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This equation tells us that the peak wavelength (color) emitted by a star is inversely proportional to the Kelvin (absolute) temperature of that star. Group
This equation tells us that the peak wavelength (color) emitted by a star is inversely proportional to the Kelvin (absolute) temperature of that star. Group of answer choices Wein's law Stefan-Boltzmann law parallax equation Kirchoff's law E = mc2
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