Basic Physics. Remaining Topics. Gravitational Potential Energy. PHYS 1403 Introduction to Astronomy. Can We Create Artificial Gravity?
|
|
- Abraham Black
- 5 years ago
- Views:
Transcription
1 PHYS 1403 Introduction to Astronomy Basic Physics Chapter 5 Remaining Topics Gravitational Potential Energy Escape Velocity Artificial Gravity Gravity Assist An Alternate Theory of Gravity Gravitational Potential Energy It is the gravitational energy the object would have above the earth surface. GPE = Gravitational Force x Distance GPE Satellite (m) Distance (r) Earth (M) Escape Velocity Escape velocity is the velocity required to escape an astronomical body For the case of Rocket on Earth If mass of the spaceship << the mass of Earth, then the escape velocity is Can We Create Artificial Gravity? M = mass of the central body in kg G = gravitational constant (6.67ˣ10-11 m3/s2/kg) r = radius of the central body For Earth it is 11.2 km/s or 24,600 miles/hour cv.nrao.edu 1
2 Concept What is Gravity Assist? Image source: NASA, STSI Source: wikipedia How to increase velocity of a spacecraft without using fuel? Source: wikipedia Gravity Assist An Alternative viewpoint of Gravity What is Gravity? Newton's View Gravity A force called gravity keeps the planets in motion around the Sun. The motion of planets can be described by Newton s laws of motion and law of gravity Space is static i.e. not expanding or contracting Space is flat Euclid s law of geometry applies The acceleration due to a force on a body depends on the mass (we call this mass inertial mass ). a = F / m i i = inertial 2
3 Einstein and Relativity Einstein ( ) Noticed that Newton s laws of motion are only correct in the limit of low velocities (speeds <<speed of light) leading to his theory of special relativity Also revised the understanding of gravity leading to his theory of general relativity The First Postulate of Relativity The principle of relativity says that observers can never detect their uniform motion, except relative to other objects. Neither of these travelers can decide who is moving and who is not. The Second Postulate of Relativity The speed of light in a vacuum is constant and will have the same value for all observers independent of their motion relative to the light source The Theory of Special Relativity The first two postulates describe the theory of special relativity Observed mass of a moving particle depends on its velocity The energy of a body at rest 0 Instead, we find E = m 0 c 2 Effects of Special Relativity The observed mass of moving electrons depends on their velocity. As the ratio of their velocity to the velocity of light, v/c, increases, the mass of the electrons relative to their mass at rest, m/m 0, increases. Such relativistic effects are quite evident in particle accelerators, which accelerate atomic particles to very high velocities. The Third Postulate of Relativity The general theory of relativity The equivalence principle: new description of gravity Observers cannot distinguish locally between inertial forces due to acceleration and uniform gravitational forces due to the presence of a massive body 3
4 Inertia and Acceleration in a Spaceship (a) An observer in a closed spaceship on the surface of a planet feels gravity. (b) In space, with the rockets smoothly firing and accelerating the spaceship, the observer feels inertial forces that are equivalent to gravitational forces. Einstein Einstein view on Gravity Uses principle of equivalence to put forth his theory of General Relativity Mass and energy are related E = mc 2 Gravity is a property of space-time not matter Gravity affects light even though it has no mass Confirmation of the Curvature of Space- Time: Mercury s Perihelion (a) Mercury s orbit precesses arc seconds per century faster than predicted by Newton s laws. (b) Even when you ignore the influences of the other planets, Mercury s orbit is not a perfect ellipse. Curved space-time near the Sun distorts the orbit from an ellipse into a rosette. The advance of Mercury s perihelion is exaggerated by a factor of about one million in this figure. Confirmation of the Curvature of Space- Time: Deflection of Sunlight Like a depression in a putting green, the curved space-time near the Sun deflects light