Linked from

The 57 pages that link to Protoplanetary disk, each with the reason it gives.

• Asteroid beltNarrower topic: The belt is leftover material from the disk that formed the Solar System.

• PlanetesimalNarrower topic: Planetesimals originate within this planet-forming environment.

• CeresNarrower topic: Ceres formed from the material left over from the Sun’s planet-forming disk.

• Planet formationNarrower topic: Planet formation begins within this rotating reservoir of material.

• Mean-motion resonanceNarrower topic: Disk-driven migration can change planetary period ratios and establish resonant chains.

• Pebble accretionNarrower topic: Pebble accretion takes place within this gas-rich environment.

• Core accretionNarrower topic: Its gas and solids supply the material from which cores and atmospheres grow.

• Grand Tack hypothesisNarrower topic: The disk supplies the torques that move Jupiter and Saturn.

• Gas giantNarrower topic: Gas giants originate in the gas-rich disks around young stars.

• Terrestrial planetNarrower topic: Terrestrial planets assembled from solid material in the inner regions of the Sun’s disk.

• Disk instabilityNarrower topic: The model operates within the massive, cold outer regions of these disks.

• Dust coagulationNarrower topic: It provides the setting in which dust coagulation can begin building planetary solids.

• Planetary accretionNarrower topic: Accretion takes place within this reservoir of solid material and gas.

• Comet nucleusNarrower topic: The nucleus’s building materials originated in the Sun’s protoplanetary disk.

• Interstellar objectNarrower topic: Interstellar visitors are likely fragments ejected from such disks during planetary-system formation.

• ProplydNarrower topic: A proplyd is an externally irradiated, observable instance of a protoplanetary disk.

• ProtoplanetNarrower topic: Protoplanets grow within this reservoir of gas and solid material.