Fig. 1

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Reflectance spectra of nine meteorites: (a) Reflectance changes with wavelength. (b) Reflectance normalized at 0.76 µm changes with wavelength. In (b), the iron meteorites show the steepest near-infrared slope, enstatite chondrites show the moderate near-infrared slope, and aubrite shows the lowest near-infrared slope, indicating that the near-infrared slope is related to the proportion of metal (or enstatite) in the enstatite-metal mixed system.
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