Fig. 12From: An evaluation method of reflectance spectra to be obtained by Hayabusa2 Near-Infrared Spectrometer (NIRS3) based on laboratory measurements of carbonaceous chondrites D 2.90 values and the D 2.76/D 2.90 ratios of NIRS3 data of the meteorite samples corrected by the method 1, plotted with those of FT-IR spectra of Murchison samples heated in vacuum (up to 600 °C, Hiroi et al. 1996) and irradiated by pulse laser (Matsuoka et al. 2015). Labels: 1 = Murchison, 2 = Murray, 3 = Y-793321, 4 = Jbilet Winselwan, 5 = Y 982086, 6 = Y 980115, 7 = Y-86720, and 8 = B-7904Back to article page