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Testing the Exomars rover in Mars-like conditions

21 October 2010

By Manuela Braun

 Challenging martian surface
zum Bild Challenging martian surface

A couple of clicks of the mouse are enough to send the ExoMars rover with its six flexible metal wheels moving across the sand tank towards the first obstacle. Bernhard Rebele, Maximilian Apfelbeck and Sebastian Kuß from the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) Institute of Robotics and Mechatronics have built a challenging obstacle course, which really puts the rover to the test. Its middle wheels scrabble obstinately against the sharp edges of the limestone. The steady grinding sound as the rover passes over the pebbles in the sand turns into an unpleasant creaking. At last, the small metal teeth manage to get a grip, and the Mars rover crawls upwards inch-by-inch until the rearmost pair of its six wheels has cleared the obstacle. The industrial stone is 25 centimetres high – the European Space Agency (ESA), which will be sending the rover into space in 2018, has set rigorous specifications for the tests it has to pass at DLR.

Journey on foot over a martian dune

 DLR webcast – ExoMars rover under test

"This sand is quite, well, let's say – benign!" says Maximilian Apfelbeck, as he lets the coarse sand and gravel flow through his fingers. He means that the rover has been fortunate; the sand is neither too coarse nor too fine. Walking through the 5.5 by 10 metre tank gives a good idea of what it would feel like to take a stroll on a martian dune. It was not easy to select the correct sand – not all sand is like what can be expected on Mars. Since no soil sample has yet been returned to Earth from Mars, ESA has had to rely on microscope images and photographs of the planet's surface, for example of the walls of actual Mars rover tracks, to evaluate what the sand is like there. The sand was then prepared specially for the tests. The trials at DLR Oberpfaffenhofen are attempting to establish: "How deep the rover’s tracks are, how much drive the wheels produce, and what types of obstacles it can drive over," Bernhard Rebele summarises, while the rover drives through the special silica sand from England.

Computer simulation

 Analysing data on a personal computer
zum Bild Analysing data on a personal computer

Eight infrared cameras track every movement of the rover and its six wheels, accurate to the millimetre; the researchers can see where and how the rover has slipped. Force sensors on the wheel suspension systems and torque sensors continuously monitor important parameters during every journey. The ExoMars rover is now driving towards a surface covered in misshapen stones. It most probably will never have to drive on such uneven ground, but the researchers want to obtain as much data as possible. "In this way, we can optimise our computer simulations," explains project leader Bernd Schäfer.

When differences between the simulation and the test rover are found, the new data are incorporated into the computer model. Later, many tests for the ExoMars rover will not have to be conducted in the 'real' world, because computer simulations will give the researchers the information they require. The findings could also be useful for future missions; if it is planned to allow a rover to travel independently over unfamiliar terrain, using a stereo camera to guide it, or to use a swarm of small crawlers – crab-like rovers with many legs – these activities can be tested out in computer simulations before the event. 

Mars-like conditions

 Elevation model of the test tank
zum Bild Elevation model of the test tank

While the six wheels and the drive system are identical to those of the actual rover, the DLR test rover weighs 100 kilograms less than the original. "That's how we simulate the lower gravity on Mars – the forces on the wheels must be as realistic as possible," says Apfelbeck. A tower mounted on top of rover simulates the exact location of the centre of gravity of the rover and the payloads that ExoMars is designed to transport across the martian surface. The rover can drive 100 metres per hour: "But it will more likely be covering such a distance in a day, to prevent damage to the electronics," explains Schäfer.

Maximilian Apfelbeck has stationed himself at the end of the tank, as a precaution. The rover is working slowly up the slope created for it by the researchers. It must be able to drive up slopes of 26 degrees to meet ESA's specifications. Sebastian Kuß continually looks over to the slope, while controlling the rover with his mouse. The steep slope is a challenge for the rover and the team. The wheels are finding it difficult to gain traction in the loose sand. Finally, Kuß sends it the command to retreat.

 Differences between fine and coarse sand
zum Bild Differences between fine and coarse sand

At the end of the test sequence, a camera on an arm scans the entire surface of the test tank and the computer builds a three-dimensional map of the surface. The vehicle's tracks and all the obstacles are precisely recorded. The scientists now have to analyse the data from the test sequence and incorporate it into their computer models. The tank contents have to be precisely rearranged for the next test sequence, to imitate the conditions on Mars as closely as possible. The scientists have to rake through the sand, add gravel and roll it all flat.

Treacherous sand for a rover

The next batch of materials is waiting. A small store next to the test facility is filled with large bags of sand and containers filled with various materials. This includes lava sand from the Eifel region (Germany/Belgium), some of it in its original condition, some of it ground repeatedly. Maximilian Apfelbeck kneels in front of one of the containers. His finger disturbs a finely ground sand, the same colour and consistency as flour. "NASA also uses this sand," he says. Just this kind of surface brought the Spirit rover to a halt on Mars. ExoMars must not suffer the same fate.

Manuela Braun
Deutsches Zentrum für Luft- und Raumfahrt (DLR) - German Aerospace Center

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Last update: 26/10/2010 10:39:23