Notes on Simple Pendulum and Harmonic Motion, Study notes of Physics

Notes on the behavior of a simple pendulum, which can be described as undergoing simple harmonic motion under certain conditions. The decomposition of weight into components along and perpendicular to the string, the equations of motion, and energy concerns for the pendulum. It also includes examples to calculate the value of gravity and the frequency of a pendulum on earth and the moon.

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Pre 2010

Uploaded on 08/30/2009

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Lecture 34 Page 1
PHYSICS 151 – Notes for Online Lecture #24
Pendula
A simple pendulum
consists of an object
suspended from a string.
The motion of the
pendulum swinging back
and forth can also be
described by simple
harmonic motion (under
certain conditions).
θ
L
T
mg θmg cos(θ)
mg sin(θ)
let’s first draw a free-body diagram for the bob on the pendulum. We can decompose the weight, mg, into a component
along the direction of the string and a component perpendicular to the string.
The component of the weight in the direction of the string will be:
mg cos)
The component of the weight perpendicular to the string is
-mg sin(θ)
Write Σ
G
F=0. We have to write one equation for each direction.
Along the string Perpendicular to the string
In the direction along the string, there is no acceleration,
so taking toward the pivot as positive,
Σ
G
F
Tmg
Tmg
alongthestring =
−=
=
0
0cos( )
cos( )
θ
θ
There is, however, acceleration in the direction
perpendicular to the string due to the unbalanced force:
Σ
G
Fma
Fmg
perpendicular to thestring =
=− sin( )θ
One of the things we learned in the last lecture, is that object that undergo simple harmonic motion following something
that looks like Hooke’s law, with the force proportional to the displacement. This equation doesn’t look like Hooke’s law.
pf3
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PHYSICS 151 – Notes for Online Lecture

Pendula A simple pendulum consists of an object suspended from a string. The motion of the pendulum swinging back and forth can also be described by simple harmonic motion (under certain conditions).

θ

L

T

mg θ^ mg cos( θ)

mg sin( θ)

let’s first draw a free-body diagram for the bob on the pendulum. We can decompose the weight, mg, into a component along the direction of the string and a component perpendicular to the string. The component of the weight in the direction of the string will be: mg cos) The component of the weight perpendicular to the string is

-mg sin(θ)

Write Σ

G

F = 0. We have to write one equation for each direction. Along the string Perpendicular to the string In the direction along the string, there is no acceleration, so taking toward the pivot as positive, Σ

G

F

T mg T mg

along the string = − = =

cos( ) 0 cos( )

θ θ

There is, however, acceleration in the direction perpendicular to the string due to the unbalanced force: Σ

G

F ma F mg

perpendicular to the string = = − sin( )θ

One of the things we learned in the last lecture, is that object that undergo simple harmonic motion following something that looks like Hooke’s law, with the force proportional to the displacement. This equation doesn’t look like Hooke’s law.

L

L

L

If θ is very small, we can make an approximation. If we let s be the displacement of the pendulum bob, s will be an arc. If

θ is small, we can write that sin θ = s L We can then write F mg

F mg s L F mg L

s

sin( )θ

so that the ‘spring constant’ for this problem is

F mg L

s

F mg L

s

F k s

= −FHG IKJ

where the effective spring constant is given by

k mg L

We can use the same relationships we derived for the mass on a spring to find the similar quantities for the pendulum

Spring Pendulum f k m

2 π

f g L

2 π

T f

m k

= 1 = 2 π T f

L

g

= 1 = 2 π

Note that, for the pendulum, all of these results are independent of the mass of the pendulum.

Ex. 24-2 : A pendulum with a frequency of 6 oscillations per second is taken to the moon, where gravity is 1/6th^ the gravity of earth. What will the pendulum’s frequency be on the moon?

Solution: The pendulum length is constant.

f g L

f g L f g L L g f

L g f

2

2

2 2

π

π

π

π

π

b g

b g

b g

Earth Moon L g f

Earth Earth

4 π 2 b g^2

L g f

Moon Moon

4 π 2 b g^2

These two must be equal, so

L g f

g f g f

g f g f f g

f f g g

f f g g

f f

g g

f f

f Hz Hz

Earth Earth

Moon Moon Earth Earth

Moon Moon Earth Moon Earth Moon

Moon Earth Moon Earth

Moon Earth Moon Earth

Moon Earth

Earth Earth

Moon Earth

Moon

2 2 2 2

2 2 2 2

2 2

(^16)

π b g π b g

b g b g

b g b g

b g b g