RECENT PUBLICATIONS RELATING to the HISTORY of ASTRONOMY Books and Pamphlets Agar, Jon. Science and Spectacle
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The Astronomical Garden of Venus and Mars-NG915: the Pivotal Role Of
The astronomical garden of Venus and Mars - NG915 : the pivotal role of Astronomy in dating and deciphering Botticelli’s masterpiece Mariateresa Crosta Istituto Nazionale di Astrofisica (INAF- OATo), Via Osservatorio 20, Pino Torinese -10025, TO, Italy e-mail: [email protected] Abstract This essay demonstrates the key role of Astronomy in the Botticelli Venus and Mars-NG915 painting, to date only very partially understood. Worthwhile coin- cidences among the principles of the Ficinian philosophy, the historical characters involved and the compositional elements of the painting, show how the astronomi- cal knowledge of that time strongly influenced this masterpiece. First, Astronomy provides its precise dating since the artist used the astronomical ephemerides of his time, albeit preserving a mythological meaning, and a clue for Botticelli’s signature. Second, it allows the correlation among Botticelli’s creative intention, the historical facts and the astronomical phenomena such as the heliacal rising of the planet Venus in conjunction with the Aquarius constellation dating back to the earliest represen- tations of Venus in Mesopotamian culture. This work not only bears a significant value for the history of science and art, but, in the current era of three-dimensional mapping of billion stars about to be delivered by Gaia, states the role of astro- nomical heritage in Western culture. Finally, following the same method, a precise astronomical dating for the famous Primavera painting is suggested. Keywords: History of Astronomy, Science and Philosophy, Renaissance Art, Educa- tion. Introduction Since its acquisition by London’s National Gallery on June 1874, the painting Venus and Mars by Botticelli, cataloged as NG915, has remained a mystery to be interpreted [1]1. -
EPSC2015-913, 2015 European Planetary Science Congress 2015 Eeuropeapn Planetarsy Science Ccongress C Author(S) 2015
EPSC Abstracts Vol. 10, EPSC2015-913, 2015 European Planetary Science Congress 2015 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2015 The “Station de Planétologie des Pyrénées” (S2P), a collaborative science program in the course of a long history at Pic du Midi observatory. F. Colas (1), A. Klotz (2), F. Vachier (1), M. Birlan (1), B. Sicardy (3), J. Lecacheux (3), M. Antuna (6), R. Behrend (4), C. Birnbaum (6), G. Blanchard (6), C. Buil (4,5), J. Caquel (6), M. Castets (5), C. Cavadore (4), B. Christophe (6), F. Cochard (4), J.L. Dauvergne (6), F. Deladerriere (6), M. Delcroix (6), V. Denoux (4), J.B. DeVanssay (6), P. Devechere (6), P. Dupouy (5), E. Frappa (6), S. Fauvaud (5), B. Gaillard (6), F. Jabet (6), M. Lavayssiere (6), T. Legault (6), A. Leroy (5), A. Maury (6), M. Meunier (6), C. Pellier (6), C. Rinner (4), E. Rolland (6), O. Stenuit (6), I. Testar (6), P. Thierry (4), O. Thizy (4), B. Tregon (5), F. Vaissiere (4), S. Vauclair (6), C. Viladrich (6), C. Angeli (6), J.E. Arlot (1), M. Assafin (28), D. Bancelin (1), D. Baratoux (29), N. Barrado-Izagirre (8), M.A. Barucci (3), L. Beauvalet (9), P. Bendjoya (13), J. Berthier (1), N. Biver (3), D. Bockelee-Morvan (3), D. Berard (3), S. Bouley (10), S. Bouquillon (9), P. Bourget (11), F. Bragas- Ribas (7), J. Camargo (7), B. Carry (1), S. Chevrel (2), M; Chevreton, (3), P. Colom (3), J. Crovisier (3), J. Demars (1), R. Despiau (2), P. Descamps (1), N. Dolez (2), A. -
Patrimoines Du Sud, 12 | 2020 Comment Évaluer L’Importance Patrimoniale D’Un Lieu Unique Et Complexe Grâce
