Copernicus, Kepler, Descartes and the Religious Basis for the End to Aristotelian Dogma
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The Influence of Copernicus on Physics
radiosources, obJects believed to be extremely distant. Counts of these The influence of Copernicus sources indicate that their number density is different at large distances on physics from what it is here. Or we may put it differently : the number density of B. Paczynski, Institute of Astronomy, Warsaw radiosources was different a long time ago from what it is now. This is in This month sees the 500th Anniver tific one, and there are some perils contradiction with the strong cosmo sary of the birth of Copernicus. To associated with it. logical principle. Also, the Universe mark the occasion, Europhysics News Why should we not make the cos seems to be filled with a black body has invited B. Paczynski, Polish Board mological principle more perfect ? microwave radiation which has, at member of the EPS Division on Phy Once we say that the Universe is the present, the temperature of 2.7 K. It is sics in Astronomy, to write this article. same everywhere, should we not also almost certain that this radiation was say that it is the same at all times ? produced about 1010 years ago when Once we have decided our place is the Universe was very dense and hot, Copernicus shifted the centre of and matter was in thermal equilibrium the Universe from Earth to the Sun, not unique, why should the time we live in be unique ? In fact such a with radiation. Such conditions are and by doing so he deprived man vastly different from the present kind of its unique position in the Uni strong cosmological principle has been adopted by some scientists. -
Cosmology Timeline
Timeline Cosmology • 2nd Millennium BCEBC Mesopotamian cosmology has a flat,circular Earth enclosed in a cosmic Ocean • 12th century BCEC Rigveda has some cosmological hymns, most notably the Nasadiya Sukta • 6th century BCE Anaximander, the first (true) cosmologist - pre-Socratic philosopher from Miletus, Ionia - Nature ruled by natural laws - Apeiron (boundless, infinite, indefinite), that out of which the universe originates • 5th century BCE Plato - Timaeus - dialogue describing the creation of the Universe, - demiurg created the world on the basis of geometric forms (Platonic solids) • 4th century BCE Aristotle - proposes an Earth-centered universe in which the Earth is stationary and the cosmos, is finite in extent but infinite in time • 3rd century BCE Aristarchus of Samos - proposes a heliocentric (sun-centered) Universe, based on his conclusion/determination that the Sun is much larger than Earth - further support in 2nd century BCE by Seleucus of Seleucia • 3rd century BCE Archimedes - book The Sand Reckoner: diameter of cosmos � 2 lightyears - heliocentric Universe not possible • 3rd century BCE Apollonius of Perga - epicycle theory for lunar and planetary motions • 2nd century CE Ptolemaeus - Almagest/Syntaxis: culmination of ancient Graeco-Roman astronomy - Earth-centered Universe, with Sun, Moon and planets revolving on epicyclic orbits around Earth • 5th-13th century CE Aryabhata (India) and Al-Sijzi (Iran) propose that the Earth rotates around its axis. First empirical evidence for Earth’s rotation by Nasir al-Din al-Tusi. • 8th century CE Puranic Hindu cosmology, in which the Universe goes through repeated cycles of creation, destruction and rebirth, with each cycle lasting 4.32 billion years. • • 1543 Nicolaus Copernicus - publishes heliocentric universe in De Revolutionibus Orbium Coelestium - implicit introduction Copernican principle: Earth/Sun is not special • 1609-1632 Galileo Galilei - by means of (telescopic) observations, proves the validity of the heliocentric Universe. -
Nicolaus Copernicus: the Loss of Centrality
