The european Mars Express mission, which was launched on 2 June 2003, is providing important new data on the geology, mineralogy and atmosphere of Mars. Mars Express is giving us information about the history of the Red Planet’s climate and explaining the role and whereabouts of water on the planet. Thanks to the High Resolution Stereo Camera (HRSC) developed in DLR's Institute of Planetary Research, Mars is being mapped in three dimensions and colour for the first time.
The Mars Express HRSC images are now published under a Creative Commons licence: ESA/DLR/FU Berlin, CC BY-SA 3.0 IGO.
Join us on a trip to our planetary neighbour. See breathtakingly beautiful pictures of its surface. Find out more about its geology, climatic history and moons, and learn about the history of its exploration.
Grabens, dendritic valleys, lava flows and the largest volcano in the Solar System – Amazing 3D animation of the Red Planet to celebrate 10 years of the Mars Express mission.
A wealth of information about Mars, its surface, subsurface and atmosphere has led to a completely new view of the Red Planet.
The images shown in this gallery were generated at the Institute for Geological Sciences at the Freie Universität Berlin and published there as 'Highlights of the Month' in 2011. They present special Mars products obtained using the HRSC camera on board Mars Express.
Today, Mars appears bone-dry and dusty – but new analyses of Istok crater provide evidence of periodic flows of debris from its walls into its interior. "What is surprising is that it must have happened reasonably often," explains Ernst Hauber, a planetary researcher at the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR).
At present, the Siloe Patera construct in the Martian highlands is the cause of much debate among scientists. Is Siloe Patera actually the remains of a supervolcano? There is evidence to suggest this – but also evidence against it. It is a current example of an interesting geoscientific debate.
On our neighbouring planet Mars, it is mainly wind – through its force and the dust and sand particles it carries – that shapes the terrain structures, wearing them away over the course of millions of years.