Doubling a blackbody's temperature doubles the number of photons it emits per second.

Name: Doubling a blackbody's temperature doubles the number of photons it emits per second.
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Doubling a blackbody's temperature increases the number of photons it emits per second, but the relationship is not linear; it increases more significantly due to the Stefan-Boltzmann law, which states that the total energy radiated per unit surface area is proportional to the fourth power of the blackbody's temperature.

Doubling a Blackbody's Temperature Doubles the Number of Photons It