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ExoMars Schiaparelli's landing site on Mars

11. August 2016

These images, acquired by the High Resolution Stereo Camera (HRSC), on board the European Mars Express spacecraft, operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR), show part of the Meridiani Planum region.

Traces of water in one of the biggest valleys on Mars

7. July 2016

With a length of 600 kilometres and a depth of up to two kilometres, Mawrth Vallis is one of the biggest valleys on Mars and a possible landing site for the ESA ExoMars and NASA Mars 2020 missions. It is entrenched in the Arabia Terra highland, which is more than four billion years old, and ends in the great Chryse Planitia lowland region.

BIROS erfolgreich ins All gestartet

BIROS fire detection satellite successfully launched into space

22. June 2016

On 22 June 2016 at 05:55 CEST, the BIROS (Bi-Spectral Infrared Optical System) microsatellite was successfully launched into space from the Satish Dhawan Space Centre in India on board a Polar Satellite Launch Vehicle (PSLV).

Krater mit zentraler Vertiefung in Noachis Terra

A crater with a central depression in Noachis Terra

2. June 2016

These images, acquired by the High Resolution Stereo Camera operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) on board the European Mars Express spacecraft show a part of the Noachis Terra region in the southern highlands of Mars. The crater shown is approximately four kilometres deep and has a diameter of roughly 50 kilometres.

Ein durchtrennter Krater in Memnonia Fossae auf dem Mars

A 'split' crater in Memnonia Fossae

28. April 2016

The images presented here, acquired by the High Resolution Stereo Camera (HRSC) operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) on board the European Space Agency (ESA) Mars Express spacecraft, show part of the Memnonia Fossae region on Mars.

Die eisigen Terrassen des Riesenkraters Hellas auf dem Mars

The icy terraces of the giant Hellas basin

23. March 2016

A diameter of 2200 kilometres and a depth of up to nine kilometres: these are the dimensions of the largest impact crater on Mars – Hellas. Only the Moon's South Pole-Aitken Basin and the Valhalla structure on Jupiter's moon, Callisto, have a similar size.

Krater Haulani

Dwarf planet Ceres – mysterious material on craters and mountains

22. March 2016

The dwarf planet Ceres is becoming an increasingly mysterious – and exciting – celestial body as the planetary researchers working on the Dawn mission acquire more and more details. The contrast-enhanced true colours show a bluish material around several craters and mountain slopes.

InSight

InSight mission's journey to Mars set for 2018

9. March 2016

In December 2015, the Mars mission InSight was put on hold, but it has now been provisionally scheduled to launch to the Red Planet at the next opportunity – in May 2018. Technical difficulties with one of the two main experiments – the seismometer – had led to the US space agency, NASA, cancelling the launch that had been planned for March 2016. Now, a decision has been made – the mission has been given a reprieve, and a new launch date in two years' time.

Die Arda%2dTäler auf den Mars: Ein sehr altes Entwässerungssystem

Arda Valles – an ancient drainage system on Mars

18. February 2016

When looking at the large-scale topography along the equator of Mars, what truly stands out are the many, extremely wide drainage channels leading north without many lateral inflows. The smaller valley systems are not so noticeable in these images. They often have multiple branches and meander across the terrain. Such valley systems can be found on Earth. Arda Valles in the Martian highlands is a good example of such a drainage system.

TerraSAR%2dX%2dAufnahme

Safer seafaring with satellites

17. February 2016

Sailing in the regions that polar researcher Arved Fuchs is currently navigating in his ship 'Dagmar Aaen' is a not an easy task. The 'Ocean Change' expedition is travelling around the Antarctic Peninsula, stopping off at a number of research stations to investigate how climate change is impacting the local environment.

A slow farewell – Time to say goodbye to Philae

12. February 2016

The last prolonged silence had already indicated that contact with the Philae lander will be increasingly unlikely, and the conditions on Comet 67P/Churyumov-Gerasimenko have become more hostile. "Unfortunately, the probability of Philae re-establishing contact with our team at the DLR Lander Control Center (LCC) is almost zero, and we will no longer be sending any commands; it would be very surprising if we received a signal now," said Stephan Ulamec Philae Project Manager of the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR).

Video: Flying over the craters of dwarf planet Ceres

29. January 2016

The dwarf planet Ceres would be quite an uncomfortable place if one were to actually stand on its surface – with a rather 'chilly' temperature of minus 60 degrees Celsius by day, which gets colder during the night. Hard, frozen ground and craters spanning kilometres – in all shapes and sizes.

Six-kilometre-deep canyons in the 'Labyrinth of the Night'

28. January 2016

Directly to the west of the gigantic graben system of Valles Marineris on Mars, lies a no less impressive region called Noctis Labyrinthus – the Labyrinth of the Night. It consists of a labyrinth of intersecting valleys and canyons up to six kilometres deep. Extending over 1200 kilometres east to west, it is almost the same length as the River Rhine.

Churyumov%2dGerasimenko

Rosetta discovers water ice on the surface of Comet 67P/Churyumov-Gerasimenko

13. January 2016

A comet is largely composed of water ice and water vapour predominates in its 'atmosphere' – the coma that forms as it nears the Sun. However, very few examples of water ice have previously been observed on the surface of a comet.

Ceres

Low-altitude flight over dwarf planet Ceres

12. January 2016

Currently just 385 kilometres away from the surface, the Dawn spacecraft is orbiting Ceres and acquiring images that show the dwarf planet at an unprecedented resolution of just 35 metres per pixel. These images allow scientists to look at a surface strewn with craters, fractures, domes and bright areas.

Mesas and wind gullies in Aeolis Mensae on Mars

21. December 2015

One of the most striking features of a global view of Mars is the dichotomy between the topographically diverse highlands in the southern hemisphere and the flat, expansive lowland plains of its northern counterpart. Many landscape features shaped by erosion can be observed in the transitional zone between the highlands and lowlands, which explains the particular geological interest in this region.

Atlas Pole

First atlas of dwarf planet Ceres published

25. November 2015

The dwarf planet Ceres measured a mere nine pixels across on an image acquired by NASA's Dawn orbiter on 1 December 2014. Since then, the planetary researchers at the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) have received thousands of images showing the dwarf planet and its unusually varied surface.

urorae Chaos %2d der Übergang von den Valles Marineris zu den großen Ausflusstälern auf dem Mars

Aurorae Chaos – the transition from Valles Marineris to the large outflow channel systems

19. November 2015

The latest images acquired by the High Resolution Stereo Camera (HRSC), operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) on board the European Space Agency (ESA) Mars Express spacecraft, show a runout of the Aurorae Chaos region – an eastern continuation of the massive Valles Marineris graben system on Mars.

TET%2dSatellitenaufnahmen

Peering through smoke – DLR satellite TET-1 delivers detailed images of the fires in Indonesia

30. October 2015

Indonesia is on fire – the island state is currently facing a bitter struggle against forest and peat fires on Sumatra and Borneo, most likely caused by illegal 'slash and burn' farming to clear the land for palm oil or timber plantations. The extremely dry conditions resulting from the El Niño weather phenomenon exacerbate this problem.

Täler Mangala und Minio auf dem Mars

Enormous masses of water flowed through Mangala Valles and Minio Vallis on Mars

15. October 2015

During Mars' geological 'Middle Ages' – the Hesperian Period – which began 3.7 billion years ago and lasted until approximately 3.1 billion years ago, strong volcanic activity was present on our neighbouring planet. Volcanoes spewed low viscosity lava that poured out in masses over the surface and gave rise to extensive plains.

 
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