IAU Executive Committee
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32Nd Saas-Fee Course 2002
IAU Executive Committee P r e s i d e n t V i c e -P r e s i d e n t s Silvia Torres-Peimbert Instituto Astronomia Franco Pacini Catherine J. Cesarsky Dpto di Astronomia UNAM Director General, ESO Apt 70 264 Universitá degli Studi Karl Schwarzschildstr. 2 Largo E. Fermi 5 Mexico DF 04510, Mexico DE 85748 Garching, Tel: 52 5 622 3906 IT 50125 Firenze, Italy Germany Tel: 39 055 27521/2232 Fax: 52 5 616 0653 Tel: 49 893 200 6227 [email protected] Fax: 39 055 22 0039 Fax: 49 893 202 362 [email protected] [email protected] Robert E. Williams P r e s i d e n t -E l e c t STScI Norio Kaifu Homewood Campus Ronald D. Ekers Director General, NAO 3700 San Martin Dr CSIRO, ATNF Osawa, Mitaka US Baltimore MD 21218 Box 76 JP Tokyo 181- 8588, Japan USA AU Epping NSW 1710 Tel: 81 422 34 3650 Tel: 1 410 338 4963 Australia Fax: 81 422 34 3690 Fax: 1 410 338 2617 Tel: 61 2 9372 4300 [email protected] [email protected] Fax: 61 2 9372 4310 [email protected] Nikolay S. Kardashev A d v i s e r s Astro Space Center G e n e r a l S e c r e t a r y Lebedev Physical Institute Robert P. Kraft (Past President) Hans Rickman Academy of Sciences Profsojuznaya ul 84/32 Lick Observatory IAU RU 117810 Moscow University of California 98 bis Blvd Arago Russian Federation US Santa Cruz CA 95064 FR 75014 Paris, France Tel: 7 095 333 2378 USA Tel: 33 1 43 25 8358 Fax: 7 095 333 2378 Fax: 1 831 426 3115 Fax: 33 1 43 25 2616 or 7 095 310 7023 [email protected] [email protected] [email protected] Johannes Andersen H o m e I n s t i t u t e Kenneth A. -
Neutron Stars: Introduction
Neutron Stars: Introduction Stephen Eikenberry 16 Jan 2018 Original Ideas - I • May 1932: James Chadwick discovers the neutron • People knew that n u clei w ere not protons only (nuclear mass >> mass of protons) • Rutherford coined the name “neutron” to describe them (thought to be p+ e- pairs) • Chadwick identifies discrete particle and shows mass is greater than p+ (by 0.1%) • Heisenberg shows that neutrons are not p+ e- pairs Original Ideas - II • Lev Landau supposedly suggested the existence of neutron stars the night he heard of neutrons • Yakovlev et al (2012) show that he in fact discussed dense stars siiltimilar to a gi ant nucl eus BEFORE neutron discovery; this was immediately adapted to “t“neutron s t”tars” Original Ideas - III • 1934: Walter Baade and Fritz Zwicky suggest that supernova eventtttts may create neutron stars • Why? • Suppg(ernovae have huge (but measured) energies • If NS form from normal stars, then the gravitational binding energy gets released • ESN ~ star … Original Ideas - IV • Late 1930s: Oppenheimer & Volkoff develop first theoretical models and calculations of neutron star structure • WldhWould have con tidbttinued, but WWII intervened (and Oppenheimer was busy with other things ) • And that is how things stood for about 30 years … Little Green Men - I • Cambridge experiment with dipole antennae to map cosmic radio sources • PI: Anthony Hewish; grad students included Jocelyn Bell Little Green Men - II • August 1967: CP 1919 discovered in the radio survey • Nov ember 1967: Bell notices pulsations at P =1.337s -
Astronomia E Astrofísica Na Plataforma Scimago Confirma Essa Tendência De Estabilização Da Quantidade De Artigo, Após Um Período De Alta Mais Intenso
UNIVERSIDADE ESTADUAL DE CAMPINAS INSTITUTO DE ESTUDOS DA LINGUAGEM LABORATÓRIO DE ESTUDOS AVANÇADOS EM JORNALISMO GIULIANA MARIA MIRANDA SANTOS DO “ASTRONOMÊS” PARA O PORTUGUÊS: a comunicação entre astrônomos e jornalistas no Brasil CAMPINAS 2015 GIULIANA MARIA MIRANDA SANTOS DO “ASTRONOMÊS” PARA O PORTUGUÊS: a comunicação entre astrônomos e jornalistas no Brasil Dissertação de mestrado apresentada ao Instituto de Estudos da Linguagem e Laboratório de Estudos Avançados em Jornalismo da Universidade Estadual de Campinas para obtenção do título de mestra em Divulgação Científica e Cultural, na área de Divulgação Científica e Cultural Orientador: Prof. Dr. Marcelo Knobel Este exemplar corresponde à versão final da dissertação defendida pela aluna. CAMPINAS 2015 Agência(s) de fomento e nº(s) de processo(s): Não se aplica. Ficha catalográfica Universidade Estadual de Campinas Biblioteca do Instituto de Estudos da Linguagem Crisllene Queiroz Custódio - CRB 8/8624 Miranda, Giuliana, 1987- M672d MirDo 'astronomês' para o português : a comunicação entre astrônomos e jornalistas no Brasil / Giuliana Maria Miranda Santos. – Campinas, SP : [s.n.], 2015. MirOrientador: Marcelo Knobel. MirDissertação (mestrado) – Universidade Estadual de Campinas, Instituto de Estudos da Linguagem. Mir1. Astronomia na comunicação de massa. 