I Nicolaus Copernicus: The Loss of Centrality The mathematician who studies the motions of the stars is surely like a blind man who, with only a staff to guide him, must make a great, endless, hazardous journey that winds through innumerable desolate places. [Rheticus, Narratio Prima (1540), 163] 1 Ptolemy and Copernicus The German playwright Bertold Brecht wrote his play Life of Galileo in exile in 1938–9. It was first performed in Zurich in 1943. In Brecht’s play two worldviews collide. There is the geocentric worldview, which holds that the Earth is at the center of a closed universe. Among its many proponents were Aristotle (384–322 BC), Ptolemy (AD 85–165), and Martin Luther (1483–1546). Opposed to geocentrism is the heliocentric worldview. Heliocentrism teaches that the sun occupies the center of an open universe. Among its many proponents were Copernicus (1473–1543), Kepler (1571–1630), Galileo (1564–1642), and Newton (1643–1727). In Act One the Italian mathematician and physicist Galileo Galilei shows his assistant Andrea a model of the Ptolemaic system. In the middle sits the Earth, sur- rounded by eight rings. The rings represent the crystal spheres, which carry the planets and the fixed stars. Galileo scowls at this model. “Yes, walls and spheres and immobility,” he complains. “For two thousand years people have believed that the sun and all the stars of heaven rotate around mankind.” And everybody believed that “they were sitting motionless inside this crystal sphere.” The Earth was motionless, everything else rotated around it. “But now we are breaking out of it,” Galileo assures his assistant. -
The Planetary Increase of Brightness During Retrograde Motion: an Explanandum Constructed Ad Explanantem
Studies in History and Philosophy of Science 54 (2015) 90e101 Contents lists available at ScienceDirect Studies in History and Philosophy of Science journal homepage: www.elsevier.com/locate/shpsa The planetary increase of brightness during retrograde motion: An explanandum constructed ad explanantem Christián Carlos Carman National University of Quilmes/CONICET, Roque Sáenz Peña 352, B1876BXD Bernal, Buenos Aires, Argentina article info abstract Article history: In Ancient Greek two models were proposed for explaining the planetary motion: the homocentric Received 5 May 2015 spheres of Eudoxus and the Epicycle and Deferent System. At least in a qualitative way, both models Received in revised form could explain the retrograde motion, the most challenging phenomenon to be explained using circular 17 September 2015 motions. Nevertheless, there is another explanandum: during retrograde motion the planets increase their brightness. It is natural to interpret a change of brightness, i.e., of apparent size, as a change in Keywords: distance. Now, while according to the Eudoxian model the planet is always equidistant from the earth, Epicycle; according to the epicycle and deferent system, the planet changes its distance from the earth, Deferent; fi Homocentric spheres; approaching to it during retrograde motion, just as observed. So, it is usually af rmed that the main ’ Brightness change reason for the rejection of Eudoxus homocentric spheres in favor of the epicycle and deferent system was that the first cannot explain the manifest planetary increase of brightness during retrograde motion, while the second can. In this paper I will show that this historical hypothesis is not as firmly founded as it is usually believed to be. -
Space, Time, and Spacetime
Fundamental Theories of Physics 167 Space, Time, and Spacetime Physical and Philosophical Implications of Minkowski's Unification of Space and Time Bearbeitet von Vesselin Petkov 1. Auflage 2010. Buch. xii, 314 S. Hardcover ISBN 978 3 642 13537 8 Format (B x L): 15,5 x 23,5 cm Gewicht: 714 g Weitere Fachgebiete > Physik, Astronomie > Quantenphysik > Relativität, Gravitation Zu Inhaltsverzeichnis schnell und portofrei erhältlich bei Die Online-Fachbuchhandlung beck-shop.de ist spezialisiert auf Fachbücher, insbesondere Recht, Steuern und Wirtschaft. Im Sortiment finden Sie alle Medien (Bücher, Zeitschriften, CDs, eBooks, etc.) aller Verlage. Ergänzt wird das Programm durch Services wie Neuerscheinungsdienst oder Zusammenstellungen von Büchern zu Sonderpreisen. Der Shop führt mehr als 8 Millionen Produkte. The Experimental Verdict on Spacetime from Gravity Probe B James Overduin Abstract Concepts of space and time have been closely connected with matter since the time of the ancient Greeks. The history of these ideas is briefly reviewed, focusing on the debate between “absolute” and “relational” views of space and time and their influence on Einstein’s theory of general relativity, as formulated in the language of four-dimensional spacetime by Minkowski in 1908. After a brief detour through Minkowski’s modern-day legacy in higher dimensions, an overview is given of the current experimental status of general relativity. Gravity Probe B is the first test of this theory to focus on spin, and the first to produce direct and unambiguous detections of the geodetic effect (warped spacetime tugs on a spin- ning gyroscope) and the frame-dragging effect (the spinning earth pulls spacetime around with it). -
