Asteroid P/2010 A2

Hubble Space Telescope images of the asteroid P/2010 A2 taken at eight epochs between 25 January and 29 May 2010 with the Wide Field Camera 3 (WFC3).

The morphology of P/2010 A2 appears to evolve slowly: this is mostly due to the recession of the object from Earth - their relative distance doubled from January to May - but also to slow, intrinsic changes in the object itself. Thanks to the superb resolution of Hubble's WPC3, this very slow evolution can be measured in order to characterize the object.

Originally suspected to be a main belt comet, this bizarre object is in fact the remnant of an asteroid collision that occurred around 10 February 2009, and the dust trail is debris from the impact.

In each panel, the image has been rotated so that the tail lies approximately horizontal. Each panel subtends 10 arcseconds in height. The images have 0.04 arcsecond pixels and are combinations of images with total integration times of about 2600 seconds through the F606W filter.

Photo credit: NASA, ESA and D. Jewitt (UCLA)



Video credit: NASA, ESA, and G. Bacon (STScI)

Notes: For more about this asteroid, see: Hubble and Rosetta Unmask Nature of Recent Asteroid Wreck, and Hubble Observes Aftermath of Possible Asteroid Collision.