The recently approved ExoMars rover is the first element of the ESA Aurora programme and is scheduled to deliver the Pasteur exobiology payload to Mars by 2015. The 0.7 kg Panoramic Camera will provide multi-spectral stereo images with 65° field-of-view (1.1 mrad/pixel) and high-resolution (85 μrad/pixel) monoscopic 'zoom' images with 5° field-of-view. The stereo wide-angle cameras (WAC) are based on the Beagle 2 Stereo Camera System heritage (Griffiths et al. (2005). Planet. Space Sci. 53, 1466-1488). The Panoramic Camera instrument is designed to fulfil the digital terrain mapping requirements of the mission as well as to provide multi-spectral geological imaging, colour and stereo panoramic images, water vapour abundance and dust optical depth measurements. It can also be used for high-resolution imaging of inaccessible locations on crater walls and to observe retrieved subsurface samples before ingestion into the rest of the Pasteur payload.

DEM, ExoMars Rover, Imaging: Multi-spectral, Imaging: Stereoscopic, Mars, Pasteur payload
dx.doi.org/10.1017/S1473550406003387
International Journal of Astrobiology
Department of Mechanical and Aerospace Engineering

Griffiths, A.D. (Andrew D.), Coates, A.J. (Andrew J.), Jaumann, R. (Ralf), Michaelis, H. (Harald), Paar, G. (Gerhard), Barnes, D. (David), … Trautner, R. (Roland). (2006). Context for the ESA ExoMars rover: The Panoramic Camera (PanCam) instrument. In International Journal of Astrobiology (Vol. 5, pp. 269–275). doi:10.1017/S1473550406003387