The Universe.Pdf
Standard 1: Students will o understand the scientific Terms to know evidence that supports theories o Big Bang Theory that explain how the universe o Doppler Effect and the solar system developed. o Redshift They will compare Earth to other o Universe objects in the solar system. Standard 1, Objective 1: Describe both the big bang theory of universe formation and the nebular theory of solar system formation and evidence supporting them. Lesson Objectives • Explain the evidence for an expanding universe. • Describe the formation of the universe according to the Big Bang Theory. Introduction The study of the universe is called cosmology. Cosmologists study the structure and changes in the present universe. The universe contains all of the star systems, galaxies, gas and dust, plus all the matter and energy that exist. The universe also includes all of space and time. Evolution of Human Understanding of the Universe What did the ancient Greeks recognize as the universe? In their model, the universe contained Earth at the center, the Sun, the Moon, five planets, and a sphere to which all the stars were attached. This idea held for many centuries until Galileo's telescope allowed people to recognize that Earth is not the center of the universe. They also found out that there are many more stars than were visible to the naked eye. All of those stars were in the Milky Way Galaxy. 13 Timeline of cosmological theories 4th century BCE — Aristotle proposes a Geocentric (Earth-centered) universe in which the Earth is stationary and the cosmos (or universe) revolves around the Earth. -
Nicolaus Copernicus
Nicolaus Copernicus Miles Life ● Born February 19, 1473 in Torun, Poland. ● Studied law and medicine at the Universities of Bologna and Padua. ● In 1514, he proposed the Sun as the center of the solar system with the Earth as a planet. ● Died May 24, 1543 in Frombork, Poland. Mathematical Accomplishments ● Copernicus formulated the Quantity Theory of Money It states that money supply has a direct, proportional relationship with the price level. ● He is considered the founder of modern astronomy He applied many principles that we know of in modern astronomy into place. ● His work established the heliocentric model His model put the Sun at the center of the Solar System with the Earth as one planet revolving around the fixed sun. Mathematical Accomplishments: Importance ● Quantity Theory of Money It remains a principal concept in economics. ● Modern Astronomy Modern astronomy is still used as a topic for the progression of humanity. ● Heliocentric Model We still use the heliocentric model as a big part of understanding the universe. Timeline 1473 1490 - 1510 - 1543 1500 1520 Birth Young Life Mid Life Death February 19 in Torun, Royal After four years at university, He proposed the Sun as the May 24 in Frombork, Poland. Prussia, Poland. He was the heh did not graduate, but he center of the solar system youngest of four children of studied law and medicine at with the Earth as a planet, and Nicolaus Copernicus Sr. the Universities of Bologna no one fixed point at the and Padua, then returned to center of the universe. Poland after witnessing a lunar eclipse in Rome in 1500. -
Searching for Monopoles Via Monopolium Multiphoton Decays
