To determine the gravitational force experienced by the body at a height equal to one-third the radius of the Earth, we begin by using Newton's law of universal gravitation.
Initially, the force of gravity on the body at the Earth's surface is given by:
\[ F_1 = \frac{GMm}{R^2} = 48 \, \text{N} \]
where \( F_1 \) is the gravitational force at the Earth's surface, \( G \) is the gravitational constant, \( M \) is the mass of the Earth, \( m \) is the mass of the body, and \( R \) is the radius of the Earth.
When the body is at a height of \( \frac{R}{3} \) above the Earth's surface, the total distance from the center of the Earth is \( R + \frac{R}{3} = \frac{4R}{3} \).
The new force, \( F_2 \), can be calculated as follows:
\[ F_2 = \frac{GMm}{\left(\frac{4R}{3}\right)^2} = \frac{GMm}{\frac{16R^2}{9}} = \frac{9GMm}{16R^2} \]
Now, we set up the ratio between the forces at the two positions:
\[\frac{F_2}{F_1} = \frac{\frac{9GMm}{16R^2}}{\frac{GMm}{R^2}} = \frac{9}{16}\]
Substituting the value of \( F_1 = 48 \, \text{N} \):
\[ F_2 = \frac{9}{16} \times 48 \, \text{N} = 27 \, \text{N} \]
Thus, the gravitational force experienced by the body at that height is \( 27 \, \text{N} \).