PHYS 21: Assignment 4 Solutions

Similar documents
Kinematics (special case) Dynamics gravity, tension, elastic, normal, friction. Energy: kinetic, potential gravity, spring + work (friction)

Chapter 8- Rotational Kinematics Angular Variables Kinematic Equations

Physics 201. Professor P. Q. Hung. 311B, Physics Building. Physics 201 p. 1/1

Physics 4A Solutions to Chapter 10 Homework

Assessment Schedule 2016 Physics: Demonstrate understanding of mechanical systems (91524)

Forces of Rolling. 1) Ifobjectisrollingwith a com =0 (i.e.no netforces), then v com =ωr = constant (smooth roll)

Rotational Dynamics continued

Your Name: PHYSICS 101 MIDTERM. Please Circle your section 1 9 am Galbiati 2 10 am Wang 3 11 am Hasan 4 12:30 am Hasan 5 12:30 pm Olsen

PHY2020 Test 2 November 5, Name:

Chapter 10 Solutions

a +3bt 2 4ct 3) =6bt 12ct 2. dt 2. (a) The second hand of the smoothly running watch turns through 2π radians during 60 s. Thus,

Your Name: PHYSICS 101 MIDTERM. Please circle your section 1 9 am Nappi 2 10 am McDonald 3 10 am Galbiati 4 11 am McDonald 5 12:30 pm Pretorius

PH1104/PH114S MECHANICS

Translational vs Rotational. m x. Connection Δ = = = = = = Δ = = = = = = Δ =Δ = = = = = 2 / 1/2. Work

are (0 cm, 10 cm), (10 cm, 10 cm), and (10 cm, 0 cm), respectively. Solve: The coordinates of the center of mass are = = = (200 g g g)

Chapter 10. Rotation

= o + t = ot + ½ t 2 = o + 2

Motion in Space. MATH 311, Calculus III. J. Robert Buchanan. Fall Department of Mathematics. J. Robert Buchanan Motion in Space

Dynamics of Rotational Motion

. d. v A v B. e. none of these.

Circular Motion, Pt 2: Angular Dynamics. Mr. Velazquez AP/Honors Physics

We define angular displacement, θ, and angular velocity, ω. What's a radian?

PHYS 111 HOMEWORK #11

Chapter 13: Oscillatory Motions

Midterm 3 Review (Ch 9-14)

Physics 207: Lecture 24. Announcements. No labs next week, May 2 5 Exam 3 review session: Wed, May 4 from 8:00 9:30 pm; here.

Torque/Rotational Energy Mock Exam. Instructions: (105 points) Answer the following questions. SHOW ALL OF YOUR WORK.

Chapter 8. Rotational Equilibrium and Rotational Dynamics

Lagrangian Dynamics: Generalized Coordinates and Forces

PC 1141 : AY 2012 /13

Chapter 8. Centripetal Force and The Law of Gravity

Notes on Torque. We ve seen that if we define torque as rfsinθ, and the N 2. i i

A Level. A Level Physics. Circular Motion (Answers) Edexcel. Name: Total Marks: /30

t = g = 10 m/s 2 = 2 s T = 2π g

Distance travelled time taken and if the particle is a distance s(t) along the x-axis, then its instantaneous speed is:

Motion Part 4: Projectile Motion

Exam 3 Practice Solutions

Momentum. The way to catch a knuckleball is to wait until it stops rolling and then pick it up. -Bob Uecker

Slide 1 / 37. Rotational Motion

Angular velocity and angular acceleration CHAPTER 9 ROTATION. Angular velocity and angular acceleration. ! equations of rotational motion

Review questions. Before the collision, 70 kg ball is stationary. Afterward, the 30 kg ball is stationary and 70 kg ball is moving to the right.

PUPC Grading Scheme. November 17, General Guidelines

Assignment 9. to roll without slipping, how large must F be? Ans: F = R d mgsinθ.

Name (please print): UW ID# score last first

PH1104/PH114S - MECHANICS

Physics 5A Final Review Solutions

Rotational motion problems

Uniform Circular Motion:-Circular motion is said to the uniform if the speed of the particle (along the circular path) remains constant.

FALL TERM EXAM, PHYS 1211, INTRODUCTORY PHYSICS I Monday, 14 December 2015, 6 PM to 9 PM, Field House Gym

Lecture 5 Review. 1. Rotation axis: axis in which rigid body rotates about. It is perpendicular to the plane of rotation.

