April 11, 2019 | A cubic metre of Mars

Tests for the InSight 'Mole'

  • Various possible scenarios are being investigated to determine what caused the Mars ‘Mole’ to stop.
  • A fully functional model of the ‘Mole’ is being tested in a box of sand that compacts quickly and in which cavities can form as a result of the hammering.
  • Focus: Space, exploration

A blue box, a cubic metre of Mars-like sand, a rock, a fully-functional model of the Mars 'Mole' and a seismometer – these are the main components with which the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) is simulating the current situation on Mars. After its first hammering operation on 28 February 2019, the DLR Heat and Physical Properties Package (HP³), the Mars Mole, was only able to drive itself about 30 centimetres into the Martian subsurface. DLR planetary researchers and engineers are now analysing how this could have happened and looking into what measures could be taken to remedy the situation. "We are investigating and testing various possible scenarios to find out what led to the 'Mole' stopping," explains Torben Wippermann, Test Leader at the DLR Institute of Space Systems in Bremen. The basis for the scientists' work: some images, temperature data, data from the radiometer and recordings made by the French Seismic Experiment for Interior Structure (SEIS) during a brief hammering test conducted on 26 March 2019.

When the NASA InSight lander arrived on the Martian surface, everything looked even better than expected. Although the lander's camera showed numerous rocks some distance away, the immediate surroundings were free of rocks and debris. The reason why the 'Mole' hammered its way quickly into the ground after being placed on the surface of Mars and was then unable to continue its progress is now being diagnosed remotely. "There are various possible explanations, to which we will have to react differently," says Matthias Grott, a planetary researcher and the HP³ Project Scientist. A possible explanation is that the 'Mole' has created a cavity around itself and is no longer sufficiently constrained by the friction between its body and the surrounding sand.

Another type of sand

In Bremen, DLR is now experimenting with a different type of sand: "Until now, our tests have been conducted using a Mars-like sand that is not very cohesive," explains Wippermann. This sand was used during earlier tests in which the 'Mole' hammered its way down a five-metre column in preparation for the mission. Now, the Mole's ground model will be tested in a box of sand that compacts quickly and in which cavities can be created by the hammering process. During some of the test runs, the researchers will also place a rock with a diameter of about 10 centimetres in the sand. Such an obstacle in the subsurface could also be the reason why the HP³ instrument has stopped penetrating further. In all experiments, a seismometer listens to the activity of the Earth-based 'Mole'. During the short 'diagnostic' hammering on Mars, SEIS recorded vibrations to learn more about the Mole's impact mechanism. Comparisons between the data obtained on Mars and the Earth-based tests help the researchers more closely understand the real-life situation. "Ideally, we will be able to reconstruct the processes on Mars as accurately as possible."

'Moles' on Earth as guinea pigs

The next steps will follow once the scientists know what caused the progress of the 'Mole' to come to a halt on 28 February 2019. Possible measures to allow the instrument to hammer further into the ground must then be meticulously tested and analysed on Earth. For this reason, a replica of the HP3 instrument has been shipped to NASA's Jet Propulsion Laboratory in Pasadena, California. There, the DLR researchers' findings can be used to test the interaction of the 'Mole', the support structure and the robotic arm to determine whether, for example, lifting or moving the external structure is the correct solution. "I think that it will be a few weeks before any further actions are carried out on Mars," says Grott. The break in activities for the Mars Mole will only come to an end once a solution has been found for the Earth-based 'Moles'.

The HP³ Instrument on NASA’s InSight mission

The InSight mission is being carried out by NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California, on behalf of the agency’s Science Mission Directorate. InSight is part of NASA’s Discovery Program. DLR is contributing the Heat Flow and Physical Properties Package (HP³) experiment to the mission. The scientific leadership lies with the DLR Institute of Planetary Research, which was also in charge of developing and implementing the experiment in collaboration with the DLR Institutes of Space Systems, Optical Sensor Systems, Space Operations and Astronaut Training, Composite Structures and Adaptive Systems, and System Dynamics and Control, as well as the Institute of Robotics and Mechatronics. Participating industrial partners are Astronika and the CBK Space Research Centre, Magson GmbH and Sonaca SA, the Leibniz Institute of Photonic Technology (IPHT) as well as Astro- und Feinwerktechnik Adlershof GmbH. Scientific partners are the ÖAW Space Research Institute at the Austrian Academy of Sciences and the University of Kaiserslautern. The DLR Microgravity User Support Center (MUSC) in Cologne is responsible for HP³ operations. In addition, the DLR Space Administration, with funding from the German Federal Ministry for Economic Affairs and Energy, supported a contribution by the Max Planck Institute for Solar System Research to the French main instrument SEIS (Seismic Experiment for Interior Structure).

Detailed information on the InSight mission and the HP³ experiment is available on DLR’s dedicated mission site with extensive background articles. You can also find information in the animation and brochure about the mission or via the hashtag #MarsMaulwurf on the DLR Twitter channel. Tilman Spohn, the Principal Investigator for the HP³ experiment, is also providing updates in the DLR Blog portal about the activities of the Mars Mole.

Written by Manuela Braun


Falk Dambowsky

Head of Media Relations, Editor
German Aerospace Center (DLR)
Corporate Communications
Linder Höhe, 51147 Cologne
Tel: +49 2203 601-3959

Prof. Dr. Tilman Spohn

HP³ Principal Investigator
German Aerospace Center (DLR)
DLR Institute of Planetary Research
Linder Höhe, 51147 Cologne

Christian Krause

German Aerospace Center (DLR)
Microgravity User Support Center (MUSC), Space Operations and Astronaut Training
Linder Höhe, 51147 Cologne

Matthias Grott

HP³ project scientist and InSight science team member; Focus on heat flow and thermal conductivity measurements; Instrument development
German Aerospace Center (DLR)
Institute of Planetary Research
Rutherfordstraße 2, 12489 Berlin

Torben Wippermann

German Aerospace Center (DLR)
Institute of Space Systems
Robert-Hooke-Straße 7, 28359 Bremen

Anko Börner

German Aerospace Center (DLR)
Institute of Optical Sensor Systems
Rutherfordstraße 2, 12489 Berlin-Adlershof

Roy Lichtenheldt

German Aerospace Center (DLR)
In­sti­tute of Sys­tem Dy­nam­ics and Con­trol
Space Systems Dynamics
Münchener Straße 20, 82234 Weßling

Martin Knapmeyer

HP³ and SEIS project sci­en­tist and mem­ber of the In­Sight sci­ence team
German Aerospace Center (DLR)
Institute of Planetary Research
Planetary Physics
Rutherfordstraße 2, 12489 Berlin

Jörg Melcher

DLR Institute of Composite Structures and Adaptice Systems

Marco Scharringhausen

Deutsches Zentrum für Luft- und Raumfahrt (DLR)
Institut für Raumfahrtsysteme
Robert-Hooke-Str. 7, 28359 Bremen