Classification of stars (AQA A-Level Physics): Flashcards

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Classification by temperature, black-body radiation
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Black body definition

Object that absorbs & emits all wavelengths of radiation

Stefan's Law formula

P=σAT4P = \sigma A T^4

Stefan-Boltzmann constant σ\sigma value

5.67×1085.67 \times 10^{-8} W m2^{-2} K4^{-4}

Stefan's Law: luminosity proportional to?

Surface area AA and fourth power of temp T4T^4

Wien's Displacement Law formula

λmaxT=2.9×103\lambda_{\text{max}} T = 2.9 \times 10^{-3} m K

Wien's constant value

2.9×1032.9 \times 10^{-3} m K

Temp increase effect on peak wavelength (Wien's)

Peak wavelength decreases (shorter wavelengths)

Black-body curve peak shift as temp increases

Shifts to shorter wavelengths

Inverse square law of intensity formula

I=P4πd2I = \frac{P}{4 \pi d^2}

Intensity definition (inverse square law)

Power per unit area

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