1. Which of the following correctly lists our cosmic address from small to large?
|
|
- Reynard Fowler
- 6 years ago
- Views:
Transcription
1 1. Which of the following correctly lists our cosmic address from small to large? (a) Earth, solar system, Milky Way Galaxy, Local Group, Local Super Cluster, universe (b) Earth, solar system, Milky Way Galaxy, Local Super Cluster, Local Group, universe (c) universe, Local Super Cluster, Local Group, Milky Way Galaxy, solar system, Earth (d) universe, Local Group, Local Super Cluster, Milky Way Galaxy, solar system, Earth (e) Earth, Local Group, Local Super Cluster, Milky Way Galaxy, solar system, universe (a) is the right answer. 2. How long is a light-second? (a) m (b) m (c) m (d) m (e) m (a) is the right answer. The speed of light is c = m/s. So one light-second is c (1 sec) = m. 3. If you are looking at a star that is 4 light-years away from Earth, you are looking at: (a) The star as it is right now (b) The star as it was 4 years ago (c) The star as it will be 4 years in the future (d) The star as it was years ago (e) The star as it will be years in the future (b). The light has to travel for 4 years to get to Earth. 4. Which one of the following is the correct description or the right usage of the Astronomical Unit (AU)? (a) 1 AU is the average distance of the most distant planet in the solar system from our sun. (b) When the parallax angle of an astronomical object is a small angle p, then the distance to that object is given by 1 AU/p. (c) 1 AU equals 1.3 light-second. (d) 1 AU equals km. (e) None of the above (b). It s the distance of Earth from the sun. 500 light-seconds or km. Distance measurement using parallax relies on our knowing 1 AU accurately. 1
2 5. What is the current estimate of the age of the universe? (a) years (b) years (c) years (d) years (e) years (e). 14 billion years. 6. Which one of the following is a false description of an astronomical object? (a) A star is a hot ball of gas powered by nuclear reaction at its core. (b) A galaxy is an island of stars in space containing stars held by gravity. (c) The observable universe may not be the whole universe. (d) The star systems can form a cluster, but galaxies do not form clusters. (e) A star system can have more than one star in the system. (d). For instance, the Local Super Cluster is a cluster of galaxies including our galaxy. 7. Where or when is the star stuff formed? (a) Only during the first 300,000 years of the universe (b) Only inside relatively light stars like our sun (c) Only inside stars much heavier than our sun (d) Only when a supernovae explosion occurs (e) Inside any bright star (e). Star stuff means heavier elements of which we are made. It is made inside bright stars. See the summary of Chapter 1. NOTE ADDED: Although (a-d) are clearly wrong since star stuff cannot be generated only in those times or places, I can see that one can conceivably be confused by the qualifier any in (e). Hence, I am going to give everyone full mark for this one. 2
3 8. If the distance to galaxy A from us is the farther than the the distance to galaxy B from us, which of the following is right? (a) If the two galaxies are within our Local Group, they can move in any directions, but the speed of A must be greater than the speed of B. (b) If the two galaxies are within our Local Group, they can move in any directions, but the speed of B must be greater than the speed of A. (c) If the two galaxies are within our Local Group, they can only move away from us but their speed can be essentially random. (d) If the two galaxies are outside of our Local Group, they can move in any directions, but the speed of B must be greater than the speed of A. (e) If the two galaxies are outside our Local Group, they only move away from us and the speed of A is greater than the speed of B. (e). Universe expands. Farther galaxies receed faster. This is the raisin problem in the homework. 