Elastic collisions in two dimensions 5B

Similar documents
Elastic collisions in two dimensions 5A

Mixed Exercise 5. For motion parallel to the wall: For motion perpendicular to the wall:

( ) Momentum and impulse Mixed exercise 1. 1 a. Using conservation of momentum: ( )

Elastic collisions in one dimension Mixed Exercise 4

Elastic collisions in two dimensions 5C

Linear Momentum and Collisions Conservation of linear momentum

A level Exam-style practice

Applications of forces Mixed exercise 7

Elastic collisions in one dimension 4D

EVALUATE: If the angle 40 is replaces by (cable B is vertical), then T = mg and

( y) ( ) ( ) ( ) ( ) ( ) Trigonometric ratios, Mixed Exercise 9. 2 b. Using the sine rule. a Using area of ABC = sin x sin80. So 10 = 24sinθ.

A-level Mathematics. MM03 Mark scheme June Version 1.0: Final

Background Trigonmetry (2A) Young Won Lim 5/5/15

CJ57.P.003 REASONING AND SOLUTION According to the impulse-momentum theorem (see Equation 7.4), F t = mv

sin! =! d y =! d T ! d y = 15 m = m = 8.6 m cos! =! d x ! d x ! d T 2 =! d x 2 +! d y =! d x 2 +! d y = 27.2 m = 30.0 m tan! =!

Proof by induction ME 8

Chapter 11 Collision Theory

(a)!! d = 17 m [W 63 S]!! d opposite. (b)!! d = 79 cm [E 56 N] = 79 cm [W 56 S] (c)!! d = 44 km [S 27 E] = 44 km [N 27 W] metres. 3.

( ) Applications of forces 7D. 1 Suppose that the rod has length 2a. Taking moments about A: acos30 3

Finds the value of θ: θ = ( ). Accept awrt θ = 77.5 ( ). A1 ft 1.1b

Your Thoughts. What is the difference between elastic collision and inelastic collision?

Review exercise 2. 1 The equation of the line is: = 5 a The gradient of l1 is 3. y y x x. So the gradient of l2 is. The equation of line l2 is: y =

Elastic strings and springs Mixed exercise 3

UNDERSTAND MOTION IN ONE AND TWO DIMENSIONS

Moments Mixed exercise 4

Physics Department Tutorial: Motion in a Circle (solutions)

OCR Maths M2. Topic Questions from Papers. Collisions

Physics Kinematics: Projectile Motion. Science and Mathematics Education Research Group

Physics 4A Solutions to Chapter 4 Homework

ENGINEERING COUNCIL DYNAMICS OF MECHANICAL SYSTEMS D225 TUTORIAL 3 CENTRIPETAL FORCE

Q Scheme Marks AOs. 1a States or uses I = F t M1 1.2 TBC. Notes

Blue and purple vectors have same magnitude and direction so they are equal. Blue and green vectors have same direction but different magnitude.

Q Scheme Marks AOs Pearson. Notes. Deduces that 21a 168 = 0 and solves to find a = 8 A1* 2.2a

, remembering that! v i 2

Get Solution of These Packages & Learn by Video Tutorials on PROJECTILE MOTION

A. unchanged increased B. unchanged unchanged C. increased increased D. increased unchanged

Q Scheme Marks AOs Pearson ( ) 2. Notes. Deduces that 21a 168 = 0 and solves to find a = 8 A1* 2.2a

( ) Trigonometric identities and equations, Mixed exercise 10

Exam-style practice: Paper 3, Section A: Statistics

Conservation of Momentum in Two Dimensions

Trigonometry and modelling 7E

h (1- sin 2 q)(1+ tan 2 q) j sec 4 q - 2sec 2 q tan 2 q + tan 4 q 2 cosec x =

Mark scheme Mechanics Year 1 (AS) Unit Test 7: Kinematics 1 (constant acceleration)

Advanced/Advanced Subsidiary. You must have: Mathematical Formulae and Statistical Tables (Pink)

Version 1.0. General Certificate of Education (A-level) June Mathematics MM03. (Specification 6360) Mechanics 3. Final.

