Preserving and Sharing the Italian Astronomical Heritage
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Demoting Pluto Presentation
WWhhaatt HHaappppeenneedd ttoo PPlluuttoo??!!!! Scale in the Solar System, New Discoveries, and the Nature of Science Mary L. Urquhart, Ph.D. Department of Science/Mathematics Education Marc Hairston, Ph.D. William B. Hanson Center for Space Sciences FFrroomm NNiinnee ttoo EEiigghhtt?? On August 24th Pluto was reclassified by the International Astronomical Union (IAU) as a “dwarf planet”. So what happens to “My Very Educated Mother Just Served Us Nine Pizzas”? OOffifficciiaall IAIAUU DDeefifinniittiioonn A planet: (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighborhood around its orbit. A dwarf planet must satisfy only the first two criteria. WWhhaatt iiss SScciieennccee?? National Science Education Standards (National Research Council, 1996) “…science reflects its history and is an ongoing, changing enterprise.” BBeeyyoonndd MMnneemmoonniiccss Science is “ not a collection of facts but an ongoing process, with continual revisions and refinements of concepts necessary in order to arrive at the best current views of the Universe.” - American Astronomical Society AA BBiitt ooff HHiiststoorryy • How have planets been historically defined? • Has a planet ever been demoted before? Planet (from Greek “planetes” meaning wanderer) This was the first definition of “planet” planet Latin English Spanish Italian French Sun Solis Sunday domingo domenica dimanche Moon Lunae Monday lunes lunedì lundi Mars Martis -
The First Discovery of an Aster Astronomer Giuseppe Piazzi in St
DISCOVERYDOM OF THE MONTHEDITORIAL 27(96), January 1, 2015 ISSN 2278–5469 EISSN 2278–5450 Discovery The first discovery of an asteroid, Ceres by Italian astronomer Giuseppe Piazzi in January 1, 1801 Brindha V *Correspondence to: E-mail: [email protected] Publication History Received: 04 November 2014 Accepted: 01 December 2014 Published: 1 January 2015 Citation Brindha V. The first discovery of an asteroid, Ceres by Italian astronomer Giuseppe Piazzi in January 1, 1801. Discovery, 2015, 27(96), 1 Publication License This work is licensed under a Creative Commons Attribution 4.0 International License. General Note Article is recommended to print as color digital version in recycled paper. Ceres was the first object considered to be an asteroid. The first asteroid discovered was 1 Ceres, or Ceres on January 1, 1801, by Giuseppe Piazzi a monk and astronomer in Sicily. It was classified as a planet for a long time and is considered a dwarf planet later. Asteroids are small, airless rocky worlds revolving around the sun that are too small to be called planets. They are also known as planetoids or minor planets. Ceres is the closest dwarf planet to the Sun and is located in the asteroid belt making it the only dwarf planet in the inner solar system. Ceres rotates on its axis every 9 hours and 4 minutes. In 2006, the International Astronomical Union voted to restore the planet designation to Ceres, decreeing that it qualifies as a dwarf planet. It does have some planet-like characteristics, including an interior that is separated into crust, mantle and core. -
Dwarf Planet Ceres
Dwarf Planet Ceres drishtiias.com/printpdf/dwarf-planet-ceres Why in News As per the data collected by NASA’s Dawn spacecraft, dwarf planet Ceres reportedly has salty water underground. Dawn (2007-18) was a mission to the two most massive bodies in the main asteroid belt - Vesta and Ceres. Key Points 1/3 Latest Findings: The scientists have given Ceres the status of an “ocean world” as it has a big reservoir of salty water underneath its frigid surface. This has led to an increased interest of scientists that the dwarf planet was maybe habitable or has the potential to be. Ocean Worlds is a term for ‘Water in the Solar System and Beyond’. The salty water originated in a brine reservoir spread hundreds of miles and about 40 km beneath the surface of the Ceres. Further, there is an evidence that Ceres remains geologically active with cryovolcanism - volcanoes oozing icy material. Instead of molten rock, cryovolcanoes or salty-mud volcanoes release frigid, salty water sometimes mixed with mud. Subsurface Oceans on other Celestial Bodies: Jupiter’s moon Europa, Saturn’s moon Enceladus, Neptune’s moon Triton, and the dwarf planet Pluto. This provides scientists a means to understand the history of the solar system. Ceres: It is the largest object in the asteroid belt between Mars and Jupiter. It was the first member of the asteroid belt to be discovered when Giuseppe Piazzi spotted it in 1801. It is the only dwarf planet located in the inner solar system (includes planets Mercury, Venus, Earth and Mars). Scientists classified it as a dwarf planet in 2006. -
