Stefan Boltzmann Law Solution

STEP 0: Pre-Calculation Summary
Formula Used
Black-Body Radiant Emittance = [Stefan-BoltZ]*Temperature^(4)
eb = [Stefan-BoltZ]*T^(4)
This formula uses 1 Constants, 2 Variables
Constants Used
[Stefan-BoltZ] - Stefan-Boltzmann Constant Value Taken As 5.670367E-8
Variables Used
Black-Body Radiant Emittance - (Measured in Watt per Square Meter) - Black-Body Radiant Emittance is the radiant flux emitted by a surface per unit area.
Temperature - (Measured in Kelvin) - Temperature is the degree or intensity of heat present in a substance or object.
STEP 1: Convert Input(s) to Base Unit
Temperature: 85 Kelvin --> 85 Kelvin No Conversion Required
STEP 2: Evaluate Formula
Substituting Input Values in Formula
eb = [Stefan-BoltZ]*T^(4) --> [Stefan-BoltZ]*85^(4)
Evaluating ... ...
eb = 2.95996701379375
STEP 3: Convert Result to Output's Unit
2.95996701379375 Watt per Square Meter --> No Conversion Required
FINAL ANSWER
2.95996701379375 2.959967 Watt per Square Meter <-- Black-Body Radiant Emittance
(Calculation completed in 00.004 seconds)

Credits

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Created by Kethavath Srinath
Osmania University (OU), Hyderabad
Kethavath Srinath has created this Calculator and 1000+ more calculators!
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Verified by Urvi Rathod
Vishwakarma Government Engineering College (VGEC), Ahmedabad
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Stefan Boltzmann Law Formula

​LaTeX ​Go
Black-Body Radiant Emittance = [Stefan-BoltZ]*Temperature^(4)
eb = [Stefan-BoltZ]*T^(4)

Define Stefan–Boltzmann law?

Stefan–Boltzmann law states that the total radiation emitted by a black body is proportional to the fourth power of its absolute temperature.This law applies only to blackbodies, theoretical surfaces that absorb all incident heat radiation.

How to Calculate Stefan Boltzmann Law?

Stefan Boltzmann Law calculator uses Black-Body Radiant Emittance = [Stefan-BoltZ]*Temperature^(4) to calculate the Black-Body Radiant Emittance, Stefan Boltzmann law that the total radiation emitted by a black body is proportional to the fourth power of its absolute temperature. Black-Body Radiant Emittance is denoted by eb symbol.

How to calculate Stefan Boltzmann Law using this online calculator? To use this online calculator for Stefan Boltzmann Law, enter Temperature (T) and hit the calculate button. Here is how the Stefan Boltzmann Law calculation can be explained with given input values -> 2.959967 = [Stefan-BoltZ]*85^(4).

FAQ

What is Stefan Boltzmann Law?
Stefan Boltzmann law that the total radiation emitted by a black body is proportional to the fourth power of its absolute temperature and is represented as eb = [Stefan-BoltZ]*T^(4) or Black-Body Radiant Emittance = [Stefan-BoltZ]*Temperature^(4). Temperature is the degree or intensity of heat present in a substance or object.
How to calculate Stefan Boltzmann Law?
Stefan Boltzmann law that the total radiation emitted by a black body is proportional to the fourth power of its absolute temperature is calculated using Black-Body Radiant Emittance = [Stefan-BoltZ]*Temperature^(4). To calculate Stefan Boltzmann Law, you need Temperature (T). With our tool, you need to enter the respective value for Temperature and hit the calculate button. You can also select the units (if any) for Input(s) and the Output as well.
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