Answer:

Step-by-step explanation:
The intensity of the radiation emitted by a black body with a certain temperature T and frequency
, is given by Planck's law:

Considering the frequency range between
and
and
the amount of energy emitted in this frequency range. Since an increase in frequency means a decrease in wavelength. Then:

Now recall that
, differentiate both sides:

Replacing this in previous equation:

Rewriting
as
and
as


Finally, we obtain Planck's radiation law in terms of wavelength