Draft Version 1 Mark scheme Further Maths Core Pure (AS/Year 1) Unit Test 1: Complex numbers 1

1. Linear Motion. Table of Contents. 1.1 Linear Motion: Velocity Time Graphs (Multi Stage) 1.2 Linear Motion: Velocity Time Graphs (Up and Down)

increases. In part (b) the impulse and initial momentum are in opposite directions and the velocity decreases.

i j k i j k i j k

b UVW is a right-angled triangle, therefore VW is the diameter of the circle. Centre of circle = Midpoint of VW = (8 2) + ( 2 6) = 100

Physics 1: Mechanics

Trigonometric Functions 6C

9 Mixed Exercise. vector equation is. 4 a

Constant acceleration, Mixed Exercise 9

FOCUS ON CONCEPTS Section 7.1 The Impulse Momentum Theorem

N12/4/PHYSI/SPM/ENG/TZ0/XX. Physics Standard level Paper 1. Tuesday 13 November 2012 (afternoon) 45 minutes INSTRUCTIONS TO CANDIDATES

Taylor Series 6B. lim s x. 1 a We can evaluate the limit directly since there are no singularities: b Again, there are no singularities, so:

PROBLEM rad/s r. v = ft/s

N10/4/PHYSI/SPM/ENG/TZ0/XX PHYSICS STANDARD LEVEL PAPER 1. Monday 8 November 2010 (afternoon) 45 minutes INSTRUCTIONS TO CANDIDATES

Unit 11: Vectors in the Plane

(a) Taking the derivative of the position vector with respect to time, we have, in SI units (m/s),

Physics 2A Chapter 3 - Motion in Two Dimensions Fall 2017

Conservation of Linear Momentum, Collisions

MATHEMATICS Unit Mechanics 3

Constant acceleration 9E

Math 104 Midterm 3 review November 12, 2018

α f k θ y N m mg Figure 1 Solution 1: (a) From Newton s 2 nd law: From (1), (2), and (3) Free-body diagram (b) 0 tan 0 then

Mark Schemes for "Solomon" M2 practice papers A to F

The Kinetic Theory of Gases

Lecture 12! Center of mass! Uniform circular motion!

Status: Unit 2, Chapter 3

Page 1. t F t m v. N s kg s. J F t SPH4U. From Newton Two New Concepts Impulse & Momentum. Agenda

Pearson Physics Level 20 Unit I Kinematics: Chapter 2 Solutions

Version 1.0. klm. General Certificate of Education June Mathematics. Mechanics 3. Mark Scheme

1a States correct answer: 5.3 (m s 1 ) B1 2.2a 4th Understand the difference between a scalar and a vector. Notes

Section 5.1: Momentum and Impulse Tutorial 1 Practice, page Given: m = 160 g = 0.16 kg;! v = 140 m/s [E] Required:! p ; E k

Rutgers University Department of Physics & Astronomy. 01:750:271 Honors Physics I Fall Lecture 4. Home Page. Title Page. Page 1 of 35.

Applications of forces 7C

Chapter 2: Motion in Two Dimensions

10.2,3,4. Vectors in 3D, Dot products and Cross Products

MEI Structured Mathematics. Module Summary Sheets. Mechanics 2 (Version B: reference to new book)

( ) ( ) ( ) ( ) ( ) ( ) ( ) ( ) Trigonometric ratios 9E. b Using the line of symmetry through A. 1 a. cos 48 = 14.6 So y = 29.

Mark Scheme (Results) Summer Home. GCE Mechanics M2 6678/01 Original Paper

Projectiles 6D. 1 At maximum height, h, the vertical component of velocity, vy = 0, a = g, s h, v 0 R( ) sin. v u 2as sin 2. U h. as required.

PhysicsAndMathsTutor.com

8.0 Definition and the concept of a vector:

MAGNETIC EFFECTS OF CURRENT-3

Kinematics - study of motion HIGHER PHYSICS 1A UNSW SESSION s o t See S&J , ,

DO PHYSICS ONLINE. WEB activity: Use the web to find out more about: Aristotle, Copernicus, Kepler, Galileo and Newton.

Simple Harmonic Motion Practice Problems PSI AP Physics B

Solutionbank Edexcel AS and A Level Modular Mathematics

Kinematics on oblique axes

Math 425 Lecture 1: Vectors in R 3, R n

The Elastic Pi Problem

Edexcel GCE Mechanics M1 Advanced/Advanced Subsidiary

Purpose of the experiment

University of Malta. Junior College

A Level. A Level Physics. MECHANICS: Momentum and Collisions (Answers) AQA, Edexcel, OCR. Name: Total Marks: /30

Exam Question 5: Work, Energy, Impacts and Collisions. June 18, Applied Mathematics: Lecture 5. Brendan Williamson.

