1 Einstein s Theory of Special Relativity Made Relatively Simple! by Christopher P. Benton, PhD Young Einstein Albert Einstein was born in 1879 and died in He didn't start talking until he was three, and at age nine he still didn't talk very well. Everyone thought he was retarded. However, he got smarter. The Ether In 1820, Thomas Young performed an experiment that indicated that light is composed of waves. However, common sense told the physicists of that day that every wave needs some sort of medium to wave through. For example, ocean waves wave through water, and sound waves wave through air (as well as water and other materials). Thus, physicists believed that light waves also needed some medium to wave through. They called this medium the ether. In 1831 two American scientists, Michelson and Morley, set up an experiment to detect the ether. The idea behind their experiment was that as the earth moves through space it would at times be moving with the ether and at other times against the ether. Suppose the earth were moving against the ether. Then the situation would be analogous to moving upstream in a boat. In that case, anything you threw downstream would move away from you faster than something that you threw upstream. Thus, physicists reasoned that as the earth moved through the ether, the speed at which light moved in one direction would be different from the speed of light in another direction. The experiment of Michelson and Morley was designed to detect this difference in speed, and thus, confirm the existence of the ether. However, when performed, the Michelson- Morley experiment detected no variation in the speed of light. As a result, scientists gradually discarded the idea of the ether (since it couldn't be detected), and they began to accept the idea that the speed of light is the same in all directions. Thus, Einstein began his theory of special relativity with two assumptions: 1. The Principle of Relativity: One cannot tell by any experiment whether one is at rest or moving uniformly (that is, moving in a straight line with constant velocity). In other words, there is no such thing as absolute rest. All motion or rest is only in relation to other observed objects (i.e. I can consider myself not to be moving with respect to the earth while at the same time I am moving very rapidly with respect to the sun). 2. The Constancy of the Speed of Light: The speed of light in a vacuum has the same value c with respect to any observer either at rest or moving uniformly (c = 186, miles per second). What Einstein then discovered was that in order for all observers to measure the same velocity for a beam of light, time would have to "flow" differently for different observers, and space would sometimes have to contract.
2 Experiment 1: Mrs. Einstein is standing in a field and Mr. Einstein is riding on a railroad car that is moving with velocity v. Mr. Einstein shines a flashlight in the direction in which he is moving. Question: What happens? Answer: Because of the principle of the constancy of the velocity of light, each observer will measure the light beam from the flashlight as traveling at the same speed. This may be contrary to what you expected as you might have thought that the observer in the field would have seen the beam moving at (the speed of light) + (the speed of the train). Nevertheless, this is not what is observed in practice. What actually occurs in the real world is that no one ever measures light moving faster or slower than c 186,000 miles per second (in a vacuum).
3 Experiment 2: Mrs. Einstein is standing in a field. Next to her is a light clock. That is, two mirrors that are reflecting a beam of light back and forth, and the journey from one mirror to the other and back again counts as one tick of the clock. Also, Mrs. Einstein is wearing a watch that is synchronized with her light clock. Standing on a railroad car is Mr. Einstein. He also has a light clock, and his clock is synchronized with Mrs. Einstein's and his own wristwatch. The railroad car is not moving. Question: What happens? Answer: Nothing unusual happens. Mr. Einstein's watch and clock stay perfectly synchronized with Mrs. Einstein's.
4 Experiment 3: We now have the same set up except that the railroad car is now moving to the left with a velocity v. Question: What happens? Answer: From Mr. Einstein's perspective, the beam of light keeps going up and down between the mirrors, but from Mrs. Einstein's perspective, the light now has to travel a diagonal path from one mirror to the other. Since Mrs. Einstein still measures the speed of light as c, she is now going to observe Mr. Einstein's light clock as ticking slower than hers since the light now has a longer distance to travel. However, since Mr. Einstein still experiences his watch as being synchronized with his clock, Mrs. Einstein will see his watch slow down along with his clock! Conclusion: If someone moves in a straight line with velocity v with respect to you, then you will observe time passing more slowly for them. With a little algebra we can compute exactly how much time will slow down. Let, L= length or height of the light clocks v = Mr. Einstein's velocity t = time between ticks on Mrs. Einstein's clock t = time between ticks on Mr. Einstein's clock as Mrs. Einstein observes it c = speed of light. We will make frequent use of the formula distance = rate x time. We now compute the distance that the light travels in two ways.
