Lecture 10 Goals Describe Friction

Slides:



Advertisements
Similar presentations
Physics 207: Lecture 10, Pg 1 Lecture 10 l Goals: Employ Newtons Laws in 2D problems with circular motion Assignment: HW5, (Chapters 8 & 9, due 3/4, Wednesday)
Advertisements

SPH3UW Today’s Agenda Friction What is it?
SPH4U: Lecture 7 Today’s Agenda
FORCE A force is any influence that can change the velocity of a body. Forces can act either through the physical contact of two objects (contact forces:
Physics 111: Mechanics Lecture 5
The Laws of Motion Physics 2053 Lecture Notes The Laws of Motion.
Chapter 10. Uniform Circular Motion
Review Chap. 5 Applying Newton’s laws
Physics 207: Lecture 7, Pg 1 Physics 207, Lecture 7, Sept. 25 Agenda: Assignment: l WebAssign Problem Set 3 due Tuesday midnight l MidTerm Thursday, Oct.
Physics 207: Lecture 11, Pg 1 Lecture 11 Goals: Assignment: l Read through Chapter 10 l MP HW5, due Wednesday 3/3 Chapter 9: Momentum & Impulse Chapter.
As the ball revolves faster, the angle increases
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lectures
Physics 151: Lecture 9, Pg 1 Physics 151: Lecture 9 l Announcements çHomework #3 (due this Fri. 9/22/06, 5 PM) çHomework #4 (due Mon. 10/2/06, 5 PM) l.
Circular Motion and Other Applications of Newton’s Laws
Newton’s Laws of Motion Problems MC Questions
Circular Motion and Other Applications of Newton’s Laws
Physics 207: Lecture 9, Pg 1 Lecture 9 l Today:  Review session Assignment: For Monday, Read Chapter 8 Exam Thursday, Oct. 2 nd from 7:15-8:45 PM Chapters.
Newton’s Laws of Motion
Circular Motion.
Physics 207: Lecture 7, Pg 1 Lecture 7 l Goals:  Solve 1D and 2D problems with forces in equilibrium and non-equilibrium (i.e., acceleration) using Newton’
Physics 207: Lecture 8, Pg 1 Lecture 8 l Goals:  Solve 1D & 2D motion with friction  Utilize Newton’s 2 nd Law  Differentiate between Newton’s 1 st,
Physics 207: Lecture 7, Pg 1 "Professor Goddard does not know the relation between action and reaction and the need to have something better than a vacuum.
Physics. Session Opener A recent space shuttle accident occurred because of failure of heat protecting devices. How was this heat generated ?
Newton’s Laws - continued
AP Physics B Summer Course 年AP物理B暑假班
Physics 201: Lecture 9, Pg 1 Lecture 8 l Goals:  Solve 1D & 2D problems introducing forces with/without friction  Utilize Newton’s 1 st & 2 nd Laws 
1 4 Topics force and net force inertia and 1 st law acceleration and 2 nd law g notation force pairs and 3 rd law force diagrams equilibrium friction.
Physics 207: Lecture 9, Pg 1 Lecture 9 l Today:  Review session Assignment: For Thursday, Read Chapter 8, first four sections Exam Wed., Feb. 18 th from.
Example 1: A 3-kg rock swings in a circle of radius 5 m
Mechanics Topic 2.2 Forces and Dynamics. Forces and Free-body Diagrams To a physicist a force is recognised by the effect or effects that it produces.
Physics 201: Lecture 19, Pg 1 Lecture 19 Goals: Specify rolling motion (center of mass velocity to angular velocity Compare kinetic and rotational energies.
1 Law of friction Properties of frictional force surface between two bodies 1.act along the surface between two bodies oppose relative motion 2.act in.
Forces of Friction When an object is in motion on a surface or through a viscous medium, there will be a resistance to the motion This is due to the interactions.
CHAPTER 6 : CIRCULAR MOTION AND OTHER APPLICATIONS OF NEWTON’S LAWS
Lecture 10 Employ Newton’s Laws in 2D problems with circular motion 1.
 Extension of Circular Motion & Newton’s Laws Chapter 6 Mrs. Warren Kings High School.
Physics 203 – College Physics I Department of Physics – The Citadel Physics 203 College Physics I Fall 2012 S. A. Yost Chapter 5 Circular Motion, Universal.
This property of all matter to continue in its present state of motion (straight line, constant speed) is called inertia. What determines how much inertia.
