Selected by ESA to be one of the eleven instruments aboard the MPO spacecraft of the BepiColombo mission, MERTIS will map the surface mineralogy of planet Mercury with a spatial resolution of at least 500 meters. It is an imaging spectrometer covering the thermal infrared, or IR, range and also contains a radiometer for thermal inertia measurements. The goals of Phase B/C1 are to define the instrument, to select technical solutions for the chosen concept, and to create an early design. Launch of the BepiColombo mission atop ESA's Ariane V launcher is planned for 2014. The journey to Mercury will take six years to complete.
| Bischoff, Addi (Adolf) | Working Group of apl. Prof. Bischoff |
| Hiesinger, Harald | Professorship for geological planetology (Prof. Hiesinger) |
| Bischoff, Addi (Adolf) | Working Group of apl. Prof. Bischoff |
| Hiesinger, Harald | Professorship for geological planetology (Prof. Hiesinger) |
| Klemm, Kerstin | Professorship for experimental and analytical planetology (Prof. Kleine) |
| Moroz, Liubov | Professorship for geological planetology (Prof. Hiesinger) |
| Multhaup, Kai | Institute for Planetology |
| Rout, Surya Snata | Professorship for geological planetology (Prof. Hiesinger) |