The Dimorphos Boulder Swarm

TL;DR

Deep Hubble images of asteroid Dimorphos reveal a large, slow-moving boulder swarm resulting from the DART impact, providing insights into ejecta dynamics and surface composition.

Contribution

This study provides detailed observations of the boulder population and their velocities post-impact, offering new data on ejecta behavior and asteroid surface properties.

Findings

Largest boulder about 7 meters in diameter

Mean velocity dispersion of boulders is 0.30 m/s

Boulders account for 0.1% of Dimorphos mass

Abstract

We present deep Hubble Space Telescope images taken to examine the ejecta from the DART spacecraft impact into asteroid Dimorphos. The images reveal an extensive population of co-moving boulders, the largest of which is about 7 m in diameter (geometric albedo 0.15 assumed). Measurements of 37 boulders show a mean sky-plane velocity dispersion of 0.30+/-0.03 m/s, only slightly larger than the 0.24 m/s gravitational escape velocity from the Didymos/Dimorphos binary system. The total boulder mass, 5e6 kg (density 2200 kg/m3 assumed), corresponds to about 0.1 percent of the mass of Dimorphos and the boulders collectively carry about 3e-5 of the kinetic energy delivered by the DART spacecraft impact. The sky-plane distribution of the boulders is asymmetric, consistent with impact into an inhomogeneous, likely rubble-pile, body. Surface boulder counts on Didymos show that the observed boulder swarm could be ejected from as little as 2 percent of the surface of Dimorphos (for example a circular crater at the impact point about 50 m in diameter). The large, slow-moving boulders are potential targets to be investigated in-situ by the upcoming ESA HERA mission.