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.
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.
Two June 2018 will mark 15 years since the launch of the European Mars Express spacecraft. Still in orbit around the Red Planet, Mars Express is one of the most successful space missions to be sent to Earth's planetary neighbour. One of the instruments still in operation is the German High Resolution Stereo Camera (HRSC).
This video shows a flight over the 102-kilometre wide Neukum Crater in the southern highlands of Mars. It is based on data acquired by the High Resolution Stereo Camera (HRSC), operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) on board the ESA Mars Express spacecraft, which has been orbiting Mars since 2003.
Images from the High Resolution Stereo Camera (HRSC) operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) on board ESA's Mars Express spacecraft show the collapsed depression Ismenia Patera. There are two hypotheses regarding the formation of this geological structure – it is either an impact crater or the caldera of a Martian supervolcano.