Patrimoines du Sud 12 | 2020 Patrimoines et numérique : un état de la recherche et des expérimentations Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce au numérique ? L’exemple du Pic du Midi How to assess the heritage significance of a unique and complex site using digital tools? The example of the Pic du Midi Loïc Jeanson, Michel Cotte, Florent Laroche et Léa Bland-Dupré Édition électronique URL : http://journals.openedition.org/pds/4837 DOI : 10.4000/pds.4837 ISSN : 2494-2782 Éditeur Conseil régional Occitanie Référence électronique Loïc Jeanson, Michel Cotte, Florent Laroche et Léa Bland-Dupré, « Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce au numérique ? L’exemple du Pic du Midi », Patrimoines du Sud [En ligne], 12 | 2020, mis en ligne le 01 septembre 2020, consulté le 02 septembre 2020. URL : http://journals.openedition.org/pds/4837 ; DOI : https://doi.org/10.4000/pds.4837 Ce document a été généré automatiquement le 2 septembre 2020. La revue Patrimoines du Sud est mise à disposition selon les termes de la Licence Creative Commons Attribution - Pas d'Utilisation Commerciale - Pas de Modification 4.0 International. Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce ... 1 Comment évaluer l’importance patrimoniale d’un lieu unique et complexe grâce au numérique ? L’exemple du Pic du Midi How to assess the heritage significance of a unique and complex site using digital tools? The example of the Pic du Midi Loïc Jeanson, Michel Cotte, Florent Laroche et Léa Bland-Dupré Introduction 1 Depuis Tarbes, le Pic du Midi semble impossible à éviter. -
THE MYTH of ORPHEUS and EURYDICE in WESTERN LITERATURE by MARK OWEN LEE, C.S.B. B.A., University of Toronto, 1953 M.A., Universi
THE MYTH OF ORPHEUS AND EURYDICE IN WESTERN LITERATURE by MARK OWEN LEE, C.S.B. B.A., University of Toronto, 1953 M.A., University of Toronto, 1957 A THESIS SUBMITTED IN PARTIAL FULFILMENT OF THE REQUIREMENTS FOR THE DEGREE OF DOCTOR OP PHILOSOPHY in the Department of- Classics We accept this thesis as conforming to the required standard THE UNIVERSITY OF BRITISH COLUMBIA September, i960 In presenting this thesis in partial fulfilment of the requirements for an advanced degree at the University of British Columbia, I agree that the Library shall make it freely available for reference and study. I further agree that permission for extensive copying of this thesis for scholarly purposes may be granted by the Head of my Department or by his representatives. It is understood that copying or publication of this thesis for financial gain shall not be allowed without my written permission. Department of The University of British Columbia Vancouver 8, Canada. ©he Pttttrerstt^ of ^riitsl} (Eolimtbta FACULTY OF GRADUATE STUDIES PROGRAMME OF THE FINAL ORAL EXAMINATION FOR THE DEGREE OF DOCTOR OF PHILOSOPHY of MARK OWEN LEE, C.S.B. B.A. University of Toronto, 1953 M.A. University of Toronto, 1957 S.T.B. University of Toronto, 1957 WEDNESDAY, SEPTEMBER 21, 1960 AT 3:00 P.M. IN ROOM 256, BUCHANAN BUILDING COMMITTEE IN CHARGE DEAN G. M. SHRUM, Chairman M. F. MCGREGOR G. B. RIDDEHOUGH W. L. GRANT P. C. F. GUTHRIE C. W. J. ELIOT B. SAVERY G. W. MARQUIS A. E. BIRNEY External Examiner: T. G. ROSENMEYER University of Washington THE MYTH OF ORPHEUS AND EURYDICE IN WESTERN Myth sometimes evolves art-forms in which to express itself: LITERATURE Politian's Orfeo, a secular subject, which used music to tell its story, is seen to be the forerunner of the opera (Chapter IV); later, the ABSTRACT myth of Orpheus and Eurydice evolved the opera, in the works of the Florentine Camerata and Monteverdi, and served as the pattern This dissertion traces the course of the myth of Orpheus and for its reform, in Gluck (Chapter V). -
The Aratean Corpus in Vat. Grec. 1087
Book reviews 249 Ultimately, this book is aimed at the general reader, more curious about the science of dark matter than its history and sociology. To even begin to understand this complex field, one must take time with this slim volume in order to appreciate how the tiniest subatomic particles are connected to the largest structures of the cosmos. Freese mixes a stiff drink, but it goes down smoothly. LISA MESSERI University of Virginia [email protected] The Aratean corpus in Vat. Grec. 1087 Antiche stele a Bisanzio. Il codice Vaticano Greco 1087. Edited by Fabio Guidetti and Anna Santoni (Edizioni della Normale, Pisa, 2013. Pp. 208 + 31 illustrations. € 20. ISBN 978-88-7642-485-4. For nearly 150 years, scholars have devoted