Torque. Introduction. Torque. PHY torque - J. Hedberg

Chapter 8 Lecture Notes

Physics 121, March 25, Rotational Motion and Angular Momentum. Department of Physics and Astronomy, University of Rochester

Announcements Oct 27, 2009

Rotational Motion. Rotational Motion. Rotational Motion

= 2 5 MR2. I sphere = MR 2. I hoop = 1 2 MR2. I disk

16. Rotational Dynamics

Physics 2210 Homework 18 Spring 2015

Your Name: PHYSICS 101 MIDTERM. Please circle your section 1 9 am Galbiati 2 10 am Kwon 3 11 am McDonald 4 12:30 pm McDonald 5 12:30 pm Kwon

Physics 141. Lecture 18. Frank L. H. Wolfs Department of Physics and Astronomy, University of Rochester, Lecture 18, Page 1

Chapter 10. Rotation of a Rigid Object about a Fixed Axis

Chapters 10 & 11: Rotational Dynamics Thursday March 8 th

Physics of Rotation. Physics 109, Introduction To Physics Fall 2017

Quiz Number 4 PHYSICS April 17, 2009

Angular Momentum. Physics 1425 Lecture 21. Michael Fowler, UVa

PHYSICS 149: Lecture 21

LAST NAME FIRST NAME DATE. Rotational Kinetic Energy. K = ½ I ω 2

Figure 1 Answer: = m

Exam Question 6/8 (HL/OL): Circular and Simple Harmonic Motion. February 1, Applied Mathematics: Lecture 7. Brendan Williamson.

Physics 101 Lecture 12 Equilibrium and Angular Momentum

Two-Dimensional Rotational Kinematics

Moment of Inertia & Newton s Laws for Translation & Rotation

31 ROTATIONAL KINEMATICS

Chapter 8: Newton s Laws Applied to Circular Motion

AP Physics 1: Rotational Motion & Dynamics: Problem Set

Rotation Quiz II, review part A

Class XI Chapter 7- System of Particles and Rotational Motion Physics

Handout 7: Torque, angular momentum, rotational kinetic energy and rolling motion. Torque and angular momentum

DYNAMICS MOMENT OF INERTIA

Physics 218 Exam 3 Spring 2010, Sections

43. A person sits on a freely spinning lab stool that has no friction in its axle. When this person extends her arms,

UNIVERSITY OF TORONTO Faculty of Arts and Science

Ch 8. Rotational Dynamics

AP Physics 1 Second Semester Final Exam Review

Rotation Angular Momentum

PSI AP Physics I Rotational Motion

Physics 2211 M Quiz #2 Solutions Summer 2017

Relating Linear and Angular Kinematics. a rad = v 2 /r = rω 2

Chapter 8: Newton s Laws Applied to Circular Motion

Chap10. Rotation of a Rigid Object about a Fixed Axis

ROTATORY MOTION. ii) iii) iv) W = v) Power = vi) Torque ( vii) Angular momentum (L) = Iω similar to P = mv 1 Iω. similar to F = ma

Welcome back to Physics 211

Rotation. Rotational Variables

Physics 123 Quizes and Examinations Spring 2002 Porter Johnson

HW3 Physics 311 Mechanics

FIGURE 2. Total Acceleration The direction of the total acceleration of a rotating object can be found using the inverse tangent function.

Chapter 9- Static Equilibrium

CP1 REVISION LECTURE 3 INTRODUCTION TO CLASSICAL MECHANICS. Prof. N. Harnew University of Oxford TT 2017

Translational Motion Rotational Motion Equations Sheet

Lecture 10. Example: Friction and Motion

Transcription:

PHYS 1: Assignment 4 Solutions Due on Feb 4 013 Prof. Oh Katharine Hyatt 1

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.43 We see immediately that there is friction in this problem, so we can t use conservation of energy. We know that for the hoop: v h =ωrrolling condition And for the box: a b =g cos θ µ k g sin θ The fact that the hoop keeps pace with the box means that v h = v b Which automatically gives us a h = a b We see that: a h = d dt (ωr) = ωr = τ I h R = τ m h R R = τ m h R We realise that gravity exerts no torque because it is exerted at the centre of mass of the hoop. The only force which exerts a torque is friction. τ =fr =µ k m h g sin θr a h = µ km h g sin θr m h R =µ k g sin θ µ k g sin θ =g cos θ µ k g sin θ µ k sin θ = cos θ µ k = 1 tan θ Page of 8

