Abd Al-Rahman Al-Sufi and His Book of the Fixed Stars: a Journey of Re-Discovery
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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. -
1 Timeline 2 Geocentric Model
Ancient Astronomy Many ancient cultures were interested in the night sky • Calenders • Prediction of seasons • Navigation 1 Timeline Astronomy timeline • ∼ 3000 B.C. Stonehenge • 2136 B.C. First record of solar eclipse by Chinese astronomers • 613 B.C. First record of Halley’s comet by Zuo Zhuan (China) • ∼ 270 B.C. Aristarchus proposes Earth goes around Sun (not a popular idea at the time) • ∼ 240 B.C. Eratosthenes estimates Earth’s circumference • ∼ 130 B.C. Hipparchus develops first accurate star map (one of the first to use R.A. and Dec) 2 Geocentric model The Geocentric Model • Greek philosopher Aristotle (384-322 B.C.) • Uniform circular motion • Earth at center of Universe Retrograde Motion • General motion of planets east- ward • Short periods of westward motion of planets • Then continuation eastward How did the early Greek philosophers make retrograde motion consistent with uniform circular motion? 3 Ptolemy Ptolemy’s Geocentric Model • Planet moves around a small circle called an epicycle • Center of epicycle moves along a larger cir- cle called a deferent • Center of deferent is at center of Earth (sort of) Ptolemy’s Geocentric Model • Ptolemy invented the device called the eccentric • The eccentric is the center of the deferent • Sometimes the eccentric was slightly off center from the center of the Earth Ptolemy’s Geocentric Model • Uniform circular motion could not account for speed of the planets thus Ptolemy used a device called the equant • The equant was placed the same distance from the eccentric as the Earth, but on the -
Fixed Stars More Than the Wandering Planets Used by Modern Astrologers
Ancients used the fixed stars more than the wandering planets used by modern astrologers. With improved technical abilities due to software enhancements, the fixed stars are beginning to make a return in present day astrology. The information contained in these pages is just a sampling of the stars and their meanings. It is designed to encourage you to look at the subject in a deeper level. When you blend the meaning of the fixed stars with the natal planets in your chart, it adds a great deal of texture to the understanding of your planet/star combination. I normally use a three degree orb of influence between stars and planets, but the commonly accepted orb is only one degree. A research project I did several years ago indicated that people felt the effects of the stars from this wider distance (which can amount to millions of miles). For example, if the planet Mercury in your natal chart is at 17° Gemini, then you will find on page four that item T is the star Rigel in the Orion constellation. Stars that are in the feet of a constellation are considered to be teacher stars in that they bring higher information down to earth to be used. Mercury represents communications, education, writing, and short trips. Combined, this could be a teacher of higher information, possibly a person who travels or writes as part of the teaching process. Again, this is a partial list of stars. Listed below are some of the books and references I have used. REFERENCE: The interpretations come from Bernadette Brady’s “Book of Fixed Stars”, the Solar Maps software program http://www.bernadettebrady.com/; , Ebertin-Hoffman’s book Fixed Stars,” Vivian Robson’s “The Fixed Stars & Constellations in Astrology” and miscellaneous sources. -
A Philosophical and Historical Analysis of Cosmology from Copernicus to Newton