from distant stars and makes them appear to lie slightly farther from the Sun than their true positions. Quora.com Einstein Theory of Gravity Comparing Newton and Einstein's View Newton Mass and energy are very different Space and time are very different Light takes the shortest distance between two points Shortest distance is a straight line in flat space Mass tells gravity how much force to exert; force tells mass how to move Einstein Mass and energy are interchangeable Space and time are interchangeable, time is the 4 th dimension In presence of gravity space is curved not flat or mass curves space-time Mass-energy tells spacetime how to curve; curved space-time tells massenergy how to move 4
5 Worm Holes Sci Fi How to Make a Worm Hole? Acknowledgment The slides in this lecture is for Tarleton: PHYS1411/PHYS1403 class use only Images and text material have been borrowed from various sources with appropriate citations in the slides, including PowerPoint slides from Seeds/Backman text that has been adopted for class. 5
Basic Physics. What We Covered Last Class. Remaining Topics. Center of Gravity and Mass. Sun Earth System. PHYS 1411 Introduction to Astronomy
PHYS 1411 Introduction to Astronomy Basic Physics Chapter 5 What We Covered Last Class Recap of Newton s Laws Mass and Weight Work, Energy and Conservation of Energy Rotation, Angular velocity and acceleration
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 informationBasic Physics. Isaac Newton ( ) Topics. Newton s Laws of Motion (2) Newton s Laws of Motion (1) PHYS 1411 Introduction to Astronomy
PHYS 1411 Introduction to Astronomy Basic Physics Chapter 5 Topics Newton s Laws Mass and Weight Work, Energy and Conservation of Energy Rotation, Angular velocity and acceleration Centripetal Force Angular
More informationAstronomy 1141 Life in the Universe 10/24/12
Friday, October 19 Newton vs. Einstein 1) Newton: Gravity is a force acting between massive objects in static, Euclidean space. Guest lecturer: Barbara Ryden 2) Einstein: Gravity is the result of the curvature
More informationLecture 23 (Gravitation, Potential Energy and Gauss s Law; Kepler s Laws) Physics Spring 2017 Douglas Fields
Lecture 23 (Gravitation, Potential Energy and Gauss s Law; Kepler s Laws) Physics 160-02 Spring 2017 Douglas Fields Gravitational Force Up until now, we have said that the gravitational force on a mass
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 informationRelativity. Astronomy 101
Lecture 29: Special & General Relativity Astronomy 101 Common Sense & Relativity Common Sense is the collection of prejudices acquired by the age of 18. Albert Einstein It will seem difficult at first,
More informationOutline. General Relativity. Black Holes as a consequence of GR. Gravitational redshift/blueshift and time dilation Curvature Gravitational Lensing
Outline General Relativity Gravitational redshift/blueshift and time dilation Curvature Gravitational Lensing Black Holes as a consequence of GR Waste Disposal It is decided that Earth will get rid of
More information7 Study Guide. Gravitation Vocabulary Review
Date Period Name CHAPTER 7 Study Guide Gravitation Vocabulary Review Write the term that correctly completes the statement. Use each term once. Kepler s second law Newton s law of universal gravitation
More informationChapter 26. Relativity
Chapter 26 Relativity Time Dilation The vehicle is moving to the right with speed v A mirror is fixed to the ceiling of the vehicle An observer, O, at rest in this system holds a laser a distance d below
More informationGravity. Announcement. Topics in Chapter 5. Topics for Today. PHYS 1403 Introduction to Astronomy. Motion. Chapter 5. Exam 1
PHYS 1403 Introduction to Astronomy Gravity Chapter 5 Announcement Exam 1 February 21 st 2018 2:25pm 3:40 pm during class time Chapter 1,2,3,4 and 5 40 Multiple Questions. One short answer essay type question.
More informationLecture 18 Vacuum, General Relativity
The Nature of the Physical World Lecture 18 Vacuum, General Relativity Arán García-Bellido 1 Standard Model recap Fundamental particles Fundamental Forces Quarks (u, d, c, s, t, b) fractional electric
More information(ii) Determine, according to an observer in one of the spaceships, the speed of the other spaceship.
