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Main Sequence
 

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Main SequenceOnline version

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by Kristine Vester
1

pressure subatomic Hotter repeats helium hydrogen red Smaller supergiant star fusion together sequence particle dense attaches nucleus protons electrons 2 combo Nuclear neutron collide

Main stars are what most stars are . They fuse hydrogen in their core . / cooler ones will take the giant branch . / bigger ones will take the branch .

Fusion is what happens in the core to produce the star's energy / light . Without , an object can not be a . Most fusion is fusing to helium .

The steps are as followed :
The core is so hot and that the causes to be flying around on their own without .
Two protons hit each other and stick . One proton turns into a . A flies off .
Another proton comes in and to the proton / neutron
Those last two steps with another group
Those two groups and stick together . We lose two of the protons leaving protons and 2 neutrons . This is a complete .

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