Historical & Cultural Astronomy
Historical & Cultural Astronomy Series Editor: WAYNE ORCHISTON, University of Southern Queensland, Australia ([email protected]) MARC ROTHENBERG, Smithsonian Institution (retired), USA ([email protected]) CLIFFORD CUNNINGHAM, University of Southern Queensland, Australia ([email protected]) Editorial Board: JAMES EVANS, University of Puget Sound, USA MILLER GOSS, National Radio Astronomy Observatory, USA DUANE HAMACHER, Monash University, Australia JAMES LEQUEUX, Observatoire de Paris, France SIMON MITTON, St. Edmund’s College Cambridge University, UK CLIVE RUGGLES, University of Leicester, UK VIRGINIA TRIMBLE, University of California Irvine, USA GUDRUN WOLFSCHMIDT, Institute for History of Science and Technology, Germany TRUDY BELL, Sky & Telescope, USA More information about this series at http://www.springer.com/series/15156 Ileana Chinnici • Guy Consolmagno Editors Angelo Secchi and Nineteenth Century Science The Multidisciplinary Contributions of a Pioneer and Innovator Editors Ileana Chinnici Guy Consolmagno INAF Vatican Observatory Osservatorio Astronomico di Palermo Vatican City State, Holy See Palermo, Italy ISSN 2509-310X ISSN 2509-3118 (electronic) Historical & Cultural Astronomy ISBN 978-3-030-58383-5 ISBN 978-3-030-58384-2 (eBook) https://doi.org/10.1007/978-3-030-58384-2 © Springer Nature Switzerland AG 2021 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifcally the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microflms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. -
NASA Spacecraft Nears Encounter with Dwarf Planet Ceres 4 March 2015
NASA spacecraft nears encounter with dwarf planet Ceres 4 March 2015 of 590 miles (950 kilometers), makes a full rotation every nine hours, and NASA is hoping for a wealth of data once the spacecraft's orbit begins. "Dawn is about to make history," said Robert Mase, project manager for the Dawn mission at NASA JPL in Pasadena, California. "Our team is ready and eager to find out what Ceres has in store for us." Experts will be looking for signs of geologic activity, via changes in these bright spots, or other features on Ceres' surface over time. The latest images came from Dawn when it was 25,000 miles (40,000 kilometers) away on February 25. This image was taken by NASA's Dawn spacecraft of dwarf planet Ceres on February 19, 2015 from a The celestial body was first spotted by Sicilian distance of nearly 29,000 miles astronomer Father Giuseppe Piazzi in 1801. "Ceres was initially classified as a planet and later called an asteroid. In recognition of its planet-like A NASA spacecraft called Dawn is about to qualities, Ceres was designated a dwarf planet in become the first mission to orbit a dwarf planet 2006, along with Pluto and Eris," NASA said. when it slips into orbit Friday around Ceres, the most massive body in the asteroid belt. Ceres is named after the Roman goddess of agriculture and harvests. The mission aims to shed light on the origins of the solar system 4.5 billion years ago, from its "rough The spacecraft on its way to circle it was launched and tumble environment of the main asteroid belt in September 2007. -
The Astronomical Work of Carl Friedrich Gauss
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector HISTORIA MATHEMATICA 5 (1978), 167-181 THE ASTRONOMICALWORK OF CARL FRIEDRICH GAUSS(17774855) BY ERIC G, FORBES, UNIVERSITY OF EDINBURGH, EDINBURGH EH8 9JY This paper was presented on 3 June 1977 at the Royal Society of Canada's Gauss Symposium at the Ontario Science Centre in Toronto [lj. SUMMARIES Gauss's interest in astronomy dates from his student-days in Gattingen, and was stimulated by his reading of Franz Xavier von Zach's Monatliche Correspondenz... where he first read about Giuseppe Piazzi's discovery of the minor planet Ceres on 1 January 1801. He quickly produced a theory of orbital motion which enabled that faint star-like object to be rediscovered by von Zach and others after it emerged from the rays of the Sun. Von Zach continued to supply him with the observations of contemporary European astronomers from which he was able to improve his theory to such an extent that he could detect the effects of planetary perturbations in distorting the orbit from an elliptical form. To cope with the complexities which these introduced into the calculations of Ceres and more especially the other minor planet Pallas, discovered by Wilhelm Olbers in 1802, Gauss developed a new and more rigorous numerical approach by making use of his mathematical theory of interpolation and his method of least-squares analysis, which was embodied in his famous Theoria motus of 1809. His laborious researches on the theory of Pallas's motion, in whi::h he enlisted the help of several former students, provided the framework of a new mathematical formu- lation of the problem whose solution can now be easily effected thanks to modern computational techniques. -
