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Circular Motion

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... time it takes an object in uniform circular motion to complete one revolution of the circle. ... a) Draw a picture showing the way the two vectors add together ... – PowerPoint PPT presentation

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Title: Circular Motion


1
Circular Motion
  • Angular Acceleration

2
Distance around a Circle
  • Circumference
  • Distance around a circle

r
3
Period and Frequency
  • The period is the time it takes an object in
    uniform circular motion to complete one
    revolution of the circle.
  • The frequency is how many revolutions an object
    in uniform circular motion completes in one
    period.
  • Relationship between period and frequency
  • T1/f
  • F1/T (unit are hertz, Hz, which is 1/second)

4
Speed, Velocity, Angular Velocity
W.S. Ratios cmtp 7
  • Omegar ?r

5
Centripetal Acceleration
  • Centripetal Acceleration
  • Acceleration due to the centripetal acceleration
  • If an object is moving in a circular motion, it
    is experiencing centripetal acceleration relative
    to the plane of circular motion.

6
Centripetal Force
  • A way to describe what a force is doing. Normal
    force, gravity, tension - each of these forces
    can be a centripetal force if it is causing an
    object to move in uniform circular motion.  

7
Centripetal Acceleration vs. Acceleration of
Gravity
  • G-force, how many gs
  • Multiple of gravity,
  • Vacuum at 600rpm, r 10cm
  • Find T in seconds or f in Hz
  • Centrifuge at 2000rpm, r 15cm
  • Find T in seconds or f in Hz

8
Relative Motion
  • Velocity of A relative to B
  • Velocity of B relative to C
  • Velocity of A relative to C
  • Must add Velocity of A (relative to B) and
    Velocity of B (relative to C) together.

9
Vector Math
  • a) Draw a picture showing the way the two
    vectors add together
  • b) Break any vectors at angles into x and y
    components
  • c) Add the x components to find the total
    displacement component along that axis
  • d) Add the y components to find the total
    displacement component along that axis
  • e) Add the total x and y components to find the
    total displacement
  • Show work for each step.

10
(No Transcript)
11
Planet Avg Radius Period (T) Angular acceleration
Mercury 57.9 0.241 39.4
Venus
Earth 150 1 5.92
Mars
Jupiter 778 11.9 0.217
Saturn
Uranus
Neptune
Pluto 5890 248 0.0038
12
Centripetal acceleration vs. mean radius
13
Centripetal acceleration vs. mean radius
14
Centripetal Force
  • Q No force is required for an object to move in
    uniform circular motion. After all, its speed is
    constant.
  • A Speed is constant, but its velocity is
    changing due to its change in direction, which
    means it is accelerating. By Newtons second law,
    this means there must be a net force causing this
    acceleration.

15
Summary
  • Uniform circular motion is movement in a circle
    at a constant speed. But while speed is constant
    in this type of motion, velocity is not. Since
    instantaneous velocity in uniform circular motion
    is always tangent to the circle, its direction
    changes as the object's position changes.

16
Summary
  • The period is the time it takes an object in
    uniform circular motion to complete one
    revolution of the circle.
  • The frequency is how many revolutions an object
    in uniform circular motion completes in one
    period.
  • T1/f
  • F1/T

17
Summary
  • Since the velocity of an object moving in uniform
    circular motion changes, it is accelerating. The
    acceleration due to its change in direction is
    called centripetal acceleration. For uniform
    circular motion, the acceleration vector has a
    constant magnitude and always points toward the
    center of the circle.

18
Summary
  • Newton's second law can be applied to an object
    in uniform circular motion. The net force causing
    centripetal acceleration is called a centripetal
    force. Like centripetal acceleration, it is
    directed toward the center of the circle.

19
Summary
  • A centripetal force is not a new type of force
    rather, it describes a role that is played by one
    or more forces in the situation, since there must
    be some force that is changing the velocity of
    the object. For example, the force of gravity
    keeps the Moon in a roughly circular orbit around
    the Earth, while the normal force of the road and
    the force of friction combine to keep a car in
    circular motion around a banked curve.

20
Homework
  • Chapter 6
  • Projectile Motion
  • 4, 5, 6, 10
  • 32, 34, 35, 36, 45, 61, 63, 64,65
  • When calculating time an object is in the air,
    consider the final height or displacement in the
    y direction. That is, how high is it when it is
    laying on the ground.
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