9. Which one of the following falsely describes a part in scientific method? (a) Making a hypothesis (b) Performing experiments to test the hypothesis (c) Analyzing the experimental outcome to determine the validity of the hypothesis (d) Deciding that the hypothesis will apply to all physical situations when it is confirmed (e) Making a new hypothesis based on the experimental outcome (d). One can never be sure that one s hypothesis will apply to all physical situations. One cannot decide what a law of nature should be. 10. Which of the following correctly describes Kepler s first law? (a) There are comets that goes around the sun only once. (b) The moon is pulled by Earth just as Earth is pulled by the moon. (c) The sun sits at one of the two foci in Earth s elliptic orbit. (d) A moving object will keep its velocity unless there is a force acting on it. (e) All forces are attractive. (c). Kepler s first law states a planet s orbit is an ellipse with the sun at one focus. Earth is a planet. 3
4 11. Which conservation law directly explains Kepler s second law? (a) Energy conservation (b) Power conservation (c) Angular momentum conservation (d) Linear momentum conservation (e) Force conservation (c). When a planet is closer to the sun, it moves faster, just like the spinning figure skater spins faster when the arms are drawn closer. NOTE ADDED: Energy conservation tells you that when a planet is closer to the sun, it must move faster since kinetic energy has to increase. However, energy conservation does not tell you how the orbit should change. In particular, energy conservation is not enough to get the equal area sweep in equal time law of Kepler. This is due to angular momentum conservation. Thus strictly speaking only (c) is the right answer. However, I realize that this distinction may be too much for an introductory course like ours. I will allow both (a) and (c) to be right. 12. Suppose a new planet is found at 16 AU from our sun. What will its period be? (a) 32 years (b) 64 years (c) 128 years (d) 256 years (e) 512 years (b). Use p 2 = a 3. p = 16 3 = 64. 4
5 13. Which one of the following about Newton s three laws of motion is true? (a) If the speed of the object is close to the speed of light, Newton s first law does not apply. False. The law of inertia applies to all speed. (b) When the speed of an object stays the same, there cannot be a net force acting on this object. False. The object can change direction. That cannot happen without a force. (c) When the velocity of an object stays the same, there cannot be a net force acting on this object. True. This is Newton s first law. (d) The laws apply only to objects on Earth. They do not apply to astronomical objects. False. The laws are universal. (e) The laws apply only to a moving object. They do not apply to a stationary object. False. 14. According to Newton s second law, (a) The acceleration caused by a force is inversely proportional to the mass of the object. True. F = ma means a = F/m. (b) The acceleration caused by the same amount of force depends not only on the mass of the object but also on the shape of the object. False. There is no shape information in F = ma. (c) Friction force does not count as a real force. False. Friction is a real force. (d) Every mass attracts every other mass. This is Newton s law of gravity, not the second law. (e) The magnitude of the gravitational force between two objects is proportional to the product of the two masses. This is Newton s law of gravity, not the second law. 15. What is the force that is directly responsible for propelling a rocket when its engine is fully on? (a) The gravitational force of large objects in space, such as galaxies, collectively acting on the rocket (b) The chemical composition of the exhaust gas (c) The reaction force exerted by the exhaust gas (d) Earth s gravity (e) Earth s angular momentum (c). This is Newton s third law. Action and Reaction. 5
6 16. What is a parsec? (a) The same as 1 light-year. (b) The same as 500 light-second. (c) The size of the observable universe. (d) The size of our solar system. (e) The distance of an object that has 1/3600 degree parallax angle (e). This is the definition. 17. Which one of the following people championed the geocentric view of the solar system? (a) Ptolemy (b) Copernicus (c) Galileo (d) Kepler (e) Newton (a). All others are advocates of the heliocentric (sun-centered) view. 18. The radius of the sun is known to be R = m. The density of the sun is known to be about kg/m 3, that is, 1 m 3 volume of the sun contains about 1, 400 kg of material. Assuming the sun is a sphere (volume = 4πR 3 /3), which of the following is a good estimate of the mass of the sun? (a) kg (b) kg (c) kg (d) kg (e) kg (e). Volume is V = 4πR 3 /3 = m 3. Multiply this by the density to get M = m kg/m 3 = kg (1) 6
