Chapter 8. Accelerated Circular Motion

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Chapter 8 Accelerated Circular Motion

8.1 Rotational Motion and Angular Displacement A new unit, radians, is really useful for angles. Radian measure θ(radians) = s = rθ s (arc length) r (radius) (s in same units as r) θ s r Full circle θ = s r = 2π r r = 2π (radians) Conversion of degree to radian measure θ(rad) = θ(deg.) 2π 360 2π 360 rad deg. = 1 rad deg.

8.1 Rotational Motion and Angular Displacement Example: Adjacent Synchronous Satellites Synchronous satellites are put into an orbit whose radius is 4.23 10 7 m. If the angular separation of the two satellites is 2.00 degrees, find the arc length that separates them. Convert degree to radian measure 2.00deg Determine arc length 2π rad 360deg s = rθ = 4.23 10 7 m = 0.0349 rad ( ) 0.0349 rad = 1.48 10 6 m (920 miles) ( )

8.1 Rotational Motion and Angular Displacement For an observer on the earth, an eclipse can occur because angles subtended by the sun and the moon are the same. θ = s Sun r Sun s Moon r Moon 9.3 mrad

8.1 Rotational Motion and Angular Displacement The angle through which the object rotates is called the angular displacement vector Δθ = θ θ o SI unit of angular displacement, radian (rad) Simplified using θ o = 0, and Δθ = θ, angular displacement vector. r Δθ Vector Counter-clockwise is + displacement Clockwise is displacement θ 0 = 0

Clicker Question 8.1 Radian measure for angles Over the course of a day (twenty-four hours), what is the angular displacement of the second hand of a wrist watch in radians? a) 1440 rad b) 2880 rad c) 4520 rad d) 9050 rad e) 543,000 rad

Clicker Question 8.1 Radian measure for angles Over the course of a day (twenty-four hours), what is the angular displacement of the second hand of a wrist watch in radians? a) 1440 rad b) 2880 rad c) 4520 rad d) 9050 rad e) 543,000 rad Second hand makes 1 rev. in 1 minute. 1 day = (1 day)(60 min./hr)(24 hr/day) = 1440 min. # rev. = ( 1 rev./min. )(1440 min.) = 1440 rev. 1 rev. = 2π radians Total θ displacement = (2π rad/min.)(1440 min.) = 9048 rad

8.2 Angular Velocity and Angular Acceleration DEFINITION OF AVERAGE ANGULAR VELOCITY ω = Δθ Δt where Δt = t t o SI Unit of Angular Velocity: radian per second (rad/s) Δθ is the same at all radii. Δt is the same at all radii. ω = Δθ Δt is the same at all radii. r 2 r 1 Δθ in time Δt Δθ Angle change θ 0 = 0

8.2 Angular Velocity and Angular Acceleration ω Case 1: Constant angular velocity, ω. r ω = Δθ Δt Δθ = ω Δt Δθ θ 0 = 0 Example: A disk rotates with a constant angular velocity of +1 rad/s. What is the angular displacement of the disk in 13 seconds? How many rotations has the disk made in that time? Δθ = ω Δt = (+1 rad/s)(13 s) = +13 rad 2π radians = 1 rotation 2π rad/rot. n rot = Δθ 2π rad/rot. = 13 rad 6.3 rad/rot = 2.1 rot.

8.2 Angular Velocity and Angular Acceleration Case 2: Angular velocity, ω, changes in time. r ω Instantaneous angular velocity at time t. Δθ ω = lim Δt =0 Δt ω 0 DEFINITION OF AVERAGE ANGULAR ACCELERATION SI Unit of Angular acceleration: radian per second squared (rad/s 2 )

8.2 Angular Velocity and Angular Acceleration Example: A Jet Revving Its Engines As seen from the front of the engine, the fan blades are rotating with an angular velocity of 110 rad/s. As the plane takes off, the angular velocity of the blades reaches 330 rad/s in a time of 14 s. Rotation is clockwise (negative) Find the angular acceleration, assuming it to be constant. ( ) ( 110rad s) α = 330rad s 14 s = 16rad s 2

8.2 The Equations of Rotational Kinematics The equations of rotational kinematics for constant angular acceleration: ANGULAR ACCELERATION ANGULAR VELOCITY ω = ω 0 + αt θ = 1 2 ( ω 0 + ω ) t TIME ANGULAR DISPLACEMENT ω 2 = ω 0 2 + 2αθ θ = ω 0 t + 1 2 αt 2

8.2 The Equations of Rotational Kinematics

8.2 The Equations of Rotational Kinematics Reasoning Strategy 1. Make a drawing. 2. Decide which directions are to be called positive (+) and negative ( ). 3. Write down the values that are given for any of the five kinematic variables. 4. Verify that the information contains values for at least three of the five kinematic variables. Select the appropriate equation. 5. When the motion is divided into segments, remember that the final angular velocity of one segment is the initial angular velocity for the next. 6. Keep in mind that there may be two possible answers to a kinematics problem.

