Fig. 6

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Radar albedo and spectral slope calculated in 1.1–1.4 µm (SS5) on M-type asteroids. The dashed line represents the upper limit of SS5 of E-type asteroids (0.18693, the value of SS5 of asteroid 2035 Stearn), which divides M-type into two parts: bodies with a low SS5 fallen into the range of SS5 of E-type (left side of the dashed line) and bodies with a higher SS5 than E-type (right side of the dashed line).
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