Linked from

The 17 pages that link to Planet formation, each with the reason it gives.

• Protoplanetary diskNarrower topic: Disk observations constrain how quickly and efficiently planets assemble.

• T Tauri starNarrower topic: Observations of T Tauri disks expose the early stages of this process.

• Cosmic dustNarrower topic: Dust grains are the starting solids whose collisions can build planetesimals.

• Debris diskNarrower topic: Debris disks preserve evidence of leftover solids and later collisions after primary planet formation.

• Planetary-mass objectNarrower topic: Whether formation history should define a planet remains contested for isolated and high-mass objects.

• Planetary systemNarrower topic: It explains how a disk becomes a planetary system.

• Epsilon EridaniNarrower topic: Its rings preserve evidence about how planetesimals and planets developed around a young star.

• ProtoplanetNarrower topic: Protoplanets are an intermediate stage in this broader process.

• TW HydraeNarrower topic: TW Hydrae’s disk offers observations of an early setting for this process.