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.

Slides:



Advertisements
Similar presentations
Physics 111: Mechanics Lecture 5
Advertisements

Chapter 4 Forces in One Dimension
Physics 201: Lecture 15, Pg 1 Lecture 15 l Goals  Employ conservation of momentum in 1 D & 2D  Introduce Momentum and Impulse  Compare Force vs time.
5. Using Newton’s Laws. Newton’s Third Law 3 Law of Action and Reaction Forces always occur in equal and opposite pairs A B A acts on B B acts on A.
Review Chap. 5 Applying Newton’s laws
Chapter 6: Circular Motion & Other Applications of Newton’s Laws
Dynamics of Uniform Circular Motion Chapter 5. Learning Objectives- Circular motion and rotation Uniform circular motion Students should understand the.
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.
Physics 215 – Fall 2014Lecture Welcome back to Physics 215 Today’s agenda: Weight, elevators, and normal forces Static and kinetic friction Tension.
Chapter 6: Work & Energy. THE COURSE THEME is NEWTON’S LAWS OF MOTION! Chs. 4, 5: Motion analysis with forces. NOW (Ch. 6): An alternative analysis using.
Chapter 5 Force and Motion (I) Kinematics vs Dynamics.
Apparent Weight Riding in a elevator– why does our weight appear to change when we start up (increase) and slow down (decrease)? Our sensation of weight.
Newton’s Laws of Motion
Forces and The Laws of Motion
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,
Chapter 4 Preview Objectives Force Force Diagrams
Physics 2.2.
Forces and the Laws of Motion Force, Mass, and Acceleration
FORCES AND LAWS OF MOTION. FORCE (push) (pull) Examples of forces: ContactField Pulling the handle of the door Pushing a stroller Hitting a tennis ball.
Physics Review Terms - Measurements time elapsed = duration of an event – there is a beginning, a middle, and an end to any event. distance = path.
Ch. 8 Momentum and its conservation
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.
Newton’s 1 st Law of Mechanics A particle will continue is a straight line at constant speed unless acted upon by a net push or pull (i.e. force). The.
Chapter 4 Newton’s Laws: Explaining Motion
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.
Today: Momentum – chapter 9 11/03 Finish momentum & review for exam 11/8 Exam 2 (5 – 8) 11/10 Rotation 11/15 Gravity 11/17 Waves & Sound 11/22 Temperature.
Chapter 4 Acceleration and Momentum. Objectives 4.1 Explain how force, mass, and acceleration are related. 4.1 Compare rates at which different objects.
Cutnell/Johnson Physics 7th edition Reading Quiz Questions
Chapter 7 Rotational Motion and the Law of Gravity
Chapter 5 Circular Motion; Gravitation. Centripetal Acceleration Centripetal means “Center Seeking” and the centripetal force on an object moving in a.
Lecture 10 Employ Newton’s Laws in 2D problems with circular motion 1.
Conceptual Example 4-4: What exerts the force to move a car?
Chapter 4 The Laws of Motion Phy 2053 Conceptual Questions Phy 2053 Conceptual Questions.
Chapter 4 The Laws of Motion. Classes of Forces Contact forces involve physical contact between two objects Field forces act through empty space No physical.
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.
Chapter 5 Dynamics of Uniform Circular Motion. 5.1 Uniform Circular Motion DEFINITION OF UNIFORM CIRCULAR MOTION Uniform circular motion is the motion.
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.
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.
Circular Motion Part 2 By: Heather Britton. Circular Motion Part 2 According to Newton’s 2nd Law, an accelerating body must have a force acting on it.
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:
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.
1 7/1/04 Midterm 1: July 9 Will cover material from Chapters 1-6 Go to the room where you usually have recitation July 6 Recitation will be a review session.
Dynamics!.
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:
Forces, The laws of Motion & Momentum.
Lecture 10 Goals Describe Friction
3.1 Work 3.2 Energy 3.3 Conservative and nonconservative forces 3.4 Power, energy and momentum conservation 3.5 Linear momentum 3.6 Collisions 3.7 Motion.
Physics 207: Lecture 13, Pg 1 Lecture 13 Goals: Assignments: l HW5, due tomorrow l For Wednesday, Read all of Chapter 10 Chapter 9 Chapter 9  Employ.
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 11, Pg 1 "Professor Goddard does not know the relation between action and reaction and the need to have something better than a vacuum.
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.
Forces and Motion Chapter 5 and 6. Focus  Force: a push or a pull  Acts on objects to change its velocity.
Copyright © by Holt, Rinehart and Winston. All rights reserved. ResourcesChapter menu Chapter 4 Force A force is a push or pull exerted on an object which.
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.
“What is uniform circular motion?” In uniform Circular motion a body travels at a constant speed on a circular path.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 5 Physics, 4 th Edition James S. Walker.
Free-Body Diagrams ForceSymbol/FormulaDescription WeightF w = mgAlways directed downward Tension ForceTPulling forces directed away from the body Normal.
Physics 207: Lecture 12, Pg 1 Lecture 12 Goals: Assignment: l HW5 due Tuesday 10/18 l For Monday: Read through Ch (Reading Quiz) Chapter 8: Chapter.
Lecture 12 Chapter 8: Solve 2D motion problems with friction
Physics 111: Mechanics Lecture 9
"Correction: It is now definitely established that a rocket can
Physics 207, Lecture 11, Oct. 8 Chapter 9: Momentum & Impulse
Lecture 10 Employ Newton’s Laws in 2D problems with circular motion
Which graph represents the motion of a ball rolling on a level friction free track? Which graph represents the motion of a ball rolling down a ramp?
AS-Level Maths: Mechanics 1 for Edexcel
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:

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 rotational motion models with friction or in free fall Chapter 9: Momentum & Impulse  Understand what momentum is and how it relates to forces  Employ momentum conservation principles  In problems with 1D and 2D Collisions  In problems having an impulse (Force vs. time)

Physics 207: Lecture 11, Pg 2 l One last reprisal of the Free Body Diagram l Remember 1 Normal Force is  to the surface 2 Friction is parallel to the contact surface 3 Radial (aka, centripetal) acceleration requires a net force Zero Gravity Ride

Physics 207: Lecture 11, Pg 3 Zero Gravity Ride A rider in a horizontal “0 gravity ride” finds herself stuck with her back to the wall. Which diagram correctly shows the forces acting on her?

Physics 207: Lecture 11, Pg 4 Banked Curves In the previous car scenario, we drew the following free body diagram for a race car going around a curve at constant speed on a flat track. Because the acceleration is radial (i.e., velocity changes in direction only) we need to modify our view of friction. n mgmg FfFf So, what differs on a banked curve?

Physics 207: Lecture 11, Pg 5 Banked Curves (high speed) 1 Draw a Free Body Diagram for a banked curve. 2 Use a rotated x-y coordinates 3 Resolve into components parallel and perpendicular to bank marmar xx xx y  N mgmg FfFf

Physics 207: Lecture 11, Pg 6 Banked Curves (constant high speed) 1 Draw a Free Body Diagram for a banked curve. 2 Use a rotated x-y coordinates 3 Resolve into components parallel and perpendicular to bank ( Note: For very small banking angles, one can approximate that F f is parallel to ma r. This is equivalent to the small angle approximation sin  = tan , but very effective at pushing the car toward the center of the curve!!) marmar xx xx y  N mgmg FfFf

Physics 207: Lecture 11, Pg 7 Banked Curves, high speed 4 Apply Newton’s 1 st and 2 nd Laws marmar xx xx y  N mg cos  FfFf mg sin   ma r cos  ma r sin   F x = -ma r cos  = - F f - mg sin   F y = ma r sin  = 0 - mg cos  + N Friction model  F f ≤  N (maximum speed when equal)

Physics 207: Lecture 11, Pg 8 Banked Curves, low speed 4 Apply Newton’s 1 st and 2 nd Laws marmar xx xx y  N mg cos  FfFf mg sin   ma r cos  ma r sin   F x = -ma r cos  = + F f - mg sin   F y = ma r sin  = 0 - mg cos  + N Friction model  F f ≤  N (minimum speed when equal but not less than zero!)

