The Assayer - Galileo
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Galileo Galilei Introduction Galileo Galilei (1564–1642) Was One of The
Galileo Galilei Introduction Galileo Galilei (1564–1642) was one of the most significant figures of the Scientific Revolution. Galileo was involved in nearly all fields of natural philosophy, including astronomy, mathematics, and what we now term “physics.” He is rightly considered one of the founders of modern physics and astronomy, and one of the main originators of the modern scientific method. Galileo’s study of motion became the foundation for Newton’s laws of motion and the principles of inertia and gravity. His astronomical studies were instrumental in supporting the heliocentric model of the solar system first propounded by Copernicus. He should also be credited with making experimentation the basis of scientific study, and with the use of mathematics as the fundamental means for expressing and validating the findings of experimental investigation. Galileo’s application of mathematics to experimental results has become one of the most important aspects of modern science. Galileo made important improvements to the telescope, which enabled him to make great advances in astronomical observation. His observations emboldened him to become the most important advocate of Copernicanism—the astronomical system created by Nicolaus Copernicus (1473–1543)—and his support ultimately ushered in the Copernican revolution in astronomy. Copernicus had devised a heliocentric model in which he posited that the Earth revolved around the sun (in perfect circles). Contrary to the Ptolemaic system and Christian cosmology, Copernicus positioned the sun as a fixed center around which Mercury, Venus, Earth, Mars, Jupiter, and Saturn orbited. Furthermore, Copernicus posited the diurnal rotation of the Earth on its own axis in addition to its annual revolutions around the sun. -
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. -
Galilei-1632 Dialogue Concerning the Two Chief World Systems
Galileo di Vincenzo Bonaulti de Galilei ([ɡaliˈlɛːo ɡaliˈlɛi]; 15 February 1564 – 8 January 1642) was an Italian astronomer, physicist and engineer, sometimes described as a polymath, from Pisa. Galileo has been called the "father of observational astronomy", the "father of modern physics", the "father of the scientific method", and the "father of modern science". Galileo studied speed and velocity, gravity and free fall, the principle of relativity, inertia, projectile motion and also worked in applied science and technology, describing the properties of pendulums and "hydrostatic balances", inventing the thermoscope and various military compasses, and using the telescope for scientific observations of celestial objects. His contributions to observational astronomy include the telescopic confirmation of the phases of Venus, the observation of the four largest satellites of Jupiter, the observation of Saturn's rings, and the analysis of sunspots. Galileo's championing of heliocentrism and Copernicanism was controversial during his lifetime, when most subscribed to geocentric models such as the Tychonic system. He met with opposition from astronomers, who doubted heliocentrism because of the absence of an observed stellar parallax. The matter was investigated by the Roman Inquisition in 1615, which concluded that heliocentrism was "foolish and absurd in philosophy, and formally heretical since it explicitly contradicts in many places the sense of Holy Scripture". Galileo later defended his views in Dialogue Concerning the Two Chief World Systems (1632), which appeared to attack Pope Urban VIII and thus alienated him and the Jesuits, who had both supported Galileo up until this point. He was tried by the Inquisition, found "vehemently suspect of heresy", and forced to recant. -
Recieved Notice Today That It Did Not Go Through
