KnowraNice modelLinked fromLinked fromThe 21 pages that link to Nice model, each with the reason it gives.All 21Broader topic 5Related 15Compared with 1Orbital resonanceBroader topic: Its migration history uses resonances to explain the giant planets' later orbital arrangement.Planetary migrationBroader topic: It explains several outer Solar System features through giant-planet migration and instability.JupiterRelated: 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.UranusBroader topic: The model explains how Uranus may have reached its present orbit during early planetary instability.Mean-motion resonanceBroader topic: Its migration history can explain the capture and distribution of resonant Kuiper belt objects.Grand Tack hypothesisCompared with: Unlike the Grand Tack, it focuses chiefly on later giant-planet rearrangement.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.Orbital migrationBroader topic: It links giant-planet migration to the Solar System's later 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.
KnowraNice modelLinked fromLinked fromThe 21 pages that link to Nice model, each with the reason it gives.All 21Broader topic 5Related 15Compared with 1Orbital resonanceBroader topic: Its migration history uses resonances to explain the giant planets' later orbital arrangement.Planetary migrationBroader topic: It explains several outer Solar System features through giant-planet migration and instability.JupiterRelated: 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.UranusBroader topic: The model explains how Uranus may have reached its present orbit during early planetary instability.Mean-motion resonanceBroader topic: Its migration history can explain the capture and distribution of resonant Kuiper belt objects.Grand Tack hypothesisCompared with: Unlike the Grand Tack, it focuses chiefly on later giant-planet rearrangement.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.Orbital migrationBroader topic: It links giant-planet migration to the Solar System's later 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.