UNIVERSITY OF NOTRE DAME
|
|
- Irma Logan
- 5 years ago
- Views:
Transcription
1 S E T T I N G A S I D E A L L A U T H O R I T Y
2
3 Setting Aside All Authority Giovanni Battista Riccioli and the Science against Copernicus in the Age of Galileo INCLUDING THE FIRST ENGLISH TRANSLATION OF M O N S I G N O R F R A N C E S C O I N G O L I S essay to Galileo disputing the Copernican system, and the first English translation of R I C C I O L I S R E P O R T S regarding his experiments with falling bodies and with the effect of air resistance on falling bodies. C H R I S T O P H E R M. G R A N E Y University of Notre Dame Press Notre Dame, Indiana
4 Copyright 2015 by the University of Notre Dame Notre Dame, Indiana All Rights Reserved Manufactured in the United States of America Library of Congress Cataloging-in-Publication Data Graney, Christopher M., 1966 Setting aside all authority : Giovanni Battista Riccioli and the science against Copernicus in the age of Galileo / Christopher M. Graney. pages cm Includes bibliographical references and index. ISBN (paperback : alkaline paper) ISBN (paperback : alkaline paper) 1. Riccioli, Giovanni Battista, Astronomers Italy Biography. 3. Jesuit scientists Italy Biography. 4. Copernicus, Nicolaus, Astronomy Italy History 17th century. 6. Science Italy History 17th century. I. Title. QB36.R386G dc The paper in this book meets the guidelines for permanence and durability of the Committee on Production Guidelines for Book Longevity of the Council on Library Resources.
5 To my sister, Laura Kathleen Graney ( ), who had a great affection for the night sky, and who took great pride in her brother s work.
6
7 Contents List of Illustrations and Tables Acknowledgments ix xiii 1 Giovanni Battista Riccioli and the New Almagest 1 2 The Universe that Riccioli Saw 9 3 The Anti-Copernican Astronomer 25 4 Stars and Adventitious Rays 45 5 Science against Copernicus, God s Starry Armies for Copernicus 63 6 Jesuits on the Tower Arguments An Angel and a Cannon The Telescope against Copernicus It Can No Longer Be Called False and Absurd 141 Appendix A: Francesco Ingoli s 1616 Essay to Galileo 163 Appendix B: Giovanni Battista Riccioli s Reports Regarding His Experiments with Falling Bodies 197 Notes 233 Works Cited 257 Index 265
8
9 Illustrations and Tables Figure 1.1. Frontispiece of Giovanni Battista Riccioli s 1651 New Almagest. Image courtesy History of Science Collections, University of Oklahoma Libraries. 3 Figure 1.2. Details from the New Almagest frontispiece, showing Jupiter, Mercury, and Venus. Images courtesy History of Science Collections, University of Oklahoma Libraries. 4 Figure 1.3. Detail from the New Almagest frontispiece, showing the world systems. Image courtesy History of Science Collections, University of Oklahoma Libraries. 4 Figure 2.1. The stars of the constellation Scorpius 11 Figure 2.2. The Moon partially eclipsed. Photo credit: NASA/Bill Ingalls. 21 Figure 2.3. Comparison of Earth s size to the distance to the stars 21 Figure 2.4. Diurnal parallax 22 Figure 3.1. Tycho Brahe s observatories. Images credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 27 Figure 3.2. One of Tycho Brahe s nontelescopic instruments. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 28 Figure 3.3. Astronomers Johannes and Elisabeth Hevelius using a nontelescopic measuring instrument. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 29 Figure 3.4. A vernier caliper. Image credit: M. Colcher. 29 ix
10 x Illustrations and Tables Figure 3.5. The hybrid geocentric hypothesis of Tycho Brahe. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 31 Figure 3.6. Annual parallax 33 Table 3.1. Tycho Brahe s apparent sizes of and average distances to celestial bodies 34 Figure 3.7. The relative sizes of celestial bodies calculated by Tycho Brahe 35 Figure 3.8. The relationship between the apparent size, the physical or true size, and the distance of a celestial body 36 Table 3.2. Tycho Brahe s apparent sizes of and average distances to the fixed stars 37 Figure 3.9. Brahe s calculated relative size for a mid-size star in the Copernican universe 38 Figure Paths of projectiles. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 39 Figure 4.1. The appearance of Venus changing over time, as seen by Galileo. Image courtesy History of Science Collections, University of Oklahoma Libraries. 55 Figure 4.2. Representations of Jupiter s cloud bands, from the New Almagest. