Class 35: Uniform circular motion Acceleration in a circular motion a - - PowerPoint PPT Presentation

class 35 uniform circular motion acceleration in a
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Class 35: Uniform circular motion Acceleration in a circular motion a - - PowerPoint PPT Presentation

Class 35: Uniform circular motion Acceleration in a circular motion a t There will be a tangential acceleration (a t ) causing the v change in speed. a c d v a t d t R The centripetal acceleration depends only on v: 2 v R a R


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SLIDE 1

Class 35: Uniform circular motion

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SLIDE 2

There will be a tangential acceleration (at) causing the change in speed. The centripetal acceleration depends only on v:

Acceleration in a circular motion ac at R 

R v a

2 R 

v

t d v d a t 

There is centripetal acceleration for circular motion even when the speed is constant (circular motion with uniform speed).

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SLIDE 3

Speed = constant. Acceleration is along the radial direction (centripetal acceleration)

Uniform circular motion ac R 

R v a

2 R 

v

t d v d a t  

The net force must be acting radially inward to produce the centripetal acceleration (Newton’s second law).

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Common misconceptions

  • 1. Why won’t the object moves towards the center? – This won’t

happen because the tangential velocity keep it in the circular

  • rbit.
  • 2. Centripetal force is a kind of force – Centripetal force is a broad

term used to described the force that causes the centripetal

  • acceleration. It is not a special type of force. Instead, radial

component of any force (gravitational force, tension, normal force etc.) can be the centripetal force.

  • 3. In a circular motion there is a centrifugal force to balance out

the centripetal force so the object is in equilibrium – It is wrong to think of circular motion as equilibrium. In fact it is far from equilibrium and it needs an “unbalanced force” for the centripetal

  • acceleration. There is no such thing as centrifugal force in an

inertial frame.

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SLIDE 5

Uniform circular motion

 r v 

 v

1 T f 

f T

v r 2 T   f 2    You just need to know one, then all other three are known! Note: speed v does not need to be constant for circular motion.

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SLIDE 6

Uniform circular motion – Example 1

A planet is running around the sun of mass M in a circular

  • rbit of radius R. Determine the period of revolution. (This

result is a particular case of Kepler’s third law that leads Newton to discover the Law of Gravitation.)

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SLIDE 7

Uniform circular motion – Example 2

If the mass is running in a circle with an angular velocity , determine the angle . (This is called a conical pendulum.)

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Uniform circular motion – Example 3

In a circular track of radius R, the road is banked at an angle . A car is running on it with a velocity v without slipping. Calculate the friction.

R v