7 19. Visible colors correspond to the wavelength range of nm nm. Which one of the following is the equivalent frequency range? (Hz = 1/s) (a) Hz Hz (b) Hz Hz (c) Hz Hz (d) Hz Hz (e) Hz Hz (e). Use λf = c. f = m/s/( m) = Hz and f = m/s/( m) = Hz 20. When the frequency of a light wave is f, what is the energy of the corresponding energy of the photon? (h is the Planck constant.) (a) E = hf (b) E = hf 2 (c) E = hf 3 (d) E = h/f (e) E = h/f 2 (a). 7
Kepler, Newton, and laws of motion
Kepler, Newton, and laws of motion First: A Little History Geocentric vs. heliocentric model for solar system (sec. 2.2-2.4)! The only history in this course is this progression: Aristotle (~350 BC) Ptolemy
More informationHow 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 informationTest 1 Review Chapter 1 Our place in the universe
Test 1 Review Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the scantrons Formulas will be projected on the screen You can use
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 informationCopyright 2010 Pearson Education, Inc. GRAVITY. Chapter 12
GRAVITY Chapter 12 Units of Chapter 12 Newton s Law of Universal Gravitation Gravitational Attraction of Spherical Bodies Kepler s Laws of Orbital Motion Gravitational Potential Energy Energy Conservation
More informationChapter 12 Gravity. Copyright 2010 Pearson Education, Inc.
Chapter 12 Gravity Units of Chapter 12 Newton s Law of Universal Gravitation Gravitational Attraction of Spherical Bodies Kepler s Laws of Orbital Motion Gravitational Potential Energy Energy Conservation
More informationLESSON 1. Solar System
Astronomy Notes LESSON 1 Solar System 11.1 Structure of the Solar System axis of rotation period of rotation period of revolution ellipse astronomical unit What is the solar system? 11.1 Structure of the
More informationMotion, Energy, and Gravity. Reminder to take out your clicker and turn it on!
Motion, Energy, and Gravity Reminder to take out your clicker and turn it on! Attendance Quiz Are you here today? Here! (a) yes (b) no (c) Opening Day is here! x Clickers I have not been able to download
More informationA = 6561 times greater. B. 81 times greater. C. equally strong. D. 1/81 as great. E. (1/81) 2 = 1/6561 as great Pearson Education, Inc.
Q13.1 The mass of the Moon is 1/81 of the mass of the Earth. Compared to the gravitational force that the Earth exerts on the Moon, the gravitational force that the Moon exerts on the Earth is A. 81 2
More informationWhat is the solar system?
Notes Astronomy What is the solar system? 11.1 Structure of the Solar System Our solar system includes planets and dwarf planets, their moons, a star called the Sun, asteroids and comets. Planets, dwarf
More informationMost 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 information7.4 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 informationGravitation 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 informationHow do we describe motion?
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity How do we describe motion? Precise definitions to describe motion: Speed: Rate at which object moves example: speed of
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 informationName and Student ID Section Day/Time:
AY2 - Overview of the Universe - Midterm #1 - Instructor: Maria F. Duran Name and Student ID Section Day/Time: 1) Imagine we ve discovered a planet orbiting another star at 1 AU every 6 months. The planet
More informationAY2 Winter 2017 Midterm Exam Prof. C. Rockosi February 14, Name and Student ID Section Day/Time
AY2 Winter 2017 Midterm Exam Prof. C. Rockosi February 14, 2017 Name and Student ID Section Day/Time Write your name and student ID number on this printed exam, and fill them in on your Scantron form.