TA [87 marks] This question is about relativistic kinematics. 1a. An observer at rest relative to Earth observes two spaceships. Each spaceship is moving with a speed of 0.85c but[5 marks] in opposite
More informationLecture 21: General Relativity Readings: Section 24-2
Lecture 21: General Relativity Readings: Section 24-2 Key Ideas: Postulates: Gravitational mass=inertial mass (aka Galileo was right) Laws of physics are the same for all observers Consequences: Matter
More informationLecture on: Newton s and Einstein s theories of gravity
University of Sulaimani Faculty of Science and Science Education School of Science Education Physics Department Lecture on: Newton s and Einstein s theories of gravity By Halo Anwar Abdulkhalaq May 2014
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 informationGeneral Relativity Traffic Jam. Noah Graham November 10, 2015
General Relativity Traffic Jam Noah Graham November 10, 2015 1 Newtonian gravity, theoretically Based on action-reaction: The earth exerts a force on an apple, which makes it fall. The heavier the objects
More informationLecture Outline Chapter 29. Physics, 4 th Edition James S. Walker. Copyright 2010 Pearson Education, Inc.
Lecture Outline Chapter 29 Physics, 4 th Edition James S. Walker Chapter 29 Relativity Units of Chapter 29 The Postulates of Special Relativity The Relativity of Time and Time Dilation The Relativity of
More informationElements of Physics II
Physics 132: Lecture 23 Elements of Physics II Agenda for Today Special Theory of relativity Inertial vs. non-inertial reference frames Postulates of SR Consequences of SR Time dilation Length contraction
More information22. Black Holes. Relativistic Length Contraction. Relativistic Time Dilation
22. Black Holes Einstein s Special Theory of Relativity Einstein s General Theory of Relativity Black holes exist in some binary star systems Supermassive black holes at of galaxy centers Two properties
More informationChapter 3 Celestial Sphere Movie
Chapter 3 Celestial Sphere Movie Gravity and Motion Projects I moved due-date for Part 1 to 10/21 I added a descriptive webpage about the projects. Preview Ch 1 Ch 2 Galileo Movie Essay 1: Backyard Astronomy
More informationKepler, 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 informationPhysics. Special Relativity
Physics Special Relativity 1 Albert Einstein, the high school dropout and patent office clerk published his ideas on Special Relativity in 1905. 2 Special vs. General Relativity Special Relativity deals
More informationChapter 13. Gravitation
Chapter 13 Gravitation 13.2 Newton s Law of Gravitation Here m 1 and m 2 are the masses of the particles, r is the distance between them, and G is the gravitational constant. G =6.67 x10 11 Nm 2 /kg 2
More information16 Relativity Momentum, Mass, Energy, and Gravity
According to special relativity, mass and energy are equivalent. According to general relativity, gravity causes space to become curved and time to undergo changes. One of the most celebrated outcomes
More informationMr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path.
Mr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path. In an accelerated frame, time runs slow compared to a non-accelerated frame. The Equivalence Principle tells
More informationCollege Physics B - PHY2054C. Special & General Relativity 11/12/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.
Special College - PHY2054C Special & 11/12/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Outline Special 1 Special 2 3 4 Special Galilean and Light Galilean and electromagnetism do predict
More informationReview Special Relativity. February 3, Absolutes of Relativity. Key Ideas of Special Relativity. Path of Ball in a Moving Train
February 3, 2009 Review Special Relativity General Relativity Key Ideas of Special Relativity No material object can travel faster than light If you observe something moving near light speed: Its time
More informationAstronomy 1 Fall 2016
Astronomy 1 Fall 2016 Lecture 14; November 10, 2016 Previously on Astro 1 Late evolution and death of intermediate-mass stars (about 0.4 M to about 4 M ): red giant when shell hydrogen fusion begins, a
More informationPHSC 1053: Astronomy Relativity
PHSC 1053: Astronomy Relativity Postulates of Special Relativity The speed of light is constant in a vacuum and will be the same for ALL observers, independent of their motion relative to the each other
More informationPhysics General Physics. Lecture 8 Planetary Motion. Fall 2016 Semester Prof. Matthew Jones
Physics 22000 General Physics Lecture 8 Planetary Motion Fall 2016 Semester Prof. Matthew Jones 1 First Midterm Exam Tuesday, October 4 th, 8:00-9:30 pm Location: PHYS 112 and WTHR 200. Covering material
More informationSpecial theory of relativity
Announcements l CAPA #9 due Tuesday April 1 l Mastering Physics Chapter 35 due April 1 l Average on exam #2 is 26/40 l For the sum of the first two exams (80 points); l >=67 4.0 l 61-66 3.5 l 50-60 3.0
More information8. The Expanding Universe, Revisited
8. The Expanding Universe, Revisited A1143: History of the Universe, Autumn 2012 Now that we have learned something about Einstein s theory of gravity, we are ready to revisit what we have learned about
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 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 informationChapter S3 Spacetime and Gravity. Agenda. Distinguishing Crackpots
Chapter S3 Spacetime and Gravity Agenda Announce: Online Quizzes Observations Extra Credit Lecture Distinguishing Crackpot/Genuine Science Review of Special Relativity General Relativity Distinguishing
More informationGeneral Relativity and Cosmology. The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang The End of Absolute Space (AS) Special Relativity (SR) abolished AS only for the special
More informationGravitation. Objectives. The apple and the Moon. Equations 6/2/14. Describe the historical development of the concepts of gravitational force.