5 On the one hand, the distance traveled is ct (distance = rate x time). But on the other hand, using the Pythagorean Theorem, we have that the distance is 2 = 2 = 2 = =. Hence, ct = which implies that c 2 t 2 = 4L 2 + v 2 t 2, which implies c 2 t 2 - v 2 t 2 = 4L 2, which implies t 2(c 2 - v 2 ) = 4L 2, which implies t 2 = = which implies t = = =. Since t = (2L)/c (i.e. time = distance/rate), this gives us t = Therefore, if t is the time between ticks on Mrs. Einstein's watch, then she will observe a longer interval of t = between ticks on Mr. Einstein's watch! Notice that this difference is not very much unless one is traveling at an extremely fast velocity.
6 Experiment 4: Super Einstein is flying through space with his twin brother, Murray, who is 186,000 miles behind him. Every time he wants to make an acceleration of 10 mph, he uses a flashlight to signal his brother so that they will accelerate together and stay the same distance apart. From Einstein's perspective, he and his brother are 186,000 miles apart, and by letting 1 second pass on his clock before accelerating, he allows the light to reach his brother right at the moment of acceleration. As a result, from Einstein's point of view he and his brother accelerate together and remain a constant 186,000 miles apart. This is what Einstein sees, but if we are standing still with respect to Einstein and his brother, then what will we see? Answer: From our perspective, two things happen. First, we say that the beam of light has less than 186,000 miles to travel since his brother is traveling toward it. Second, we are going to see Einstein's clock as running slow. Thus, for two reasons we are going to see Einstein's brother get the signal to accelerate before a full second has passed on Einstein's clock and he begins his own acceleration. Hence, the distance between Einstein and his brother gets shorter. However, if we stop our analysis at this point, then we are going to wind up with a contradiction, because if Einstein and his brother keep accelerating, and if we keep seeing his brother accelerate first, then eventually distance between them will become so small that Murray will run into Einstein. However, from Einstein's perspective, he and his brother stay a constant 186,000 miles apart! How can we resolve this seeming contradiction? Only by making a very bizarre assumption. In order to keep Murray from running into his brother the shortening of the distance between Einstein and his brother must be compensated for by a contraction of length in a direction parallel to the direction in which Einstein and his brother are moving! In other words, from our point of view, Einstein and his brother are getting shorter so that some distance always remains between them in spite of their accelerations. In the next experiment we will derive a formula that will show us by just how much lengths contract.
7 Experiment 5: Next to Einstein, a light clock lies on its side on a railroad car as the car moves to the left with velocity v. Question: How is the length of the clock affected? Answer: We know that the time between ticks on the moving clock, as we see it, will be Let, t =. t 1 = time it takes the light to go from the first mirror to the second (right to left), as we perceive it. t 2 = time that it takes the light to go from the second mirror back to the first, as we perceive it. L = length of the light clock, as we perceive it. We can analyze the situation as follows: From the above picture we see that the distance the light traveled in time t 1 was L + vt 1. However, this distance is also equal to ct 1 (rate x time). Also, the distance the light traveled on the return trip was L - vt 2 = ct 2. Solving for t 1, we have L + vt 1 = ct 1 which implies that L = ct 1 - vt 1,
8 which implies L = (c - v)t 1, which implies t 1 =. Similarly, L - vt 2 = ct 2 which implies that L = ct 2 + vt 2, which implies L = (c + v)t 2, which implies t 2 =. Thus, t = t 1 + t 2 = = = which implies that =. Since t = (2L)/c, = which implies that =,
9 which implies =, which implies =, which implies L = L. Conclusion: Since is less than 1, this shows that we will measure the length of Einstein s light clock as being less than ours. Thus, when an object is moving in a straight line with a fixed velocity v, we will see its length, as measured in the direction in which it is moving, shorten.
