The color temperature of a light source is the temperature of an ideal black-body radiator that radiates light of comparable hue to that of the light source. Color temperature is a characteristic of visible light that has important applications in lighting, photography, videography, publishing, manufacturing, astrophysics, horticulture,
and other fields. In practice, color temperature is only meaningful for
light sources that do in fact correspond somewhat closely to the
radiation of some black body, i.e., those on a line from reddish/orange
via yellow and more or less white to blueish white; it does not make
sense to speak of the color temperature of, e.g., a green or a purple
light. Color temperature is conventionally stated in the unit of
absolute temperature, the Kelvin, having the unit symbol K.
Color temperatures over 5,000K are called cool colors (bluish white), while lower color temperatures (2,700–3,000 K) are called warm colors (yellowish white through red).[1] This relation, however, is a psychological one in contrast to the physical relation implied by Wien's displacement law, according to which the spectral peak is shifted towards shorter wavelengths (resulting in a more blueish white) for higher temperatures. en.wikipedia.org/wiki/Color_temperature
Color temperatures over 5,000K are called cool colors (bluish white), while lower color temperatures (2,700–3,000 K) are called warm colors (yellowish white through red).[1] This relation, however, is a psychological one in contrast to the physical relation implied by Wien's displacement law, according to which the spectral peak is shifted towards shorter wavelengths (resulting in a more blueish white) for higher temperatures. en.wikipedia.org/wiki/Color_temperature