Color Temperature Converter – Kelvin, Mired, and White Balance
Colour temperature is one of the most practical concepts in photography, cinematography, and lighting design. It describes the hue of a light source by comparing it to the colour emitted by a theoretical black-body radiator heated to a given absolute temperature. This converter lets you switch between Kelvin (K) and Mired (micro reciprocal degree), identify the real-world light source associated with a value, and find the nearest camera white-balance preset — all in a single step.
What Is Kelvin in the Context of Light?
Kelvin measures the colour appearance of a light source on a scale that runs from warm orange-red at the low end to cool blue-white at the high end. Common reference points:
- 1800–2000 K — candlelight, very warm amber glow
- 2700–3200 K — incandescent and tungsten bulbs, the familiar warm light of older household lamps and studio tungsten fixtures
- 4000 K — cool white fluorescent tubes, neutral office lighting
- 5200–5500 K — direct noon sunlight and electronic flash, the standard for "daylight" colour in cameras and film stock
- 6500 K — overcast sky, slightly blue-tinted
- 7500 K — open shade under a clear blue sky, noticeably cool
Counterintuitively, higher Kelvin values produce cooler, bluer light while lower values produce warmer, more amber light. This is because the physics of thermal radiation means that hotter objects glow blue-white, while cooler objects glow orange-red.
What Is Mired?
Mired (pronounced "MY-red") stands for micro reciprocal degree and is calculated as Mired = 1,000,000 / K. The inverse relationship means that lower Kelvin values (warmer light) have higher Mired values, and higher Kelvin values (cooler light) have lower Mired values.
The Mired scale is widely used in photographic filter and gel systems because equal numerical differences in Mired represent perceptually equal shifts in colour appearance across the entire Kelvin range. A shift of 50 Mired looks the same to the human eye whether you are moving from 2000 K to 2083 K or from 6000 K to 6383 K. In the Kelvin scale, those intervals are very different in size, making gel selection inconsistent.
Kelvin to Mired Conversion Formula
The conversion is a simple reciprocal calculation:
Mired = 1,000,000 ÷ KK = 1,000,000 ÷ Mired
Example: 5500 K = 1,000,000 ÷ 5500 = 181.82 Mired. Conversely, 181.82 Mired = 1,000,000 ÷ 181.82 = 5500 K.
Camera White Balance Presets
Most digital cameras offer fixed white-balance presets that correspond to standard Kelvin values:
- Tungsten / Incandescent (~3200 K, ~313 Mired) — removes the orange cast from household and studio tungsten lighting.
- Fluorescent (~4000 K, ~250 Mired) — compensates for the green tint of older fluorescent tubes.
- Daylight (~5200 K, ~192 Mired) — calibrated for direct sunlight in the middle of the day.
- Flash (~5500 K, ~182 Mired) — matches the colour output of most on-camera and studio strobes.
- Cloudy (~6000 K, ~167 Mired) — warms up the slightly blue cast of overcast skies.
- Shade (~7500 K, ~133 Mired) — corrects the strongly blue light in open shade under a clear sky.
Mired Shift and Photographic Gels
A Mired shift is the Mired difference between two colour temperatures. It tells you exactly which type and strength of correction gel to place over a light to match your target. The formula is:
Mired Shift = Mired(target) − Mired(source)
A positive shift (target is warmer / lower K) calls for a CTO (colour temperature orange) gel. A negative shift (target is cooler / higher K) calls for a CTB (colour temperature blue) gel. For example, converting a 5600 K daylight source to 3200 K tungsten requires a +131 Mired CTO gel.
Approximate Colour Swatch
This tool renders an approximate colour swatch for any entered Kelvin value using the Tanner Helland Planckian locus algorithm, which curve-fits the sRGB coordinates of a theoretical black body across the visible-light temperature range. The swatch is a visual guide only — actual perceived colour depends on your display calibration, ambient lighting, and the specific light source involved.
Practical Uses
The colour temperature converter is useful for:
- Photographers converting Kelvin to Mired when selecting Lee or Rosco correction filters for their lenses.
- Cinematographers calculating the gel needed to match practical tungsten fixtures with HMI daylight sources on a set.
- Lighting designers specifying LED fixtures or mixing light sources of different colour temperatures in architectural installations.
- Display calibration professionals checking whether a monitor's white point (typically 6500 K or D65) matches a particular printing standard.
- Students and educators learning the relationship between Kelvin, Mired, and perceived light colour in optics or photography courses.
Accuracy and Limitations
All arithmetic uses JavaScript double-precision floating-point, which is accurate to approximately 15 significant digits — far beyond any practical need for colour-temperature work. The light-source identification uses broadly accepted Kelvin ranges; your specific bulb or fixture may differ slightly from the listed range. The colour swatch is an approximation of a perfect black-body radiator and will not match real-world sources exactly — use it as a directional guide rather than a precise colour reference.