The formula to calculate the Black-Body Radiant Emittance is:
\[ e_b = \sigma \cdot T^4 \]
Where:
Black-Body Radiant Emittance is the radiant flux emitted by a surface per unit area.
Let's assume the following value:
Using the formula:
\[ e_b = 5.670367E-8 \cdot 85^4 \]
Evaluating:
\[ e_b = 2.95996701379375 \text{ W/m²} \]
The Black-Body Radiant Emittance is 2.95996701379375 W/m².
| Temperature (K) | Black-Body Radiant Emittance (W/m²) |
|---|---|
| 80 | 2.322582323200 |
| 81 | 2.440907062166 |
| 82 | 2.563696307886 |
| 83 | 2.691060972738 |
| 84 | 2.823113329989 |
| 85 | 2.959967013794 |
| 86 | 3.101737019195 |
| 87 | 3.248539702123 |
| 88 | 3.400492779397 |
| 89 | 3.557715328724 |
| 90 | 3.720327788700 |