Basic Physics. Remaining Topics. Gravitational Potential Energy. PHYS 1403 Introduction to Astronomy. Can We Create Artificial Gravity?

Similar documents
Basic Physics. What We Covered Last Class. Remaining Topics. Center of Gravity and Mass. Sun Earth System. PHYS 1411 Introduction to Astronomy

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

Basic Physics. Isaac Newton ( ) Topics. Newton s Laws of Motion (2) Newton s Laws of Motion (1) PHYS 1411 Introduction to Astronomy

Astronomy 1141 Life in the Universe 10/24/12

Lecture 23 (Gravitation, Potential Energy and Gauss s Law; Kepler s Laws) Physics Spring 2017 Douglas Fields

A = 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.

Relativity. Astronomy 101

Outline. General Relativity. Black Holes as a consequence of GR. Gravitational redshift/blueshift and time dilation Curvature Gravitational Lensing

7 Study Guide. Gravitation Vocabulary Review

Chapter 26. Relativity

Gravity. Announcement. Topics in Chapter 5. Topics for Today. PHYS 1403 Introduction to Astronomy. Motion. Chapter 5. Exam 1

Lecture 18 Vacuum, General Relativity

(ii) Determine, according to an observer in one of the spaceships, the speed of the other spaceship.

Lecture 21: General Relativity Readings: Section 24-2

Lecture on: Newton s and Einstein s theories of gravity

CIRCULAR MOTION AND UNIVERSAL GRAVITATION

General Relativity Traffic Jam. Noah Graham November 10, 2015

Lecture Outline Chapter 29. Physics, 4 th Edition James S. Walker. Copyright 2010 Pearson Education, Inc.

Elements of Physics II

22. Black Holes. Relativistic Length Contraction. Relativistic Time Dilation

Chapter 3 Celestial Sphere Movie

Kepler, Newton, and laws of motion

Physics. Special Relativity

Chapter 13. Gravitation

16 Relativity Momentum, Mass, Energy, and Gravity

Mr Green sees the shorter, straight, green path and Mr. Red sees the longer, curved, red path.

College Physics B - PHY2054C. Special & General Relativity 11/12/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.

Review Special Relativity. February 3, Absolutes of Relativity. Key Ideas of Special Relativity. Path of Ball in a Moving Train

Astronomy 1 Fall 2016

PHSC 1053: Astronomy Relativity

Physics General Physics. Lecture 8 Planetary Motion. Fall 2016 Semester Prof. Matthew Jones

Special theory of relativity

8. The Expanding Universe, Revisited

Name: Earth 110 Exploration of the Solar System Assignment 1: Celestial Motions and Forces Due on Tuesday, Jan. 19, 2016

More examples: Summary of previous lecture

Chapter S3 Spacetime and Gravity. Agenda. Distinguishing Crackpots

General Relativity and Cosmology. The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang

Gravitation. Objectives. The apple and the Moon. Equations 6/2/14. Describe the historical development of the concepts of gravitational force.

12:40-2:40 3:00-4:00 PM

Neutron Stars. Properties of Neutron Stars. Formation of Neutron Stars. Chapter 14. Neutron Stars and Black Holes. Topics for Today s Class

Questions Chapter 13 Gravitation

Space and Time Before Einstein. The Problem with Light. Admin. 11/2/17. Key Concepts: Lecture 28: Relativity

Physics 12. Unit 5 Circular Motion and Gravitation Part 2

ASTR 200 : Lecture 30. More Gravity: Tides, GR, and Gravitational Waves

PHYSICS 12 NAME: Gravitation

Welcome back to Physics 211. Physics 211 Spring 2014 Lecture Gravity

A SIMULATION OF THE MOTION OF AN EARTH BOUND SATELLITE

Gravity: What s the big attraction? Dan Wilkins Institute of Astronomy

PHYS 101 Previous Exam Problems. Gravitation

Astronomy 421. Lecture 24: Black Holes

Black Holes and Curved Space-time. Paths of Light and Matter. The Principle of Equivalence. Implications of Gravity Bending Light

The Early Universe: A Journey into the Past

Special Relativity: The laws of physics must be the same in all inertial reference frames.

