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Stephan-Boltzmann Law

Last modified by
on
Jul 24, 2020, 6:28:07 PM
Created by
on
Oct 4, 2014, 8:00:07 AM
j*=σT4
(T)Temperature
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The Stephan-Boltzman Law calculator computes power radiated from a black body based on the body's thermodynamic temperature (T).

INSTRUCTIONS: Choose the preferred units and enter the following:

  • (T)  This is the thermodynamic temperature of the object.

Energy Radiated: The calculator returns the energy radiated in W/m2.  However, this can be automatically converted into lux or lambert units via the pull-down menu.

The Math / Science

According to the Stefan-Boltzmann law, a doubling of temperature means an increase of energy emitted at the surface increases by a factor of 16. This means that a star with twice the temperature has 16 times the energy.

To solve for this, use the following equation:

F=σT4

where

F is the Energy flux
 σ is the boltzmann constant
 T is the temperature


This equation, Stephan-Boltzmann Law, references 1 page
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