The energy required to take a body from the surface of the earth to a height equal to the radius of the earth is \( W \). The energy required to take this body from the surface of the earth to a height equal to twice the radius of the earth is:
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The gravitational potential energy change follows an inverse relationship with distance, making energy calculations crucial in celestial mechanics.
The energy required to move a body from the surface of the Earth to a height \( h \) is given by:
\[
W = GMm \left(\frac{1}{R} - \frac{1}{R+h}\right)
\]
For height \( h = R \):
\[
W_1 = GMm \left(\frac{1}{R} - \frac{1}{2R}\right) = \frac{GMm}{2R} = W
\]
For height \( h = 2R \):
\[
W_2 = GMm \left(\frac{1}{R} - \frac{1}{3R}\right) = \frac{2GMm}{3R} = \frac{4W}{3}
\]
Thus, the required energy is \( \frac{4W}{3} \).