Uniform Circular Motion Centripetal forces keep these children moving in a circular path.
Frictional Forces  Two types: - static – applies to stationary objects - kinetic – applies to sliding (moving) objects  Like F N, the Frictional Force.
Force & Newton’s Laws of Motion. FORCE Act of pulling or pushing Act of pulling or pushing Vector quantity that causes an acceleration when unbalanced.
Physics 207: Lecture 11, Pg 1 Lecture 11 l Goals:  Employ Newton’s Laws in 2D problems with circular motion  Relate Forces with acceleration Assignment:
Physics 207: Lecture 10, Pg 1 Lecture 10 l Goals:  Exploit Newton’s 3 rd Law in problems with friction  Employ Newton’s Laws in 2D problems with circular.
Copyright © 2009 Pearson Education, Inc. Chapter 5 Using Newton’s Laws: Friction, Circular Motion, Drag Forces.
Physics 207: Lecture 8, Pg 1 Lecture 9 l Goals  Describe Friction in Air (Ch. 6)  Differentiate between Newton’s 1 st, 2 nd and 3 rd Laws  Use Newton’s.
Physics 207: Lecture 11, Pg 1 Lecture 11 Goals: Assignment: l Read through Chapter 10, 1 st four section l MP HW6, due Wednesday 3/3 Chapter 8: Employ.
Physics 207: Lecture 8, Pg 1 Lecture 8 l Goals:  Differentiate between Newton’s 1 st, 2 nd and 3 rd Laws  Use Newton’s 3 rd Law in problem solving Assignment:
Lecture 8 Static friction and Kinetic or Sliding friction.
Newton’s 1 st Law of Motion. Newton’s 1 st Law Newton’s 1 st Law: An object at rest stays at rest and an object in motion stays in motion, unless acted.
Chapter 6.2. Uniform Circular Motion Centripetal forces keep these children moving in a circular path.
Chapter 5 Two Dimensional Forces Equilibrium An object either at rest or moving with a constant velocity is said to be in equilibrium The net force acting.
Newton’s 1 st Law of Motion. Newton’s 1 st Law Newton’s 1 st Law: An object at _______stays at _______and an object in motion stays in motion, unless.
Physics 207: Lecture 8, Pg 1 Lecture 8 l Goals:  Differentiate between Newton’s 1 st, 2 nd and 3 rd Laws  Use Newton’s 3 rd Law in problem solving Assignment:
Physics 215 – Fall 2014Lecture Welcome back to Physics 215 Today’s agenda: More on free-body diagrams and force components Applying Newton’s laws.
Physics 207: Lecture 9, Pg 1 Lecture 9 l Goals  Describe Friction in Air (Ch. 6), (not on 1 st Exam)  Differentiate between Newton’s 1 st, 2 nd and 3.
Physics 207: Lecture 8, Pg 1 Lecture 8 l Goals: (Finish Chap. 6 and begin Ch. 7)  Solve 1D & 2D motion with friction  Utilize Newton’s 2 nd Law  Differentiate.
Physics 1501: Lecture 8, Pg 1 Physics 1501: Lecture 8 l Announcements çHomework #3 : due next Monday l Topics çReview of Newton’s Laws. çFriction çSome.
PHY 151: Lecture Forces of Friction 5.9 Newton’s Second Law.
Physics 1501: Lecture 9, Pg 1 Physics 1501: Lecture 9 l Announcements çHomework #3 : due next Monday çBut HW 04 will be due the following Friday (same.
Physics 218 Lecture 8: Dynamics Alexei Safonov.
Newton’s Laws.
Chapter 6 Force and Motion II. Forces of Friction When an object is in motion on a surface or through a viscous medium, there will be a resistance to.
SPH4U: Friction What is it? Systematic catagories of forces
Two Dimensional Forces
Lecture 11 Goals: Employ Newton’s Laws in 2D problems with circular motion Relate Forces with acceleration Assignment: HW5, (Chapter 7, 8 and 9 due.
SPH4U: Lecture 7 Today’s Agenda
Centripetal forces keep these children moving in a circular path.
Lecture 7 Goals: Solve 1D and 2D problems with forces in equilibrium and non-equilibrium (i.e., acceleration) using Newton’ 1st and 2nd laws. Differentiate.
Lecture 10 Employ Newton’s Laws in 2D problems with circular motion
Lecture 11 Goals: Employ Newton’s Laws in 2D problems with circular motion Relate Forces with acceleration Assignment: HW5, (Chapter 7, 8 and 9 due.
Presentation transcript:

