[meteorite-list] Hubble Witnesses an Asteroid Mysteriously Disintegrating (2013 R3)

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu, 6 Mar 2014 07:40:24 -0800 (PST)
Message-ID: <201403061540.s26FeOWb007070_at_zagami.jpl.nasa.gov>

http://www.spacetelescope.org/news/heic1405/

Hubble witnesses an asteroid mysteriously disintegrating
6 March 2014

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.

"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 metres 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 kilometres 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 vaporising. The object is too cold for ices
to significantly sublimate, and it has presumably maintained its nearly
480-million-kilometre 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 [1] - 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.

Notes

[1] 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.
Notes for editors

The Hubble Space Telescope is a project of international cooperation between
ESA and NASA.

[1] The results will be published in a paper entitled "Disintegrating
Asteroid P/2013 R3", to appear in the Astrophysical Journal Letters
on 6 March 2014.

[2] The international team of astronomers in this study consists of D.
Jewitt (UCLA, USA), J. Agarwal (MPS, Germany), J. Li (UCLA, USA), H. Weaver
(Johns Hopkins University, USA), M. Mutchler (STScI, USA), and S. Larson
(University of Arizona, USA).

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

    Science paper

Contacts

Jessica Agarwal
Max Planck Institute for Solar System Research
Goettingen, Germany
Tel: +49 551 384 979 346
Email: Agarwal at mps.mpg.de

David Jewitt
University of California at Los Angeles
Los Angeles, USA
Tel: +1-310-825-2521
Email: jewitt at ucla.edu

Georgia Bladon
ESA/Hubble, Public Information Officer
Garching, Germany
Tel: +49-89-3200-6855
Email: gbladon at partner.eso.org
Received on Thu 06 Mar 2014 10:40:24 AM PST