Ast ch 4-5 practice Test Multiple Choice

Size: px
Start display at page:

Download "Ast ch 4-5 practice Test Multiple Choice"

Transcription

1 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, the sun is 1/50th of the circumference of the sky (about 7 ) south of the zenith. Based on this information, what is the circumference of Earth? a. 25,000 miles b. 10 miles c miles d miles e miles 2. The book "De Revolutionibus Orbium Coelestium" a. describes how Galileo's observations and Kepler's calculations proved the Copernican theory. b. describes the construction of Galileo's telescope and his observations. c. is a dialog written to convince the general public of the merits of the Copernican theory. d. first described the Copernican theory. e. describes the Tychonian theory. 3. The Copernican system was no more accurate than the Ptolemaic system in predicting the positions of the planets because a. the Copernican system used the old value for the radius of Earth. b. Copernicus had been unable to detect parallax. c. the Copernican system included uniform circular motion. d. in the Copernican system only Mercury and Venus orbit the sun, all other planets orbited Earth. e. Copernicus used inaccurate data from Ptolemy's system. 4. A is a commonly accepted set of scientific ideas and assumptions. a. theory b. paradigm c. hypothesis d. natural law e. model 5. A is a single conjecture that can be tested. a. hypothesis b. paradigm c. natural law d. model e. theory 6. Saturn is on average 10 AU from the sun. What is the approximate orbital period of Saturn? a. 10 years b. 32 years c. 100 years d years e. 1,000,000 years

2 7. An apparent westward motion of a planet in the sky compared to the background stars (as viewed from the Earth) when observed on successive nights is referred to as a. epicycle b. retrograde motion c. prograde motion d. heliocentric motion e. deferent 8. According to Aristotle an object with no forces in it will a. move faster and faster. b. stop moving eventually. c. move at a constant speed forever. 9. According to Galileo, the acceleration of a freely falling object due to gravity is the larger the mass of the object. a. larger b. smaller c. always the same 10. Galileo found that a. falling objects fall at a constant speed. b. heavy and light objects fall at the same rate. c. heavy objects fall faster than lighter objects. d. the moon's orbit is elliptical. e. only objects made of earth and water fell to the ground. 11. Gravity obeys the inverse square law. This statement implies that the gravitational force of one body on another will be apart. a. two times stronger at 2 meters than at 6 meters b. three times stronger at 2 meters than at 6 meters c. six times weaker at 2 meters than at 6 meters d. nine times stronger at 2 meters than at 6 meters e. The brightness of the force will not change with distance between the two bodies. 12. The circular velocity of a satellite orbiting Earth is given by. In this equation, a. M represents the mass of the satellite, and r is its radius. b. M represents the mass of Earth and r the radius of Earth. c. M represents the mass of the satellite and r the distance from Earth to the satellite. d. M represents the mass of Earth and r the distance from Earth to the satellite. e. M represents the mass of the satellite and r the distance from Earth's surface to the satellite. 13. A(n) orbit is one where the orbiting object is always above the same location on Earth's surface. a. elliptical b. geosynchronous c. closed d. hyperbolic e. parabolic 14. The radius of Earth is 6378 km. The force of gravity on a 1 kg ball at Earth's surface is 9.8 kg m s 2. What is the force of gravity on this same ball when the ball is located 12,756 km from Earth's center?

3 G = N m 2 kg 2 a kg m s 2 b kg m s 2 c. 4.9 kg m s 2 d kg m s 2 e. 9.8 kg m s What is the circular velocity of an object orbiting Earth at a distance of 100,000 km from Earth's center? G = N m 2 kg 2 a. 2 m/s b. 20 m/s c. 200 m/s d m/s e. 20,000 m/s 16. One of the first tests of the general theory of relativity was a. the description of the orbit of the moon. b. the determination of the speed of light to be constant. c. the change in mass of a particle moving at a high speed. d. the demonstration of a hammer and a feather falling at the same rate on the moon. e. the determination of the rate of advance of the perihelion of Mercury's orbit. 17. If the mass of the Earth decreased by a factor of two with no change in radius, your weight would a. increase by a factor of 4. b. increase by a factor of 2. c. stay the same. d. decrease by a factor of 2 e. decrease by a factor of The force due to gravity between two objects depends on I. the mass of each object. II. the distance each object is from Earth. III. the distance between the two objects. IV. the speed of light. a. I & II b. I & III c. II & IV d. I, II, & III e. I, II, III, & IV 19. Since gravity behaves as an inverse square relation the force due to gravity between two masses a. will increase as the distance between the two masses increases. b. will decrease as the square of the distance between the two masses increases. c. will cause the two masses to move away from each other. d. will cause the two masses to move in a straight line. e. will cause the two masses to orbit each other. 20. Which type of curve would accurately represent a closed orbit? a. ellipse

