To solve this problem, we need to understand how the gravitational force changes as the distance from the center of the Earth increases. The gravitational force acting on an object is given by Newton's law of universal gravitation:
F = \frac{{G \cdot m_1 \cdot m_2}}{{r^2}}
where:
For an object on the surface of the Earth, the gravitational force is also expressed as F = mg, where m is the mass of the object and g is the acceleration due to gravity at the surface of the Earth. In this case, the weight of the object is 72 N.
When the object is moved to a height above the Earth's surface, the distance from the center of the Earth becomes R + h, where R is the radius of the Earth and h is the height above the Earth's surface. In this problem, h = \frac{R}{2}, so the distance from the center is 1.5R.
The gravitational force at a height h is given by:
F_h = \frac{{G \cdot m_1 \cdot m_2}}{{(R + h)^2}} = \frac{{G \cdot m_1 \cdot m_2}}{{(1.5R)^2}}
Dividing this by the force at the surface:
\frac{{F_h}}{{F}} = \frac{{R^2}}{{(1.5R)^2}} = \frac{1}{(1.5)^2} = \frac{1}{2.25}
Plugging in the weight of the object:
F_h = 72 \times \frac{1}{2.25} = 72 \times \frac{4}{9} = 32 \text{ N}
Thus, the gravitational force exerted on the object when it is at a height \frac{R}{2} above the Earth's surface is 32 N.
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)