2. Comunicação de massa e linguagem. 3. Jornalismo - Brasil. 4. Divulgação científica - Brasil. 5. Pesquisadores - Brasil. 6. Jornalistas - Brasil. 7. Assessores de imprensa - Brasil. I. Knobel, Marcelo,1968-. II. Universidade Estadual -
ESO to Build World's Biggest Eye on the Sky 11 June 2012
ESO to build world's biggest eye on the sky 11 June 2012 36/) and Switzerland voted in favour of the start of the E-ELT programme. Four further countries voted in favour ad referendum: Belgium, Finland, Italy, and the United Kingdom. The remaining four Member States are actively working towards joining the programme in the near future. Following the resolution, spending on elements of the project other than the initial civil works will not commence until the contributions pledged by the Member States, as agreed in the funding principles Artist's impression of the European Extremely Large approved by Council in late 2011, exceed 90% of Telescope (E-ELT) in its enclosure on Cerro Armazones, the 1083 million euro cost-to-completion (at 2012 a 3060-metre mountaintop in Chile's Atacama Desert. The 39.3-meter E-ELT will be the largest optical/infrared prices). telescope in the world -- the world's biggest eye on the sky. Operations are planned to start early in the next On the current schedule the first large E-ELT decade, and the E-ELT will tackle some of the biggest industrial contracts would have to be approved and scientific challenges of our time. Credit: ESO/L. Calçada major funding committed within the next year. This is expected to provide sufficient time for the conditions to be satisfied: the confirmations of the votes from Belgium, Finland, Italy, and the United ESO's governing body, the Council, met today, at Kingdom; other Member States to join the project; the ESO Headquarters in Garching, Germany. -
The Specola Vaticana: Astronomy at the Vatican
Organizations, People and Strategies in Astronomy 2 (OPSA 2), 217-230 Ed. A. Heck, © 2013 Venngeist. THE SPECOLA VATICANA: ASTRONOMY AT THE VATICAN GUY CONSOLMAGNO AND CHRISTOPHER CORBALLY Specola Vaticana V-00120, Vatican City State [email protected] [email protected] Abstract. The Vatican is an independent nation, with its own national astronomical observatory, the Specola Vaticana (Vatican Observatory). As- tronomy has been supported at the Vatican since the 1582 reform of the calendar; the present-day Observatory has been in operation since 1891. The work of the observatory is divided between two sites, one in the pa- pal summer gardens south of Rome, Italy, and the other affiliated with the Steward Observatory at the University of Arizona, in Tucson, Arizona, USA. Research undertaken by current staff members ranges from cosmol- ogy and the study of galactic evolution to meteoritics and meteors. Given the stable funding provided by the Vatican, the Observatory has specialized in long-term mapping and cataloguing projects that would be difficult to mount under a traditional three-year funding cycle. These have included participation in the Carte du Ciel photographic map of the sky; the at- lases of spectra produced by its Spectrochemical Laboratory; surveys of star clusters and peculiar stars; and the cataloguing of meteorite physical properties. 1. Astronomy in the Holy See Before 1891 To the Christian church, the study of creation has long been supported as an act of worshipping the Creator. Astronomy was one of the seven subjects that made up the curriculum of the medieval universities, which were themselves founded by the Church. -
Libro Resumen Sea2016v55 0.Pdf
