Asteroidal disruption, through high-velocity collisions or rotational spin-up, is believed to be the primary mechanism for the production and destruction of small asteroids. These authors report observations of P/2010 A2 — a previously unknown inner-belt asteroid with a peculiar, comet-like morphology — that reveal an approximately 120-metre-diameter nucleus with an associated tail of millimetre-sized dust particles. They conclude that it is most probably the evolving remnant of a recent asteroidal disruption in February/March 2009.
- David Jewitt
- Harold Weaver
- Michal Drahus