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How Solar systems form
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It all starts with accreation, with a whispy cloud of gas and dust
Resulting in this flat spinning disk
Here occurs heating and cooling
Nuclear fission happens when hydrogen atoms fuse into helium.
When enough material collects at the center of the disk, nuclear fission begins, the sun eats a lot of it up
The material left behind the sun clumped up together into bigger and bigger pieces
These clumps became planets, dwarf planets, asteroids , comets and moons
Only rocky things could survive close to the sun so gaseous and icy material collected far away
Comets and asteroids form from the left over remains of the solar system formation
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