Linked from

The 38 pages that link to Planetary migration, each with the reason it gives.

• Orbital resonanceRelated: Migration can sweep resonances across small bodies and capture them into new orbital relationships.

• Star systemRelated: Migration helps explain why planets may end far from their formation locations.

• Planetary scienceRelated: Migration may explain planetary system layouts that cannot arise from local formation alone.

• Asteroid beltRelated: Early giant-planet migration may have sculpted and populated the belt.

• SaturnRelated: Migration models help explain Saturn’s present orbit and its role in Solar System evolution.

• Tidal heatingRelated: Migration can alter eccentricities and resonances, changing tidal heating over time.

• PlanetRelated: Migration can rearrange a system and help planets clear or share orbital regions.

• Nice modelNarrower topic: The model’s central process is migration driven by exchanges of orbital energy and angular momentum.

• Planet formationRelated: Migration can reshape planetary systems while their disks are still present.

• UranusRelated: Migration models use Uranus's orbit and the outer planets' arrangement to reconstruct Solar System history.

• Super-EarthRelated: Migration offers a route for many close-orbiting super-Earths to reach their observed locations.

• Mean-motion resonanceRelated: Changing orbital periods sweep resonances across small-body populations and can capture them.

• Pebble accretionRelated: Pebble accretion changes a growing planet's mass while disk torques move it through the pebble supply.

• Core accretionRelated: Migration can bring a planet formed farther out into a close-in orbit.

• Grand Tack hypothesisNarrower topic: The Grand Tack is a specific, large-scale episode of planetary migration.

• Rings of SaturnRelated: Ring structures can preserve clues about past satellite orbits and gravitational interactions.

• Trans-Neptunian objectRelated: Neptune's migration could have captured and rearranged objects in the Kuiper belt.

• Gas giantRelated: Newly formed giant planets can move substantially from their birth orbits.

• Kirkwood gapRelated: Changes in Jupiter’s orbit may have reshaped resonances and asteroid distributions.

• Terrestrial planetRelated: Migration models help explain how giant planets may have altered the delivery and orbits of rocky worlds.

• 51 Pegasi bRelated: Migration offers a leading explanation for how a giant planet reached such a tight orbit.

• Disk instabilityRelated: Migration may carry a fragment formed far from its star toward a tighter orbit.

• Planetary accretionRelated: Migration can move accreting planets through regions with different solid supplies.

• Free-floating planetRelated: Migration can bring planets into encounters that end in ejection.

• Planet NineRelated: Formation models must explain how a proposed distant planet reached and retained its hypothesized orbit.

• Planetary massRelated: Planetary masses affect how strongly planets exchange angular momentum and migrate.

• Trojan asteroidNarrower topic: Migration can alter Trojan orbits and help explain how distant populations were assembled.

• ExomoonRelated: A planet's migration can destabilize, capture, or remove its moons.

• Irregular satelliteRelated: Changing planetary orbits can alter satellite stability and the conditions for capture.

• Planetary systemRelated: Migration can rearrange a system long after planets begin forming.

• Didier QuelozRelated: Hot Jupiters such as 51 Pegasi b prompted theories of migration from distant formation sites.

• Rogue planetRelated: Migration can bring planets into unstable configurations that trigger ejection.

• Scattered discRelated: Neptune’s outward migration helped shape the distant small-body populations, including the scattered disc.

• Jupiter TrojanRelated: Migration can move stable regions and capture small bodies into Trojan orbits.

• Titius–Bode lawRelated: It can reshape orbital spacing, unlike the law’s fixed numerical prescription.

• Epsilon EridaniRelated: Migration could help explain how giant planets and debris belts acquired their present arrangement.

• Sub-brown dwarfRelated: Disk-born planetary-mass objects can be displaced or ejected from their original systems.

• Hills cloudRelated: Early Solar System migration may have scattered icy bodies into distant reservoirs.