Study of hydrated asteroids via their polarimetric properties at low phase angles

Open Access

Fig. 6

(a) Comparison between the polarimetric properties (P_min and h) with the diameters. (b) Comparison between the polarimetric properties (P_min and h) and the thermal inertia given in MacLennan & Emery (2022). The Ch-type asteroids (DeMeo et al. 2009) are colored by the sky blue. In both a and b, asteroids with ${\hat{R}}_{0.7} + σ {\hat{R}}_{0.7} < 1$ ${\hat R_{0.7}} + \sigma {\hat R_{0.7}} < 1$ (i.e., Ch-type asteroids) are colored.

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