ASTRONOMICAL JOURNEYS Diffusion and Socialization of the Knowledge of the Sky
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
General Vertical Files Anderson Reading Room Center for Southwest Research Zimmerman Library
“A” – biographical Abiquiu, NM GUIDE TO THE GENERAL VERTICAL FILES ANDERSON READING ROOM CENTER FOR SOUTHWEST RESEARCH ZIMMERMAN LIBRARY (See UNM Archives Vertical Files http://rmoa.unm.edu/docviewer.php?docId=nmuunmverticalfiles.xml) FOLDER HEADINGS “A” – biographical Alpha folders contain clippings about various misc. individuals, artists, writers, etc, whose names begin with “A.” Alpha folders exist for most letters of the alphabet. Abbey, Edward – author Abeita, Jim – artist – Navajo Abell, Bertha M. – first Anglo born near Albuquerque Abeyta / Abeita – biographical information of people with this surname Abeyta, Tony – painter - Navajo Abiquiu, NM – General – Catholic – Christ in the Desert Monastery – Dam and Reservoir Abo Pass - history. See also Salinas National Monument Abousleman – biographical information of people with this surname Afghanistan War – NM – See also Iraq War Abousleman – biographical information of people with this surname Abrams, Jonathan – art collector Abreu, Margaret Silva – author: Hispanic, folklore, foods Abruzzo, Ben – balloonist. See also Ballooning, Albuquerque Balloon Fiesta Acequias – ditches (canoas, ground wáter, surface wáter, puming, water rights (See also Land Grants; Rio Grande Valley; Water; and Santa Fe - Acequia Madre) Acequias – Albuquerque, map 2005-2006 – ditch system in city Acequias – Colorado (San Luis) Ackerman, Mae N. – Masonic leader Acoma Pueblo - Sky City. See also Indian gaming. See also Pueblos – General; and Onate, Juan de Acuff, Mark – newspaper editor – NM Independent and -
Program and Abstracts of 2017 Congress / Programme Et Résumés
1 Sponsors | Commanditaires Gold Sponsors | Commanditaires d’or Silver Sponsors | Commanditaires d’argent Other Sponsors | Les autres Commanditaires 2 Contents Sponsors | Commanditaires .......................................................................................................................... 2 Welcome from the Premier of Ontario .......................................................................................................... 5 Bienvenue du premier ministre de l'Ontario .................................................................................................. 6 Welcome from the Mayor of Toronto ............................................................................................................ 7 Mot de bienvenue du maire de Toronto ........................................................................................................ 8 Welcome from the Minister of Fisheries, Oceans and the Canadian Coast Guard ...................................... 9 Mot de bienvenue de ministre des Pêches, des Océans et de la Garde côtière canadienne .................... 10 Welcome from the Minister of Environment and Climate Change .............................................................. 11 Mot de bienvenue du Ministre d’Environnement et Changement climatique Canada ................................ 12 Welcome from the President of the Canadian Meteorological and Oceanographic Society ...................... 13 Mot de bienvenue du président de la Société canadienne de météorologie et d’océanographie ............. -
Exercise E1: Finding Your Way Around the Sky
E – Star Finding Exercise E1: Finding Your Way Around the Sky Student name: ________________________ Class: ____________ Date: _____________ Check the box with the correct answer. Question 1: What is the orientation of the Big Dipper asterism in winter? a. It appears upside down. b. It sits with its handle downwards. c. It appears to sit upright, resting upon its bowl. d. The Big Dipper is not visible in the winter. Question 2: Polaris is part of which constellation? (Hint: Select Constellations from the Settings view to display IAU Boundaries and Show Names). a. Cepheus b. Draco c. Ursa Minor d. Ursa Major Question 3: What happens to the position of Polaris in your sky as time advances over a period of a year? a. It remains absolutely fixed, and does not change its position. b. The north celestial pole revolves about Polaris. c. It revolves in a very small circle around the north celestial pole. d. Its altitude changes by + and - 23.5 degrees throughout the year because of the tilt of the Earth's spin axis. Starry Night College Version 7 1 Question 4: What is the relationship between the altitude of Polaris and the latitude of the observer? a. There is no relationship between these two parameters. b. The altitude of Polaris is almost the same as the latitude of the observer. c. The altitude of Polaris is almost the equal to 90 degrees minus the latitude of the observer. d. The latitude equals the altitude of Polaris minus the altitude of the North celestial Pole. Question 5: What is the nearest star to the south celestial pole, as shown in the Main Window? (Hint: Use the Search facility to locate these stars and zoom in towards the SCP. -
A Needs Analysis Study of Amateur Astronomers for the National Virtual Observatory : Aaron Price1 Lou Cohen1 Janet Mattei1 Nahide Craig2
A Needs Analysis Study of Amateur Astronomers For the National Virtual Observatory : Aaron Price1 Lou Cohen1 Janet Mattei1 Nahide Craig2 1Clinton B. Ford Astronomical Data & Research Center American Association of Variable Star Observers 25 Birch St, Cambridge MA 02138 2Space Sciences Laboratory University of California, Berkeley 7 Gauss Way Berkeley, CA 94720-7450 Abstract Through a combination of qualitative and quantitative processes, a survey was con- ducted of the amateur astronomy community to identify outstanding needs which the National Virtual Observatory (NVO) could fulfill. This is the final report of that project, which was conducted by The American Association of Variable Star Observers (AAVSO) on behalf of the SEGway Project at the Center for Science Educations @ Space Sci- ences Laboratory, UC Berkeley. Background The American Association of Variable Star Observers (AAVSO) has worked on behalf of the SEGway Project at the Center for Science Educations @ Space Sciences Labo- ratory, UC Berkeley, to conduct a needs analysis study of the amateur astronomy com- munity. The goal of the study is to identify outstanding needs in the amateur community which the National Virtual Observatory (NVO) project can fulfill. The AAVSO is a non-profit, independent organization dedicated to the study of vari- able stars. It was founded in 1911 and currently has a database of over 11 million vari- able star observations, the vast majority of which were made by amateur astronomers. The AAVSO has a rich history and extensive experience working with amateur astrono- mers and specifically in fostering amateur-professional collaboration. AAVSO Director Dr. Janet Mattei headed the team assembled by the AAVSO. -
Flaming Star the Flaming Star Nebula (IC 405) in the Constellation Auriga Is a Surprisingly Colorful and Dramatic Emission/Reflection Nebula
WESTCHESTER AMATEUR ASTRONOMERS January 2016 Image Copyright: Mauri Rosenthal Flaming Star The Flaming Star Nebula (IC 405) in the constellation Auriga is a surprisingly colorful and dramatic emission/reflection nebula. In This Issue . The most prominent star in the image is the variable blue dwarf AE pg. 2 Events For January Aurigae, burning with sufficient intensity to knock electrons off pg. 3 Almanac the hydrogen molecules found in a cloud 5 light years across, pg. 4 Vivian Towers which in turn emit red light. The bluish gray area is not from ion- pg. 5 The Radio Sky ized Oxygen (as found in the Veil Nebula); rather it is mostly a pg. 11 Kepler cloud of carbon dust, which reflects the blue light from the nearby pg. 12 President’s Report star. The result is an emission/reflection nebula 1500 light years distant and accessible from the suburbs with a small telescope. Mauri Rosenthal imaged this from his backyard in Scarsdale with a guided Questar 3.5” telescope over two nights in November using CLS (broadband) and H-alpha (narrowband) filters. Total exposure time was 9.5 hours. SERVING THE ASTRONOMY COMMUNITY SINCE 1986 1 WESTCHESTER AMATEUR ASTRONOMERS January 2016 WAA January Lecture Club Dates 2016 “Light Pollution” Friday January 8th, 7:30pm 2016 Lecture Dates Leinhard Lecture Hall, January 8 June 3 February 5 Sept. 16 Pace University, Pleasantville, NY March 4 October 7 Charles Fulco will speak on light pollution, the Inter- April 1 November 4 national Dark-Sky Association and preserving our May 6 December 2 night sky. -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