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 58 Figure 4.3. A star as seen through a small aperture telescope. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 60 Figure 5.1. Illustrations of the Moon and Sun from Locher s 1614 Disquisitions. Images credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 65 Figure 5.2. Diagram of phases of Venus from Locher s 1614 Disquisitions. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 66 Figure 5.3. The Jovian system as illustrated in Locher s 1614 Disquisitions. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 67 Figure 5.4. Thomas Digges s sketch of the Copernican system. Image courtesy History of Science Collections, University of Oklahoma Libraries. 78 Figure 6.1. Pendulum diagram from the New Almagest. Image credit: ETH- Bibliothek Zürich, Alte und Seltene Drucke. 89 Figure 6.2. Riccioli s diagram of the Asinelli tower in Bologna. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 94
11 Illustrations and Tables xi Figure 6.3. Map of the Moon from the New Almagest. Image courtesy History of Science Collections, University of Oklahoma Libraries. 99 Figure 6.4. Detail from the New Almagest map of the Moon. Image courtesy History of Science Collections, University of Oklahoma Libraries. 100 Figure 7.1. Detail from Digges s sketch of the Copernican system. Image courtesy History of Science Collections, University of Oklahoma Libraries. 109 Figure 7.2. Diagram from the New Almagest, showing Galileo s hypothesis regarding the motion of a heavy ball falling from a high tower. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 110 Figure 7.3. Diagrams from the New Almagest, showing the motions of falling bodies on a rotating, Sun-orbiting Earth. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 111 Figure 8.1. Diagram representing cannon shots on a rotating Earth 117 Figure 8.2. Figure from the New Almagest, showing the trajectories of a cannon fired to the north versus fired to the east. Images credit: ETH- Bibliothek Zürich, Alte und Seltene Drucke. 119 Figure 8.3. Diagram based on a sketch by Newton, showing an object dropped from a high tower on a rotating Earth 123 Figure 9.1. Riccioli s Jupiter and Saturn figures with comparison of the sizes of Sirius and Alcor. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 131 Figure 9.2. Riccioli s table of the telescopic sizes of stars, from the New Almagest. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 131 Figure 9.3. Riccioli s tables showing the calculated physical sizes of Sirius and Alcor from the New Almagest. Images credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke Figure 9.4. The effect, or lack thereof, of the telescope on the star size question. 136 Figure The Foucault pendulum at the Kentucky Science Center in Louisville 149 Figure Diffraction pattern formed by light passing through a circular aperture. Image credit: Wikimedia Commons. 155
12 xii Illustrations and Tables Figure A.1. A mechanical orrery. Images courtesy of Todd Timberlake, Berry College. 192 Figure B.1. Riccioli s diagram of the Asinelli tower in Bologna, with details. Image credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 202 Table B.1. New Almagest data table showing times and distances for eightounce clay balls dropped from varying heights 206 Table B.2. New Almagest data tables for pairs of balls dropped from the same height 210 Figure B.2. New Almagest data table showing times and distances for eightounce clay balls dropped from varying heights. Image credit: ETH- Bibliothek Zürich, Alte und Seltene Drucke. 221 Figure B.3. New Almagest data tables for pairs of balls dropped from the same height. Images credit: ETH-Bibliothek Zürich, Alte und Seltene Drucke. 224 Figure B.4. Plot of Riccioli s data from table B Figure B.5. Plot of Riccioli s four fully independent measurements from table B Figure B.6. Plots of distance travelled vs. time for two different balls falling through air 231
Giovanni Battista Riccioli and the New Almagest
1 Giovanni Battista Riccioli and the New Almagest The New Almagest was astronomy. What was not in the New Almagest did not need to be known. England s top astronomer the first Astronomer Royal, John Flamsteed
More informationEarth Science, 13e Tarbuck & Lutgens
Earth Science, 13e Tarbuck & Lutgens Origins of Modern Astronomy Earth Science, 13e Chapter 21 Stanley C. Hatfield Southwestern Illinois College Early history of astronomy Ancient Greeks Used philosophical