Circles, Mixed Exercise 6

Transcription:

Elastic collisions in two dimensions 5B a First collision: e=0.5 cos α = cos30 () sin α = 0.5 sin30 () Squaring and adding equations () and () gies: cos α+ sin α = 4cos 30 + sin 30 (cos α+ sin α)= 4 3 4 + 4 = 3 4 = 3 =.80ms (3 s.f.) Diiding equation () by equation () gies: = 0.5 tan 30 = 3 α = 6. (3 s.f.) Pearson Education Ltd 08 Copying permitted for purchasing institution only. This material is not copyright free.

b Second collision: e=0.5 cosβ = cos(90 α) = sin α (3) sinβ = 0.5 sin(90 α) = 0.5 cos α (4) Squaring and adding equations (3) and (4) gies: cos β+ sin β = sin α+ 0.5 cos α As = 3, by Pythagoras sinα = 3 and cosα = 3 3 (cos β+ sin β)= 3 + 3 3 = 3 4 4 3 = =ms Diiding equation (4) by equation (3) gies: tanβ = 0.5 = 3 = 3 β= 60 Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free.

a First collision for motion parallel to the wall: cos0 = cos40 () = cos40 cos0 = 0.85ms (3 s.f.) b sin 0 = e sin 40 () Diiding equation () by equation () gies: tan 0 = etan 40 tan 0 e= = 0.434 (3 s.f.) tan 40 c Second collision for motion parallel to the wall: cosα = cos70 (3) sinα = e sin 70 (4) Diiding equation (4) by equation (3) gies: tan0 tan70 = e tan 70 = tan 40 but tan 0 tan70 = So = = tan(90 40 ) = tan 50 tan 40 α = 50 Substituting into equation (3) gies: cos50 = cos70 cos40 cos50 = cos70 cos0 but cos50 = sin 40 and cos70 = sin 0 cos40 sin 0 So = cos0 sin 40 tan 0 = = tan 40 0.434ms (3 s.f.) Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 3

3 a First collision let the angle the sphere makes with the wall after the collision be α 0.3cosα = 0.5cos30 () 0.5 3 cosα = = 0.9433 0.3 α = 9.7 (3 s.f.) After the impact with the first wall, the sphere moes at 9.7 to the wall b 0.3sinα = 0.5esin30 () Diiding equation () by equation () gies: = e tan 30 tan9.7 e= = = 0.6 (3 s.f.) tan30 tan30 c First collision let the angle the sphere makes with the wall after the collision be β and its speed after the collision be cosβ = 0.3cos(90 α) = 0.3sin α (3) sinβ = 0.3esin(90 α) = 0.3ecos α (4) Squaring and adding equations (3) and (4) gies: cos β + sin β = 0.3 sin α+ 0.3 e cos α (cos β+ sin β) = 0.3 ( cos α+ e cos α) = 0.059( 0.9433 + 0.6 0.9433 ) = 0.04 Kinetic energy after second collision m = = = 0. 0.04 0.00 J (3 s.f.) Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 4

4 a First collision let the angle the sphere makes with the wall after the collision be α, its speed before impact be u and its speed after impact Kinetic energy before first collision = u So u = 9 u= 3m s cos α = 3cos60 =.5 () sin α = 0.75 3sin 60 =.5 3 () Squaring and adding equations () and () gies: cos α+ sin α =.5+ 3.7969 (cos α+ sin α)= 6.0469 =.46ms (3 s.f.) Diiding equation () by equation () gies: = 0.75tan60 = 0.75 3 α = 5.4 (3 s.f.) b Second collision for motion parallel to the wall: cosβ = cos(90 α) = sin α (3) sinβ = 0.6 sin(90 α) = 0.6 cos α (4) Squaring and adding equations (3) and (4) gies: cos β + sin β = sin α+ 0.36 cos α (cos β+ sin β) = (sin α+ 0.36 cos α) = 6.0469(0.679+ 0.3395) = 4.60685 Kinetic energy after second collision = m = 4.60685= 4.6 J (3 s.f.) Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 5

5 First collision cosβ = ucos α () sinβ = eusin α () Diiding equation () by equation () gies: tanβ =e Second collision wcosθ = cos(90 β) = sin β (3) wsinθ = esin(90 β) = ecos β (4) Diiding equation (4) by equation (3) gies: e tanθ = tanβ = e e = = cotα = tan(90 α) So θ = 90 α, which means that after the collision with the second wall the sphere s path is parallel to its original path but in the opposite direction. Substituting for θ in equation (3) gies: wcosθ = wcos(90 α) = sinβ wsinα = sinβ So from equation () wsinα = sinβ = eusinα w= eu, the speed after the second collision Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 6

6 First impact: u cosα = ucos45 = () u sinα = eusin 45 = () 3 Squaring and adding equations () and () gies: cos α+ sin α =u + 6 = u 3 Diiding equation () by equation () gies: = α = 30 3 So 80 30 30 = 80 β β = 60 Second impact: wcosθ = cos60 = (3) wsinθ = esin60 = (4) Squaring and adding equations (3) and (4) gies: w cos θ + w sin θ = + 4 4 w u = = 3 u w= = 3 3u ms 3 Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 7

