Sci­en­tif­ic ob­jec­tives of the mis­sion

Asteroid broken into pieces, artist’s impression
Artist's impression of an asteroid that has split into numerous fragments. Vesta and Ceres were spared such massive destruction, representing ideal research objects to learn more about the time when our Solar System originated.



Dawn is an exceptionally exciting mission for planetary researchers. Vesta and Ceres bear witness to the time in which the planets in the Solar System were formed. It is thought that the two bodies have hardly changed since their formation, four and a half billion years ago. They are ideal research objects for catching a glimpse of the past of our 'cosmic neighbourhood'.

Alongside looking back at the period when our Solar System formed, the mission is also investigating the structure and composition of asteroids. Smaller cosmic strays are constantly crossing the path of Earth around the Sun. By studying the larger parent asteroids, planetary researchers expect to learn more about these smaller bodies and the potential risk they pose to Earth.

Photographic data and gravitational measurements will be used to determine the mass, shape, volume and rotation speed of Vesta and Ceres. The Dawn spacecraft will determine their composition, from which their thermal development since their formation can be derived. In addition, these measurements will contribute to clarifying the connection between asteroids and meteorites, which are fragments of asteroids.

Dawn will image the surface of Ceres and Vesta to draw conclusions about their tectonic and impact history. Measurements of their gravity and precise determination of their rotational characteristics will allow the size of any metallic core to be estimated. Furthermore, infrared and gamma ray spectroscopy will be used to search for water-bearing minerals.

The scientific objectives of the Dawn mission are:

  • determining the inner structure, density and homogeneity of the two protoplanets Vesta and Ceres;
  • determining their shape, size, composition and mass;
  • studying the morphology of the surface (crater distribution) of both asteroids;
  • determining the thermal history and size of the cores of Vesta and Ceres;
  • a greater understanding of the role of water during the development of the asteroids;
  • checking the current hypothesis which sees Vesta as the mother body of the howardite, eucrite and diogenite meteorites, HED for short
  • investigating which meteorites come from Ceres;
  • investigating the geological environment of the HED meteorites.

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Falk Dambowsky

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German Aerospace Center (DLR)
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Ulrich Köhler

German Aerospace Center (DLR)
Institute of Planetary Research
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