Emissive Power of Blackbody Solution

STEP 0: Pre-Calculation Summary
Formula Used
Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^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
Emissive Power of Blackbody - (Measured in Watt per Square Meter) - Emissive Power of Blackbody is the energy of thermal radiation emitted in all directions per unit time from each unit area of a surface of blackbody at any given temperature.
Temperature of Blackbody - (Measured in Kelvin) - Temperature of Blackbody is defined as the degree of hotness or coldness of blackbody.
STEP 1: Convert Input(s) to Base Unit
Temperature of Blackbody: 275 Kelvin --> 275 Kelvin No Conversion Required
STEP 2: Evaluate Formula
Substituting Input Values in Formula
Eb = [Stefan-BoltZ]*(T^4) --> [Stefan-BoltZ]*(275^4)
Evaluating ... ...
Eb = 324.296262683594
STEP 3: Convert Result to Output's Unit
324.296262683594 Watt per Square Meter --> No Conversion Required
FINAL ANSWER
324.296262683594 324.2963 Watt per Square Meter <-- Emissive Power of Blackbody
(Calculation completed in 00.021 seconds)

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Created by Ayush gupta
University School of Chemical Technology-USCT (GGSIPU), New Delhi
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Emissive Power of Blackbody
​ LaTeX ​ Go Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^4)
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Area of Surface 2 given Area 1 and Radiation Shape Factor for Both Surfaces
​ LaTeX ​ Go Surface Area of Body 2 = Surface Area of Body 1*(Radiation Shape Factor 12/Radiation Shape Factor 21)
Emissive Power of Blackbody
​ LaTeX ​ Go Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^4)
Absorptivity given Reflectivity and Transmissivity
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Emissive Power of Blackbody Formula

​LaTeX ​Go
Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^4)
Eb = [Stefan-BoltZ]*(T^4)

What is Radiation?

Radiation is energy that comes from a source and travels through space at the speed of light. This energy has an electric field and a magnetic field associated with it, and has wave-like properties. You could also call radiation “electromagnetic waves”.

What is Blackbody?

A black body is defined as the body which absorbs all the electromagnetic radiation (that is light) that strikes it irrespective of the angle of incidence and frequency of the radiation.

How to Calculate Emissive Power of Blackbody?

Emissive Power of Blackbody calculator uses Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^4) to calculate the Emissive Power of Blackbody, The Emissive Power of Blackbody formula is defined as the product of stefan boltzmann constant and temperature of blackbody raised to it's fourth power. Emissive Power of Blackbody is denoted by Eb symbol.

How to calculate Emissive Power of Blackbody using this online calculator? To use this online calculator for Emissive Power of Blackbody, enter Temperature of Blackbody (T) and hit the calculate button. Here is how the Emissive Power of Blackbody calculation can be explained with given input values -> 324.2963 = [Stefan-BoltZ]*(275^4).

FAQ

What is Emissive Power of Blackbody?
The Emissive Power of Blackbody formula is defined as the product of stefan boltzmann constant and temperature of blackbody raised to it's fourth power and is represented as Eb = [Stefan-BoltZ]*(T^4) or Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^4). Temperature of Blackbody is defined as the degree of hotness or coldness of blackbody.
How to calculate Emissive Power of Blackbody?
The Emissive Power of Blackbody formula is defined as the product of stefan boltzmann constant and temperature of blackbody raised to it's fourth power is calculated using Emissive Power of Blackbody = [Stefan-BoltZ]*(Temperature of Blackbody^4). To calculate Emissive Power of Blackbody, you need Temperature of Blackbody (T). With our tool, you need to enter the respective value for Temperature of Blackbody 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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