2 ...................................................................................................................................... 4 .................................................................................................. 4 ........................................................................................................... 4 PATROCINADORES .................................................................................................................... 5 RESUMEN PROGRAMA GENERAL ............................................................................................ 7 PLANO BIZKAIA ARETOA .......................................................................................................... 8 .......................................................................................... 9 CONFERENCIAS PLENARIAS ................................................................................................... 14 ............................................................................................. 19 ................................................................................................ 21 ............... 23 CIENCIAS PLANETARIAS ......................................................................................................... 25 - tarde ....................................................................................................... 25 - ............................................................................................ 28 - tarde ................................................................................................ -
Br Guy Consolmagno SJ Vatican Observatory L’Aigle Meteorite a Quick and Dirty Technique for Measuring Heat Capacity
Why Do We Do Science? Br Guy Consolmagno SJ Vatican Observatory L’Aigle meteorite A quick and dirty technique for measuring heat capacity 75" 73" 71" 69" 67" 65" 63" Mass$(grams)$ 61" } LN2 boil off 59" 57" 55" 600" 700" 800" 900" 1000" 1100" Time$(seconds)$ http://www.killerasteroids.org/impact.php “What do I tell my mom?” College of Charleston, Charleston, South Carolina. photo credit: Nicole, http://livinginflux.com/ Tunnel below Building 26, MIT from The Fellowship of the Ring Vivek Pancoar, skiing instructor for Adventure Trekking in Auli. © Photo: Santosh Kunwar Hacky Sack Howcast Videos: How to Play Hacky Sack How do you win this game? How do you win this game? • Approval others • Fame • Tenure • Successful students • Grant money • Cited publications • Prizes • Academic freedom Are any of these ends in themselves? Table of Contents Science 13 December 2013 How do you win this game? • Curiosity • Pleasure in solving problems • Pleasure in finding patterns • Truth • Love Are any of these ends in themselves? How do you win this game? • Approval of others • Curiosity • Tenure • Pleasure in solving problems • Grant money • Pleasure in finding patterns • Prizes • Truth • Fame • Love • Academic freedom • Successful students • Cited publications Would you sacrifice anything on list one to obtain anything on list two? How do you win this game? • Approval of others • Curiosity • Tenure • Pleasure in solving problems • Grant money • Pleasure in finding patterns • Prizes • Truth • Fame • Love • Academic freedom • Successful students • Cited publications -
Pulsars,Magnetars and Fast Radio Bursts
Pulsars,Magnetars and Fast Radio Bursts: Roger Blandford KIPAC Stanford 30 xi 2017 CPT 1 Charles Messier 30 xi 2017 CPT 2 Sam Okoye discovers compact radio source 30 xi 2017 CPT 3 Franco Pacini predicts Crab Nebula Powered by Neutron Star 30 xi 2017 CPT 4 Jocelyn Bell Discovers Pulsars 30 xi 2017 CPT 5 Neutron Stars •~10 km radius •Giant nucleus; 1057 neutrons •Magnetic field ~ 1012 Gauss •Superfluidity •Superconductivity •Thick crust •Shallow ocean 30 xi 2017 CPT 6 Crab Pulsar 30 xi 2017 CPT to 400 GeV7 ! Millisecond Pulsars • Rapidly spinning pulsars • 1 day -> 1-10 milliseconds! • Fastest 716 Hz F5# • Weak magnetic field • One has planets • Many in globular clusters • Recycled and spun up 30 xi 2017 CPT 8 Binary Pulsars •Hulse-Taylor binary pulsar •Tests of general relativity •Gravitational