Lecture 10 Goals Describe Friction Problem solving with Newton’s 1st, 2nd and 3rd Laws Forces in circular and curvelinear motion 1

Another experiment: A modified Atwood’s machine Two blocks, m1 & m2, are connected by a massless frictionless string/pulley on the table as shown. The table surface is frictionless and little g acts downward. What is the acceleration of the horizontal block? m2 m2g N T Requires two FBDs and Newton’s 3rd Law. T m1 Mass 1 S Fy = m1a1y= T – m1g m1g Correlated motion: |a1y| = | a2x| ≡ a If m1 moves up moves m2 right Mass 2 S Fx = m2a2x = -T S Fy = 0 = N – m2g

Another experiment: A modified Atwood’s machine Two blocks, m1 & m2, are connected by a massless frictionless string/pulley on the table as shown. The table surface is frictionless and little g acts downward. What is the acceleration of the horizontal block. m2 m2g N T Requires two FBDs and Newton’s 3rd Law. T m1 Mass 1 A. S Fy = m1 a= T – m1g m1g Subbing in T from B into A m1 a= - m2 a – m1g m1 a + m2 a = m1g a = m1g / (m1 + m2 ) Mass 2 B. S Fx = m2 a = -T S Fy = 0 = N – m2g

A “special” contact force: Friction What does it do? It opposes motion (velocity, actual or that which would occur if friction were absent!) How do we characterize this in terms we have learned? Friction results in a force in a direction opposite to the direction of motion (actual or, if static, then “inferred”)! i j N FAPPLIED ma fFRICTION mg

If no acceleration No net force So frictional force just equals applied force Key point: It is conditional! j N FAPPLIED i fFRICTION mg

Friction... Friction is caused by the “microscopic” interactions between the two surfaces:

Friction: Static friction Static equilibrium: A block with a horizontal force F applied, S Fx = 0 = -F + fs  fs = F S Fy = 0 = - N + mg  N = mg FBD F fs N mg As F increases so does fs m

Static friction, at maximum (just before slipping) Equilibrium: A block, mass m, with a horizontal force F applied, Direction: A force vector  to the normal force vector N and the vector is opposite to the direction of acceleration if m were 0. Magnitude: fS is proportional to the magnitude of N fs = ms N N F m fs mg

Kinetic or Sliding friction (fk < fs) Dynamic equilibrium, moving but acceleration is still zero As F increases fk remains nearly constant (but now there acceleration is acceleration) FBD S Fx = 0 = -F + fk  fk = F S Fy = 0 = - N + mg  N = mg v N F m1 fk mg fk = mk N

Model of Static Friction (simple case) Magnitude: f is proportional to the applied forces such that fs ≤ ms N ms called the “coefficient of static friction” Direction: Opposite to the direction of system acceleration if m were 0

Sliding Friction Direction: A force vector  to the normal force vector N and the vector is opposite to the velocity. Magnitude: fk is proportional to the magnitude of N fk = k N ( = Kmg in the previous example) The constant k is called the “coefficient of kinetic friction” Logic dictates that S > K for any system

Coefficients of Friction Material on Material s = static friction k = kinetic friction steel / steel 0.6 0.4 add grease to steel 0.1 0.05 metal / ice 0.022 0.02 brake lining / iron 0.3 tire / dry pavement 0.9 0.8 tire / wet pavement 0.7

