Step 1: Relation of gravity inside the earth.
For a sphere of uniform density, acceleration due to gravity at a distance \(r\) from the centre is directly proportional to \(r\):
\[
g(r) \propto r
\]
Step 2: Gravity at the earth’s surface.
At the surface, \(r = R\), so
\[
g_{\text{surface}} \propto R
\]
Step 3: Gravity at halfway to the centre.
Halfway towards the centre means \(r = \frac{R}{2}\).
\[
g_{\text{half}} \propto \frac{R}{2}
\]
Step 4: Ratio calculation.
\[
g_{\text{surface}} : g_{\text{half}} = R : \frac{R}{2} = 2 : 1
\]
Step 5: Conclusion.
The required ratio is \(2 : 1\).