Linked from

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

• AsteroidRelated: Asteroids originated as solid material in the Sun’s early disk.

• Planetary migrationRelated: Its gravity and fluid response can drive migration before the gas disperses.

• Interstellar dustRelated: Dust grains in these disks collide, grow, and supply the solid building material of planets.

• Kuiper beltRelated: The Kuiper belt's objects began as planet-building material in the Sun's disk.

• Solar SystemRelated: The Solar System’s early disk set the conditions for planet formation.

• Gravitational instabilityRelated: Strong disk self-gravity can fragment the disk into bound clumps.

• PlanetRelated: Planet formation begins in the material orbiting a young star.

• Solar nebulaRelated: Disks observed around young stars provide modern analogues for the solar nebula.

• T Tauri starRelated: Its evolving structure records the conditions for planet formation around T Tauri stars.

• Herschel Space ObservatoryRelated: Herschel measured water and other molecules in disks that supply material for planets.

• Nebular hypothesisRelated: The disk provides the setting and raw material for planetary assembly.

• Spitzer Space TelescopeRelated: Infrared observations traced warm dust and molecules in planet-forming disks.

• Orbital migrationRelated: Its gas and solids provide material that exchanges momentum with forming planets.

• Pre-main-sequence starRelated: Its evolution alongside the central star links stellar youth to the formation of planetary systems.

• Large Binocular TelescopeRelated: Infrared imaging can reveal structures in disks that mark planet-forming processes.

• Planetary systemRelated: It supplies the material from which planets and smaller bodies assemble.

• Substellar objectRelated: Disk-based formation can produce objects in the planetary-mass range.

• Carbon planetRelated: Disk chemistry and transport determine whether carbon-rich building material can accumulate.

• Herbig Ae/Be starRelated: The circumstellar disks around these stars can host planet formation.

• Rho Ophiuchi cloud complexRelated: Young stars in the complex allow studies of disks at early evolutionary stages.

• Atacama Large Millimeter/submillimeter ArrayRelated: ALMA images disk structures that trace dust growth and possible planet formation.

• Trapezium ClusterRelated: Young stars near the cluster retain disks exposed to intense ultraviolet radiation.

• TW HydraeRelated: Its disk makes TW Hydrae a direct laboratory for studying planet-forming material.