Radiation emitted by small body Solution

STEP 0: Pre-Calculation Summary
Formula Used
Emitted Radiation = Emissivity*[Stefan-BoltZ]*(Temperature^4)
Eemit = ε*[Stefan-BoltZ]*(T^4)
This formula uses 1 Constants, 3 Variables
Constants Used
[Stefan-BoltZ] - Stefan-Boltzmann Constant Value Taken As 5.670367E-8
Variables Used
Emitted Radiation - (Measured in Watt per Square Meter) - Emitted Radiation is the radiation emitted by a body.
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.
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
Emissivity: 0.95 --> No Conversion Required
Temperature: 85 Kelvin --> 85 Kelvin No Conversion Required
STEP 2: Evaluate Formula
Substituting Input Values in Formula
Eemit = ε*[Stefan-BoltZ]*(T^4) --> 0.95*[Stefan-BoltZ]*(85^4)
Evaluating ... ...
Eemit = 2.81196866310406
STEP 3: Convert Result to Output's Unit
2.81196866310406 Watt per Square Meter --> No Conversion Required
FINAL ANSWER
2.81196866310406 2.811969 Watt per Square Meter <-- Emitted Radiation
(Calculation completed in 00.004 seconds)

Credits

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Vallurupalli Nageswara Rao Vignana Jyothi Institute of Engineering and Technology (VNRVJIET), Hyderabad
Sai Venkata Phanindra Chary Arendra has created this Calculator and 100+ more calculators!
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Shri Madhwa Vadiraja Institute of Technology and Management (SMVITM), Udupi
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Kirchhoff's Law Calculators

Temperature of Small Body using Absorptivity and Absorbed Radiation
​ LaTeX ​ Go Temperature = (Absorbed Radiation/([Stefan-BoltZ]*Absorptivity))^0.25
Temperature of Small Body given Emissivity and Emitted Radiation
​ LaTeX ​ Go Temperature = (Emitted Radiation/(Emissivity*[Stefan-BoltZ]))^0.25
Radiation Absorbed by Small Body Per Unit of its Surface Area
​ LaTeX ​ Go Absorbed Radiation = Absorptivity*[Stefan-BoltZ]*(Temperature^4)
Radiation emitted by small body
​ LaTeX ​ Go Emitted Radiation = Emissivity*[Stefan-BoltZ]*(Temperature^4)

Radiation emitted by small body Formula

​LaTeX ​Go
Emitted Radiation = Emissivity*[Stefan-BoltZ]*(Temperature^4)
Eemit = ε*[Stefan-BoltZ]*(T^4)

What is Kirchhoff law?

The total hemispherical emissivity of a surface at temperature T is equal to its total hemispherical absorptivity for radiation coming from a blackbody at the same temperature. This relation, which greatly simplifies the radiation analysis, was first developed by Gustav Kirchhoff in 1860 and is now called Kirchhoff’s law.

How to Calculate Radiation emitted by small body?

Radiation emitted by small body calculator uses Emitted Radiation = Emissivity*[Stefan-BoltZ]*(Temperature^4) to calculate the Emitted Radiation, Radiation emitted by small body formula is defined as the total energy radiated per unit surface area of a small body, which is proportional to the fourth power of its absolute temperature, and is a fundamental concept in understanding thermal radiation and its applications in various fields. Emitted Radiation is denoted by Eemit symbol.

How to calculate Radiation emitted by small body using this online calculator? To use this online calculator for Radiation emitted by small body, enter Emissivity (ε) & Temperature (T) and hit the calculate button. Here is how the Radiation emitted by small body calculation can be explained with given input values -> 2.811969 = 0.95*[Stefan-BoltZ]*(85^4).

FAQ

What is Radiation emitted by small body?
Radiation emitted by small body formula is defined as the total energy radiated per unit surface area of a small body, which is proportional to the fourth power of its absolute temperature, and is a fundamental concept in understanding thermal radiation and its applications in various fields and is represented as Eemit = ε*[Stefan-BoltZ]*(T^4) or Emitted Radiation = Emissivity*[Stefan-BoltZ]*(Temperature^4). 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 & Temperature is the degree or intensity of heat present in a substance or object.
How to calculate Radiation emitted by small body?
Radiation emitted by small body formula is defined as the total energy radiated per unit surface area of a small body, which is proportional to the fourth power of its absolute temperature, and is a fundamental concept in understanding thermal radiation and its applications in various fields is calculated using Emitted Radiation = Emissivity*[Stefan-BoltZ]*(Temperature^4). To calculate Radiation emitted by small body, you need Emissivity (ε) & Temperature (T). With our tool, you need to enter the respective value for Emissivity & 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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