«So the fact that we can still see these disks around a 10 - to 20 - million - year - old star means that the dust is being replenished by collisions
between planetesimals.»
Not exact matches
In contrast to earlier observations the team did not observe dust that will later form into planets, but dust created in collisions
between small planets of a few kilometres in size — objects called
planetesimals that are similar to the asteroids and comets of the Solar System.
An image of the circumstellar dust disk around the young star HR4796A, which is thought to have been created by collisions
between asteroids and
planetesimals that were left over following the star's formation.