To determine the relation between h_1, h_2, and h_3, we can employ the equations of motion under gravity. For an object falling freely under gravity, the distance covered in time t can be calculated using the equation:
s = \frac{1}{2}gt^2
where g is the acceleration due to gravity, which is approximately 9.8 \, \text{m/s}^2.
First, we will calculate the distances h_1, h_2 - h_1, and h_3 - h_2, covered in consecutive 5-second intervals:
From these calculations, the distances for each interval are: h_1 = 122.5 \, \text{m}, h_2 - h_1 = 367.5 \, \text{m}, and h_3 - h_2 = 612.5 \, \text{m}.
The ratio of the distances covered in each interval is: h_1 : (h_2 - h_1) : (h_3 - h_2) = 122.5 : 367.5 : 612.5, which simplifies to the proportionalities h_1 = \frac{h_2}{3} = \frac{h_3}{5}.
Thus, the correct relation is: h_1 = \frac{h_2}3 = \frac{h_3}5.