-00229-6 - Unravelling Starlight: William and Margaret Huggins and the Rise of the New Astronomy Barbara J. Becker Excerpt More information 1 Introduction where in the murky depths of mind do idea-seeds sleep? what seasons do they know that make them wont to wake and grow in spasms – madly now, dormant then – entangling all within their ken: synaptic vines to clamber to the very stars. My interest in the life and work of English astronomer William Huggins (1824–1910) began over twenty years ago in a graduate seminar on conceptual transfer within and among specialised scientific communities. The exchange of cultural baggage is a subtle dynamic that practitioners, particularly those working in long-established disciplines, usually take care to shield from public view. Our little group spent the semester analysing the far more transparent machinery of newer, still-developing hybrid disciplines like geophysics, bio- chemistry and astrobiology. The topic meshed well with my own research interests at the time. I wanted to learn more about how the boundaries of scientific disciplines are established, policed and altered: What are the rules members must follow in investigating the natural world? What questions are deemed appropriate to ask? What do good answers to such questions look like and how can they be recognised? What constitutes an acceptable way of finding those answers? Who is allowed to participate in the search? Who says? How better to find answers to these questions than to watch a scientific discipline during a period of change? I chose to explore the origins of astrophysics, a mature hybrid science that blends the methods, instruments and theories of chemistry and physics, as well as those of both mathematical and descriptive astronomy.