More informationExam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti
Exam # 3 Tue 12/06/2011 Astronomy 100/190Y Exploring the Universe Fall 11 Instructor: Daniela Calzetti INSTRUCTIONS: Please, use the `bubble sheet and a pencil # 2 to answer the exam questions, by marking
More informationGravity & The Distances to Stars. Lecture 8. Homework 2 open Exam on Tuesday in class bring ID and #2 pencil
1 Gravity & The Distances to Stars Lecture 8 Homework 2 open Exam on Tuesday in class bring ID and #2 pencil 2 Preparing for the Exam 1 Exams in this class are multiple choice, but the questions can be
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 informationBasics of Kepler and Newton. Orbits of the planets, moons,
Basics of Kepler and Newton Orbits of the planets, moons, Kepler s Laws, as derived by Newton. Kepler s Laws Universal Law of Gravity Three Laws of Motion Deriving Kepler s Laws Recall: The Copernican
More informationThe Cosmic Perspective Seventh Edition. Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Chapter 4 Lecture
Chapter 4 Lecture The Cosmic Perspective Seventh Edition Making Sense of the Universe: Understanding Motion, Energy, and Gravity 2014 Pearson Education, Inc. Making Sense of the Universe: Understanding
More information2010 Pearson Education, Inc. Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion: Examples from Daily Life Some of the topics we will explore: How do we describe motion? (Speed,
More informationAST 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 informationPhysics Test 7: Circular Motion page 1
Name Physics Test 7: Circular Motion page 1 hmultiple Choice Read each question and choose the best answer by putting the corresponding letter in the blank to the left. 1. The SI unit of angular speed
More informationChapter 13: universal gravitation
Chapter 13: universal gravitation Newton s Law of Gravitation Weight Gravitational Potential Energy The Motion of Satellites Kepler s Laws and the Motion of Planets Spherical Mass Distributions Apparent
More informationName. F = ma P 2 = a 3 (M + m) P 2 = a 3. maxt = 2900 K m
Spring 2019 Astronomy - Test 1 Test form D Name Do not forget to write your name and fill in the bubbles with your student number, and fill in test form D on the answer sheet. Write your name above as
More informationASTR : Stars & Galaxies (Spring 2019)... Study Guide for Midterm 1
ASTR-1200-01: Stars & Galaxies (Spring 2019)........................ Study Guide for Midterm 1 The first midterm exam for ASTR-1200 takes place in class on Wednesday, February 13, 2019. The exam covers
More informationASTRONOMY 1010 Exam 1 September 21, 2007
ASTRONOMY 1010 Exam 1 September 21, 2007 Name Please write and mark your name and student number in the Scantron answer sheet. FILL THE BUBBLE IN THE "TEST FORM" BOX CORRESPONDING TO YOUR TEST VERSION
More informationEARTH SCIENCE UNIT 9 -NOTES ASTRONOMY
EARTH SCIENCE UNIT 9 -NOTES ASTRONOMY UNIT 9- ASTRONOMY 2 THE SOLAR SYSTEM I. The Solar System:. a. Celestial Body:. i. Examples:. b. MAIN COMPONENTS/MEMBERS OF THE SOLAR SYSTEM: i. 1. Planets are objects
More information21/11/ /11/2017 Space Physics AQA Physics topic 8
Space Physics AQA Physics topic 8 8.1 Solar System, Orbits and Satellites The eight planets of our Solar System Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune As well as the eight planets, the
More informationWhat is a Satellite? A satellite is an object that orbits another object. Ex. Radio satellite, moons, planets
Planetary Orbit Planetary Orbits What shape do planets APPEAR to orbit the sun? Planets APPEAR to orbit in a circle. What shape do the planets orbit the sun??? Each planet Orbits the Sun in an ellipse
More informationIn 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 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 informationASTR 150. Planetarium Shows begin Sept 9th. Register your iclicker! Last time: The Night Sky Today: Motion and Gravity. Info on course website
Planetarium Shows begin Sept 9th Info on course website Register your iclicker! Last time: The Night Sky Today: Motion and Gravity ASTR 150 Hang on tight! Most math all semester-- get it over with right
More informationBy; Jarrick Serdar, Michael Broberg, Trevor Grey, Cameron Kearl, Claire DeCoste, and Kristian Fors
By; Jarrick Serdar, Michael Broberg, Trevor Grey, Cameron Kearl, Claire DeCoste, and Kristian Fors What is gravity? Gravity is defined as the force of attraction by which terrestrial bodies tend to fall
More informationHow do we describe motion?