University of Central Florida STARS Electronic Theses and Dissertations, 2004-2019 2017 Scientific transformations: a philosophical and historical analysis of cosmology from Copernicus to Newton Manuel-Albert Castillo University of Central Florida Part of the History of Science, Technology, and Medicine Commons Find similar works at: https://stars.library.ucf.edu/etd University of Central Florida Libraries http://library.ucf.edu This Masters Thesis (Open Access) is brought to you for free and open access by STARS. It has been accepted for inclusion in Electronic Theses and Dissertations, 2004-2019 by an authorized administrator of STARS. For more information, please contact [email protected]. STARS Citation Castillo, Manuel-Albert, "Scientific transformations: a philosophical and historical analysis of cosmology from Copernicus to Newton" (2017). Electronic Theses and Dissertations, 2004-2019. 5694. https://stars.library.ucf.edu/etd/5694 SCIENTIFIC TRANSFORMATIONS: A PHILOSOPHICAL AND HISTORICAL ANALYSIS OF COSMOLOGY FROM COPERNICUS TO NEWTON by MANUEL-ALBERT F. CASTILLO A.A., Valencia College, 2013 B.A., University of Central Florida, 2015 A thesis submitted in partial fulfillment of the requirements for the degree of Master of Arts in the department of Interdisciplinary Studies in the College of Graduate Studies at the University of Central Florida Orlando, Florida Fall Term 2017 Major Professor: Donald E. Jones ©2017 Manuel-Albert F. Castillo ii ABSTRACT The purpose of this thesis is to show a transformation around the scientific revolution from the sixteenth to seventeenth centuries against a Whig approach in which it still lingers in the history of science. I find the transformations of modern science through the cosmological models of Nicholas Copernicus, Johannes Kepler, Galileo Galilei and Isaac Newton. -
Introduction to Astronomy from Darkness to Blazing Glory
Introduction to Astronomy From Darkness to Blazing Glory Published by JAS Educational Publications Copyright Pending 2010 JAS Educational Publications All rights reserved. Including the right of reproduction in whole or in part in any form. Second Edition Author: Jeffrey Wright Scott Photographs and Diagrams: Credit NASA, Jet Propulsion Laboratory, USGS, NOAA, Aames Research Center JAS Educational Publications 2601 Oakdale Road, H2 P.O. Box 197 Modesto California 95355 1-888-586-6252 Website: http://.Introastro.com Printing by Minuteman Press, Berkley, California ISBN 978-0-9827200-0-4 1 Introduction to Astronomy From Darkness to Blazing Glory The moon Titan is in the forefront with the moon Tethys behind it. These are two of many of Saturn’s moons Credit: Cassini Imaging Team, ISS, JPL, ESA, NASA 2 Introduction to Astronomy Contents in Brief Chapter 1: Astronomy Basics: Pages 1 – 6 Workbook Pages 1 - 2 Chapter 2: Time: Pages 7 - 10 Workbook Pages 3 - 4 Chapter 3: Solar System Overview: Pages 11 - 14 Workbook Pages 5 - 8 Chapter 4: Our Sun: Pages 15 - 20 Workbook Pages 9 - 16 Chapter 5: The Terrestrial Planets: Page 21 - 39 Workbook Pages 17 - 36 Mercury: Pages 22 - 23 Venus: Pages 24 - 25 Earth: Pages 25 - 34 Mars: Pages 34 - 39 Chapter 6: Outer, Dwarf and Exoplanets Pages: 41-54 Workbook Pages 37 - 48 Jupiter: Pages 41 - 42 Saturn: Pages 42 - 44 Uranus: Pages 44 - 45 Neptune: Pages 45 - 46 Dwarf Planets, Plutoids and Exoplanets: Pages 47 -54 3 Chapter 7: The Moons: Pages: 55 - 66 Workbook Pages 49 - 56 Chapter 8: Rocks and Ice: -
Glossary Glossary
Glossary Glossary Albedo A measure of an object’s reflectivity. A pure white reflecting surface has an albedo of 1.0 (100%). A pitch-black, nonreflecting surface has an albedo of 0.0. The Moon is a fairly dark object with a combined albedo of 0.07 (reflecting 7% of the sunlight that falls upon it). The albedo range of the lunar maria is between 0.05 and 0.08. The brighter highlands have an albedo range from 0.09 to 0.15. Anorthosite Rocks rich in the mineral feldspar, making up much of the Moon’s bright highland regions. Aperture The diameter of a telescope’s objective lens or primary mirror. Apogee The point in the Moon’s orbit where it is furthest from the Earth. At apogee, the Moon can reach a maximum distance of 406,700 km from the Earth. Apollo The manned lunar program of the United States. Between July 1969 and December 1972, six Apollo missions landed on the Moon, allowing a total of 12 astronauts to explore its surface. Asteroid A minor planet. A large solid body of rock in orbit around the Sun. Banded crater A crater that displays dusky linear tracts on its inner walls and/or floor. 250 Basalt A dark, fine-grained volcanic rock, low in silicon, with a low viscosity. Basaltic material fills many of the Moon’s major basins, especially on the near side. Glossary Basin A very large circular impact structure (usually comprising multiple concentric rings) that usually displays some degree of flooding with lava. The largest and most conspicuous lava- flooded basins on the Moon are found on the near side, and most are filled to their outer edges with mare basalts. -
