To determine the gravitational force on an object at an altitude equal to one-third of Earth's radius, Newton's law of universal gravitation is applied.
The initial gravitational force on the object at Earth's surface is:
\[ F_1 = \frac{GMm}{R^2} = 48 \, \text{N} \]
where \( F_1 \) represents the surface gravitational force, \( G \) is the gravitational constant, \( M \) is Earth's mass, \( m \) is the object's mass, and \( R \) is Earth's radius.
At a height of \( \frac{R}{3} \) above the surface, the total distance from Earth's center is \( R + \frac{R}{3} = \frac{4R}{3} \).
The new gravitational force, \( F_2 \), is calculated as:
\[ F_2 = \frac{GMm}{\left(\frac{4R}{3}\right)^2} = \frac{GMm}{\frac{16R^2}{9}} = \frac{9GMm}{16R^2} \]
The ratio of the forces at the two positions is:
\[\frac{F_2}{F_1} = \frac{\frac{9GMm}{16R^2}}{\frac{GMm}{R^2}} = \frac{9}{16}\]
Using \( F_1 = 48 \, \text{N} \):
\[ F_2 = \frac{9}{16} \times 48 \, \text{N} = 27 \, \text{N} \]
Therefore, the gravitational force on the object at this height is \( 27 \, \text{N} \).