What is emissive power of perfectly black body at 1000k
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A black body, is an ideal object that perfectly obeys the laws of thermal radiation.
- A black body refers to a thermal radiation-emitting opaque artifact. A perfect black body is one that absorbs and reflects none of the incoming light. Such an object would seem completely black at room temperature
- The emissivity of the black body in thermal equilibrium is ε = 1.0. A source with lower emissivity is often referred to as a gray body, regardless of frequency. Thus, T1 = 1000°C + 273 = 1273 K
- A black body's total emissive power Eb is the total radiant energy released by the black body in all directions over the whole range of wavelengths (λ = 0 – ∞) per unit area per unit time.
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