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Rosetta overview 
Objective Rosetta's main objective is to rendezvous with Comet 67P/Churyumov-Gerasimenko. It will study the nucleus of the comet and its environment in great detail for a period of nearly two years, and land a probe on its surface.
For more in-depth scientific and technical details of our Space Science Programme and missions, follow this link.
Rosetta will be the first mission ever to land on a comet. After its lander reaches the comet, the main spacecraft will follow the comet for many months as it heads towards the Sun. Rosetta's task is to study comets, which are considered the primitive building blocks of the Solar System. This will help us to understand if life on Earth began with the help of 'comet seeding'. Rosetta is one of the most challenging missions ever attempted. Many of the complex navigation and landing manoeuvres need to take place automatically with absolutely no room for error. The complications of sending a small spacecraft halfway across the Solar System and making a soft landing on a small comet are immense.
What's special? Rosetta will be the first space mission to journey beyond the main asteroid belt and rely solely on solar cells for power generation, rather than the traditional radio-isotope thermal generators. The new solar-cell technology used on the orbiter's two giant solar panels allows it to operate over 800 million kilometres from the Sun, where sunlight levels are only 4% of those on Earth. Hundreds of thousands of specially developed non-reflective silicon cells generate up to 8700 Watts in the inner Solar System and around 400 Watts for the deep-space comet encounter The Rosetta mission will achieve many historic firsts:
Spacecraft The main spacecraft measures 2.8 x 2.1 x 2.0 metres, on which all subsystems and payload equipment are mounted. There are two 14-metre solar panels with a total area of 64 square metres. At launch, the vehicle weighs approximately 3000 kilograms (fully fuelled) including 1670 kilograms of propellant, 165 kilograms of scientific payload for the orbiter, and 100 kilograms for the lander. The large number of complex scientific instruments needs to be accommodated on one side of the spacecraft, which must permanently face the comet during the operational phase of the mission. Until its release, the lander is carried on the opposite side of the orbiter to the large high-gain antenna dish. As it arrives on the comet, the Rosetta lander uses three different techniques (self-adjusting landing gear, harpoons, and a drill) to ensure that once it has arrived on the surface of the comet, it stays there.
As soon as it touches down, two harpoons will anchor the probe to the surface, the self-adjusting landing gear will ensure that it stays upright, even on a slope and then the lander's feet will drill into the ground. These devices will help counteract the fact that there is very low gravity on a comet.
The lander will focus on the study of the composition and structure of the comet nucleus material. Goals include the determination of the elements that exist, traces of minerals and isotopic composition of the comet's surface and immediate subsurface. The comet's surface strength, density, texture, porosity, ice phases and thermal properties will also be studied. Texture investigations will include microscopic studies of individual grains. Journey The journey to Rosetta's final destination will involve complex fly-bys of other planets. Partnerships The orbiter's scientific payload includes 11 experiments and the small lander which is equipped with its own payload of scientific instruments. Scientific consortia from institutes across Europe and the United States have provided these state-of-the-art instruments.
The lander is provided by a European consortium headed by the German Aerospace Research Institute (DLR). Other members of the consortium are ESA, CNES and institutes from Austria, Finland, France, Hungary, Ireland, Italy, and the United Kingdom.
Last update: 2 March 2004
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