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 C2/D are to define the instrument in detail and to manufacture a qualification model and a flight unit. 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) |
Bauch, Karin | Professorship for geological planetology (Prof. Hiesinger) |
Morlok, Andreas | Professorship for geological planetology (Prof. Hiesinger) |
Moroz, Liubov | Professorship for geological planetology (Prof. Hiesinger) |
Multhaup, Kai | Institute for Planetology |
Reiss, Dennis | Professorship for geological planetology (Prof. Hiesinger) |
Rout, Surya Snata | Professorship for geological planetology (Prof. Hiesinger) |