4 b. hyperbola c. parabola d. straight line True/False Indicate whether the statement is true or false. 21. Viewed from the center of Stonehenge, the summer solstice sun rises behind the Heelstone. 22. Parallax is the apparent change in location of an object due to the motion of the observer. 23. Many classical astronomers believed Earth could not move because they detected no parallax. 24. The Ptolemaic model of the universe was heliocentric. 25. Classical Greek astronomers believed the motions of the heavens could be described by uniform circular motion. 26. The Copernican model of the solar system has the planets orbit the sun along elliptical paths. 27. Copernicus was the first to propose that Earth moves around the sun. 28. Galileo wrote the Almagest. 29. Galileo used a telescope to observe the phases of Venus. 30. If a planet orbits the sun at a distance of 4 AU, then its orbital period is 8 years. 31. Kepler's 2 nd of planetary motion states that the orbits of the planets are ellipses with the Sun at one focus. 32. Kepler completed the Rudolphine Tables. 33. Galileo believed that motion stopped in the absence of a force. 34. The force due to gravity has the mathematical form:. 35. The law of gravitation is termed universal because it is a property of all material objects. 36. Changing the direction of a moving body does not change its velocity. 37. The lunar tides on Earth are making the moon recede from Earth. 38. The apparent positions of stars around the sun during an eclipse have been used to prove the general theory of relativity. 39. The neap tides can only occur when the Moon's position is at or near one of its orbital nodes.

5 40. The spring tides occur during the new and full lunar phases. Completion Complete each statement. 41. is a description of the Ptolemaic model of the solar system. 42. The first observations of objects in the solar system that orbit neither the sun nor Earth were made by. 43. Uranus' orbital period is 84 years. How far is Uranus from the sun? 44. Tables based on a heliocentric model of the universe which used elliptical orbits for the planets were more accurate than. 45. The modern first astronomer to propose a heliocentric model for the solar system was. 46. The of a particle is the mass we would measure if the particle were not moving. 47. A ball is dropped from the top of a science building. What is the speed of the ball after falling for three seconds? 48. The states that an observer cannot distinguish locally the difference between inertial forces due to acceleration and uniform gravitational forces due to the presence of a massive object. 49. What is the speed of light in meters per second? 50. Once a theory has been tested thoroughly and is confidently believed by scientists it becomes a.

Practice Test DeAnza College Astronomy 04 Test 1 Spring Quarter 2009

Practice 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 information

Gravitation and the Motion of the Planets

Gravitation and the Motion of the Planets Gravitation and the Motion of the Planets 1 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 go around

More information

Gravitation and the Waltz of the Planets

Gravitation 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 information

Gravitation and the Waltz of the Planets. Chapter Four

Gravitation 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 information

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe

Lecture #4: Plan. Early Ideas of the Heavens (cont d): Geocentric Universe Heliocentric Universe Lecture #4: Plan Early Ideas of the Heavens (cont d): Shape & size of the Earth Size & distance of Moon & Sun Geocentric Universe Heliocentric Universe Shape of the Earth Aristotle (Greece, 384 322 B.C.)

More information

Earth Science, 13e Tarbuck & Lutgens

Earth 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 information

The History of Astronomy. Please pick up your assigned transmitter.