radiation •Double pulsar •Two pulsars; now just one •Triple pulsar •Principle of Equivalence 30 xi 2017 CPT 9 GW 170817, GBM 170817A – BNS! Binary neutron star 30 xi 2017 CPT 10 combined mass - 2.73-2.78 Msun Validated Conjectures-Discovery Space Cosmography Background Nucleosynthesis Jet formation Nuclear physics Stellar evolution Relativistic shocks GR works Tests of GR SGRB=BNS … Heavy elements Distances g-rays beamed Wave30 xi 2017speed =c CPT 11 Pulsar Timing Array •LIGO gravitational waves •Directly •Wavelengths ~ 1000 km •Timing pulsars •Wavelengths ~ light years 30 xi 2017 CPT 12 Crab Nebula Spectrum TeV Synchrotron Radiation Compton Scattering 30 xi 2017 Radio CPT Gamma Rays 13 Flaring behavior Buehler et al April 2011 Power~1029W Singular -
New Online Platforms FAITH & SCIENCE VISIT OUR NEW
PROOF BETTS PRINTING PROOF BETTS PRINTING PROOF BETTS PRINTING Fall 2017 PROOF BETTSembracing, encouraging andPRINTING promoting scientific study PROOFOnline Newsletter BETTS PRINTING Your Gift Supports Our Work! You Donate PROOFcan go Directly to our Donation BETTS PRINTING Page from Here. Thank you! The Catholic Astronomer Greetings! We hope you enjoy getting our news directly to your inbox. Please let us know what you think or if you want to change how you receive this. PROOFThank you! BETTS PRINTING Guess What The Big News is this Month - The Eclipse! From a live interview for Busted Halo on Sirius XM to a TIME Magazine article to a football stadium at Benedictine College in Atchison, Kansas, the Vatican Observatory was very busy with the Great American Eclipse. PROOFCatholic News Service wrote about Br. Guy's visit to Kentucky whileBETTS Fr. Paul Mueller PRINTING contributed to an article about how even Popes can get spooked by an eclipse. Be sure to read the fascinating Catholic Astronomer Blog articles about all our Eclipse PROOFexperiences. Take a look at some of the photos we gathered, too.BETTS PRINTING FAITH & SCIENCE The Vatican Observatory Totality Composite by Claudio Costa, a Vatican Observatory docent in Castel Fr. James Kurzynski, Catholic Astronomer Gandolfo, takenVISIT in Casper, Wyoming. OURBlogger, and hisNEW parishioners in New Online Platforms PROOFMenomonie, Wisconsin.BETTS PRINTING DIGITAL LIBRARY With the Catholic Astronomer blog and the Faith and PROOF BETTSScience libraryPRINTING the VOF is moving further into the technological world. Many of you receive our newest online item: the monthly newsletter. If you do not and would like to please go to our website, PROOF BETTSwww.vofoundation.org, PRINTING to complete the mailing list form. -
6 My Bright Abyss: Thoughts on Modern Belief 34 Why Science
EXPLORING THE INTEGRATION OF FAITH, JUSTICE, AND THE INTELLECTUAL LIFE IN JESUIT, CATHOLIC explore HIGHER EDUCATION P UBLISHED BY THE I GNATIAN C ENTER AT S ANTA C LARA U NIVERSITY SPRING 2014 VOL. 17 6 My Bright Abyss: 18 Why Is God for 34 Why Science 46 The Fragility Thoughts on Christians Good Needs God of Faith Modern Belief for Nothing? Published by the Ignatian Center for Jesuit Education at Santa Clara University SPRING 2014 EXPLORING THE INTEGRATION OF FAITH, JUSTICE, AND THE INTELLECTUAL LIFE IN JESUIT, CATHOLIC HIGHER EDUCATION Michael C. McCarthy, S.J. ’87 Executive Director Theresa Ladrigan-Whelpley Editor Elizabeth Kelley Gillogly ’93 Managing Editor Amy Kremer Gomersall ’88 Design Ignatian Center Advisory Board Margaret Taylor, Chair Katie McCormick Gerri Beasley Charles Barry Dennis McShane, M.D. Patti Boitano Russell Murphy Jim Burns Mary Nally Ternan Simon Chin Saasha Orsi 4 Dialogue and Depth: Nicole Clawson William Rewak, S.J. Michael Engh, S.J. Exploring What Good Is God? Jason Rodriguez Frederick Ferrer Richard Saso Introduction to Spring 2014 explore Javier Gonzalez Robert Scholla, S.J. Michael Hack BY THERESA LADRIGAN-WHELPLEY Gary Serda Catherine Horan-Walker Catherine Wolff Tom Kelly Michael Zampelli, S.J. Michael McCarthy, S.J. 6 My Bright Abyss: Thoughts on Modern Belief explore is published once per year by the Ignatian Center for Jesuit Education at Santa Clara University, BY CHRISTIAN WIMAN 500 El Camino Real, Santa Clara, CA 95053-0454. 408-554-6917 (tel) 408-551-7175 (fax) www.scu.edu/ignatiancenter 10 On Modern Faith: “Out of the The views expressed in explore do not necessarily represent the views of the Ignatian Center. -
