By 2001, over 900 candidate stars had been found to possess a debris disk.

It is part of a system that also contains a debris disk and at least four massive planets.

In 2003 it was determined that this is more likely a circumstellar debris disk.

This indicated the presence of a debris disk in orbit around the star.

There is a debris disk located at least 86 astronomical units from the star.

These systems are usually referred to as "debris disks".

This strong field would brake against the debris disk left behind by the supernova, which has thus far been unknown to science.

In 1984, Beta was the first star discovered to have a debris disk.

The debris disk is likely to be composed of mainly heavier metals.

This debris disk has been extensively studied since that time.