M^Ittt of ^J^Iutfoyl^ Mr. Ehtesham Bin Hasan
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Scienza E Cultura Universitalia
SCIENZA E CULTURA UNIVERSITALIA Costantino Sigismondi (ed.) ORBE NOVUS Astronomia e Studi Gerbertiani 1 Universitalia SIGISMONDI, Costantino (a cura di) Orbe Novus / Costantino Sigismondi Roma : Universitalia, 2010 158 p. ; 24 cm. – ( Scienza e Cultura ) ISBN … 1. Storia della Scienza. Storia della Chiesa. I. Sigismondi, Costantino. 509 – SCIENZE PURE, TRATTAMENTO STORICO 270 – STORIA DELLA CHIESA In copertina: Imago Gerberti dal medagliere capitolino e scritta ORBE NOVVS nell'epitaffio tombale di Silvestro II a S. Giovanni in Laterano (entrambe le foto sono di Daniela Velestino). Collana diretta da Rosalma Salina Borello e Luca Nicotra Prima edizione: maggio 2010 Universitalia INTRODUZIONE Introduzione Costantino Sigismondi L’edizione del convegno gerbertiano del 2009, in pieno anno internazionale dell’astronomia, si è tenuta nella Basilica di S. Maria degli Angeli e dei Martiri il 12 maggio, e a Seoul presso l’università Sejong l’11 giugno 2009. La scelta della Basilica è dovuta alla presenza della grande meridiana voluta dal papa Clemente XI Albani nel 1700, che ancora funziona e consente di fare misure di valore astrometrico. Il titolo di questi atti, ORBE NOVUS, è preso, come i precedenti, dall’epitaffio tombale di Silvestro II in Laterano, e vuole suggerire il legame con il “De Revolutionibus Orbium Coelestium” di Copernico, sebbene il contesto in cui queste parole sono tratte vuole inquadrare Gerberto nel suo ministero petrino come il nuovo pastore per tutto il mondo: UT FIERET PASTOR TOTO ORBE NOVVS. Elizabeth Cavicchi del Massachussets Institute of Technology, ha riflettuto sulle esperienze di ottica geometrica fatte da Gerberto con i tubi, nel contesto contemporaneo dello sviluppo dell’ottica nel mondo arabo con cui Gerberto era stato in contatto. -
The Mathematical Work of John Napier (1550-1617)
BULL. AUSTRAL. MATH. SOC. 0IA40, 0 I A45 VOL. 26 (1982), 455-468. THE MATHEMATICAL WORK OF JOHN NAPIER (1550-1617) WILLIAM F. HAWKINS John Napier, Baron of Merchiston near Edinburgh, lived during one of the most troubled periods in the history of Scotland. He attended St Andrews University for a short time and matriculated at the age of 13, leaving no subsequent record. But a letter to his father, written by his uncle Adam Bothwell, reformed Bishop of Orkney, in December 1560, reports as follows: "I pray you Sir, to send your son John to the Schools either to France or Flanders; for he can learn no good at home, nor gain any profit in this most perilous world." He took an active part in the Reform Movement and in 1593 he produced a bitter polemic against the Papacy and Rome which was called The Whole Revelation of St John. This was an instant success and was translated into German, French and Dutch by continental reformers. Napier's reputation as a theologian was considerable throughout reformed Europe, and he would have regarded this as his chief claim to scholarship. Throughout the middle ages Latin was the medium of communication amongst scholars, and translations into vernaculars were the exception until the 17th and l8th centuries. Napier has suffered badly through this change, for up till 1889 only one of his four works had been translated from Latin into English. Received 16 August 1982. Thesis submitted to University of Auckland, March 1981. Degree approved April 1982. Supervisors: Mr Garry J. Tee Professor H.A. -
Mathematicians
