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Heat Transfer is the amount of heat that is transferred per unit of time in some material, usually measured in watts (joules per second). Check FAQs
q=ε[Stefan-BoltZ]A(T14-T24)
q - Heat Transfer?ε - Emissivity?A - Area?T1 - Temperature of Surface 1?T2 - Temperature of Surface 2?[Stefan-BoltZ] - Stefan-Boltzmann Constant?

Black Bodies Heat Exchange by Radiation Example

With values
With units
Only example

Here is how the Black Bodies Heat Exchange by Radiation equation looks like with Values.

Here is how the Black Bodies Heat Exchange by Radiation equation looks like with Units.

Here is how the Black Bodies Heat Exchange by Radiation equation looks like.

-1119.9937Edit=0.95Edit5.7E-850Edit(101Edit4-151Edit4)
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Black Bodies Heat Exchange by Radiation Solution

Follow our step by step solution on how to calculate Black Bodies Heat Exchange by Radiation?

FIRST Step Consider the formula
q=ε[Stefan-BoltZ]A(T14-T24)
Next Step Substitute values of Variables
q=0.95[Stefan-BoltZ]50(101K4-151K4)
Next Step Substitute values of Constants
q=0.955.7E-850(101K4-151K4)
Next Step Prepare to Evaluate
q=0.955.7E-850(1014-1514)
Next Step Evaluate
q=-1119.99370862799W
LAST Step Rounding Answer
q=-1119.9937W

Black Bodies Heat Exchange by Radiation Formula Elements

Variables
Constants
Heat Transfer
Heat Transfer is the amount of heat that is transferred per unit of time in some material, usually measured in watts (joules per second).
Symbol: q
Measurement: PowerUnit: W
Note: Value can be positive or negative.
Emissivity
Emissivity is the ability of an object to emit infrared energy. Emissivity can have a value from 0 (shiny mirror) to 1.0 (blackbody). Most organic or oxidized surfaces have emissivity close to 0.95.
Symbol: ε
Measurement: NAUnit: Unitless
Note: Value should be between 0 to 1.
Area
The area is the amount of two-dimensional space taken up by an object.
Symbol: A
Measurement: AreaUnit:
Note: Value should be greater than 0.
Temperature of Surface 1
Temperature of Surface 1 is the temperature of the 1st surface.
Symbol: T1
Measurement: TemperatureUnit: K
Note: Value can be positive or negative.
Temperature of Surface 2
Temperature of Surface 2 is the temperature of the 2nd surface.
Symbol: T2
Measurement: TemperatureUnit: K
Note: Value can be positive or negative.
Stefan-Boltzmann Constant
Stefan-Boltzmann Constant relates the total energy radiated by a perfect black body to its temperature and is fundamental in understanding blackbody radiation and astrophysics.
Symbol: [Stefan-BoltZ]
Value: 5.670367E-8

Other Formulas to find Heat Transfer

​Go Heat Exchange by Radiation due to Geometric Arrangement
q=εA[Stefan-BoltZ]SF(T14-T24)

Other formulas in Conduction, Convection and Radiation category

​Go Non Ideal Body Surface Emittance
e=ε[Stefan-BoltZ]Tw4
​Go Radiation energy emitted by black body per unit time and surface area
q'=[Stefan-BoltZ]T4
​Go Radiation energy emitted by black body in time interval given emissive power
E=EbSAN
​Go Radiation energy emitted by black body in time interval given temperature
E=[Stefan-BoltZ]T4SATotalΔt

How to Evaluate Black Bodies Heat Exchange by Radiation?

Black Bodies Heat Exchange by Radiation evaluator uses Heat Flux = Emissivity*[Stefan-BoltZ]*Area*(Temperature of Surface 1^(4)-Temperature of Surface 2^(4)) to evaluate the Heat Transfer, Black Bodies Heat Exchange by Radiation formula is defined as a measure of the net heat exchange per unit area between a black body and its surroundings due to thermal radiation, considering the emissivity, surface area, and temperatures of the two bodies. Heat Transfer is denoted by q symbol.

How to evaluate Black Bodies Heat Exchange by Radiation using this online evaluator? To use this online evaluator for Black Bodies Heat Exchange by Radiation, enter Emissivity (ε), Area (A), Temperature of Surface 1 (T1) & Temperature of Surface 2 (T2) and hit the calculate button.

FAQs on Black Bodies Heat Exchange by Radiation

What is the formula to find Black Bodies Heat Exchange by Radiation?
The formula of Black Bodies Heat Exchange by Radiation is expressed as Heat Flux = Emissivity*[Stefan-BoltZ]*Area*(Temperature of Surface 1^(4)-Temperature of Surface 2^(4)). Here is an example- 77.69741 = 0.95*[Stefan-BoltZ]*41*(101.01^(4)-91.114^(4)).
How to calculate Black Bodies Heat Exchange by Radiation?
With Emissivity (ε), Area (A), Temperature of Surface 1 (T1) & Temperature of Surface 2 (T2) we can find Black Bodies Heat Exchange by Radiation using the formula - Heat Flux = Emissivity*[Stefan-BoltZ]*Area*(Temperature of Surface 1^(4)-Temperature of Surface 2^(4)). This formula also uses Stefan-Boltzmann Constant .
What are the other ways to Calculate Heat Transfer?
Here are the different ways to Calculate Heat Transfer-
  • Heat Flux=Emissivity*Cross Sectional Area*[Stefan-BoltZ]*Shape Factor*(Temperature of Surface 1^(4)-Temperature of Surface 2^(4))OpenImg
Can the Black Bodies Heat Exchange by Radiation be negative?
Yes, the Black Bodies Heat Exchange by Radiation, measured in Power can be negative.
Which unit is used to measure Black Bodies Heat Exchange by Radiation?
Black Bodies Heat Exchange by Radiation is usually measured using the Watt[W] for Power. Kilowatt[W], Milliwatt[W], Microwatt[W] are the few other units in which Black Bodies Heat Exchange by Radiation can be measured.
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