- Vesta, the second largest object in the main asteroid belt, is a protoplanet, not an asteroid.
- Vesta formed within 300 million years of the beginning of the solar system's existence.
- Pieces of Vesta have been found on Earth in the form of a particular type of meteorite.
Vesta, the second largest object in the main asteroid belt, has an iron core, a varied surface, layers of rock and possibly a magnetic field - all signs of a planet in the making, not an asteroid.
So concludes an international team of scientists treated to a virtual front row seat at Vesta for the past 10 months, courtesy of NASA's Dawn robotic probe.
PHOTOS: Giant Asteroid Vesta's Mysteries Revealed
They have a bit more ground to cover before Dawn leaves Vesta's cratered, lava-like surface in late August to rendezvous with the king of the asteroid belt, Ceres, another type of protoplanet believed to be flush with water ice.
Already however, the Dawn science team has confirmed long-held theories about Vesta's history, a timeline that dates back to within 300 million years of the beginning of the solar system's existence.
"Vesta is like a time probe we haven't had in the solar system before," Dawn lead scientist Christopher Russell, with the University of California, Los Angeles, told Discovery News.
"We have a body that formed very, very early so we know from Vesta what conditions were like back then. We would not have learned that from a body like the moon or Earth. We would not be able to go back that far in time," he said.
ANALYSIS: Asteroid Vesta Not An Asteroid After All
From meteorites - some of which now have been directly sourced to Vesta - scientists know that the solar system is about 4.6 billion years old. Analysis of craters on the moon date back a little more than 3 billion years. Evidence of earlier geologic lunar events were obliterated during a period of heavy bombardment, a fate Vesta apparently escaped.
Which is not to say the body, which spans about 330 miles in diameter, is without scars. Among the pits imaged by Dawn is a double-whammy crater - a basin inside a basin - that is believed to be the source of two groups of meteorites found on Earth.
"There is evidence in the meteoritic record to give us co-incident dates with the two impacts that we've dated on Vesta," Russell said.
Scientists also found rings around the impact basins, a phenomenon that may be related to Vesta's iron core.
"We haven't done simulations of this so we don't really know yet," Russell said. "I would guess that the iron core sort of holds Vesta in place and the (impacting body) rings around that."
ANALYSIS: Asteroid Vesta Comes into Focus
As to why Vesta never made it to full planethood, scientists point to Jupiter. When the giant gas planet formed, nearby bodies such as Vesta found their orbits perturbed.
"Jupiter started to act like a spoon in a pot, stirring up the asteroid belt and the asteroids started bumping into one another. If they're just out there gently orbiting and everything is going smoothly, then without Jupiter in the picture, they would gather mass and get bigger and bigger and bigger. But with Jupiter there, stirring the pot, then the asteroids start bumping into one another and breaking apart, so nothing grew in that region, but started to shrink," Russell said.
Vesta has been somewhat reduced by collisions, but it - unlike smaller bodies - survived.
"At the moment, we do not have any evidence of any other bodies like Vesta. It was not completely destroyed, like many other asteroids in the main belt," planetary scientist Maria Cristina De Sanctis, with Italy's National Institute for Astrophysics in Rome, told Discovery News.
The findings are included in six papers on Vesta published in this week's Science.