March 13, 2006

Erica Hupp/ Merrilee Fellows
Headquarters, Washington
(202) 358-1237/ (818) 393-0754

William Jeffs
Johnson Space Center, Houston
(281) 483-5111

RELEASE: 06-091

NASA'S STARDUST FINDINGS MAY ALTER VIEW OF COMET FORMATION

Samples from comet Wild 2 have surprised scientists, indicating the
formation of at least some comets may have included materials ejected
by the early sun to the far reaches of the solar system.

Scientists have found minerals formed near the sun or other stars in
the samples returned to Earth by NASA's Stardust spacecraft in
January. The findings suggest materials from the center of the solar
system could have traveled to the outer reaches where comets formed.
This may alter the way scientists view the formation and composition
of comets.

"The interesting thing is we are finding these high-temperature
minerals in materials from the coldest place in the solar system,"
said Donald Brownlee, Stardust principal investigator from the
University of Washington, Seattle.

Scientists have long thought of comets as cold, billowing clouds of
ice, dust and gases formed on the edges of the solar system. But
comets may not be so simple or similar. They may prove to be diverse
bodies with complex histories. Comet Wild 2 seems to have had a more
complex history than thought.

"We have found very high-temperature minerals, which supports a
particular model where strong bipolar jets coming out of the early
sun propelled material formed near to the sun outward to the outer
reaches of the solar system," said Michael Zolensky, Stardust curator
and co-investigator at NASA's Johnson Space Center, Houston. "It
seems that comets are not composed entirely of volatile rich
materials but rather are a mixture of materials formed at all
temperature ranges, at places very near the early sun and at places
very remote from it."

One mineral found in the material brought back by Stardust is olivine,
a primary component of the green sand found on some Hawaiian beaches.
It is among the most common minerals in the universe, but scientists
were surprised to find it in cometary dust.

Olivine is a compound of iron, magnesium and other elements. The
Stardust sample is primarily magnesium. Along with olivine, the dust
from Wild 2 contains high-temperature minerals rich in calcium,
aluminum and titanium.

Stardust passed within 149 miles of comet Wild 2 in January 2004,
trapping particles from the comet in an exposed gel. Its return
capsule parachuted to the Utah desert on Jan. 15. The science
canister with the Wild 2 sample arrived at Johnson on Jan. 17.
Samples have been distributed to approximately 150 scientists for
study.

"The collection of cometary particles is greater than we ever
expected," said Stardust Deputy Principal Investigator Peter Tsou of
NASA's Jet Propulsion Laboratory, Pasadena, Calif. "The collection
includes about two dozen large tracks visible to the unaided eye."

The grains are tiny, most smaller than a hair's width. Thousands of
them appear to be embedded in the glass-like aerogel. A single grain
of 10 microns, only one-hundredth of a millimeter (.0004 inches), can
be sliced into hundreds of samples for scientists.

In addition to cometary particles, Stardust gathered interstellar dust
samples during its seven-year journey. The team at Johnson's
curatorial facility hopes to begin detailed scanning of the
interstellar tray within a month. They will initiate the Stardust at
Home project. It will enable volunteers from the public to help
scientists locate particles.

After registering, Stardust at Home participants may download a
virtual microscope. The microscope will connect to a server and
download "focus movies." The movies are images of the Stardust
Interstellar Dust Collector from an automated microscope at the
Cosmic Dust Lab at Johnson. Participants will search each field for
interstellar dust impacts.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the
Stardust mission for NASA's Science Mission Directorate, Washington.
Lockheed Martin Space Systems, Denver, developed and operated the
spacecraft.

Stardust science team members presented their first findings this week
at the annual Lunar and Planetary Science Conference in League City,
Texas.

For more information about Stardust on the Web, visit:

http://www.nasa.gov/stardust

For information about NASA and agency programs on the Web, visit:

http://www.nasa.gov/home

        
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