A source glowing because it is hot — flame, filament, star — shines by incandescence. Its spectrum is the continuous thermal spectrum of Chapter 2, and its peak obeys Wien’s law (Proposition 2.7),
our quantitative tool from now on: peak measured, temperature known.
Examples
Example 11.13 (A very inefficient lamp)
A tungsten filament at peaks at , deep in the infrared: most of the electric power leaves as invisible radiation, only about as light — the incandescent bulb was mainly a heater.