Forces at different angles Case1: Downward angled force with friction Case 2: Upwards angled force with friction Cases 3,4: Up against the wall Questions: Does it slide? What happens to the normal force? What happens to the frictional force? Cases 3, 4 Case 2 Case 1 ff F F N N N F ff ff mg mg mg

Many Forces are Conditional Notice what happens if we change the direction of the applied force The normal force can increase or decrease j N > mg F i Let a=0 fF mg

An experiment S Fy = 0 = T – m1g S Fx = 0 = -T + fs = -T + mS N Two blocks are connected on the table as shown. The table has unknown static and kinetic friction coefficients. Design an experiment to find mS m2 m2g N T Mass 1 S Fy = 0 = T – m1g fS T m1 Mass 2 S Fx = 0 = -T + fs = -T + mS N S Fy = 0 = N – m2g m1g T = m1g = mS m2g  mS = m1/m2

A conceptual question: A flying bird in a cage You have a bird in a cage that is resting on your upward turned palm.  The cage is completely sealed to the outside (at least while we run the experiment!).  The bird is initially sitting at rest on the perch.  It decides it needs a bit of exercise and starts to fly. Question: How does the weight of the cage plus bird vary when the bird is flying up, when the bird is flying sideways, when the bird is flying down? Follow up question: So, what is holding the airplane up in the sky? 

3rd Law : Static Friction with a bicycle wheel You are pedaling hard and the bicycle is speeding up. What is the direction of the frictional force? You are breaking and the bicycle is slowing down

Static Friction with a bicycle wheel You are pedaling hard and the bicycle is speeding up. What is the direction of the frictional force? Hint…you are accelerating to the right a = F / m Ffriction, on B from E is to the right Ffriction, on E from,B is to the left

Home Exercise Newton’s Third Law A fly is deformed by hitting the windshield of a speeding bus.  v The force exerted by the bus on the fly is, greater than equal to less than that exerted by the fly on the bus.

Home Exercise Newton’s Third Law A fly is deformed by hitting the windshield of a speeding bus.  v The force exerted by the bus on the fly is, B. equal to that exerted by the fly on the bus.

Home Exercise Newton’s 3rd Law Same scenario but now we examine the accelerations A fly is deformed by hitting the windshield of a speeding bus.  v The magnitude of the acceleration, due to this collision, of the bus is greater than equal to less than that of the fly.

Home Exercise Newton’s 3rd Law Solution By Newton’s third law these two forces form an interaction pair which are equal (but in opposing directions).  Thus the forces are the same However, by Newton’s second law Fnet = ma or a = Fnet/m. So Fb, f = -Ff, b = F0 but |abus | = |F0 / mbus | << | afly | = | F0/mfly | Answer for acceleration is (C)

Force pairs on an Inclined plane Forces on the block (static case) Normal Force Friction Force f= mN Forces on the plane by block y q x

Putting it all together gives two different accelerations, The inclined plane coming and going (not static): the component of mg along the surface > kinetic friction Fx = max = mg sin q ± uk N Fy = may = 0 = -mg cos q + N Putting it all together gives two different accelerations, ax = g sin q ± uk g cos q. A tidy result but ultimately it is the process of applying Newton’s Laws that is key.

Inclined plane with “Normal” and Frictional Forces Static Equilibrium Case Dynamic Equilibrium (see 1) Dynamic case with non-zero acceleration “Normal” means perpendicular Normal Force Friction Force S F = 0 Fx= 0 = mg sin q – f Fy= 0 = –mg cos q + N with mg sin q = f ≤ mS N if mg sin q > mS N, must slide Critical angle ms = tan qc f mg sin q q y mg cos q q q x Block weight is mg

Inclined plane with “Normal” and Frictional Forces Static Equilibrium Case Dynamic Equilibrium Friction opposite velocity (down the incline) “Normal” means perpendicular Normal Force v Friction Force fK S F = 0 Fx= 0 = mg sin q – fk Fy= 0 = –mg cos q + N fk = mk N = mk mg cos q Fx= 0 = mg sin q – mk mg cos q mk = tan q (only one angle) mg sin q q y mg cos q q q x mg