Gravitation Objectives Describe the historical development of the concepts of gravitational force. Describe and calculate how the magnitude of the gravitational force between two objects depends on their
More information12:40-2:40 3:00-4:00 PM
Physics 294H l Professor: Joey Huston l email:huston@msu.edu l office: BPS3230 l Homework will be with Mastering Physics (and an average of 1 hand-written problem per week) Help-room hours: 12:40-2:40
More informationNeutron Stars. Properties of Neutron Stars. Formation of Neutron Stars. Chapter 14. Neutron Stars and Black Holes. Topics for Today s Class
Foundations of Astronomy 13e Seeds Phys1403 Introductory Astronomy Instructor: Dr. Goderya Chapter 14 Neutron Stars and Black Holes Cengage Learning 2016 Topics for Today s Class Neutron Stars What is
More informationQuestions Chapter 13 Gravitation
Questions Chapter 13 Gravitation 13-1 Newton's Law of Gravitation 13-2 Gravitation and Principle of Superposition 13-3 Gravitation Near Earth's Surface 13-4 Gravitation Inside Earth 13-5 Gravitational
More informationSpace and Time Before Einstein. The Problem with Light. Admin. 11/2/17. Key Concepts: Lecture 28: Relativity
Admin. 11/2/17 1. Class website http://www.astro.ufl.edu/~jt/teaching/ast1002/ 2. Optional Discussion sections: Tue. ~11.30am (period 5), Bryant 3; Thur. ~12.30pm (end of period 5 and period 6), start
More informationPhysics 12. Unit 5 Circular Motion and Gravitation Part 2
Physics 12 Unit 5 Circular Motion and Gravitation Part 2 1. Newton s law of gravitation We have seen in Physics 11 that the force acting on an object due to gravity is given by a well known formula: F
More informationASTR 200 : Lecture 30. More Gravity: Tides, GR, and Gravitational Waves
ASTR 200 : Lecture 30 More Gravity: Tides, GR, and Gravitational Waves 1 Topic One : Tides Differential tidal forces on the Earth. 2 How do tides work???? Think about 3 billiard balls sitting in space
More informationPHYSICS 12 NAME: Gravitation
NAME: Gravitation 1. The gravitational force of attraction between the Sun and an asteroid travelling in an orbit of radius 4.14x10 11 m is 4.62 x 10 17 N. What is the mass of the asteroid? 2. A certain
More informationWelcome back to Physics 211. Physics 211 Spring 2014 Lecture Gravity
Welcome back to Physics 211 Today s agenda: Newtonian gravity Planetary orbits Gravitational Potential Energy Physics 211 Spring 2014 Lecture 14-1 1 Gravity Before 1687, large amount of data collected
More informationA SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE
DOING PHYSICS WITH MATLAB A SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE Download Directory: Matlab mscripts mec_satellite_gui.m The [2D] motion of a satellite around the Earth is computed from
More informationGravity: What s the big attraction? Dan Wilkins Institute of Astronomy
Gravity: What s the big attraction? Dan Wilkins Institute of Astronomy Overview What is gravity? Newton and Einstein What does gravity do? Extreme gravity The true power of gravity Getting things moving
More informationPHYS 101 Previous Exam Problems. Gravitation
PHYS 101 Previous Exam Problems CHAPTER 13 Gravitation Newton s law of gravitation Shell theorem Variation of g Potential energy & work Escape speed Conservation of energy Kepler s laws - planets Orbits
More informationAstronomy 421. Lecture 24: Black Holes
Astronomy 421 Lecture 24: Black Holes 1 Outline General Relativity Equivalence Principle and its Consequences The Schwarzschild Metric The Kerr Metric for rotating black holes Black holes Black hole candidates
More informationBlack Holes and Curved Space-time. Paths of Light and Matter. The Principle of Equivalence. Implications of Gravity Bending Light
Black Holes and Curved Space-time When a massive star collapses at the end of its life, it can become a black hole A black is an object that is so massive that light cannot escape from it The theory that
More informationThe Early Universe: A Journey into the Past
The Early Universe A Journey into the Past Texas A&M University March 16, 2006 Outline Galileo and falling bodies Galileo Galilei: all bodies fall at the same speed force needed to accelerate a body is
More informationSpecial Relativity: The laws of physics must be the same in all inertial reference frames.
