A number of sites were considered as the possible location
where Beagle 2 will come to rest. The feature that all the
sites had in common was that they showed evidence of fluvial
processing by large volumes of water.
Other criteria taken into consideration were the altitude
and latitude on Mars. Too high and there is insufficient atmospheric
density to allow the Beagle 2 parachutes to slow the lander
for a safe touch down. Both height and also too far north
or south away from the equator will increase the need for
additional thermal protection as the climate worsens. The
northern hemisphere is our favoured destination because here
in the martian lowlands the planet will be coming from spring
into summer during the time Beagle is working in 2004.
When seeking safe conditions for a Beagle 2 landing site
the team had to consider slopes and the frequency and angularity
of boulders. The spacecraft needs to find some rocks to carry
out its programme of scientific investigations but not so
many that the gas-filled impact protection is ruptured and
bursts.
The final decision about where to land was needed in 2001
to allow ESA controllers to work out the details of the Mars
Express flight plan.
Dr John Bridges from the Natural History Museum, London,
Dr David Rothery from The Open University Earth Sciences Department
and several colleagues worked on selecting the Beagle 2 landing
site.