Step 1: Write the gravitational acceleration on the surface.
For a sphere of mass \(M\) and radius \(R\), gravitational acceleration at the surface is
\[
a_0=\frac{GM}{R^2}
\]
where \(G\) is the gravitational constant.
Step 2: Write the gravitational acceleration at a distance \(r\) from the centre.
For a point outside the sphere,
\[
a=\frac{GM}{r^2}
\]
According to the question,
\[
a=\frac{a_0}{4}
\]
Substitute the expressions:
\[
\frac{GM}{r^2}=\frac{1}{4}\left(\frac{GM}{R^2}\right)
\]
Step 3: Simplify the equation.
Cancel \(GM\) from both sides:
\[
\frac{1}{r^2}=\frac{1}{4R^2}
\]
Taking reciprocal,
\[
r^2=4R^2
\]
\[
r=2R
\]
Step 4: Final conclusion.
Hence, the required distance from the centre of the sphere is
\[
\boxed{2R}
\]