[meteorite-list] NASA's Swift And Hubble Probe Asteroid Collision Debris

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu, 28 Apr 2011 08:49:34 -0700 (PDT)
Message-ID: <201104281549.p3SFnYOU005172_at_zagami.jpl.nasa.gov>

April 28, 2011

Trent J. Perrotto
Headquarters, Washington
202-358-0321
trent.j.perrotto at nasa.gov

Lynn Chandler
Goddard Space Flight Center, Greenbelt, Md.
301-286-2806
lynn.chandler-1 at nasa.gov

RELEASE: 11-128

NASA'S SWIFT AND HUBBLE PROBE ASTEROID COLLISION DEBRIS

WASHINGTON -- Late last year, astronomers noticed an asteroid named
Scheila had unexpectedly brightened, and it was sporting short-lived
plumes. Data from NASA's Swift satellite and Hubble Space Telescope
showed these changes likely occurred after Scheila was struck by a
much smaller asteroid.

"Collisions between asteroids create rock fragments, from fine dust to
huge boulders, that impact planets and their moons," said Dennis
Bodewits, an astronomer at the University of Maryland in College Park
and lead author of the Swift study. "Yet this is the first time we've
been able to catch one just weeks after the smash-up, long before the
evidence fades away."

Asteroids are rocky fragments thought to be debris from the formation
and evolution of the solar system approximately 4.6 billion years
ago. Millions of them orbit the sun between Mars and Jupiter in the
main asteroid belt. Scheila is approximately 70 miles across and
orbits the sun every five years.

"The Hubble data are most simply explained by the impact, at 11,000
mph, of a previously unknown asteroid about 100 feet in diameter,"
said Hubble team leader David Jewitt at the University of California
in Los Angeles. Hubble did not see any discrete collision fragments,
unlike its 2009 observations of P/2010 A2, the first identified
asteroid collision.

The studies will appear in the May 20 edition of The Astrophysical
Journal Letters and are available online.

Astronomers have known for decades that comets contain icy material
that erupts when warmed by the sun. They regarded asteroids as
inactive rocks whose destinies, surfaces, shapes and sizes were
determined by mutual impacts. However, this simple picture has grown
more complex over the past few years.

During certain parts of their orbits, some objects, once categorized
as asteroids, clearly develop comet-like features that can last for
many months. Others display much shorter outbursts. Icy materials may
be exposed occasionally, either by internal geological processes or
by an external one, such as an impact.

On Dec. 11, 2010, images from the University of Arizona's Catalina Sky
Survey, a project of NASA's Near Earth Object Observations Program,
revealed Scheila to be twice as bright as expected and immersed in a
faint comet-like glow. Looking through the survey's archived images,
astronomers inferred the outburst began between Nov. 11 and Dec. 3.

Three days after the outburst was announced, Swift's
Ultraviolet/Optical Telescope (UVOT) captured multiple images and a
spectrum of the asteroid. Ultraviolet sunlight breaks up the gas
molecules surrounding comets; water, for example, is transformed into
hydroxyl and hydrogen. But none of the emissions most commonly
identified in comets, such as hydroxyl or cyanogen, show up in the
UVOT spectrum. The absence of gas around Scheila led the Swift team
to reject scenarios where exposed ice accounted for the activity.

Images show the asteroid was flanked in the north by a bright dust
plume and in the south by a fainter one. The dual plumes formed as
small dust particles excavated by the impact were pushed away from
the asteroid by sunlight. Hubble observed the asteroid's fading dust
cloud on Dec. 27, 2010, and Jan. 4, 2011.

The two teams found the observations were best explained by a
collision with a small asteroid impacting Scheila's surface at an
angle of less than 30 degrees, leaving a crater 1,000 feet across.
Laboratory experiments show a more direct strike probably wouldn't
have produced two distinct dust plumes. The researchers estimated the
crash ejected more than 660,000 tons of dust -- equivalent to nearly
twice the mass of the Empire State Building.

"The dust cloud around Scheila could be 10,000 times as massive as the
one ejected from comet 9P/Tempel 1 during NASA's UMD-led Deep Impact
mission," said co-author Michael Kelley, also at the University of
Maryland. "Collisions allow us to peek inside comets and asteroids.
Ejecta kicked up by Deep Impact contained lots of ice, and the
absence of ice in Scheila's interior shows that it's entirely unlike
comets."

NASA's Goddard Space Flight Center in Greenbelt, Md., manages Hubble
and Swift. Hubble was built and is operated in partnership with the
European Space Agency. Science operations for both missions include
contributions from many national and international partners. For more
information, video and images associated with this release, visit:

http://www.nasa.gov/topics/universe/features/asteroid-collision.html
        
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Received on Thu 28 Apr 2011 11:49:34 AM PDT