Vesta is one of the brightest objects in the solar system and the only asteroid in the so-called main belt between Mars and Jupiter visible to the naked eye from Earth. Dawn has found that some areas on Vesta can be nearly twice as bright as others, revealing clues about the asteroid’s history.
“Our analysis finds this bright material originates from Vesta and has undergone little change since the formation of Vesta over 4 billion years ago,” said Jian-Yang Li from the University of Maryland, College Park. “We’re eager to learn more about what minerals make up this material and how the present Vesta surface came to be.”
Bright areas appear everywhere on Vesta but are most predominant in and around craters. The areas vary from several hundred feet to around 10 miles (16 kilometers) across. Rocks crashing into the surface of Vesta seem to have exposed and spread this bright material. This impact process may have mixed the bright material with darker surface material.
While scientists had seen some brightness variations in previous images of Vesta from NASA’s Hubble Space Telescope, Dawn scientists did not expect such a wide variety of distinct dark deposits across its surface. The dark materials on Vesta can appear dark gray, brown, and red. They sometimes appear as small, well-defined deposits around impact craters. They also can appear as larger regional deposits, like those surrounding the impact craters scientists have nicknamed the “snowman.”
“One of the surprises was the dark material is not randomly distributed,” said David Williams from Arizona State University in Tempe. “This suggests underlying geology determines where it occurs.”
The dark materials seem to be related to impacts and their aftermath. Scientists theorize that carbon-rich asteroids could have hit Vesta at speeds low enough to produce some of the smaller deposits without blasting away the surface.
Higher-speed asteroids also could have hit Vesta’s surface and melted the volcanic basaltic crust, darkening existing surface material. That melted conglomeration appears in the walls and floors of impact craters, on hills and ridges, and underneath brighter, more recent material called ejecta — material thrown out from a space rock impact.
Vesta’s dark materials suggest that the giant asteroid may preserve ancient materials from the asteroid belt and beyond, possibly from the birth of the solar system.
“Some of these past collisions were so intense, they melted the surface,” said Brett Denevi from the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland. “Dawn’s ability to image the melt marks a unique find. Melting events like these were suspected, but never before seen on an asteroid.”
Dawn launched in September 2007. It will reach its second destination, Ceres, in February 2015.
“Dawn’s ambitious exploration of Vesta has been going beautifully,” said Marc Rayman from NASA’s Jet Propulsion Laboratory in Pasadena, California. “As we continue to gather a bounty of data, it is thrilling to reveal fascinating alien landscapes.”
