Planetary Diagrams — Descriptions, Models, Theories: from Carolingian Deployments to Copernican Debates
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Invited Talks and Lectures
Invited Talks and Lectures Fundamental Problems in Planetary Science and Astrobiology 13th IAU-Abdul Jabbar Astronomy Workshop Bangladesh University of Engineering and Technology Dhaka, Bangladesh (November 6, 2020) Terrestrial Planet Formation in Modern Era: Current State and Future Direction Pathways to Habitability Bad Hofgastein, Austria (January 12-18, 2020) Life Stories; A Career in Planetology Keynote Presentation at EPSC-DPS 2019 Geneva, Switzerland (September 15, 2019) Planets in Binary Stars Institute of Physical Sciences of the National Autonomous University of Mexico (ICF-UNAM) Cuernavaca, Mexico (February 20, 2019) New Advances in the Formation of Terrestrial Planets National Institute for Space Research San Jose Campos, Brazil (October 2, 2018) Four Lectures on Exoplanet Formation and Kepler Telescope’s Discoveries 3rd Astrobiology School at the National Observatory of Brazil Rio de Janeiro, Brazil (October 1 – 5, 2018) Planet Formation: The Gateway to Astrobiology Keynote talk at the 3rd AbGradE Symposium Berlin, Germany (September 22 – 24, 2018) From Dust to Planets Summer School on the Formation and Evolution of Stars and Planets, the Early Solar System, and the Emergence of Life Vienna, Austria (August 17 – 18, 2018) Modern Simulations of Terrestrial Planet Formation and the Origin of Earth’s Water Leibniz Institute for Astrophysics Potsdam, Germany (June 7, 2018) Modern Simulations of Terrestrial Planet Formation and the Origin of Earth’s Water University of Groningen Groningen, Netherlands (June 4, 2018) Modern Simulations -
Implementing Eratosthenes' Discovery in the Classroom: Educational
Implementing Eratosthenes’ Discovery in the Classroom: Educational Difficulties Needing Attention Nicolas Decamp, C. de Hosson To cite this version: Nicolas Decamp, C. de Hosson. Implementing Eratosthenes’ Discovery in the Classroom: Educational Difficulties Needing Attention. Science and Education, Springer Verlag, 2012, 21 (6), pp.911-920. 10.1007/s11191-010-9286-3. hal-01663445 HAL Id: hal-01663445 https://hal.archives-ouvertes.fr/hal-01663445 Submitted on 18 Dec 2017 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. Sci & Educ DOI 10.1007/s11191-010-9286-3 Implementing Eratosthenes’ Discovery in the Classroom: Educational Difficulties Needing Attention Nicolas De´camp • Ce´cile de Hosson Ó Springer Science+Business Media B.V. 2010 Abstract This paper presents a critical analysis of the accepted educational use of the method performed by Eratosthenes to measure the circumference of Earth which is often considered as a relevant means of dealing with issues related to the nature of science and its history. This method relies on a number of assumptions among which the parallelism of sun rays. The assumption of sun rays parallelism (if it is accurate) does not appear spontaneous for students who consider sun rays to be divergent. -
Astronomy and Hipparchus
CHAPTER 9 Progress in the Sciences: Astronomy and Hipparchus Klaus Geus Introduction Geography in modern times is a term which covers several sub-disciplines like ecology, human geography, economic history, volcanology etc., which all con- cern themselves with “space” or “environment”. In ancient times, the definition of geography was much more limited. Geography aimed at the production of a map of the oikoumene, a geographer was basically a cartographer. The famous scientist Ptolemy defined geography in the first sentence of his Geographical handbook (Geog. 1.1.1) as “imitation through drafting of the entire known part of the earth, including the things which are, generally speaking, connected with it”. In contrast to chorography, geography uses purely “lines and label in order to show the positions of places and general configurations” (Geog. 1.1.5). Therefore, according to Ptolemy, a geographer needs a μέθοδος μαθεματική, abil- ity and competence in mathematical sciences, most prominently astronomy, in order to fulfil his task of drafting a map of the oikoumene. Given this close connection between geography and astronomy, it is not by default that nearly all ancient “geographers” (in the limited sense of the term) stood out also as astronomers and mathematicians: Among them Anaximander, Eudoxus, Eratosthenes, Hipparchus, Poseidonius and Ptolemy are the most illustrious. Apart from certain topics like latitudes, meridians, polar circles etc., ancient geography also took over from astronomy some methods like the determina- tion of the size of the earth or of celestial and terrestrial distances.1 The men- tioned geographers Anaximander, Eudoxus, Hipparchus, Poseidonius and Ptolemy even constructed instruments for measuring, observing and calculat- ing like the gnomon, sundials, skaphe, astrolabe or the meteoroscope.2 1 E.g., Ptolemy (Geog. -
A Solstice Sundial
