Answer:
[tex]g'=\frac{g__R}{4}[/tex]
Explanation:
Given:
Now as we know that the value of gravity of any heavenly body is at height h is given as:
[tex]g'=g__{R}} \times \frac{R^2}{(2R)^2}[/tex]
[tex]g'=\frac{g__R}{4}[/tex]
∴The gravitational field strength will become one-fourth of what it is at the surface of the moon.