In an astrophysical simulation of stellar nucleosynthesis, two helium-3 nuclei undergo fusion to produce a helium-4 nucleus and two protons.
2 helium-3→helium-4+2 protons 2\text{ helium-3} \rightarrow \text{helium-4} + 2\text{ protons} 2 helium-3→helium-4+2 protonsThis difference in mass is converted into energy.
Calculate the percentage of the original mass that has been converted to energy. Give your answer to 2 significant figures.