Hubble and Keck Telescope Observations of Active Asteroid 288P/300163 (2006 VW139)

TL;DR

This study uses Hubble and Keck telescopes to analyze the dust ejection and physical properties of active asteroid 288P/300163, revealing prolonged low-velocity dust ejection likely driven by sublimation of near-surface ice.

Contribution

First detailed high-resolution imaging and modeling of dust ejection dynamics for asteroid 288P, suggesting sublimation-driven activity and potential binary nucleus features.

Findings

Dust ejection speeds between 0.06 and 0.3 m/s

Dust mass estimated at ~9 million kg

Prolonged dust ejection starting before July 2011

Abstract

We present Hubble Space Telescope and Keck 10 meter telescope observations of active asteroid 288P/300163 (2006 VW139) taken to examine ejected dust. The nucleus is a C-type object with absolute magnitude $H_V$ = 17.0$\pm$0.1 and estimated diameter $\sim$2.6 km (for assumed visual geometric albedo $p_V$ = 0.04). Variations in the brightness of the nucleus at the 10% to 15% level are significant in both 2011 December and 2012 October but we possess too few data to distinguish variations caused by activity from those caused by rotation. The dust scattering cross-section in 2011 December is $\sim$40 km$^2$, corresponding to a dust mass $\sim$9$\times$10$^6$ kg (88 $\mu$m mean particle radius assumed). The full width at half maximum of the debris sheet varies from $\sim$100 km near the nucleus to $\sim$1000 km 30arcsec (40,000 km) east of it. Dust dynamical models indicate ejection speeds between 0.06 and 0.3 m s$^{-1}$, particle sizes between 10 and 300 $\mu$m and an inverse square-root relation between particle size and velocity. Overall, the data are most simply explained by prolonged, low velocity ejection of dust, starting in or before 2011 July and continuing until at least 2011 October. These properties are consistent with the sublimation of near-surface ice aided by centrifugal forces. The high spatial resolution of our HST images (52 km per pixel) reveals details that remained hidden in previous ground-based observations, such as the extraordinarily small vertical extent of the dust sheet, ejection speeds well below the nucleus escape speed, and the possibility of a binary nucleus.