Evidence of Shock Metamorphism Effects in Allochthonous Breccia Deposits from the Colônia Crater, São Paulo, Brazil
International Journal of Geosciences, 2013, 4, 274-282 http://dx.doi.org/10.4236/ijg.2013.41A025 Published Online January 2013 (http://www.scirp.org/journal/ijg) Evidence of Shock Metamorphism Effects in Allochthonous Breccia Deposits from the Colônia Crater, São Paulo, Brazil Victor F. Velázquez1, Claudio Riccomini2, José M. Azevedo Sobrinho3, Mikhaela A. J. S. Pletsch1, Alethéa E. Martins Sallun3, William Sallun Filho3, Jorge Hachiro2 1Escola de Artes, Ciências e Humanidades, Universidade de São Paulo, São Paulo, Brasil 2Instituto de Geociências, Universidade de São Paulo, São Paulo, Brasil 3Instituto Geológico, Secretaria do Meio Ambiente, São Paulo, Brasil Email: [email protected] Received October 16, 2012; revised November 17, 2012; accepted December 19, 2012 ABSTRACT The 3.6 km-diameter Colônia impact crater, centred at 23˚52'03"S and 46˚42'27"W, lies 40 km to the south-west of the São Paulo city. The structure was formed on the crystalline basement rocks and displays a bowl-shaped with steeper slope near the top that decreases gently toward the centre of the crater. Over recent years were drilled two boreholes inside the crater, which reached a maximum depth of 142 m and 197 m. Geological profile suggests four different lithological associations: 1) unshocked crystalline basement rocks (197 - 140 m); 2) fractured/brecciated basement rocks (140 - 110 m); 3) polymictic allochthonous breccia deposits (110 - 40 m); and 4) post-impact deposits (40 - 0 m). Petrographic characterisation of the polymictic allochthonous breccia reveals a series of distinctive shock-metamorphic features, including, among others, planar deformation features in quartz, feldspar and mica, ballen silica, granular tex- ture in zircon and melt-bearing impact rocks. -
Instruction Manual Meade Instruments Corporation
Instruction Manual 7" LX200 Maksutov-Cassegrain Telescope 8", 10", and 12" LX200 Schmidt-Cassegrain Telescopes Meade Instruments Corporation NOTE: Instructions for the use of optional accessories are not included in this manual. For details in this regard, see the Meade General Catalog. (2) (1) (1) (2) Ray (2) 1/2° Ray (1) 8.218" (2) 8.016" (1) 8.0" Secondary 8.0" Mirror Focal Plane Secondary Primary Baffle Tube Baffle Field Stops Correcting Primary Mirror Plate The Meade Schmidt-Cassegrain Optical System (Diagram not to scale) In the Schmidt-Cassegrain design of the Meade 8", 10", and 12" models, light enters from the right, passes through a thin lens with 2-sided aspheric correction (“correcting plate”), proceeds to a spherical primary mirror, and then to a convex aspheric secondary mirror. The convex secondary mirror multiplies the effective focal length of the primary mirror and results in a focus at the focal plane, with light passing through a central perforation in the primary mirror. The 8", 10", and 12" models include oversize 8.25", 10.375" and 12.375" primary mirrors, respectively, yielding fully illuminated fields- of-view significantly wider than is possible with standard-size primary mirrors. Note that light ray (2) in the figure would be lost entirely, except for the oversize primary. It is this phenomenon which results in Meade 8", 10", and 12" Schmidt-Cassegrains having off-axis field illuminations 10% greater, aperture-for-aperture, than other Schmidt-Cassegrains utilizing standard-size primary mirrors. The optical design of the 4" Model 2045D is almost identical but does not include an oversize primary, since the effect in this case is small. -
Celestial Gymnastics # 02
PLANETARIUM EDUCATIONTM (Class Test) 9A Celestial Gymnastics # 02 www.leoplanetaria.com 9A Celestial Gymnastics 02 Max. Duration: 00min Max. Marks: 00 Date:____/____/______ TM Name: _______________________________ Class: ______ Sec: ________ Roll No:______ TM Planetarium Education www.leoplanetaria.com Tick (þ) mark the correct answer or fill in the blank. 