Clicker Question 8.2 Rotational motion kinematics Given the initial and final angular velocity of a disk and the total angular displacement of the disk, the angular acceleration of of the disk can be obtained with which single equation? a) ω = ω 0 + αt b) θ = 1 2 (ω + ω 0 )t c) θ = ω 0 t + 1 2 αt2 d) ω 2 = ω 0 2 + 2αθ e) none of the above

Clicker Question 8.2 Rotational motion kinematics Given the initial and final angular velocity of a disk and the total angular displacement of the disk, the angular acceleration of of the disk can be obtained with which single equation? a) ω = ω 0 + αt b) θ = 1 (ω + ω )t 2 0 c) θ = ω 0 t + 1 2 αt2 d) ω 2 = ω 2 0 + 2αθ e) none of the above No time given! ω 2 = ω 2 0 + 2αθ α = ω 2 2 ω 0 2θ

8.2 The Equations of Rotational Kinematics Example: A disk has an initial angular velocity of +375 rad/s. The disk accelerates and reaches a greater angular velocity after rotating ω through an angular displacement r of +44.0 rad. ω 0 If the angular acceleration has a constant value of +1740 rad/s 2, find the final angular velocity of the disk. Given: ω 0 = +375 rad/s,θ = +44 rad, α = 1740 rad/s 2 Want: final angular velocity, ω. No time! ω 2 = ω 0 2 + 2αθ = (375 rad/s) 2 + 2(1740 rad/s 2 )(+44 rad) ω = 542 rad/s

8.3 Angular Variables and Tangential Variables ω = angular velocity - same at all radii (radians/s) α = angular acceleration - same at all radii (radians/s 2 ) v T = tangential velocity - different at each radius a T = tangential acceleration - different at each radius Direction is tangent to circle at that θ v T = ωr a T = αr v T (m/s) ω (rad/s) r (m) a T (m/s 2 ) α (rad/s 2 ) r (m)

8.3 Angular Variables and Tangential Variables Example: A Helicopter Blade A helicopter blade has an angular speed of 6.50 rev/s and an angular acceleration of 1.30 rev/s 2. For point 1 on the blade, find the magnitude of (a) the tangential speed and (b) the tangential acceleration. Convert revolutions to radians ( )( 2" rad rev) = 40.8 rad s! = 6.50 rev s ( ) 2" rad rev! = 1.30 rev s 2 ( ) = 8.17 rad s 2 v T =!r = ( 40.8rad s) ( 3.00 m) = 122m s a T = "r = ( 8.17rad s 2 )( 3.00 m) = 24.5m s 2

8.3 Rolling Motion The tangential speed of a point on the outer edge of the tire is equal to the speed of the car over the ground. v = v T =!r a = a T =!r

8.3 Centripetal Acceleration with Tangential Acceleration r! a C v T =!r r! a!! a C! a T Uniform circular motion! in rad/s constant Non-uniform circular motion Changing ω = ω 0 + αt ( ) 2 a C = v 2 T r =!r r =! 2 r a T =!r a total = a C 2 +! 2 r 2

Chapter 4.5 Force Generating Uniform Circular Motion

4.5 Centripetal Force Newton s Second Law When a net external force acts on an object of mass m, the acceleration that results is directly proportional to the net force and has a magnitude that is inversely proportional to the mass. The direction of the acceleration is the same as the direction of the net force. Vector Equations

4.5 Centripetal Force Thus, in uniform circular motion there must be a net force to produce the centripetal acceleration. The centripetal force is the name given to the net force required to keep an object moving on a circular path. The direction of the centripetal force always points toward the center of the circle and continually changes direction as the object moves. F C = ma C = m v2 r Magnitudes

4.5 Centripetal Force Example: The Effect of Speed on Centripetal Force The model airplane has a mass of 0.90 kg and moves at constant speed on a circle that is parallel to the ground. The path of the airplane and the guideline lie in the same horizontal plane because the weight of the plane is balanced by the lift generated by its wings. Find the tension in the 17 m guideline for a speed of 19 m/s. Tension vector points inward! T = F C = m v2 r T

4.5 Centripetal Force Example: The Effect of Speed on Centripetal Force The model airplane has a mass of 0.90 kg and moves at constant speed on a circle that is parallel to the ground. The path of the airplane and the guideline lie in the same horizontal plane because the weight of the plane is balanced by the lift generated by its wings. Find the tension in the 17 m guideline for a speed of 19 m/s. Tension is the centripetal force necessary to maintain airplane in the circle T = F C = m v2 r engine keeps speed up wings keep it from falling Tension vector points inward! T

4.5 Centripetal Force Conceptual Example: A Trapeze Act In a circus, a man hangs upside down from a trapeze, legs bent over and arms downward, holding his partner. Is it harder for the man to hold his partner when the partner hangs straight down and is stationary or when the partner is swinging through the straight-down position? Tension in arms maintains circular motion but also must counter the gravitational force (weight)

4.5 Centripetal Force Conceptual Example: A Trapeze Act In a circus, a man hangs upside down from a trapeze, legs bent over and arms downward, holding his partner. Is it harder for the man to hold his partner when the partner hangs straight down and is stationary or when the partner is swinging through the straight-down position? Tension in arms maintains circular motion but also must counter the gravitational force (weight) F C = m v2 r F = +T W = F C T = W + F C v T v W = mg

4.5 Banked Curves On an unbanked curve, the static frictional force provides the centripetal force.

4.5 Banked Curves On a frictionless banked curve, the centripetal force is the horizontal component of the normal force. The vertical component of the normal force balances the car s weight. Compression of the banked road provides the normal force. The normal force pushes against the car to 1) support the weight and 2) provides the centripetal force required for the car to move in a circle.

4.5 Banked Curves F C = F N sin! = m v2 r Combining the two relationships can determine the speed necessary to keep the car on the track with the given angle

4.5 Artificial Gravity Example: Artificial Gravity At what speed must the surface of a space station move so that an astronaut experiences a normal force on the feet equal to the weight on earth? The radius is 1700 m. v = rg = ( 1700 m) ( 9.80m s 2 ) = 130 m/s

4.5 Vertical Circular Motion Normal forces are created by stretching of the hoop. v 3 2 must be > g r to stay on the track F N 4 = m v 2 4 r