Force and Motion a Science A–Z Physical Series Word Count: 1,484

Total Page:16

File Type:pdf, Size:1020Kb

Force and Motion a Science A–Z Physical Series Word Count: 1,484 Force and Motion A Science A–Z Physical Series Word Count: 1,484 Written by Ron Fridell Visit www.sciencea-z.com www.sciencea-z.com KEY ELEMENTS USED IN THIS BOOK Force and The Big Idea: Force and motion are fundamental to all matter in the universe. A force is anything that can push or pull on an object. Forces influence objects that are at rest or that are already in motion. Isaac Newton’s three laws of motion involve inertia, mass, velocity, and Motion momentum. Key forces include gravity, friction, and magnetism. A force is required to do work, and generating a force requires energy. Energy can be stored as potential energy, or it can have kinetic energy—the energy of motion. Energy can also be converted and exchanged through energy transfer. Objects move in predictable ways. By learning about force and motion, we come to understand how using forces can produce motions that allow us to be safe and to enjoy ourselves. Key words: attract, direction, distance, electricity, electromagnetism, energy, energy transfer, engine, force, friction, gravity, heat energy, inertia, kinetic energy, law, lines of force, magnetism, mass, momentum, motion, potential energy, reaction, rest, sound energy, speed, velocity, weight, work Key comprehension skills: Cause and Effect Other suitable comprehension skills: Classify information; compare and contrast; elements of a genre; identify facts; interpret charts, graphs, and diagrams; main idea and details Key reading strategy: Visualize Other suitable reading strategies: Ask and answer questions; connect to prior knowledge; retell; summarize Photo Credits: Front cover: © Corbis; back cover: © James Steidl/Dreamstime.com; title page: © iStockphoto.com/ Latta Pictures; page 3: © iStockphoto.com/Scott Sharick; page 4: © iStockphoto.com/Kristian Sekulic; page 5 (top left): © iStockphoto.com/Kim Gunkel; page 5 (top right): © Pavel Siamionau/123RF; page 5 (bottom): © iStockphoto.com/Joshua Hodge Photography; page 6 (top): courtesy of NASA/ Dennis Sabo; page 6 (bottom): © iStockphoto.com/otisabi; page 7 (top), 22 (top): © Jupiterimages Corporation; page 7 (bottom): © Jean-Leon Huens/National Geographic Society/Corbis; page 8: © iStockphoto.com/Andreas Steinhart; page 9 (top): © iStockphoto.com/Marko Roeper; page 9 (bottom): © iStockphoto.com/Andrey Artykov; page 10 (main): © iStockphoto.com/Vernon Wiley; page 10 (inset): © Pavel Losevsky/123RF; page 11: © iStockphoto.com/Kenneth Sponsler; page 12: © iStockphoto.com/ ranplett; page 13 (top): © iStockphoto.com/Enrique Ramos Lopez; page 13 (bottom): © iStockphoto. com/Claudia Dewald; page 14: © iStockphoto.com/Craig Dingle; page 15: courtesy of NASA; page 16 (top left): © iStockphoto.com/Darren Mower; page 16 (top right): © iStockphoto.com/nullplus; page 16 (bottom): © iStockphoto.com/One Clear Vision; page 17 (top): © iStockphoto.com/Sarah Salmela; page 17 (bottom): © iStockphoto.com/Marzanna Syncerz; page 18: © 3desc/Dreamstime.com; page 19 (top): © iStockphoto.com/Billy Gadbury; page 20: © iStockphoto.com/Stephen Dumayne; page 21 (top): © Learning A–Z; page 22 (bottom left): © Rmarmion/Dreamstime.com; page 22 (bottom right): © iStockphoto.com/Linda Kloosterhof; page 23 (top): © iStockphoto.com/Simon Podgorsek; page 23 (bottom): © Andreas Weiss/Dreamstime.com; page 24: © iStockphoto.com/Iia Dukhnovska Illustration Credit: pages 12, 18, 19: © Learning A–Z; page 21 (bottom): Signe Nordin/© Learning A–Z Written by Ron Fridell Force and Motion © Learning A–Z. Written by Ron Fridell All rights reserved. www.sciencea-z.com www.sciencea-z.com Table of Contents ro ll spinning Introduction ....................................................... 4 i spinning p n spinning s spinning g l Motion Needs a Force ....................................... 5 i spinningri jumping th e ng The Laws of Motion .......................................... 7 Newton’s First Law of Motion ......................... 8 creeping Newton’s Second Law of Motion .................... 10 Introduction Newton’s Third Law of Motion ...................... 12 The words above tell about motion. They Types of Forces ................................................ 13 describe different ways things move. Motion Gravity ........................................................... 13 is all around you. There is even motion inside Friction ........................................................... 16 you. Your blood is moving right now. Magnetism ...................................................... 18 For every motion, there is a force. In this Force, Motion, and Work ................................ 20 book, you will learn about motion and the Energy ............................................................... 21 forces that make things move. Potential and Kinetic Energy ......................... 