10 Experiment 6: Einstein's wife wants him to jump through hoops, but he wonders if anything strange will happen with regard to lengths that are perpendicular to his direction of motion. Conclusion: Let us suppose that when an object moves that there is a contraction of length in the direction that is perpendicular to its line of motion. Then the diagrams below will show that this assumption leads to a contradiction. By this assumption, if the hoop considers itself as standing still, then Einstein shrinks in the direction perpendicular to his motion and has no trouble going through the hoop. On the other hand, if Einstein considers himself as standing still and the hoop as moving toward him, then by our assumption he would see the hoop contract, and conceivably, he might then be unable to pass through the hoop. This is a contradiction, though, since we can't have Einstein both passing through and not passing through the hoop. The assumption that leads to this contradiction is that lengths perpendicular to our line of motion will contract. An assumption that these lengths would expand leads to a similar contradiction. Thus, we can only conclude that there will be no change at all in lengths that are perpendicular to our line of motion. The only lengths that change are those that are parallel to our line of motion, as we showed in the previous experiment.
11 Experiment 7: Mrs. Einstein is standing in a field and she sees two simultaneous flashes of lightning. Mr. Einstein is on a railroad car moving to the left with velocity v. Question: What will Mr. Einstein see? Answer: Mr. Einstein will see the light flash on the left first since he is moving toward that light and away from the flash on the right. Thus, he will not agree that the flashes of light occurred at the same time. In fact, from his perspective, Mrs. Einstein is the one that is moving, and he will say that it is only because of her movement that she happened to perceive both flashes of light as happening simultaneously.
12 Experiment 8: Mr. Einstein is on a railroad car moving to the left with velocity v, and on his car are two light bulbs that, from his perspective, come on simultaneously. To confirm this, he could also rig some sort of detector that would go off only if both beams of light arrive at his position simultaneously. Question: What will Mrs. Einstein see? Answer: She will agree that both beams of light reach Mr. Einstein at the same time. However, since from her point of view the light on the right has greater distance to travel, she will see the light on the right come on first! Conclusion: From the above experiments we see that events which may be simultaneous for one observer can happen in a different sequence for another observer. This leads us to the startling conclusion that there is no such thing as a universal "now" for which everyone will agree on what happens "now". That is, I can see two events as happening "now" while another observer will see one event happening "now" with the other event yet to occur!
13 Experiment 9: Mr. Einstein drops his wife's favorite potted plant while traveling at a high velocity. It shatters. Meanwhile, his wife is standing in the field watching. Question: What will they each observe? Answer: They both agree that the pot shatters when it hits the surface and that Mr. Einstein is in BIG trouble. However, from Mrs. Einstein's point of view, Mr. Einstein's time slows down and she sees the plant fall in slow motion. This raises the question of why the pot shatters if it seems to gently float to the surface of Mr. Einstein's railroad car. The answer has to do with momentum. Momentum is the amount of "punch" something has. Physicists define momentum as the product of mass and velocity (momentum = mass x velocity). For instance, a car hitting you at 1 mph will do a lot more damage than a feather hitting you at 1 mph because it has more "punch". This extra punch or momentum is a consequence of the car's greater mass. Likewise, if both Mr. and Mrs. Einstein agree that the dropped pot shatters, then this is because the momentum of the pot has remained unchanged. However, since Mrs. Einstein sees the pot falling with less velocity, this also means that its mass must have increased in order for momentum to be conserved. Conclusion: When an object goes fast with respect to us, not only do we see its clocks slow down and its length shorten, we also see an increase in its mass!
14 Conclusions An Obvious Objection Objection: He says my clock slows down and that my distances shrink when I know that it is really his time and space that are changing. Answer: Actually, there is no contradiction to each of us observing the other's clocks and distances changing. There would only be a contradiction if both of us were making our measurements from the same frame of reference and then arrived at different results. However, in order to be in the same frame of reference, one of us would have to alter his motion in order to bring it in line with the other person's. When this happens, extra forces are brought into play and that person is no longer moving with a constant velocity with respect to us. This destroys the symmetry of the situation, and results in one of us definitely having a slower clock. Experimental Verification: Several relativistic effects have been confirmed experimentally. For example, highly accurate atomic clocks have been synchronized with one another and then one has been flown at high speeds in a jet for a sufficient length of time, and when compared with each other again, less time is found to have passed on the clock that was moving at high speeds. It has also been observed that atomic particles decay more slowly when moving at high speeds as predicted by relativity. In addition, many other experiments have been performed over the years that provide ample verification of the predictions of relativity. Final Conclusions: Space and time are stranger than we imagine, and our usual ideas of space and time are just as inaccurate as the belief that people once had that the earth is flat. Much of our confusion results from the assumption that time and space are things that exist independently of objects. However, try to imagine a universe in which no objects exist. In such a universe there would be no points of reference from which to measure the passage of time or distances in space. In such an existence, time and space would only exist as mental constructs. Thus, if we can accept that time is only a measurement that is made of the separation between parts of an observed sequence of events and that distance is only a measurement of the separation between events that are observed to occur at the same time, then it is not so surprising that observers in different frames of reference will measure these things differently. In other words, the universe is relatively... interesting!
