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Fig. B.2


Thermal inertia of (6) Hebe derived from the thermophysical modeling. The overall preferred solution (lower reduced χ2) is ~60 J m-2 s-0.5 K-1 for data acquired at heliocentric distance r< 2.1 AU and ~40 J m-2 s-0.5 K-1 for data taken at r> 2.6 AU. While this might be indicative of changing thermal inertia with temperature, one should be extremely cautious when interpreting this result, as a range of solutions cannot be ruled out based on the χ2 values presented here.

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