4.3 Conservation Laws in Astronomy

Transformation of velocities

The Early Universe: A Journey into the Past

Gravity. Newton s Law of Gravitation Kepler s Laws of Planetary Motion Gravitational Fields

Gravity and Spacetime: Why do things fall?

Newton s Legacy. 1- accelerate to break free of Earth. Rocket Science: How to send a spacecraft to Mars

Chapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Physics Mechanics Lecture 30 Gravitational Energy

Postulate 2: Light propagates through empty space with a definite speed (c) independent of the speed of the source or of the observer.

Gravitation & Kepler s Laws

Chapter S3 Spacetime and Gravity Pearson Education, Inc.

Centers of Galaxies. = Black Holes and Quasars

Physics 114A Introduction to Mechanics (without calculus)

Lecture 34. General relativity

Lecture 10: General Relativity I

Advanced Higher Physics

Copyright 2010 Pearson Education, Inc. GRAVITY. Chapter 12

Chapter 12 Gravity. Copyright 2010 Pearson Education, Inc.

Why do we need a new theory?

Welcome back to Physics 215

Today in Astronomy 102: Einstein studies gravity

Circular Motion and Gravity Lecture 5

The Milky Way. Mass of the Galaxy, Part 2. Mass of the Galaxy, Part 1. Phys1403 Stars and Galaxies Instructor: Dr. Goderya

Testing Genaral Relativity 05/14/2008. Lecture 16 1

Syllabus and Schedule for ASTRO 210 (Black Holes)

Gravity. The Universal Force

PY1008 / PY1009 Physics Gravity I

Gravity and the Orbits of Planets

Sag A Mass.notebook. September 26, ' x 8' visual image of the exact center of the Milky Way

Class 16. Prof J. Kenney October 31, Relativity

The interpretation is that gravity bends spacetime and that light follows the curvature of space.

Unit 5 Gravitation. Newton s Law of Universal Gravitation Kepler s Laws of Planetary Motion

ASTR 200 : Lecture 31. More Gravity: Tides, GR, and Gravitational Waves

How to Measure and Record Light Spectrograph. The Photographic plate now obsolete Turbulence

Welcome back to Physics 215

Chapter 13. Universal Gravitation

Slide 1 / The discovery of Universal Gravitation is associated with: Robert Hook Isaac Newton James Joule Max Plank Christian Huygens

Gravity and Orbits. Objectives. Clarify a number of basic concepts. Gravity

Natural Questions. About 2000 years ago Greek scientists were confused about motion. and developed a theory of motion

1 A= one Angstrom = 1 10 cm

Relativity. Class 16 Prof J. Kenney June 18, boss

Chapter 3 - Gravity and Motion. Copyright (c) The McGraw-Hill Companies, Inc. Permission required for reproduction or display.

Physics 120 Quantum Physics and Beyond Today!

Circular Motion & Gravitation FR Practice Problems

(b) The period T and the angular frequency ω of uniform rotation are related to the cyclic frequency f as. , ω = 2πf =

Today in Astronomy 102: Einstein studies gravity

Lecture PowerPoints. Chapter 6 Physics for Scientists and Engineers, with Modern Physics, 4 th edition Giancoli

Transcription:

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? 1 2 2 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

Concept What is Gravity Assist? https://www.youtube.com/watch?v=jkgrvl69mma https://www.youtube.com/watch?v=2r9smrho-oc Image source: NASA, STSI Source: wikipedia How to increase velocity of a spacecraft without using fuel? Source: wikipedia Gravity Assist https://www.youtube.com/watch?v=0iagrditiie 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

Einstein and Relativity Einstein (1879 1955) 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

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 42.98 0.04 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

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