Scientists are People, Too: Biographies of Astronomical Scientists as a Literary Introduction to the Heliocentric Theory Autry McMorris Welch Middle School INTRODUCTION The Setting and Objectives One of the teaching tools that teachers often use is to take advantage of their students’ prior knowledge. This allows students to connect with the author or subject. Many students have had astronomical awareness or experiences as simple as Aristotle’s in 320 BC – that the Earth must be round because it casts a crescent shape on the moon. For me, it was an incidental thing that I sometimes noticed the moon out in the mornings and evenings when I walked my dogs. Almost as a type of entertainment, I started to anticipate where the moon would be positioned on my next walk. I found myself exhilarated as I could correctly anticipate its position. The key for me was that the moon was moving west, but because of the Earth’s rotation, it appeared to be moving east. At that moment, I shared an icon of truth with the great masters. Astronomy is very complex, to say the least. Some students, aware of their limitations, would not begin to broach the subject except from a non-threatening position. What if an introductory course were to be available that introduced the periphery of the subject? What if selected writings, biographies, autobiographies, theories and the like were a part of a curriculum to superimpose our literary devices of today on great works that were written hundreds of years ago? Copernicus described himself somewhat as candid and clear enough that both the unlearned as well as the learned might see that he was not seeking to flee from the judgment of any man, even if someone provided a guard against the bites of slanderers, the proverb holds that there is no medicine for the bite of a sycophant. -
A Phenomenology of Galileo's Experiments with Pendulums
BJHS, Page 1 of 35. f British Society for the History of Science 2009 doi:10.1017/S0007087409990033 A phenomenology of Galileo’s experiments with pendulums PAOLO PALMIERI* Abstract. The paper reports new findings about Galileo’s experiments with pendulums and discusses their significance in the context of Galileo’s writings. The methodology is based on a phenomenological approach to Galileo’s experiments, supported by computer modelling and close analysis of extant textual evidence. This methodology has allowed the author to shed light on some puzzles that Galileo’s experiments have created for scholars. The pendulum was crucial throughout Galileo’s career. Its properties, with which he was fascinated from very early in his career, especially concern time. A 1602 letter is the earliest surviving document in which Galileo discusses the hypothesis of pendulum isochronism.1 In this letter Galileo claims that all pendulums are isochronous, and that he has long been trying to demonstrate isochronism mechanically, but that so far he has been unable to succeed. From 1602 onwards Galileo referred to pendulum isochronism as an admirable property but failed to demonstrate it. The pendulum is the most open-ended of Galileo’s artefacts. After working on my reconstructed pendulums for some time, I became convinced that the pendulum had the potential to allow Galileo to break new ground. But I also realized that its elusive nature sometimes threatened to undermine the progress Galileo was making on other fronts. It is this ambivalent nature that, I thought, might prove invaluable in trying to understand crucial aspects of Galileo’s innovative methodology. -
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. -
Ch. 3: the Solar System
1 Ch. 3: The Solar System Brief outline: Ideas of Copernicus >> Galileo >> Kepler >> Isaac Newton This chapter discusses how the scientific contributions by Copernicus, Galileo and Kepler led to Newton's discovery of the Universal Gravitation. • It must be understood that the ancient Greek ‘philosophers-scientists’ had various opinions about the ‘center of the universe’ and the relation between Earth and the Sun. Some thought that the Sun is at the center. Others that it is Earth. • Aristotle (384-322 BC) chose to follow the opinion that it is Earth. It appears that he also believed that heavier bodies fall faster than light ones, and many other things. • Much later in 312 AD Constantine was made emperor of Rome and protector of Christianity. Christianity evolved rapidly after the council of Nicaea (AD 325), when intellectuals/philosophers within the Catholic church made efforts to establish doctrine that would make the ideas found in the bible more complete, and eventually added concepts of both Plato and then Aristotle. • Once this was done it became DOGMA of the church, and to attack this view was to attack the foundation of the church. And so this incorrect view lasted for over 1,000 years, until Copernicus. <Nicolaus Copernicus> (1473-1543) Ideas The earth is NOT the center of the universe, although it is the center of the moon’s orbit and of its own gravity. The sun is the center of the planetary system and the sphere of stars. Earth is just one of the planets. Since the moon rotates around the Earth, the heavenly bodies do not share the same center. -
