Linked from

The 10 pages that link to Debris disk, each with the reason it gives.

• Protoplanetary diskCompared with: It is a later, largely gas-poor stage distinct from a protoplanetary disk.

• Planetary ringsCompared with: Debris disks surround stars rather than planets and span vastly larger scales.

• Tidal disruptionRelated: Disruption and collisions can replenish the orbiting debris from which such disks form.

• Poynting–Robertson effectBroader topic: Drag alters the distribution of grains supplied by collisions in these disks.

• Meteor showerNarrower topic: Meteor streams are localized Solar System debris, rather than broad circumstellar disks.

• FomalhautNarrower topic: Fomalhaut’s defining circumstellar structure is a resolved debris disk.

• Epsilon EridaniNarrower topic: Epsilon Eridani’s dusty belts are observed debris structures, not directly imaged planets.

• Tau CetiBroader topic: Tau Ceti’s debris disc is prominent and may indicate a dynamically active outer system.

• Circumstellar discBroader topic: This later evolutionary stage is sustained by collisions among solid bodies.

• TW HydraeCompared with: Unlike a mature debris disk, TW Hydrae retains gas from its primordial disk.