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity How do we describe motion? Precise definitions to describe motion: Speed: Rate at which object moves $ speed = distance!#"units
More informationHow do we describe motion?
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion: Examples from Everyday Life Our goals for learning: How do we describe motion? How is mass different
More informationStars, Galaxies, and the Universe
Stars, Galaxies, and the Universe Chapter Test A Multiple Choice Write the letter of the correct answer on the line at the left. 1. What is a giant ball of hot gases that undergo nuclear fusion? a. a planet
More informationo Terms to know o Big Bang Theory o Doppler Effect o Redshift o Universe
Standard 1: Students will understand the scientific evidence that supports theories that explain how the universe and the solar system developed. They will compare Earth to other objects in the solar system.
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 informationAstronomy 1143 Final Exam Review Answers
Astronomy 1143 Final Exam Review Answers Prof. Pradhan April 24, 2015 What is Science? 1. Explain the difference between astronomy and astrology. 2. What number is the metric system based around? What
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 informationChapter 5 Centripetal Force and Gravity. Copyright 2010 Pearson Education, Inc.
Chapter 5 Centripetal Force and Gravity v Centripetal Acceleration v Velocity is a Vector v It has Magnitude and Direction v If either changes, the velocity vector changes. Tumble Buggy Demo v Centripetal
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 informationLecture 13. Gravity in the Solar System
Lecture 13 Gravity in the Solar System Guiding Questions 1. How was the heliocentric model established? What are monumental steps in the history of the heliocentric model? 2. How do Kepler s three laws
More informationPHYSICS. Chapter 13 Lecture FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E RANDALL D. KNIGHT Pearson Education, Inc.
PHYSICS FOR SCIENTISTS AND ENGINEERS A STRATEGIC APPROACH 4/E Chapter 13 Lecture RANDALL D. KNIGHT Chapter 13 Newton s Theory of Gravity IN THIS CHAPTER, you will learn to understand the motion of satellites
More informationMore examples: Summary of previous lecture
More examples: 3 N Individual Forces Net Force 5 N 37 o 4 N Summary of previous lecture 1 st Law A net non zero force is required to change the velocity of an object. nd Law What happens when there is
More informationPhys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 1
Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 1 MULTIPLE CHOICE (Right answers are reported in red) 1.. A solar system contains a. primarily planets. b. large amounts of gas and dust
More informationASTRONOMY LECTURE NOTES MIDTERM REVIEW. ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens
ASTRONOMY LECTURE NOTES MIDTERM REVIEW ASTRONOMY LECTURE NOTES Chapter 1 Charting the Heavens How Do We Locate Objects in the Sky? Local-Sky Coordinates versus Celestial-Sphere Coordinates When the sky
More informationBeyond the Solar System 2006 Oct 17 Page 1 of 5
I. Stars have color, brightness, mass, temperature and size. II. Distances to stars are measured using stellar parallax a. The further away, the less offset b. Parallax angles are extremely small c. Measured
More informationMaking Sense of the Universe (Chapter 4) Why does the Earth go around the Sun? Part, but not all, of Chapter 4
Making Sense of the Universe (Chapter 4) Why does the Earth go around the Sun? Part, but not all, of Chapter 4 Based on part of Chapter 4 This material will be useful for understanding Chapters 8 and 11
More information5. Universal Laws of Motion
5. Universal Laws of Motion If I have seen farther than others, it is because I have stood on the shoulders of giants. Sir Isaac Newton (164 177) Physicist Image courtesy of NASA/JPL Sir Isaac Newton (164-177)
More informationu Today I will look for key ideas in the text to support the role gravity has on the formation of the planets.
