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Dawn was NASAs first truly interplanetary spaceship. The mission featured extended stays at two very different extraterrestrial bodies: giant asteroid Vesta and dwarf planet Ceres. Both small worlds reside in the debris-strewn main asteroid belt between Mars and Jupiter.
These measurements will help determine the thermal history, size of the core, role of water in asteroid evolution and what meteorites found on Earth come from these bodies, with the ultimate goal of understanding the conditions and processes present at the solar systems earliest epoch and the role of water content and
The Dawn mission was designed to study two large bodies in the asteroid belt in order to answer questions about the formation of the Solar System, as well as to test the performance of its ion thrusters in deep space.
About this book This book describes the Dawn mission, its exploration and scientific objectives, the instruments that accomplish those objectives, the operations plan and the education and outdocHub plan. It is directed to those studying asteroids and the evolution of the solar system.
Dawn measured Ceres surface composition and found a chemical (ammonia), which requires the colder temperatures of the outer solar systembeyond the orbit of Jupiterto condense. Ceres may have formed there and then drifted closer to the Sun.

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Dawn data helped confirm Vesta as the parent body of the family of meteorites known as howardite-eucrite-diogenite (HED) [16]. Intriguingly, more HED meteorites are known than meteorites identified as originating on the Moon or Mars [17].

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