Abstract

Abstract We develop a shape model of asteroid 16 Psyche using observations acquired in a wide range of wavelengths: Arecibo S-band delay-Doppler imaging, Atacama Large Millimeter Array (ALMA) plane-of-sky imaging, adaptive optics (AO) images from Keck and the Very Large Telescope (VLT), and a recent stellar occultation. Our shape model has dimensions 278 (−4/+8 km) × 238(−4/+6 km) × 171 km (−1/+5 km), an effective spherical diameter D eff = 222-1/+4 km, and a spin axis (ecliptic lon, lat) of (36°, −8°) ± 2°. We survey all the features previously reported to exist, tentatively identify several new features, and produce a global map of Psyche. Using 30 calibrated radar echoes, we find Psyche’s overall radar albedo to be 0.34 ± 0.08 suggesting that the upper meter of regolith has a significant metal (i.e., Fe–Ni) content. We find four regions of enhanced or complex radar albedo, one of which correlates well with a previously identified feature on Psyche, and all of which appear to correlate with patches of relatively high optical albedo. Based on these findings, we cannot rule out a model of Psyche as a remnant core, but our preferred interpretation is that Psyche is a differentiated world with a regolith composition analogous to enstatite or CH/CB chondrites and peppered with localized regions of high metal concentrations. The most credible formation mechanism for these regions is ferrovolcanism as proposed by Johnson et al. (2020).

Highlights

  • Asteroid 16 Psyche is the largest Tholen (1984) M-class asteroid and a target of the NASA Discovery mission Psyche (Elkins-Tanton et al 2017, 2020)

  • Visible and near-infrared spectra (Bell et al 1989), optical polarimetry (Dollfus et al 1979), thermal observations (Matter et al 2013), and radar observations (Ostro et al 1985; Magri et al 2007a; Shepard et al 2008, 2017) all support the hypothesis that its surface to near-surface is dominated by metal

  • We examine topographical and optical albedo features discussed in previous work (Shepard et al 2017; Viikinkoski et al 2018; Ferrais et al 2020), produce a global map, and overlay it with radar albedo values, a proxy for metal concentrations in the upper meter of the regolith

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Summary

Introduction

Asteroid 16 Psyche is the largest Tholen (1984) M-class asteroid and a target of the NASA Discovery mission Psyche (Elkins-Tanton et al 2017, 2020). Recent studies of Psyche have converged to size estimates (effective diameter) between 220 and 230 km, and to spin poles within a few degrees of (36°, −8°) (ecliptic lon, lat) (Shepard et al 2017; Drummond et al 2018; Viikinkoski et al 2018; Ferrais et al 2020). Given this size, mass estimates have led to a consensus that Psyche’s overall bulk density is between 3400 and 4100 kg m−3 (Elkins-Tanton et al 2020), which places constraints on its internal structure, composition, and possible origin.

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