During carbon burning in a massive star, two carbon-12 nuclei fuse to form a neon-20 nucleus and a helium-4 nucleus. The equation for this reaction is:
612C+612C→1020Ne+24He ^{12}_{6}\text{C} + ^{12}_{6}\text{C} \rightarrow ^{20}_{10}\text{Ne} + ^{4}_{2}\text{He} 612C+612C→1020Ne+24HeData for these nuclei are given in the table below:
| Nucleus | Mass / u |
|---|---|
| 612C^{12}_{6}\text{C}612C | 12.0000012.0000012.00000 |
| 1020Ne^{20}_{10}\text{Ne}1020Ne | 19.9924419.9924419.99244 |
| 24He^{4}_{2}\text{He}24He | 4.002604.002604.00260 |
Constants:
Calculate, in J, the energy released when this reaction occurs.
One model of nuclear fusion suggests that fusion happens when nuclei touch. Initially, the two carbon nuclei are separated so that the electrostatic force between them is negligible. They move towards each other until they fuse. Fusion occurs when their centres are separated by a distance of 5.4×10−15 m5.4 \times 10^{-15}\text{ m}5.4×10−15 m. Calculate the total change in electrostatic potential energy, in J, between the initial positions and final positions of the nuclei.
128 exam-style questions on AQA A Level Physics Radioactivity (A-level only), covering Rutherford scattering (A-level only), $\alpha$ , $\beta$ and $\gamma$ radiation (A-level only), Radioactive decay (A-level only), Nuclear instability (A-level only), Nuclear radius (A-level only), Mass and energy (A-level only), Induced fission (A-level only), and Safety aspects (A-level only). Each one has a worked solution and a mark scheme showing where the marks go.