To determine the change in potential energy when a body is taken from the Earth's surface to a height equal to twice the Earth's radius, we can use the gravitational potential energy formula:
The gravitational potential energy at a distance r from the center of the Earth is given by:
U = -\frac{GMm}{r}
where:
Initially, the body is on the surface of the Earth, so:
U_1 = -\frac{GMm}{R}
When the body is at a height equal to twice the radius of the Earth, the distance from the center of the Earth becomes 3R. Therefore, the potential energy at this height is:
U_2 = -\frac{GMm}{3R}
The change in potential energy (\Delta U) is the difference between the final potential energy U_2 and the initial potential energy U_1:
\Delta U = U_2 - U_1 = \left(-\frac{GMm}{3R}\right) - \left(-\frac{GMm}{R}\right)
Simplifying the expression yields:
\Delta U = -\frac{GMm}{3R} + \frac{GMm}{R}
\Delta U = \frac{GMm}{R} \left(1 - \frac{1}{3}\right)
\Delta U = \frac{GMm}{R} \times \frac{2}{3}
\Delta U = \frac{2}{3} \times \frac{GMm}{R}
Now, using the fact that the gravitational force mg = \frac{GMm}{R^2}, we can rewrite \frac{GMm}{R} as mgR. Thus, the change in potential energy is:
\Delta U = \frac{2}{3} mgR
Therefore, the correct answer is \frac{2}{3} mgR, which corresponds to the option ⅔ mgR.