15 This work is licensed under a Creative Commons Attribution-NonCommercial- NoDerivs 3.0 Unported License.
Special Theory of Relativity A Brief introduction Classical Physics At the end of the 19th century it looked as if Physics was pretty well wrapped up. Newtonian mechanics and the law of Gravitation had
Chapter One Peculiar Consequences Imagine that you are an astronaut on a trip to the moon. Actually, this is not too hard to imagine. You ve seen pictures of it happening in real life. But your trip is
Correct Resolution of the Twin Paradox Michael Huemer In the following, I explain the Twin Paradox, which is supposed to be a paradoxical consequence of the Special Theory of Relativity (STR). I give the
Chapter S3 Spacetime and Gravity What are the major ideas of special relativity? Spacetime Special relativity showed that space and time are not absolute Instead they are inextricably linked in a four-dimensional
Chapter 5 Perspective in Motion: Galilean Relativity and the Doppler Effect Much can be and has been written about the astronomer, mathematician, and physicist Galileo Galilei (1564-1642). Galileo's was
Einstein s Theory of relativity The theory of relativity has two parts. The Special Theory of Relativity relates the measurements of the same events made by two different observers moving relative to each
Where does E = mc come from? Richard Conn Henry, The Johns Hopkins University, Baltimore MD The location of an event one beat of your heart, say is given by its three space coordinates, and its time coordinate
Part 1 Relativity Chapter 7 Special theory of relativity Historical Background By the beginning of th century experimental observation that Newtonian s mechanics was not able to explain (Michelson's and
General Physics (PHY 2140) Lecture 25 Modern Physics Relativity Time dilation, length contraction http://www.physics.wayne.edu/~apetrov/phy2140/ Chapter 26 1 If you want to know your progress so far, please
The Special Theory of Relativity explained to children (from 7 to 107 years old) Charles-Michel Marle firstname.lastname@example.org Université Pierre et Marie Curie, Paris, France Albert Einstein Century International
The Doppler effect and the twin paradox revisited In section 1, we will introduce the Doppler effect. In section 2, we will introduce its relativistic version. In section 3, we will apply the Doppler effect
Today Example of the use of vectors Announcements: River River HW#3 is due Wed. (tomorrow) at 8 am. Look for two new extra credit problems on CAPA HW#4 will be due next Wednesday as usual Exam # Thurs.
Relativity and Rocketry By Phil Charlesworth In 1905 a little known patent clerk and part-time scientist published three scientific papers that laid the foundations of modern physics. The first paper explained
1 Speed of light is the maximal possible speed We saw that the length of a moving object shrinks. If its length at rest was l 0, then when it is moving with velocity v its length becomes l = l 0 But what
Albert Einstein and the Miracle Year Special Relativity The year 1905 is often referred to as the Annus Mirabilis (or year of miracles). In this year, Albert Einstein, a 23-year old with an undergraduate
Unit 1 Cycle 2 Beginnings: Is it moving? Purpose So far in this Unit, you have looked at different ways to describe the position of an object that is not moving. However, many objects do not stay in one
LASER INTERFEROMETER GRAVITATIONAL WAVE OBSERVATORY LIGO CALIFORNIA INSTITUTE OF TECHNOLOGY MASSACHUSETTS INSTITUTE OF TECHNOLOGY Educational Activity LIGO-T080159-v1-G 6 November 2008 What Time is It?
