1. Begin as clouds of dust and gas called nebulae
2. Gravity may cause the nebula to contract
3. Matter in the gas cloud will begin to condense into a dense region called a protostar
4. The protostar continues to condense, it heats up. Eventually, it reaches a critical mass and nuclear fusion begins
5. Begins the main sequence phase of the star
6. Very large, massive stars burn their fuel much faster than smaller stars
7. Eventually, the star's fuel will begin to run out
8. It will expand into what is known as a red giant
9. Massive stars will become red supergiants
10. Most average stars will blow away their outer atmospheres to form a planetary nebula
11. If the star is massive enough, the collapse will trigger a violent explosion known as a supernova
12. If the remaining mass of the star is about 1.4 times that of our Sun, the core is unable to support itself and it will collapse further to become a neutron star
13. If the remaining mass of the star is more than about three times that of the Sun, it will collapse so completely that it will literally disappear from the universe. What is left behind is an intense region of gravity called a black hole