| Small Bodies Mission Support |
The DAWN spacecraft launched September 27, 2007, 7:34 a.m. EDT.
DAWN completed an initial check phase in early December 2007
and began its interplanetary cruise phase on December 17-21, 2007.
A Mars gravity assist is scheduled for February 9, 2009. It will put the
spacecraft on a trajectory to rendezvous with the asteroid 4 Vesta
in August 2011. After 11 months of observing, the spacecraft will
depart from Vesta in May 2012 and spend over 2.5 years years travelling
to the dwarf planet Ceres (or 1 Ceres, the asteroid). DAWN will
rendezvous with Ceres in February 2015 and will spend 6 months taking
measurements before departing in July 2015 (end of mission).
Dawn's primary science goal is to gain an understanding of the conditions
and processes occurring when the solar system was only about 10 million years old.
It will measure the size, shape, mass, volume and spin rate of the two
protoplanets, Vesta and Ceres, to determine their internal structure, density and
homogeneity. Dawn will also investigate their thermal history by measuring the
elemental and mineral abundances. It will image their surfaces to determine their
bombardment and tectonic history, and use gravity, spin and magnetic data to limit
the size of any metallic core.
The DAWN Mission web site is maintained by UCLA.
The SBN is the lead PDS node to archive the DAWN mission data.
| Instrument/Investigation | Measuring | Small Bodies Data available below |
|---|---|---|
| Framing Camera (FC) | Full surface imagery in seven colors at Vesta and three at Ceres | none |
| Visible and Infrared Mapping Spectrometer (VIR) | Full surface mineralogical mapping in three bands: 0.35-0.9, 0.8-2.5, and 2.4-5.0 micron | none |
| Gamma Ray and Neutron Detector (GRaND) | Abundances of major rock-forming elements (O, Mg, Al, Si, Ca, Ti, and Fe), trace elements (Gd and Sm), long-lived radioactive elements (K, Th, and U), and light elements such as H, C, and N which are major constituents of ices | none |
| Radio Science (RSS) | Radio tracking to determine mass, gravity field, principal axes, rotational axis and moments of inertia | none |
| Instrument/ Investigation Description | Target | Description of Available Data | Data Link |
|---|---|---|---|
| No data available yet | |||
| Target | Target Type | Other Data Sets Targeting this Object |
|---|---|---|
| 4 Vesta | Asteroid | |
| 1 Ceres/Ceres | Asteroid/Dwarf Planet |
Last update: 26 March 2008, McLaughlin