This image of the giant asteroid Vesta was obtained by NASA's Dawn spacecraft in the evening Nov. 27 PST (early morning Nov. 28, UTC), as it was spiraling down from its high altitude mapping orbit to low altitude mapping orbit. Low altitude mapping orbit is the closest orbit Dawn will be making, at an average of 130 miles (210 kilometers) above the giant asteroid's surface. The framing camera obtained this image of an area in the northern mid-latitudes of Vesta from an altitude of about 140 miles (230 kilometers).
The Dawn mission to the asteroids Vesta and Ceres is managed by NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, for NASA's Science Mission Directorate, Washington. UCLA is responsible for overall Dawn mission science. The Dawn Framing Cameras have been developed and built under the leadership of the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, with significant contributions by DLR German Aerospace Center, Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The Framing Camera project is funded by the Max Planck Society, DLR, and NASA/JPL.esearch, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team.
More information about Dawn is online at http://dawn.jpl.nasa.gov .
Name | Value | Additional Values |
---|---|---|
Target | 4 Vesta | |
System | Main Belt | |
Target Type | Asteroid | |
Mission | Dawn | |
Instrument Host | Dawn | |
Host Type | Orbiter | |
Instrument | Framing Camera (FC) | |
Detector | ||
Extra Keywords | Grayscale | |
Acquisition Date | ||
Release Date | 2011-12-12 | |
Date in Caption | ||
Image Credit | NASA/JPL-Caltech/UCLA/MPS/DLR/IDA | |
Source | photojournal.jpl.nasa.gov/catalog/PIA15175 | |
Identifier | PIA15175 |