Ptolemy's Almagest
Ptolemy’s Almagest: Fact and Fiction Richard Fitzpatrick Department of Physics, UT Austin Euclid’s Elements and Ptolemy’s Almagest • Ancient Greece -> Two major scientific works: Euclid’s Elements and Ptolemy’s “Almagest”. • Elements -> Compendium of mathematical theorems concerning geometry, proportion, number theory. Still highly regarded. • Almagest -> Comprehensive treatise on ancient Greek astronomy. (Almost) universally disparaged. Popular Modern Criticisms of Ptolemy’s Almagest • Ptolemy’s approach shackled by Aristotelian philosophy -> Earth stationary; celestial bodies move uniformly around circular orbits. • Mental shackles lead directly to introduction of epicycle as kludge to explain retrograde motion without having to admit that Earth moves. • Ptolemy’s model inaccurate. Lead later astronomers to add more and more epicycles to obtain better agreement with observations. • Final model hopelessly unwieldy. Essentially collapsed under own weight, leaving field clear for Copernicus. Geocentric Orbit of Sun SS Sun VE − vernal equinox SPRING SS − summer solstice AE − autumn equinox WS − winter solstice SUMMER93.6 92.8 Earth AE VE AUTUMN89.9 88.9 WINTER WS Successive passages though VE every 365.24 days Geocentric Orbit of Mars Mars E retrograde station direct station W opposition retrograde motion Earth Period between successive oppositions: 780 (+29/−16) days Period between stations and opposition: 36 (+6/−6) days Angular extent of retrograde arc: 15.5 (+3/−5) degrees Immovability of Earth • By time of Aristotle, ancient Greeks knew that Earth is spherical. Also, had good estimate of its radius. • Ancient Greeks calculated that if Earth rotates once every 24 hours then person standing on equator moves west to east at about 1000 mph. -
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. -
Ibrāhīm Ibn Sinān Ibn Thābit Ibn Qurra
From: Thomas Hockey et al. (eds.). The Biographical Encyclopedia of Astronomers, Springer Reference. New York: Springer, 2007, p. 574 Courtesy of http://dx.doi.org/10.1007/978-0-387-30400-7_697 Ibrāhīm ibn Sinān ibn Thābit ibn Qurra Glen Van Brummelen Born Baghdad, (Iraq), 908/909 Died Baghdad, (Iraq), 946 Ibrāhīm ibn Sinān was a creative scientist who, despite his short life, made numerous important contributions to both mathematics and astronomy. He was born to an illustrious scientific family. As his name suggests his grandfather was the renowned Thābit ibn Qurra; his father Sinān ibn Thābit was also an important mathematician and physician. Ibn Sinān was productive from an early age; according to his autobiography, he began his research at 15 and had written his first work (on shadow instruments) by 16 or 17. We have his own word that he intended to return to Baghdad to make observations to test his astronomical theories. He did return, but it is unknown whether he made his observations. Ibn Sinān died suffering from a swollen liver. Ibn Sinān's mathematical works contain a number of powerful and novel investigations. These include a treatise on how to draw conic sections, useful for the construction of sundials; an elegant and original proof of the theorem that the area of a parabolic segment is 4/3 the inscribed triangle (Archimedes' work on the parabola was not available to the Arabs); a work on tangent circles; and one of the most important Islamic studies on the meaning and use of the ancient Greek technique of analysis and synthesis. -
Al-Biruni: a Great Muslim Scientist, Philosopher and Historian (973 – 1050 Ad)
