Wien's Law Formula:
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Color temperature is a characteristic of visible light that describes the color of light emitted by an idealized black-body radiator. It is measured in kelvins (K) and indicates whether light appears warm (yellow/red) or cool (blue).
The calculator uses Wien's displacement law:
Where:
Explanation: Wien's law states that the wavelength at which the emission of a black body peaks is inversely proportional to its temperature.
Details: Color temperature is crucial in photography, lighting design, display technology, and astronomy. It helps determine the quality and characteristics of light sources and their applications in various fields.
Tips: Enter the wavelength in nanometers (nm). The value must be greater than 0. Common visible light wavelengths range from 380 nm (violet) to 750 nm (red).
Q1: What is the relationship between wavelength and color temperature?
A: Shorter wavelengths correspond to higher color temperatures (bluer light), while longer wavelengths correspond to lower color temperatures (redder light).
Q2: What are typical color temperature values?
A: Candlelight: ~1800K, Incandescent bulbs: 2700-3000K, Daylight: 5000-6500K, Overcast sky: 6500-8000K.
Q3: Is this calculation accurate for all light sources?
A: This calculation is most accurate for black-body radiators. Real light sources may have different spectral distributions.
Q4: Can I use this for LED lighting?
A: While LEDs approximate black-body radiation, their actual color temperature may vary due to phosphor coatings and manufacturing processes.
Q5: What is the visible spectrum range?
A: The human eye typically perceives light between 380 nm (violet) and 750 nm (red), corresponding to color temperatures from approximately 7600K to 3900K.