



To understand how acceleration due to gravity changes with depth and height relative to Earth's surface, we analyze two key scenarios.
1. Acceleration at Depth (gdepth):
The acceleration due to gravity at depth $d$ below Earth's surface is given by:
$ g_{\text{depth}} = g_{\text{surface}} \left( 1 - \frac{d}{R} \right) $
where:
- $g_{\text{surface}}$ = surface gravity (9.8 m/s²)
- $R$ = Earth's radius
- $d$ = depth below surface
This can alternatively be expressed as:
$ g_{\text{depth}} = g_{\text{surface}} \left( \frac{r}{R} \right) $
where $r = R - d$ is the distance from Earth's center.
2. Acceleration at Height (gheight):
For height $h$ above the surface:
$ g_{\text{height}} = g_{\text{surface}} \left( \frac{R^2}{(R + h)^2} \right) $
3. Key Observations:
a) At Earth's center ($d = R$):
$ g_{\text{depth}} = 0 $ (gravity cancels out)
b) At surface ($d = 0$):
$ g_{\text{depth}} = g_{\text{surface}} $ (maximum value)
c) Above surface ($h > 0$):
Gravity decreases with height as the denominator $(R + h)^2$ grows.
4. Conclusion:
Gravity increases linearly from center to surface, then decreases inversely with square of distance above surface. The governing equations are:
For depth: $ g_{\text{depth}} = g_{\text{surface}} \left( 1 - \frac{d}{R} \right) $
For height: $ g_{\text{height}} = g_{\text{surface}} \left( \frac{R^2}{(R + h)^2} \right) $
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:
A small point of mass \(m\) is placed at a distance \(2R\) from the center \(O\) of a big uniform solid sphere of mass \(M\) and radius \(R\). The gravitational force on \(m\) due to \(M\) is \(F_1\). A spherical part of radius \(R/3\) is removed from the big sphere as shown in the figure, and the gravitational force on \(m\) due to the remaining part of \(M\) is found to be \(F_2\). The value of the ratio \( F_1 : F_2 \) is: 