VIRTIS, visible infrared thermal imaging spectrometer for the ROSETTA mission

The baseline model payload of Rosetta includes a visual infrared spectral and thermal mapper among the instruments on board the spacecraft orbiting around the comet. This instrument will allow the following scientific goals to be achieved: to characterise the nucleus surface composition (concentration of the ices, mineralogical composition of dust, characteristics of organic compounds); to determine the surface temperature distribution and the dust and gas distribution in the inner cometary coma; to map the asteroid´s surface mineralogical composition. In order to achieve these scientific objectives the authors are projecting an instrument composed of two channels: an imaging spectrometer (VIRTIS-M, where M means Mapping mode) and a high resolution spectrometer (VIRTIS-H)