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Thursday, June 23, 2011

Dawn Nears Start of Year-Long Stay at Giant Asteroid

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE 818-354-5011
http://www.jpl.nasa.gov

Priscilla Vega/Jia-Rui Cook 626-298-3290/818-354-0850
Jet Propulsion Laboratory, Pasadena, Calif.
priscilla.r.vega@jpl.nasa.gov / jccook@jpl.nasa.gov

Dwayne C. Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

News release: 2011-192 June 23, 2011

Dawn Nears Start of Year-Long Stay at Giant Asteroid

The full version of this story with accompanying images is at:
http://www.jpl.nasa.gov/news/news.cfm?release=2011-192&cid=release_2011-192

PASADENA, Calif. – NASA's Dawn spacecraft is on track to begin the first extended visit to a large
asteroid. The mission expects to go into orbit around Vesta on July 16 and begin gathering science
data in early August. Vesta resides in the main asteroid belt and is thought to be the source of a large
number of meteorites that fall to Earth.

"The spacecraft is right on target," said Robert Mase, Dawn project manager at NASA's Jet
Propulsion Laboratory in Pasadena, Calif. "We look forward to exploring this unknown world during
Dawn's one-year stay in Vesta's orbit."

After traveling nearly four years and 1.7 billion miles (2.7 billion kilometers), Dawn is approximately
96,000 miles (155,000 kilometers) away from Vesta. When Vesta captures Dawn into its orbit on
July 16, there will be approximately 9,900 miles (16,000 kilometers) between them. When orbit is
achieved, they will be approximately 117 million miles (188 million kilometers) away from Earth.

After Dawn enters Vesta's orbit, engineers will need a few days to determine the exact time of
capture. Unlike other missions where a dramatic, nail-biting propulsive burn results in orbit insertion
around a planet, Dawn has been using its placid ion propulsion system to subtly shape its path for
years to match Vesta's orbit around the sun.

Images from Dawn's framing camera, taken for navigation purposes, show the slow progress toward
Vesta. They also show Vesta rotating about 65 degrees in the field of view. The images are about
twice as sharp as the best images of Vesta from NASA's Hubble Space Telescope, but the surface
details Dawn will obtain are still a mystery.

"Navigation images from Dawn's framing camera have given us intriguing hints of Vesta, but we're
looking forward to the heart of Vesta operations, when we begin officially collecting science data,"
said Christopher Russell, Dawn principal investigator, at UCLA. "We can't wait for Dawn to peel
back the layers of time and reveal the early history of our solar system."

Dawn's three instruments are all functioning and appear to be properly calibrated. The visible and
infrared mapping spectrometer, for example, has started to obtain images of Vesta that are larger than
a few pixels in size. During the initial reconnaissance orbit, at approximately 1,700 miles (2,700
kilometers), the spacecraft will get a broad overview of Vesta with color pictures and data in different
wavelengths of reflected light. The spacecraft will move into a high-altitude mapping orbit, about 420
miles (680 kilometers) above the surface to systematically map the parts of Vesta's surface
illuminated by the sun; collect stereo images to see topographic highs and lows; acquire higher-
resolution data to map rock types at the surface; and learn more about Vesta's thermal properties.

Dawn then will move even closer, to a low-altitude mapping orbit approximately 120 miles (200
kilometers) above the surface. The primary science goals of this orbit are to detect the byproducts of
cosmic rays hitting the surface and help scientists determine the many kinds of atoms there, and
probe the protoplanet's internal structure. As Dawn spirals away from Vesta, it will pause again at the
high-altitude mapping orbit. Because the sun's angle on the surface will have progressed, scientists
will be able to see previously hidden terrain while obtaining different views of surface features.

"We've packed our year at Vesta chock-full of science observations to help us unravel the mysteries
of Vesta," said Carol Raymond, Dawn's deputy principal investigator at JPL. Vesta is considered a
protoplanet, or body that never quite became a full-fledged planet.

Dawn launched in September 2007. Following a year at Vesta, the spacecraft will depart for its
second destination, the dwarf planet Ceres, in July 2012. Dawn's mission to Vesta and Ceres is
managed by JPL for NASA's Science Mission Directorate in Washington. Dawn is a project of the
directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville,
Ala.

UCLA is responsible for overall Dawn mission science. Orbital Sciences Corp. of Dulles, Va.,
designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar
System Research, the Italian Space Agency and the Italian National Astrophysical Institute are part of
the mission team. JPL is managed for NASA by the California Institute of Technology in Pasadena.

For more information about Dawn, visit: http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov .
You can also follow the mission on Twitter at: http://www.twitter.com/NASA_Dawn .

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