21 Energy Transfer .............................................. 23 Conclusion ....................................................... 24 Glossary ............................................................ 25 Index ................................................................. 26 3 4 Motion Needs a Force Machines can be a force. A huge engine You need a force to move something. can push a rocket into Lifting, pushing, and pulling are all forces. space. A small electric Where do forces come from? motor can turn the Sometimes the force comes from a blades of a fan or person. When you lift your books, power a toy car. you are the force. If you push a car, Nature is also a you are the force. If you pull a force. Breezes make rope to play tug-of-war, you leaves shake in the are the force. treetops. Ocean waves push make boats bob in the water. Earthquakes lift shake the ground. pull The outer layer of Earth is made of pieces called plates. Earth’s plates move in several ways. The force of these moving plates causes earthquakes. 5 6 The Laws of Motion Scientists have done tests A law is a rule that people must follow. But on motion for hundreds of in science, law has another meaning. A law explains how things in the world always work. years. British scientist Isaac Newton discovered the force we call gravity. You cannot Newton’s First Law of Motion see gravity. But it causes Isaac Newton is known for his three laws things to fall toward the ground. of motion. These laws explain how things move. The first law has two parts. Some people think that Newton discovered gravity when a falling apple hit him on the Part one says that an object at rest will not head. That’s not true. But Newton did notice move unless a force moves it. For example, that things always fell down toward the your bike will stay parked until something ground. He would watch closely and make moves it. notes. That is how he discovered gravity. Part two says that an object will keep SIR ISAAC NEWTON (1642–1727) Isaac Newton lived on a farm in England. Instead of farming, moving in the same he chose to study math and science. He made many way unless a new important discoveries. At age 27, Newton did tests on light. He was the first force changes how person to state that light was it moves. It will keep made up of all moving at the same Why is it important to wear the colors of the a seat belt? Think about rainbow. He is now speed and in the same Newton’s first law of motion. one of the most famous scientists direction. If you pedal of all time! your bike faster or turn, your bike will change speed or direction. If you brake, it will stop. 7 8 Inertia (in-ER-shuh) makes an object keep Newton’s Second Law of Motion doing what it is doing. An object at rest will Newton’s second law of motion has to not move unless a force moves it. An object’s do with mass and speed. Mass is the amount motion will not change unless a force stops of matter, or physical stuff, in an object. For it or changes its speed or direction. Newton’s example, a huge boulder has a lot more mass first law of motion is also called the law than a tiny pebble. of inertia. This law says that an object’s motion depends on how much mass it has and how much force is needed to move it. A boulder has more mass than a small rock, so more force would be needed to move it or to stop it from rolling. An object has inertia when it is at rest or moving. A force is needed to make the object move, stop, or change direction. 9 10 Newton’s Third Law of Motion Newton’s third law of motion says that every force or action has an equal and opposite reaction. So, if you lift a 9 kg (20 lb.) box, the box This train has a large mass and a high speed. This means it has pulls down with an equal a lot of momentum. It would take a very strong force to slow or stop this train! force of 9 kg (20 lbs.). The second law is also about speed. The This law helps you faster an object moves, the more speed it understand why a balloon full has, and the more force is needed to stop it. of air goes flying if you let it go before you tie it. Air rushes out Think about a train speeding down a track. the open end. An opposite force pushes It has a lot of mass and speed. So a strong on the far end. This opposite force makes force is needed to overcome its inertia and the balloon fly. make it stop. The force in a moving object is called B momentum. The more speed and mass an object has, the more momentum it has. A 1. Air rushes out the open end (arrow A). 2. An equal, opposite Velocity is an object’s speed in a certain direction. force pushes on the Scientists measure momentum by multiplying an far end of the balloon object’s mass by its velocity. (arrow B). mass x velocity = momentum 3. The balloon flies around the room! 11 12 Types of Forces Imagine standing next to a tall building. You and the building both have mass. So you You have read about how people, machines, both pull on each other because of gravity.