considerable effort trying understand the various means by which the astrothesic knowledge of the Graeco-Roman world passed to the modern age. Thanks to the magisterial work of Paul Kunitzsch and others, our grasp of the tortuous journey of Ptolemy’s Syntaxis mathematike from the original Greek to its Latin translations in the twelfth century has become much firmer. But despite the attention of a far wider range of scholars, the intricacies of the transmission of the Phaenomena of Aratus to the Latin West remain more elusive. This is primarily due to the fact that, soon after its composition, the poem attracted a huge entourage of ancillary material: the so-called ‘Aratean corpus’, composed of a rudimentary star catalogue, sets of celestial maps, a series of illustrated mythological explanations of the forms of the individual constellations and a potted biography of the author. -
Photométrie Et Astrométrie Des Satellites De Jupiter : Application À La Campagne De Phénomènes Mutuels 2015 Eléonore Saquet
Photométrie et Astrométrie des Satellites de Jupiter : application à la campagne de phénomènes mutuels 2015 Eléonore Saquet To cite this version: Eléonore Saquet. Photométrie et Astrométrie des Satellites de Jupiter : application à la campagne de phénomènes mutuels 2015. Astrophysique [astro-ph]. Université Paris sciences et lettres, 2017. Français. NNT : 2017PSLEO013. tel-01887821 HAL Id: tel-01887821 https://tel.archives-ouvertes.fr/tel-01887821 Submitted on 4 Oct 2018 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. A` mes parents, qui ont rendu possible le rˆeve d’une petite fille. T´elescope T1M du Pic du Midi. Cr´edit : St´ephane Vetter. Remerciements Ce m´emoire conclue mon travail de th`ese r´ealis´e`al’Institut de M´ecanique C´eleste et de Calculs des Eph´em´erides. Il n’aurait pas ´et´epossible sans l’appui d’un certain nombre de personnes, auxquelles je tiens `aexprimer ma sinc`ere gratitude. Je tiens tout d’abord `aremercier mes deux directeurs de th`ese Vincent Robert et Jean-Eudes Arlot de m’avoir propos´ece sujet puis de m’avoir encadr´ee pendant ces trois ann´ees. -
Observation of Venus and Mercury Transits from the Pic-Du-Midi Observatory
MEETING VENUS C. Sterken, P. P. Aspaas (Eds.) The Journal of Astronomical Data 19, 1, 2013 Observation of Venus and Mercury Transits from the Pic-du-Midi Observatory Guy Ratier 43 rue des Longues All´ees, F-45800 Saint-Jean-de-Braye, France Sylvain Rondi Soci´et´eAstronomique de France, 3 rue Beethoven, F-75016 Paris France Abstract. The Pic-du-Midi, on the French side of the Pyr´en´ees, became a state observatory in the summer of 1882. The first major astronomical event to be observed was the Venus transit of 6 December 1882. Unfortunately this attempt by the well-known Henry brothers was unsuccessful due to bad weather conditions. During the twentieth century, the Pic-du-Midi became famous for the quality of its solar and planetary observations. In the sixties, Jean R¨osch decided to use this experience to monitor the transits of Mercury. The objective was not to measure the parallax, but to determine the diameter of the planet in order to confirm its high density. Observations were made using a photometric method – the Hertzsprung method – during the transits of 1960, 1970 and 1973. The pioneer work of Ch. Boyer on the rotation of the Venus atmosphere as well as some experiments involving Lyot coronographs are also noteworthy. A Venus transit was finally observed on 8 June 2004 with a new CCD camera, providing a significant contribution to the model of the Venus mesosphere. This opened the field for new observations in 2012. 1. Early days of the Pic-du-Midi Observatory The site of the “Pic-du-Midi de Bigorre”, on the forefront of the Pyr´en´ees, has been known since ages as an ideal location to carry out astronomical observations. -
Tourmalet & Cycling's Greatest Challenges