A SOLSTICE SUNDIAL JACKIE JONES arlier this year a group of us went on holiday to It being Wales, one is never sure about the weather, so we South Wales; as the period covered the summer prepared for different methods of establishing the north– E solstice, we decided it should be celebrated in south line. In the hope of a sunny day and being able some form. Following the experience of the sundial on to draw a line from the shadow of a vertical pole, we Crosby Beach just before the BSS Conference in Liverpool calculated how solar noon would relate to watch time. in April 2016,1 I decided another seaside sundial would be Taking into account the longitude, which was 4° west appropriate. equalling 16 minutes; equation of time, dial slow by As with that event, planning the dial and exactly where it 1 minute 42 seconds and the one hour for British Summer will be, in advance, is essential. With the aid of maps and Time gave us a watch time of 13:17:42 – probably a bit Google Earth we located a south-facing sandy beach just a over-accurate for our needs. We also planned to have a few minutes’ walk from where we were staying. The compass, knowing the correction from magnetic to true latitude of the bay is 51° 34ʹ north and we agreed to north. construct a solar-time horizontal dial using only natural On a coastal walk a few days before the solstice, we found materials found nearby. Before leaving home, I drew out on the perfect long sticks needed for the gnomon and supports; metre-wide paper the layout of the afternoon hour lines for we were then fully prepared. -
The Sundial Cities
The Sundial Cities Joel Van Cranenbroeck, Belgium Keywords: Engineering survey;Implementation of plans;Positioning;Spatial planning;Urban renewal; SUMMARY When observing in our modern cities the sun shade gliding along the large surfaces of buildings and towers, an observer can notice that after all the local time could be deduced from the position of the sun. The highest building in the world - the Burj Dubai - is de facto the largest sundial ever designed. The principles of sundials can be understood most easily from an ancient model of the Sun's motion. Science has established that the Earth rotates on its axis, and revolves in an elliptic orbit about the Sun; however, meticulous astronomical observations and physics experiments were required to establish this. For navigational and sundial purposes, it is an excellent approximation to assume that the Sun revolves around a stationary Earth on the celestial sphere, which rotates every 23 hours and 56 minutes about its celestial axis, the line connecting the celestial poles. Since the celestial axis is aligned with the axis about which the Earth rotates, its angle with the local horizontal equals the local geographical latitude. Unlike the fixed stars, the Sun changes its position on the celestial sphere, being at positive declination in summer, at negative declination in winter, and having exactly zero declination (i.e., being on the celestial equator) at the equinoxes. The path of the Sun on the celestial sphere is known as the ecliptic, which passes through the twelve constellations of the zodiac in the course of a year. This model of the Sun's motion helps to understand the principles of sundials. -
Institute of Theoretical Astronomy, 10, Kutuzov Quay, St.Petersburg, 191187, Russia
The Library of the Institute of Theoretical Astronomy of the Russian Academy of Sciences (1924 -1994). History, Present State, Perspectives for the Future M.V.Lapteva Institute of Theoretical Astronomy, 10, Kutuzov Quay, St.Petersburg, 191187, Russia e-mail: [email protected] fax: (812) 272-79-68 The Library of the Institute of Theoretical Astronomy (formerly The Library of the Astronomical Institute of the People’s Commisariat of Edu- cation, USSR (1924 - 1938); the Library of the Astronomical Institute of the USSR Academy of Sciences (1939 - 1943 (Dec. 16))) was established by the decision of the first director and founder of the Institute, Boris Vasil’evich Numerov (1891 - 1941), an outstanding astronomer in the fields of celestial mechanics, astrometry and geodesy, a corresponding member of the USSR Academy of Sciences since 1929 and a very gifted person who perished a victim to a repressive stalinist regime in 1941. The basis of the Library holdings formed the collections of books and pe- riodicals belonging to the Computational and Astronomo-Geodetic Institutes which merged in 1923 to form the Astronomical Institute. From the time of its foundation (1924) to 1930 the library had no profes- sional librarian. Beginning with 1924 and to 1936 (the time of his arrest) the director of the Institute B.V.Numerov devoted much of his time and efforts to primary and then current acquisition of relevant publications. During his numerous scientific missions abroad (Germany, USA, the coun- tries of the South America, etc) along with equipment he purchased urgently needed foreign publications and laid the basis for exchange of publications with foreign astronomical institutions since from 1922 the Institute started publishing its own works: 1. -
9 · the Growth of an Empirical Cartography in Hellenistic Greece
