Temperature of black body to emit certain amount of radiation energy Formula

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Temperature is the degree or intensity of heat present in a substance or object. Check FAQs
T=(E[Stefan-BoltZ]SATotalΔt)0.25
T - Temperature?E - Energy?SATotal - Total Surface Area?Δt - Time Interval or Time Period?[Stefan-BoltZ] - Stefan-Boltzmann Constant?

Temperature of black body to emit certain amount of radiation energy Example

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Here is how the Temperature of black body to emit certain amount of radiation energy equation looks like with Values.

Here is how the Temperature of black body to emit certain amount of radiation energy equation looks like with Units.

Here is how the Temperature of black body to emit certain amount of radiation energy equation looks like.

89.4033Edit=(240Edit5.7E-853Edit1.25Edit)0.25
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Temperature of black body to emit certain amount of radiation energy Solution

Follow our step by step solution on how to calculate Temperature of black body to emit certain amount of radiation energy?

FIRST Step Consider the formula
T=(E[Stefan-BoltZ]SATotalΔt)0.25
Next Step Substitute values of Variables
T=(240J[Stefan-BoltZ]531.25s)0.25
Next Step Substitute values of Constants
T=(240J5.7E-8531.25s)0.25
Next Step Prepare to Evaluate
T=(2405.7E-8531.25)0.25
Next Step Evaluate
T=89.4032996234355K
LAST Step Rounding Answer
T=89.4033K

Temperature of black body to emit certain amount of radiation energy Formula Elements

Variables
Constants
Temperature
Temperature is the degree or intensity of heat present in a substance or object.
Symbol: T
Measurement: TemperatureUnit: K
Note: Value can be positive or negative.
Energy
Energy is the amount of work done.
Symbol: E
Measurement: EnergyUnit: J
Note: Value can be positive or negative.
Total Surface Area
Total Surface Area is the total area of the surface of a three-dimensional object.
Symbol: SATotal
Measurement: AreaUnit:
Note: Value should be greater than 0.
Time Interval or Time Period
Time interval or time period is the time duration between two events/entities of interest.
Symbol: Δt
Measurement: TimeUnit: s
Note: Value should be greater than 0.
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 in Heat Emission due to Radiation category

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

How to Evaluate Temperature of black body to emit certain amount of radiation energy?

Temperature of black body to emit certain amount of radiation energy evaluator uses Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25 to evaluate the Temperature, Temperature of black body to emit certain amount of radiation energy formula is defined as the temperature at which a black body emits a certain amount of radiation energy, which is dependent on the energy emitted, the Stefan-Boltzmann constant, the total surface area, and the time duration. Temperature is denoted by T symbol.

How to evaluate Temperature of black body to emit certain amount of radiation energy using this online evaluator? To use this online evaluator for Temperature of black body to emit certain amount of radiation energy, enter Energy (E), Total Surface Area (SATotal) & Time Interval or Time Period (Δt) and hit the calculate button.

FAQs on Temperature of black body to emit certain amount of radiation energy

What is the formula to find Temperature of black body to emit certain amount of radiation energy?
The formula of Temperature of black body to emit certain amount of radiation energy is expressed as Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25. Here is an example- 89.4033 = (240/([Stefan-BoltZ]*53*1.25))^0.25.
How to calculate Temperature of black body to emit certain amount of radiation energy?
With Energy (E), Total Surface Area (SATotal) & Time Interval or Time Period (Δt) we can find Temperature of black body to emit certain amount of radiation energy using the formula - Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25. This formula also uses Stefan-Boltzmann Constant .
Can the Temperature of black body to emit certain amount of radiation energy be negative?
Yes, the Temperature of black body to emit certain amount of radiation energy, measured in Temperature can be negative.
Which unit is used to measure Temperature of black body to emit certain amount of radiation energy?
Temperature of black body to emit certain amount of radiation energy is usually measured using the Kelvin[K] for Temperature. Celsius[K], Fahrenheit[K], Rankine[K] are the few other units in which Temperature of black body to emit certain amount of radiation energy can be measured.
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