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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 />

32

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