11P10

11P10 Thermal Properties


Amrita OLABS Virtual Labs
Newton's Law of Cooling
Notice that initially the temperature of the hot liquid drops very fast meaning the rate of cooling is high, but as the temperature decreases, the rate of cooling decreases and takes infinite time to reach the surrounding temperature.


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Planck's Law of Black-body Radiation: 
Wein's Displacement Law:

Useful to show two different temperatures and the wavelength where the maximum intensity occurs.


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Wavelength to Colour relationship

400 to 800 nm Visible Light Spectrum



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Temperature to Colour relationship

As temperature of source increases the colour of radiation changes to higher frequency. Wein's displacement law and Stefan's Law.



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