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The inconsistency of the sun's energy output with chemical processes and how nuclear fusion of light nuclei, specifically the proton-proton cycle, provides a solution. The role of electric charge, temperature, and the steps involved in the fusion process, resulting in the formation of helium-4 and the release of excess energy.
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Light nuclei have relatively high rest masses.
H ‐ 1:
u - H ‐ 2: 2. u - He ‐ 3: 3. u - He ‐ 4: 4. u - C ‐ 12: 12. u Energy is available compared to heavy mass nuclei. - Si ‐ 28: 27. - Fe ‐ 56: 55.
Electric charge causes positive nuclei to repel. At high temperatures nuclei get close enough for the nuclear force to pull them together. fusion startingnuclei heaviernucleus otherparticles
Fusion takes place two particles at a time.
Step
two protons form a deuterium nucleus with positron and a neutrino. hydrogennuclei withone protoneach neutron neutrino: related toelectrons by theweak nuclear force photons electron positron: positivecharged electron;annihilates to formphotons
Step
Two helium
nuclei collide. They rearrange particles so that very stable helium
is formed with two extra protons spit out.^ helium- helium- proton next
The fusion reaction in a star is exothermic.
H ‐1:
u - He ‐4: 4. u This is less than 4 hydrogen masses so there is energy released.
Find the mass energy difference.
4(1.0078) ‐ (4.0030)
Convert to MeV.
(0. u)(931. MeV/u)
This is per single fusion reaction.