CTPU-PTC-21-13, OCHA-PP-365 Searching for Monopoles via Monopolium Multiphoton Decays Neil D. Barrie1y, Akio Sugamoto2z, Matthew Talia3x, and Kimiko Yamashita4{ 1 Center for Theoretical Physics of the Universe, Institute for Basic Science (IBS), Daejeon, 34126, Korea 2Department of Physics, Graduate School of Humanities and Sciences, Ochanomizu University, 2-1-1 Ohtsuka, Bunkyo-ku, Tokyo 112-8610, Japan 3Astrocent, Nicolaus Copernicus Astronomical Center Polish Academy of Sciences, ul. Bartycka 18, 00-716 Warsaw, Poland 4 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China [email protected], [email protected], x [email protected], { [email protected] Abstract We explore the phenomenology of a model of monopolium based on an electromagnetic dual formulation of Zwanziger and lattice gauge theory. The monopole is assumed to have a finite-sized inner structure based on a 't Hooft-Polyakov like solution, with the magnetic charge uniformly distributed on the surface of a sphere. The monopole and anti-monopole potential becomes linear plus Coulomb outside the sphere, analogous to the Cornell potential utilised in the study of quarkonium states. Discovery of a resonance feature in the diphoton channel as well as in a higher multiplicity photon channel would be a smoking gun for the existence arXiv:2104.06931v1 [hep-ph] 14 Apr 2021 of monopoles within this monopolium construction, with the mass and bound state properties extractable. Utilising the current LHC results in the diphoton channel, constraints on the monopole mass are determined for a wide range of model parameters. These are compared to the most recent MoEDAL results and found to be significantly more stringent in certain parameter regions, providing strong motivation for exploring higher multiplicity photon final state searches. -
“Point at Infinity Hape of the World
“Point at Infinity hape of the World Last week, we began a series of posts dedicated to thinking about immortality. If we want to even pretend to think precisely about immortality, we will have to consider some fundamental questions. What does it mean to be immortal? What does it mean to live forever? Are these the same thing? And since immortality is inextricably tied up in one’s relationship with time, we must think about the nature of time itself. Is there a difference between external time and personal time? What is the shape of time? Is time linear? Circular? Finite? Infinite? Of course, we exist not just across time but across space as well, so the same questions become relevant when asked about space. What is the shape of space? Is it finite? Infinite? It is not hard to see how this question would have a significant bearing on our thinking about immortality. In a finite universe (or, more precisely, a universe in which only finitely many different configurations of maer are possible), an immortal being would encounter the same situations over and over again, would think the same thoughts over and over again, would have the same conversations over and over again. Would such a life be desirable? (It is not clear that this repetition would be avoidable even in an infinite universe, but more on that later.) Today, we are going to take a lile historical detour to look at the shape of the universe, a trip that will take us from Ptolemy to Dante to Einstein, a trip that will uncover a remarkable confluence of poetry and physics. -
The Arithmetic of the Spheres
The Arithmetic of the Spheres Je↵ Lagarias, University of Michigan Ann Arbor, MI, USA MAA Mathfest (Washington, D. C.) August 6, 2015 Topics Covered Part 1. The Harmony of the Spheres • Part 2. Lester Ford and Ford Circles • Part 3. The Farey Tree and Minkowski ?-Function • Part 4. Farey Fractions • Part 5. Products of Farey Fractions • 1 Part I. The Harmony of the Spheres Pythagoras (c. 570–c. 495 BCE) To Pythagoras and followers is attributed: pitch of note of • vibrating string related to length and tension of string producing the tone. Small integer ratios give pleasing harmonics. Pythagoras or his mentor Thales had the idea to explain • phenomena by mathematical relationships. “All is number.” A fly in the ointment: Irrational numbers, for example p2. • 2 Harmony of the Spheres-2 Q. “Why did the Gods create us?” • A. “To study the heavens.”. Celestial Sphere: The universe is spherical: Celestial • spheres. There are concentric spheres of objects in the sky; some move, some do not. Harmony of the Spheres. Each planet emits its own unique • (musical) tone based on the period of its orbital revolution. Also: These tones, imperceptible to our hearing, a↵ect the quality of life on earth. 3 Democritus (c. 460–c. 370 BCE) Democritus was a pre-Socratic philosopher, some say a disciple of Leucippus. Born in Abdera, Thrace. Everything consists of moving atoms. These are geometrically• indivisible and indestructible. Between lies empty space: the void. • Evidence for the void: Irreversible decay of things over a long time,• things get mixed up. (But other processes purify things!) “By convention hot, by convention cold, but in reality atoms and• void, and also in reality we know nothing, since the truth is at bottom.” Summary: everything is a dynamical system! • 4 Democritus-2 The earth is round (spherical). -
