Junk0, your original question regarded detection of chemical composition of the planetary surfaces(or atmospheres). As the others tried to explain to you, this has got nothing to do with how bright a planet is.
Light coming from a very faint, faraway, small planet will have the same spectrum as light coming from a bright, close one - as long as their chemical composition is the same.
Here's an example of what it looks like:
You just look for dips in the spectrum, and compare them with the amount of light you receive in other wavelenghts. Since you're using ratios, it's independent of the total amount of light you get.
The key words for further reading are "planetary spectroscopy", or just spectroscopy.
How bright a planet is on the sky, on the other hand, depends on:
1. how far away from the source of light(the Sun) it is
2. how large it is - meaning surface area that reflects the light*
3. what is its reflective surface made of, aka its albedo - defined as the ratio of incident light and reflected light
4. how far away from the observer it is
Black body radiation is another kettle of fish.
Its spectrum AND "brightness"(for planets its in far infrared, so invisible to a naked eye) depends on Temperature, so even though the brightness falls with distance from the observer, the blackbody spectrum stays the same, allowing us to deduce the temperature.
This is the only EM radiation that planets actually produce themselves.
Since its wavelengths are very long in the case of planets, they're not very useful for detecting chemical composition by looking for dips in the spectrum, as most elements absorb light of much shorter wavelenghts.
It's important to remember that the blackbody spectrum and absorbtion spectrum are two different things. They are connected with completely different phenomena, and in our case occupy completely different wavelenghts.
*So this means half of the sphere surface area(which is 4*∏*R
2). Notice that larger area means larger radius, and that in turn means that the larger planet has got larger volume, AND providing the density is the same between the two bodies, larger mass. So the mass, surface and volume points are closely interconnected, and it makes little sense to separate them like you did. The basic variables are density and radius, and in our case only radius matters.