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![]() Beagle 2 team assesses possible Mars landing sites EUROPEAN SPACE AGENCY RELEASE Posted: Jan. 27, 2000
"Chryse is a region of flood channels which have brought materials from the southern highlands down over the northern plains. The Maja Vallis channel area in Chryse is of particular interest because Viking and Mars Orbiter images show the presence of some layering in isolated mesas (elevated flat surfaces, like plateau). Such layers might include hard pans (crust) formed through precipitation of salts from groundwater or ephemeral lakes. "Tritonis Lacus is on the margin of the Elysium plains and consists of a more eroded landscape. This erosion has left a generally smooth surface which would be suitable for a safe landing." Selection of the final site will be made in February 2001 based on the outcome of detailed modelling of the landing activity at both sites and after consultation with the scientific community at an international workshop. "We are reviewing all the images we can get from Mars Global Surveyor (NASA's spacecraft currently in orbit around Mars). The site must be suitable for the science we want to do and be compatible with the entry and descent of Beagle 2," says Colin Pillinger, Principal Investigator for Beagle 2. "The delivery of Beagle by Mars Express requires complicated manoeuvres which use extra fuel. So the final selection will also take into account extensive studies to make sure that the implications for the spacecraft are acceptable," adds Rudi Schmidt, Mars Express Project Manager.
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