The kelvin is often used in the measure of the
colour temperature of light sources. Colour temperature is based upon the principle that a
black body radiator emits light of which the colour depends on the temperature of the radiator. Black bodies with temperatures below about 4000 K appear reddish whereas those above about 7500 K appear bluish. Colour temperature is important in the fields of image projection and
photography where a colour temperature of approximately 5600 K is required to match "daylight" film emulsions. In
astronomy, the
stellar classification of stars and their place on the
Hertzsprung–Russell diagram are based, in part, upon their surface temperature, known as
effective temperature. The photosphere of the
Sun, for instance, has an effective temperature of 5778 K.