Star Color Stars give off light at every wavelength, but peak in intensity at a certain wavelengths We can determine the color of a star by measuring the peak wavelength o Pass the light through a spectrograph (measures light intensity at each wavelength) o Pass the light through a color filter (only let light pass through at certain wavelengths) and measure the wavelength intensity Most common color filters are U (ultraviolet), B (blue), and V (photovisual) Wavelength vs. Intensity (Figure 24-2) o Radiation follows a fairly smooth curve o Peak in radiation intensity at certain wavelengths o Each line represents a different star (with different Temperatures) Notice the hotter stars peak in the blue (they appear to be the color blue in the sky) and cooler stars peak in the red Blue hot is hotter than red hot Star Color and Temperature There is a set of physical laws that govern this relationship o Planck's law dictates the peak intensity of the radiation Considers stars close to an idealized case of a blackbody something that absorbs all the radiation that falls on it (perfect absorber and perfect emitter) o Wein's displacement law relates temperature to wavelength λmax T = constant In other words: If T increases, λmax decreases If T decreases, λmax increases Example: If Star A has a Temperature of 10,000 K and a wavelength twice that of Star B, what is Star B's Temperature? o Stefan-Boltzmann law relates energy emitted with temperature Energy = σ T4 Note that if temperature increases even slightly, energy output increases greatly Example: If a star's temperature doubles, how much more energy will it be giving off?