More informationPeer Led Team Learning. Tycho Brahe in his observatory His careful observations and records are his most important legacy
Birth of Modern Astronomy Celestial Motion Lab starts this week NS 017 Bring lab manual to lab Do Prelab 1 before you go! Peer Led Team Learning Tuesday 5:45 to 7:45 PM Library Room 205 Add ES104X CRN
More informationPlanets & The Origin of Science
Planets & The Origin of Science Reading: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Sept. 26 Office Hours: Monday,
More informationCopernican Revolution 15 Jan. Copernican Revolution: questions on reading assignment
Copernican Revolution 15 Jan Final exam is Wed, May 6 th, not 5 th. Questions on reading Motion of the sun & planets Ptolemy s Almagest Copernicus de Revolutionibus Orbium Caelestium, (Concerning Revolutions
More informationIn so many and such important. ways, then, do the planets bear witness to the earth's mobility. Nicholas Copernicus
In so many and such important ways, then, do the planets bear witness to the earth's mobility Nicholas Copernicus What We Will Learn Today What did it take to revise an age old belief? What is the Copernican
More informationCopernican Revolution. Motions of the sky. Motions of the sky. Copernican Revolution: questions on reading assignment
Copernican Revolution Motion of the sun & planets Ptolemy s Almagest Copernicus de Revolutionibus Orbium Caelestium, (Concerning Revolutions of the Heavenly Spheres), 1543 Galileo refutes Ptolemy with
More informationNext Homework Due. Feb. 20
This week: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Feb. 20 Office Hours: Monday, 3-4 Did you see the Lunar Eclipse?
More informationcosmogony geocentric heliocentric How the Greeks modeled the heavens
Cosmogony A cosmogony is theory about ones place in the universe. A geocentric cosmogony is a theory that proposes Earth to be at the center of the universe. A heliocentric cosmogony is a theory that proposes
More informationLecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo
Lecture #5: Plan The Beginnings of Modern Astronomy Kepler s Laws Galileo Geocentric ( Ptolemaic ) Model Retrograde Motion: Apparent backward (= East-to-West) motion of a planet with respect to stars Ptolemy
More informationPeer Led Instruction. Celestial Motion. Get your lab manual. Tycho Brahe
Celestial Motion Chapter 21, pages 597-606 Chapter 22, pages 615-619 Lab starts this week NS 017 Peer Led Instruction Library Wednesday 6:30 to 8:30 PM Kristin Mooney Science Education Major Add ES104X
More informationChapter 02 The Rise of Astronomy
Chapter 02 The Rise of Astronomy Multiple Choice Questions 1. The moon appears larger when it rises than when it is high in the sky because A. You are closer to it when it rises (angular-size relation).
More informationPhysics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion
Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits Planetary Motion Geocentric Models --Many people prior to the 1500 s viewed the! Earth and the solar system using a! geocentric
More informationEarth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy
2006 Pearson Prentice Hall Lecture Outlines PowerPoint Chapter 21 Earth Science 11e Tarbuck/Lutgens This work is protected by United States copyright laws and is provided solely for the use of instructors
More informationCh. 22 Origin of Modern Astronomy Pretest
Ch. 22 Origin of Modern Astronomy Pretest Ch. 22 Origin of Modern Astronomy Pretest 1. True or False: Early Greek astronomers (600 B.C. A.D. 150) used telescopes to observe the stars. Ch. 22 Origin of
More informationPosition 3. None - it is always above the horizon. Agree with student 2; star B never crosses horizon plane, so it can t rise or set.
Position 3 None - it is always above the horizon. N E W S Agree with student 2; star B never crosses horizon plane, so it can t rise or set. Imaginary plane No; the Earth blocks the view. Star A at position
More informationPHYS 160 Astronomy Test #1 Fall 2017 Version B
PHYS 160 Astronomy Test #1 Fall 2017 Version B 1 I. True/False (1 point each) Circle the T if the statement is true, or F if the statement is false on your answer sheet. 1. An object has the same weight,
More informationHow Astronomers Learnt that The Heavens Are Not Perfect
1 How Astronomers Learnt that The Heavens Are Not Perfect Introduction In this packet, you will read about the discoveries and theories which changed the way astronomers understood the Universe. I have
More informationLearning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?
