Difficulty: Easy
Correct Answer: black body
Explanation:
Introduction / Context:
In thermal radiation, every surface is described by three fundamental radiative properties: absorptivity (α), reflectivity (ρ), and transmissivity (τ). Understanding the extreme cases helps students classify real materials and approximate them in engineering calculations.
Given Data / Assumptions:
Concept / Approach:
The definition of a black body is a surface that absorbs all incident radiant energy at every wavelength and direction. Therefore its α = 1. Because total must sum to 1, a black body necessarily has ρ = 0 and τ = 0. It is also the ideal emitter: its emissive power at a given temperature is the maximum possible among all bodies.
Step-by-Step Solution:
Verification / Alternative check:
Kirchhoff’s law at thermal equilibrium states emissivity equals absorptivity. If α = 1, emissivity = 1, matching the notion that a black body is also a perfect emitter (reference curve for radiation exchange).
Why Other Options Are Wrong:
Grey body: absorptivity/emissivity are constant with wavelength but less than 1.Opaque body: simply means τ = 0; it can still reflect. Here ρ = 0, so this is a special case, not the general term.White body: ideal reflector with ρ = 1, not consistent with α = 1.Translucent body: implies τ > 0, which contradicts τ = 0.
Common Pitfalls:
Confusing “black” in radiation with visible color; a surface may appear shiny black visually yet not behave as an ideal black body across all wavelengths.
Final Answer:
black body
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