Thermophysical Characteristics of OSIRIS-REx Target Asteroid (101955) Bennu

preprint2015arXivOpen access

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[Mu¨\ddot{u}ller et al, 2012]{Muller2012}, \cite[Emery et al., 2014]{Emery2014}). We find that the asteroid bears an effective diameter of 510−40+6510^{+6}_{-40} m, a geometric albedo of 0.047−0.0011+0.00830.047^{+0.0083}_{-0.0011}, a roughness fraction of 0.04−0.04+0.260.04^{+0.26}_{-0.04}, and thermal inertia of 240−60+440 Jm−2s−0.5K−1240^{+440}_{-60}\rm~Jm^{-2}s^{-0.5}K^{-1} 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 1.31.3 to 3131~mm. Our outcome suggests that Bennu is suitable for the OSIRIS-REx mission to return samples to Earth.

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