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Why Mars looks red, but its rocks are not all red

Curiosity's colour-corrected mosaic of the brown layered Mont Mercou cliff on Mars beneath pale clouds after sunset

Oxidized iron minerals colour fine dust that coats and circulates around Mars. Rover samples reveal a more varied planet beneath that familiar appearance.

Mars gets much of its reddish appearance from fine dust containing oxidized iron minerals. That dusty coating, spread across the ground and lifted into the atmosphere, can dominate our view without making every rock beneath it red.

Curiosity's colour-corrected mosaic of the brown layered Mont Mercou cliff on Mars beneath pale clouds after sunset
Mont Mercou in Gale Crater, photographed by Curiosity's Mastcam just after sunset on March 19, 2021. This mission-produced mosaic combines 21 images and is colour-corrected for a human-eye-like view. It provides landscape context; a photograph alone does not identify its minerals. Cover and image: NASA/JPL-Caltech/Malin Space Science Systems (MSSS), PIA24622; released May 28, 2021. Image and processing details; MSSS news-media terms; JPL image-use policy. No SpaceEve alteration.Click to enlarge.

A planet-wide appearance from fine material

Iron is part of the chemistry of Martian rocks. When it reacts with oxygen-bearing substances, it can form different iron oxides and related minerals. These altered materials help give the dust its rusty colour. The comparison with rust describes the chemistry; it does not mean modern Mars has Earth's wet, oxygen-rich conditions.

Winds break up, mix and redistribute surface material. Dust also enters the atmosphere, helping make Mars look broadly reddish from a distance. Up close, the ground includes brown, tan, gold and gray materials. A thin, widespread coating can make a diverse landscape look more uniform.

Curiosity found a different colour inside a rock

In February 2013, Curiosity drilled a rock named John Klein in Gale Crater. Its Mastcam photograph shows gray-green powder in the rover's scoop, alongside red residue left by an earlier dust-and-sand sample from Rocknest.

White-balanced Curiosity Mastcam image of gray-green John Klein drill powder in a metal scoop, with red Rocknest residue on the scoop wall
Gray-green John Klein drill powder sits in Curiosity's scoop on February 20, 2013. The red residue on its wall came from the earlier Rocknest dust-and-sand sample. This is a mission white-balanced image, representing Earth-like lighting; it is not a before-and-after view of the Mont Mercou cliff. Image: NASA/JPL-Caltech/Malin Space Science Systems (MSSS), PIA16729; released February 20, 2013. Sample identity and processing; MSSS news-media terms; JPL image-use policy. No SpaceEve alteration.Click to enlarge.

The mission team's description of the sample connects that difference to the oxidation state of iron: the John Klein powder was less oxidized. Gray material can still contain iron. Colour depends on its chemical form and surrounding minerals, rather than simply on whether iron is present.

Which kind of rust colours the dust?

Iron oxides are a family of materials, rather than a single red ingredient. Identifying their exact mixture matters because different minerals can record different environmental histories.

A study published in Nature Communications on February 25, 2025 compared orbital and rover spectra with laboratory mixtures. Its authors found that very fine ferrihydrite mixed with basalt and sulfate best matched Martian dust observations. Ferrihydrite is a water-bearing iron mineral, so they interpreted its persistence as evidence for ancient cold, wet alteration followed by drying.

That is a reconstruction based on mineral signatures, experiments and calculations. It does not establish water flowing today or evidence of life. The mission account of the research explains why the mineral question goes beyond the simple label “rust.”

Reading the colours in rover pictures

Lighting, camera response and image processing also affect colour. The scoop image is white-balanced to show materials under Earth-like illumination. The Mont Mercou landscape is a separate, colour-corrected mosaic from 2021, taken after sunset; its appearance should not be compared with the 2013 powder as if they were matched samples.

Pictures reveal useful contrasts, but instruments that measure how light varies with wavelength, and tools that analyse composition, provide stronger tests of mineral identity. Mars's red appearance is a clue to widespread surface alteration, not a complete description of the planet's rocks.

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