Black body radiation verses spectral lines.

In summary, the conversation explores the concept of blackbody radiation and spectral lines produced by heated objects and energized electrons. The discussion raises the question of why some objects produce blackbody radiation instead of their specific frequency of spectral lines and why the sun has a yellow glow despite hydrogen's spectral line color being pink. The answer lies in the properties of materials like iron, which have overlapping wave functions and emit a continuous spectrum of light when heated. The conversation also delves into the effects of pressure on spectral lines and the relationship between spectral lines and blackbody radiation.
  • #1
Forestman
212
2
When objects are heated they produce blackbody radiation which varies with their temperature, and when the electrons in the orbitals of atoms are given energy they produce radiation at specific frequencies known as spectral lines. My question is this.

When an object, say a piece of mental is heated why does it produce blackbody radiation instead of its specific frequency of spectral lines that would result from its electrons jumping up, and then falling to a lower energy level? What happens with atoms that make blackbody radiation different from spectral line radiation? Why would the sun glow yellow instead of pink which is hydrogens spectral line color.

I understand that the answer is heat and temperature, but why?
 
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  • #2
When you deal with a material like iron and you heat it up and it glows red and other colors if you heat it hotter and eventually white hot . We are not dealing with individual atoms that have discrete orbitals . There are a lot of atoms in the iron and their wave functions over lap, so the electrons can occupy more regions in space and emit a continuous spectrum of light. Iron is not a black body but you get the idea.
 
  • #3
Thanks Cragar.
 
  • #4
When it comes to the sun, its a little more complicated. Spectral lines are broadened by high pressure, the pressure changes the energies of the orbitals randomly. For a given temperature, a line cannot go above the black body radiation. So the lines push up to the black body limit, and broaden out. If you have a lot of lines, what you will get in the limit as pressure approaches infinity is the black body spectrum.
 
  • #5
Thanks Rap.
 

1. What is black body radiation?

Black body radiation is the electromagnetic radiation emitted by a perfect black body, which is an idealized object that absorbs and emits all radiation equally at all wavelengths and temperatures.

2. What are spectral lines?

Spectral lines are specific wavelengths of light emitted or absorbed by an atom or molecule, which are unique to each element and can be used to identify the chemical composition of a substance.

3. How are black body radiation and spectral lines related?

Black body radiation and spectral lines are both forms of electromagnetic radiation, but they have different origins. Black body radiation is emitted by a hot object, while spectral lines are produced when electrons in an atom or molecule transition between energy levels.

4. What is the difference between continuous and discrete spectra?

A continuous spectrum, such as black body radiation, contains all wavelengths of light within a certain range. A discrete spectrum, like spectral lines, only contains specific wavelengths of light at distinct energy levels.

5. How do black body radiation and spectral lines contribute to our understanding of the universe?

Black body radiation and spectral lines provide valuable information about the temperature and composition of celestial objects. For example, the presence of specific spectral lines can indicate the presence of certain elements in stars and galaxies, while the intensity of black body radiation can reveal the temperature of these objects.

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