Special Relativity: The laws of physics must be the same in all inertial reference frames. Inertial Reference Frame: One in which an object is observed to have zero acceleration when no forces act on it
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 informationTransformation of velocities
Announcements l Help room hours (1248 BPS) Ian La Valley(TA) Mon 4-6 PM Tues 12-3 PM Wed 6-9 PM Fri 10 AM-noon l LON-CAPA #9 due on Thurs Nov 15 l Third hour exam Thursday Dec 6 l Final Exam Tuesday Dec
More informationThe Early Universe: A Journey into the Past
Gravity: Einstein s General Theory of Relativity The Early Universe A Journey into the Past Texas A&M University March 16, 2006 Outline Gravity: Einstein s General Theory of Relativity Galileo and falling
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 informationGravity and Spacetime: Why do things fall?
Gravity and Spacetime: Why do things fall? A painless introduction to Einstein s theory of space, time and gravity David Blair University of WA Abstract I present a simple description of Einstein s theory
More informationNewton s Legacy. 1- accelerate to break free of Earth. Rocket Science: How to send a spacecraft to Mars
Reading: today: web-based reading on satellite orbits; Chap. 3 Sec. 5 Chap. 7, Sect. 1, 2 (for next week) Exam 1: Tuesday, September 26, 6:45-8:00. Room assignments on course website ESSAY QUESTION Homework
More informationChapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 3 - Gravity and Motion Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. In 1687 Isaac Newton published the Principia in which he set out his concept
More informationPhysics Mechanics Lecture 30 Gravitational Energy
Physics 170 - Mechanics Lecture 30 Gravitational Energy Gravitational Potential Energy Gravitational potential energy of an object of mass m a distance r from the Earth s center: Gravitational Potential
More informationPostulate 2: Light propagates through empty space with a definite speed (c) independent of the speed of the source or of the observer.
Einstein s Special Theory of Relativity 1 m E = mv E =m*c m* = KE =m*c - m c 1- v p=mv p=m*v c 9-1 Postulate 1: The laws of physics have the same form in all inertial reference frames. Postulate : Light
More informationGravitation & Kepler s Laws
Gravitation & Kepler s Laws What causes YOU to be pulled down to the surface of the earth? THE EARTH.or more specifically the EARTH S MASS. Anything that has MASS has a gravitational pull towards it. F
More informationChapter S3 Spacetime and Gravity Pearson Education, Inc.