The Impact of Copernicanism on Judicial Astrology at the English Court, 1543-1660 ______
Clemson University TigerPrints All Theses Theses 1-2011 'In So Many Ways Do the Planets Bear Witness': The mpI act of Copernicanism on Judicial Astrology at the English Court, 1543-1660 Justin Dohoney Clemson University, [email protected] Follow this and additional works at: https://tigerprints.clemson.edu/all_theses Part of the History of Science, Technology, and Medicine Commons Recommended Citation Dohoney, Justin, "'In So Many Ways Do the Planets Bear Witness': The mpI act of Copernicanism on Judicial Astrology at the English Court, 1543-1660" (2011). All Theses. 1143. https://tigerprints.clemson.edu/all_theses/1143 This Thesis is brought to you for free and open access by the Theses at TigerPrints. It has been accepted for inclusion in All Theses by an authorized administrator of TigerPrints. For more information, please contact [email protected]. "IN SO MANY WAYS DO THE PLANETS BEAR WITNESS": THE IMPACT OF COPERNICANISM ON JUDICIAL ASTROLOGY AT THE ENGLISH COURT, 1543-1660 _____________________________________________________ A Thesis Presented to the Graduate School of Clemson University _______________________________________________________ In Partial Fulfillment of the Requirements for the Degree Master of Arts History _______________________________________________________ by Justin Robert Dohoney August 2011 _______________________________________________________ Accepted by: Pamela Mack, Committee Chair Alan Grubb Megan Taylor-Shockley Caroline Dunn ABSTRACT The traditional historiography of science from the late-nineteenth through the mid-twentieth centuries has broadly claimed that the Copernican revolution in astronomy irrevocably damaged the practice of judicial astrology. However, evidence to the contrary suggests that judicial astrology not only continued but actually expanded during the sixteenth and early seventeenth centuries. During this time period, judicial astrologers accomplished this by appropriating contemporary science and mathematics. -
To Save the Phenomena
To Save the Phenomena Prof. David Kaiser Thursday, June 23, 2011, STS.003 Heavens unit Overarching questions: Are representations of astronomical phenomena true or merely useful? How does scientific knowledge travel? I. Ptolemy and the Planets II. Medieval Islamic Astronomy III. Copernican Revolutions Readings: Ptolemy, The Almagest, 5-14, 86-93; Al-Tusi, Memoir on Astronomy, 194-222; Lindberg, Beginnings of Western Science, 85-105. Timeline Ancient Medieval 500 BCE 500 CE 1450 Renaissance Enlightenment 1450 1700 1850 Modern 1850 today Thursday, June 23, 2011, STS.003 Puzzle of the Planets ―planet‖ = ―wanderer‖ 1. Planets roughly follow the path of the sun (within 5˚of the ecliptic). 2. They tend to move W to E over the year, but with varying speeds. 3. They sometimes display retrograde motion. 4. They appear brightest during retrograde. Plato‘s challenge: ―to save the phenomena.‖ ―By the assumption of what uniform and orderly motions can the apparent motions of the planets be accounted for?‖ Retrograde Motion Illustration explaining retrograde motion removed due to copyright restrictions. Mars, 2003 Geocentrism Nearly all of the ancient scholars assumed geocentrism: that the Earth sits at rest in the middle of the cosmos, while the sun, planets, and stars revolve around it. Aristotle, ca. 330 BCE ―[Some people think] there is nothing against their supposing the heavens immobile and the earth as turning on the same axis from west to east very nearly one revolution a day. But it has escaped their notice in the light of what happens around us in the air that such a notion would seem altogether absurd.‖ “That the Earth does not in any way move Aristotle, De Caelo locally” – Ptolemy, Almagest, 1:7 Flat Earth? No! Nearly all Greek scholars assumed that the Earth was a perfect sphere.