We are given that the value of gravitational acceleration \( g' \) at a height \( h \) above the Earth's surface is \( \frac{g}{\sqrt{3}} \), where \( g \) is the acceleration due to gravity at the Earth's surface.
The formula for gravitational acceleration at a height \( h \) above the Earth's surface is given by:
\[
g' = \frac{g R^2}{(R + h)^2}
\]
where:
- \( g \) is the acceleration due to gravity on the surface of the Earth,
- \( R \) is the radius of the Earth,
- \( h \) is the height above the Earth's surface.
We are given that:
\[
g' = \frac{g}{\sqrt{3}}
\]
Substitute this into the equation:
\[
\frac{g}{\sqrt{3}} = \frac{g R^2}{(R + h)^2}
\]
Cancel out \( g \) from both sides:
\[
\frac{1}{\sqrt{3}} = \frac{R^2}{(R + h)^2}
\]
Now, square both sides to eliminate the square root:
\[
\frac{1}{3} = \frac{R^2}{(R + h)^2}
\]
Cross-multiply:
\[
3 R^2 = (R + h)^2
\]
Expand the right-hand side:
\[
3 R^2 = R^2 + 2Rh + h^2
\]
Simplify:
\[
3 R^2 - R^2 = 2Rh + h^2
\]
\[
2 R^2 = 2Rh + h^2
\]
Rearrange the equation:
\[
2 R^2 = h(2R + h)
\]
Solve for \( h \):
\[
h = \frac{2 R^2}{2R + h}
\]
Approximate for \( h \) (assuming \( h \ll R \), so \( h \) is much smaller than \( R \)):
\[
h \approx R \sqrt{3}
\]
Thus, the height \( h \) is approximately \( R \sqrt{3} \).