The History of Astronomy. Please pick up your assigned transmitter. The History of Astronomy Please pick up your assigned transmitter. When did mankind first become interested in the science of astronomy? 1. With the advent of modern computer technology (mid-20 th century)

More information

PHYS 160 Astronomy Test #1 Fall 2017 Version B

PHYS 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 information

PHYS 155 Introductory Astronomy

PHYS 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 information

Be able to explain retrograde motion in both the current and Ptolemy s models. You are likely to get an essay question on a quiz concerning these.

Be able to explain retrograde motion in both the current and Ptolemy s models. You are likely to get an essay question on a quiz concerning these. Astronomy 110 Test 2 Review Castle Chapters 6, 7, and possibly 8 NOTE: THIS IS NOT MEANT TO BE EXHAUSTIVE, THIS IS TO HELP THE YOU TRAIN ON THE QUESTION FORMATS AND THE CONCEPTS. Just because an issue

More information

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky.

Most of the time during full and new phases, the Moon lies above or below the Sun in the sky. 6/16 Eclipses: We don t have eclipses every month because the plane of the Moon s orbit about the Earth is different from the plane the ecliptic, the Earth s orbital plane about the Sun. The planes of

More information

Gravitation Part I. Ptolemy, Copernicus, Galileo, and Kepler

Gravitation 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 information

All that is required to measure the diameter of the Earth is a person with stick and a brain.

All that is required to measure the diameter of the Earth is a person with stick and a brain. All that is required to measure the diameter of the Earth is a person with stick and a brain. -adapted from Big Bang, Simon Singh, p.13 1 Announcements: Quiz #2: Monday, September 26 at beginning of class.

More information

Chapter 02 The Rise of Astronomy

Chapter 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 information

Introduction To Modern Astronomy I

Introduction To Modern Astronomy I ASTR 111 003 Fall 2006 Lecture 03 Sep. 18, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch1: Astronomy and the Universe Ch2: Knowing the Heavens

More information

Earth Science, 11e. Origin of Modern Astronomy Chapter 21. Early history of astronomy. Early history of astronomy. Early history of astronomy

Earth 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 information

Copernican Revolution. Motions of the sky. Motions of the sky. Copernican Revolution: questions on reading assignment

Copernican 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 information

Astronomy Notes Chapter 02.notebook April 11, 2014 Pythagoras Aristotle geocentric retrograde motion epicycles deferents Aristarchus, heliocentric

Astronomy 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 information

1. The Moon appears larger when it rises than when it is high in the sky because

1. 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 information

ASTR 2310: Chapter 2

ASTR 2310: Chapter 2 Emergence of Modern Astronomy Early Greek Astronomy Ptolemaic Astronomy Copernican Astronomy Galileo: The First Modern Scientist Kepler's Laws of Planetary Motion Proof of the Earth's Motion Early Greek

More information

Benefit of astronomy to ancient cultures

Benefit 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 information

Ch. 22 Origin of Modern Astronomy Pretest

Ch. 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 information

The 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. 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 information

Learning Objectives. one night? Over the course of several nights? How do true motion and retrograde motion differ?

Learning 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 information

18. Kepler as a young man became the assistant to A) Nicolaus Copernicus. B) Ptolemy. C) Tycho Brahe. D) Sir Isaac Newton.

18. 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 information

7.4 Universal Gravitation

7.4 Universal Gravitation Circular Motion Velocity is a vector quantity, which means that it involves both speed (magnitude) and direction. Therefore an object traveling at a constant speed can still accelerate if the direction

More information

Astronomy 1 Fall 2016

Astronomy 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 information

Today FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus.

Today FIRST HOMEWORK DUE. Ancient Astronomy. Competing Cosmologies. Geocentric vs. Heliocentric. Ptolemy vs. copernicus. Today FIRST HOMEWORK DUE Ancient Astronomy Competing Cosmologies Geocentric vs. Heliocentric Ptolemy vs. copernicus Retrograde Motion Phases of Venus Galileo 1 3.1 The Ancient Roots of Science Our goals

More information

BROCK 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. 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 information

Ancient Cosmology: A Flat Earth. Alexandria

Ancient 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 information

b. Remember, Sun is a second or third generation star the nebular cloud of dust and gases was created by a supernova of a preexisting

b. 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 information

Unit 2: Celestial Mechanics

Unit 2: Celestial Mechanics Unit 2: Celestial Mechanics The position of the Earth Ptolemy (90 168 AD) Made tables that allowed a user to locate the position of a planet at any past, present, or future date. In order to maintain circular

