Physics 207, Lecture 5, Sept. 20 Agenda Chapter 4

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Physics 207, Lecture 5, Sept. 20 Agenda Chapter 4 Kinematics in 2 or 3 dimensions Independence of x, y and/or z components Circular motion Curved paths and projectile motion Frames of reference Radial and tangential acceration Assignment: For Monday read Chapter 5 and look at Chapter 6 WebAssign Problem Set 2 due Tuesday next week (start ASAP) 1

Chapter 4: Motion in 2 (and 3) dimensions 3-D Kinematics See text: 4-1 Chapter 4: Motion in 2 (and 3) dimensions 3-D Kinematics The position, velocity, and acceleration of a particle in 3-dimensions can be expressed as: r = x i + y j + z k v = vx i + vy j + vz k (i , j , k unit vectors ) a = ax i + ay j + az k Which can be combined into the vector equations: r = r(t) v = dr / dt a = d2r / dt2

Instantaneous Velocity The instantaneous velocity is the limit of the average velocity as ∆t approaches zero The direction of the instantaneous velocity is along a line that is tangent to the path of the particle’s direction of motion. The magnitude of the instantaneous velocity vector is the speed. (The speed is a scalar quantity) v

Average Acceleration The average acceleration of a particle as it moves is defined as the change in the instantaneous velocity vector divided by the time interval during which that change occurs. The average acceleration is a vector quantity directed along ∆v

Instantaneous Acceleration The instantaneous acceleration is the limit of the average acceleration as ∆v/∆t approaches zero The instantaneous acceleration is a vector with components parallel (tangential) and/or perpendicular (radial) to the tangent of the path Changes in a particle’s path may produce an acceleration The magnitude of the velocity vector may change The direction of the velocity vector may change (Even if the magnitude remains constant) Both may change simultaneously (depends: path vs time)

Motion along a path ( displacement, velocity, acceleration ) 3-D Kinematics : vector equations: r = r(t) v = dr / dt a = d2r / dt2 y v2 Velocity : v = dr / dt vav = r / t path v2 v1 -v1 v Acceleration : a = dv / dt aav = v / t x

General 3-D motion with non-zero acceleration: v a = + path and time t a a a = 0 Two possible options: Change in the magnitude of v a = 0 Change in the direction of v a = 0 Animation Uniform Circular Motion is one specific case:

Uniform Circular Motion See text: 4-4 Uniform Circular Motion What does it mean ? How do we describe it ? What can we learn about it ?

Average acceleration in UCM: See text: 4-4 Average acceleration in UCM: Even though the speed is constant, velocity is not constant since the direction is changing: must be some acceleration ! Consider average acceleration in time t aav = v / t v -v1 v2 v2 R v1 seems like v (hence v/t ) points toward the origin !

Instantaneous acceleration in UCM: See text: 4-4 Instantaneous acceleration in UCM: Again: Even though the speed is constant, velocity is not constant since the direction is changing. As t goes to zero in v / t dv / dt = a a = dv / dt R Now a points in the - R direction.

Acceleration in UCM: This is called Centripetal Acceleration. Calculating the magnitude: |v1| = |v2| = v Similar triangles: v1 v2 v But R = vt for small t v2 v1 R So: R

Period and Frequency  = 2 / T = 2f Recall that 1 revolution = 2 radians Period (T) = seconds / revolution = distance / speed = 2pR / v Frequency (f) = revolutions / second = 1/T (a) Angular velocity () = radians / second (b) By combining (a) and (b)  = 2 f Realize that: Period (T) = seconds / revolution So T = 1 / f = 2/ R v s  v R s  = 2 / T = 2f

Recap: Centripetal Acceleration See text: 4-4 Recap: Centripetal Acceleration UCM results in acceleration: Magnitude: a = v2 / R =  R Direction: - r (toward center of circle) a R 

Lecture 5, Exercise 1 Uniform Circular Motion A fighter pilot flying in a circular turn will pass out if the centripetal acceleration he experiences is more than about 9 times the acceleration of gravity g. If his F18 is moving with a speed of 300 m/s, what is the approximate radius of the tightest turn this pilot can make and survive to tell about it ? (Let g = 10 m/s2) (a) 10 m (b) 100 m (c) 1000 m (d) 10,000 m UCM (recall) Magnitude: a = v2 / R Direction: (toward center of circle)

