paper

Fragmenting Active Asteroid 331P/Gibbs

arXiv:2111.09900 · doi:10.3847/1538-3881/ac2a3c

Abstract

We describe active asteroid 331P/Gibbs (2012 F5) using archival Hubble Space Telescope data taken between 2015 and 2018. 331P is an outer main-belt active asteroid with a long-lived debris trail that formed in 2011. Embedded in the debris trail we identify 19 fragments with radii between 0.04 and 0.11 km (albedo 0.05 assumed) containing about 1 percent of the mass of the primary nucleus. The largest shows a photometric range (1.5 magnitudes), a V-shaped minimum and a two-peaked lightcurve period near 9 hours, consistent with a symmetric contact binary (Drahus and Waniak 2016). Less convincing explanations are that 331P-A is a monolithic, elongated splinter or that its surface shows hemispheric 4:1 albedo variations. The debris trail is composed of centimeter sized and larger particles ejected with characteristic 10 cm s speeds following a size distribution with index q = 3.7+/-0.1 to 4.1+/-0.2. The HST data show that earlier, ground-based measurements of the nucleus were contaminated by near-nucleus debris, which cleared by 2015. We find that the primary nucleus has effective radius 0.8+/-0.1 km and is in rapid rotation (3.26+/-0.01 hour, range 0.25 magnitudes, minimum density 1600 kg/m3 if strengthless. The properties of 331P are consistent with a) formation about 1.5 Myr ago by impact shattering of a precursor body (Novakovic et al. 2014) b) spin-up by radiation torques to critical rotation c) ejection of about 1 percent of the nucleus mass in mid-2011 by rotational instability and d) subsequent evolution of the fragments and dispersal of the debris by radiation pressure.

27 pages, 12 figures

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