1. The obvious choice reference of a central circle on a rotating ball’s surface as a starting or zero reference point of its latitudes is (A) North pole (B) South pole (C) Equator (D) Prime meridian 2. Which of the following point on the surface of a rotating ball when viewed from space is called its North Pole? (A) (B) 3. Which of the following diagram from a vantage point from where you have a bird’s eye view of the solar system is correct? (A) (B) 4. From where on the Earth over a period of one year you can see the entire celestial sphere – you would miss no star, no planet or any other object of the sky. (A) North pole (B) South pole (C) Equator (D) Prime meridian 5. Which constellation helps you find the pole star of the southern hemisphere of the Earth? (A) Crux (B) Ursa Major (C) Orion (D) Ursa Minor 6. The height of the pole star in our skies as we move from equator towards the poles... (A) Increases (B) Decreases (C) Remains unchanged 7. Prime Meridian passes through... (A) Allahabad (B) London (C) New York (D) Paris 8. Who laid the laws of motion for celestial bodies in space? (A) Kepler (B) Newton (C) Galileo (D) Copernicus Pg 1/3 C Leo Planetaria Astronomy Education Pvt. -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Catalogues Par Titres-Textes Janvier 2009
fonds documentaire-NTA TEXTES classement au 15/01/2009 Classement par titre Titre texte Nom Auteur texte Prénom Adaption / doublon/ Titre du Année NB Textes / Nature Auteur texte Titre original Edition Collection N° coll p. Traduction quantité regroupement Edition document objet Trauma ABBOTT Jeff Cherche midi (le) Livre de 2006 506 Texte poche Reflet de Sam (le) ABIER Gilles Actes Sud - Heyoka 2002 46 1 Texte Papiers Jeunesse Jésus, Marie, Joseph! ABSOUS/ Philippe/ ABS éditions 17 Texte BEAUFILS/ BONNE/ Emmanuel/ CHEVROT/ Françoise/ DESGAGNE/ Michelle/ LAGUENS/ MARTIN Richard/ J-P./ Pascal Botte et sa chaussette ACHTERNBUSCH Herbert Der Stiefel und Fix René L'Arche 1994 2 Texte (la) sein Socken Ella ACHTERNBUSCH Herbert Ella Yersin Claude Botte et sa L'Arche 1994 3 Texte chaussette (la) / Ella / Susn Gust ACHTERNBUSCH Herbert 2 version papier Texte Gust ACHTERNBUSCH Herbert Gust Yersin Claude L'Arche 1984 61 1 Texte Sintflut ACHTERNBUSCH Herbert Theater Suhrkamp 1298 1986 13_64 7 Texte Susn ACHTERNBUSCH Herbert Susn Yersin Claude Botte et sa L'Arche 1994 3 Texte chaussette (la) / Ella / Susn Son du ciel austral (le) ACWORTH Elaine Composing Famchon (I.) 2 T.ACW 182 1122 Lansman Découverte 3 1995 77 1 Texte Venus du Théâtre australien Baye (la) ADRIEN Philippe Gourmandise Version papier 1967 2 Texte Ces feuilles de ma AHMED THIAM Thierno Funérailles d'un SEPIA 1994 255 14 Texte pauvritude cochon et 13 autres nouvelles Tac-tic à la rue des AKAKPO Gustave 4 petites comédies Lansman / 2004 7_16 4 Texte Pingouins pour une Comédie Comédie de vol. 2 Saint-Etienne Scènes de comédie ALAIN Avant-scène Avant-scène théâtre 188 1959 38_40 2 Texte théâtre (l') Page 1 fonds documentaire-NTA TEXTES classement au 15/01/2009 Classement par titre Nb Nb Nb Nb Genre Résumé Langue Nationalité Public Niveau Age Figurants pers H F Enfant roman Théâtre Parce que Sam est expulsé de l'école, il doit rester chez sa grand-mère. -
Who Actually Invented the Astronomical Telescope?
The International Year of Astronomy Vision To help the citizens of the world rediscover their place in the Universe through the day and night time sky, and thereby engage a personal sense of wonder and discovery. Celebration A global celebration of astronomy and its contributions to society and culture, highlighted by the 400th anniversary of the first use of an astronomical telescope by Galileo. Goals & Objectives Increase scientific awareness. Promote widespread access to new knowledge and observing experiences. Empower astronomical communities in developing countries. Support and improve formal and informal science education. Provide a modern image of science and scientists. Facilitate new networks and strengthen existing ones. Improve the gender-balanced representation of scientists at all levels and promote greater involvement by underrepresented minorities in scientific and engineering careers. Facilitate the preservation and protection of the world’s cultural and natural heritage of dark skies and historical astronomical sites. Organisational Structure IAU President: Catherine Cesarsky IAU General Secretary: Karel van der Hucht Chair: Catherine Cesarsky Secretary: Lars Lindberg Christensen Coordinator: Pedro Russo Organisational Current Status (203 days to go…) 118 National Nodes / Aim: 140 Nations 64 National Websites 20 Organisational Nodes 16 Organisational Associates 11 Cornerstone Projects 2 Special Projects 11 Special Task Groups 100 Hours of Astronomy • 100 Hours of Astronomy Global Cornerstone Project • Task group co-chairs: