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.
Mars' north polar cap looks like a gigantic spiral of ice and snow. Dark troughs are interspersed with ice-clad hills. This simulated overflight of the North Pole reveals its permanent ice cap and large Chasma Boreale truogh.
The latest images from the HRSC camera show a triple crater formed by asteroid impacts in the Terra Sirenum region on Mars. On the crater floor are layered deposits that indicate the long-term existence of a lake.
Huge masses of water once flowed over the surface of Mars to form one of the largest outflow channels on the planet – Kasei Valles. These images, acquired by the High Resolution Stereo Camera (HRSC) show a section of the mouth of this outflow channel system, which lies in the transition region where the Chryse Planitia lowlands merge into the Martian highlands.