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.
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.
A wealth of information about Mars, its surface, subsurface and atmosphere has led to a completely new view of the Red Planet.
This animation shows a flight over the region of the Chasmata Melas, Candor and Ophir in the central part of Valles Marineris. 'Chasma' (= Greek for "fissure/canyon", plural 'chasmata') refers to deep valleys and canyons on Mars and Venus bound by steep cliff faces.
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.
The richly varied terrain of Hellespontus Montes on Mars is showcased in these images, acquired by the High Resolution Stereo Camera (HRSC) operated by DLR on board ESA's Mars Express spacecraft. On the western edge of the huge Hellas Planitia impact basin, traces can be seen of the icy streams that once flowed here.
A myriad of terrain types are found across the Terra Sirenum region in the southern highlands of Mars. Within the Atlantis basin, a complex and rugged landscape spread across roughly 200 kilometres known as Atlantis Chaos just begins to exemplify the broad diversity of geological processes that occurred in this relatively small area.