Hubble views the disintegration of asteroid P/2013 R3, providing detailed observations that pinpoint the process responsible.
The NASA/ESA Hubble Space Telescope has photographed the never-before-seen break-up of an asteroid, which has fragmented into as many as ten smaller pieces. Although fragile comet nuclei have been seen to fall apart as they approach the Sun, nothing like the breakup of this asteroid, P/2013 R3, has ever been observed before in the asteroid belt.
“This is a rock. Seeing it fall apart before our eyes is pretty amazing,” said David Jewitt of UCLA, USA, who led the astronomical forensics investigation.
The crumbling asteroid, designated P/2013 R3, was first noticed as an unusual, fuzzy-looking object on 15 September 2013 by the Catalina and Pan-STARRS sky surveys. Follow-up observations on 1 October with the Keck Telescope on Mauna Kea, Hawaii, revealed three co-moving bodies embedded in a dusty envelope that is nearly the diameter of Earth.
This video shows a number of NASA/ESA Hubble Space Telescope observations of asteroid P/2013 R3, as viewed over a time period of just over two months in 2013. The fragments are visible moving around, and new chunks of material appear as time passes. The observations were taken using Hubble on 29 October 2013, 15 November 2013, 13 December 2013, and 14 January 2014. Credit: NASA, ESA, D. Jewitt (UCLA), and M. Kornmesser
“Keck showed us that this thing was worth looking at with Hubble,” Jewitt said. With its superior resolution, the space-based Hubble observations soon showed that there were really ten distinct objects, each with comet-like dust tails. The four largest rocky fragments are up to 200 meters in radius, about twice the length of a football pitch.
The Hubble data showed that the fragments are drifting away from each other at a leisurely 1.5 kilometers per hour — slower than the speed of a strolling human. The asteroid began coming apart early last year, but the latest images show that pieces continue to emerge.
“This is a really bizarre thing to observe — we’ve never seen anything like it before,” says co-author Jessica Agarwal of the Max Planck Institute for Solar System Research, Germany. “The break-up could have many different causes, but the Hubble observations are detailed enough that we can actually pinpoint the process responsible.”
The ongoing discovery of more fragments makes it unlikely that the asteroid is disintegrating due to a collision with another asteroid, which would be instantaneous and violent in comparison to what has been observed. Some of the debris from such a high-velocity smash-up would also be expected to travel much faster than has been observed.
It is also unlikely that the asteroid is breaking apart due to the pressure of interior ices warming and vaporizing. The object is too cold for ices to significantly sublimate, and it has presumably maintained its nearly 480-million-kilometer distance from the Sun for much of the age of the Solar System.
This leaves a scenario in which the asteroid is disintegrating due to a subtle effect of sunlight that causes the rotation rate to slowly increase over time. Eventually, its component pieces gently pull apart due to centrifugal force. The possibility of disruption by this phenomenon — known as the YORP effect  — has been discussed by scientists for several years but, so far, never reliably observed.
For break-up to occur, P/2013 R3 must have a weak, fractured interior, probably the result of numerous ancient and non-destructive collisions with other asteroids. Most small asteroids are thought to have been severely damaged in this way, giving them a “rubble pile” internal structure. P/2013 R3 itself is probably the product of collisional shattering of a bigger body some time in the last billion years.
“This is the latest in a line of weird asteroid discoveries, including the active asteroid P/2013 P5, which we found to be spouting six tails,” says Agarwal. “This indicates that the Sun may play a large role in disintegrating these small Solar System bodies, by putting pressure on them via sunlight.”
P/2013 R3’s remnant debris, weighing in at 200,000 tonnes, will provide a rich source of meteoroids in the future. Most will eventually plunge into the Sun, but a small fraction of the debris may one day blaze across our sky as meteors.
 In full, this effect is known as the Yarkovsky–O’Keefe–Radzievskii–Paddack effect. This effect occurs when light from the Sun is absorbed by a body and then re-emitted as heat. When the shape of the emitting body is not perfectly regular, more heat is emitted from some regions than others. This creates a small imbalance that causes a small but constant torque on the body, which changes its spin rate.
Reference: “Disintegrating Asteroid P/2013 R3” by David Jewitt, Jessica Agarwal, Jing Li, Harold Weaver, Max Mutchler and Stephen Larson, 6 March 2014, The Astrophysical Journal Letters.