7 a First impact: cos α = 5cos30 () sin α = 0.8 5sin30 () Squaring and adding equations () and () gies: 3 cos α+ sin α = 5 + 6 4 4 9 = = 4.77ms (3 s.f.) 4 Diiding equation () by equation () gies: 4 = 0.8 tan 30 = α = 4.8 (3 s.f.) 5 3 b Second impact: cosβ = cos(45 + α ) (3) sinβ = 0.8 sin(45 + α ) (4) Diiding equation (4) by equation (3) gies: tanβ= 0.8tan(45 +α)=0.8tan(45 + 4.79 )=.733 β= 65.3 (3 s.f.) From equation (3) cos65.9 = cos(45 +α) = 4.77 cos69.79 cos65.9 = 3.94ms (3 s.f.) c If e > 0.8 and e remains unchanged, (45 + α) and do not change; howeer, tan β increases, so β increases and (which depends on and cos β) increases. So the elocity of the sphere after the second collision would be greater and the angle it makes with the wall after the collision would be greater. Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 8

8 a Since first collision causes no change to the i component, first collision must be with the wall parallel to this ector. Considering j components only for the first collision: =4e e= Considering only the i component changes for the second collision: 5=ep=p p=.5 ( u ) Loss of kinetic energy= m = m + + 4 = m 4 4 3 = m J 8 ((5 4 ) (.5 )) b Initial elocity, u = 5i 4j and final elocity, =.5i + j The coefficients of i and j hae the same ratio in both cases, but the signs of both are reersed: u and are therefore antiparallel. The sphere is deflected through a total angle of 80. 9 a First collision let the angle the sphere makes with the wall after the collision be α, and its speed after impact For motion parallel to wall: cos α =.5cos45 () For motion perpendicular to wall: sinα = 0.6.5sin45 () Diiding equation () by equation () gies: = 0.6 tan 45 5 = 0.6 cos α = 34 α = 30.964 = 3.0 (3 s.f.) Substituting into equation () gies: 5 34 = 5 = 7 =.065...=.06ms Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 9

9 b First collision let the angle the sphere makes with the wall after the collision be β, and its speed after impact For motion parallel to wall: cosβ= cos(60 α) (3) For motion perpendicular to wall: sinβ = 0.6 sin(60 α) (4) Diiding equation (4) by equation (3) gies: tanβ= 0.6 tan(60 30.964 )=0.33308... β=8.4 cosβ= 0.9488 Substituting into equation (3) gies: 7 0.9488= 0.8743=.8997 (4 d.p.) Kinetic energy after second collision= 0..8997 = 0.80 J (3 s.f.) Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free. 0

0 First collision For motion parallel to wall: cosα =0cos30 () For motion perpendicular to wall: sinα = 0.7 0sin30 () Diiding equation () by equation () gies: = 0.7tan30 7 0 3 = cosα = 0 3 349 α =.005 (3 d.p.) Substituting into equation () gies: 0 3 3 349 = 0 = 349 First collision For motion parallel to wall: cosβ= cos(80 75 α)= cos8.994 (3) For motion perpendicular to wall: sinβ = 0.5 sin(80 75 α)= 0.5 sin8.994 (4) Diiding equation (4) by equation (3) gies: tanβ= 0.5tan8.994 = 4.0687 β = 76.9 (3 d.p.) Substituting into equation (3) gies: 349 cos 76.9 = cos8.994 = 4.7736 Loss of kinetic energy= m(u ) = ( 0 4.7736 ) = 77. J (3 s.f.) Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free.

Challenge a i Vertical component of motion is not changed by collision with wall. Therefore time taken for ball to reach floor for the first time is time taken for ball to fall m from rest. s= ut+ at = 9.8 t t= = 0.4575... 4.9 Horizontal component of motion is 0 m s before collides with wall and 0.6 0 = m s after collision. So time taken to reach wall: s.4 t = = = 0. s 0 So time for which ball traelling at m s is t = 0.4575 0. = 0.33 75 Distance traelled in this time = t = 0.3375 = 3.98 m (3 s.f.) The ball first bounces on the floor 3.98 m from the wall. ii Vertical component of speed immediately before it hits the floor: =u + as = 9.8 = 9.6 Vertical component of speed immediately after it hits the floor = 0.6 9.6 Maximum height gien when ertical component is again zero, so: =u + as 0=(0.6 9.6) ( 9.8 s) s=0.6 = 0.36m The maximum height after this bounce is 0.36 m. b If the ball is hotter and e increases, the horizontal speed after hitting the wall will be greater and the ball will therefore trael further before hitting the floor. Similarly, the ertical component of the speed immediately after it hits the floor will be greater and the maximum height after the first bounce will also be greater. Pearson Education Ltd 08. Copying permitted for purchasing institution only. This material is not copyright free.