[meteorite-list] NASA's Hubble Captures First Images Of Aftermath Of Possible Asteroid Collision

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Wed, 13 Oct 2010 13:34:10 -0700 (PDT)
Message-ID: <201010132034.o9DKYAF6010234_at_zagami.jpl.nasa.gov>

Oct. 13, 2010

J.D. Harrington
Headquarters, Washington
202-358-5241
j.d.harrington at nasa.gov

Donna Weaver
Space Telescope Science Institute, Baltimore
410-338-4493
dweaver at stsci.edu

David Jewitt
University of California, Los Angeles
310-825-2521
jewitt at ucla.edu


RELEASE: 10-253

NASA'S HUBBLE CAPTURES FIRST IMAGES OF AFTERMATH OF POSSIBLE ASTEROID COLLISION

WASHINGTON -- NASA's Hubble Space Telescope has captured the first
snapshots of a suspected asteroid collision. The images show a
bizarre X-shaped object at the head of a comet-like trail of
material.

In January, astronomers began using Hubble to track the object for
five months. They thought they had witnessed a fresh asteroid
collision, but were surprised to learn the collision occurred in
early 2009.

"We expected the debris field to expand dramatically, like shrapnel
flying from a hand grenade," said astronomer David Jewitt of the
University of California in Los Angeles, who is a leader of the
Hubble observations. "But what happened was quite the opposite. We
found that the object is expanding very, very slowly."

The peculiar object, dubbed P/2010 A2, was found cruising around the
asteroid belt, a reservoir of millions of rocky bodies between the
orbits of Mars and Jupiter. It is estimated modest-sized asteroids
smash into each other about once a year. When the objects collide,
they inject dust into interplanetary space. But until now,
astronomers have relied on models to make predictions about the
frequency of these collisions and the amount of dust produced.

Catching colliding asteroids is difficult because large impacts are
rare while small ones, such as the one that produced P/2010 A2, are
exceedingly faint. The two asteroids that make up P/2010 A2 were
unknown before the collision because they were too faint to be
noticed. The collision itself was unobservable because of the
asteroids' position in relation to the sun.

About 10 or 11 months later, in January 2010, the Lincoln Near-Earth
Research (LINEAR) Program Sky Survey spotted the comet-like tail
produced by the collision. But only Hubble discerned the X pattern,
offering unequivocal evidence that something stranger than a comet
outgassing had occurred.

Although the Hubble images give compelling evidence for an asteroid
collision, Jewitt says he still does not have enough information to
rule out other explanations for the peculiar object. In one such
scenario, a small asteroid's rotation increases from solar radiation
and loses mass, forming the comet-like tail.

"These observations are important because we need to know where the
dust in the solar system comes from, and how much of it comes from
colliding asteroids as opposed to 'outgassing' comets," Jewitt said.
"We also can apply this knowledge to the dusty debris disks around
other stars, because these are thought to be produced by collisions
between unseen bodies in the disks. Knowing how the dust was produced
will yield clues about those invisible bodies."

The Hubble images, taken from January to May 2010 with the telescope's
Wide Field Camera 3, reveal a point-like object about 400 feet wide,
with a long, flowing dust tail behind a never-before-seen X pattern.
Particle sizes in the tail are estimated to vary from about 1/25th of
an inch to an inch in diameter.

The 400-foot-wide object in the Hubble image is the remnant of a
slightly larger precursor body. Astronomers think a smaller rock,
perhaps 10 to 15 feet wide, slammed into the larger one. The pair
probably collided at high speed, about 11,000 mph, which smashed and
vaporized the small asteroid and stripped material from the larger
one. Jewitt estimates that the violent encounter happened in February
or March 2009 and was as powerful as the detonation of a small atomic
bomb.

Sunlight radiation then swept the debris behind the remnant asteroid,
forming a comet-like tail. The tail contains enough dust to make a
ball 65 feet wide, most of it blown out of the bigger body by the
impact-caused explosion. The science journal Nature will publish the
findings in the Oct. 14 issue.

"Once again, Hubble has revealed unexpected phenomena occurring in our
celestial 'back yard," said Eric Smith, Hubble Program scientist at
NASA Headquarters in Washington. "Though it's often Hubble's deep
observations of the universe or beautiful images of glowing nebulae
in our galaxy that make headlines, observations like this of objects
in our own solar system remind us how much exploration we still have
to do locally."

Astronomers do not have a good explanation for the X shape. The
crisscrossed filaments at the head of the tail suggest that the
colliding asteroids were not perfectly symmetrical. Material ejected
from the impact, therefore, did not make a symmetrical pattern, a bit
like the ragged splash made by throwing a rock into a lake. Larger
particles in the X disperse very slowly and give this structure its
longevity.

Astronomers plan to use Hubble again next year to view the object.
Jewitt and his colleagues hope to see how far the dust has been swept
back by the sun's radiation and how the mysterious X-shaped structure
has evolved.

For images, movies, and more information about asteroid encounter
P/2010 A2, visit:

http://hubblesite.org/news/2010/34

and

http://www.nasa.gov/hubble
        
-end-
Received on Wed 13 Oct 2010 04:34:10 PM PDT