Physics 207: Lecture 11, Pg 9 Banked Curves, constant speed v max = (gr) ½ [ (  + tan  ) / (1 -  tan  )] ½ v min = (gr) ½ [  (tan  -  ) / (1 +  tan  )] ½ Dry pavement “Typical” values of r = 30 m, g = 9.8 m/s 2,  = 0.8,  = 20 ° v max = 20 m/s (45 mph) v min = 0 m/s (as long as  > 0.36 ) Wet Ice “Typical values” of r = 30 m, g = 9.8 m/s 2,  = 0.1,  =20 ° v max = 12 m/s (25 mph) v min = 9 m/s (Ideal speed is when frictional force goes to zero)

Physics 207: Lecture 11, Pg 10 Banked Curves, Testing your understanding Free Body Diagram for a banked curve. Use rotated x-y coordinates Resolve into components parallel and perpendicular to bank N mgmg FfFf At this moment you press the accelerator and, because of the frictional force (forward) by the tires on the road you begin to accelerate in that direction. How does the radial acceleration change? marmary x 

Physics 207: Lecture 11, Pg 11 Navigating a hill Knight concept exercise: A car is rolling over the top of a hill at speed v. At this instant, A. n > w. B. n = w. C. n < w. D.We can’t tell about n without knowing v. This occurs when the normal force goes to zero or, equivalently, when all the weight is used to achieve circular motion. F c = mg = m v 2 /r  v = (gr) ½ (just like an object in orbit) Note this approach can also be used to estimate the maximum walking speed. At what speed does the car lose contact?

Physics 207: Lecture 11, Pg 12 Orbiting satellites v T = (gr) ½

Physics 207: Lecture 11, Pg 13 Locomotion: how fast can a biped walk?

Physics 207: Lecture 11, Pg 14 How fast can a biped walk? What about weight? (a)A heavier person of equal height and proportions can walk faster than a lighter person (b)A lighter person of equal height and proportions can walk faster than a heavier person (c)To first order, size doesn’t matter

Physics 207: Lecture 11, Pg 15 How fast can a biped walk? What about height? (a)A taller person of equal weight and proportions can walk faster than a shorter person (b)A shorter person of equal weight and proportions can walk faster than a taller person (c)To first order, height doesn’t matter

Physics 207: Lecture 11, Pg 16 How fast can a biped walk? What can we say about the walker’s acceleration if there is UCM (a smooth walker) ? Acceleration is radial ! So where does it, a r, come from? (i.e., what external forces act on the walker?) 1. Weight of walker, downwards 2. Friction with the ground, sideways

Physics 207: Lecture 11, Pg 17 Impulse & Linear Momentum l Transition from forces to conservation laws Newton’s Laws  Conservation Laws Conservation Laws  Newton’s Laws They are different faces of the same physics NOTE: We have studied “impulse” and “momentum” but we have not explicitly named them as such Conservation of momentum is far more general than conservation of mechanical energy

Physics 207: Lecture 11, Pg 18 Forces vs time (and space, Ch. 10) l Underlying any “new” concept in Chapter 9 is (1) A net force changes velocity (either magnitude or direction) (2) For any action there is an equal and opposite reaction l If we emphasize Newton’s 3 rd Law and emphasize changes with time then this leads to the Conservation of Momentum Principle

Physics 207: Lecture 11, Pg 19 Example 1 A 2 kg block, initially at rest on frictionless horizontal surface, is acted on by a 10 N horizontal force for 2 seconds (in 1D). What is the final velocity? l F is to the positive & F = ma thus a = F/m = 5 m/s 2 v = v 0 + a  t = 0 m/s + 2 x 5 m/s = 10 m/s (+ direction) Notice: v - v 0 = a  t  m (v - v 0 ) = ma  t  m  v = F  t If the mass had been 4 kg …what is the final velocity? - + F (N) time (s)

