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The above is an attempt to render the visible spectrum on your monitor. Different wavelengths of light (λ, from .380 μm to .750 μm) are seen by the human eye as different colors (V=violet, B=blue, G=green, Y=yellow, O=orange, R=red). For the following questions, you should assume blue light corresponds to a wavelength of .450 μm, green light corresponds to a wavelength of .550 μm, and red light corresponds to a wavelength of .700 μm. Of course there is a continuum of color variation across the color spectrum.
The following plots (called spectra, or spectral energy distributions) display the amount of light energy as a function of wavelength. The y-axis has been labeled "Energy Flux". Properly speaking it is "spectral irradiance" but is often labeled "Intensity" in textbooks. You can think of it as the amount of light energy (watts) of a particular wavelength (μm) hitting a square meter (m2). When we need a symbol to denote this quantity we will denote it as Fλ.
This quiz deals exclusively with ideal "blackbody" spectra. The light you would receive from such an object just depends on the object's radius, distance from you, and temperature. The next quiz will deal with more complex spectra, like that from the Sun.
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