Confluence: Online Journal of World Philosophies, Volume 4
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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 -
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. -
The Copernican Revolution (1957) Is a Decidedly Non-Revolutionary Astronomer Who Unwittingly Ignited a Conceptual Revolution in the European Worldview
Journal of Applied Cultural Studies vol. 1/2015 Stephen Dersley The Copernican Hypotheses Part 1 Summary. The Copernicus constructed by Thomas S. Kuhn in The Copernican Revolution (1957) is a decidedly non-revolutionary astronomer who unwittingly ignited a conceptual revolution in the European worldview. Kuhn’s reading of Copernicus was crucial for his model of science as a deeply conservative discourse, which presented in The Structure of Scientific Revolutions (1962). This essay argues that Kuhn’s construction of Copernicus and depends on the suppression of the most radical aspects of Copernicus’ thinking, such as the assumptions of the Commentariolus (1509-14) and the conception of hypothesis of De Revolutionibus (1543). After comparing hypo- thetical thinking in the writings of Aristotle and Ptolemy, it is suggested that Copernicus’ concep- tual breakthrough was enabled by his rigorous use of hypothetical thinking. Keywords: N. Copernicus hypothesis, T. S. Kuhn, philosophy of science Stephen Dersley, University of Warwick, Faculty of Social Sciences Alumni, Coventry CV4 7AL, United Kingdom, e-mail: [email protected] Kuhn’s Paradigm n The Copernican Revolution, Thomas Kuhn was at pains to construct an image of ICopernicus as a decidedly non-revolutionary astronomer. Kuhn’s model of scientific revolutions, first embodied in The Copernican Revolution and then generalised to the status of a theory in The Structure of Scientific Revolutions, conceives of science as be- 100 Stephen Dersley ing, for the majority of the time, a deeply conservative activity. In Kuhn’s model, scien- tists who are engaged in the business of doing every day scientific work do so at the behest of of a reigning paradigm that completely dictates their field of enquiry and functions as an imperceptible intellectual strait-jacket. -
1 Science LR 2711
A Scientific Response to the Chester Beatty Library Collection Contents The Roots Of Modern Science A Scientific Response To The Chester Beatty Library Collection 1 Science And Technology 2 1 China 3 Science In Antiquity 4 Golden Age Of Islamic Science 5 Transmission Of Knowledge To Europe 6 A Scientific Response To The Chester Beatty Library Collections For Dublin City Of Science 2012 7 East Asian Collections The Great Encyclopaedia of the Yongle Reign (Yongle Dadian) 8 2 Phenomena of the Sky (Tianyuan yuli xiangyi tushuo) 9 Treatise on Astronomy and Chronology (Tianyuan lili daquan) 10 Illustrated Scrolls of Gold Mining on Sado Island (Sado kinzan zukan) 11 Islamic Collections Islamic Medicine 12 3 Medical Compendium, by al-Razi (Al-tibb al-mansuri) 13 Encyclopaedia of Medicine, by Ibn Sina (Al-qanun fi’l-tibb) 14 Treatise on Surgery, by al-Zahrawi (Al-tasrif li-man ‘ajiza ‘an al-ta’lif) 15 Treatise on Human Anatomy, by Mansur ibn Ilyas (Tashrih al-badan) 16 Barber –Surgeon toolkit from 1860 17 Islamic Astronomy and Mathematics 18 The Everlasting Cycles of Lights, by Muhyi al-Din al-Maghribi (Adwar al-anwar mada al-duhur wa-l-akwar) 19 Commentary on the Tadhkira of Nasir al-Din al-Tusi 20 Astrolabes 21 Islamic Technology 22 Abbasid Caliph, Ma’mum at the Hammam 23 European Collections European Science of the Middle Ages 24 4 European Technology: On Military Matters (De Re Militari) 25 European Technology: Concerning Military Matters (De Re Militari) 26 Mining Technology: On the Nature of Metals (De Re Metallica) 27 Fireworks: The triumphal -
The Copernican Revolution, the Scientific Revolution, and The