MATHEMATICIANS [MATHEMATICIANS] Authors: Oliver Knill: 2000 Literature: Started from a list of names with birthdates grabbed from mactutor in 2000. Abbe [Abbe] Abbe Ernst (1840-1909) Abel [Abel] Abel Niels Henrik (1802-1829) Norwegian mathematician. Significant contributions to algebra and anal- ysis, in particular the study of groups and series. Famous for proving the insolubility of the quintic equation at the age of 19. AbrahamMax [AbrahamMax] Abraham Max (1875-1922) Ackermann [Ackermann] Ackermann Wilhelm (1896-1962) AdamsFrank [AdamsFrank] Adams J Frank (1930-1989) Adams [Adams] Adams John Couch (1819-1892) Adelard [Adelard] Adelard of Bath (1075-1160) Adler [Adler] Adler August (1863-1923) Adrain [Adrain] Adrain Robert (1775-1843) Aepinus [Aepinus] Aepinus Franz (1724-1802) Agnesi [Agnesi] Agnesi Maria (1718-1799) Ahlfors [Ahlfors] Ahlfors Lars (1907-1996) Finnish mathematician working in complex analysis, was also professor at Harvard from 1946, retiring in 1977. Ahlfors won both the Fields medal in 1936 and the Wolf prize in 1981. Ahmes [Ahmes] Ahmes (1680BC-1620BC) Aida [Aida] Aida Yasuaki (1747-1817) Aiken [Aiken] Aiken Howard (1900-1973) Airy [Airy] Airy George (1801-1892) Aitken [Aitken] Aitken Alec (1895-1967) Ajima [Ajima] Ajima Naonobu (1732-1798) Akhiezer [Akhiezer] Akhiezer Naum Ilich (1901-1980) Albanese [Albanese] Albanese Giacomo (1890-1948) Albert [Albert] Albert of Saxony (1316-1390) AlbertAbraham [AlbertAbraham] Albert A Adrian (1905-1972) Alberti [Alberti] Alberti Leone (1404-1472) Albertus [Albertus] Albertus Magnus -
Abd Al-Rahman Al-Sufi and His Book of the Fixed Stars: a Journey of Re-Discovery
ResearchOnline@JCU This file is part of the following reference: Hafez, Ihsan (2010) Abd al-Rahman al-Sufi and his book of the fixed stars: a journey of re-discovery. PhD thesis, James Cook University. Access to this file is available from: http://eprints.jcu.edu.au/28854/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://eprints.jcu.edu.au/28854/ 5.1 Extant Manuscripts of al-Ṣūfī’s Book Al-Ṣūfī’s ‘Book of the Fixed Stars’ dating from around A.D. 964, is one of the most important medieval Arabic treatises on astronomy. This major work contains an extensive star catalogue, which lists star co-ordinates and magnitude estimates, as well as detailed star charts. Other topics include descriptions of nebulae and Arabic folk astronomy. As I mentioned before, al-Ṣūfī’s work was first translated into Persian by al-Ṭūsī. It was also translated into Spanish in the 13th century during the reign of King Alfonso X. The introductory chapter of al-Ṣūfī’s work was first translated into French by J.J.A. Caussin de Parceval in 1831. However in 1874 it was entirely translated into French again by Hans Karl Frederik Schjellerup, whose work became the main reference used by most modern astronomical historians. In 1956 al-Ṣūfī’s Book of the fixed stars was printed in its original Arabic language in Hyderabad (India) by Dārat al-Ma‘aref al-‘Uthmānīa. -
The Longitude of the Mediterranean Throughout History: Facts, Myths and Surprises Luis Robles Macías
The longitude of the Mediterranean throughout history: facts, myths and surprises Luis Robles Macías To cite this version: Luis Robles Macías. The longitude of the Mediterranean throughout history: facts, myths and sur- prises. E-Perimetron, National Centre for Maps and Cartographic Heritage, 2014, 9 (1), pp.1-29. hal-01528114 HAL Id: hal-01528114 https://hal.archives-ouvertes.fr/hal-01528114 Submitted on 27 May 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. e-Perimetron, Vol. 9, No. 1, 2014 [1-29] www.e-perimetron.org | ISSN 1790-3769 Luis A. Robles Macías* The longitude of the Mediterranean throughout history: facts, myths and surprises Keywords: History of longitude; cartographic errors; comparative studies of maps; tables of geographical coordinates; old maps of the Mediterranean Summary: Our survey of pre-1750 cartographic works reveals a rich and complex evolution of the longitude of the Mediterranean (LongMed). While confirming several previously docu- mented trends − e.g. the adoption of erroneous Ptolemaic longitudes by 15th and 16th-century European cartographers, or the striking accuracy of Arabic-language tables of coordinates−, we have observed accurate LongMed values largely unnoticed by historians in 16th-century maps and noted that widely diverging LongMed values coexisted up to 1750, sometimes even within the works of one same author. -
1. Quellen 2. Geozentrische Weltbilder 2.1 Heutige Naive Vorstellung 2.2
