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Assuming the earth to be a uniform spher...

Assuming the earth to be a uniform sphere of mass M and radium R. which of the following graphs represents the variation of acceleration due to gravity with distance .r. from the centre of the earth.

A

B

C

D

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The correct Answer is:
To solve the problem of how the acceleration due to gravity (g) varies with distance (r) from the center of the Earth, we can break it down into two distinct regions: outside the Earth and inside the Earth. ### Step-by-Step Solution: 1. **Understanding the Problem**: - We need to analyze how the acceleration due to gravity changes as we move from the center of the Earth to a point outside its surface. 2. **Acceleration Outside the Earth** (r > R): - When we are outside the Earth (at a distance r from the center where r > R), we can treat the Earth as a point mass located at its center. - The formula for gravitational acceleration at a distance r from the center of a mass M is given by: \[ g = \frac{GM}{r^2} \] - Here, G is the gravitational constant, M is the mass of the Earth, and r is the distance from the center of the Earth. - As r increases, g decreases with the square of the distance (inversely proportional to \( r^2 \)). 3. **Acceleration At the Surface of the Earth** (r = R): - At the surface of the Earth (r = R), the acceleration due to gravity is: \[ g = \frac{GM}{R^2} \] 4. **Acceleration Inside the Earth** (r < R): - When we are inside the Earth (at a distance r from the center where r < R), we can use the concept of a uniform spherical shell. - According to the shell theorem, the gravitational force inside a uniform spherical shell is zero. Therefore, only the mass that is at a radius less than r contributes to the gravitational acceleration. - The effective mass \( m' \) that contributes to gravity at distance r is: \[ m' = \frac{4}{3} \pi r^3 \rho \] - Here, \( \rho \) is the density of the Earth. - The acceleration due to gravity inside the Earth is given by: \[ g' = \frac{G m'}{r^2} = \frac{G \left(\frac{4}{3} \pi r^3 \rho\right)}{r^2} = \frac{4}{3} \pi G \rho r \] - This shows that \( g' \) is directly proportional to r when r < R. 5. **Graphical Representation**: - From the analysis: - For r < R, g increases linearly with r. - For r = R, g reaches its maximum value. - For r > R, g decreases as \( \frac{1}{r^2} \). - Therefore, the graph of g vs. r will show a linear increase from the center to the surface, and then a decrease as we move away from the surface. 6. **Conclusion**: - The correct graph representing the variation of acceleration due to gravity with distance from the center of the Earth is option 2, which shows a linear increase up to R and then a decrease inversely proportional to \( r^2 \) beyond R.
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