The Copernican Revolution, the Scientific Revolution, and the Mechanical Philosophy Conor Mayo-Wilson University of Washington Phil. 401 January 19th, 2017 2 Prediction and Explanation, in particular, the role of mathematics, causation, primary and secondary qualities, microsctructure in prediction and explanation, and 3 Empirical Theories, in particular, the place of the earth in the solar system, the composition of matter, and the causes of terrestial and celestial motion. We're on our way to meeting goal three, but we've got two more to go ::: Course Goals By the end of the quarter, students should be able to explain in what ways the mechanical philosophers agreed and disagreed with Aristotle and scholastics about 1 Epistemology, in particular, the role of testimony, authority, experiment, and logic as sources of knowledge, 3 Empirical Theories, in particular, the place of the earth in the solar system, the composition of matter, and the causes of terrestial and celestial motion. We're on our way to meeting goal three, but we've got two more to go ::: Course Goals By the end of the quarter, students should be able to explain in what ways the mechanical philosophers agreed and disagreed with Aristotle and scholastics about 1 Epistemology, in particular, the role of testimony, authority, experiment, and logic as sources of knowledge, 2 Prediction and Explanation, in particular, the role of mathematics, causation, primary and secondary qualities, microsctructure in prediction and explanation, and Course Goals By the end of the quarter, -
Chapter 2: the Copernican Revolution
1 Name________________________ Unit 2: The Copernican Revolution Vocabulary: Define each term below in a complete sentence on a separate sheet of paper. (Terms that are *, please illustrate) Cosmology Retrograde Motion* Geocentric* Epicycle* Deferent* Ptolemaic Model* Heliocentric* Copernican Revolution Ellipse* Focus* Semi-major axis* Eccentricity Perihelion* Aphelion* Sidereal orbital period Escape Velocity* Inertia Mass Newtonian Mechanics Gravitational Field Stonehenge* Acceleration Gravity* A. Ancient Astronomy 1.Where is Stonehenge? When and who built it? -Salisbury Plain, _______________ -Began 2800-finished __________ B.C. -took 1700 years 2.What was Stonehenge’s purpose? -3-dimensional ____________________, for religious and agriculture purposes -brought in large boulders (up to 50 tons) from miles away 3. What ancient cultures were accomplished in ancient astronomy? -Mayans- ____________Temple in Mexico- used for human sacrifices when the planet Venus appeared -Plains Indians- Big Horn Medicine Wheel, ____________________ -Chinese- 12th century, kept accurate records of comets, and a ‘guest star’ later known as a supernova, visible during the __________ -Muslims- a vital link between ancient Greece and the Renaissance (dark ages), saved astronomical data, developed trigonometry, names stars such as Rigel, _____________ and Vega B. The Geocentric Universe 1.What Greek word is the word planet derived from, why did they get this name? -________________—meandering wanderer, stay close to ecliptic, why? 2. Explain the difference between retrograde and prograde motion: -Prograde motion- ___________________ -Retrograde motion- _____________________ 3. What did Aristotle mean by a geocentric universe? -Geo= Earth -___________________________ 4. How was the geocentric Earth explained by epicycle and deferent? -_____________- small orbits -______________- larger orbits C. Model of the Solar System 1.Who was Nicholas Copernicus? -______________________- rediscovered heliocentric model from ancient Greece-Aristarchus 2. -
The Roots of Astronomy
