The CIE 1960 UCS does not define a luminance or lightness component, but the Y tristimulus value of the XYZ color space or a lightness index similar to W* of the CIE 1964 color space are sometimes used.
Today, the CIE 1960 UCS is mostly used to calculate correlated color temperature, where the isothermal lines are perpendicular to the Planckian locus. As a uniform chromaticity space, it has been superseded by the CIE 1976 UCS.
Background
Judd determined that a more uniform color space could be found by a simple projective transformation of the CIEXYZ tristimulus values:
(Note: What we have called "G" and "B" here are not the G and B of the CIE 1931 color space and in fact are "colors" that do not exist at all.)
Judd was the first to employ this type of transformation, and many others were to follow. Converting this RGB space to chromaticities one finds[clarification needed The following formulae do not agree with u=R/(R+G+B) and v=G/(R+G+B)]
Relation to CIE XYZ
U, V, and W can be found from X, Y, and Z using:
Going the other way:
We then find the chromaticity variables as:
We can also convert from u and v to x and y:
Relation to CIELUV
Source From Wikipedia
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