Space SC.8.E.5.4 SC.8.E.5.4: Explore the Law of Universal Gravitation by explaining the role that gravity plays in the formation of planets, stars, and solar systems, and determining their motions Game
More information4.1 Describing Motion
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion Our goals for learning: How do we describe motion? How is mass different from weight? How do we describe
More informationGravity and Orbits. Objectives. Clarify a number of basic concepts. Gravity
Gravity and Orbits Objectives Clarify a number of basic concepts Speed vs. velocity Acceleration, and its relation to force Momentum and angular momentum Gravity Understand its basic workings Understand
More information4.1 Describing Motion. How do we describe motion? Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 4.1 Describing Motion Our goals for learning: How do we describe motion? How is mass different from weight? How do we describe
More informationCIRCULAR MOTION AND UNIVERSAL GRAVITATION
CIRCULAR MOTION AND UNIVERSAL GRAVITATION Uniform Circular Motion What holds an object in a circular path? A force. String Friction Gravity What happens when the force is diminished? Object flies off in
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: 30 Examination date: 10 November 2014 Time limit: 50 min Time of Examination: 9:00
More informationAnswer Key for Exam C
Answer Key for Exam C 2 points each Choose the answer that best completes the question. Read each problem carefully and read through all the answers. Take your time. If a question is unclear, ask for clarification
More informationAnswer Key for Exam B
Answer Key for Exam B 2 points each Choose the answer that best completes the question. Read each problem carefully and read through all the answers. Take your time. If a question is unclear, ask for clarification
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 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 information4π 2 G(M1+M2 ) p2 = Newton s 3 Laws of Motion AST 105. Introduction to Astronomy: The Solar System. Newton's Version of Kepler's Third Law
REVIEW Newton s 3 Laws of Motion AST 105 Introduction to Astronomy: The Solar System Announcement: First Midterm this Thursday 02/25 Newton's Version of Kepler's Third Law Newton's Version of Kepler's
More informationAstro Lecture 12. Energy and Gravity (Cont d) 13/02/09 Habbal Astro Lecture 12 1
Astro 110-01 Lecture 12 Energy and Gravity (Cont d) 13/02/09 Habbal Astro110-01 Lecture 12 1 Energy due to movement of Kinetic Energy: object E k = ½ m v 2 13/02/09 Habbal Astro110-01 Lecture 12 2 Gravitational
More information4.3 Conservation Laws in Astronomy
4.3 Conservation Laws in Astronomy Our goals for learning: Why do objects move at constant velocity if no force acts on them? What keeps a planet rotating and orbiting the Sun? Where do objects get their
More informationBROCK UNIVERSITY. 1. About 2300 years ago, Aristotle argued that the Earth is spherical based on a number of observations, one of which was that
BROCK UNIVERSITY Page 1 of 10 Test 2: November 2015 Number of pages: 10 Course: ASTR 1P01, Section 2 Number of students: 861 Examination date: 7 November 2015 Time limit: 50 min Time of Examination: 13:00
More informationAnswer Key for Exam D
Answer Key for Exam D 2 points each Choose the answer that best completes the question. Read each problem carefully and read through all the answers. Take your time. If a question is unclear, ask for clarification
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 informationSOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES
SOLAR SYSTEM, STABILITY OF ORBITAL MOTIONS, SATELLITES Q1. The figure below shows what scientists over 1000 years ago thought the solar system was like. Give one way that the historical model of the solar
More informationKepler Galileo and Newton
Kepler Galileo and Newton Kepler: determined the motion of the planets. Understanding this motion was determined by physicists like Galileo and Newton and many others. Needed to develop Physics as a science:
More informationProperties of Motion. Force. Examples of Forces. Basics terms and concepts. Isaac Newton
Properties of Motion It took about 2500 years to different generations of philosophers, mathematicians and astronomers to understand Aristotle's theory of Natural Motion and Violent Motion: Falling bodies
More informationChapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Copyright 2012 Pearson Education, Inc.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity 1 4.1 Describing Motion: Examples from Everyday Life Our goals for learning: How do we describe motion? How is mass different
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 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 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 information9/12/2010. 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 informationGRAVITY IS AN ATTRACTIVE FORCE
WHAT IS GRAVITY? Gravity: force of attraction between objects due to their mass Gravity is a noncontact force that acts between two objects at any distance apart GRAVITY IS AN ATTRACTIVE FORCE Earth s
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 informationGravity 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 informationGraspIT Questions AQA GCSE Physics Space physics
A. Solar system: stability of orbital motions; satellites (physics only) 1. Put these astronomical objects in order of size from largest to smallest. (3) Fill in the boxes in the correct order. the Moon
More informationIntroduction 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 informationAstronomy. Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe.
