Physics 111 Lecture 6 Work-Energy -Power Dr.Ali ÖVGÜN

Similar documents
Physics 101 Lecture 7 Kinetic Energy and Work

Physics 231 Lecture 9

Energy present in a variety of forms. Energy can be transformed form one form to another Energy is conserved (isolated system) ENERGY

Mechanics and Heat. Chapter 5: Work and Energy. Dr. Rashid Hamdan

PHYSICS 231 INTRODUCTORY PHYSICS I

Physics 231 Lecture 12

Chapter 5: Energy. Energy is one of the most important concepts in the world of science. Common forms of Energy

Chapter 6 Work, Energy, and Power. Copyright 2010 Pearson Education, Inc.

Physics 111. Lecture 15 (Walker: 7.1-2) Work & Energy March 2, Wednesday - Midterm 1

Ground Rules. PC1221 Fundamentals of Physics I. Introduction to Energy. Energy Approach to Problems. Lectures 13 and 14. Energy and Energy Transfer

Chapter 07: Kinetic Energy and Work

Chapter 4. Energy. Work Power Kinetic Energy Potential Energy Conservation of Energy. W = Fs Work = (force)(distance)

Physics 2010 Work and Energy Recitation Activity 5 (Week 9)

25/01/2014. Chapter 4: Work, Energy and Power. Work of a force. Chapter 4: Work, Energy and Power (First part) Work = Force x Displacement

Chapter 6. Work and Kinetic Energy. Richard Feynman Nobel Prize in physics (1965)

Physics 101 Lecture 12 Equilibrium and Angular Momentum

Chapter 6. Work and Energy

Chapter 7 Work and Kinetic Energy. Copyright 2010 Pearson Education, Inc.

Which iceboat crosses the finish line with more kinetic energy (KE)?

Ground Rules. PC1221 Fundamentals of Physics I. Lectures 13 and 14. Energy and Energy Transfer. Dr Tay Seng Chuan

Ground Rules. PC1221 Fundamentals of Physics I. Introduction to Energy. Energy Approach to Problems. Lectures 13 and 14. Energy and Energy Transfer

One-Dimensional Motion Review IMPORTANT QUANTITIES Name Symbol Units Basic Equation Name Symbol Units Basic Equation Time t Seconds Velocity v m/s

Fs (30.0 N)(50.0 m) The magnitude of the force that the shopper exerts is f 48.0 N cos 29.0 cos 29.0 b. The work done by the pushing force F is

Lecture 3. > Potential Energy. > Conservation of Energy. > Power. (Source: Serway; Giancoli) Villacorta--DLSUM-SCIENVP-L Term01

Today: Work, Kinetic Energy, Potential Energy. No Recitation Quiz this week

Power: Sources of Energy

Chapter 5 Work and Energy

( ) = ( ) W net = ΔKE = KE f KE i W F. F d x. KE = 1 2 mv2. Note: Work is the dot product of F and d. Work-Kinetic Energy Theorem

There are two types of forces: conservative (gravity, spring force) nonconservative (friction)

Chapter 5 Gravitation Chapter 6 Work and Energy

Conservation of Energy and Momentum

Physics 101 Lecture 5 Newton`s Laws

Chapter 5. Work and Energy. continued

Physics 111 Lecture 4 Newton`s Laws

Lecture 9. > Potential Energy. > Conservation of Energy. > Power. (Source: Serway; Giancoli) Villacorta--DLSUM-BIOPHY1-L Term01

The Electric Potential Energy

Lecture 7 Chapter 7 Work Energy Potential Energy Kinetic Energy

Physics Unit 4:Work & Energy Name:

CHAPTER 4 NEWTON S LAWS OF MOTION

Units are important anyway

Forces of Friction Contact between bodies with a relative velocity produces friction opposite

The Electric. Potential Energy

Physics 111. Lecture 18 (Walker: 8.3-4) Energy Conservation I March 11, Conservation of Mechanical Energy

Review D: Potential Energy and the Conservation of Mechanical Energy

Work Up an Incline. Work = Force x Distance. Push up: 1500J. What is the PE at the top? mg = 500N. An incline is a simple machine!

