Abstract
In this work, we investigate the thermophysical properties, including thermal inertia, roughness fraction and surface grain size of OSIRIS-REx target asteroid (101955) Bennu by using a thermophysical model with the recently updated 3D radar-derived shape model (\cite[Nolan et al., 2013]{Nolan2013}) and mid-infrared observations (\cite[Mller et al, 2012]{Muller2012}, \cite[Emery et al., 2014]{Emery2014}). We find that the asteroid bears an effective diameter of m, a geometric albedo of , a roughness fraction of , and thermal inertia of for our best-fit solution. The best-estimate thermal inertia suggests that fine-grained regolith may cover a large portion of Bennu's surface, where a grain size may vary from to ~mm. Our outcome suggests that Bennu is suitable for the OSIRIS-REx mission to return samples to Earth.
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