More information

What was once so mysterious about planetary motion in our sky? We see apparent retrograde motion when we pass by a planet

What was once so mysterious about planetary motion in our sky? We see apparent retrograde motion when we pass by a planet What was once so mysterious about planetary motion in our sky? Planets usually move slightly eastward from night to night relative to the stars. You cannot see this motion on a single night. But sometimes

More information

a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU

a. 0.5 AU b. 5 AU c. 50 AU d.* AU e AU 1 AST104 Sp04: WELCOME TO EXAM 1 Multiple Choice Questions: Mark the best answer choice. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1. A galaxy

More information

Introduction To Modern Astronomy II

Introduction 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 information

Planetary Orbits: Kepler s Laws 1/18/07

Planetary 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

The History of Astronomy. Theories, People, and Discoveries of the Past

The 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 information

ASTRO 6570 Lecture 1

ASTRO 6570 Lecture 1 ASTRO 6570 Lecture 1 Historical Survey EARLY GREEK ASTRONOMY: Earth-centered universe - Some radical suggestions for a sun-centered model Shape of the Earth - Aristotle (4 th century BCE) made the first

More information

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets) Models of the Universe:

Days of the week: - named after 7 Power (moving) objects in the sky (Sun, Moon, 5 planets)   Models of the Universe: Motions of the Planets ( Wanderers ) Planets move on celestial sphere - change RA, Dec each night - five are visible to naked eye Mercury, Venus, Mars, Jupiter, Saturn Days of the week: - named after 7

More information

Chapter 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. 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 information

EXAM #2. ANSWERS ASTR , Spring 2008

EXAM #2. ANSWERS ASTR , Spring 2008 EXAM #2. ANSWERS ASTR 1101-001, Spring 2008 1. In Copernicus s heliocentric model of the universe, which of the following astronomical objects was placed in an orbit around the Earth? The Moon 2. In his

More information

a. 0.1 AU b. 10 AU c light years d light years

a. 0.1 AU b. 10 AU c light years d light years 1 AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the best answer choice on the bubble form. Read all answer choices before making selection. (No credit given when multiple answers are marked.) 1.

More information

Chapter 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. 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 information

Copernican Revolution 15 Jan. Copernican Revolution: questions on reading assignment

Copernican 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 information

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force

9/12/2010. The Four Fundamental Forces of Nature. 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force The Four Fundamental Forces of Nature 1. Gravity 2. Electromagnetism 3. The Strong Nuclear Force 4. The Weak Nuclear Force The Universe is made of matter Gravity the force of attraction between matter

More information

Evidence that the Earth does not move: Greek Astronomy. Aristotelian Cosmology: Motions of the Planets. Ptolemy s Geocentric Model 2-1

Evidence 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 information

Models of the Solar System, Gravitation and the motion of the Planets A.K.A DEAD WHITE GUYS WEEK! 1/28/14

Models of the Solar System, Gravitation and the motion of the Planets A.K.A DEAD WHITE GUYS WEEK! 1/28/14 Models of the Solar System, Gravitation and the motion of the Planets A.K.A DEAD WHITE GUYS WEEK! 1/28/14 Cosmogony A cosmogony is theory about ones place in the universe. A geocentric cosmogony is a theory

More information

Johannes Kepler ( ) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it!

Johannes Kepler ( ) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it! Johannes Kepler (1571-1630) German Mathematician and Astronomer Passionately convinced of the rightness of the Copernican view. Set out to prove it! Kepler s Life Work Kepler sought a unifying principle

More information

Early Theories. Early astronomers believed that the sun, planets and stars orbited Earth (geocentric model) Developed by Aristotle

Early 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 information

Gravity. 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 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 information

Midterm 1: Friday Sept 25 (this Friday) Practice Midterm on course web page (also under Supplementary Material > Midterm 1)

