KnowraNice modelLinked fromLinked fromThe 21 pages that link to Nice model, each with the reason it gives.All 21Broader topic 5Related 15Compared with 1JupiterRelated: It describes how Jupiter’s interactions with other giants may have rearranged their orbits.Kuiper beltRelated: It links giant-planet migration to the belt's dynamical structure.Late Heavy BombardmentRelated: Its original version proposed that giant-planet migration triggered a late surge of impacts.Solar SystemRelated: It links giant-planet migration to the distribution of distant icy objects and impactors.Asteroid beltRelated: It offers a route for scattering and repopulating small bodies in the belt.SaturnRelated: Planetary migration may have influenced Saturn’s orbit and the outer Solar System.Solar System formationRelated: It links later giant-planet migration to the present arrangement of distant small bodies.Kirkwood gapRelated: It provides one framework for studying how early planetary migration altered resonant asteroid populations.Nebular hypothesisRelated: It addresses how the giant planets reached their present orbital arrangement.Trojan asteroidRelated: Planetary migration in this model can capture and redistribute Trojan asteroids.Long-period cometRelated: Planetary migration and scattering help explain the emplacement of distant icy bodies.Scattered discRelated: It describes early planetary dynamics that could scatter icy bodies into distant orbits.Jupiter TrojanRelated: In this model, planetary migration captured and redistributed many Jupiter Trojans.Titius–Bode lawRelated: It explains major rearrangements of the outer Solar System without relying on the distance rule.Formation and evolution of the Solar SystemRelated: It explains how an initially compact giant-planet system could produce today’s distant populations.