This new image of the Mawrth Vallis region on Mars reveals a world rich in iron, magnesium and aluminium.
Cameras orbiting Mars can capture more colours than our eyes can see. The European Colour and Stereo Surface Imaging System (CaSSIS) onboard the ExoMars Trace Gas Orbiter (TGO) reveals a striking diversity of colour.
This CaSSIS image exposes yellow layers containing iron and magnesium-rich clays, overlain by white and blue layers rich in aluminium. Some heavily eroded layers appear dark.
The metallic colours of this vibrant landscape tell a story of mineralogical diversity that started around 3.6 billion years ago. The area is located south of the dichotomy boundary – a ridge that encircles Mars, marking where the southern highlands meet the northern lowlands. Mawrth Vallis continues to intrigue scientists with its geological complexity. Liquid water did once run through this area, which was shortlisted as one of the most promising landing sites for the ExoMars Rosalind Franklin rover Another region, Oxia Planum, was chosen as the spot where Rosalind Franklin will hunt for signs of life.
In the meantime, TGO keeps gathering information from orbit around Mars to understand its ancient past and potential habitability. TGO’s full science mission began in 2018. The spacecraft is not only returning spectacular images, but also providing the best inventory of the planet’s atmospheric gases and mapping the planet’s surface for water-rich locations. Understanding the history of water on Mars and if this once allowed life to flourish is at the heart of ESA’s ExoMars missions.
TGO captured this image on 11 February 2024m, centred at 18.8°W, 24.4°N.