Rodolfo Smiljanic
Rodolfo Smiljanic Contact address: Tel. +48 22 329 6115 Nicolaus Copernicus Astronomical Center E-mail: [email protected] Polish Academy of Sciences http://users.camk.edu.pl/rsmiljanic ul. Bartycka 18 ORCID: 0000-0003-0942-7855 00-716 Warsaw, Poland Researcher ID: A-1789-2008 Employment Since Nov. 2018 Associate Professor Dec. 2015 { Nov. 2018 Assistant Professor Dec. 2012 { Nov. 2015 Postdoctoral Researcher (100% independent research) Nicolaus Copernicus Astronomical Center Polish Academy of Sciences { Poland Oct. 2009 { Sep. 2012 ESO Fellow (75% independent research, 25% functional duties) European Southern Observatory { Germany Functional Duty: User Support Astronomer for UVES@VLT Jan. 2009 { Sep. 2009 Posdoctoral Researcher University of S~aoPaulo { Brazil Education and degrees June 2018 Habilitation Nicolaus Copernicus Astronomical Center { Poland Sep. 2006 { Nov. 2007 Visiting student at ESO { Germany Mar. 2005 { Dec. 2008 Doctor of Sciences (December 8, 2008) Mar. 2003 { Mar. 2005 Master of Sciences (March 8, 2005) University of S~aoPaulo { Brazil PhD and Master's advisor: Beatriz Barbuy Mar. 1998 { Feb. 2003 Astronomer (February 24, 2003) Federal University of Rio de Janeiro { Brazil Prizes and Awards • Sonata Bis research grant from NCN for the research project \Playing CHESS with stars: decoding the Galactic chemical enrichment history with stellar chemical abundances" (awarded in February 2020 for 5 years): 2 204 160,00 PLN • OPUS Grant from the NCN for the research project \Near-UV stellar spectroscopy: uncovering the past and building the future" (awarded in May 2019) for 3 years: 1 239 420 PLN • Financial support to organize a scientific workshop in Poland (awarded by ESO on May 2017): 5 000 EUR. -
The Fourteenth Marcel Grossmann Meeting on Recent Developments in Theoretical and Experimental General Relativity, Astrophysics
September 4, 2017 9:39 ws-procs961x669 MG-14 – Proceedings (Part D) D433 page 3372 3372 The renaissance of general relativity in Rome: Main actors, research programs and institutional structures Luisa Bonolis∗ Max Planck Institute for the History of Science, Berlin, Germany ∗E-mail: [email protected] Adele La Rana Sapienza University, Rome, Italy E-mail: [email protected] Roberto Lalli Max Planck Institute for the History of Science, Berlin, Germany E-mail: [email protected] We show that the revitalization of General Relativity (GR) in Rome during the 1960s was mainly shaped by the confluence of two different research programs centered around two authoritative figures: the first was the focusing of former Levi–Civita’s student Carlo Cattaneo on the mathematical problems of GR and the establishment of a research group in Rome; the second was sparked by the return in Italy of the astrophysicist Livio Gratton in 1960. We also argue that the material possibilities for a novel confluence between previously separated fields in the Roman environment was made possible by deep institutional changes and, especially, by the organizational choices and visions of Edoardo Amaldi who was leading the postwar reconstruction of Italian physics. Keywords: General relativity; relativistic astrophysics; Tullio Levi–Civita; Giuseppe Armellini; Enrico Fermi; Carlo Cattaneo; Edoardo Amaldi; Livio Gratton. The First Phase: The interwar period In the late 1960s, General Relativity (GR) definitely returned to the mainstream of physics, coming into focus in connection with major astrophysical discoveries and becoming an internationally visible, highly active field of research. In order to The Fourteenth Marcel Grossmann Meeting Downloaded from www.worldscientific.com better elucidate how this historical process — the so-called Renaissance of GR, as Clifford Will christened it — developed in Rome during the 1960s, it is necessary to put it in relation to the research and teaching of GR in the Roman institutional settings starting from the early 1920s.