Midterm 1: Friday Sept 25 (this Friday) Practice Midterm on course web page (also under Supplementary Material > Midterm 1) Reminders 1 No Online Quiz this Week 2 Midterm 1: Friday Sept 25 (this Friday) Bring OU ID Pencil Eraser 3 Practice Midterm on course web page (also under Supplementary Material > Midterm 1) 4 All lectures

More information

Exam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points)

Exam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points) Exam #1 Study Guide (Note this is not all the information you need to know for the test, these are just SOME of the main points) Moon Phases Moon is always ½ illuminated by the Sun, and the sunlit side

More information

cosmogony geocentric heliocentric How the Greeks modeled the heavens

cosmogony 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 information

How Astronomers Learnt that The Heavens Are Not Perfect

How 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 information

Occam s Razor: William of Occam, 1340(!)

Occam s Razor: William of Occam, 1340(!) Reading: OpenStax, Chapter 2, Section 2.2 &2.4, Chapter 3, Sections 3.1-3.3 Chapter 5, Section 5.1 Last time: Scales of the Universe Astro 150 Spring 2018: Lecture 2 page 1 The size of our solar system,

More information

BROCK 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. 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: 30 Examination date: 10 November 2014 Time limit: 50 min Time of Examination: 9:00

More information

Astr 1050 Mon. Feb. 6, 2017

Astr 1050 Mon. Feb. 6, 2017 Astr 1050 Mon. Feb. 6, 2017 Finish Ch. 2: Discovering the Universe Eclipses Phases of the moon Start Ch. 3: Science (and History) of Astronomy Reading: For Friday: Chapter 3 Chapter #3 on MA Due Wednesday

More information

Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

Claudius 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 information

lightyears observable universe astronomical unit po- laris perihelion Milky Way

lightyears observable universe astronomical unit po- laris perihelion Milky Way 1 Chapter 1 Astronomical distances are so large we typically measure distances in lightyears: the distance light can travel in one year, or 9.46 10 12 km or 9, 600, 000, 000, 000 km. Looking into the sky

More information

Equation of orbital velocity: v 2 =GM(2/r 1/a) where: G is the gravitational constant (G=6.67x10 11 N/m 3 kg), M is the mass of the sun (or central

Equation of orbital velocity: v 2 =GM(2/r 1/a) where: G is the gravitational constant (G=6.67x10 11 N/m 3 kg), M is the mass of the sun (or central Everything in Orbit Orbital Velocity Orbital velocity is the speed at which a planetary body moves in its orbit around another body. If orbits were circular, this velocity would be constant. However, from

More information

You should have finished reading Chapter 3, and started on chapter 4 for next week.

You should have finished reading Chapter 3, and started on chapter 4 for next week. Announcements Homework due on Sunday at 11:45pm. Thank your classmate! You should have finished reading Chapter 3, and started on chapter 4 for next week. Don t forget your out of class planetarium show

More information

2. Who first reached India by sailing around the South African Cape?

2. Who first reached India by sailing around the South African Cape? PHY 1033 HIS 3931 IDH 331 Mid-term exam solutions Exam was Oct. 20, 2016 Solutions posted Oct. 23, 2016 Part I (30 points) Mulitple choice. Choose the best selection 1. Which of the following did Aristotle

More information

Wednesday, January 28

Wednesday, January 28 Ptolemy to Copernicus Wednesday, January 28 Astronomy of the ancients Many ancient cultures took note of celestial objects and celestial lphenomena. They noted tdcertain ti patterns in the heavens and

More information

Announcements. Topics To Be Covered in this Lecture

Announcements. 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 information

Pull out a ½ sheet or use the back of your old quiz

Pull out a ½ sheet or use the back of your old quiz Pull out a ½ sheet or use the back of your old quiz Weekly Schedule Today Hw # 2 due Quiz # 2 Geocentric vs. Heliocentric models Kepler s Laws Astronomy InteracGves Newton and Gravity Lecture tutorials

More information

Things 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. 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 information

January 19, notes.notebook. Claudius Ptolemaeus Second Century AD. Jan 5 7:37 AM

January 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 information

Scientific Method. Ancient Astronomy. Astronomy in Ancient Times

Scientific Method. Ancient Astronomy. Astronomy in Ancient Times Scientific Method Chapter 2: The Copernican Revolution The Birth of Modern Science Ancient Astronomy Models of the Solar System Laws of Planetary Motion Newton s Laws Laws of Motion Law of Gravitation