Inclined plane with “Normal” and Frictional Forces 3. Dynamic case with non-zero acceleration Result depends on direction of velocity Weight of block is mg Normal Force Friction Force Sliding Down q v mg sin q fk Sliding Up Fx= max = mg sin q ± fk Fy= 0 = –mg cos q + N fk = mk N = mk mg cos q Fx= max = mg sin q ± mk mg cos q ax = g sin q ± mk g cos q

Velocity and acceleration plots: Notice that the acceleration is always down the slide and that, even at the turnaround point, the block is always motion although there is an infinitesimal point at which the velocity of the block passes through zero. At this moment, depending on the static friction the block may become stuck.

Forces with rotation about a fixed axis Key steps Identify forces (i.e., a FBD) Identify axis of rotation Circular motion implies ar & Fr = mar Apply conditions (position, velocity & acceleration)

Consider a person on a swing: Example The pendulum axis of rotation Consider a person on a swing: (A) (B) (C) When is the tension equal to the weight of the person + swing? (A) At the top of the swing (turnaround point) (B) Somewhere in the middle (C) At the bottom of the swing (D) Never, it is always greater than the weight (E) Never, it is always less than the weight

Example Gravity, Normal Forces etc. mg T q y x axis of rotation vt mg T at top of swing vt = 0 Fr = m 02 / r = 0 = T – mg cos q T = mg cos q T < mg at bottom of swing vt is max Fr = m ac = m vt2 / r = T - mg T = mg + m vt2 / r T > mg

Conical Pendulum (Not a simple pendulum) Swinging a ball on a string of length L around your head (r = L sin q) axis of rotation S Fr = mar = T sin q S Fz = 0 = T cos q – mg so T = mg / cos q (> mg) mar = (mg / cos q ) (sin q ) ar = g tan q = vT2/r  vT = (gr tan q)½ L r Period: T= 2p r / vT =2p (r cot q /g)½ = 2p (L cos q /g)½

Conical Pendulum (very different) Swinging a ball on a string of length L around your head axis of rotation r L Period: t = 2p r / vT =2p (r cot q /g)½ = 2p (L cos q / g )½ = 2p (5 cos 5 / 9.8 )½ = 4.38 s = 2p (5 cos 10 / 9.8 )½ = 4.36 s = 2p (5 cos 15 / 9.8 )½ = 4.32 s

Another example of circular motion Loop-the-loop 1 A match box car is going to do a loop-the-loop of radius r. What must be its minimum speed vt at the top so that it can manage the loop successfully ?

Loop-the-loop 1 To navigate the top of the circle its tangential velocity vT must be such that its centripetal acceleration at least equals the force due to gravity. At this point N, the normal force, goes to zero (just touching). Fr = mar = mg = mvt2/r vt = (gr)1/2 vT mg

Loop-the-loop 2 The match box car is going to do a loop-the-loop. If the speed at the bottom is vB, what is the normal force, N, at that point? Hint: The car is constrained to the track. Fr = mar = mvB2/r = N - mg N = mvB2/r + mg N v mg

Loop-the-loop 3 Once again the car is going to execute a loop-the-loop. What must be its minimum speed at the bottom so that it can make the loop successfully? This is a difficult problem to solve using just forces. We will skip it now and revisit it using energy considerations later on…

Orbiting satellites vt = (gr)½ Net Force: ma = mg = mvt2 / r gr = vt2 vt = (gr)½ The only difference is that g is less because you are further from the Earth’s center!

Geostationary orbit The radius of the Earth is ~6000 km but at 36000 km you are ~42000 km from the center of the earth. Fgravity is proportional to 1/r2 and so little g is now ~10 m/s2 / 50 vT = (0.20 * 42000000)½ m/s = 3000 m/s At 3000 m/s, period T = 2p r / vT = 2p 42000000 / 3000 sec = = 90000 sec = 90000 s/ 3600 s/hr = 24 hrs Orbit affected by the moon and also the Earth’s mass is inhomogeneous (not perfectly geostationary) Great for communication satellites (1st pointed out by Arthur C. Clarke)

Recap Assignment: HW5 For Tuesday: Read Chapter 7.1-7.4 1