
To find the change in weight of the object as it falls from point A to B, we need to understand how gravitational force varies with distance from the center of the Earth.
The gravitational force or weight at a distance \(r\) from the center of the Earth is given by:
\(W = \frac{G M_E m}{r^2}\)
Where:
Initially, the object is at a distance \(R_E + \frac{R_E}{2} = \frac{3R_E}{2}\) from the center of the Earth at point A.
At this point, the weight is:
\(W_A = \frac{G M_E m}{\left(\frac{3R_E}{2}\right)^2} = \frac{4 G M_E m}{9 R_E^2}\)
At point B (distance \(2R_E\) from the center of the Earth), the weight is:
\(W_B = \frac{G M_E m}{(2 R_E)^2} = \frac{G M_E m}{4 R_E^2}\)
We need to find the change in weight, \(\Delta W = W_A - W_B\):
\(\Delta W = \frac{4 G M_E m}{9 R_E^2} - \frac{G M_E m}{4 R_E^2}\)
\(\Delta W = \frac{16 G M_E m}{36 R_E^2} - \frac{9 G M_E m}{36 R_E^2}\)
\(\Delta W = \frac{(16 - 9) G M_E m}{36 R_E^2}\)
\(\Delta W = \frac{7 G M_E m}{36 R_E^2}\)
The change in gravitational force (weight) can be calculated using a simplified approach with given data assuming \(g = 10 \, \text{m/s}^2\):
\(\Delta W = m \cdot (g_1 - g_2)\)
Where:
\(\Delta W = 100 \cdot (4.44 - 2.5) = 100 \cdot 1.94 = 194 \, \text{N}\)
Since the calculation of \(\Delta W\) gives around 194 N, we can correct this to a nearby logical choice. Hence, the nearest integer from the given options and practical assumption lead us to our answer: