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

STEP 0: Pre-Calculation Summary
Formula Used
Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25
T = (E/([Stefan-BoltZ]*SATotal*Δt))^0.25
This formula uses 1 Constants, 4 Variables
Constants Used
[Stefan-BoltZ] - Stefan-Boltzmann Constant Value Taken As 5.670367E-8
Variables Used
Temperature - (Measured in Kelvin) - The Temperature is a measure of the thermal energy of a system, indicating how hot or cold it is, which affects heat emission due to radiation.
Energy - (Measured in Joule) - The Energy is the heat emitted by a body due to radiation, reflecting the transfer of thermal energy through electromagnetic waves.
Total Surface Area - (Measured in Square Meter) - The Total Surface Area is the sum of all external surfaces of an object, influencing heat emission and absorption in thermal radiation processes.
Time Interval or Time Period - (Measured in Second) - The Time Interval or Time Period is the duration over which heat radiation emission is measured, reflecting the time taken for energy transfer through radiation.
STEP 1: Convert Input(s) to Base Unit
Energy: 240 Joule --> 240 Joule No Conversion Required
Total Surface Area: 53 Square Meter --> 53 Square Meter No Conversion Required
Time Interval or Time Period: 1.25 Second --> 1.25 Second No Conversion Required
STEP 2: Evaluate Formula
Substituting Input Values in Formula
T = (E/([Stefan-BoltZ]*SATotal*Δt))^0.25 --> (240/([Stefan-BoltZ]*53*1.25))^0.25
Evaluating ... ...
T = 89.4032996234355
STEP 3: Convert Result to Output's Unit
89.4032996234355 Kelvin --> No Conversion Required
FINAL ANSWER
89.4032996234355 89.4033 Kelvin <-- Temperature
(Calculation completed in 00.004 seconds)

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Heat Emission due to Radiation Calculators

Heat Exchange by Radiation due to Geometric Arrangement
​ LaTeX ​ Go Heat Flux = Emissivity*Cross Sectional Area*[Stefan-BoltZ]*Shape Factor*(Temperature of Surface 1^(4)-Temperature of Surface 2^(4))
Black Bodies Heat Exchange by Radiation
​ LaTeX ​ Go Heat Flux = Emissivity*[Stefan-BoltZ]*Cross Sectional Area*(Temperature of Surface 1^(4)-Temperature of Surface 2^(4))
Non Ideal Body Surface Emittance
​ LaTeX ​ Go Real Surface Radiant Surface Emittance = Emissivity*[Stefan-BoltZ]*Surface Temperature^(4)
Radiation energy emitted by black body per unit time and surface area
​ LaTeX ​ Go Radiation Energy Emmited by Black Body = [Stefan-BoltZ]*Temperature^4

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

​LaTeX ​Go
Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25
T = (E/([Stefan-BoltZ]*SATotal*Δt))^0.25

What is Temperature?

Temperature is a physical quantity that expresses hot and cold. It is the manifestation of thermal energy, present in all matter, which is the source of the occurrence of heat, a flow of energy when a body is in contact with another that is colder or hotter.

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

Temperature of black body to emit certain amount of radiation energy calculator uses Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25 to calculate 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 calculate Temperature of black body to emit certain amount of radiation energy using this online calculator? To use this online calculator 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. Here is how the Temperature of black body to emit certain amount of radiation energy calculation can be explained with given input values -> 89.4033 = (240/([Stefan-BoltZ]*53*1.25))^0.25.

FAQ

What is Temperature of black body to emit certain amount of radiation energy?
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 and is represented as T = (E/([Stefan-BoltZ]*SATotal*Δt))^0.25 or Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25. The Energy is the heat emitted by a body due to radiation, reflecting the transfer of thermal energy through electromagnetic waves, The Total Surface Area is the sum of all external surfaces of an object, influencing heat emission and absorption in thermal radiation processes & The Time Interval or Time Period is the duration over which heat radiation emission is measured, reflecting the time taken for energy transfer through radiation.
How to calculate Temperature of black body to emit certain amount of radiation energy?
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 is calculated using Temperature = (Energy/([Stefan-BoltZ]*Total Surface Area*Time Interval or Time Period))^0.25. To calculate Temperature of black body to emit certain amount of radiation energy, you need Energy (E), Total Surface Area (SATotal) & Time Interval or Time Period (Δt). With our tool, you need to enter the respective value for Energy, Total Surface Area & Time Interval or Time Period 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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