Wednesday, August 20, 2008
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Home : GALILEO AVIONICA : Space : Electro-Optics Mission Payloads

Space

Electro-optic Mission Payloads
From design to manufacturing and testing of optical payloads, mastering optics, focal plane assembly, electronics and precision mechanics, Galileo Avionica has developed a unique competence in mission payloads with outstanding performance, for a high quality observation of the Earth and of far and faint space objects. Starting with the design and assembly of the hyper-spectral instrument GOME for the ESA ERS-2 mission, Galileo Avionica has developed state-of-the-art spectrometers and hyper-spectral cameras for the observation of the Earth, planets and comets. Other scientific payloads for space missions include instruments for planetary in-situ analysis and micro-gravity facilities.

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VIRTIS - Visible InfraRed Thermal Imaging Spectrometer 
Imaging spectrometer for remote sensing in the visible to mid-infrared bands. Selected by ESA as an orbiter payload for the Venus Express mission and for the Rosetta mission to the comet 67P/Churyumov-Gerasimenko. A VIRTIS-like product has been developed for the NASA DAWN discovery mission under an ASI-JPL agreement. VIRTIS combines a high-resolution VIS and IR imaging in the 0.25 to 5 µm range at moderate spectral resolution (VIRTIS-M channel), developed in-house, and a high resolution spectroscope in the 2 to 5 µm range (VIRTIS-H channel). Galileo Avionica led the system engineering, integration and testing of the whole instrument.
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GOME - Global Ozone Monitoring Experiment 
Optical spectrometer in the UV band designed to measure daily total ozone column content and vertical ozone profile in the atmosphere, detecting other minor atmospheric components. The data delivered by GOME is assembled in monthly and seasonal maps of ozone distribution which contribute to the forecast of long term evolution of the atmosphere. GOME will be deployed on all METOP satellites of the Eumetsat Polar System (EPS).
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GIADA - Grain Impact Analyser and Dust Accumulator 
Multi sensor equipment designed to measure the physical properties of the cometary dust (number of particles, their mass and speed) by means of optical systems and piezoelectric transducers (microbalances). GIADA is part of the Rosetta mission payload to study the comet dust flux evolution and grain dynamic properties.
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VIMS - Visible InfraRed Mapping Spectrometer 
Remote sensing instrument developed for ASI as part of the Italian contribution to the NASA Cassini mission. VIMS is installed on the Cassini Orbiter: its primary scientific objective is to provide two dimensional, multispectral, high resolution images for the detailed study of the composition and structure of Saturn ring system and atmosphere.
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