Physics 207: Lecture 11, Pg 20 Twice the mass l Same force l Same time Half the acceleration (a = F / m ’ ) l Half the velocity ! ( 5 m/s ) F (N) Time (sec) Before

Physics 207: Lecture 11, Pg 21 Example 1 l Notice that the final velocity in this case is inversely proportional to the mass (i.e., if thrice the mass….one-third the velocity). l Here, mass times the velocity always gives the same value. (Always 20 kg m/s.) F (N) Time (sec) Area under curve is still the same ! Force x change in time = mass x change in velocity

Physics 207: Lecture 11, Pg 22 Example l There many situations in which the sum of the product “mass times velocity” is constant over time l To each product we assign the name, “momentum” and associate it with a conservation law. (Units: kg m/s or N s) l A force applied for a certain period of time can be graphed and the area under the curve is the “impulse” F (N) Time (sec) Area under curve : “impulse” With: m  v = F avg  t

Physics 207: Lecture 11, Pg 23 Force curves are usually a bit different in the real world

Physics 207: Lecture 11, Pg 24 Example with Action-Reaction l Now the 10 N force from before is applied by person A on person B while standing on a frictionless surface l For the force of A on B there is an equal and opposite force of B on A F (N) Time (sec) A on B B on A M A x  V A = Area of top curve M B x  V B = Area of bottom curve Area (top) + Area (bottom) = 0

Physics 207: Lecture 11, Pg 25 Example with Action-Reaction M A  V A + M B  V B = 0 M A [V A (final) - V A (initial) ] + M B [V B (final) - V B (initial) ] = 0 Rearranging terms M A V A (final) +M B V B (final) = M A V A (initial) +M B V B (initial) which is constant regardless of M or  V (Remember: frictionless surface)

Physics 207: Lecture 11, Pg 26 Example with Action-Reaction M A V A (final) +M B V B (final) = M A V A (initial) +M B V B (initial) which is constant regardless of M or  V Define MV to be the “momentum” and this is conserved in a system if and only if the system is not acted on by a net external force (choosing the system is key) Conservation of momentum is a special case of applying Newton’s Laws

Physics 207: Lecture 11, Pg 27 Applications of Momentum Conservation 234 Th 238 U Alpha Decay 4 He v1v1 v2v2 Explosions Radioactive decay: Collisions

Physics 207: Lecture 11, Pg 28 Impulse & Linear Momentum l Newton’s 2 nd Law: Fa F = ma l This is the most general statement of Newton’s 2 nd Law pv p ≡ mv pv (p is a vector since v is a vector) So p x = mv x and so on (y and z directions) l Definition: For a single particle, the momentum p is defined as:

Physics 207: Lecture 11, Pg 29 Momentum Conservation l Momentum conservation (recasts Newton’s 2 nd Law when net external F = 0) is an important principle l It is a vector expression (P x, P y and P z ).  And applies to any situation in which there is NO net external force applied (in terms of the x, y & z axes).

Physics 207: Lecture 11, Pg 30 Momentum Conservation l Many problems can be addressed through momentum conservation even if other physical quantities (e.g. mechanical energy) are not conserved l Momentum is a vector quantity and we can independently assess its conservation in the x, y and z directions (e.g., net forces in the z direction do not affect the momentum of the x & y directions)

Physics 207: Lecture 11, Pg 31 Exercise 2 Momentum Conservation A. Box 1 B. Box 2 C. same l Two balls of equal mass are thrown horizontally with the same initial velocity. They hit identical stationary boxes resting on a frictionless horizontal surface. l The ball hitting box 1 bounces elastically back, while the ball hitting box 2 sticks.  Which box ends up moving fastest ? 1 2

Physics 207: Lecture 11, Pg 32 Lecture 11 Assignment: l For Monday: Read through Chapter 10, 1 st four sections l MP HW6 due Wednesday 3/3