How to find the intensity of radiation

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SUMMARY

The discussion focuses on calculating the intensity of radiation from a star with a radius of 9.0 x 103 m and a surface temperature of 10,000 K, using the Stefan-Boltzmann law. The total power radiated is determined using the formula P = σAeT4, where σ is the Stefan-Boltzmann constant and e is the emissivity. The brightness as seen from a planet located 2.4 x 1011 m away is calculated with b = P / (4πd2). The distinction between intensity and brightness is clarified, confirming that intensity refers to energy per time per surface area, while brightness relates to the color spectrum of the star.

PREREQUISITES
  • Understanding of the Stefan-Boltzmann law
  • Knowledge of blackbody radiation concepts
  • Familiarity with the formulas for power and intensity
  • Basic principles of isotropic radiation
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  • Learn about blackbody radiation and its significance in astronomy
  • Explore the differences between intensity and brightness in physics
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zaf
Hello Forum members

I need help on a homework problem that I am unable to solve. the problem is as follows

Given the radius of a star of 9.0 * 10^3 m and surface temperature of
10000 k (blackbody)find the intensity of radiation (watts/m^2) incident on a planet that is located 2.4 * 10^11 m from the star

I found the total power radiated from the star by using stefans and taking the area to be 4 pi r^2 so P = sAeT^4

s is the stefan-Boltzmann constant
and e is emissivity of 1 for a blackbody

then I could also find the brightness for that star as seen from another planet 2.4*10^11 m away from the star by using

b = P / (4*pi*d^2)

d being the distance...but i do'nt think that this is the answer

can someone help ?
 
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I'm no great physicist but I don't see how you can answer the question without know what portion of the star's "sky" the planet subtends. That's is a really large planet will intercept more of the stars total radiation (which is what you have calculated) than a small planet will.
 
I understand your response...but i guess that issue has not been taken into consideration by the prof...basically it is know that the intensity of radiation is inversely propotional to the distane...I need to somehow incorporate that in my solution
 
Last edited by a moderator:
Originally posted by HallsofIvy
I'm no great physicist but I don't see how you can answer the question without know what portion of the star's "sky" the planet subtends. That's is a really large planet will intercept more of the stars total radiation (which is what you have calculated) than a small planet will.

This statement is correct, however notice that the question asks for the intensity, not the total power. The intensity of an isotropic radiator, such as a star will be uniform for a given distance, d.

I see no problem with how the problem is worked out, other than you suddenly switch to solving for the brightness (all the equations are still correct, just need to replace b with I (Intensity).

Claude.
 
Ok..maybe you are correct...but i am not so sure whether brightness and intensity mean the same thing...brightness is a measure of the maximum wavelength of the color spectrum of a star...intensity is the measure of energy.
 
I think intensity = energy per time per surface area.
Or power per surface area.
So your original answer is OK, I think.
 

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