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Titan Colours & Palettes

Moons · Moon

Titan’s golden haze: a natural-colour view of a moon whose surface is hidden in visible light.

Titan: Cassini natural-colour composite
Cassini natural-colour composite Approximate visible appearance
Credit: NASA/JPL/Space Science Institute. · released 2005-04-22

About Titan

Titan, Saturn’s largest moon, has an atmosphere of about 95% nitrogen and 5% methane. Sunlight and energetic particles break those molecules apart, making a thick orange haze that hides the surface from view.

Facts, with what each measures
ClassificationMoon
Parent bodySaturn
Mean radius2,574.8 km ± 0.02 kmmean radius · NASA JPL Solar System Dynamics
Orbital period15.9 daysorbital period around Saturn · mean elements, epoch 2000-01-01.5 TDB · NASA JPL Solar System Dynamics

Why these colours?

All haze

Cassini’s natural-colour composite shows only the atmosphere: a smooth golden-orange ball. The surface is seen only at wavelengths outside human vision.

From: Cassini natural-colour composite Approximate visible appearance

Colour clusters describe pixels in an image; they cannot identify a mineral, a gas or a physical temperature. Shares of pixels describe the sampled region of the image, not the object’s surface.

Colours from selected views

Palettes sampled from identified images and regions, or calculated from a documented model. These values describe each image or model, not one permanent colour of Titan.

Cassini natural-colour composite

Sampled from this image · Cassini natural-colour composite

  • #A38536RGB 163, 133, 54region average
  • #0F0D08RGB 15, 13, 819% of the region
  • #EFC64FRGB 239, 198, 7918% of the region
  • #C69F41RGB 198, 159, 6518% of the region
  • #987A34RGB 152, 122, 5216% of the region
  • #372E18RGB 55, 46, 2415% of the region
  • #675326RGB 103, 83, 3815% of the region
See where these colours came from
Cassini natural-colour composite
  • View: Cassini natural-colour composite (Approximate visible appearance)
  • Image file: img/nasa-pia06230.jpg, sha256 b7c651c7b2e98739…
  • Region: x 12.7%, y 13.6%, 64.9% × 74.9% of the image. Region: bounding box of the object; sky pixels darker than OKLab L 0.10 excluded.
  • Method: k-means clustering in OKLab, pcke-oklab-kmeans-1; colours measured from the published file.

Creative palettes inspired by Titan

A design derived from the selected representation. It is not a scientific colour measurement. Each colour keeps the sampled colour it was made from.

Titan Haze

Inspired by this object

  • #73716ERGB 115, 113, 110from #0F0D08
  • #EFD9A0RGB 239, 217, 160from #EFC64F
  • #DAC597RGB 218, 197, 151from #C69F41
  • #C2B28ERGB 194, 178, 142from #987A34
  • #8C8679RGB 140, 134, 121from #372E18
  • #A89C83RGB 168, 156, 131from #675326

Titan’s golden haze softened into warm neutrals.

Explore the views

Titan: Cassini natural-colour composite
NASA describes this as a natural-colour composite: the orange is Titan’s thick hazy atmosphere. Processing by the mission team affects colour.

No supported 3D model is available for this view. You can still inspect the source imagery and palette.

Use these colours

Every palette above opens in the palette generator. With JavaScript you can also add colours to your cosmic palette, save them, make a gradient or pattern, preview them in a design or a room (you choose which colour goes on which surface), check digital accessibility and export them. Each colour keeps the view and sample it came from.

Paint matches compare digital swatches for design inspiration. They are not physical equivalents of light from space. Edits create a new design palette. The original representation remains unchanged.

Questions about Titan’s colours

Why can’t we see Titan’s surface?

Its orange haze blocks visible light; instruments see through it only at other wavelengths.

Sources

Image credits

  • Cassini natural-colour composite: NASA/JPL/Space Science Institute. NASA media (not copyrighted; see the NASA image and media guidelines). Resized for the web from the publisher’s file (sha256 96c7c1f99bb609655014f9586428b20168c5e5825a5db98dedfceb598fb86942).

Images were resized once for the web; colours were measured from the published files (k-means in OKLab, pcke-oklab-kmeans-1); calculated colours use the CIE 1931 2° observer. Facts last reviewed 25 October 2026. Catalogue pcke-cosmos-2026-10-25, page revision aad30f5525a7. No ESA, ESO or NASA endorsement is implied.

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