1 of 8 2/29/2016 11:17 PM Signed in as Weida Wu, Instructor Help Sign Out Rutgers Analytical Physics 750:228, Spring 2016 ( RUPHY228S16 ) My Courses Course Settings University Physics with Modern Physics,
CHAPTER 3 ACTIVITY 1: Gravitational Force and Acceleration LEARNING TARGET: You will determine the relationship between mass, acceleration, and gravitational force. PURPOSE: So far in the course, you ve
Physics 10 Midterm 1 1. What property of waves, did the project Mogul rely on? A. interference B. beats C. bending on slow side D. dispersion E. None of the above Mogul project use the sound channel, look
The Theory of Relativity 1. THE SPECIAL THEORY In 1905, his annum mirabilis, Einstein revolutionized physics with, among other things, his special theory of relativity. With it he completely overturned
Names Date OBJECTIVES WEEK 2: INTRODUCTION TO MOTION To discover how to use a motion detector. To explore how various motions are represented on a distance (position) time graph. To explore how various
PH300 Modern Physics SP11 Each ray of light moes in the coordinate system 'at rest' with the definite, constant elocity c, independent of whether this ray of light is emitted by a body at rest or a body
Lecture 23 Einstein on the Relativity of Length and Time Patrick Maher Scientific Thought II Spring 2010 Review Clocks at A and B are synchronous if, when a ray of light is sent from A to B and reflected
Team: Newton s Third Law, Momentum, Center of Mass Part I. Newton s Third Law Atomic Springs When you push against a wall, you feel a force in the opposite direction. The harder you push, the harder the
1 Deformation of the Bodies by the Result of Length Contraction: A new Approach to the Lorentz Contraction Bayram Akarsu, Ph.D Erciyes University Kayseri/ Turkiye 2 Abstract It has been more than a century
Team: Newton s Third Law, Momentum, Center of Mass Newton s Third Law is a deep statement on the symmetry of interaction between any two bodies in the universe. How is the pull of the earth on the moon
Some Special Relativity Formulas 1 Introduction The purpose of this handout is simple: to give you power in using special relativity! Even though you may not, at this stage, understand exactly where all
Chapter 2 Position, Velocity, and Acceleration In this section, we will define the first set of quantities (position, velocity, and acceleration) that will form a foundation for most of what we do in this
306 MATHEMATICS APPENDIX 2 INTRODUCTION TO MATHEMATICAL MODELLING A2.1 Introduction Right from your earlier classes, you have been solving problems related to the real-world around you. For example, you
Activity 5 A Moving Frame of Reference GOALS In this activity you will: Observe the motion of a ball from a stationary position and while moving at a constant velocity. Observe the motion of a ball from
Ask a dozen people to name a genius and the odds are that 'Einstein' will spring to their lips. Ask them the meaning of 'relativity' and few of them will be able to tell you what it is. The ABC of Relativity
Have you heard the story about Isaac Newton and the apple? Newton was a scientist who lived about 300 years ago. He made many important discoveries about how and why things move. The apple story goes like
GENERAL RELATIVITY - Einstein 1915 Starting problem: Special Relativity only applies to inertial reference frames, where no forces are involved. How to describe gravity then? [Note: some material in these
Team: Newton s Third Law, Momentum, Center of Mass Newton s Third Law is a deep statement on the symmetry of interaction between any two bodies in the universe. How is the pull of the earth on the moon
Kinematics: The Gravity Lab Teacher Advanced Version (Grade Level: 8 12) *** Experiment with Audacity and Excel to be sure you know how to do what s needed for the lab*** Kinematics is the study of how
The speed of things is always changing. Your car speeds up and slows down. If you slow down gradually, it feels very different from slamming on the brakes and stopping fast. In this section we will learn
Lecture 2 Displacement Speed Average velocity Instantaneous velocity Gravity and acceleration Cutnell+Johnson: chapter 2 Most physics classes start by studying the laws describing how things move around.