Chapter S3 Spacetime and Gravity What are the major ideas of general relativity? Spacetime Special relativity showed that space and time are not absolute. Instead, they are inextricably linked in a four-dimensional
More informationCenters of Galaxies. = Black Holes and Quasars
Centers of Galaxies = Black Holes and Quasars Models of Nature: Kepler Newton Einstein (Special Relativity) Einstein (General Relativity) Motions under influence of gravity [23] Kepler The planets move
More informationPhysics 114A Introduction to Mechanics (without calculus)
Physics 114A Introduction to Mechanics (without calculus) A course about learning basic physics concepts and applying them to solve real-world, quantitative, mechanical problems Lecture 34 Einstein s s
More informationLecture 34. General relativity
Lecture 34 The Shape of Space General Relativity Curvature of Space Critical Density Dark Energy Apr 17, 2006 Astro 100 Lecture 34 1 General relativity So far, just needed simple Newton's Gravity. Because
More informationLecture 10: General Relativity I
Lecture 10: General Relativity I! Recap: Special Relativity and the need for a more general theory! The strong equivalence principle! Gravitational time dilation! Curved space-time & Einstein s theory
More informationAdvanced Higher Physics
Wallace Hall Academy Physics Department Advanced Higher Physics Astrophysics Problems Data Common Physical Quantities QUANTITY SYMBOL VALUE Gravitational acceleration g 9.8 m s -2 Radius of Earth R E 6.4
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 informationWhy do we need a new theory?
Lecture 7: General Relativity We now begin our foray into the beautiful, yet sophisticated theory of General Relativity. At first we will explain the need for a new theory and then outline the ideas. We
More informationWelcome back to Physics 215
Welcome back to Physics 215 Today s agenda: More rolling without slipping Newtonian gravity Planetary orbits Gravitational Potential Energy Physics 215 Spring 2018 Lecture 13-1 1 Rolling without slipping
More informationToday in Astronomy 102: Einstein studies gravity
Today in Astronomy 102: Einstein studies gravity The principle of equivalence Gravitational time dilation, specialrelativistic time dilation, and the Doppler effect Curved spacetime and the nature of tides
More informationCircular Motion and Gravity Lecture 5
Circular Motion and Gravity Lecture 5 ˆ Today we talk about circular motion. There are two reasons to do this... ˆ Last week we talked about Newton s laws in problems dealing with straight-line motion.
More informationThe Milky Way. Mass of the Galaxy, Part 2. Mass of the Galaxy, Part 1. Phys1403 Stars and Galaxies Instructor: Dr. Goderya
Foundations Chapter of Astronomy 15 13e Our Milky Way Seeds Phys1403 Stars and Galaxies Instructor: Dr. Goderya Selected Topics in Chapter 15 A view our Milky Way? The Size of our Milky Way The Mass of
More informationTesting Genaral Relativity 05/14/2008. Lecture 16 1
There is a big difference between the Newtonian and the Relativistic frameworks: Newtonian: Rigid flat geometry, universal clocks Gravitational force between objects Magic dependence on mass Relativistic:
More informationSyllabus and Schedule for ASTRO 210 (Black Holes)
Black Holes Syllabus and Schedule for ASTRO 210 (Black Holes) The syllabus and schedule for this class are located at: http://chartasg.people.cofc.edu/chartas/teaching.html Gravity is Universal Gravity
More informationGravity. The Universal Force
Gravity The Universal Force Universal Gravitation What is gravity? Gravity makes things fall Gravity makes bubbles rise Gravity made the earth round, and makes the stars shine, but WHAT IS GRAVITY??? Universal
More informationPY1008 / PY1009 Physics Gravity I
PY1008 / PY1009 Physics Gravity I M.P. Vaughan Learning Objectives The concept of the centre of mass Fundamental forces Newton s Law of Gravitation Coulomb s Law (electrostatic force) Examples of Newton
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 informationSag A Mass.notebook. September 26, ' x 8' visual image of the exact center of the Milky Way
8' x 8' visual image of the exact center of the Milky Way The actual center is blocked by dust and is not visible. At the distance to the center (26,000 ly), this image would span 60 ly. This is the FOV
More informationClass 16. Prof J. Kenney October 31, Relativity
Class 16 Prof J. Kenney October 31, 2016 Relativity Length contraction (moving sticks are shorter) A measuring stick at rest has a length Lo. When it is propelled at velocity v, it has a shorter length
More informationThe interpretation is that gravity bends spacetime and that light follows the curvature of space.
