Evidence of a metal-rich surface for the Asteroid (16) Psyche from interferometric observations in the thermal infrared

Abstract

We describe the first determination of thermal properties and size of the M-type Asteroid (16) Psyche from interferometric observations obtained with the Mid-Infrared Interferometric Instrument (MIDI) of the Very Large Telescope Interferometer. We used a thermophysical model to interpret our interferometric data. Our analysis shows that Psyche has a low macroscopic surface roughness. Using a convex 3-D shape model obtained by Kaasalainen et al. (Kaasalainen, M., Torppa, J., Piironen, J. [2002]. Icarus 159, 369–395), we derived a volume-equivalent diameter for (16) Psyche of 247±25km or 238±24km, depending on the possible values of surface roughness. Our corresponding thermal inertia estimates are 133 or 114Jm−2s−0.5K−1, with a total uncertainty estimated at 40Jm−2s−0.5K−1. They are among the highest thermal inertia values ever measured for an asteroid of this size. We consider this as a new evidence of a metal-rich surface for the Asteroid (16) Psyche.