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Astronomy · L4 · Blackbody radiation: Stefan-Boltzmann, Wien's law, and stellar L-R-T · flowchart

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by @openstemUpdated Astronomy
Observed stellar spectrumFind peak wavelength λ_maxSurface temperature TApparent brightness + distanceLuminosity LL = 4πR²σT⁴Stellar radius RWien's law: T = b/λ_maxInverse-square law

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