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.
94 exam-style questions on Edexcel GCSE Physics 6.5 Uses and dangers of radioactivity, covering 6.5.1 Uses of radioactivity, 6.5.2 Dangers of ionising radiation and precautions, 6.5.3 Half-life and radiation dangers, 6.5.4 Safety precautions for radiation exposure, and 6.5.5 Contamination and irradiation. Each one has a worked solution and a mark scheme showing where the marks go.