Assume that the Earth is a solid sphere of uniform density and a tunnel is dug along its diameter. When a particle is released in this tunnel, it executes a simple harmonic motion. The mass of the particle is 100g. The time period of the motion of the particle will be (approximately):
A
24hours
B
1hour24minutes
C
1hour40minutes
D
12hours
Answer
Correct answer:B
Step-by-step solution
Standard Method
Given: Earth is assumed to be a uniform solid sphere, a tunnel is dug along its diameter, and the particle mass is 100g.
Find: The time period of oscillation inside the Earth.
At a distance x from the centre of the Earth, the gravitational field inside a uniform sphere is proportional to displacement:
E=R3GMx
Hence the acceleration of the particle is directed toward the centre:
a=−R3GMx
This is the condition for simple harmonic motion, so
ω=R3GM
Using g=R2GM,
ω=Rg
Therefore,
T=ω2π=2πgR
Now substitute R=6400×103m and g=10m/s2:
T=2×3.14×106400×103=2×3.14×800s
So,
T≈5026s
which is approximately 1hour24minutes.
Therefore, the correct option is B.
Using the SHM result inside a uniform sphere
Given: Motion of a particle through a diameter tunnel inside a uniform Earth.
Find: The approximate time period.
For SHM inside the Earth, the effective force is proportional to displacement:
F=−R3GMr
and therefore
a=mF=−R3GMr
So the time period is
T=2πGMR3
Using
g=R2GM
we get
T=2πgR
Now take
R=6400km=6.4×106m
and
g=10m/s2
Then
T=2π106.4×106=2π6.4×105T≈2π×800=5026s
This is approximately 1hour24minutes.
The particle mass does not affect the time period. Although one the solution marks option A, the worked numerical result clearly matches 1hour24minutes, so the correct option is B.
Common mistakes
Using the mass 100g in the time-period calculation. This is wrong because for SHM inside a uniform sphere, the acceleration is independent of the particle mass. Use T=2πgR only.
Assuming the gravitational field inside the Earth is constant and equal to surface gravity everywhere. This is wrong because inside a uniform sphere the field varies linearly with displacement from the centre. Use the restoring acceleration proportional to x.
Using the outside-Earth gravitational formula directly for the entire motion. That formula applies outside or at the surface, not inside the sphere. For motion through the tunnel, use the inside-sphere relation a∝−x.
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