Galileo Galilei and the Scientific Revolution Ashley Leidal Junior
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Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
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 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. -
Galileo's Assayer
University of Nevada, Reno Galileo's Assayer: Sense and Reason in the Epistemic Balance A thesis submitted in partial fulfillment of the requirements for the degree of Master of Arts in History. by James A Smith Dr. Bruce Moran/Thesis Advisor May 2018 c by James A Smith 2018 All Rights Reserved THE GRADUATE SCHOOL We recommend that the thesis prepared under our supervision by JAMES A. SMITH entitled Galileo's Assayer: Sense and Reason in the Epistemic Balance be accepted in partial fulfillment of the requirements for the degree of MASTER OF ARTS Bruce Moran, Ph.D., Advisor Edward Schoolman, Ph.D., Committee Member Carlos Mariscal, Ph.D., Committee Member Stanislav Jabuka, Ph.D., Graduate School Representative David W. Zeh, Ph.D., Dean, Graduate School May, 2018 i Abstract Galileo's The Assayer, published in 1623, represents a turning point in Galileo's philo- sophical work. A highly polemical \scientific manifesto," The Assayer was written after his astronomical discoveries of the moons of Jupiter and sunspots on a rotating sun, but before his mature Copernican work on the chief world systems (Ptolemaic versus Copernican). The Assayer included major claims regarding the place of math- ematics in natural philosophy and how the objects of the world and their properties can be known. It's in The Assayer that Galileo wades into the discussion about the ultimate constituents of matter and light, namely, unobservable particles and atoms. Galileo stressed the equal roles that the senses and reason served in the discovery of knowledge, in contradistinction to Aristotelian authoritarian dogma that he found to hinder the processes of discovery and knowledge acquisition. -
On the Infinite in Leibniz's Philosophy
On the Infinite in Leibniz's Philosophy Elad Lison Interdisciplinary Studies Unit Science, Technology and Society Ph.D. Thesis Submitted to the Senate of Bar-Ilan University Ramat-Gan, Israel August 2010 This work was carried out under the supervision of Dr. Ohad Nachtomy (Department of Philosophy), Bar-Ilan University. Contents א.……………………………….…………………………………………Hebrew Abstract Prologue…………………………………………………………...………………………1 Part A: Historic Survey Methodological Introduction…………………………………………………………..15 1. Aristotle: Potential Infinite………………………………………………………….16 2. Thomas Aquinas: God and the Infinite………………………………………..…….27 3. William of Ockham: Syncategorematic and Actual Infinite……………………..….32 4. Rabbi Abraham Cohen Herrera: Between Absolute Unity and Unbounded Multitude………………………………………………………………………..….42 5. Galileo Galilei: Continuum Constructed from Infinite Zero's………………………49 6. René Descartes: Infinite as Indefinite…………………………………………….…58 7. Pierre Gassendi: Rejection of the Infinite…………………………………………...69 8. Baruch Spinoza: Infinite Unity…………………………………………………...…73 9. General Background: Leibniz and the History of the Infinite……………………....81 Summary…………………………………………………………………………….…94 Part B: Mathematics Introduction…………………………………………………………………………….99 1. 'De Arte Combinatoria' as a Formal Basis for Thought: Retrospective on Leibniz's 1666 Dissertation………………………………………………………………....102 2. Leibniz and the Infinitesimal Calculus……………………………………….……111 2.1. Mathematical Background: Mathematical Works in 16th-17th Centuries…..111 2.2. Leibniz's Mathematical Development…………………………………….…127 -
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, -
A New Vision of the Senses in the Work of Galileo Galilei
Perception, 2008, volume 37, pages 1312 ^ 1340 doi:10.1068/p6011 Galileo's eye: A new vision of the senses in the work of Galileo Galilei Marco Piccolino Dipartimento di Biologia, Universita© di Ferrara, I 44100 Ferrara, Italy; e-mail: [email protected] Nicholas J Wade University of Dundee, Dundee DD1 4HN, Scotland, UK Received 4 December 2007 Abstract. Reflections on the senses, and particularly on vision, permeate the writings of Galileo Galilei, one of the main protagonists of the scientific revolution. This aspect of his work has received scant attention by historians, in spite of its importance for his achievements in astron- omy, and also for the significance in the innovative scientific methodology he fostered. Galileo's vision pursued a different path from the main stream of the then contemporary studies in the field; these were concerned with the dioptrics and anatomy of the eye, as elaborated mainly by Johannes Kepler and Christoph Scheiner. Galileo was more concerned with the phenomenology rather than with the mechanisms of the visual process. His general interest in the senses was psychological and philosophical; it reflected the fallacies and limits of the senses and the ways in which scientific knowledge of the world could be gathered from potentially deceptive appearances. Galileo's innovative conception of the relation between the senses and external reality contrasted with the classical tradition dominated by Aristotle; it paved the way for the modern understanding of sensory processing, culminating two centuries later in Johannes Mu« ller's elaboration of the doctrine of specific nerve energies and in Helmholtz's general theory of perception. -