Geographical Distribution of the Italian Astronomical Observatories
Figure 25.1: Geographical distribution of the Italian Astronomical Observatories 226 25. Italian Astronomical Observatories and their Historical Instruments Collections Ileana Chinnici (Palermo, Italy) 25.1 A Brief Historical Introduction made by famous instruments-makers of that time, such as Ramsden, Short, Sisson, etc. while the typical equip- Italy has a high number of astronomical observatories ment of an Italian observatory in the middle of the 19th in comparison with its territorial extension. This is due century consisted of astronomical instruments made by to historical reasons, as Italy results from a political Reichenbach, Fraunhofer, Repsold, Merz and others. process of unification and annexation of several small The ancient observatories, built upon towers or states into which the country was divided – a process palaces in the middle of the cities, have mostly preserved (the Risorgimento) which was carried out mainly around their original building and their historical architecture; th the half of 19 century. a special mention is to be deserved to the Naples Obser- The first “institutional” Observatories in Italy were vatory, located on the hill of the Capodimonte: it was th established in the 18 century, as in the majority of the first architectural complex in Italy specially planned the other European nations. At that time, Italy was and built to be an astronomical observatory; it dates composed by seven states and since 1711 to 1819 each back to 1819, thus preceding the Pulkovo Observatory, of these states established one or two Observatories in established in 1839, which will serve later as architec- its territory. tural model for many observatories all over the world. -
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. -
ANDREA FERRARA Curriculum Vitae and Publication List Scuola
ANDREA FERRARA Curriculum Vitae and Publication List Scuola Normale Superiore Pisa, Italy Cosmology Professor HIGHLIGHTS • Cosmology Professor at Scuola Normale Superiore, Pisa, Italy • Dean of the Class of Sciences, Scuola Normale Superiore, Pisa, Italy • Former Prorector for Education, Internationalization and Placement at Scuola Normale Superiore, Pisa, Italy • INAF Board of Governors Member (2014 – 2015) • Joint Professor at the Institute for the Physics and Mathematics of the Universe, Tokyo, Japan • European Research Council (ERC) Advanced Grant Award (2017) • Honorary Blaauw Professorship, Groningen University, The Netherlands • Beatrice Tinsley Centennial Professorship, University of Texas at Austin, USA • Severo Ochoa Prize, Instituto de Astrofisica de Canarias, Spain • Alexander von Humboldt Foundation, Humboldt Research Award • Top Italian Scientist #52 • 174 among Invited, Review and Summary talks at International Conferences • 102 Colloquia in top scientific/academic institutes of 11 major countries • Expert evaluator of EU, European Science Foundation and National Research Grants Programs of USA, Germany, Portugal, Holland, Israel, France, Ireland, Switzerland, Norway, Austria • 50 among Master, PhD students and Post Docs supervised; 10 have received awards for their Thesis work • Astronomy & Astrophysics Journal and Dataset Papers in Physics: Editorial Board Member • 270 refereed papers in international Journals, 140 in conference proceedings (Scopus ID: 7201825167) • From the Google Scholar database, the H-index is 68; his i10-index is 224 • The total number of citations to his papers is 17,417 (6798 since 2013) • His top five most cited papers have more than 2,731 citations. EDUCATION 1986 National Research Council / CNR Pisa, Scientific Programming Course reg.# 5458 1988 University of Pisa, Pisa, Laurea in Physics; Thesis: Dust Expulsion from the Disk of Spiral Galaxies Advisor: Prof. -
(Physical Geographical Historical Dictionary of Tuscany, 1833) Written
