Large Particles in Active Asteroid P/2010 A2

Abstract

Previously unknown asteroid P/2010 A2 rose to prominence in 2010 by forming a transient, comet-like tail consisting of ejected dust. The observed dust production was interpreted as either the result of a hypervelocity impact with a smaller body or of a rotational disruption. We have re-observed this object, finding that large particles remain a full orbital period after the initial outburst. In the intervening years, particles smaller than ~3 mm in radius have been dispersed by radiation pressure, leaving only larger particles in the trail. Since the total mass is dominated by the largest particles, the radiation pressure filtering allows us to obtain a more reliable estimate of the debris mass than was previously possible. We find that the mass contained in the debris is ~5x10^8 kg (assumed density 3000 kg m^-3), the ratio of the total debris mass to the nucleus mass is ~0.1 and that events like P/2010 A2 contribute <3% to the Zodiacal dust production rate. Physical properties of the nucleus and debris are also determined.

16 pages, 4 figures; ApJLett, in Press

References in corpus (7)

• The Active Asteroids
• Dynamics of rotationally fissioned asteroids: Source of observed small asteroid systems
• Dynamical Model for the Zodiacal Cloud and Sporadic Meteors
• A collision in 2009 as the origin of the debris trail of asteroid P/2010 A2
• P/2010A2 LINEAR - I: An impact in the Asteroid Main Belt
• P/2010 A2 LINEAR II: dynamical dust modelling
• AzTEC 1.1 mm Observations of the MBM12 Molecular Cloud

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