Suspected asteroid collision leaves trailing debris

New Hubble images show a complex X-pattern of debris near the nucleus of a comet-like object.Provided by STScI, Baltimore, Maryland
By | Published: February 2, 2010 | Last updated on May 18, 2023
Asteroid collision debris
A comet-like object imaged by the Hubble Space Telescope, called P/2010 A2, shows a complex X-pattern of filamentary structures near the nucleus. The debris pattern and trailing streamers of dust suggest a head-on collision between two asteroids.
NASA, ESA, and D. Jewitt (University of California, Los Angeles)
February 2, 2010
NASA’s Hubble Space Telescope has observed a mysterious X-shaped debris pattern and trailing streamers of dust that suggest a head-on collision between two asteroids. Astronomers have long thought the asteroid belt is being ground down through collisions, but such a smashup has never been seen before.

Asteroid collisions are energetic, with an average impact speed of more than 11,000 mph (17,700 km/h), or 5 times faster than a rifle bullet. The comet-like object imaged by Hubble, called P/2010 A2, was first discovered by the Lincoln Near-Earth Asteroid Research, or LINEAR, program sky survey January 6. New Hubble images taken January 25 and 29 show a complex X-pattern of filamentary structures near the nucleus.

“This is quite different from the smooth dust envelopes of normal comets,” said principal investigator David Jewitt of the University of California at Los Angeles. “The filaments are made of dust and gravel, presumably recently thrown out of the nucleus. Some are swept back by radiation pressure from sunlight to create straight dust streaks. Embedded in the filaments are comoving blobs of dust that likely originated from tiny unseen parent bodies.”

Hubble shows that the main nucleus of P/2010 A2 lies outside its own halo of dust. Scientists have never seen this before in a comet-like object. The nucleus is estimated to be 460 feet (140 meters) in diameter.

Normal comets fall into the inner regions of the solar system from icy reservoirs in the Kuiper Belt and Oort Cloud. As a comet neasr the Sun and warms up, ice near the surface vaporizes and ejects material from the solid comet nucleus via jets. But P/2010 A2 may have a different origin. It orbits in the warm, inner regions of the asteroid belt where its nearest neighbors are dry rocky bodies lacking volatile materials.

This leaves open the possibility that the complex debris tail is the result of an impact between two bodies, rather than ice simply melting from a parent body.

“If this interpretation is correct, two small and previously unknown asteroids recently collided, creating a shower of debris that is being swept back into a tail from the collision site by the pressure of sunlight,” Jewitt said.

The main nucleus of P/2010 A2 would be the surviving remnant of this so-called hypervelocity collision.

“The filamentary appearance of P/2010 A2 is different from anything seen in Hubble images of normal comets, consistent with the action of a different process,” Jewitt said. An impact origin also would be consistent with the absence of gas in spectra recorded using ground-based telescopes.

The asteroid belt contains abundant evidence of ancient collisions that have shattered precursor bodies into fragments. The orbit of P/2010 A2 is consistent with membership in the Flora asteroid family, produced by collisional shattering more than 100 million years ago. One fragment of that ancient smashup may have struck Earth 65 million years ago, triggering a mass extinction that wiped out the dinosaurs. But, until now, no such asteroid-asteroid collision has been caught “in the act.”

At the time of the Hubble observations, the object was approximately 180 million miles (290 million km) from the Sun and 90 million miles (145 million km) from Earth. Hubble’s new Wide Field Camera 3 (WFC3) recorded the images.