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The value of ‘ g ’ at a particular point...

The value of ‘ g ’ at a particular point is `9.8 m//s^(2)` . Suppose the earth suddenly shrinks uniformly to half its present size without losing any mass. The value of ‘ g ’ at the same point (assuming that the distance of the point from the centre of earth does not shrink) will now be

A

`4.9 m//sec^(2)`

B

`3.1 m//sec^(2)`

C

`9.8 m//sec^(2)`

D

`19.6 m//sec^(2)`

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The correct Answer is:
To solve the problem, we need to understand how the gravitational acceleration \( g \) is affected by changes in the Earth's size while keeping its mass constant. ### Step-by-Step Solution: 1. **Understanding the formula for gravitational acceleration**: The gravitational acceleration \( g \) at a distance \( r \) from the center of a mass \( M \) is given by the formula: \[ g = \frac{GM}{r^2} \] where \( G \) is the gravitational constant. 2. **Initial conditions**: We are given that the value of \( g \) at a particular point is \( 9.8 \, \text{m/s}^2 \). This is calculated using the radius of the Earth \( R \) and the mass of the Earth \( M \). 3. **Change in Earth's size**: The problem states that the Earth shrinks uniformly to half its present size. This means the new radius \( r' \) is: \[ r' = \frac{R}{2} \] 4. **Mass remains constant**: The mass of the Earth remains the same, so \( M \) does not change. 5. **Calculating new gravitational acceleration**: We can now calculate the new gravitational acceleration \( g' \) at the same point (which is now at a distance \( R \) from the center of the Earth): \[ g' = \frac{GM}{(R)^2} \] Since the point is still at distance \( R \) from the center of the Earth, we can see that: \[ g' = \frac{GM}{R^2} \] 6. **Comparison of \( g \) and \( g' \)**: The original gravitational acceleration \( g \) was calculated at the radius \( R \): \[ g = \frac{GM}{R^2} \] Since the mass \( M \) and the distance \( R \) from the center of the Earth have not changed, we find that: \[ g' = g = 9.8 \, \text{m/s}^2 \] ### Conclusion: Thus, the value of \( g \) at the same point after the Earth shrinks to half its size (while keeping mass constant) remains the same: \[ g' = 9.8 \, \text{m/s}^2 \]
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