A mercury drop of radius \( 1 \) cm is divided into \( 10^6 \) droplets of equal size. If the surface tension of mercury is \( 35 \times 10^{-3} \) N/m, then the change in surface energy in the process is:
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For problems involving surface energy, compute the change in surface area using volume conservation principles before applying \( \Delta U = S \Delta A \).