Kepler s Laws Learning Objectives! Do the planets move east or west over the course of one night? Over the course of several nights? How do true motion and retrograde motion differ?! What are geocentric
More informationGravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler
Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler Celestial motions The stars: Uniform daily motion about the celestial poles (rising and setting). The Sun: Daily motion around the celestial
More informationAstronomy 100 Section 2 MWF Greg Hall. Outline. Total Lunar Eclipse Time Lapse. Homework #1 is due Friday, 11:50 a.m.!!!!!
Astronomy 100 Section 2 MWF 1200-1300 100 Greg Hall Leslie Looney Phone: 217-244-3615 Email: lwl @ uiuc. edu Office: Astro Building #218 Office Hours: MTF 10:30-11:30 a.m. or by appointment Homework #1
More informationDeAnza College Winter First Midterm Exam MAKE ALL MARKS DARK AND COMPLETE.
FAMILY NAME : (Please PRINT!) GIVEN NAME : (Please PRINT!) Signature: ASTRONOMY 4 DeAnza College Winter 2018 First Midterm Exam MAKE ALL MARKS DARK AND COMPLETE. Instructions: 1. On your Parscore sheet
More informationGravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields
Gravity Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields Simulation Synchronous Rotation https://www.youtube.com/watch?v=ozib_l eg75q Sun-Earth-Moon System https://vimeo.com/16015937
More informationAncient Cosmology: A Flat Earth. Alexandria
Today Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo FIRST HOMEWORK DUE How d it work? Ancient Cosmology: A Flat Earth Here there be
More informationThe Scientific Revolution
The Scientific Revolution What is a Revolution? A Revolution is a complete change, or an overthrow of a government, a social system, etc. The Scientific Revolution In the 1500s and 1600s the Scientific
More informationd. Galileo Galilei i. Heard about lenses being used to magnify objects 1. created his own telescopes to 30 power not the inventor! 2. looked
1. Age of Reason a. Nicolaus Copernicus 1473-1543 i. Commenteriolus manuscript circulated from 1512 1. unpublished 2. Heliocentric hypothesis ii. On the Revolutions of the Planets published year of his
More informationChapter 2 The Science of Life in the Universe
In ancient times phenomena in the sky were not understood! Chapter 2 The Science of Life in the Universe The Ancient Greeks The Scientific Method Our ideas must always be consistent with our observations!
More information,.~ Readlng ~ What,~,~~ is a geocentric system? Chapter3 J 73
Earth at the Center When the ancient Greeks watched the stars move across the sky, they noticed that the patterns of the stars didn t change. Although the stars seemed to move, they stayed in the same
More informationToday. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws Laws of Motion. Laws of Motion
Today Planetary Motion Tycho Brahe s Observations Kepler s Laws Laws of Motion Laws of Motion In 1633 the Catholic Church ordered Galileo to recant his claim that Earth orbits the Sun. His book on the
More informationPlanets & The Origin of Science
Planets & The Origin of Science Reading: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Feb. 26 Office Hours: Monday, 12-2
More informationEvidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1
Greek Astronomy Aristotelian Cosmology: Evidence that the Earth does not move: 1. Stars do not exhibit parallax: 2-1 At the center of the universe is the Earth: Changeable and imperfect. Above the Earth
More informationClaudius Ptolemaeus Second Century AD. Jan 5 7:37 AM
Claudius Ptolemaeus Second Century AD Jan 5 7:37 AM Copernicus: The Foundation Nicholas Copernicus (Polish, 1473 1543): Proposed the first modern heliocentric model, motivated by inaccuracies of the Ptolemaic
More informationChapter 4. The Origin Of Modern Astronomy. Is okay to change your phone? From ios to Android From Android to ios
Chapter 4 The Origin Of Modern Astronomy Slide 14 Slide 15 14 15 Is Change Good or Bad? Do you like Homer to look like Homer or with hair? Does it bother you when your schedule is changed? Is it okay to
More informationAst ch 4-5 practice Test Multiple Choice
Ast ch 4-5 practice Test Multiple Choice 1. The distance from Alexandria to Syene is about 500 miles. On the summer solstice the sun is directly overhead at noon in Syene. At Alexandria on the summer solstice,
More informationThings to do today. Terminal, Astronomy is Fun. Lecture 24 The Science of Astronomy. Scientific Thinking. After this lecture, please pick up:
Things to do today After this lecture, please pick up: Review questions for the final exam Homework#6 (due next Tuesday) No class on Thursday (Thanksgiving) Final exam on December 2 (next Thursday) Terminal,
More informationChanging times was one of those years. Scientists consider it to be vitally important in the history of astronomy.
Changing times Astronomy is a dynamic and ever-changing science, where new discoveries are regularly made. But some periods prove to eclipse others in terms of revolutionary discoveries. 1609 was one of
More informationAstronomy- The Original Science
Astronomy- The Original Science Imagine that it is 5,000 years ago. Clocks and modern calendars have not been invented. How would you tell time or know what day it is? One way to tell the time is to study
More informationBenefit of astronomy to ancient cultures
Benefit of astronomy to ancient cultures Usefulness as a tool to predict the weather (seasons) Usefulness as a tool to tell time (sundials) Central Africa (6500 B.C.) Alignments Many ancient cultures built
More informationWhat is a Revolution? A Revolution is a complete change, or an overthrow of a government, a social system, etc.
CW10 p374 Vocab What is a Revolution? A Revolution is a complete change, or an overthrow of a government, a social system, etc. The Scientific Revolution In the 1500s and 1600s the Scientific Revolution
More informationToday. Planetary Motion. Tycho Brahe s Observations. Kepler s Laws of Planetary Motion. Laws of Motion. in physics
Planetary Motion Today Tycho Brahe s Observations Kepler s Laws of Planetary Motion Laws of Motion in physics Page from 1640 text in the KSL rare book collection That the Earth may be a Planet the seeming
More informationb. Remember, Sun is a second or third generation star the nebular cloud of dust and gases was created by a supernova of a preexisting
1. Evolution of the Solar System Nebular hypothesis, p 10 a. Cloud of atoms, mostly hydrogen and helium b. Gravitational collapse contracted it into rotating disc c. Heat of conversion of gravitational
More informationThe Scientific Method
The Scientific Method Objectives: 1. Outline the scientific method. 2. Explain why the scientific method has been more successful than other approaches to understanding the universe. 3. Distinguish between
More informationD. A system of assumptions and principles applicable to a wide range of phenomena that has been repeatedly verified
ASTRONOMY 1 EXAM 1 Name Identify Terms - Matching (20 @ 1 point each = 20 pts.) 1 Solar System G 7. aphelion N 14. eccentricity M 2. Planet E 8. apparent visual magnitude R 15. empirical Q 3. Star P 9.
More informationThe History of Astronomy
The History of Astronomy The History of Astronomy Earliest astronomical record: a lunar calendar etched on bone from 6500 B.C. Uganda. Also we find early groups noted the Sun, Moon, Mercury, Venus, Earth,
More informationPractice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009
Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009 Multiple Choice Identify the letter of the choice that best completes the statement or answers the question. Mark answer on Scantron.
More informationPlanets & The Origin of Science
Planets & The Origin of Science Reading: Chapter 2 Required: Guided Discovery (p.44-47) Required: Astro. Toolbox 2-1 Optional: Astro. Toolbox 2-2, 2-3 Next Homework Due. Sept. 25 Office Hours: Monday,
More informationIntroduction To Modern Astronomy II
ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy II Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens
More information1. The Moon appears larger when it rises than when it is high in the sky because
2-1 Copyright 2016 All rights reserved. No reproduction or distribution without the prior written consent of 1. The Moon appears larger when it rises than when it is high in the sky because A. you are
More informationThe History of Astronomy. Theories, People, and Discoveries of the Past
The History of Astronomy Theories, People, and Discoveries of the Past Early man recorded very little history. Left some clues in the form of petrographs. Stone drawings that show eclipses, comets, supernovae.