Astronomy Study of objects in space such as the Sun, stars, planets, comets, gas, & galaxies. *Also, the Earth s place in the universe. Universe = everything that exists Disclaimer: Astrology is NOT science!!!
More informationNewton s Laws and the Nature of Matter
Newton s Laws and the Nature of Matter The Nature of Matter Democritus (c. 470-380 BCE) posited that matter was composed of atoms Atoms: particles that can not be further subdivided 4 kinds of atoms: earth,
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 informationThe Hertzsprung Russell Diagram. The Main Sequence
The Hertzsprung Russell Diagram H R diagram plots stellar luminosity against surface temperature Luminosity ranges 10-4 10 4 L. Temperature ranges by a factor of 10 increases to the left spectral sequence
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 informationlightyears 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 informationa. 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 informationChapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity. Copyright 2009 Pearson Education, Inc.
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity How do we describe motion? Precise definitions to describe motion: Speed: Rate at which object moves speed = distance time
More informationTest 4 Final Review. 5/2/2018 Lecture 25
Test 4 Final Review 5/2/2018 Lecture 25 Apparent daily motion of celestial objects is due to earth s rotation Seasons are created due to the title of the Earth relative to the Sun Phases of the moon due
More informationTHE SUN AND THE SOLAR SYSTEM
Chapter 26 THE SUN AND THE SOLAR SYSTEM CHAPTER 26 SECTION 26.1: THE SUN S SIZE, HEAT, AND STRUCTURE Objectives: What is the Sun s structure and source of energy? Key Vocabulary: Fusion Photosphere Corona
More informationAP Physics C Textbook Problems
AP Physics C Textbook Problems Chapter 13 Pages 412 416 HW-16: 03. A 200-kg object and a 500-kg object are separated by 0.400 m. Find the net gravitational force exerted by these objects on a 50.0-kg object
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 informationAgenda Announce: 4.1 Describing Motion. Tests. How do we describe motion?
Chapter 4 Making Sense of the Universe: Understanding Motion, Energy, and Gravity Agenda Announce: Stony Brook talk this Friday on Precision Cosmology Project Part I due in one week before class: one paragraph
More informationAstronomy, PART 2. Vocabulary. A. Universe - Our Milky Way Galaxy is one of of galaxies in an expanding universe.
Astronomy, PART 2 Vocabulary Aphelion Asteroid Astronomical Unit Comet Constellation Crater Eccentricity Eclipse Equinox Geocentric model Gravitation Heliocentric model Inertia Jovian Perihelion Revolution
More informationChapter 4: Energy, Motion, Gravity. Enter Isaac Newton, who pretty much gave birth to classical physics
Chapter 4: Energy, Motion, Gravity Enter Isaac Newton, who pretty much gave birth to classical physics Know all of Kepler s Laws well Chapter 4 Key Points Acceleration proportional to force, inverse to
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 informationAstron 104 Laboratory #4 Gravity and Orbital Motion
Name: Date: Section: Astron 104 Laboratory #4 Gravity and Orbital Motion Section 5.5, 5.6 Introduction No astronomical object can stand still gravity makes certain of this. Newton s Law of Universal Gravitation
More information