More information

ASTR-1010: Astronomy I Course Notes Section III

ASTR-1010: Astronomy I Course Notes Section III ASTR-1010: Astronomy I Course Notes Section III Dr. Donald G. Luttermoser Department of Physics and Astronomy East Tennessee State University Edition 2.0 Abstract These class notes are designed for use

More information

Plato ( BC) All natural motion is circular Reason is more important than observation

Plato ( BC) All natural motion is circular Reason is more important than observation Plato (428-348 BC) All natural motion is circular Reason is more important than observation Aristotle (384-322 BC) Physics elements earth water air fire quintessence Eratosthenes (276-195 BC) He measured

More information

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

ASTR 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 information

Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are

Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are Exam #1 Covers material from first day of class, all the way through Tides and Nature of Light Supporting reading chapters 1-5 Some questions are concept questions, some involve working with equations,

More information

4. Gravitation & Planetary Motion. Mars Motion: 2005 to 2006

4. Gravitation & Planetary Motion. Mars Motion: 2005 to 2006 4. Gravitation & Planetary Motion Geocentric models of ancient times Heliocentric model of Copernicus Telescopic observations of Galileo Galilei Systematic observations of Tycho Brahe Three planetary laws

More information

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017

Lecture 3: History of Astronomy. Astronomy 111 Monday September 4, 2017 Lecture 3: History of Astronomy Astronomy 111 Monday September 4, 2017 Reminders Labs start this week Homework #2 assigned today Astronomy of the ancients Many ancient cultures took note of celestial objects

More information

AST 105. Introduction to Astronomy: The Solar System. Announcement: First Midterm this Thursday 02/25

AST 105. Introduction to Astronomy: The Solar System. Announcement: First Midterm this Thursday 02/25 AST 105 Introduction to Astronomy: The Solar System Announcement: First Midterm this Thursday 02/25 REVIEW Newton s 3 Laws of Motion 1. An object moves at constant velocity if there is no net force acting

More information

Position 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. 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 information

The Origin of Modern Astronomy. Nicolai Copernicus ( )

The Origin of Modern Astronomy. Nicolai Copernicus ( ) The Origin of Modern Astronomy Nicolai Copernicus (1473-1543) Goals for Today Complete our study of the Moon: lunar phases, the Sun-Earth-Moon geometry, and the eclipses Tides and their origin Earth's

More information

Test Bank for Life in the Universe, Third Edition Chapter 2: The Science of Life in the Universe

Test Bank for Life in the Universe, Third Edition Chapter 2: The Science of Life in the Universe 1. The possibility of extraterrestrial life was first considered A) after the invention of the telescope B) only during the past few decades C) many thousands of years ago during ancient times D) at the

More information

Chapter. Origin of Modern Astronomy

Chapter. 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 information

Chapter 2 The Science of Life in the Universe

Chapter 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

Astronomy Lesson 8.1 Astronomy s Movers and Shakers

Astronomy Lesson 8.1 Astronomy s Movers and Shakers 8 Astronomers.notebook Astronomy Lesson 8.1 Astronomy s Movers and Shakers Aristotle 384 322 BCE Heavenly objects must move on circular paths at constant speeds. Earth is motionless at the center of the

More information

Astronomy 101 Exam 2 Form Akey

Astronomy 101 Exam 2 Form Akey Astronomy 101 Exam 2 Form Akey Name: Lab section number: (In the format M0**. See back page; if you get this wrong you may not get your exam back!) Exam time: one hour and twenty minutes Please put bags

More information

The Birth of Astronomy. Lecture 3 1/24/2018

The Birth of Astronomy. Lecture 3 1/24/2018 The Birth of Astronomy Lecture 3 1/24/2018 Fundamental Questions of Astronomy (life?) What is the shape of the Earth? How big is the planet we live on? Why do the stars move across the sky? Where is Earth

