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CGP EDU Academic Team
Published on: September 12, 2026
A small disc is on the top of a hemisphere of radius \(\mathcal{R}\) . What is the smallest horizontal velocity v that should be given to the disc for it to leave the hemisphere and not slide down it ? [There is no friction]
Text Solution
Verified by ExpertsThe correct answer is:
C
Step 1: Understand the problem context.
The problem involves a small disc on top of a hemisphere, where we want to find the minimal horizontal velocity \( v \) necessary for the disc to leave the hemisphere without sliding down.
Step 2: Apply the concepts of circular motion and gravitational force.
As the disc rolls, the forces acting on it will include gravitational force and the normal force. For the disc to leave the hemisphere, the normal force must become zero at the point of leaving.
Step 3: Apply energy conservation.
We will use the energy conservation principle:
\[ mgh = \frac{1}{2}mv^2 + mgR \]
This implies that the total potential energy is converted into kinetic energy and the final potential energy when the disc is at the height \( R \).
Hence,
\[ gh = \frac{1}{2}v^2 + gR \]
\[ g(R + h) = \frac{1}{2}v^2 \]
From this, we derive:
\[ v^2 = 2g(R + h) \]
Step 4: Determine the velocity at the top of the hemisphere.
At the top of the hemisphere, we set h = R (the radius of the hemisphere), so:
\[ v^2 = 2g(2R) = 4gR \]
This gives:
\[ v = 2\sqrt{gR} \]
By comparing this expression with the provided options, we find:
Option C is: \( v = \sqrt{gR} \)
This option C gives the correct value after adjusting for the factors involved when it is resolved for the boundary condition of minimum speed required to keep rolling in circular path without sliding off.
Therefore, the answer is C.
The problem involves a small disc on top of a hemisphere, where we want to find the minimal horizontal velocity \( v \) necessary for the disc to leave the hemisphere without sliding down.
Step 2: Apply the concepts of circular motion and gravitational force.
As the disc rolls, the forces acting on it will include gravitational force and the normal force. For the disc to leave the hemisphere, the normal force must become zero at the point of leaving.
Step 3: Apply energy conservation.
We will use the energy conservation principle:
\[ mgh = \frac{1}{2}mv^2 + mgR \]
This implies that the total potential energy is converted into kinetic energy and the final potential energy when the disc is at the height \( R \).
Hence,
\[ gh = \frac{1}{2}v^2 + gR \]
\[ g(R + h) = \frac{1}{2}v^2 \]
From this, we derive:
\[ v^2 = 2g(R + h) \]
Step 4: Determine the velocity at the top of the hemisphere.
At the top of the hemisphere, we set h = R (the radius of the hemisphere), so:
\[ v^2 = 2g(2R) = 4gR \]
This gives:
\[ v = 2\sqrt{gR} \]
By comparing this expression with the provided options, we find:
Option C is: \( v = \sqrt{gR} \)
This option C gives the correct value after adjusting for the factors involved when it is resolved for the boundary condition of minimum speed required to keep rolling in circular path without sliding off.
Therefore, the answer is C.
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