Asteroide P/2010 A2 seen by the space telescope Hubble - Comet-like Asteroid P/2010 A2 -...

Asteroide P/2010 A2 seen by the space telescope Hubble - Comet-like Asteroid P/2010 A2 - P/2010 A2 is not a comet but the result of the collision between two asteroides located in the asteroid belt between Mars and Jupiter. This remains of asteroid (lower left) is about 150 metres in diameter and is accompanied by a long trail of debris and dust. Photo obtained in light visible on January 29, 2010 by the Hubble space telescope, approximately 140 million km from the object. This is a NASA Hubble Space Telescope picture of a comet-like object called P/2010 A2, which was first discovered by the LINEAR (Lincoln Near-Earth Asteroid Research program) sky survey on January 6. The object appears so unusual in ground-based telescopic images that discretionary time on Hubble was used to take a close-up look. This picture, from the January 29 observation, shows a bizarre X-pattern of filamentary structures near the point-like nucleus of the object and trailing streamers of dust. This object is not a comet but instead the product of a head-on collision between two asteroids traveling five times faster than a rifle bullet (5 kilometers per second). Astronomers have long thought that the asteroid belt is being ground down through collisions, but such a smashup has never before been seen. The filaments are made of dust and gravel, presumably recently thrown out of the 460-foot-diameter nucleus. Some of the filaments are swept back by radiation pressure from sunlight to create straight dust streaks. Embedded in the filaments are co-moving blobs of dust that likely originate from tiny unseen parent bodies. An impact origin would also be consistent with the absence of gas in spectra recorded using ground-based telescopes. At the time of the Hubble observations, the object was approximately 180 million miles (300 million km) from the Sun and 90 million miles (140 million km) from Earth. The Hubble images were recorded with the new Wide Field Camera 3 (WFC3)