To solve the problem of determining how deep inside the earth a man needs to go so that his weight becomes one-fourth of that on the earth’s surface, we can use the concept of gravitational force inside a spherical body.
The gravitational force at a distance \( r \) from the center of the Earth, but inside it, can be given by the formula:
\(F = \frac{G \cdot M(r)}{r^2}\), where \( M(r) \) is the mass contained within radius \( r \).
Inside the Earth, the gravitational force depends linearly on \( r \) because the shell of mass outside radius \( r \) does not contribute to the gravitational force at that point. Therefore, we can find \( M(r) \) using:
\(M(r) = M \cdot \left(\frac{r}{R}\right)^3\), where \( M \) is the total mass of the Earth and \( R \) is the Earth's radius.
The gravitational force \( F \) inside the Earth becomes:
\(F_{\text{inside}} = \frac{G \cdot M \cdot r}{R^3}\)
Now, the weight (gravitational force) at the surface of the Earth is:
\(F_{\text{surface}} = \frac{G \cdot M}{R^2}\)
We need the weight to become one-fourth of that on the Earth’s surface. Thus:
\(\frac{F_{\text{inside}}}{F_{\text{surface}}} = \frac{1}{4}\)
Substitute the expressions we derived for both the inside and surface force:
\(\frac{\frac{G \cdot M \cdot r}{R^3}}{\frac{G \cdot M}{R^2}} = \frac{1}{4}\)
Simplifying, we find:
\(\frac{r}{R} = \frac{1}{4}\)
Thus, \( r = \frac{R}{4} \).
This implies that the depth inside the Earth \( d \) where the man needs to go is:
\(d = R - r = R - \frac{R}{4} = \frac{3R}{4}\)
Therefore, the man should go to a depth of \( \frac{3R}{4} \) inside the Earth so that his weight becomes one-fourth of that on the Earth’s surface.
The correct option is \(\frac{3R}{4}\).