7/8 General Theory of Relativity GR Two Postulates of the General Theory of Relativity: 1. The laws of physics are the same in all frames of reference. 2. The principle of equivalence. Three statements
More informationUnit 5 Gravitation. Newton s Law of Universal Gravitation Kepler s Laws of Planetary Motion
Unit 5 Gravitation Newton s Law of Universal Gravitation Kepler s Laws of Planetary Motion Into to Gravity Phet Simulation Today: Make sure to collect all data. Finished lab due tomorrow!! Universal Law
More informationASTR 200 : Lecture 31. More Gravity: Tides, GR, and Gravitational Waves
ASTR 200 : Lecture 31 More Gravity: Tides, GR, and Gravitational Waves 1 Topic One : Tides Differential tidal forces on the Earth. 2 How do tides work???? Think about 3 billiard balls sitting in space
More informationHow to Measure and Record Light Spectrograph. The Photographic plate now obsolete Turbulence
PHYS 1411 Introduction to Astronomy Light and Telescope Chapter 6 Chapter 6 topics we have covered so far Radiation Information from Space Wave properties, light as a wave and particle, Electromagnetic
More informationWelcome back to Physics 215
Welcome back to Physics 215 Today s agenda: Gravity 15-2 1 Current assignments HW#15 due Monday, 12/12 Final Exam, Thursday, Dec. 15 th, 3-5pm in 104N. Two sheets of handwritten notes and a calculator
More informationChapter 13. Universal Gravitation
Chapter 13 Universal Gravitation Planetary Motion A large amount of data had been collected by 1687. There was no clear understanding of the forces related to these motions. Isaac Newton provided the answer.
More informationSlide 1 / The discovery of Universal Gravitation is associated with: Robert Hook Isaac Newton James Joule Max Plank Christian Huygens
Slide 1 / 22 1 The discovery of Universal Gravitation is associated with: Robert Hook Isaac Newton James Joule Max Plank hristian Huygens Slide 2 / 22 2 Two objects with equal masses of 1 kg each are separated
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 informationNatural Questions. About 2000 years ago Greek scientists were confused about motion. and developed a theory of motion
Natural Questions First natural question: Next question: What these things made of? Why and how things move? About 2000 years ago Greek scientists were confused about motion. Aristotle --- First to study
More information1 A= one Angstrom = 1 10 cm
Our Star : The Sun )Chapter 10) The sun is hot fireball of gas. We observe its outer surface called the photosphere: We determine the temperature of the photosphere by measuring its spectrum: The peak
More informationRelativity. Class 16 Prof J. Kenney June 18, boss
Relativity Class 16 Prof J. Kenney June 18, 2018 boss Length contraction (moving sticks are shorter) A measuring stick at rest has a length Lo. When it is propelled at velocity v, it has a shorter length
More informationChapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter 3 - Gravity and Motion Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display. In 1687 Isaac Newton published the Principia in which he set out his concept
More informationPhysics 120 Quantum Physics and Beyond Today!
Physics 120 Quantum Physics and Beyond Today! General Relativity Accelerated Frames General Relativity Light in General Relativity Motion and Time in General Relativity Back to Quantum Entanglement? More
More informationCircular Motion & Gravitation FR Practice Problems
1) A mass m is attached to a length L of string and hung straight strainght down from a pivot. Small vibrations at the pivot set the mass into circular motion, with the string making an angle θ with the
More information(b) The period T and the angular frequency ω of uniform rotation are related to the cyclic frequency f as. , ω = 2πf =
PHY 302 K. Solutions for problem set #9. Non-textbook problem #1: (a) Rotation frequency of 1 Hz means one revolution per second, or 60 revolutions per minute (RPM). The pre-lp vinyl disks rotated at 78
More informationToday in Astronomy 102: Einstein studies gravity
Today in Astronomy 102: Einstein studies gravity q The principle of equivalence q Gravitational time dilation, specialrelativistic time dilation, and the Doppler effect q Curved spacetime and the nature
More informationLecture PowerPoints. Chapter 6 Physics for Scientists and Engineers, with Modern Physics, 4 th edition Giancoli
Lecture PowerPoints Chapter 6 Physics for Scientists and Engineers, with Modern Physics, 4 th edition Giancoli 2009 Pearson Education, Inc. This work is protected by United States copyright laws and is
More information