http://www.esa.int/esaCP/SEM3LY2PGQD_index_0.html

Two asteroid fly-bys for Rosetta
European Space Agency 
11 March 2004

ESA PR 15-2004. 

Today the Rosetta Science Working Team has made the final selection of 
the asteroids that Rosetta will observe at close quarters during its 
journey to Comet 67P/Churyumov-Gerasimenko.  Steins and Lutetia lie 
in the asteroid belt between the orbits of Mars and Jupiter.
 
Rosetta's scientific goals always included the possibility of studying
one or more asteroids from close range. However, only after Rosetta's launch
and its insertion into interplanetary orbit could the ESA mission managers
assess how much fuel was actually available for fly-bys. Information from the
European Space Operations Centre (ESOC) in Germany enabled Rosetta's
Science Working Team to select a pair of asteroids of high scientific interest,
well within the fuel budget. 

The selection of these two excellent targets was made possible by the high
accuracy with which the Ariane 5 delivered the spacecraft into its orbit. 
This of course leaves sufficient fuel for the core part of the mission, 
orbiting Comet 67P/Churyumov-Gerasimenko for 17 months when Rosetta reaches 
its target in 2014.

Asteroids are primitive building blocks of the Solar System, left over from 
the time of its formation about 4600 million years ago. Only a few asteroids 
have so far been observed from nearby. They are very different in shape and 
size, ranging from a few kilometres to over 100 kilometres across, and in 
their composition. 

The targets selected for Rosetta, Steins and Lutetia, have rather different
properties. Steins is relatively small, with a diameter of a few kilometres, 
and will be visited by Rosetta on 5 September 2008 at a distance of just 
over 1700 kilometres. This encounter will take place at a relatively low 
speed of about 9 kilometres per second during Rosetta's first excursion 
into the asteroid belt.

Lutetia is a much bigger object, about 100 kilometres in diameter. Rosetta 
will pass within about 3000 kilometres on 10 July 2010 at a speed of 15 
kilometres per second. This will be during Rosetta's second passage 
through the asteroid belt. 

Rosetta will obtain spectacular images as it flies by these primordial rocks. 
Its onboard instruments will provide information on the mass and density of 
the asteroids, thus telling us more about their composition, and will also 
measure their subsurface temperature and look for gas and dust around them. 

Rosetta began its journey just over a week ago, on 2 March, and is well on 
its way. Commissioning of its instruments has already started and is 
proceeding according to plan.

"Comets and asteroids are the building blocks of our Earth and the other 
planets in the Solar System. Rosetta will conduct the most thorough analysis 
so far of three of these objects," said Prof. David Southwood, Director of 
ESA's Science Programme. "Rosetta will face lots of challenges during its 
12-year journey, but the scientific insights that we will gain into the 
origin of the Solar System and, possibly, of life are more than rewarding." 

For further information, please contact:

ESA Media Relations Division
Tel: +33(0)1.53.69.7155
Fax: +33(0)1.53.69.7690  
 

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