Recommended publications
  • Glossary Physics (I-Introduction)
    1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay.
    [Show full text]
  • Classical Mechanics
    Classical Mechanics Hyoungsoon Choi Spring, 2014 Contents 1 Introduction4 1.1 Kinematics and Kinetics . .5 1.2 Kinematics: Watching Wallace and Gromit ............6 1.3 Inertia and Inertial Frame . .8 2 Newton's Laws of Motion 10 2.1 The First Law: The Law of Inertia . 10 2.2 The Second Law: The Equation of Motion . 11 2.3 The Third Law: The Law of Action and Reaction . 12 3 Laws of Conservation 14 3.1 Conservation of Momentum . 14 3.2 Conservation of Angular Momentum . 15 3.3 Conservation of Energy . 17 3.3.1 Kinetic energy . 17 3.3.2 Potential energy . 18 3.3.3 Mechanical energy conservation . 19 4 Solving Equation of Motions 20 4.1 Force-Free Motion . 21 4.2 Constant Force Motion . 22 4.2.1 Constant force motion in one dimension . 22 4.2.2 Constant force motion in two dimensions . 23 4.3 Varying Force Motion . 25 4.3.1 Drag force . 25 4.3.2 Harmonic oscillator . 29 5 Lagrangian Mechanics 30 5.1 Configuration Space . 30 5.2 Lagrangian Equations of Motion . 32 5.3 Generalized Coordinates . 34 5.4 Lagrangian Mechanics . 36 5.5 D'Alembert's Principle . 37 5.6 Conjugate Variables . 39 1 CONTENTS 2 6 Hamiltonian Mechanics 40 6.1 Legendre Transformation: From Lagrangian to Hamiltonian . 40 6.2 Hamilton's Equations . 41 6.3 Configuration Space and Phase Space . 43 6.4 Hamiltonian and Energy . 45 7 Central Force Motion 47 7.1 Conservation Laws in Central Force Field . 47 7.2 The Path Equation .
    [Show full text]
  • THE EARTH's GRAVITY OUTLINE the Earth's Gravitational Field
    GEOPHYSICS (08/430/0012) THE EARTH'S GRAVITY OUTLINE The Earth's gravitational field 2 Newton's law of gravitation: Fgrav = GMm=r ; Gravitational field = gravitational acceleration g; gravitational potential, equipotential surfaces. g for a non–rotating spherically symmetric Earth; Effects of rotation and ellipticity – variation with latitude, the reference ellipsoid and International Gravity Formula; Effects of elevation and topography, intervening rock, density inhomogeneities, tides. The geoid: equipotential mean–sea–level surface on which g = IGF value. Gravity surveys Measurement: gravity units, gravimeters, survey procedures; the geoid; satellite altimetry. Gravity corrections – latitude, elevation, Bouguer, terrain, drift; Interpretation of gravity anomalies: regional–residual separation; regional variations and deep (crust, mantle) structure; local variations and shallow density anomalies; Examples of Bouguer gravity anomalies. Isostasy Mechanism: level of compensation; Pratt and Airy models; mountain roots; Isostasy and free–air gravity, examples of isostatic balance and isostatic anomalies. Background reading: Fowler §5.1–5.6; Lowrie §2.2–2.6; Kearey & Vine §2.11. GEOPHYSICS (08/430/0012) THE EARTH'S GRAVITY FIELD Newton's law of gravitation is: ¯ GMm F = r2 11 2 2 1 3 2 where the Gravitational Constant G = 6:673 10− Nm kg− (kg− m s− ). ¢ The field strength of the Earth's gravitational field is defined as the gravitational force acting on unit mass. From Newton's third¯ law of mechanics, F = ma, it follows that gravitational force per unit mass = gravitational acceleration g. g is approximately 9:8m/s2 at the surface of the Earth. A related concept is gravitational potential: the gravitational potential V at a point P is the work done against gravity in ¯ P bringing unit mass from infinity to P.
