Power Delivered From Black Body

AI Thread Summary
The discussion revolves around calculating the power delivered by a black body source at different wavelengths, specifically near 1 µm and 10 µm, with a temperature of 1000 K. The maximum power delivery occurs at the wavelength calculated using the formula λpeak = 2.898 x 10^-3/T, which indicates a peak at approximately 2.898 µm. Participants express confusion over the lack of surface area information needed for calculations in part a, leading to difficulties in determining absolute power values. They also discuss the application of Planck's law for spectral density, noting that it requires multiplication by area and wavelength interval to yield power. Overall, the conversation highlights the challenges in interpreting the problem and the importance of understanding the relationships between wavelength, power density, and black body characteristics.
ThatGuyYeah
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Homework Statement


The power delivered in narrow spectrum range near 10 µm from black body source with temperature 1000 K is 10 µW.

Not Solved
a) What power would be delivered in narrow spectrum range near 1 µm?

Solved
b) At what wavelength the power delivered takes its maximum?
c) Find this maximum value.

Homework Equations


For b and c, you are using:

λpeak = 2.898 x 10-3/T

That aspect of this problem is easy and was solvable.

For a, I would assume that one would use:

P = σAT4

Problem is that the question doesn't give surface area at all, only λ. Plugging what was given doesn't produce the relationship at all (even squaring the given λ = 10 µm only produces 5.6 µW). I don't know if it is a bad question or missing something obvious.

I also tried E = σT4 and got 5.7 W/cm2. I would assume that I would have to calculate per 1 µm?

The other alternative solution I tried was using Radiant flux density (Planck’s law):

W = 2hc25 x 1/(e(hc/λkT)-1) and the numbers still seem off.

The Attempt at a Solution


From above.

Also, based on the information above and solving part b and c that moving closer to the black body (2.898 µm) will produce the highest power and would dip off after as we approach 1 µm, but it feels like there is something missing in part a.
 
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ThatGuyYeah said:
For a, I would assume that one would use:

P = σAT4

Problem is that the question doesn't give surface area at all, only λ. Plugging what was given doesn't produce the relationship at all (even squaring the given λ = 10 µm only produces 5.6 µW). I don't know if it is a bad question or missing something obvious.
You don't know the size of the black body, and therefore can't say anything about the total power emitted. I don't understand what "squaring the given λ = 10 µm" means. Do you know what λ is?

ThatGuyYeah said:
The other alternative solution I tried was using Radiant flux density (Planck’s law):

W = 2hc25 x 1/(e(hc/λkT)-1) and the numbers still seem off.
Again, if you don't know how big the black body is, you can't get an absolute number. But this equation is a good starting place. You need to figure out how to use it correctly for your problem.
ThatGuyYeah said:
Also, based on the information above and solving part b and c that moving closer to the black body (2.898 µm) will produce the highest power and would dip off after as we approach 1 µm, but it feels like there is something missing in part a.
Moving closer? I guess you're indeed confused about what λ is.
 
For this question, yes, I am confused about the purpose of λ.

For all intents and purposes (and to prevent you from continuing the assumption I am a total idiot) I know that λ is wavelength, which is the distance between successive crests (high points) of any type of wave (ala period). Problem is that part a is extremely arbitrary.

When I meant by 'moving closer' I was referring to the Power Density/Wavelength chart (http://hyperphysics.phy-astr.gsu.edu/hbase/quantum/radfrac.html) where if you are starting at 10 µm and approach the λpeak of 2.898 µm, you hit the maximum Power Density. But if you move away from the peak number and continue decreasing the value to 1 µm, there is supposed to be a drop off in power density (via the Power Desnity/Wavelength chart). Problem is like you said, I don't know the size of the black body.

Now, with that in mind, I did compute W = 2hc2/λ5 x 1/(e(hc/λkT)-1) at first using the given variables just to see if this was the right approach.

2hc2 = 2 (6.67 x 10-34) (2.99 x 108)2 = 1.19 x 10-16

λ5 = (10 μm)5 = 100000 μm5

Dividing those two will get = 1.19 x 10-21

1/(e(hc/λkT)-1) = e1.99 x 10-25/1.38 x 10-19 = e9.173 x 10-23 ≈ 1 - 1 ≈ 9.173 x 10-23 = 1.09 x 1022

Multiplying the two will get 12.971, but given we were dealing with rounding errors and the sort, I can assume that @ 10 μm & T = 1000 K, P ≈ 10 μW
 
That formula does not provide a power, in W.
It is spectral density. In order to get power you need to multiply by area and wavelength interval.
So there is no reason to expect to get 10 μW.

But you don't need area, it is the same in both cases. And I suppose you can assume the same wavelength interval (a narrow one).
It's just a matter of ratios.
 
ThatGuyYeah said:
For all intents and purposes (and to prevent you from continuing the assumption I am a total idiot) I know that λ is wavelength, which is the distance between successive crests (high points) of any type of wave (ala period). Problem is that part a is extremely arbitrary.
To make things clear, I never thought you were an idiot! For one thing, there is a different between idiocy and ignorance. And it's not like I have never been confused before :)

nasu said:
It's just a matter of ratios.
This.
 
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