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    ESA > Our Activities > Space Science > Mars Express

    Mars Express mission facts

    How the mission was named: Mars Express is so called because it will be built more quickly than any other comparable planetary mission. Beagle 2 was named after the ship in which Charles Darwin sailed when formulating his ideas about evolution.
    Prime contractor: Astrium, Toulouse, France, leading a consortium of 24 companies from 15 European countries and the US
    Launch date: 2 June 2003
    Launcher: Soyuz/Fregat, built by Starsem, the European/Russian launcher consortium
    Launch mass: 1120 kg (including 113 kg orbiter payload and 60 kg lander)
    Lander: Beagle 2
    Orbiter instruments: High Resolution Stereo Camera (HRSC); Energetic Neutral Atoms Analyser (ASPERA); Planetary Fourier Spectrometer (PFS); Visible and Infra Red Mineralogical Mapping Spectrometer (OMEGA); Sub-Surface Sounding Radar Altimeter (MARSIS); Mars Radio Science Experiment (MaRS); Ultraviolet and Infrared Atmospheric Spectrometer (SPICAM);
    Spacecraft operations: European Space Operations Centre (ESOC), Darmstadt, Germany
    Ground stations: ESA ground station in New Norcia, near Perth, Australia. Foreseen operational duration: One Martian year (687 Earth days) is funded. The spacecraft is designed for a further Martian year's operation.
    Arrival at Mars: December 2003
    Lander mission management: University of Leicester, UK
    The Mars Express Orbiter will:
    • image the entire surface at high resolution (10 metres/pixel) and selected areas at super resolution (2 metres/pixel);
    • produce a map of the mineral composition of the surface at 100 metre resolution;
    • map the composition of the atmosphere and determine its global circulation;
    • determine the structure of the sub-surface to a depth of a few kilometres;
    • determine the effect of the atmosphere on the surface;
    • determine the interaction of the atmosphere with the solar wind.
    The Beagle 2 lander was planned to:
    • determine the geology and the mineral and chemical composition of the landing site;
    • search for life signatures (exobiology);
    • study the weather and climate.

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    • Orbiter instruments
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    • Planetary Fourier Spectrometer
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    • MaRS - Radio Science Experiment
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