Fig. 7From: Characterization of asteroid analogues by means of emission and reflectance spectroscopy in the 1- to 100-µm spectral rangeEmissivity and reflectance measurements for serpentine; left panel shows emissivity in vacuum and under purging, compared with 1-R in the NIR-MIR; right panel shows emissivity in vacuum compared with 1-R in the TIRBack to article page