Lecture 5, Exercise 1 Solution Answer (c)

Example: Newton & the Moon What is the acceleration of the Moon due to its motion around the earth? T = 27.3 days = 2.36 x 106 s (period ~ 1 month) R = 3.84 x 108 m (distance to moon) RE = 6.35 x 106 m (radius of earth) R RE

Moon... Calculate angular frequency: So  = 2.66 x 10-6 rad s -1. Now calculate the acceleration. a = 2R = 0.00272 m/s2 = .000278 g direction of a is toward center of earth (-R ).

Radial and Tangential Quantities For uniform circular motion v a

Radial and Tangential Quantities What about non-uniform circular motion ? v a aq is along the direction of motion ar is perpendicular to the direction of motion

Lecture 5, Exercise 2 The Pendulum q = 30° Which statement best describes the motion of the pendulum bob at the instant of time drawn ? the bob is at the top of its swing. which quantities are non-zero ? 1m A) vr = 0 ar = 0 vq  0 aq  0 B) Vr = 0 ar  0 vq  0 aq = 0 C) vr = 0 ar  0 vq = 0 aq  0

Lecture 5, Exercise 2 The Pendulum Solution NOT uniform circular motion : is circular motion so must be ar not zero, Speed is increasing so aq not zero q = 30° 1m a At the top of the swing, the bob temporarily stops, so v = 0. aq ar C) vr = 0 ar  0 vq = 0 aq  g In the next lecture we will learn about forces and how to calculate just what a is.

Relative motion and frames of reference Reference frame S is stationary Reference frame S’ is moving at vo This also means that S moves at – vo relative to S’ Define time t = 0 as that time when the origins coincide

Relative Velocity Two observers moving relative to each other generally do not agree on the outcome of an experiment For example, observers A and B below see different paths for the ball

Relative Velocity, equations The positions as seen from the two reference frames are related through the velocity r’ = r – vo t The derivative of the position equation will give the velocity equation v’ = v – vo These are called the Galilean transformation equations

y(t) motion governed by 1) a = -g y 2) vy = v0y – g t Central concept for problem solving: “x” and “y” components of motion treated independently. Again: man on the cart tosses a ball straight up in the air. You can view the trajectory from two reference frames: y(t) motion governed by 1) a = -g y 2) vy = v0y – g t 3) y = y0 + v0y – g t2/2 Reference frame on the moving train. x motion: x = vxt Reference frame on the ground. Net motion: R = x(t) i + y(t) j (vector)

Acceleration in Different Frames of Reference The derivative of the velocity equation will give the acceleration equation v’ = v – vo a’ = a The acceleration of the particle measured by an observer in one frame of reference is the same as that measured by any other observer moving at a constant velocity relative to the first frame.

Lecture 5, Exercise 3 Relative Motion You are swimming across a 50 m wide river in which the current moves at 1 m/s with respect to the shore. Your swimming speed is 2 m/s with respect to the water. You swim across in such a way that your path is a straight perpendicular line across the river. How many seconds does it take you to get across? a) b) c) d) 2m/s 1m/s 50m

Lecture 5, Exercise 3 Solution y x Choose x axis along riverbank and y axis across river The time taken to swim straight across is (distance across) / (vy ) Since you swim straight across, you must be tilted in the water so that your x component of velocity with respect to the water exactly cancels the velocity of the water in the x direction: 1m/s y x 2m/s m/s

Lecture 5, Exercise 3 Solution The y component of your velocity with respect to the water is The time to get across is y x 50m m/s Answer (c)

Recap First mid-term exam in just two weeks, Thursday Oct. 5 Chapter 4 Kinematics in 2 or 3 dimensions Independence of x, y and/or z components Circular motion Curved paths and projectile motion Frames of reference Radial and tangential acceration Assignment: For Monday read Chapter 5 and look at Chapter 6 WebAssign Problem Set 2 due Tuesday next week (start ASAP) 1