Chapter 6 Energy and Oscillations

Lecture 10 Mechanical Energy Conservation; Power

PHYSICS 149: Lecture 17

Physics 1A Lecture 6B. "If the only tool you have is a hammer, every problem looks like a nail. --Abraham Maslow

Kinetic Energy and Work

Work Done by a Constant Force

ENERGY. Conservative Forces Non-Conservative Forces Conservation of Mechanical Energy Power

PHYSICS - CLUTCH CH 07: WORK & ENERGY.

. According to the workenergy theorem (Equation 6.3), the work done by the net external force W catapult

Be on time Switch off mobile phones. Put away laptops. Being present = Participating actively

Lecture III. Introduction to Mechanics, Heat, and Sound /FIC 318

Conservation of Mechanical Energy 8.01

Physics 101 Lecture 10 Rotation

Chapter 8. Conservation of Energy

Tutorial 1 Calculating the Kinetic Energy of a Moving Object

Other Examples of Energy Transfer

Lectures Chapter 6 (Cutnell & Johnson, Physics 7 th edition)

Work and Energy continued

Lecture 7: More on Newton s Laws

Chapter 4. Forces and Newton s Laws of Motion. continued

Chapter 5. Work and Energy. continued

Physics 10 Lecture 7A. "Energy and persistence conquer all things. --Benjamin Franklin

The Laws of Motion. Newton s first law Force Mass Newton s second law Gravitational Force Newton s third law Examples

PHYSICS 231 INTRODUCTORY PHYSICS I

Physics 1A Lecture 4B. "Fig Newton: The force required to accelerate a fig inches per second. --J. Hart

Chapter 4. Dynamics: Newton s Laws of Motion. That is, describing why objects move

Isaac Newton ( ) 1687 Published Principia Invented Calculus 3 Laws of Motion Universal Law of Gravity

Chapter 4. The Laws of Motion. Dr. Armen Kocharian

Lecture PowerPoints. Chapter 6 Physics: Principles with Applications, 7 th edition Giancoli

Lecture 7. Forces. Important note: First Exam is next Tuesday, Feb. 6, 8:15-9:45 pm (see link on Canvas for locations)

WORK, POWER & ENERGY

13.7 Power Applied by a Constant Force

Newton s First Law and IRFs

Physics 121. Tuesday, February 19, Physics 121. Tuesday, February 19, Physics 121. Course announcements. Topics:

Chapter 7 Kinetic Energy and Work

AP PHYSICS 1. Energy 2016 EDITION

Physics 11 HW #6 Solutions

PHY 101. Work and Kinetic Energy 7.1 Work Done by a Constant Force

Recall: Gravitational Potential Energy

Physics 1401V October 28, 2016 Prof. James Kakalios Quiz No. 2

Chapter 4 FORCES AND NEWTON S LAWS OF MOTION PREVIEW QUICK REFERENCE. Important Terms

Pre-AP Physics Chapter 1 Notes Yockers JHS 2008

Chapter 6 Work and Energy

Section 1 Changes in Motion. Chapter 4. Preview. Objectives Force Force Diagrams

Physics 111. Applying Newton s Laws. Lecture 9 (Walker: 5.4-5) Newton s Third Law Free Body Diagram Solving 2-D Force Problems Weight & Gravity

Solutions to Physics: Principles with Applications, 5/E, Giancoli Chapter 6

Chapter 07: Kinetic Energy and Work

Chapter 3: Force, Work and Energy

XI PHYSICS. M. Affan Khan LECTURER PHYSICS, AKHSS, K.

