
Astronomers using data from NASA's Wide-field Infrared Survey Explorer (WISE) have identified 28 new families of asteroids in the main belt between Mars and Jupiter.
The findings are a critical step in understanding the origins of asteroid families, and the collisions thought to have created these rocky clans.
An asteroid family is formed when a collision breaks apart a large parent body into fragments of various sizes. Some collisions leave giant craters. For example, the asteroid Vesta's southern hemisphere was excavated by two large impacts.
Other smash-ups are catastrophic, shattering an object into numerous fragments. The cast-off pieces move together in packs, travelling on the same path around the Sun, but over time the pieces become more and more spread out.
"We're separating zebras from the gazelles," said Joseph Masiero of NASA's Jet Propulsion Laboratory in Pasadena, California, and lead author of the study.
"Before, asteroid family members were harder to tell apart because they were travelling in nearby packs. But now we have a better idea of which asteroid belongs to which family," Masiero said in a statement.





