The Roots of Astronomy • Already in the stone and bronze ages, human cultures realized the cyclic nature of motions in the sky. • Monuments dating back to ~ 3000 B.C. show alignments with astronomical significance. • Those monuments were probably used as calendars or even to predict eclipses. Stonehenge • Constructed: 3000 – 1800 B.C. Summer solstice Heelstone • Alignments with locations of sunset, sunrise, moonset and moonrise at summer and winter solstices • Probably used as calendar. Other Examples All Over the World Big Horn Medicine Wheel (Wyoming) Other Examples All Over the World (2) Caracol (Maya culture, approx. A.D. 1000) Ancient Greek Astronomers (1) • Unfortunately, there are no written documents about the significance of stone and bronze age monuments. • First preserved written documents about ancient astronomy are from ancient Greek philosophy. • Greeks tried to understand the motions of the sky and describe them in terms of mathematical (not physical!) models. Ancient Greek Astronomers (2) Models were generally wrong because they were based on wrong “first principles”, believed to be “obvious” and not questioned: 1. Geocentric Universe: Earth at the Center of the Universe. 2. “Perfect Heavens”: Motions of all celestial bodies described by motions involving objects of “perfect” shape, i.e., spheres or circles. Ancient Greek Astronomers (3) • Eudoxus (409 – 356 B.C.): Model of 27 nested spheres • Aristotle (384 – 322 B.C.), major authority of philosophy until the late middle ages: Universe can be divided in 2 parts: 1. Imperfect, -
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.. -
The Persian-Toledan Astronomical Connection and the European Renaissance
Academia Europaea 19th Annual Conference in cooperation with: Sociedad Estatal de Conmemoraciones Culturales, Ministerio de Cultura (Spain) “The Dialogue of Three Cultures and our European Heritage” (Toledo Crucible of the Culture and the Dawn of the Renaissance) 2 - 5 September 2007, Toledo, Spain Chair, Organizing Committee: Prof. Manuel G. Velarde The Persian-Toledan Astronomical Connection and the European Renaissance M. Heydari-Malayeri Paris Observatory Summary This paper aims at presenting a brief overview of astronomical exchanges between the Eastern and Western parts of the Islamic world from the 8th to 14th century. These cultural interactions were in fact vaster involving Persian, Indian, Greek, and Chinese traditions. I will particularly focus on some interesting relations between the Persian astronomical heritage and the Andalusian (Spanish) achievements in that period. After a brief introduction dealing mainly with a couple of terminological remarks, I will present a glimpse of the historical context in which Muslim science developed. In Section 3, the origins of Muslim astronomy will be briefly examined. Section 4 will be concerned with Khwârizmi, the Persian astronomer/mathematician who wrote the first major astronomical work in the Muslim world. His influence on later Andalusian astronomy will be looked into in Section 5. Andalusian astronomy flourished in the 11th century, as will be studied in Section 6. Among its major achievements were the Toledan Tables and the Alfonsine Tables, which will be presented in Section 7. The Tables had a major position in European astronomy until the advent of Copernicus in the 16th century. Since Ptolemy’s models were not satisfactory, Muslim astronomers tried to improve them, as we will see in Section 8. -
Astro110-01 Lecture 7 the Copernican Revolution
Astro110-01 Lecture 7 The Copernican Revolution or the revolutionaries: Nicolas Copernicus (1473-1543) Tycho Brahe (1546-1601) Johannes Kepler (1571-1630) Galileo Galilei (1564-1642) Isaac Newton (1642-1727) who toppled Aristotle’s cosmos 2/2/09 Astro 110-01 Lecture 7 1 Recall: The Greek Geocentric Model of the heavenly spheres (around 400 BC) • Earth is a sphere that rests in the center • The Moon, Sun, and the planets each have their own spheres • The outermost sphere holds the stars • Most famous players: Aristotle and Plato 2/2/09 Aristotle Plato Astro 110-01 Lecture 7 2 But this made it difficult to explain the apparent retrograde motion of planets… Over a period of 10 weeks, Mars appears to stop, back up, then go forward again. Mars Retrograde Motion 2/2/09 Astro 110-01 Lecture 7 3 A way around the problem • Plato had decreed that in the heavens only circular motion was possible. • So, astronomers concocted the scheme of having the planets move in circles, called epicycles, that were themselves centered on other circles, called deferents • If an observation of a planet did not quite fit the existing system of deferents and epicycles, another epicycle could be added to improve the accuracy • This ancient system of astronomy was codified by the Alexandrian Greek astronomer Ptolemy (A.D. 100–170), in a book translated into Arabic and called Almagest. • Almagest remained the principal textbook of astronomy for 1400 years until Copernicus 2/2/09 Astro 110-01 Lecture 7 4 So how does the Ptolemaic model explain retrograde motion? Planets really do go backward in this model. -
