A gray body is defined such that
Monochromatic emissivity of the body is independent of wave length
A gray body is a useful model in thermal radiation studies. It represents an idealized surface whose radiative properties are simpler than those of real surfaces.
The key characteristic defining a gray body relates to its monochromatic emissivity ($\epsilon_{\lambda}$). Monochromatic emissivity is the ratio of the radiation emitted by a surface at a specific wavelength to the radiation emitted by a blackbody at the same wavelength and temperature.
For an idealized gray body, this monochromatic emissivity ($\epsilon_{\lambda}$) is constant and does not change with the wavelength ($\lambda$) of the radiation. Mathematically, this is represented as:
$$ \epsilon_{\lambda}(\lambda, T) = \epsilon = \text{constant} $$
This means that a gray body emits and absorbs radiation proportionally less than a blackbody across all wavelengths, with the same proportionality factor ($\epsilon$) applying universally.
Let's evaluate the given options based on this definition:
In essence, a gray body simplifies radiation analysis by assuming that its emissivity value is constant regardless of the wavelength of radiation. This makes calculations involving heat transfer by radiation more manageable, although it is an idealization.
If plate 1 is also a diffuse and gray surface with an emissivity value of 0.8, the net radiation heat exchange (in kW/m2) between plate 1 and plate 2 is
For an opaque surface, the absorptivity (α) , transitivity (τ) and reflectivity (ρ) are related by the equation
In a radiative heat transfer, a gray surface is one