Astronomers identify the four billion year old asteroid family in solar system; likely to be the oldest

Astronomers have identified the oldest known asteroid family, which extends throughout the inner region of the main asteroid belt. [caption id=“attachment_3895201” align=“alignleft” width=“380”] Image Courtesy: Southwest Research Institute[/caption] The team also discovered a relatively sparse region of the main asteroid belt, where the few asteroids present are likely pristine relics from early in solar system history. “The family we identified has no name, because it is not clear which asteroid is the parent,” said Kevin Walsh, astronomer at Southwest Research Institute in the US and co-author of a study published online in the journal Science. “This family is so old that it appears to have formed over four billion years ago, before the gas giants in the outer solar system moved into their current orbits. The giant planet migration shook up the asteroid belt, removing many bodies, possibly including the parent of this family,” Walsh said. Finding and studying asteroid families allows scientists to better understand the history of main belt asteroids. But identifying the very oldest asteroid families, those billions of years old, is challenging, because over time, a family spreads out. As asteroids rotate in orbit around the Sun, their surfaces heat up during the day and cool down at night. This creates radiation that can act as a sort of mini-thruster, causing asteroids to drift widely over time. After billions of years, family members would be almost impossible to identify, until now. The team used a novel technique, searching asteroid data from the inner region of the belt for old, dispersed families. They looked for the “edges” of families, those fragments that have drifted the furthest. “Each family member drifts away from the centre of the family in a way that depends on its size, with small guys drifting faster and further than the larger guys,” said team leader Marco Delbo, an astronomer from the Observatory of Cote d’Azur in Nice, France. “If you look for correlations of size and distance, you can see the shapes of old families,” Delbo noted. “By identifying all the families in the main belt, we can figure out which asteroids have been formed by collisions and which might be some of the original members of the asteroid belt,” Walsh said. “We identified all known families and their members and discovered a gigantic void in the main belt, populated by only a handful of asteroids. These relics must be part of the original asteroid belt. That is the real prize, to know what the main belt looked like just after it formed,” Walsh noted. The team plans to apply this new technique to the entire asteroid belt to reveal more about the history of the solar system by identifying the primordial asteroids versus fragments of collisions.