SIMPLE PENDULUM ON SUN
INTRODUCTION
Sun
is our star in the center of our solar system. Consider a fire resistant
pendulum on the surface of Sun ready to swing. A pendulum is a weight suspended
from a pivot so that it can swing freely. It has a bob [mass] suspended from a
frictionless pivot via a string. The central position of the bob i.e. when the
pendulum is at rest is called its Mean position. When the bob is made to swing
on the application of external force, it oscillates back and forth about this
mean position. The maximum distance traversed by the bob from the mean position
is known as amplitude. The amplitude is measured in radians which is a unit of
angle. The time taken by the pendulum to complete one full oscillation is
called the Time Period. For small amplitude less than 1 radian, the time period
is independent of amplitude of the pendulum. We intend to determine the time
period of such a pendulum on Sun.
ASSUMPTIONS
1. The string has no tension or compression
2. The pendulum is indestructible and it is immune to destruction by
gravity, high temperature or solar winds
3. Air and wind resistance are negligible
4. Effect of Gravitational Time dilation is negligible
CALCULATION
The
time period of a simple pendulum is given by,
T =
2π*√ (l/g) (Eqn. 1)
Where,
T –
Time period [s]
l –
Length of the pendulum [m]
g –
Acceleration due to gravity on Sun [m/s2]
g =
273.7 m/s2 (Eqn. 2)
Let
the length of pendulum be
l =
1 m (Eqn.
3)
Now
substitute equations (2), (3) in equation (1)
T = 2π*√ (1/273.7)
T = 2π*√ (3.6536*10-3)
T = 2π*0.0604
T = 0.3797 s (Eqn.
4)
This
is the time period of a simple pendulum on Sun. It means any pendulum
performing small oscillations will always take approximately 1/3 second to
complete one cycle anywhere on Sun provided the value of gravity is same
everywhere and the effects of friction are neglected. Due to high gravity of
Sun, the time period is extremely small, way smaller than that on Earth and
Jupiter.
CONCLUSION
We
thus determined the time period of a simple pendulum on Sun.
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