Problem Set 05 Solution Key

Stellar Properties and Evolution ยท Instructor-facing artifact

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Worked Solutions and Rubric Notes

1. Inverse-Square Brightness

Flux scales as 1/d^2, so F_B/F_A = 1/3^2 = 1/9. The farther star appears nine times fainter even though it has the same luminosity.

Rubric: Award credit for setup, physical reasoning, units, calculation or evidence, and interpretation. Distinguish arithmetic slips from conceptual errors.

2. Radius from Luminosity and Temperature

At the same temperature, L scales as R^2. R/Rsun = sqrt(100) = 10. It is much larger than the Sun at the same temperature, consistent with a giant or bright giant region rather than the main sequence Sun.

Rubric: Award credit for setup, physical reasoning, units, calculation or evidence, and interpretation. Distinguish arithmetic slips from conceptual errors.

3. Main-Sequence Lifetime Scaling

t/t_sun = 5/600 = 0.00833. Lifetime = 0.00833 x 10 billion years = 83 million years. The high luminosity overwhelms the larger fuel supply.

Rubric: Award credit for setup, physical reasoning, units, calculation or evidence, and interpretation. Distinguish arithmetic slips from conceptual errors.

4. Cluster Turnoff Interpretation

Cluster B is older. Hot blue stars are massive and short-lived, so if they are still on the main sequence the cluster is young. A Sun-like turnoff means more massive stars have already evolved away, implying older age.

Rubric: Award credit for setup, physical reasoning, units, calculation or evidence, and interpretation. Distinguish arithmetic slips from conceptual errors.

Textbook Problem Rationale

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