THE STUDY of SATURN's RINGS 1 Thesis Presented for the Degree Of
1 THE STUDY OF SATURN'S RINGS 1610-1675, Thesis presented for the Degree of Doctor of Philosophy in the Field of History of Science by Albert Van Haden Department of History of Science and Technology Imperial College of Science and Teohnology University of London May, 1970 2 ABSTRACT Shortly after the publication of his Starry Messenger, Galileo observed the planet Saturn for the first time through a telescope. To his surprise he discovered that the planet does.not exhibit a single disc, as all other planets do, but rather a central disc flanked by two smaller ones. In the following years, Galileo found that Sa- turn sometimes also appears without these lateral discs, and at other times with handle-like appendages istead of round discs. These ap- pearances posed a great problem to scientists, and this problem was not solved until 1656, while the solution was not fully accepted until about 1670. This thesis traces the problem of Saturn, from its initial form- ulation, through the period of gathering information, to the final stage in which theories were proposed, ending with the acceptance of one of these theories: the ring-theory of Christiaan Huygens. Although the improvement of the telescope had great bearing on the problem of Saturn, and is dealt with to some extent, many other factors were in- volved in the solution of the problem. It was as much a perceptual problem as a technical problem of telescopes, and the mental processes that led Huygens to its solution were symptomatic of the state of science in the 1650's and would have been out of place and perhaps impossible before Descartes. -
The Role and Place of Galileo in the First Scientific Revolution
The role and place of Galileo in the first Scientific Revolution Galileo’s birthday: February, 15, 1564 Gheorghe Stratan NTAA-Dubna, 2014 Two Books: Copernicus and Newton YEAR DESCARTES KEPLER GALILEO | | | 1564…………...……….………………………………………….BORN | 1571………………..…………..…BORN……………………………… | | | | | | 1596…….BORN…...........….Mysterium.Cosm……………… 1600----------------------------------------------------------------- | | | 1609…………..| ……….........Astronomia Nova | 1610…………..|………………..……..|.......Sidereus Nuncius 1613…………..|..…………………………Letters on Sunspots 1618-------------WAR------------------WAR--------------WAR YEAR DESCARTES KEPLER GALILEI 1619……..…I……...................Harmonices..Mundi……………..I 1621..………I..………….....Epitome..Astronomiae……………..I 1623………..I…..…………………I…………………..Saggiatore I 1630…..……I……………………Dies………………................... 1632……......I…..……..…………………………………Dialogue 1633..………I.….……………………………………….........Trial 1637……Method………………………………………………….. 1638……......I.....................................................Two.New.Sciences 1642………..I…………………………………………………Dies 1650……..Dies…………………………………………………… Descartes, philosopher and mathematician (31.03.1596 – 11.02.1650) Kepler, the discoverer of planetary laws of motion (27.12.1571 — 15. 11.1630) Galileo, father of Modern Science (15. 02.1564 — 08. 01.1642) Galileo’s astronomical discoveries Galileo sees the Moon like a new Earth Galileo sees new stars Galileo sees four satellites of Jupiter Further observations: Saturn Further observations: Venus Christian Huygens Explains Galileo (1659) Galileo writes -
The Oldest Translation of the Almagest Made for Al-Maʾmūn by Al-Ḥasan Ibn Quraysh: a Text Fragment in Ibn Al-Ṣalāḥ’S Critique on Al-Fārābī’S Commentary
