Worksheet: The Stefan–Boltzmann Law

In this worksheet, we will practice converting between the temperature of a blackbody and its radiant emittance using the Stefan–Boltzmann law.

Q1:

A black body at 3 0 0 0 K radiates electromagnetic radiation with the peak intensity in the infrared range. A peak-intensity photon has a frequency of 3 . 1 0 × 1 0 Hz. What is the wavelength of this photon?

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