The energy, EEE, released in nuclear fusion is equivalent to the loss in mass, mmm, according to the equation:
E=mc2 E = mc^2 E=mc2where c c\,c is the speed of light:
c=3.00×108 m/s c = 3.00 \times 10^8 \text{ m/s} c=3.00×108 m/sIn 1 second, the energy radiated by the massive star Vega is 1.80 × 1028 J.
Calculate the loss in mass of Vega in 1 second.
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.