A blackbody, by definition is an ideal system that absorbs all radiation incident on it.
If a good approximation of a black body is a small hole leading to the inside of a hollow object, then am I right in saying that the pupils of an eye are a good approximation of a black body because they are also holes to a (near) spherical cavity?
If yes, do they also emit blackbody radiation in accordance with the Planck wavelength distribution function, and is this why they appear black?
Best Answer
Any approximation has a region of applicability - that is the conditions where one can apply it or not:
Remark: Note also that one can define the black body radiation without resorting to a (largely historical) concept of the black body - as an equilibrium state of a photon gas: see, e.g., the discussion in this thread.