More information

Astronomy 101 Exam 2 Form Bkey

Astronomy 101 Exam 2 Form Bkey Astronomy 101 Exam 2 Form Bkey Name: Lab section number: (In the format M0**. See back page; if you get this wrong you may not get your exam back!) Exam time: one hour and twenty minutes Please put bags

More information

Origins of Modern Astronomy

Origins of Modern Astronomy PHYS 1411 Introduction to Astronomy Origins of Modern Astronomy Chapter 4 Topics in Chapter 4 Chapter 4 talks about the history of Astronomy and the development of the model of the solar system. Brief

More information

Astronomy 101 Exam 2 Form Dkey

Astronomy 101 Exam 2 Form Dkey Astronomy 101 Exam 2 Form Dkey Name: Lab section number: (In the format M0**. See back page; if you get this wrong you may not get your exam back!) Exam time: one hour and twenty minutes Please put bags

More information

Copernican Revolution. ~1500 to ~1700

Copernican 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 information

Gravity and the Orbits of Planets

Gravity and the Orbits of Planets Gravity and the Orbits of Planets 1. Gravity Galileo Newton Earth s Gravity Mass v. Weight Einstein and General Relativity Round and irregular shaped objects 2. Orbits and Kepler s Laws ESO Galileo, Gravity,

More information

In this chapter, you will consider the force of gravity:

In this chapter, you will consider the force of gravity: Gravity Chapter 5 Guidepost In this chapter, you will consider the force of gravity: What were Galileo s insights about motion and gravity? What were Newton s insights about motion and gravity? How does

More information

Planets & The Origin of Science

Planets & 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 information

Physics Unit 7: Circular Motion, Universal Gravitation, and Satellite Orbits. Planetary Motion

Physics 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 information

Review 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 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 information

towards the modern view

towards the modern view Brief review of last time: Og through Tycho Brahe Early Science 1 Reading: Chap. 2, Sect.2.4, Ch. 3, Sect. 3.1 Homework 3: Due Tomorrow and Mon. Homework 4: Now available, due next recitation cycle, or

More information

Observing the Solar System 20-1

Observing the Solar System 20-1 Observing the Solar System 20-1 Ancient Observations The ancient Greeks observed the sky and noticed that the moon, sun, and stars seemed to move in a circle around the Earth. It seemed that the Earth

More information

Space Notes Covers Objectives 1 & 2

Space Notes Covers Objectives 1 & 2 Space Notes Covers Objectives 1 & 2 Space Introduction Space Introduction Video Celestial Bodies Refers to a natural object out in space 1) Stars 2) Comets 3) Moons 4) Planets 5) Asteroids Constellations

More information

Chapter 2 The Copernican Revolution

Chapter 2 The Copernican Revolution Chapter 2 The Copernican Revolution Units of Chapter 2 2.1 Ancient Astronomy 2.2 The Geocentric Universe 2.3 The Heliocentric Model of the Solar System The Foundations of the Copernican Revolution 2.4

More information

Topic 10: Earth in Space Workbook Chapters 10 and 11

Topic 10: Earth in Space Workbook Chapters 10 and 11 Topic 10: Earth in Space Workbook Chapters 10 and 11 We can imagine all the celestial objects seen from Earth the sun, stars, the Milky way, and planets as being positioned on a celestial sphere. Earth

More information

Be able to assess how each of the geocentric and heliocentric models explains rising and setting, motion of the Sun, motion of the planets.

Be able to assess how each of the geocentric and heliocentric models explains rising and setting, motion of the Sun, motion of the planets. Astronomy 110 Test 2 Review (also quiz 2) NOTE: THIS IS NOT MEANT TO BE EXHAUSTIVE, THIS IS TO HELP THE YOU TRAIN ON THE QUESTION FORMATS AND THE CONCEPTS. Just because an issue is mentioned here does

More information

Lecture #5: Plan. The Beginnings of Modern Astronomy Kepler s Laws Galileo

Lecture #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 information

How big is the Universe and where are we in it?

How big is the Universe and where are we in it? Announcements Results of clicker questions from Monday are on ICON. First homework is graded on ICON. Next homework due one minute before midnight on Tuesday, September 6. Labs start this week. All lab

More information