This image shows a model of the protoplanet Vesta, using scientists'  best guess to date of what the surface of the protoplanet might look  like.
It was created as part of an exercise for NASA's Dawn mission  involving mission planners at NASA's Jet Propulsion Laboratory and  science team members at the Planetary Science Institute in Tuscon, Ariz. 
The images incorporate the best data on dimples and bulges of  the protoplanet Vesta from ground-based telescopes and NASA's Hubble  Space Telescope.
The cratering and small-scale surface variations are  computer-generated, based on the patterns seen on the Earth's moon, an  inner solar system object with a surface appearance that may be similar  to Vesta.
Vesta, located in the main asteroid belt between Mars  and Jupiter, formed very early in the history of the solar system and  has one of the oldest surfaces in the system. Scientists are eager to  get their first close-up look so they can better understand this early  chapter.
Dawn science planners have used images like these to  ensure optimal images when Dawn gets into orbit around Vesta in July  2011.
The Dawn mission to Vesta and Ceres is managed by the Jet  Propulsion Laboratory, a division of the California Institute of  Technology in Pasadena, for NASA's Science Mission Directorate in  Washington, DC.
It is a project of the Discovery Program managed at  NASA's Marshall Space Flight Center.
For more information about the Dawn mission visit http://www.nasa.gov/dawn and http://dawn.jpl.nasa.gov .
Image credit: NASA/JPL-Caltech/UCLA/PSI
Subscribe to:
Post Comments (Atom)

No comments:
Post a Comment