1. Quellen 2. Geozentrische Weltbilder 2.1 Heutige naive Vorstellung 2.2 Epizykel 2.3 Exzenter Alfred Holl 2.4 Untere Planeten Weltmodelle im Mittelalter 3. Heliozentrisch-geostationär 4. Heliozentrisch-heliostationär Vom geozentrischen zum heliozentrischen Weltbild 5. Astronomische Tafeln (Erfurt CA 2° 19, 78v) Alfred Holl, Weltmodelle 09.03.2013/1 1. Quellen 1.1 Deutsche Sphära Konrad von Megenberg (~1309-1374) Deutsche Sphära wahrscheinlich zwischen 1340 und 1349 in Wien Cgm 156, Cgm 328, Graz II/470 ed. Matthaei 1912 ed. Brévart 1980 (Deutsche Sphaera, Cgm 156, 1r aus Mai, Paul: Ausstellungskatalog, 2009, 155) Alfred Holl, Weltmodelle 09.03.2013/2 1. Quellen Quellen (alle basierend auf Ptolemaios): 1.1 Deutsche Sphära Johannes von Sacrobosco (~1200-~1256) Tractatus de sphaera materiali 1233 Entstehung bis in 16. Jh. universitäre Astronomie-Einführung (ed. Thorndyke 1949, Brévart 1980) auf der Basis von al-Fargani (~863), De scientia astrorum übers. von Johannes Hispalensis (akt. 1135-1153) (ed. Campani 1910, Carmody 1943) al-Battani (-929), Opus astronomicum / Zig übersetzt von Plato von Tivoli (aktiv 1134-1145) (ed. Nallino 1903) Kommentare zu Sacrobosco (z.B. Cecco d’Ascoli) (Cgm 156, 1r) Puechlein von der Spera (~1375) (ed. Brévart 1979) Alfred Holl, Weltmodelle 09.03.2013/3 1. Quellen 1.2 Französische volkssprachliche Sphära Nicole Oresme (~1323-1382) Traité de l’espère (zwischen 1362 und 1377) (ed. Myers 1940, McCarthy 1943) ebenfalls auf der Basis von Johannes von Sacrobosco Nicole Oresme mit Armillarsphäre (www.nicole-oresme.com) (Bibliothèque Nationale, Paris, France, fonds français 565, fol. 1r) Alfred Holl, Weltmodelle 09.03.2013/4 1. Quellen 1.3 Autoren und Übersetzer Adelhard von Bath Adelhard (-1142) Gerhard von Cremona (-1187) Plato von Tivoli / Tiburtinus (-1145) Robert von Chester / Reading (-1150) / Hisp. -
Lecture 25.Key
Astronomy 330: Extraterrestrial Life This class (Lecture 25): Evolution of Worldview Sean Sarcu Saloni Sheth ! ! Next Class: Lifetime Vincent Abejuela Cassandra Jensen Music: Astronomy – Metallica 2 x 2 page pdf articles due next Tues Drake Equation Frank That’s 2.7 intelligent systems/year Drake N = R* × fp × ne × fl × fi × fc × L # of # of Star Fraction of Fraction advanced Earthlike Fraction on Fraction that Lifetime of formation stars with that civilizations planets per which life evolve advanced rate planets commun- we can system arises intelligence civilizations icate contact in our Galaxy today 30 0.8 4 x 0.47 0.2 0.3 comm./ yrs/ stars/ systems/ = 1.88 life/ intel./ intel. comm. yr star planets/ planet life system • Requires civilization to undergo three steps: 1. A correct appreciation of the size and nature of the Worldview Universe 2. A realization of their place in the Universe 3. A belief that the odds for life are reasonable. The beings of Q’earth must have taken their Q’astro Intelligent ET Life must want to communicate with us 330 class and came up with a good number of communicable civilizations in the Q’drake This means they MUST equation. believe in the possibility of us (and other ET life) Requirements: ! 1) Understand size and scale of the cosmos ASTR 330 2) Realize their place in the cosmos 3) Believe the odds for life elsewhere are reasonable Alien 3 Our Worldview First worldview: Earth Centric Why? Natural observations imply we are stationary 4 • The Mayans computed the length of year to within a few Ancient Astronomy seconds (0.001%). -
The History of Arabic Sciences: a Selected Bibliography
THE HISTORY OF ARABIC SCIENCES: A SELECTED BIBLIOGRAPHY Mohamed ABATTOUY Fez University Max Planck Institut für Wissenschaftsgeschichte, Berlin A first version of this bibliography was presented to the Group Frühe Neuzeit (Max Planck Institute for History of Science, Berlin) in April 1996. I revised and expanded it during a stay of research in MPIWG during the summer 1996 and in Fez (november 1996). During the Workshop Experience and Knowledge Structures in Arabic and Latin Sciences, held in the Max Planck Institute for the History of Science in Berlin on December 16-17, 1996, a limited number of copies of the present Bibliography was already distributed. Finally, I express my gratitude to Paul Weinig (Berlin) for valuable advice and for proofreading. PREFACE The principal sources for the history