The energy released in the fusion of \( 2 \, \text{kg} \) of hydrogen deep in the sun is \( E_H \) and the energy released in the fission of \( 2 \, \text{kg} \) \( {}^{235}\!U \) is \( E_U \). The ratio \( \dfrac{E_H}{E_U} \) is approximately:
(Consider the fusion reaction as \( 4\,{}^{1}_{1}\!H + 2e^{-} \rightarrow {}^{4}_{2}\!He + 2\nu + 6\gamma + 26.7 \, \text{MeV} \) , energy released in the fission reaction of \( {}^{235}\!U \) is \( 200 \, \text{MeV} \) per fission nucleus and \( N_A = 6.023 \times 10^{23} \))