6.0 Energy Conservation. 6.1 Work

Chapter 4. Table of Contents. Section 1 Changes in Motion. Section 2 Newton's First Law. Section 3 Newton's Second and Third Laws

Sometimes (like on AP test) you will see the equation like this:

Worksheet for Exploration 6.1: An Operational Definition of Work

The relationship between force and distance has a name. WORK

Chapters 5-6. Dynamics: Forces and Newton s Laws of Motion. Applications

Transcription:

Physics 111 Lecture 6 Work-Energy -Power Dr.Ali ÖVGÜN EMU Physics Department www.aovgun.com

Why Energy? q Why do we need a concept o energy? q The energy approach to describing motion is particularly useul when Newton s Laws are diicult or impossible to use. q Energy is a scalar quantity. It does not have a direction associated with it. October 7-13, 013

Kinetic Energy q Kinetic Energy is energy associated with the state o motion o an object q For an object moving with a speed o v K = 1 mv q SI unit: joule (J) 1 joule = 1 J = 1 kg m /s October 7-13, 013

Kinetic Energy or Various Objects KE = 1 mv October 7-13, 013

K = 1 mv Why? October 7-13, 013

Work W q Start with 1 mv 1 mv 0 = FxΔx Work W q Work provides a link between orce and energy q Work done on an object is transerred to/rom it q I W > 0, energy added: transerred to the object q I W < 0, energy taken away: transerred rom the object October 7-13, 013

Deinition o Work W q The work, W, done by a constant orce on an object is deined as the product o the component o the orce along the direction o displacement and the magnitude o the displacement W ( F cosθ )Δ x n F is the magnitude o the orce n Δ x is the magnitude o the object s displacement n θ is the angle between =!! F Δ x!! F and Δx October 7-13, 013

Work Unit q This gives no inormation about n the time it took or the displacement to occur n the velocity or acceleration o the object q Work is a scalar quantity q SI Unit n Newton meter = Joule n N m = J mv n J = kg m / s = ( kg m / s ) m W ( F cosθ )Δ x = 1 1 mv0 = ( F cosθ ) Δx!! F Δ x October 7-13, 013

Work: + or -? q Work can be positive, negative, or zero. The sign o the work depends on the direction o the orce relative to the displacement!! W ( F cosφ) s = F s q Work positive: i 90 > φ> 0 q Work negative: i 180 > φ> 90 q Work zero: W = 0 i φ= 90 q Work maximum i φ= 0 q Work minimum i φ = 180 October 7-13, 013

Work done by a Gravitational Force q Gravitational Force n Magnitude: mg n Direction: downwards to the Earth s center q Work done by Gravitational Force r r W = FΔ rcosθ = F Δ W net = 1 mv 1 mv 0 W g = mgδr cosθ November 3, 008

Example: When Work is Zero q A man carries a bucket o water horizontally at constant velocity. q The orce does no work on the bucket q Displacement is horizontal q Force is vertical q cos 90 = 0 W ( F cosθ ) Δx October 7-13, 013

Example: Work Can Be Positive or Negative q Work is positive when liting the box q Work would be negative i lowering the box n The orce would still be upward, but the displacement would be downward October 7-13, 013

Work Done by a Constant q Force The work W done a system by an agent exerting a constant orce on the system is the product o the magnitude F o the orce, the magnitude Δr o the displacement o the point o application o the orce, and cosθ, where θ is the angle between the orce and displacement vectors: W!! F Δr = FΔr cosθ W I W III I III F! = 0 Δr! F! Δr! = FΔr F! Δr! II W II W IV = FΔr F! Δr! IV = FΔr cosθ October 7-13, 013

Work and Force q An Eskimo returning pulls a sled as shown. The total mass o the sled is 50.0 kg, and he exerts a orce o 1.0 10 N on the sled by pulling on the rope. How much work does he do on the sled i θ = 30 and he pulls the sled 5.0 m? W = ( F cosθ ) Δx = (1.0 10 = 5. 10 J N)(cos30! )(5.0m) October 7-13, 013

Work Done by Multiple Forces q I more than one orce acts on an object, then the total work is equal to the algebraic sum o the work done by the individual orces W net = W by individual orces n Remember work is a scalar, so this is the algebraic sum W net = W + W + W = ( F cosθ ) Δr g N F October 7-13, 013

