Tycho Brahe's Geo- Heliocentric Model of Scientific Explanation: A
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
History of Astrometry
5 Gaia web site: http://sci.esa.int/Gaia site: web Gaia 6 June 2009 June are emerging about the nature of our Galaxy. Galaxy. our of nature the about emerging are More detailed information can be found on the the on found be can information detailed More technologies developed by creative engineers. creative by developed technologies scientists all over the world, and important conclusions conclusions important and world, the over all scientists of the Universe combined with the most cutting-edge cutting-edge most the with combined Universe the of The results from Hipparcos are being analysed by by analysed being are Hipparcos from results The expression of a widespread curiosity about the nature nature the about curiosity widespread a of expression 118218 stars to a precision of around 1 milliarcsecond. milliarcsecond. 1 around of precision a to stars 118218 trying to answer for many centuries. It is the the is It centuries. many for answer to trying created with the positions, distances and motions of of motions and distances positions, the with created will bring light to questions that astronomers have been been have astronomers that questions to light bring will accuracies obtained from the ground. A catalogue was was catalogue A ground. the from obtained accuracies Gaia represents the dream of many generations as it it as generations many of dream the represents Gaia achieving an improvement of about 100 compared to to compared 100 about of improvement an achieving orbit, the Hipparcos satellite observed the whole sky, sky, whole the observed satellite Hipparcos the orbit, ear Y of them in the solar neighbourhood. -
The Astronomers Tycho Brahe and Johannes Kepler
Ice Core Records – From Volcanoes to Supernovas The Astronomers Tycho Brahe and Johannes Kepler Tycho Brahe (1546-1601, shown at left) was a nobleman from Denmark who made astronomy his life's work because he was so impressed when, as a boy, he saw an eclipse of the Sun take place at exactly the time it was predicted. Tycho's life's work in astronomy consisted of measuring the positions of the stars, planets, Moon, and Sun, every night and day possible, and carefully recording these measurements, year after year. Johannes Kepler (1571-1630, below right) came from a poor German family. He did not have it easy growing Tycho Brahe up. His father was a soldier, who was killed in a war, and his mother (who was once accused of witchcraft) did not treat him well. Kepler was taken out of school when he was a boy so that he could make money for the family by working as a waiter in an inn. As a young man Kepler studied theology and science, and discovered that he liked science better. He became an accomplished mathematician and a persistent and determined calculator. He was driven to find an explanation for order in the universe. He was convinced that the order of the planets and their movement through the sky could be explained through mathematical calculation and careful thinking. Johannes Kepler Tycho wanted to study science so that he could learn how to predict eclipses. He studied mathematics and astronomy in Germany. Then, in 1571, when he was 25, Tycho built his own observatory on an island (the King of Denmark gave him the island and some additional money just for that purpose). -
Galileo in Early Modern Denmark, 1600-1650
1 Galileo in early modern Denmark, 1600-1650 Helge Kragh Abstract: The scientific revolution in the first half of the seventeenth century, pioneered by figures such as Harvey, Galileo, Gassendi, Kepler and Descartes, was disseminated to the northernmost countries in Europe with considerable delay. In this essay I examine how and when Galileo’s new ideas in physics and astronomy became known in Denmark, and I compare the reception with the one in Sweden. It turns out that Galileo was almost exclusively known for his sensational use of the telescope to unravel the secrets of the heavens, meaning that he was predominantly seen as an astronomical innovator and advocate of the Copernican world system. Danish astronomy at the time was however based on Tycho Brahe’s view of the universe and therefore hostile to Copernican and, by implication, Galilean cosmology. Although Galileo’s telescope attracted much attention, it took about thirty years until a Danish astronomer actually used the instrument for observations. By the 1640s Galileo was generally admired for his astronomical discoveries, but no one in Denmark drew the consequence that the dogma of the central Earth, a fundamental feature of the Tychonian world picture, was therefore incorrect. 1. Introduction In the early 1940s the Swedish scholar Henrik Sandblad (1912-1992), later a professor of history of science and ideas at the University of Gothenburg, published a series of works in which he examined in detail the reception of Copernicanism in Sweden [Sandblad 1943; Sandblad 1944-1945]. Apart from a later summary account [Sandblad 1972], this investigation was published in Swedish and hence not accessible to most readers outside Scandinavia. -
