Calculate Color Temperature
Wien's displacement law for temperature and peak wavelength
Color Temperature Calculator (JavaScript)
Wien's law
For blackbody radiation, λmax·T = b with b = 2.897771955·10⁻³ m·K.
Example calculations
Example 1: Solar surface
Given: T = 5778 K
Result: λmax ≈ 501 nm
Example 2: Incandescent lamp
Given: T = 2700 K
Result: λmax ≈ 1073 nm (near infrared)
Example 3: Temperature from λmax
Given: λmax = 650 nm
Result: T ≈ 4458 K
Formulas and comprehensive description
Wien's displacement law describes the relation between blackbody temperature and wavelength of maximum emission. Higher temperatures shift the maximum toward shorter wavelengths. This is central for astrophysics, spectral analysis, and lighting engineering.
Wien law
Temperature
Peak wavelength
Displacement constant
Practical relevance
Description
What is Color Temperature?
Color temperature is a measure of the color of light emitted by a radiation source. It is based on the physical property that hot objects (blackbodies) emit light in various colors. Color temperature is measured in Kelvin (K) and describes the temperature at which an ideal blackbody would emit light of the same color as the observed light source.
Wien's Displacement Law
Wien's displacement law (named after Wilhelm Wien) describes the fundamental relationship between the temperature of an ideal radiator and the wavelength of its maximum radiation:
- λmax – wavelength of maximum radiation in meters (m)
- T – absolute temperature in Kelvin (K)
- b – Wien's displacement constant ≈ 2.898 × 10⁻³ m·K
Physical Interpretation
The higher the temperature, the shorter the wavelength of maximum radiation:
- Low temperatures (1000–3000 K): Maximum in red/infrared range → warm, reddish light (e.g., incandescent bulbs)
- Medium temperatures (4000–6000 K): Maximum in yellow-white range → neutral light (e.g., sunlight, 5778 K)
- High temperatures (7000–10000 K): Maximum in blue range → cool, bluish light (e.g., clear sky)
- Very high temperatures (>10000 K): Maximum in UV range → very blue light (e.g., hot stars)
Typical Color Temperatures of Light Sources
| Light Source | Color Temperature (K) | Characterization |
|---|---|---|
| Candlelight | 1900 K | Very warm, deep orange |
| Incandescent bulb (40W) | 2500 K | Warm, yellow-orange |
| Incandescent bulb (100W) | 2700 K | Warm, yellow |
| Halogen lamp | 3200 K | Warm-white |
| Daylight (9 AM, 3 PM) | 4000–5000 K | Neutral-white |
| Sunlight (Noon) | 5778 K | Neutral-white |
| Overcast sky | 6500 K | Cool-white |
| Clear sky (Noon) | 7500 K | Bluish-white |
| Clear sky (Horizon) | 10000 K | Strongly bluish |
Practical Applications
- Photography and film: White balance is adjusted to match the color temperature of the light source
- Lighting engineering: Selection of lamps for different rooms and moods
- Astronomy: Determination of stellar surface temperature (e.g., Sun: 5778 K, red giants: 3000 K, blue supergiants: >30000 K)
- Thermography: Temperature measurement via infrared radiation
- Display technology: Color temperature settings for screens and monitors
Notes on Blackbody Assumption
Wien's displacement law applies exactly to ideal blackbodies. Real light sources deviate from this, but generally follow this law approximately. Phosphors and LED lamps can have artificially generated color temperatures that do not correspond to thermal radiation, but are still specified in Kelvin (correlated color temperature).
Note
|
|
|
|