Difficulty: Easy
Correct Answer: all of these
Explanation:
Introduction / Context:
Emissive power characterizes how much thermal radiation a surface emits. For real (non-black) bodies, several variables influence emission.
Given Data / Assumptions:
Concept / Approach:
Blackbody emission depends only on temperature (E_b = σT^4). Real surfaces have emissivity ε that depends on wavelength, temperature, and surface condition (oxidation, roughness, finish), so E = ε(λ,T,material) * σT^4 (integrated over spectrum).
Step-by-Step Solution:
Recognize temperature drives the σT^4 magnitude.Acknowledge physical nature (polished vs. oxidized) alters ε.Wavelength dependence means spectral emissive power varies across λ.
Verification / Alternative check:
Spectral emissivity charts show strong dependence on wavelength and surface finish for metals and ceramics.
Why Other Options Are Wrong:
Common Pitfalls:
Assuming a constant ε across all wavelengths; using blackbody assumption for shiny metals, leading to large errors.
Final Answer:
all of these
Discussion & Comments