Level 3 Physics: Demonstrate understanding of Waves Doppler Effect and Beats - Answers In 03, AS 953 replaced AS 9050. The Mess that is NCEA Assessment Schedules. In AS 9050 there was an Evidence column
Toronto, Canada December 29, 2013 Second Edition 2013, Revision 2.1 The Neo-classical Theory of Relativity by Valentin T. Danci Introduction to the Neo-classical Theory of Relativity... 3 1. The conceptual
55 Name Date Partners LAB 6: GRAVITATIONAL AND PASSIVE FORCES And thus Nature will be very conformable to herself and very simple, performing all the great Motions of the heavenly Bodies by the attraction
Physics 605 Mechanical Energy (Read objectives on screen.) No, I haven t been playing with this toy the whole time you ve been gone, but it is kind of hypnotizing, isn t it? So where were we? Oh yes, we
Physics 1103 Wave Interactions (picture of beach on screen) Today, we go back to the beach to investigate more wave interactions. For example, what makes these waves change direction as they approach the
Harmonic Motion: The Pendulum Lab Student Version In this lab you will set up a pendulum using rulers, string, and small weights and measure how different variables affect the period of the pendulum. You
3637_CassidyTX_09 6/14/02 12:08 PM Page 405 C H A P T E R9 Einstein and Relativity Theory 9.1 The New Physics 9.2 Albert Einstein 9.3 The Relativity Principle 9.4 Constancy of the Speed of Light 9.5 Simultaneous
Special Relativity and Electromagnetism Yannis PAPAPHILIPPOU CERN United States Particle Accelerator School, University of California - Santa Cruz, Santa Rosa, CA 14 th 18 th January 2008 1 Outline Notions
First 100 Instant Words the had out than of by many first and words then water a but them been to not these called in what so who is all some oil you were her sit that we would now it when make find he
Chapter 27 Solutions PSS 27.2 The Electric Field of a Continuous Distribution of Charge Description: Knight Problem-Solving Strategy 27.2 The Electric Field of a Continuous Distribution of Charge is illustrated.
STEM Fuse GAME:IT Unit 2 Key formulas for math & physics calculations used in game development Definition of velocity Velocity is similar to speed but it has direction. Let's recap what a speed is. Speed
CT16-1 Which of the following is necessary to make an object oscillate? i. a stable equilibrium ii. little or no friction iii. a disturbance A: i only B: ii only C: iii only D: i and iii E: All three Answer:
Version 00 Relativity tubman (23) This print-out should have 36 questions. Multiple-choice questions may continue on the next column or page find all choices before answering. AP B 993 MC 40 00 0.0 points
Physics of Rocket Flight In order to understand the behaviour of rockets it is necessary to have a basic grounding in physics, in particular some of the principles of statics and dynamics. This section
CD Our Own Way Lyrics Beverly Granoff 2012 1. All The Things We See 2. Remember the Rules 3. You and Me 4. This Too Shall Pass 5. My Best Try 6. Our Own Way 7. A Little Help From You 8. My La La Melody
Physics for Scientists and Engineers with Modern Physics, Chapters 39 46, Seventh Edition Raymond A. Serway and John W. Jewett, Jr. Physics Acquisition Editor: Chris Hall Publisher: David Harris Vice President,
Introduction to Special Relativity Dr. Bob Gardner Great Ideas in Science (PHYS 2018) Notes based on Differential Geometry and Relativity Theory: An Introduction by Richard Faber 1 Chapter 2. Special Relativity:
Introduction Understanding Relativity or How to do Effective Thought Experiments Ian M. Sefton School of Physics, The University of Sydney I.Sefton@physics.usyd.edu.au After some years absence, the topic
Worksheet Math 124 Week 1 Worksheet for Week 1: Circles and lines This worksheet is a review of circles and lines, and will give you some practice with algebra and with graphing. Also, this worksheet introduces
Lecture 7: The Doppler Effect The doppler effect is the phenomenon we have all noticed, that a sound produced by a moving source, or which you hear while you are moving, has its perceived frequency shifted
Time and Causation in Gödel s Universe. John L. Bell In 1949 the great logician Kurt Gödel constructed the first mathematical models of the universe in which travel into the past is, in theory at least,
National 4/5 Physics Dynamics and Space Summary Notes The coloured boxes contain National 5 material. Section 1 Mechanics Average Speed Average speed is the distance travelled per unit time. distance (m)
Light Waves Test Question Bank Standard/Advanced Name: Question 1 (1 point) The electromagnetic waves with the highest frequencies are called A. radio waves. B. gamma rays. C. X-rays. D. visible light.