More informationAST 2010 Descriptive Astronomy Study Guide Exam I
AST 2010 Descriptive Astronomy Study Guide Exam I Wayne State University 1 Introduction and overview Identify the most significant structures in the universe: Earth, planets, Sun, solar system, stars,
More informationChapter 2. The Rise of Astronomy. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 2 The Rise of Astronomy Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Periods of Western Astronomy Western astronomy divides into 4 periods Prehistoric
More informationDirections: Read each slide
Directions: Read each slide and decide what information is needed. Some slides may have red or yellow or orange underlined. This information is a clue for you to read more carefully or copy the information
More informationAnnouncements. Topics To Be Covered in this Lecture
Announcements! Tonight s observing session is cancelled (due to clouds)! the next one will be one week from now, weather permitting! The 2 nd LearningCurve activity was due earlier today! Assignment 2
More informationOf Mites and Men: Johannes Kepler on Stars and Size (with an English translation of Chapter 16 of his 1606 De Stella Nova)
Of Mites and Men: Johannes Kepler on Stars and Size (with an English translation of Chapter 16 of his 1606 De Stella Nova) Christopher M. Graney Jefferson Community & Technical College Louisville, KY 40272
More informationMonday, October 3, 2011
We do not ask for what useful purpose the birds do sing, for song is their pleasure since they were created for singing. Similarly, we ought not ask why the human mind troubles to fathom the secrets of
More informationPHYS 160 Astronomy Test #1 Name Answer Key Test Version A
PHYS 160 Astronomy Test #1 Name Answer Key Test Version A True False Multiple Choice 1. T 1. C 2. F 2. B 3. T 3. A 4. T 4. E 5. T 5. B 6. F 6. A 7. F 7. A 8. T 8. D 9. F 9. D 10. F 10. B 11. B 12. D Definitions
More information1 Astronomy: The Original Science
CHAPTER 18 1 Astronomy: The Original Science SECTION Studying Space BEFORE YOU READ After you read this section, you should be able to answer these questions: How do astronomers define a day, a month,
More informationAstronomy 1 Fall 2016
Astronomy 1 Fall 2016 Comet Halley Edmund Halley, a friend of Newton s used Newton s math to predict the return of a comet seen at intervals of 76 years. Lecture 3; September 29, 2016 Previously on Astro-1
More informationMotions of the Planets ASTR 2110 Sarazin
Motions of the Planets ASTR 2110 Sarazin Motion of Planets Retrograde Motion Inferior Planets: Mercury, Venus Always near Sun on Sky Retrograde motion when very close to Sun on sky (Every other time) Superior
More informationCompeting Models. The Ptolemaic system (Geocentric) The Copernican system (Heliocentric)
Competing Models The Ptolemaic system (Geocentric) The Copernican system (Heliocentric) How did Galileo solidify the Copernican revolution? Galileo overcame major objections to the Copernican view. Three
More informationThe Copernican Revolution
The Copernican Revolution Nicolaus Copernicus (1473-1543) De Revolutionibus Orbium Coelestium (1543) [ On the Revolutions of the Celestial Spheres ] The Ptolemaic Cosmology: Geocentric and Geostatic The
More informationHow High Is the Sky? Bob Rutledge
How High Is the Sky? Bob Rutledge Homer s Physics: Feb 16 2007 The Sun 8 Light Minutes Away 2 The Pleiades 300 Light Years Away (and inside our galaxy) [The nearest star, Proxima Cen, is only 4.2 light
More informationEarly Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle
Planetary Motion Early Theories Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle Stars appear to move around Earth Observations showed
More informationCopernican Revolution. ~1500 to ~1700
~1500 to ~1700 Copernicus (~1500) Brahe (~1570) Kepler (~1600) Galileo (~1600) Newton (~1670) The Issue: Geocentric or Heliocentric Which model explains observations the best? Copernicus (~1500) Resurrected
More informationMotion in the Heavens
Motion in the Heavens Most ancient cultures believed that the earth was the centre of the universe. Most felt that the planets, stars, moon and sun revolved around the earth. This is known as a geocentric
More informationThe great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley. Monday, October 3, 2011
The great tragedy of science the slaying of a beautiful hypothesis by an ugly fact. -Thomas Huxley 1 Chapter 4 The Origin of Modern Astronomy Outline I. The Roots of Astronomy A. Archaeoastronomy B. The
More informationCopernican Astronomy. Nicolaus gets the ball rolling
Copernican Astronomy Nicolaus gets the ball rolling Recap: Problems for Ptolemy In Ptolemy s model the sun s orbit (around the earth) is rather special. The sun has no epicycle, just a deferent The epicycles
More informationFirst MIDTERM Exam: Mon, Sep. 22, covering chapters tutorials (review later today).
