1. Dust and gas cloud is present in a galaxy
2. The gravitational attraction between the gas/dust particles draws them together
3. The cloud becomes more concentrated, as the particles get closer
4. The temperature and pressure of the cloud increases as the particles get pushed so close together
5. Eventually the pressure gets so great that the gas/dust particles are able to fuse together
6. Fusion occurs as the light (mainly hydrogen gas) nuclei fuse together to form helium nuclei, creating a large amount of energy
7. This release opposes the collapsing of the cloud due to gravity
8. So eventually an equilibrium forms, where the energy released due to fusion balances the pressure of gravitational collapse
9. Eventually the star runs out of gas to fuse, so it collapses
10. If Massive, the star will collapse, increasing the pressure + temperature of the core, meaning heavier elements can fuse. Once all the fusion has happened, it is too massive to be stable, so the star collapses, rebounds on its centre and produces a supernova
11. What remains is either a neutron star or black hole
12. If Normal-sized, the same process happens, less fusion occurs however (less fuel to fuse), the star collapses, and produces a planetary nebula, a lower scale supernova, and a white dwarf remains