Sacred Rhetorical Invention in the String Theory Movement
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Communication Studies Theses, Dissertations, and Student Research Communication Studies, Department of Spring 4-12-2011 Secular Salvation: Sacred Rhetorical Invention in the String Theory Movement Brent Yergensen University of Nebraska-Lincoln, [email protected] Follow this and additional works at: https://digitalcommons.unl.edu/commstuddiss Part of the Speech and Rhetorical Studies Commons Yergensen, Brent, "Secular Salvation: Sacred Rhetorical Invention in the String Theory Movement" (2011). Communication Studies Theses, Dissertations, and Student Research. 6. https://digitalcommons.unl.edu/commstuddiss/6 This Article is brought to you for free and open access by the Communication Studies, Department of at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Communication Studies Theses, Dissertations, and Student Research by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. SECULAR SALVATION: SACRED RHETORICAL INVENTION IN THE STRING THEORY MOVEMENT by Brent Yergensen A DISSERTATION Presented to the Faculty of The Graduate College at the University of Nebraska In Partial Fulfillment of Requirements For the Degree of Doctor of Philosophy Major: Communication Studies Under the Supervision of Dr. Ronald Lee Lincoln, Nebraska April, 2011 ii SECULAR SALVATION: SACRED RHETORICAL INVENTION IN THE STRING THEORY MOVEMENT Brent Yergensen, Ph.D. University of Nebraska, 2011 Advisor: Ronald Lee String theory is argued by its proponents to be the Theory of Everything. It achieves this status in physics because it provides unification for contradictory laws of physics, namely quantum mechanics and general relativity. While based on advanced theoretical mathematics, its public discourse is growing in prevalence and its rhetorical power is leading to a scientific revolution, even among the public. -
Galileo Galilei by Beatrix Mccrea Galileo Galilei Was an Italian Physicist, Engineer, and Astronomer Bestknown for Disc
3/24/2019 Galileo Galilei - Google Docs Galileo Galilei By Beatrix McCrea Galileo Galilei was an Italian physicist, engineer, and astronomer bestknown for discovering the four largest moons on Jupiter and his theory of gravity. His theory of gravity stated that if a bowling ball and a feather dropped at the same time in space they would land at the same time. He also invented the thermometer and an astronomical telescope. Galileo Galilei was born to Vincenzo Galilei and Giulia Ammanniti in Piza, Italy on February 15, 1564. He was the first of six children. There were two things that happened which led Galileo to find that he loved math and science. On The Famous People the text states “the first incident happened in 1581 when he first noticed that a chandelier despite swinging in small and large arcs took almost the same time to return to the first position.” The other incident was when he accidentally attended a geometry lecture. Both these incidents made Galileo find his love for science. Galileo discovered the four largest moons on Jupiter. On Biography.com it says Galileo Galilei was best known for discovering Jupiter and it’s four biggest moons. The names were Io, Europa, Ganymede, and Callisto. They were discovered by Galileo in January of 1610. Galileo used a better version of the telescope that made him made to see the four moons. Galileo Galilei had a very popular theory of gravity, that if there was no air resistance (like in space) you would drop a bowling ball and a feather and they would land at the exact same time. -
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. -
Galileo Telecommunications
Chapter 4 Galileo Telecommunications Jim Taylor, Kar-Ming Cheung, and Dongae Seo 4.1 Mission and Spacecraft Description This chapter describes how the Galileo orbiter received and transmitted data with the Deep Space Network (DSN). The relay communications subsystems and the link between the Galileo probe and the orbiter are also described briefly. The chapter is at a functional level, intended to illuminate the unique mission requirements and constraints that led to both design of the communications system and how the mission had to be modified and operated in flight. Augmenting the spacecraft downlink design and the supporting ground system for science return with only the low-gain antenna (LGA) was a particular challenge for the Galileo planetary mission. The Galileo orbiter was designed and built at the Jet Propulsion Laboratory (JPL) in Pasadena, California, and the Galileo probe was designed and built at the NASA Ames Research Center (ARC) in Sunnyvale, California. The orbiter flight team was located at JPL, as was the probe flight team during that portion of the mission. 4.1.1 The Mission The Galileo spacecraft was launched in 1989 aboard the Space Shuttle Atlantis (STS [Space Transportation System]-34). Its primary objective was to study the Jovian System. The Galileo launch delay after the Challenger Space Shuttle 81 82 Chapter 4 accident in 1986 necessitated a change in the strategy to get Galileo to Jupiter.1 The original strategy was a relatively direct flight to Jupiter with a single gravity assist at Mars. The new mission plan had to work with less propulsion, so it made use of a longer, much less direct flight, with gravitational assists from Venus once and Earth twice, to give the spacecraft enough energy to get to Jupiter.