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The value of acceleration due to gravity...

The value of acceleration due to gravity on the surface of earth is `x`. At an altitude of `h` from the surface of the earth, its value is `y`. If `R` is the radius of earth, then the value of `h` is

A

`(sqrt(x/y)-1)R`

B

`(sqrt(y/x)-1)R`

C

`sqrt(y/x)R`

D

`sqrt(x/y)R`

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The correct Answer is:
To solve the question, we need to find the height \( h \) at which the acceleration due to gravity changes from \( x \) (on the surface of the Earth) to \( y \) (at height \( h \)). The formula for gravitational acceleration at a distance \( r \) from the center of the Earth is given by: \[ g = \frac{GM}{r^2} \] Where: - \( G \) is the universal gravitational constant, - \( M \) is the mass of the Earth, - \( r \) is the distance from the center of the Earth. 1. **Gravitational acceleration on the surface of the Earth:** \[ x = \frac{GM}{R^2} \quad \text{(where \( R \) is the radius of the Earth)} \] 2. **Gravitational acceleration at height \( h \):** \[ y = \frac{GM}{(R + h)^2} \] 3. **Setting up the equations:** We have two equations: - Equation 1: \( x = \frac{GM}{R^2} \) - Equation 2: \( y = \frac{GM}{(R + h)^2} \) 4. **Dividing Equation 1 by Equation 2:** \[ \frac{x}{y} = \frac{(R + h)^2}{R^2} \] 5. **Cross-multiplying:** \[ x \cdot R^2 = y \cdot (R + h)^2 \] 6. **Taking the square root of both sides:** \[ \sqrt{\frac{x}{y}} = \frac{R + h}{R} \] 7. **Rearranging the equation:** \[ R + h = R \cdot \sqrt{\frac{x}{y}} \] 8. **Solving for \( h \):** \[ h = R \cdot \sqrt{\frac{x}{y}} - R \] \[ h = R \left( \sqrt{\frac{x}{y}} - 1 \right) \] Thus, the value of \( h \) is: \[ h = R \left( \sqrt{\frac{x}{y}} - 1 \right) \]

To solve the question, we need to find the height \( h \) at which the acceleration due to gravity changes from \( x \) (on the surface of the Earth) to \( y \) (at height \( h \)). The formula for gravitational acceleration at a distance \( r \) from the center of the Earth is given by: \[ g = \frac{GM}{r^2} \] Where: - \( G \) is the universal gravitational constant, ...
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