    [Show full text]
  • Force and Motion
    Force and motion Science teaching unit Disclaimer The Department for Children, Schools and Families wishes to make it clear that the Department and its agents accept no responsibility for the actual content of any materials suggested as information sources in this publication, whether these are in the form of printed publications or on a website. In these materials icons, logos, software products and websites are used for contextual and practical reasons. Their use should not be interpreted as an endorsement of particular companies or their products. The websites referred to in these materials existed at the time of going to print. Please check all website references carefully to see if they have changed and substitute other references where appropriate. Force and motion First published in 2008 Ref: 00094-2008DVD-EN The National Strategies | Secondary 1 Force and motion Contents Force and motion 3 Lift-off activity: Remember forces? 7 Lesson 1: Identifying and representing forces 12 Lesson 2: Representing motion – distance/time/speed 18 Lesson 3: Representing motion – speed and acceleration 27 Lesson 4: Linking force and motion 49 Lesson 5: Investigating motion 66 © Crown copyright 2008 00094-2008DVD-EN The National Strategies | Secondary 3 Force and motion Force and motion Background This teaching sequence bridges from Key Stage 3 to Key Stage 4. It links to the Secondary National Strategy Framework for science yearly learning objectives and provides coverage of parts of the QCA Programme of Study for science. The overall aim of the sequence is for pupils to review and refine their ideas about forces from Key Stage 3, to develop a meaningful understanding of ways of representing motion (graphically and through calculation) and to make the links between different kinds of motion and forces acting.
    [Show full text]
  • Newtonian Mechanics Is Most Straightforward in Its Formulation and Is Based on Newton’S Second Law
    CLASSICAL MECHANICS D. A. Garanin September 30, 2015 1 Introduction Mechanics is part of physics studying motion of material bodies or conditions of their equilibrium. The latter is the subject of statics that is important in engineering. General properties of motion of bodies regardless of the source of motion (in particular, the role of constraints) belong to kinematics. Finally, motion caused by forces or interactions is the subject of dynamics, the biggest and most important part of mechanics. Concerning systems studied, mechanics can be divided into mechanics of material points, mechanics of rigid bodies, mechanics of elastic bodies, and mechanics of fluids: hydro- and aerodynamics. At the core of each of these areas of mechanics is the equation of motion, Newton's second law. Mechanics of material points is described by ordinary differential equations (ODE). One can distinguish between mechanics of one or few bodies and mechanics of many-body systems. Mechanics of rigid bodies is also described by ordinary differential equations, including positions and velocities of their centers and the angles defining their orientation. Mechanics of elastic bodies and fluids (that is, mechanics of continuum) is more compli- cated and described by partial differential equation. In many cases mechanics of continuum is coupled to thermodynamics, especially in aerodynamics. The subject of this course are systems described by ODE, including particles and rigid bodies. There are two limitations on classical mechanics. First, speeds of the objects should be much smaller than the speed of light, v c, otherwise it becomes relativistic mechanics. Second, the bodies should have a sufficiently large mass and/or kinetic energy.
    [Show full text]
  • Physical Science Forces and Motion Vocabulary
    Physical Science -Forces and Motion Vocabulary 1. scientific method - The way we learn and study the world around us through a process of steps. ( Six Giant Hippos Eat Red & Orange Candy) 2. position – the exact location of an object. 3. direction – the line or course along which something moves. 4. speed – measures how fast an object is moving in a given amount of time. 5. motion – the change in position of an object. 6. constant – remaining steady and unchanged (stays the same.) 7. force – push or pull 8. interaction – the action or influence of people, groups or things on one another. 9. exert – to put forth as strength (exert a force) 10. friction - a force that opposes (goes against) motion. Friction is created when two surfaces rub together. Effects of friction: slowing down or stopping an object, producing heat, or wearing away an object. 11. Newton’s 1 st Law of Motion : an object at rest will stay at rest and an object in motion will stay in motion until a force acts upon it. 12. inertia – the tendency for an object to keep doing what it is doing (resting or moving) 13. mass – the amount of matter (“stuff”) - in an object. 14. weight - the amount of force (pull) that gravity has on an object's mass. Your weight depends on the gravitational pull of your location. 15. gravity – a force that attracts (pulls) all objects to the center of the Earth 16. acceleration – the changes in an object’s motion. This can be speeding up, slowing down or changing direction.
