Would you please explain blackbody radiation in your own words?
Black body radiation is radiation emitted from a black body, so the first question is, what's a black body?
Basically, it's anything that absorbs all light that falls on it. They're abstract objects that don't exist in reality, but there are a number of objects that are close enough, or which act in the same way as black bodies. The empty backdrop of space, the blackness between stars in the sky, is
basically a black body, because it absorbs all light - insofar as light shone into the night sky doesn't reflect back, so it's like it's all been absorbed.
The key feature of a black body is that any light emitted by it is purely a product of heat. It absorbs incoming light, but its temperature still makes it shine. The light emitted can be plotted as a graph of its frequency (from microwaves and infra-red, through visible and ultra-violet, to X-ray and gamma ray) against the intensity of each type of light:
So if you have something that is, or operates like, a black body, then its spectrum will look like one of those curves. We can thus work out its temperature very accurately by looking at the outputted light.
You may have heard of the CMBR, or the Cosmic Microwave Background Radiation. As I mentioned, the blackness of space can be treated as a black body, so any light 'emitted' by it must, according to the Big Bang theory, fit a black body curve. More than that, the theory predicts which curve it should fit (namely, it should fit the '2.75K' curve). When we measured its spectrum and plotted on the same graph as the predicted black body spectrum of that temperature, this is what we got:
As the graph states, theory and observation agree. This is one of the single most impressive pieces of evidences in all of science (in my humble opinion).
So, what is black body radiation? It's the idealised spectrum of light emitted by an object by virtue of its heat alone (and not due to, say, the reflection of light being shone at it, whether due to total absorption of light, or the lack of any such light). Some objects are pretty close approximations of a black body (
such as the Sun), and some aren't objects but operate
like a black body (
such as the CMBR), so the concept is very useful in astrophysics.