http://stardust.jpl.nasa.gov

Stardust Sets New Distance Record 
April 18, 2002

Since its launch on February 7, 1999, the Stardust spacecraft 
has traveled over two billion kilometers completing one and 
a half elliptical orbits around the Sun. On Thursday, April
18th, the mission will reach a major milestone when it arrives 
at its furthest distance from the Sun, also known as its aphelion. 

At this time the spacecraft will be 2.72 Astronomical Units 
(407 million kilometers or 253 million miles) from the Sun, and 
near the middle of the asteroid belt. This is the farthest 
distance ever reached by a solar-powered spacecraft. Far beyond 
the orbit of Mars, the sunlight intensity is only 13% of what 
we see at Earth resulting in very cold temperatures and
diminished power generation by the spacecraft's solar cells. 
The spacecraft is performing excellently in this environment 
and operations teams at the Jet Propulsion Laboratory, California 
and Lockheed Martin Astronautics, Denver are eager to enter the 
final phases of the mission. 

After aphelion, Stardust will begin falling back towards the Sun 
and by the end of the mission, in January 2006, it will have completed 
another loop and a half around the Sun. On January 2, 2004, on its final 
solar orbit, Stardust will fly past comet Wild 2 to collect samples and 
return them to Earth in 2006. In January 2006, the samples will be
delivered by parachute inside the Stardust Sample Return Capsule to 
the Utah Testing and Training Range. 

The comet samples that Stardust will be collecting and returning to 
Earth have been preserved since the early formation of the Solar System. 
During the Solar System's formation, they accumulated to form comets 
beyond the orbit of Neptune and they are believed to be the initial 
building blocks of planets and life as we know it. The returned
samples from Stardust will be distributed world wide to scientists 
who will study them with the best microanalytical techniques available.
The mission will provide fundamental insights into the nature of 
materials that aided in the formation of planets, both in the solar 
system and around other stars. 

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