Fusion: Creating a Star on Earth - General Atomics Fusion Education
Fusion: Creating a Star on Earth - General Atomics Fusion Education
Fusion: Creating a Star on Earth - General Atomics Fusion Education
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Therm<strong>on</strong>uclear Reacti<strong>on</strong>s in the Sun<br />
1H 1 + 1 H 1 1 H 2 + 1 e 0<br />
In the first reacti<strong>on</strong>, 2 prot<strong>on</strong>s combine<br />
to form deuterium and a positr<strong>on</strong>.<br />
One of the prot<strong>on</strong>s is c<strong>on</strong>verted into<br />
a neutr<strong>on</strong> and a posit<strong>on</strong><br />
prot<strong>on</strong> neutr<strong>on</strong><br />
positr<strong>on</strong><br />
1H 2 + 1 H 1 2 He 3 + (gamma)<br />
radiati<strong>on</strong><br />
In the 2nd reacti<strong>on</strong> a<br />
prot<strong>on</strong> + deuterium unite<br />
to form the light isotope<br />
of helium, 2 He 3<br />
2He 3 + 2 He 3 2He 4 + 1 H 1 + 1 H1<br />
The first two reacti<strong>on</strong>s must<br />
occur twice for the 3rd<br />
reacti<strong>on</strong> to occur<br />
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