Tourmalet & Cycling's Greatest Challenges - The Easier Way The peloton of the Tour de France has no time to enjoy the beautiful valleys and mountains of the central Pyrenees, or its authentic villages, great places to stay, and interesting regional cuisine. You will share their cycling challenges with the not insignificant help of e-bikes and travelling at your own pace, then be able to relax each evening in a way they can only dream of. If you love cycling and you love a challenge, but are not superhuman, this is the holiday for you - and one you will remember for all the best reasons. 7 nights - 6 days e-bike cycling Minimum required 1 From point to point With luggage transportation Self-guided Code : FP9PUTF The plus points • The major climbs and cols of the Tour de France • Cycling made easier - and much more enjoyable - thanks to electric bikes • An independent holiday - cycle at your own pace • Good quality, comfortable accommodation - and good meals too FP9PUTF Last update 29/12/2020 1 / 13 Before departure, please check that you have an updated fact sheet. FP9PUTF Last update 29/12/2020 2 / 13 The Tour de France's days in the Pyrenees are the most challenging cycling in the world. Now imagine you breezing up the Col du Tourmalet with a big grin on your face as you reach the summit of the Col d'Aubisque. You can now enjoy the most interesting and famous sections of the Tour de France route with the help of an electric bike - and Purely Pyrenees, the leading walking and cycling tour operator in the Pyrenees. -
The Epoch of the Constellations on the Farnese Atlas and Their Origin in Hipparchus’S Lost Catalogue
JHA, xxxvi (2005) THE EPOCH OF THE CONSTELLATIONS ON THE FARNESE ATLAS AND THEIR ORIGIN IN HIPPARCHUS’S LOST CATALOGUE BRADLEY E. SCHAEFER, Louisiana State University, Baton Rouge 1. BACKGROUND The Farnese Atlas is a Roman statue depicting the Titan Atlas holding up a celestial globe that displays an accurate representation of the ancient Greek constellations (see Figures 1 and 2). This is the oldest surviving depiction of the original Western constellations, and as such can be a valuable resource for studying their early development. The globe places the celestial fi gures against a grid of circles (including the celestial equator, the tropics, the colures, the ecliptic, the Arctic Circle, and the Antarctic Circle) that allows for the accurate positioning of the constellations. The positions shift with time due to precession, so the observed positions on the Farnese Atlas correspond to some particular date. Also, the declination of the Arctic and Antarctic Circles will correspond to a particular latitude for the observer whose observations were adopted by the sculptor. Thus, a detailed analysis of the globe will reveal the latitude and epoch for the observations incorporated in the Atlas; and indeed these will specify enough information that we can identify the observer. Independently, a detailed comparison of the constellation symbols on the Atlas with those from the other surviving ancient material also uniquely points to the same origin for the fi gures. The Farnese Atlas1 fi rst came to modern attention in the early sixteenth century when it became part of the collection of antiquities in the Farnese Palace in Rome, hence its name. -
Solar Survey at Pic Du Midi: Calibrated Data and Improved Images Laurent Koechlin1, Luc Dettwiller2, Maurice Audejean3, Maël Valais1, and Arturo López Ariste1
A&A 631, A55 (2019) Astronomy https://doi.org/10.1051/0004-6361/201732504 & c L. Koechlin et al. 2019 Astrophysics Solar survey at Pic du Midi: Calibrated data and improved images Laurent Koechlin1, Luc Dettwiller2, Maurice Audejean3, Maël Valais1, and Arturo López Ariste1 1 Institut de recherches en astrophysique et planétologie, Université de Toulouse, CNRS, CNES, UPS, 14 Avenue Edouard Belin, 31400 Toulouse, France e-mail: [email protected] 2 Lycée Blaise Pascal, 36 Avenue Carnot, 63037 Clermont-Ferrand Cedex, France 3 Observateurs associés, Rue de la Cau, 65200 Bagnères de Bigorre, France Received 20 December 2017 / Accepted 5 September 2019 ABSTRACT Context. We carry out a solar survey with images of the photosphere, prominences, and corona at Pic du Midi observatory. This sur- vey, named CLIMSO (for CLIchés Multiples du SOleil), is in the following