Beagle 2 DEM
3D Vision System for the martian lander Beagle 2
Function
Coordination of 3D Vision
Contact Information
Description
The project aim was to generate a precise data set (= mapping of the immediate vicinity of the lander from stereo images) immediately after touchdown of the Beagle 2 Lander (Boxing day, 2003). These data were then to be used for detecting, measuring and classifying interesting objects and for pinpoint navigation of the robot arm and its sensors (microscope, spectrometer, etc.) based on precise object coordinates. Further requirements for 3D image processing were the generation of image mosaics in all given spectral bands, the distortion correction of panoramic mirror images immediately after landing, as well as a possible re-calibration of the system in case of geometric changes of the robot arm.
The system combined existing know-how at JR in the field of image-based navigation (various ESA studies since 1990), stereo reconstruction (industry projects such as the DIBIT tunnel scanner), and camera calibration to provide the digital elevation model (DEM) immediately after landing, taking into account environmental influences and system parameter changes such as the geometry of the robot arm.
In addition to the 3D imaging software components (DEM generation, mosaiking, mechanisms for on-line calibration) both cameras were calibrated geometrically (incl. influences of the used filters, temperature and pressure), camera-to-robot arm calibration was performed and some tools for navigation by means of star images were implemented.
The functionality of the entire system was successfully tested during the pre-launch tests, but Beagle 2 was lost during the approach to the Red Planet. Nevertheless, the tools for 3D image data processing are further available for remote sensing and industrial applications:
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DEM generation from a set of stereo images
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Image mosaiking
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Calibration Camera-to-robot arm
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Procedures for geometric camera calibration in dependence on physical influences (temperature, pressure)
Project Duration
1999 - 2003
Main Partners
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Mullard Space Science Laboratory (MSSL) www.mssl.ucl.ac.uk
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University of Wales, Aberystwyth www.aber.ac.uk
Funding
- Joanneum Research
- Austrian Federal Ministry for Transport, Innovation and Technology

Figure 1: Calibration of the Beagle 2 Cameras

Figure 2: Testing of Robot Arm, Cameras and PAW at Leicester Space Center

Figure 3: Rendering of stereo-derived DEM during testing
Videos
- Animation of Beagle2 Lander Beagle2.avi
- Digital Elevation Modell DEM.avi
Poster
Interviews
References
Griffiths, A, Coates, A, Josset, J, Paar, G, Hofmann,
B, Pullan, D, Rueffer, P, Sims, M, and Pillinger, C (2005).
The Beagle 2 stereo camera
system
Planetary and Space ScienceDecember 2005, Vol 53/14-15:1466-1482.
Paar, G, Griffiths, A, Barnes, D, Coates, A, and Bauer,
A (2005).
The Beagle 2 Camera Heritage for
Pasteur
Geophysical Research Abstracts - European Geosciences Union, 7 -
06815(SRef-ID: 1607-7962/gra/EGU05-A-06815):7.
Barnes, D, Phillips, N, and Paar, G (2003).
Beagle2 Simulation and Calibration for Ground
Segment Operations
In: 7th International Symposium on Artificial Intelligence, Robotics
and Automation in Space, Nara, Japan, May 19-23, 2003.