In the Dizionario geografico fisico storico della Toscana (Physical geographical historical dictionary of Tuscany , 1833) written by Emanuele Repetti, Arcetri is described as a hill on the southern outskirts of Florence comprising a group of small villages, beautiful villas and country houses between San Miniato and the Villa of Poggio Imperiale, continuing towards Costa di San Giorgio, Belvedere and Boboli. The countryside around Arcetri is known for its beau - tiful panorama and for its historical and scientific back - ground. The Villa “Il Gioiello” where Galileo Galilei spent the last years of his life and the convent of San Matteo where his daughter Suor Maria Celeste resided, are all lo - cated near the Observatory. But above all, Arcetri is known for its scientific insti - Plan of the new Observatory to be tutes: the Observatory, the National Institute of Applied built on the “Podere Optics, the Galileo Galilei Institute for Theoretical della Capella” on the top of the Arcetri hill, Physics, and the Department of Astronomy and Space Sci - [before 1872] ence of the University of Florence. 1 The history of the Arcetri Astrophysical Observatory is preserved in the Observatory Archives and a wide col - lection of papers and correspondence documents the de - velopment of Italian astronomical research during the nineteenth and twentieth centuries. THE ARCETRI ASTROPHYSICAL OBSERVATORY AND ITS HISTORY Although astronomical studies in Tuscany go back to the times of the Accademia del Cimento (1657) and de - spite the small group of physicists formed by Pietro Leopol - do I di Lorena, who also supplied the Observatory with as - tronomical and meteorological instrumentation, a real school of astronomy only emerged on the 20 th of Febru - ary 1807 when the queen of Etruria, Maria Luisa, destined the “Real Museo” (Royal Museum) for public education. -
Mini Planet' with Water Ice 8 September 2005
Largest Asteroid May Be 'Mini Planet' With Water Ice 8 September 2005 Observations of 1 Ceres, the largest known From those snapshots, the astronomers determined asteroid, have revealed that the object may be a that the asteroid has a nearly round body. The "mini planet," and may contain large amounts of diameter at its equator is wider than at its poles. pure water ice beneath its surface. Computer models show that a nearly round object The observations by NASA's Hubble Space like Ceres has a differentiated interior, with denser Telescope also show that Ceres shares material at the core and lighter minerals near the characteristics of the rocky, terrestrial planets like surface. All terrestrial planets have differentiated Earth. Ceres' shape is almost round like Earth's, interiors. Asteroids much smaller than Ceres have suggesting that the asteroid may have a not been found to have such interiors. "differentiated interior," with a rocky inner core and a thin, dusty outer crust. The astronomers suspect that water ice may be buried under the asteroid's crust because the "Ceres is an embryonic planet," said Lucy A. density of Ceres is less than that of the Earth's McFadden of the Department of Astronomy at the crust, and because the surface bears spectral University of Maryland, College Park and a evidence of water-bearing minerals. They estimate member of the team that made the observations. that if Ceres were composed of 25 percent water, it "Gravitational perturbations from Jupiter billions of may have more water than all the fresh water on years ago prevented Ceres from accreting more Earth. -
Iau Commission C3 Newsletter
IAU COMMISSION C3 NEWSLETTER HISTORY OF ASTRONOMY Welcome to the winter solstice edition of the newsletter We wish everyone health and happiness in the new year. of IAU Commission C3 (History of Astronomy). This The next issue of the newsletter will be in June 2021. issue features the announcement of a new Project Group Please send our Secretary any news you would like us to and reports of pre-existing Working Groups and Project include. Groups since the last newsletter in June 2020. It contains Sara Schechner, Secretary news of upcoming conferences, reports of recent Wayne Orchiston, President meetings, a list of notable publications, and tables of Christiaan Sterken, Vice-President content from a journal devoted to the history of astronomy. The newsletter also contains announcements of research and PhD opportunities in the history of TABLE OF CONTENTS astronomy as well as an introduction to a new Ourania Network. And of course, you will find news from Reports of Working Groups & Project Groups 2 members, announcements of awards, and obituaries. Making History 15 Oral History 24 We are excited to introduce some new sections to the Art & Exhibitions 26 newsletter. The “Making History” section includes Announcements 30 reports on the Astronomy Genealogy Project (AstroGen), Awards and Honors 34 analysis of the Vatican Observatory’s guest book, and the News from Members 35 rescue of a medieval manuscript by Lewis of Caerleon. In In Memoriam 37 the “Oral History” section, there is a first-hand account Notable Publications 39 of the founding of the Journal of Astronomical History and Journal Contents 41 Heritage.