The database currently contains:

• NIR reflectance spectra of ice mixed with various concentration of sulfate (Massé et al. 2010) for the interpretation of planetary icy surfaces (Mars polar caps and icy satellites)
• NIR reflectance spectra sands wet with pure water (various origins and compositions) at different steps of drying for the interpretation of terrestrial coastal areas and possible flowing on Mars (unpublished)

The database will contain soon:

• NIR reflectance spectra of pure water ice at different temperature and crushed at different grain sizes (Taffin et al., 2011)
• Raman spectra of icy moons analogous clathrates (Bollengier et al., 2013 ; Bezacier et al., 2014)
• NIR reflectance spectra of olivine altered in martian conditions (Dehouck et al., 2014)
• Raman spectra of volcanic glasses