To calculate the gain in potential energy when an object is taken to a height above the surface of the Earth, where this height is equal to three times the radius of the Earth, we use the formula for gravitational potential energy in the gravitational field:
The gravitational potential energy \(U\) at a height \(h\) above the Earth's surface is given by:
\(U = -\frac{GMm}{r + h}\)
where:
Instead of \(U = -\frac{GMm}{r}\) for the surface, the change in potential energy is:
\(\Delta U = GMm \left( \frac{1}{r} - \frac{1}{r+h} \right)\)
At the surface of the Earth, the gravitational potential energy is:
\(U_{\text{surface}} = -\frac{GMm}{r}\)
At a height \(h = 3r\) above the surface, it is:
\(U_{\text{height}} = -\frac{GMm}{r + 3r} = -\frac{GMm}{4r}\)
The gain in potential energy, therefore, is:
\(\Delta U = U_{\text{height}} - U_{\text{surface}} = -\frac{GMm}{4r} - \left(-\frac{GMm}{r}\right)\) \(\Delta U = GMm\left(\frac{1}{r} - \frac{1}{4r}\right) = GMm \left(\frac{3}{4r}\right)\)
Now, using the simplified gravitational potential energy change considering \(g = \frac{GM}{r^2}\), we have:
\(\Delta U = mgr \left(\frac{3}{4}\right) = m \cdot g \cdot r \cdot \frac{3}{4}\)
Substitute \(m = 1 \, \text{kg}\), \(g = 10 \, \text{m/s}^2\), and \(r = 6.4 \times 10^6 \, \text{m}\):
\(\Delta U = 1 \times 10 \times 6.4 \times 10^6 \times \frac{3}{4} = 48 \times 10^6 \, \text{J}\)
Therefore, the gain in potential energy is 48 MJ.
The gain in potential energy of the object,
ΔU=Uf–Ui
ΔU=−\(\frac{GMm}{4R}+\frac{GMm}{R}\)
\(ΔU=\frac{3GMm}{4R}\)
\(ΔU=\frac{3}{4}mgR\)
\(ΔU= 48 x 10^6J\)
\(ΔU= 48 MJ\)
So, the correct option is (A): 48 MJ
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Consider the following two reactions A and B: 
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The formula for the Centre of Mass:

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