Fig. 5
Spectral parameters for asteroids (black dots), meteorites (squares) and laboratory altered meteorites (triangles for heated and stars for laser irradiated). a) Albedo vs. Vis slope (0.44–0.70 μm). b) NIR1 slope (1.10–1.45 μm) vs. NIR2 slope (1.6–2.3 μm). c) Center of the 0.7 μm band vs. standard deviation. d) Depth of the 0.7 μm band vs. band SSR.
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