Black Body Radiation: Find Temperature of Panel PM in Radiation Equilibrium

In summary, the insertion of a new black panel between the two sheets of material will change the radiation balance of the system.
  • #1
SEEDS
12
0
***** SHEETS two ideally black of the area 1:5 mETER SQUARE are located opposite of each other in vacuum.
The first SHEET P1 has the FIXED temperature T1 = 0o C, the second SHEET P2 has the
fIXED temperature T2 = 100o C.

Now an additional black panel PM of the same size is brought between the panels P1 and P2.
a) What will be the temperature TM of the panel PM in the radiation equilibrium?Can anyone just give me some hints ?
 
Last edited:
Physics news on Phys.org
  • #2
Welcome to PF - this should be posted in the homework forum and you should make an attempt at the question first.

It will reach an equilibrium temperature where the energy it receives is equal to the energy it emits. What's the equation linking blackbody power and temperature?
 
  • #3
Ok, Thanks a lot for the hint . I tried it please take a look at it ...

According to Stefans LAW

P=SAT^(4) P = Power radiated in W (J/s)
s = Stefan's Constant 5.67 x 10-8 W m-2 K-4
A = Surface area of body (m²)
T = Temperature of body (K)To Find out the temperature of Pm :-

P =SAT2^(4)---(A)

Where Sigma = 5.67 x 10-8 W m-2 K-4
Area = 1.5 m^2
Temperature in Degrees Kelvin = 373.15

Therefore according to eqn A,
P = 1649.068 W ...

Now My Question is ,

Is the calculated power is from panel P2 ?
If it is then how i will approach to the temperature of Pm ?Boundary effects shall be negligible.
 
  • #4
Correct, The power flows both ways, a larger amount flows from hot->cold and a smaller amount back. The amount of power is just the difference in emmission for the two temperatures.
ie. P = sA(T14 - T24) for each panel.
So you have,

1, between T1 and the new panel
P = sA(TM4 - T14)

2, between the new panel and T2
P = sA(T24 - TM4)

Now for an equilibrium the two powers must be equal - otherwise the muiddle one would be changing in temperature. So simply set the two equations equal to each other and do a bit or re-aranging.
Hint, would you expect the answer to depend on the area if all three are the same size?

Note - depending on how idealised the question is you might want to consider what power flows off the other sides of the outer 2 plates. Since you aren;t given a temperature for the surroundings you shoudl probably assume they are at an infitie distance or zero temperature.
 
  • #5
Thanks a lot for the help ,
sA(TM4 - T14) = sA (T24 - TM4) By canceling sA

(TM4 - T14) = (T24 - TM4)

Tm4 = (T24 - T14)/2

Tm4 = 6.9106 10^9 .

How does the radiation balance of P2 change with the insertion of PM?

Thanks again
 
Last edited:
  • #6
Think you might have a small typo.
Tm4 = (T24+T14)/2

Remember that because you are multiplying it has to be absolute temperature.

And before you type in any numbers, what temperature would you expect - roughly?
 
  • #7
mgb_phys said:
Think you might have a small typo.
Tm4 = (T24+T14)/2

Remember that because you are multiplying it has to be absolute temperature.

And before you type in any numbers, what temperature would you expect - roughly?
Ohh Sorry ..

Now i got it ,

Tm4 = (T24 + T14)/2
Tm = 334.21 Kelvin

How does the radiation balance of P2 change with the insertion of PM?

What i m getting is radiation balance of P2 with P1 will change after the insertion but how can we define it ?
 

1. What is black body radiation?

Black body radiation refers to the electromagnetic radiation emitted by an object that absorbs all incoming radiation and reflects none. This type of radiation follows a specific distribution of wavelengths and intensities, which is determined by the temperature of the object.

2. How is black body radiation related to finding the temperature of a panel in radiation equilibrium?

In order to find the temperature of a panel in radiation equilibrium, we must consider the black body radiation emitted by the panel. The temperature of the panel can be determined by analyzing the spectrum of the emitted radiation and using the Stefan-Boltzmann law, which relates the temperature of a black body to the intensity of its radiation.

3. What is the Stefan-Boltzmann law?

The Stefan-Boltzmann law states that the total energy radiated by a black body per unit surface area is proportional to the fourth power of its absolute temperature. This means that as the temperature of a black body increases, the amount of radiation it emits also increases exponentially.

4. How do we know when a panel is in radiation equilibrium?

A panel is in radiation equilibrium when the amount of energy it absorbs from incoming radiation is equal to the amount of energy it emits through black body radiation. This equilibrium is reached when the temperature of the panel remains constant over time.

5. What factors affect the temperature of a panel in radiation equilibrium?

The temperature of a panel in radiation equilibrium is primarily affected by the intensity and wavelength distribution of the incoming radiation, as well as the properties of the panel itself, such as its material and surface characteristics. Additionally, external factors like air temperature and wind speed can also influence the temperature of the panel.

Similar threads

  • Introductory Physics Homework Help
Replies
7
Views
4K
  • Introductory Physics Homework Help
Replies
5
Views
2K
Replies
29
Views
2K
  • Introductory Physics Homework Help
Replies
12
Views
1K
Replies
5
Views
2K
Replies
9
Views
2K
Replies
4
Views
928
  • Quantum Physics
Replies
4
Views
1K
Replies
8
Views
2K
  • Introductory Physics Homework Help
Replies
2
Views
2K
Back
Top