UC Davis UC Davis Previously Published Works
UC Davis UC Davis Previously Published Works Title The anthropology of incommensurability Permalink https://escholarship.org/uc/item/3vx742f4 Journal Studies in History and Philosophy of Science, 21(2) ISSN 0039-3681 Author Biagioli, M Publication Date 1990 DOI 10.1016/0039-3681(90)90022-Z Peer reviewed eScholarship.org Powered by the California Digital Library University of California MARIO BIAGIOLP’ THE ANTHROPOLOGY OF INCOMMENSURABILITY I. Incommensurability and Sterility SINCE IT entered the discourse of history and philosophy of science with Feyerabend’s “Explanation, Reduction, and Empiricism” and Kuhn’s The Structure of Scient$c Revolutions, the notion of incommensurability has problematized the debate on processes of theory-choice.’ According to Kuhn, two scientific paradigms competing for the explanation of roughly the same set of natural phenomena may not share a global linguistic common denominator. As a result, the possibility of scientific communication and dialogue cannot be taken for granted and the process of theory choice can no longer be reduced to the simple picture presented, for example, by the logical empiricists. By analyzing the dialogue (or rather the lack of it) between Galileo and the Tuscan Aristotelians during the debate on buoyancy in 1611-1613, I want to argue that incommensurability between competing paradigms is not just an unfortunate problem of linguistic communication, but it plays an important role in the process of scientific change and paradigm-speciation. The breakdown of communication during the -
Overturning the Paradigm of Identity with Gilles Deleuze's Differential
A Thesis entitled Difference Over Identity: Overturning the Paradigm of Identity With Gilles Deleuze’s Differential Ontology by Matthew G. Eckel Submitted to the Graduate Faculty as partial fulfillment of the requirements for the Master of Arts Degree in Philosophy Dr. Ammon Allred, Committee Chair Dr. Benjamin Grazzini, Committee Member Dr. Benjamin Pryor, Committee Member Dr. Patricia R. Komuniecki, Dean College of Graduate Studies The University of Toledo May 2014 An Abstract of Difference Over Identity: Overturning the Paradigm of Identity With Gilles Deleuze’s Differential Ontology by Matthew G. Eckel Submitted to the Graduate Faculty as partial fulfillment of the requirements for the Master of Arts Degree in Philosophy The University of Toledo May 2014 Taking Gilles Deleuze to be a philosopher who is most concerned with articulating a ‘philosophy of difference’, Deleuze’s thought represents a fundamental shift in the history of philosophy, a shift which asserts ontological difference as independent of any prior ontological identity, even going as far as suggesting that identity is only possible when grounded by difference. Deleuze reconstructs a ‘minor’ history of philosophy, mobilizing thinkers from Spinoza and Nietzsche to Duns Scotus and Bergson, in his attempt to assert that philosophy has always been, underneath its canonical manifestations, a project concerned with ontology, and that ontological difference deserves the kind of philosophical attention, and privilege, which ontological identity has been given since Aristotle. -
Copernicus and Tycho Brahe
THE NEWTONIAN REVOLUTION – Part One Philosophy 167: Science Before Newton’s Principia Class 2 16th Century Astronomy: Copernicus and Tycho Brahe September 9, 2014 TABLE OF CONTENTS I. The Copernican Revolution .................................................................................................................. 1 A. Ptolemaic Astronomy: e.g. Longitudes of Mars ................................................................... 1 B. A Problem Raised for Philosophy of Science ....................................................................... 2 C. Background: 13 Centuries of Ptolemaic Astronomy ............................................................. 4 D. 15th Century Planetary Astronomy: Regiomantanus ............................................................. 5 E. Nicolaus Copernicus: A Brief Biography .............................................................................. 6 F. Copernicus and Ibn al-Shāţir (d. 1375) ……………………………………………………. 7 G. The Many Different Copernican Revolutions ........................................................................ 9 H. Some Comments on Kuhn’s View of Science ……………………………………………... 10 II. De Revolutionibus Orbium Coelstium (1543) ..................................................................................... 11 A. From Basic Ptolemaic to Basic Copernican ........................................................................... 11 B. A New Result: Relative Orbital Radii ................................................................................... 12 C. Orbital -
