درجة حرارة اللون في الفلك. In astronomy, the color temperature is defined by the local slope of the SPD at a given wavelength, or, in practice, a wavelength range.Given, for example, the color magnitudes B and V which are calibrated to be equal for an A0V star (e.g. Vega), the stellar color temperature is given by the temperature for which the color index of a black-body ...
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