    [Show full text]
  • Glossary of Materials Engineering Terminology
    Glossary of Materials Engineering Terminology Adapted from: Callister, W. D.; Rethwisch, D. G. Materials Science and Engineering: An Introduction, 8th ed.; John Wiley & Sons, Inc.: Hoboken, NJ, 2010. McCrum, N. G.; Buckley, C. P.; Bucknall, C. B. Principles of Polymer Engineering, 2nd ed.; Oxford University Press: New York, NY, 1997. Brittle fracture: fracture that occurs by rapid crack formation and propagation through the material, without any appreciable deformation prior to failure. Crazing: a common response of plastics to an applied load, typically involving the formation of an opaque banded region within transparent plastic; at the microscale, the craze region is a collection of nanoscale, stress-induced voids and load-bearing fibrils within the material’s structure; craze regions commonly occur at or near a propagating crack in the material. Ductile fracture: a mode of material failure that is accompanied by extensive permanent deformation of the material. Ductility: a measure of a material’s ability to undergo appreciable permanent deformation before fracture; ductile materials (including many metals and plastics) typically display a greater amount of strain or total elongation before fracture compared to non-ductile materials (such as most ceramics). Elastic modulus: a measure of a material’s stiffness; quantified as a ratio of stress to strain prior to the yield point and reported in units of Pascals (Pa); for a material deformed in tension, this is referred to as a Young’s modulus. Engineering strain: the change in gauge length of a specimen in the direction of the applied load divided by its original gauge length; strain is typically unit-less and frequently reported as a percentage.
    [Show full text]
  • PHYS 419: Classical Mechanics Lecture Notes NEWTON's
    PHYS 419: Classical Mechanics Lecture Notes NEWTON's LAW I. INTRODUCTION Classical mechanics is the most axiomatic branch of physics. It is based on only a very few fundamental concepts (quantities, \primitive" terms) that cannot be de¯ned and virtually just one law, i.e., one statement based on experimental observations. All the subsequent development uses only logical reasoning. Thus, classical mechanics is nowadays sometimes considered to be a part of mathematics and indeed some research in this ¯eld is conducted at departments of mathematics. However, the outcome of the classical mechanics developments are predictions which can be veri¯ed by performing observations and measurements. One spectacular example can be predictions of solar eclipses for virtually any time in the future. Various textbooks introduce di®erent numbers of fundamental concepts. We will use the minimal possible set, just the concepts of space and time. These two are well-known from everyday experience. We live in a three-dimensional space and have a clear perception of passing of time. We can also easily agree on how to measure these quantities. We will denote the position of a point in space by a vector r. If we de¯ne an arbitrary Cartesian coordinate system, this vector can be described by a set of three components: r = [x; y; z] = xx^ + yy^ + zz^ where x^; y^, and z^ are unit vectors along the axes of the coordinate system. If the point is moving in the coordinate system, r = r(t). Thus, each component of r is a single-variable function, e.g., x = x(t).
    [Show full text]
  • UNIT 13: ANGULAR MOMENTUM and TORQUE AS VECTORS Approximate Classroom Time: Two 100 Minute Sessions
    Name ______________________ Date(YY/MM/DD) ______/_________/_______ St.No. __ __ __ __ __-__ __ __ __ Section__________ UNIT 13: ANGULAR MOMENTUM AND TORQUE AS VECTORS Approximate Classroom Time: Two 100 minute sessions Help! Pure logical thinking cannot yield us any knowledge of the empirical world; all knowledge of reality starts from experi- ence and ends in it. -- A. Einstein OBJECTIVES 1. To understand the definitions of torque and angular momentum as vector quantities. 2. To understand the mathematical properties and some applications of the vector cross product. 3. To understand the relationship between torque and an- gular momentum. 4. To understand the Law of Conservation of Angular Mo- mentum. © 1990-93 Dept. of Physics & Astronomy, Dickinson College Supported by FIPSE (U.S. Dept. of Ed.) and NSF. Modified for SFU by N. Alberding, 2005. Page 13-2 Workshop Physics II Activity Guide SFU 1057 OVERVIEW 10 min This unit presents us with a consolidation and extension of the concepts in rotational motion that you studied in the last unit. In the last unit you studied the analogy and re- lationships between rotational and linear quantities (i.e. position and angle, linear velocity and angular velocity, linear acceleration and angular acceleration, and force and torque) without taking into account, in any formal way, the fact that these quantities actually behave like the mathe- matical entities we call vectors. We will discuss the vector nature of rotational quantities and, in addition, define a new vector quantity called angular momentum which is the rotational analogue of linear momentum. Angular momentum and torque are special vectors because they are the product of two other vectors – a position vector and a force or linear momentum vector.