Al-Biruni: A Great Muslim Scientist, Philosopher and Historian (973 – 1050 Ad) Riaz Ahmad Abu Raihan Muhammad bin Ahmad, Al-Biruni was born in the suburb of Kath, capital of Khwarizmi (the region of the Amu Darya delta) Kingdom, in the territory of modern Khiva, on 4 September 973 AD.1 He learnt astronomy and mathematics from his teacher Abu Nasr Mansur, a member of the family then ruling at Kath. Al-Biruni made several observations with a meridian ring at Kath in his youth. In 995 Jurjani ruler attacked Kath and drove Al-Biruni into exile in Ray in Iran where he remained for some time and exchanged his observations with Al- Khujandi, famous astronomer which he later discussed in his work Tahdid. In 997 Al-Biruni returned to Kath, where he observed a lunar eclipse that Abu al-Wafa observed in Baghdad, on the basis of which he observed time difference between Kath and Baghdad. In the next few years he visited the Samanid court at Bukhara and Ispahan of Gilan and collected a lot of information for his research work. In 1004 he was back with Jurjania ruler and served as a chief diplomat and a spokesman of the court of Khwarism. But in Spring and Summer of 1017 when Sultan Mahmud of Ghazna conquered Khiva he brought Al-Biruni, along with a host of other scholars and philosophers, to Ghazna. Al-Biruni was then sent to the region near Kabul where he established his observatory.2 Later he was deputed to the study of religion and people of Kabul, Peshawar, and Punjab, Sindh, Baluchistan and other areas of Pakistan and India under the protection of an army regiment. -
Sirius - Wikipedia Coordinates: 06 H 4 5 M 08.9 1 7 3 S, −1 6 ° 4 2 ′ 5 8.01 7 ″
12/2/2018 Sirius - Wikipedia Coordinates: 06 h 4 5 m 08.9 1 7 3 s, −1 6 ° 4 2 ′ 5 8.01 7 ″ Sirius Sirius (/ˈsɪriəs/, a romanization of Greek Σείριος, Seirios, lit. "glowing" or "scorching") is a star system Sirius A and B and the brightest star in the Earth's night sky. With a visual apparent magnitude of −1.46, it is almost twice as bright as Canopus, the next brightest star. The system has the Bayer designation Alpha Canis Majoris (α CMa). What the naked eye perceives as a single star is a binary star system, consisting of a white main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, called Sirius B. The distance separating Sirius A from its companion varies between 8.2 and 31.5 AU.[24] Sirius appears bright because of its intrinsic luminosity and its proximity to Earth. At a distance of 2.6 parsecs (8.6 ly), as determined by the Hipparcos astrometry satellite,[2][25][26] the Sirius system is one of Earth's near neighbours. Sirius is gradually moving closer to the Solar System, so it will slightly increase in brightness over the next 60,000 years. After that time its distance will begin to increase and it will become fainter, but it will continue to be the brightest star in the Earth's night sky for the next 210,000 years.[27] The position of Sirius (circled). Sirius A is about twice as massive as the Sun (M☉) and has an absolute visual magnitude of 1.42. -
SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE November 2003 NEWSLETTER
Volume 8, Issue 11 SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE November 2003 NEWSLETTER The sole Newsletter dedicated to Solar Eclipses INDEX 2 SECalendar November Dear SENL reader, 6 Artis planetarium 6 CNN tonight 6 Antiquity of 'Dragon's Head and Tail' When we are finishing this newsletter, some of the die 7 New Sony videocamera with 3 Megapixel CCD hards are on its way to observe the total solar eclipse 8 Total irradiance graph 9 Eclipse retrocalculations of 23 November 2003. Indeed, some of the eclipse 10 Saros 139/144 and 129/134 chasers left with the icebreaker from South Africa to- 11 Question about eclipse seasons 11 Virus wards the Antarctic. Hopefully they will have a safe 11 Nasa Eclipse Site CD journey and we hope of course a safe return. 11 Picture Logo NASA WebPages 12 Fast question...... Many others will leave for Australia and will observe the 13 "Our Mr. Sun" 13 An eclipse/transit calculator for your mobile phone! eclipse from the air. We wish them of course all suc- 14 3d pix of eclipse cess with the observations of the eclipse. Hopefully we 15 25 october Mercury occultation by new moon 16 Giant sunspot approaching the Sun's centre will see some nice images of the eclipses, and their ac- 16 Live solar images , and northern lights counts in a few weeks time. 17 Satellites eclipsed 18 New Moon Oct 2003 The total lunar eclipse is another challenge for this 19 NASA Scientist Dives Into Perfect Space Storm 20 On the shortest time lap between tw o totalities in the same month.