9 · The Growth of an Empirical Cartography in Hellenistic Greece PREPARED BY THE EDITORS FROM MATERIALS SUPPLIED BY GERMAINE AUJAe There is no complete break between the development of That such a change should occur is due both to po cartography in classical and in Hellenistic Greece. In litical and military factors and to cultural developments contrast to many periods in the ancient and medieval within Greek society as a whole. With respect to the world, we are able to reconstruct throughout the Greek latter, we can see how Greek cartography started to be period-and indeed into the Roman-a continuum in influenced by a new infrastructure for learning that had cartographic thought and practice. Certainly the a profound effect on the growth of formalized know achievements of the third century B.C. in Alexandria had ledge in general. Of particular importance for the history been prepared for and made possible by the scientific of the map was the growth of Alexandria as a major progress of the fourth century. Eudoxus, as we have seen, center of learning, far surpassing in this respect the had already formulated the geocentric hypothesis in Macedonian court at Pella. It was at Alexandria that mathematical models; and he had also translated his Euclid's famous school of geometry flourished in the concepts into celestial globes that may be regarded as reign of Ptolemy II Philadelphus (285-246 B.C.). And it anticipating the sphairopoiia. 1 By the beginning of the was at Alexandria that this Ptolemy, son of Ptolemy I Hellenistic period there had been developed not only the Soter, a companion of Alexander, had founded the li various celestial globes, but also systems of concentric brary, soon to become famous throughout the Mediter spheres, together with maps of the inhabited world that ranean world. -
Need and Possibilities of Astronomy Teaching in the Finnish Comprehensive School
UNIVERSITY OF HELSINKI REPORT SERIES IN PHYSICS HU•P•D124 Need and possibilities of astronomy teaching in the Finnish comprehensive school Irma Hannula DEPARTMENT OF PHYSICAL SCIENCES P.O. BOX FIN•00014 UNIVERSITY OF HELSINKI HELSINKI, FINLAND Academic Dissertation To be presented, with the permission of the Faculty of Science of the University of Helsinki, for public criticism in the Small Auditorium E204 of the Department of Physical Sciences, on July 29th, 2005, at 12 o’clock. Helsinki 2005 ISBN 952•10•2103•9 (printed version) ISSN 0356•0961 ISBN 952•10•2104•7 (pdf•version) http://ethesis.helsinki.fi/ Photo: Aurora Borealis /Irma Hannula Yliopistopaino Helsinki Daniel my dear first•born grandchild you are joy and blessing for my life! I. Hannula: Need and possibilities of astronomy teaching in the Finnish comprehensive school, University of Helsinki, 2005, vii, 250 p., University of Helsinki, Report Series in Physics, HU•P•D124, ISBN 952•10• 2103•9 (printed version), ISSN 0356•0961, ISBN 952•10•2104•7 (pdf•version), http://ethesis.helsinki.fi/. Classification (INSPEC): A0140D, A0140E, A0140G, A0140J, A0190 Keywords: astronomy teaching, worldview, attitude, conceptual and processual structure Abstract The purpose of this work is to create a research•based foundation for planning the structure, content and methods of astronomy teaching in the Finnish comprehensive school. At first, a critical analysis of the significance of astronomy teaching from the point of view of the educational aims was made, in order to verify the need of it and to find significance factors, which would offer a basis for defining principles of astronomy teaching. -
Determining True North on Mars by Using a Sundial on Insight D
Determining True North on Mars by Using a Sundial on InSight D. Savoie, A. Richard, M. Goutaudier, N. Onufer, M. Wallace, D. Mimoun, K. Hurst, N. Verdier, P. Lognonné, N. Mäki, et al. To cite this version: D. Savoie, A. Richard, M. Goutaudier, N. Onufer, M. Wallace, et al.. Determining True North on Mars by Using a Sundial on InSight. Space Science Reviews, Springer Verlag, 2019, 215 (1), pp.215:2. hal-01977462 HAL Id: hal-01977462 https://hal.sorbonne-universite.fr/hal-01977462 Submitted on 10 Jan 2019 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. Determining true North on Mars by using a sundial on InSight D. Savoiea,∗, A. Richardb,∗∗, M. Goutaudierb, N.P. Onuferc, M.C. Wallacec, D. Mimoune, K. Hurstc, N. Verdierf, P. Lognonnéd, J.N. Makic, B. Banerdtc aSYRTE, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, LNE, 61 avenue de l’Observatoire 75014 Paris, France bPalais de la Découverte, Av. Franklin D. Roosevelt, 75008 Paris, France cNASA Jet Propulsion Laboratory, Pasadena, California dInstitut de Physique du Globe de Paris, Université Paris Diderot, Paris, France eInstitut Supérieur de l’Aéronautique et de l’Espace, ISAE, Toulouse, France fFrench National Space Agency, CNES, Paris, France Abstract In this work, we demonstrate the possibility to determine the true North direction on Mars by using a gnomon on the InSight mission. -
Arab Conference on Astronomy and Geophysics the 5Th Assembly (ACAG-5) By: Sultana N