Zurich Open Repository and Archive University of Zurich Main Library Strickhofstrasse 39 CH-8057 Zurich www.zora.uzh.ch Year: 2020 The Oldest Translation of the Almagest Made for al-Maʾmūn by al-Ḥasan ibn Quraysh: A Text Fragment in Ibn al-Ṣalāḥ’s Critique on al-Fārābī’s Commentary Thomann, Johannes DOI: https://doi.org/10.1484/M.PALS-EB.5.120176 Posted at the Zurich Open Repository and Archive, University of Zurich ZORA URL: https://doi.org/10.5167/uzh-190243 Book Section Accepted Version Originally published at: Thomann, Johannes (2020). The Oldest Translation of the Almagest Made for al-Maʾmūn by al-Ḥasan ibn Quraysh: A Text Fragment in Ibn al-Ṣalāḥ’s Critique on al-Fārābī’s Commentary. In: Juste, David; van Dalen, Benno; Hasse, Dag; Burnett, Charles. Ptolemy’s Science of the Stars in the Middle Ages. Turnhout: Brepols Publishers, 117-138. DOI: https://doi.org/10.1484/M.PALS-EB.5.120176 The Oldest Translation of the Almagest Made for al-Maʾmūn by al-Ḥasan ibn Quraysh: A Text Fragment in Ibn al-Ṣalāḥ’s Critique on al-Fārābī’s Commentary Johannes Thomann University of Zurich Institute of Asian and Oriental Research [email protected] 1. Life and times of Ibn al-Ṣalāḥ (d. 1154 ce) The first half of the twelfth century was a pivotal time in Western Europe. In that period translation activities from Arabic into Latin became a common enterprise on a large scale in recently conquered territories, of which the centres were Toledo, Palermo and Antioch. This is a well known part of what was called the Renaissance of the Twelfth Century.1 Less known is the situation in the Islamic World during the same period. -
The Galileo Affair in Context: an Investigation of Influences on the Church During Galileo’S 1633 Trial
Xavier University Exhibit Honors Bachelor of Arts Undergraduate 2020-5 The Galileo Affair In Context: An Investigation of Influences on The Church During Galileo’s 1633 Trial Evan W. Lamping Xavier University, Cincinnati, OH Follow this and additional works at: https://www.exhibit.xavier.edu/hab Part of the Ancient History, Greek and Roman through Late Antiquity Commons, Ancient Philosophy Commons, Classical Archaeology and Art History Commons, Classical Literature and Philology Commons, and the Other Classics Commons Recommended Citation Lamping, Evan W., "The Galileo Affair In Context: An Investigation of Influences on The Church During Galileo’s 1633 Trial" (2020). Honors Bachelor of Arts. 45. https://www.exhibit.xavier.edu/hab/45 This Capstone/Thesis is brought to you for free and open access by the Undergraduate at Exhibit. It has been accepted for inclusion in Honors Bachelor of Arts by an authorized administrator of Exhibit. For more information, please contact [email protected]. Evan Lamping Dr. Byrne CPHAB Thesis The Galileo Affair In Context: An Investigation of Influences on The Church During Galileo’s 1633 Trial 1 I. Introduction When most people learn about the Galileo controversy of 1633, their knowledge of the affair is most commonly comprised of the facts of his condemnation on counts of heresy and possibly some other details about how and why his inquisition was conducted. These details are often simply concerned with the Church’s indefensible view of the earth as the center of the universe, combined with some scripture passages describing the sun as standing still or the earth being fixed in place and unmovable. -
A Modern Almagest an Updated Version of Ptolemy’S Model of the Solar System
A Modern Almagest An Updated Version of Ptolemy’s Model of the Solar System Richard Fitzpatrick Professor of Physics The University of Texas at Austin Contents 1 Introduction 5 1.1 Euclid’sElementsandPtolemy’sAlmagest . ......... 5 1.2 Ptolemy’sModeloftheSolarSystem . ..... 5 1.3 Copernicus’sModeloftheSolarSystem . ....... 10 1.4 Kepler’sModeloftheSolarSystem . ..... 11 1.5 PurposeofTreatise .................................. .. 12 2 Spherical Astronomy 15 2.1 CelestialSphere................................... ... 15 2.2 CelestialMotions ................................. .... 15 2.3 CelestialCoordinates .............................. ..... 15 2.4 EclipticCircle .................................... ... 17 2.5 EclipticCoordinates............................... ..... 18 2.6 SignsoftheZodiac ................................. ... 19 2.7 Ecliptic Declinations and Right Ascenesions. ........... 20 2.8 LocalHorizonandMeridian ............................ ... 20 2.9 HorizontalCoordinates.............................. .... 23 2.10 MeridianTransits .................................. ... 24 2.11 Principal Terrestrial Latitude Circles . ......... 25 2.12 EquinoxesandSolstices. ....... 25 2.13 TerrestrialClimes .................................. ... 26 2.14 EclipticAscensions .............................. ...... 27 2.15 AzimuthofEclipticAscensionPoint . .......... 29 2.16 EclipticAltitudeandOrientation. .......... 30 3 Dates 63 3.1 Introduction...................................... .. 63 3.2 Determination of Julian Day Numbers . .... 63 4 Geometric