Step 1: Understanding the Concept:
The acceleration due to gravity ($g$) varies with both height above the surface and depth below the surface.
As you go deeper into the Earth, the mass of the "shell" above you does not exert a net gravitational force. Only the mass within a sphere of your current radius counts.
This leads to a linear decrease in gravity as depth increases.
Step 2: Key Formula or Approach:
The formula for gravity at a depth $d$ is:
\[ g_d = g \left( 1 - \frac{d}{R} \right) \]
where $g$ is gravity at the surface, $d$ is depth, and $R$ is the radius of the Earth.
Detailed Explanation:
The problem states that at depth $d$, the gravity is half of its surface value:
\[ g_d = \frac{g}{2} \]
Substitute this into the formula:
\[ \frac{g}{2} = g \left( 1 - \frac{d}{R} \right) \]
Dividing both sides by $g$:
\[ \frac{1}{2} = 1 - \frac{d}{R} \]
Rearranging the terms:
\[ \frac{d}{R} = 1 - \frac{1}{2} \]
\[ \frac{d}{R} = \frac{1}{2} \]
\[ d = \frac{R}{2} \]
Thus, at a depth equal to half of the Earth's radius, gravity becomes half.
Step 3: Final Answer:
The required depth is $\frac{R}{2}$.