15. Galileo and Aristotle on Motion. I. Aristotle's Theory of Motion Two basic principles: I. No motion without a mover in contact with moving body. II. Distinction between: (a) Natural motion: mover is
Work and Energy Ch. 6 Work = Force Distance Work increases the energy of an object. Energy can be converted back to work. Therefore, energy and work have the same unit: Newton meter = Nm Energy per gram,
Lecture 7: Light Waves Isaac Newton (1643-1727) was born in the year Galileo died He discovered the Law of Gravitation in 1665 He developed the Laws of Mechanics that govern all motions In order to solve
STE Physics Intro Name 1. Mass, Force and Gravity Before attempting to understand force, we need to look at mass and acceleration. a) What does mass measure? The quantity of matter(atoms) b) What is the
Fry Instant Words High Frequency Words The Fry list of 600 words are the most frequently used words for reading and writing. The words are listed in rank order. First Hundred Group 1 Group 2 Group 3 Group
Mechanics Lecture Notes Notes for lectures 2 and 3: Motion in a circle. Introduction The important result in this lecture concerns the force required to keep a particle moving on a circular path: if the
5 Question 1. [Marks 20] An unmarked police car P is, travelling at the legal speed limit, v P, on a straight section of highway. At time t = 0, the police car is overtaken by a car C, which is speeding
LAB 9b NONINERTIAL FRAMES EXPERIMENTAL QUESTION In this lab, you will explore the distinction between inertial and non-inertial reference frames. According to chapter N9, Newton s second law fails to hold
TEACHER BACKGROUND INFORMATION THERMAL ENERGY In general, when an object performs work on another object, it does not transfer all of its energy to that object. Some of the energy is lost as heat due to
Chapter 3 Falling Objects and Projectile Motion Gravity influences motion in a particular way. How does a dropped object behave?!does the object accelerate, or is the speed constant?!do two objects behave
Chapter 14 Understand how Forces act on Structures 14.1 Introduction The analysis of structures considered here will be based on a number of fundamental concepts which follow from simple Newtonian mechanics;
Rocket Principles Outside ir Pressure Inside ir Pressure ir Moves Balloon Moves rocket in its simplest form is a chamber enclosing a gas under pressure. small opening at one end of the chamber allows the
Weekly Focus: Reading for Comprehension Weekly Skill: Numeracy Skills in Science Lesson Summary: This week students will continue reading for comprehension with reading passages on speed, velocity, and
October 19, 2015 Unification of the laws of the Earth and the Universe Why do planets appear to wander slowly across the sky? Key Words Newton s Laws of motion, and Newton s law of universal gravitation:
Modern Physics (PHY 3305) Lecture Notes Modern Physics (PHY 3305) Lecture Notes Relativistic Paradoxes and Kinematics (Ch..4-.5) SteveSekula, 6 January 00 (created 3 December 009) CHAPTER.4-.6 Review of
lecture 20 Topics: Precession of tops Nutation Vectors in the body frame The free symmetric top in the body frame Euler s equations The free symmetric top ala Euler s The tennis racket theorem As you know,
Harmonic Motion: The Pendulum Lab Teacher Version In this lab you will set up a pendulum using rulers, string, and small weights and measure how different variables affect the period of the pendulum. You
80 Newton s Laws of Motion R EA D I N G Isaac Newton was a British scientist whose accomplishments included important discoveries about light, motion, and gravity. You may have heard the legend about how
Reading 1.2 Newton s Cradle Getting Ready Have you ever played pool? The game begins with a breaking shot in which a player scatters several balls that are grouped together by shooting one ball into them.
You can describe the motion of an object by its position, speed, direction, and acceleration. 4.1 Motion Is Relative An object is moving if its position relative to a fixed point is changing. 4.1 Motion
What is Energy? What is the relationship between energy and work? Compare kinetic and potential energy What are the different types of energy? What is energy? Energy is the ability to do work. Great, but
4.1 Motion Is Relative You can describe the motion of an object by its position, speed, direction, and acceleration. An object is moving if its position relative to a fixed point is changing. 4.1 Motion