The Libya Montes highland region is one of the oldest areas on Mars. The latest images from HRSC identify a number of drainage channels and dense valley networks.
Among the most remarkable geological formations on Mars is the vast shield volcano Olympus Mons that towers up to 26 kilometres above the surrounding plains. It is situated on the Tharsis plateau, a volcanic province the size of Europe. Volcanism is a widespread phenomenon on Mars.
It looks simple: the rover heads straight for the landing craft, uses a gripper arm to remove a sensor unit from the loading bay and takes it quickly to the determined deposit location, where seismic measurements are then carried out. Everything takes place without human intervention, as the rover, lander and sensor unit complete their job autonomously and effectively.
On 20 June 2017, the European Space Agency (ESA) gave the go-ahead for the further development of the PLATO space telescope. The German Aerospace Center (Deutsches Zentrum für Luft-und Raumfahrt; DLR) is leading the international consortium responsible for the construction and scientific operation of the space telescope.
These images from the HRSC Mars camera show an impact crater in the southern highlands with remarkable surface features. Unusually light-toned deposits and so-called ‘chaos terrain’ are visible inside the crater.
Harsh Vardhan, Union Minister of Science and Technology, Earth Sciences of the Government of India, visited the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) on 29 May 2017 as part of the German-Indian Intergovernmental Consultations.
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.
Scientists from the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) teamed up with I.S.A.R. Germany (International Search and Rescue) and Germandrones to take part in an international disaster rehearsal from 8 to 10 May 2017.
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.