2. As the nebula gathers more and more mass their gravitational pull increases, forcing more atoms together. This process is known as accretion, and the result is a protostar.
1. When a nebula , which is a enormous cloud of dust and gas,collects enough mass it begins to collapse under its own gravity. when nuclear fusion begins a star is created.
3. A protostar becomes a high mass main sequence star when its core temperature exceeds 10 million K.
4. Next, super giants develop. They develop when massive main-sequence stars run out of hydrogen in their cores. At this point they start to expand,
5. When stars run out of hydrogen to fuse in their cores, stars above about 10 times the mass of the Sun become super giants and then undergo a supernova. The explosion is very bright and powerful.
Supernova!
6. When the core collapses, the blast wave slams into the dense material above, which thwarts the explosion. Instead of creating a supernova, the star implodes, forming a black hole.
7. If a star doesn't turn into a black hole, the ultra-dense remnants of the imploding core which are left behind are known as a neutron star, as its electrons and protons are crushed together in the huge gravity to form neutrons.
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