of Arabic and Islamic sciences are of course original works written mainly in Arabic between the VIIIth and the XVIth centuries, for the most part. A great part of this scientific material is still in original manuscripts, but many texts had been edited since the XIXth century, and in many cases translated to European languages. In the case of sciences as astronomy and mechanics, instruments and mechanical devices still extant and preserved in museums throughout the world bring important informations. A total of several thousands of mathematical, astronomical, physical, alchemical, biologico-medical manuscripts survived. They are written mainly in Arabic, but some are in Persian and Turkish. The main libraries in which they are preserved are those in the Arabic World: Cairo, Damascus, Tunis, Algiers, Rabat ... as well as in private collections. Beside this material in the Arabic countries, the Deutsche Staatsbibliothek in Berlin, the Biblioteca del Escorial near Madrid, the British Museum and the Bodleian Library in England, the Bibliothèque Nationale in Paris, the Süleymaniye and Topkapi Libraries in Istanbul, the National Libraries in Iran, India, Pakistan.. -
Bīrūnī's Telescopic-Shape Instrument for Observing the Lunar
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Revistes Catalanes amb Accés Obert Bīrūnī’s Telescopic-Shape Instrument for Observing the Lunar Crescent S. Mohammad Mozaffari and Georg Zotti Abstract:This paper deals with an optical aid named barbakh that Abū al-Ray¬ān al- Bīrūnī (973–1048 AD) proposes for facilitating the observation of the lunar crescent in his al-Qānūn al-Mas‘ūdī VIII.14. The device consists of a long tube mounted on a shaft erected at the centre of the Indian circle, and can rotate around itself and also move in the vertical plane. The main function of this sighting tube is to provide an observer with a darkened environment in order to strengthen his eyesight and give him more focus for finding the narrow crescent near the western horizon about the beginning of a lunar month. We first briefly review the history of altitude-azimuthal observational instruments, and then present a translation of Bīrūnī’s account, visualize the instrument in question by a 3D virtual reconstruction, and comment upon its structure and applicability. Keywords: Astronomical Instrumentation, Medieval Islamic Astronomy, Bīrūnī, Al- Qānūn al-Mas‘ūdī, Barbakh, Indian Circle Introduction: Altitude-Azimuthal Instruments in Islamic Medieval Astronomy. Altitude-azimuthal instruments either are used to measure the horizontal coordinates of a celestial object or to make use of these coordinates to sight a heavenly body. They Suhayl 14 (2015), pp. 167-188 168 S. Mohammad Mozaffari and Georg Zotti belong to the “empirical” type of astronomical instruments.1 None of the classical instruments mentioned in Ptolemy’s Almagest have the simultaneous measurement of both altitude and azimuth of a heavenly object as their main function.2 One of the earliest examples of altitude-azimuthal instruments is described by Abū al-Ray¬ān al- Bīrūnī for the observation of the lunar crescent near the western horizon (the horizontal coordinates are deployed in it to sight the lunar crescent). -
Stellarium for Cultural Astronomy Research
RESEARCH The Simulated Sky: Stellarium for Cultural Astronomy Research Georg Zotti Ludwig Boltzmann Institute for Archaeological Prospection and Virtual Archaeology, Vienna, Austria [email protected] Susanne M. Hoffmann Friedrich-Schiller-Universität Jena, Michael-Stifel-Center/ Institut für Informatik and Physikalisch- Astronomische Fakultät, Jena, Germany [email protected] Alexander Wolf Altai State Pedagogical University, Barnaul, Russia [email protected] Fabien Chéreau Stellarium Labs, Toulouse, France [email protected] Guillaume Chéreau Noctua Software, Hong Kong [email protected] Abstract: For centuries, the rich nocturnal environment of the starry sky could be modelled only by analogue tools such as paper planispheres, atlases, globes and numerical tables. The immer- sive sky simulator of the twentieth century, the optomechanical