The Nova Stella and Its Observers
Running title: Nova stella 1572 AD The Nova Stella and its Observers P. Ruiz–Lapuente ∗,∗∗ 1. Introduction In 1572, physicists were still living with the concepts of mechanics inherited from Aris- totle and with the classification of the elements from the Greek philosopher. The growing criticism towards the Aristotelian views on the natural world could not turn very produc- tive, because the necessary elements of calculus and the empirical tools to move into a better frame were still lacking. However, in astronomy, observers had witnessed by that time the comet of 1556 and they would witness a new one in 1577. Moreover, since 1543 when De Revolutionibus Orbium Caelestium by Copernicus came to light, the apparent motion of the planets had a radically different explanation from the ortodox geocentrism. The new helio- centric view slowly won supporters among astronomers. The explanations concerning the planetary motions would depart from the “common sense” intuitions that had placed the earth sitting still at the center of the planetary system. Thus the “nova stella” in 1572 happened in the middle of the geocentric–versus–heliocentric debate. The other “nova”, the one that would be observed in 1604 by Kepler, came just shortly after the posthumous publication of Tycho Brahe’s Astronomiae Instauratae Progymnasmata1 which contains most of the debates in relation to the appearance of the “new star”2. arXiv:astro-ph/0502399v1 21 Feb 2005 The machinery moving the planetary spheres, i.e. the intrincate system of solid spheres rotating by the motion imparted to them as the wheels in a clock, was not directly affected by the new heliocentric proposal. -
Three Editions of the Star Catalogue of Tycho Brahe*
A&A 516, A28 (2010) Astronomy DOI: 10.1051/0004-6361/201014002 & c ESO 2010 Astrophysics Three editions of the star catalogue of Tycho Brahe Machine-readable versions and comparison with the modern Hipparcos Catalogue F. Verbunt1 andR.H.vanGent2,3 1 Astronomical Institute, Utrecht University, PO Box 80 000, 3508 TA Utrecht, The Netherlands e-mail: [email protected] 2 URU-Explokart, Faculty of Geosciences, Utrecht University, PO Box 80 115, 3508 TC Utrecht, The Netherlands 3 Institute for the History and Foundations of Science, PO Box 80 000, 3508 TA Utrecht, The Netherlands Received 6 January 2010 / Accepted 3 February 2010 ABSTRACT Tycho Brahe completed his catalogue with the positions and magnitudes of 1004 fixed stars in 1598. This catalogue circulated in manuscript form. Brahe edited a shorter version with 777 stars, printed in 1602, and Kepler edited the full catalogue of 1004 stars, printed in 1627. We provide machine-readable versions of the three versions of the catalogue, describe the differences between them and briefly discuss their accuracy on the basis of comparison with modern data from the Hipparcos Catalogue. We also compare our results with earlier analyses by Dreyer (1916, Tychonis Brahe Dani Scripta Astronomica, Vol. II) and Rawlins (1993, DIO, 3, 1), finding good overall agreement. The magnitudes given by Brahe correlate well with modern values, his longitudes and latitudes have error distributions with widths of 2, with excess numbers of stars with larger errors (as compared to Gaussian distributions), in particular for the faintest stars. Errors in positions larger than 10, which comprise about 15% of the entries, are likely due to computing or copying errors. -
Cosmology, Extraterrestrial Life, and the Development and Character Of
COSMOLOGY, EXTRATERRESTRIAL LIFE, AND THE DEVELOPMENT AND CHARACTER OF WESTERN EUROPEAN THOUGHT IN THE SEVENTEENTH AND EIGHTEENTH CENTURIES Emily Simpson, B.A. Thesis Prepared for the Degree of MASTER OF ARTS UNIVERSITY OF NORTH TEXAS August 2011 APPROVED: Marilyn Morris, Major Professor Laura Stern, Committee Member Michael Leggiere, Committee Member Richard B. McCaslin, Chair of the Department of History James D. Meernik, Acting Dean of the Toulouse Graduate School Simpson, Emily. Cosmology, Extraterrestrial Life, and the Development and Character of Western European Thought in the Seventeenth and Eighteenth Centuries. Master of Arts (History), August 2011, 108 pp., 132 titles. Cosmology, as an all-encompassing theoretical construction of universal