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|  |  |  |  | | | | Article Images |  | What stops Mars Express getting lost in space? 29 January 2004
 | | The Mars Express orbiter is checking its attitude and distance from Mars. |  |  |  |  |
| | | |  | Radio communications between Rosetta and the ground
use a newly developed deep-space antenna which was built
by ESA at New Norcia, near Perth in Western Australia.
It is operated by Xantic.
Credits: ESA |  |  |  |  |
| | | |  | | A view of the ESOC control room in Darmstadt, Germany. Pictured on 7 January 2004 during the Mars Express mission. |  |  |  |  |
| | | | Seeing stars keeps Mars Express in line
 | | Mars Express orbiter's main engine is firing for Mars Orbit Insertion (MOI). |  |  |  |  |
| | | |  | | An artist’s impression of Rosetta waking from deep-space hibernation to rendezvous with Comet 67P/Churyumov-Gerasimenko in 2014.
Rosetta’s 11-year expedition began in March 2004, with an Ariane 5 launch from Kourou in French Guiana, and the spacecraft was then sent towards the outer Solar System. The long journey includes three gravity assists at Earth (2004, 2007, 2009), one at Mars (2007), and two asteroid encounters: (2867) Steins (2008) and (21) Lutetia (2010).
After the third Earth-gravity assist and a large deep-space manoeuvre, the spacecraft will go into hibernation (July 2011 – January 2014). During this period, Rosetta will record its maximum distances from the Sun (about 800 million kilometres) and Earth (about 1 thousand million kilometres). The spacecraft will be reactivated prior to the comet-rendezvous manoeuvre, during which the thrusters will fire for several hours to slow the relative drift rate between the spacecraft and comet to about 25 m/s.
Credits: ESA, image by AOES Medialab |  |  |  |  |
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|  | Looking at Mars More about... Mars Express overviewRelated articles ESOC Mission OperationsInterplanetary trajectoriesGetting it right: An interview with Rudi SchmidtMore Mars missions Voyages to MarsNASA's MER web siteJapan Aerospace Exploration Agency
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