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.43 H + R 1.49 We see that there is no friction in this problem, so we can use conservation of energy. Let s call the speed of the ball as it exits the track v f : P E =mgh KE = 1 mv + I ω E =P E + KE de dt =0 mgh =mgh + 1 mv f + mr 5 ω f From the rolling condition, we see that So: ω f = v f R mgh =mgh + 1 mv f + m 5 v f g(h h) = 7 v f = 10 v f 10g(H h) 7 Then, using our kinematics knowledge, we see that: h = gt h t = g x =v f t 0(H h)h = 7 0(60 0)(0) = 7 40 =0m 7 =47.8m Page 3 of 8

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.49 H + R 1.50 Again there is no friction, so we can use conservation of energy. In order for the marble to just stay on the track, the normal force exerted on it by the track at the top of the loop should be exactly 0. Since the marble is on a circular section of track, this is the same as saying that gravity provides all the centripetal acceleration. This condition can be written: So, from conservation of energy: g = v top R H + R 1.51 mgh =mgr + 1 mv top + I ω =mgr + 1 mr vtop mgr + 5 R = 3 mgr + 1 5 mgr = 17 10 mgr h = 17 10 R To solve this, we can just write down the torques and use Newton s third law. We know that: To find the angular acceleration α: ma =W T τ =T R =Iα = mr T R = mra = RW 3 T R =RW T = W 3 a R α = T R I = T R mr = W 3mR = g 3R RT Page 4 of 8

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.51 H + R 1.5 We use Newton s third law again: ma =mg sin θ T where T is the tension T R =Iα I = m R T = m Rα = m R a R = m a ma =mg sin θ 1 ma 3 ma =mg sin θ a = 3 g sin θ So the tape unwinds with constant acceleration. Now we can use a kinematics equation: l =v 0 t + 1 at L = 1 at where T is the unwinding time T = L a L 3 T = g sin θ 3L = g sin θ Page 5 of 8

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.5 H + R 1.57 We can use energy methods again: mgh = 1 Iω + 1 mv mgh = 1 v mr 5 R + 1 mv = 7 10 mv 10 v = 7 gh x =v cos θt y = v sin θt 1 gt gx y = x tan θ v cos θ 7x y = x tan θ 0h cos θ Plugging in the numbers the question gives us, we find: x = 5.34 m Page 6 of 8

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.57 H + R 1.59 Let s call the velocity of the centre of mass v c, and the velocity of the far end (the one her hand isn t on) v f. We see that she throws the stick with ω 0. Let s call the angular velocity about the centre of mass ω. v c = ω 0L v f =ω 0 L = ω =ω 0 πn =θ(t ) =ωt v c =gt t = v c g πn =ω v c g ω 0 L gπn =ω 0 gπn =ω0l gπn ω 0 = L ay =(vc f ) (vc) i gh =v c 0 look at the falling behavior ωl h = v c g = ω 0L 4 1 g = gπnl 8Lg = πnl 4 Page 7 of 8

Katharine Hyatt PHYS 1 (Prof. Oh ): Assignment 4 Solutions H + R 1.59 H + R 1.60 We realize that the ball stops slipping when the rolling condition is met, when ωr = v We see that the only torque on the ball comes from friction: And the ball is decelerating linearly due to friction: τ =Iα fr = mr α 5 α = 5µmgR mr = 5µg R ω =αt = 5µg R v =v 0 µmgt ωr =v 0 µgt 5µgT =v 0 µgt 7µgT =v 0 T = v 0 7µg We can check our units - ms 1 m 1 s = s so our units make sense. K + K 6.35 As the block rocks sideways without slipping, the point of contact between it and the sphere is Rθ. As long as the centre of mass is inside the Rθ envelope (closer to the vertical than Rθ) then the block won t fall off. If the centre of mass obeys this condition, a restoring torque exists. If the centre of mass doesn t obey the condition, a restorting torque is impossible. Assuming that R L, the block will be unstable if: Rθ < L tan θ R <L < L θ for small angles Page 8 of 8