Target:
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I can describe how energy is produced in the core of the sun.
The Proton-Proton Chain
How do we turn hydrogen into helium and make energy?
The process is called the Proton-Proton (PP) Chain, and it operates inside the Sun and stars of similar mass.
Step 1: Smash two protons together to make deuterium
positron: like an electron, but with positive charge
neutrino: very light, hard-to-detect particle
Step 2: A proton crashes into a deuterium nucleus, making helium-3
gamma ray: very high energy photon
Do Steps 1 and 2 again, so that we have two helium-3 nuclei. Then (69% of the time):
Step 3: Mash two helium-3 nuclei together to make helium-4
Actually this is the most common path to making helium in the Sun, but not the only one. After Step 2 is complete, other reactions can take place -- the PPII chain (31% of the time):
Or even the PPIII chain (rare, 0.3% of the time):
So what did we do?
We essentially turned 4 protons into
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1 helium nucleus
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1 positron (this positron will bump into a electron and annihilate, creating a gamma ray - energy!).
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1 gamma ray (energy!)
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1 neutrino
Draw a diagram to represent the proton-proton chain
Astronomy: Stars, Galaxies and Cosmology Page
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