Announcements First MIDTERM Exam: Mon, Sep. 22, covering chapters 1 3 + tutorials (review later today). Interim grades online, coded by class ID. See course website Grades tab. Another great night for
More informationModule 3: Astronomy The Universe Topic 6 Content: The Age of Astronomy Presentation Notes
Module 3: Astronomy The Universe The Age of Astronomy was marked by the struggle to understand the placement of Earth in the universe and the effort to understand planetary motion. Behind this struggle
More informationsome center of the Universe (he mentions the Pythagorean central fire ) and that the
Fragmentary Notes on Aristotle s On the Heavens Aristotle had considered and rejected both the proposition that the Earth revolves about some center of the Universe (he mentions the Pythagorean central
More informationName Class Date. For each pair of terms, explain how the meanings of the terms differ.
Skills Worksheet Chapter Review USING KEY TERMS 1. Use each of the following terms in a separate sentence: year, month, day, astronomy, electromagnetic spectrum, constellation, and altitude. For each pair
More information2. See FIGURE B. In the Renaissance times, he proposed this model of the solar system (name this person).
ASTRONOMY 5 MIDTERM EXAM PART I SPRING 2019 60 QUESTIONS 50 POINTS: Part I of the midterm constitutes the Take-Home part of the entire Midterm Exam. Additionally, this Take-Home part is divided into two
More informationPhysics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Goals of the course. What will we cover? How do we do this?
Physics 107 Ideas of Modern Physics (uw.physics.wisc.edu/~rzchowski/phy107) Main emphasis is Modern Physics: essentially post-1900 Why 1900? Two radical developments: Relativity & Quantum Mechanics Both
More informationAstronomy 1010 Planetary Astronomy Sample Questions for Exam 1
Astronomy 1010 Planetary Astronomy Sample Questions for Exam 1 Chapter 1 1. A scientific hypothesis is a) a wild, baseless guess about how something works. b) a collection of ideas that seems to explain
More information2. See FIGURE B. This person in the FIGURE discovered that this planet had phases (name the planet)?
ASTRONOMY 2 MIDTERM EXAM PART I SPRING 2019 60 QUESTIONS 50 POINTS: Part I of the midterm constitutes the Take-Home part of the entire Midterm Exam. Additionally, this Take-Home part is divided into two
More information2X CLAUDIUS PTOLEMY BIOGRAPHY 780L
2X CLAUDIUS PTOLEMY BIOGRAPHY 780L CLAUDIUS PTOLEMY AN EARTH-CENTERED VIEW OF THE UNIVERSE Born 85 CE Hermiou, Egypt Died 165 CE Alexandria, Egypt By Cynthia Stokes Brown, adapted by Newsela Claudius Ptolemy
More informationHistory of Astronomy. PHYS 1411 Introduction to Astronomy. Tycho Brahe and Exploding Stars. Tycho Brahe ( ) Chapter 4. Renaissance Period
PHYS 1411 Introduction to Astronomy History of Astronomy Chapter 4 Renaissance Period Copernicus new (and correct) explanation for retrograde motion of the planets Copernicus new (and correct) explanation
More informationRENAISSANCE ASTRONOMY
RENAISSANCE ASTRONOMY Question What kind of observations would conclusively prove that the Earth is in orbit around the Sun? 1 Galileo Galilei Galileo Galilei [1564 1642, Italy] Considered the Father of
More informationJanuary 19, notes.notebook. Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM
8.1 notes.notebook Claudius Ptolemaeus Second Century AD Jan 5 7:7 AM Copernicus: The Foundation Nicholas Copernicus (Polish, 147 154): Proposed the first modern heliocentric model, motivated by inaccuracies
More information18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.
Name: Date: 1. The word planet is derived from a Greek term meaning A) bright nighttime object. B) astrological sign. C) wanderer. D) nontwinkling star. 2. The planets that were known before the telescope
More informationReview of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes
Review of previous concepts!! Earth s orbit: Year, seasons, observed constellations, Polaris (North star), day/night lengths, equinoxes Celestial poles, celestial equator, ecliptic, ecliptic plane (Fig
More informationNicolaus gets the ball rolling
Copernican Astronomy Nicolaus gets the ball rolling Problems for Ptolemy In Ptolemy s model the sun s s orbit (around the earth) is rather special. The sun has no epicycle,,just a deferent The epicycles
More informationContents: -Information/Research Packet. - Jumbled Image packet. - Comic book cover page. -Comic book pages. -Example finished comic
Contents: -Information/Research Packet - Jumbled Image packet - Comic book cover page -Comic book pages -Example finished comic Nicolaus Copernicus Nicholas Copernicus was a Polish astronomer who lived
More informationChapter 26 Section 1 pages Directed Reading Section: Viewing the Universe
Name: Period: Chapter 26 Section 1 pages 659-666 Directed Reading Section: Viewing the Universe 1. How did observations of the sky help sailors in the past? 2. What is the main reason people study the
More informationPHYS 155 Introductory Astronomy
PHYS 155 Introductory Astronomy - observing sessions: Sunday Thursday, 9pm, weather permitting http://www.phys.uconn.edu/observatory - Exam - Tuesday March 20, - Review Monday 6:30-9pm, PB 38 Marek Krasnansky
More informationGriffith Observatory Field Trip Guide
To enter the Griffith Observatory you must make a reservation for a seat on a shuttle. There is a cost associated with each shuttle ticket and it is $8.00. There is no other way to enter Griffith Observatory!
