Do all bodies radiate at all frequencies?

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SUMMARY

All bodies with a temperature above absolute zero radiate energy according to the Stefan-Boltzmann Law, expressed as P = AeσT^4. To determine the frequency of emitted radiation based on temperature, Planck's radiation law provides the necessary frequency distribution. For gases, which do not behave as perfect black bodies, the emitted radiation occurs in specific spectral bands. Understanding these principles is essential for calculating the heat required to make a gas emit visible light.

PREREQUISITES
  • Understanding of the Stefan-Boltzmann Law
  • Familiarity with Planck's radiation law
  • Knowledge of black body radiation concepts
  • Basic principles of gas behavior and emission spectra
NEXT STEPS
  • Research the application of Planck's radiation law in practical scenarios
  • Explore the differences between black body and non-black body radiation
  • Investigate methods for measuring the temperature of gases to achieve visible light emission
  • Study the specific emission spectra of various gases
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Physicists, engineers, and anyone interested in thermodynamics, particularly those studying radiation and heat transfer in gases and solids.

zeromodz
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I know that all bodies with a temperature above absolute zero radiate energy away as the following.

P = AeσT^4

However, I wanted to know how you could find the frequency of the power being emitted just by knowing the temperature. For example, how would I find out how much heat I need to put in a specific gas in order for it to radiate visible light (make it glow). I know that the hotter you get it, the more variety of frequencies you get.
 
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zeromodz said:
I know that all bodies with a temperature above absolute zero radiate energy away as the following.

P = AeσT^4

However, I wanted to know how you could find the frequency of the power being emitted just by knowing the temperature. For example, how would I find out how much heat I need to put in a specific gas in order for it to radiate visible light (make it glow). I know that the hotter you get it, the more variety of frequencies you get.
The frequency distribution as a function of temperature is given by Planck's radiation law. See for example: http://en.wikipedia.org/wiki/Planck%27s_law"

AM
 
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