Problem Solving Strategy q Identiy the initial and inal positions o the body, and draw a ree body diagram showing and labeling all the orces acting on the body q Choose a coordinate system q List the unknown and known quantities, and decide which unknowns are your target variables q Calculate the work done by each orce. Be sure to check signs. Add the amounts o work done by each orce to ind the net (total) work W net q Check whether your answer makes sense October 7-13, 013

Kinetic Energy q Kinetic energy associated with the motion o an object 1 K = mv q Scalar quantity with the same unit as work q Work is related to kinetic energy 1 mv 1 mv 0 = F netδ x W = KE KE = ΔKE net i October 7-13, 013

Work-Energy Theorem q When work is done by a net orce on an object and the only change in the object is its speed, the work done is equal to the change in the object s kinetic energy W net = K K i = ΔK n Speed will increase i work is positive n Speed will decrease i work is negative W net = 1 mv 1 mv 0 October 7-13, 013

Potential Energy q Potential energy is associated with the position o the object q Gravitational Potential Energy is the energy associated with the relative position o an object in space near the Earth s surace q The gravitational potential energy n n n n PE mgy m is the mass o an object g is the acceleration o gravity y is the vertical position o the mass relative the surace o the Earth SI unit: joule (J) November 3, 008

Reerence Levels q A location where the gravitational potential energy is zero must be chosen or each problem n The choice is arbitrary since the change in the potential energy is the important quantity n Choose a convenient location or the zero reerence height n oten the Earth s surace n may be some other point suggested by the problem n Once the position is chosen, it must remain ixed or the entire problem November 3, 008

q PE = mgy q W g = mg( y Work and Gravitational = FΔy cosθ = q Units o Potential Energy are the same as those o Work and Kinetic Energy W grav ity Potential Energy y i = ) PE mg( y i i PE y )cos0 November 3, 008

xtended Work-Energy Theorem q The work-energy theorem can be extended to include potential energy: Wnet = KE KEi = ΔKE W grav ity PE q I we only have gravitational orce, then KE KE i = = q The sum o the kinetic energy and the gravitational potential energy remains constant at all time and hence is a conserved quantity PE i i KE + PE = PE + i PE PE KE i W net = W gravity November 3, 008

Extended Work-Energy Theorem q We denote the total mechanical energy by q Since E = KE + PE KE + PE = PE + i KE i q The total mechanical energy is conserved and remains the same at all times 1 1 mv i + mgyi = mv + mgy q I there is riction orce PE + KE = E + KE + PE E i i Lostbyriction Lostbyriction = d November 3, 008

Problem-Solving Strategy q Deine the system q Select the location o zero gravitational potential energy n Do not change this location while solving the problem q Identiy two points the object o interest moves between n One point should be where inormation is given n The other point should be where you want to ind out something November 3, 008

Platorm Diver q A diver o mass m drops rom a board 10.0 m above the water s surace. Neglect air resistance. q (a) Find is speed 5.0 m above the water surace q (b) Find his speed as he hits the water November 3, 008

Platorm Diver q (a) Find is speed 5.0 m above the water surace 1 1 mv i + mgyi = mv + mgy 1 0 + gy i = v + mgy v = g( y i y ) = (9.8m / s )(10m 5m) = 9.9m / s q (b) Find his speed as he hits the water 1 0 + mgy i = mv + 0 v = gyi =14m / s November 3, 008

Power q Work does not depend on time interval q The rate at which energy is transerred is important in the design and use o practical device q The time rate o energy transer is called power q The average power is given by W P = Δt n when the method o energy transer is work October 7-13, 013

Units o Power qthe SI unit o power is called the watt n 1 watt = 1 joule / second = 1 kg. m / s 3 qa unit o power in the US Customary system is horsepower n 1 hp = 550 t. lb/s = 746 W qunits o power can also be used to express units o work or energy n 1 kwh = (1000 W)(3600 s) = 3.6 x10 6 J October 7-13, 013

Problems October 7-13, 013

October 7-13, 013

October 7-13, 013

October 7-13, 013

October 7-13, 013