reality, serves as one of the best indicators for a variety of philosophical, scientific, and cultural values. Within any cosmological system, the question of extraterrestrial life is an important element. Mere existence or nonexistence, however, only exposes a small portion of the ideological significance behind the contemplation of life outside of earth. The manners by which both believers and disbelievers justify their opinions and the ways they characterize other worlds and their inhabitants show much more about the particular ideas behind such decisions and the general climate of thought surrounding those who consider the topic. By exploring both physical and abstract structures of the universe, and specifically concepts on the plurality of worlds and extraterrestrial life, Western European thought in the seventeenth and eighteenth centuries reveals not an era of pure advancement and modernization, but as a time of both tradition and change. Copyright 2011 by Emily Simpson ii TABLE OF CONTENTS CHAPTERS Page 1 INTRODUCTION……………………………………………………………………………1 2 THE POSITION AND QUALITIES OF EARTH, PHYSICAL AND METAPHYSICAL 154 3 MAN’S PLACE IN THE COSMOS .................................................................................. -
History of Astronomy
NASE publications History of Astronomy History of Astronomy Jay Pasachoff, Magda Stavinschi, Mary Kay Hemenway International Astronomical Union, Williams College (Massachusetts, USA), Astronomical Institute of the Romanian Academy (Bucarest, Romania), University of Texas (Austin, USA) Summary This short survey of the History of Astronomy provides a brief overview of the ubiquitous nature of astronomy at its origins, followed by a summary of the key events in the development of astronomy in Western Europe to the time of Isaac Newton. Goals • Give a schematic overview of the history of astronomy in different areas throughout the world, in order to show that astronomy has always been of interest to all the people. • List the main figures in the history of astronomy who contributed to major changes in approaching this discipline up to Newton: Tycho Brahe, Copernicus, Kepler and Galileo. • Conference time constraints prevent us from developing the history of astronomy in our days, but more details can be found in other chapters of this book Pre-History With dark skies, ancient peoples could see the stars rise in the eastern part of the sky, move upward, and set in the west. In one direction, the stars moved in tiny circles. Today, when we look north, we see a star at that position – the North Star, or Polaris. It isn't a very bright star: 48 stars in the sky are brighter than it, but it happens to be in an interesting place. In ancient times, other stars were aligned with Earth's north pole, or sometimes, there were no stars in the vicinity of the pole. -
Bajodah Abdulrahman.Pdf
CEU eTD Collection ABSTRACT The aim of my inquiry is to examine Ikhwan al-Safa’s (“Brethren of Purity”) creationist arguments against the Aristotelian doctrine of the world’s eternity. Arguing for creationism, Ikhwan al-Safa employ the Neoplatonic emanation theory as it is developed in their tenth- century Arabic encyclopedia. However, some historians have claimed that Ikhwan al-Safa’s emanation theory is a veiled attack on creationism that embraces the Aristotelian doctrine of the world’s eternity. Ikhwan al-Safa’s philosophical project is thus characterized as a project that aims either to reconcile or propagate a presupposed conflict between philosophy and religion, expressed for instance in this tension between Aristotelianism and creationism. This characterization allegedly lurks behind opposing historical testimonies regarding Ikhwan al- Safa’s identity and doctrine which I claim is contemporarily reproduced in similar terms with Ikhwan al-Safa’s scholarship. While both historical and contemporary characterizations tempt a double reading approach to Ikhwan al-Safa’s philosophy, I consider their philosophical project within the tradition of early Arabic philosophy, whose enterprise can be characterized as a natural theology project which does not presuppose a conflict between philosophy and religion. While Ikhwan al-Safa identify the philosophical tension between creationism and the world’s eternity doctrine, I demonstrate that Ikhwan al-Safa use emanation theory rather to substantiate their creationist arguments in light of their overall identification of creation with emanation. Consequently, Ikhwan al-Safa’s reception of Aristotelian and Neoplatonic sources should be recognized as a particular CEU eTD Collection philosophical synthesis of both with creationism, for they did not merely transmit these sources, but assimilated them into the Islamic context of 10th century Iraq.