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Stefan-Boltzmann Law and Wein's Law

Stefan-Boltzmann Law

It measures the luminosity of a star, which is defined as the power radiated

The total power radiated by a star is directly proportional to its surface area and to the fourth power of its temperature

Wein's

(displacement)

Law

Most objects emit radiation at many wavelength, however, there is one wavelength where an object emits the largest amount of radiation

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