spectral lines: Fe XIII corona (1.075 µm), Hα (656.3 nm), and He I (1.083 µm) prominences, and Hα and Ca II (393.4 nm) photosphere. All frames cover 1.3 times the diameter of the Sun with an angular resolution approaching one arcsecond. The frame rate is one per minute per channel (weather permitting) for the prominences and chromosphere, and one per hour for the Fe XIII corona. This survey started in 2007 for the disk and prominences and in 2015 for the corona. We have almost completed one solar cycle and hope to cover several more, keeping the same wavelengths or adding others. Aims. We seek to make the CLIMSO images easier to use and more profitable for the scientific community. -
Project Periodic Report
PROJECT PERIODIC REPORT Grant Agreement number: 654208 Project acronym: EPN2020-RI Project title: EUROPLANET 2020 Research Infrastructure Call identifier: H2020-INFRAIA-1-2014-2015 Date of latest version of Annex I against which the assessment will be made: 1st March 2016 Periodic report: 1st □ 2nd X 3rd □ 4th □ Period covered: from 1 March 2017 to 31 August 2018 Project website address: http://www.europlanet-2020-ri.eu/ 1 Table of Content List of Figures 7 List of Tables 10 Table of Main Acronyms 11 Project Summary 11 1. Background 11 2. Europlanet 2020 Research Infrastructure - Impact to date 11 3. Collaborations with other EU projects 14 4. Future Plans and Sustainability 15 5. Conclusion 15 1. WP1: Management 16 1.1 Explanation of the work carried out by the beneficiaries and overview of progress 16 Task 1.1 - Management structure and tools 16 Task 1.2 - Regular operations of the management structure 16 Task 1.3 - Reporting 17 Task 1.4 - Call for proposals, evaluation and validation of Transnational Access visits 17 Task 1.5 – Sustainability and Financial Plan 26 Task 1.6 - Data management 27 1.2 Impact 27 2. Deviations from Annex 1 30 2.1 Amendments 30 2.2.2 Additional proposed changes 31 3. Financial reports 31 2. WP2 - TA 1: Planetary Field Analogues (PFA) 34 1.1 Explanation of the work carried out by the beneficiaries and overview of progress 34 Task 2.1-Rio Tinto (INTA) 34 Task 2.2-Ibn Battuta Centre (IRSPS) 35 Task 2.3- The glacial and volcanically active areas of Iceland, Iceland (MATIS) 36 Task 2.4 Lake Tirez (INTA) 37 Task 2.5-Danakil Depression, Ethiopia (IRSPS) 38 1.2 Impact 40 3. -
Heritage Sites of Astronomy and Archaeoastronomy in the Context of the UNESCO World Heritage Convention
Heritage Sites of Astronomy and Archaeoastronomy in the context of the UNESCO World Heritage Convention Thematic Study, vol. 2 Clive Ruggles and Michel Cotte with contributions by Margaret Austin, Juan Belmonte, Nicolas Bourgeois, Amanda Chadburn, Danielle Fauque, Iván Ghezzi, Ian Glass, John Hearnshaw, Alison Loveridge, Cipriano Marín, Mikhail Marov, Harriet Nash, Malcolm Smith, Luís Tirapicos, Richard Wainscoat and Günther Wuchterl Edited by Clive Ruggles Published by Ocarina Books Ltd 27 Central Avenue, Bognor Regis, West Sussex, PO21 5HT, United Kingdom and International Council on Monuments and Sites Office: International Secretariat of ICOMOS, 49–51 rue de la Fédération, F–75015 Paris, France in conjunction with the International Astronomical Union IAU–UAI Secretariat, 98-bis Blvd Arago, F–75014 Paris, France Supported by Instituto de Investigaciones Arqueológicas (www.idarq.org), Peru MCC–Heritage, France Royal Astronomical Society, United Kingdom ISBN 978–0–9540867–6–3 (e-book) ISBN 978–2–918086–19–2 (e-book) © ICOMOS and the individual authors, 2017 All rights reserved A preliminary version of this publication was presented at a side-event during the 39th session of the UNESCO World Heritage Committee (39COM) in Bonn, Germany, in July 2015 Front cover photographs: Star-timing device at Al Fath, Oman. © Harriet Nash Pic du Midi Observatory, France. © Claude Etchelecou Chankillo, Peru. © Iván Ghezzi Starlight over the church of the Good Shepherd, Tekapo, New Zealand. © Fraser Gunn Table of contents Preface ......................................................................................................................................