More informationThe History of Astronomy
The History of Astronomy http://www.ichundmeinmitbewohner.de/wpcontent/uploads/2013/05/mauna-kea-2.jpg Mauna Kea Observatories, HI Astronomy Through The Ages Astronomy is a very old science. Chemistry
More informationHistory of Astronomy - Part I. Ancient Astronomy. Ancient Greece. Astronomy is a science that has truly taken shape only in the last couple centuries
History of Astronomy - Part I Astronomy is a science that has truly taken shape only in the last couple centuries Many advances have been made in your lifetime However, astronomical concepts and ideas
More informationAstronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric
Around 2500 years ago, Pythagoras began to use math to describe the world around him. Around 200 years later, Aristotle stated that the Universe is understandable and is governed by regular laws. Most
More information2.4 The Birth of Modern Astronomy
2.4 The Birth of Modern Astronomy Telescope invented around 1600 Galileo built his own, made observations: Moon has mountains and valleys Sun has sunspots, and rotates Jupiter has moons (shown): Venus
More informationUnit 6 Lesson 1 How Do the Sun, Earth, and Moon Interact? Copyright Houghton Mifflin Harcourt Publishing Company
Unit 6 Lesson 1 How Do the Sun, Earth, and Moon Interact? Night and Day Earth rotates, or turns like a top. Earth s rotation causes day and night. Earth rotates around an imaginary line called an axis,
More informationGravitation and the Waltz of the Planets
Gravitation and the Waltz of the Planets Chapter Four Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets
More informationGravitation and the Waltz of the Planets. Chapter Four
Gravitation and the Waltz of the Planets Chapter Four Guiding Questions 1. How did ancient astronomers explain the motions of the planets? 2. Why did Copernicus think that the Earth and the other planets
More informationName: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016
Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016 Why are celestial motions and forces important? They explain the world around us.
More informationBROCK UNIVERSITY. 1. The observation that the intervals of time between two successive quarter phases of the Moon are very nearly equal implies that
BROCK UNIVERSITY Page 1 of 10 Test 1: November 2014 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 961 Examination date: 7 November 2014 Time limit: 50 min Time of Examination: 17:00
More informationThe Observer. Schedule of public programs on last page!
The Observer January 2012 (#30) Schedule of public programs on last page! Cool Stuff in the Winter Sky: Venus, Mars, and Jupiter put on a Show The three most prominent planets in the night sky Venus, Mars,
More informationASTR 1010 Spring 2016 Study Notes Dr. Magnani
The Copernican Revolution ASTR 1010 Spring 2016 Study Notes Dr. Magnani The Copernican Revolution is basically how the West intellectually transitioned from the Ptolemaic geocentric model of the Universe
More informationChapter. Origin of Modern Astronomy
Chapter Origin of Modern Astronomy 22.1 Early Astronomy Ancient Greeks Astronomy is the science that studies the universe. It includes the observation and interpretation of celestial bodies and phenomena.
More informationChapter 16 The Solar System
Chapter 16 The Solar System Finding the Standard Time and Date at Another Location Example When it is 12 noon in London, what is the standard time in Denver, Colorado (40 N, 105 W)? Section 15.3 Finding
More informationPlanetary Orbits: Kepler s Laws 1/18/07
Planetary Orbits: Kepler s Laws Announcements The correct link for the course webpage http://www.lpl.arizona.edu/undergrad/classes/spring2007/giacalone_206-2 The first homework due Jan 25 (available for
More information