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Fusion and Stars · Paper 1 — Free Physics SL Practice Questions

1FoundationMCQNuclear fusion and energy production in stars1 markPaper 1~2 min
A binding energy per nucleon graph shows that hydrogen-1 has a binding energy per nucleon of approximately 0 MeV0\ \text{MeV} and helium-4 has a binding energy per nucleon of approximately 7.1 MeV7.1\ \text{MeV}. When four hydrogen nuclei fuse to form one helium-4 nucleus, which statement correctly explains why energy is released?
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Solutions

2FoundationMCQLife cycle of stars1 markPaper 1~2 min
A star spends several billion years on the main sequence before its luminosity increases by a factor of approximately 10310^3. Which evolutionary stage is responsible for this sharp luminosity increase?
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Solutions

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