Arab Conference on Astronomy and Geophysics the 5th Assembly (ACAG-5) By: Sultana N. Nahar, The Ohio State University The international Arab Conference on Astronomy and Geophysics (ACAG) has been held every two years since its initiation in 2008 by the Minister of Higher Education and Scientific Research of Egypt and the General Secretary of the League of Arab States. The objectives are to hold ACAG in all Arab states and strengthen the collaborations among the Arab countries. However, any non-Arabic country is welcome to join. I attended the 5th Assembly held at the National Research Institute of The author of this article, Sultana N. Astronomy and Geophysics (NRIAG) in Helwan, Egypt during Nahar, the first woman Guest of Honor at October 17 - 20, 2016. It was my honor to be invited as the first female ACAG-5. Guest of Honor at ACAG along with two Emirs from the United Arab Emirates. As told, I might be the first female guest of honor at any other Arab conferences. NRIAG in Egypt has been the main host for ACAGs, but the plan is now to move to other Arab countries. Egypt is the most attractive place for students and researchers of North African and Middle-Eastern countries for education and research. Founded in 1839 in Boulac, NRIAG (previously the Helwan observatory) is the oldest observatory in North Africa. It moved to Abbassia and then to Helwan in 1903 where it is currently located. It runs 11 labs all over Egypt with space and solar, seismology, geomagnetism, geoelectric, and geodynamics research labs. -
How Big Is the Earth?
Document ID: 04_01_13_1 Date Received: 2013-04-01 Date Revised: 2013-07-24 Date Accepted: 2013-08-16 Curriculum Topic Benchmarks: M4.4.8, M5.4.12, M8.4.2, M8.4.15, S15.4.4, S.16.4.1, S16.4.3 Grade Level: High School [9-12] Subject Keywords: circumference, radius, Eratosthenes, gnomon, sun dial, Earth, noon, time zone, latitude, longitude, collaboration Rating: Advanced How Big Is the Earth? By: Stephen J Edberg, Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, M/S 183-301, Pasadena CA 91011 e-mail: [email protected] From: The PUMAS Collection http://pumas.jpl.nasa.gov ©2013, Jet Propulsion Laboratory, California Institute of Technology. ALL RIGHTS RESERVED. Eratosthenes, the third librarian of the Great Library of Alexandria, measured the circumference of Earth around 240 B.C.E. Having learned that the Sun passed through the zenith1 on the summer solstice2 as seen in modern day Aswan, he measured the length of a shadow on the solstice in Alexandria. By converting the measurement to an angle he determined the difference in latitude – what fraction of a circle spanned the separation – between Aswan and Alexandria. Knowing the physical distance between Aswan and Alexandria allowed him to determine the circumference of Earth. Cooperating schools can duplicate Eratosthenes’ measurements without the use of present day technology, if desired. Sharing their data permits students to calculate the circumference and the radius of Earth. The measurements do not require a site on the Tropic of Cancer (or the Tropic of Capricorn) but they must be made at local solar noon on the same date. -
Evaluation Report for the Division of Theoretical Astronomy of NAOJ Piet
Evaluation Report for the Division of Theoretical Astronomy of NAOJ Piet Hut, Yipeng Jing, Doug Lin, Shin Mineshige, Masayuki Umemura February 2008 1. Summary We are impressed by the many accomplishments that have been made in the Theory and Computation Division of the National Astronomical Observatory of Japan (NAOJ) in the past four years. We agree with the self-evaluation report of the Division, which has high- lighted many important areas of research to which the Division has made major contri- butions. In particular, we agree with their analysis of their scienti¯c output: they have published a large number of papers with signi¯cant impact on the international community. If anything, the self-evaluation has been too modest. The Division of Theoretical Astronomy / Center for Computational Astrophysics (DTA/CfCA) is truly an international center of excellence in computational astrophysics, one of the most important centers of that type in the world. Much progress has been made on the development and application of numerical algorithms as well as actual hardware which enable large scale computation in areas ranging from solar system formation to the emergence of structure in the Universe. The 4D2U initiative has produced an e®ective package for public outreach as well as a valuable research tool. We strongly endorse future expansion of the theoretical e®ort especially in the development of innovative algorithms and state-of-the-art simulations. These simulations can provide predictions as well as interpretations of observations to be obtained from the various next- generation astronomical facilities. No matter how important direct observations and pure theoretical thought may be, their signi¯cance can only be understood through the bridge between the two that is provided by means of detailed simulations.