planetarium, provided new ways for representing and teaching about the sky, but the high construction and running costs meant that they have not become common. However, in recent decades, “desktop planetarium programs” running on personal computers have gained wide attention. Modern incarnations are immensely versatile tools, mostly targeted towards the community of amateur astronomers and for knowledge transfer in transdisciplinary research. Cultural astronomers also value the possibili- ties they give of simulating the skies of past times or other cultures. With this paper, we provide JSA 6.2 (2020) 221–258 ISSN (print) 2055-348X https://doi.org/10.1558/jsa.17822 ISSN (online) 2055-3498 222 Georg Zotti et al. an extended presentation of the open-source project Stellarium, which in the last few years has been enriched with capabilities for cultural astronomy research not found in similar, commercial alternatives. -
ASTR 101L Astronomical Motions I: the Night Sky (Spring)
ASTR 101L Astronomical Motions I: The Night Sky (Spring) Early Greek observers viewed the sky as a transparent sphere which surrounded the Earth. They divided the stars into six categories of brightness and arranged the stars into groupings called constellations (as did many other cultures). Most of the names of the eighty-eight constellations we use today are based on Greek mythology and their Latin translations. Modern astronomy uses the constellation designations to map the sky. On skymaps, the size of the dot is usually related to the brightness of the object (look on your planisphere). Most only show the brightest stars. They are typically named from brightest to faintest using a letter from the Greek alphabet (α, β, γ, etc.) and the constellation name in the genitive form; e.g. alpha (α) Cygni is the brightest star in Cygnus. Many stars also have Arabic names such as Betelgeuse, Algol, and Arcturus; α Cygni is named Deneb and α Ursa Minoris is more commonly known as Polaris. Either designation is correct. In the exercise “Angles and Parallax,” you made a cross-staff and quadrant and learned how to use them to measure objects inside. Now we will use them to measure objects in the night sky, much like Tycho Brahe did in the 1500’s. Remember to record the date, time, and conditions when making any astronomical observations! All numerical data should be recorded to one decimal place. Objectives: . Measure angular separations and altitudes of objects in the night sky with instruments . Estimate angular separations and altitudes of objects in the night sky with your hands . -
Build Your Own Planisphere
Make your own planisphere Dominic Ford 2014{2021 A planisphere is a simple hand-held device which shows a map of which stars are visible in the night sky at any particular time. By rotating a wheel, it shows how stars move across the sky through the night, and how different constellations are visible at different times of year. Here, I present a kit which you can download and print to make your own planisphere out of paper or cardboard. The design of a planisphere depends on the geographic location where it is to be used, since different stars are visible from different places. I have created kits for use at a wide range of latitudes, which you can download from https://in-the-sky.org/planisphere/ The planisphere presented in this document is designed for use at a latitude of 35◦N . What you need • Two sheets of A4 paper, or preferably thin card. • Scissors. • A split-pin fastener. • Optional: one sheet of transparent plastic, e.g. acetate designed for use with overhead projectors. • Optional: A little glue. Assembly instructions Step 1 { Planispheres look slightly different depending on where you live. The planisphere prepared in this document is designed for use anywhere on Earth which is within a few degrees of latitude 35◦N . If you live elsewhere, you should download an alternative kit from https://in-the-sky.org/planisphere/ Step 2 { Print the pages at the back of this PDF file, showing the star wheel and the body of the planisphere, onto two separate sheets of paper, or more preferably onto thin card.