A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair
ASTRONOMY AND ASTROPHYSICS - A History of Astronomy, Astrophysics and Cosmology - Malcolm Longair A HISTORY OF ASTRONOMY, ASTROPHYSICS AND COSMOLOGY Malcolm Longair Cavendish Laboratory, University of Cambridge, JJ Thomson Avenue, Cambridge CB3 0HE Keywords: History, Astronomy, Astrophysics, Cosmology, Telescopes, Astronomical Technology, Electromagnetic Spectrum, Ancient Astronomy, Copernican Revolution, Stars and Stellar Evolution, Interstellar Medium, Galaxies, Clusters of Galaxies, Large- scale Structure of the Universe, Active Galaxies, General Relativity, Black Holes, Classical Cosmology, Cosmological Models, Cosmological Evolution, Origin of Galaxies, Very Early Universe Contents 1. Introduction 2. Prehistoric, Ancient and Mediaeval Astronomy up to the Time of Copernicus 3. The Copernican, Galilean and Newtonian Revolutions 4. From Astronomy to Astrophysics – the Development of Astronomical Techniques in the 19th Century 5. The Classification of the Stars – the Harvard Spectral Sequence 6. Stellar Structure and Evolution to 1939 7. The Galaxy and the Nature of the Spiral Nebulae 8. The Origins of Astrophysical Cosmology – Einstein, Friedman, Hubble, Lemaître, Eddington 9. The Opening Up of the Electromagnetic Spectrum and the New Astronomies 10. Stellar Evolution after 1945 11. The Interstellar Medium 12. Galaxies, Clusters Of Galaxies and the Large Scale Structure of the Universe 13. Active Galaxies, General Relativity and Black Holes 14. Classical Cosmology since 1945 15. The Evolution of Galaxies and Active Galaxies with Cosmic Epoch 16. The Origin of Galaxies and the Large-Scale Structure of The Universe 17. The VeryUNESCO Early Universe – EOLSS Acknowledgements Glossary Bibliography Biographical SketchSAMPLE CHAPTERS Summary This chapter describes the history of the development of astronomy, astrophysics and cosmology from the earliest times to the first decade of the 21st century. -
How Do Planets Move?
How Do Planets Move? 1 We know that the Sun is at the centre of the solar system Eight planets orbit it 2 However, this has not always been believed! 3 These people all believed different things about the solar system. Firstly, when do you think Place them on the timeline these civilizations/people lived? alKatabi Aristotle Ancient Egyptians Plotemy alHazen Tusi Ancient Indians Early Humans Us in 2020 4 For thousands of years, people believed that the Earth was the centre of the solar system. By observing the Sun, during the day, it seemed obvious that it was moving around planet Earth. Early Humans Plotemy Ancient Indians Ancient Egyptians Aristotle 5 Ptolemy’s model became the accepted view for hundreds of years. However, during the time of the Islamic Golden Age, some scientists started to criticise his model. Alhazen was the first to outright disagree with the Ptolemaic Model. Plotemy alHazen 6 Other Islamic scientists explored the idea of heliocentrism. However, Tusi was the first real scientist to propose the Heliocentric Model (what we believe today!)... alHazen Tusi ? To be continued (next lesson)... 7 Activity WALT understand the geocentric model of the solar system Can you draw a diagram to show the geocentric model? Can you summarise the key people who were involved in creating this model of the solar system? 8 Firstly, let's ensure that we remember/can say the name... WALT understand the geocentric model of the solar system What does this What does the root word prefix mean? mean? Geo- is a prefix derived in or at the from a Greek word centre; meaning "earth" central.