BLACK BODY RADIATION

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Landus Mumbere Expedito
DISTRIBUTION OF ENERGY WITHIN THE SPECTRUM OF A BLACK BODY (SPHERAL DISTRIBUTION OF BLACK BODY RADIATION)

Features (observations) of the curves shown

  • The curves at lower temperatures lie completely inside those at higher temperatures,
  • The intensity for each wavelength increases with increase in wavelength but the increase is faster on the side of the shorter wavelength, 
  • At each temperature T, the energy emitted is maximum for a certain wave length  which decreases with rising temperature.

NOTE: The dotted line shows the locus of the peaks of the curves for the different temperatures.

Conclusions from the above observations

  • A body radiates energy at a rate which is determined by the nature of the surface and its temperature, 
  • A body absorbs energy at a rate determined by the nature of the surface and the temperature of the surroundings, 
  • The area under any particular curve is the total energy radiated per unit surface area per second; at the corresponding temperature. 
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