    [Show full text]
  • 2.5. Applications to Physics and Engineering 2.5.1. Work. Work Is
    2.5. APPLICATIONS TO PHYSICS AND ENGINEERING 63 2.5. Applications to Physics and Engineering 2.5.1. Work. Work is the energy produced by a force F pushing a body along a given distance d. If the force is constant, the work done is the product W = F d . · The SI (international) unit of work is the joule (J), which is the work done by a force of one Newton (N) pushing a body along one meter (m). In the American system a unit of work is the foot-pound. Since 1 N = 0.224809 lb and 1 m = 3.28084 ft, we have 1 J = 0.737561 ft lb. More generally, assume that the force is variable and depends on the position. Let F (x) be the force function. Assume that the force pushes a body from a point x = a to another point x = b. In order to find the total work done by the force we divide the interval [a, b] into small subintervals [xi 1, xi] so that the change of F (x) is small along each subinterval. Then− the work done by the force in moving the body from xi 1 to xi is approximately: − ∆W F (x∗) ∆x , i ≈ i where ∆x = xi xi 1 = (b a)/n and xi∗ is any point in [xi 1, xi]. So, the total work is− − − − n n W = ∆W F (x∗) ∆x . i ≈ i i=1 i=1 X X As n the Riemann sum at the right converges to the following integral:→ ∞ b W = F (x) dx .
    [Show full text]
  • PHYSICS 149: Lecture 15
    PHYSICS 149: Lecture 15 • Chapter 6: Conservation of Energy – 6.3 Kinetic Energy – 6.4 Gravitational Potential Energy Lecture 15 Purdue University, Physics 149 1 ILQ 1 Mimas orbits Saturn at a distance D. Enceladus orbits Saturn at a distance 4D. What is the ratio of the periods of their orbits? A) Tm/Te = 1/8 T23∝ r 2 ⎛⎞ 3 B) Tm/Te =1/4= 1/4 Tm ⎛⎞D ⎜⎟= ⎜⎟ ⎝⎠TDE ⎝⎠4 C) Tm/Te = 1/2 ⎛⎞T 11 D) T /T =2= 2 ⎜⎟m = = m e ⎝⎠TE 64 8 Lecture 15 Purdue University, Physics 149 2 ILQ 2 A pendulum bob swings back and forth along a circular path. Does the tension in the string do any work on the bob? Does gravity do work on the bob? A) only tension does work B) both do work C) neither do work D) only gravity does work Lecture 15 Purdue University, Physics 149 3 Energy • Energy is “conserved” meaning it can not be created nor destroyed – Can change form – Can be transferred • Total Energy of an isolated system does not change with time • Forms – Kinetic Energy Motion – Potential Energy Stored – Heat – Mass (E=mc2) • Units: Joules = kg m2 /s/ s2 Lecture 15 Purdue University, Physics 149 4 Definition of “Work” in Physics • Work is a scalar quantity (not a vector quantity). • Units: J (Joule), N⋅m, kg⋅m2/s2, etc. – Unit conversion: 1 J = 1N1 N⋅m = 1kg1 kg⋅m2/s2 • Work is denoted by W (not to be confused by weight W). Lecture 15 Purdue University, Physics 149 5 Total Work • When several forces act on an object, the “total” work is the sum of the work done by each force individually: Lecture 15 Purdue University, Physics 149 6 ILQ 1 You are towing a car up a hill with constant velocity.
    [Show full text]
  • Force, Motion, & Energy
    SOL 4.2 Force, Motion and Energy Moving Objects 1. Did you know that everything in the world can be organized into two categories or groups? These two groups are matter and energy. If something is not matter, it’s energy. Let’s investigate energy! 2. Energy is all around us. We can see it as light, feel it as heat, hear it as sound, and produce it as we do work. Energy can be divided into two groups: kinetic and potential. Kinetic energy is the energy of motion. All moving objects have kinetic energy. When an object is in motion, it changes its position by moving in a direction: up, down, forward, or backward. 3. Potential energy is stored energy. Even when an object is sitting still, it has energy stored inside that can be turned into kinetic energy (motion). An excellent example is a baseball pitcher. Right before a pitcher throws the baseball, he stands very still (stored energy). As he winds up and releases the ball, the stored energy is changed into kinetic energy, the energy of motion! But what caused the ball to move? 4. For an object to move, there must be a force. A force is a push or pull that causes an object to move, change direction, change speed, or stop. Without a force, an object that is moving will continue to move and an object at rest will remain at rest. Some forces are greater than other forces, and the greater the force the greater the motion. We can measure how great or small a motion is by measuring the speed of an object.
    [Show full text]