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This suggests either that a second mechanism was at work for that planet, or that the early simulations did not reproduce the evolution of the giant planets orbits.

The migration of the outer planets is also necessary to account for the existence and properties of the Solar System 's outermost regions.

Neptune's high eccentricity causes its mean-motion resonances to overlap and orbits in the region between Neptune and its mean motion resonances to become chaotic.

The orbits of objects between Neptune and the edge of the planetesimal disk at this time can evolve outward onto stable low-eccentricity orbits within this region.

When Neptune's eccentricity is damped by dynamical friction they become trapped on these orbits. These objects form a dynamically-cold belt, since their inclinations remain small during the short time they interact with Neptune.

Later, as Neptune migrates outward on a low eccentricity orbit, objects that have been scattered outward are captured into its resonances and can have their eccentricities decline and their inclinations increase due to the Kozai mechanism , allowing them to escape onto stable higher-inclination orbits.

Other objects remain captured in resonance, forming the plutinos and other resonant populations. These two population are dynamically hot, with higher inclinations and eccentricities; due to their being scattered outward and the longer period these objects interact with Neptune.

This evolution of Neptune's orbit produces both resonant and non-resonant populations, an outer edge at Neptune's resonance, and a small mass relative to the original planetesimal disk.

The excess of low-inclination plutinos in other models is avoided due to Neptune being scattered outward, leaving its resonance beyond the original edge of the planetesimal disk.

The differing initial locations, with the cold classical objects originating primarily from the outer disk, and capture processes, offer explanations for the bi-modal inclination distribution and its correlation with compositions.

It predicts a greater average eccentricity in classical Kuiper belt object orbits than is observed 0. It also cannot explain the apparent complete absence of gray objects in the cold population, although it has been suggested that color differences arise in part from surface evolution processes rather than entirely from differences in primordial composition.

The shortage of the lowest-eccentricity objects predicted in the Nice model may indicate that the cold population formed in situ.

In addition to their differing orbits the hot and cold populations have differing colors. The cold population is markedly redder than the hot, suggesting it has a different composition and formed in a different region.

Objects scattered outward by Neptune onto orbits with semi-major axis greater than 50 AU can be captured in resonances forming the resonant population of the scattered disc , or if their eccentricities are reduced while in resonance they can escape from the resonance onto stable orbits in the scattered disc while Neptune is migrating.

When Neptune's eccentricity is large its aphelion can reach well beyond its current orbit. Objects that attain perihelia close to or larger than Neptune's at this time can become detached from Neptune when its eccentricity is damped reducing its aphelion, leaving them on stable orbits in the scattered disc.

Objects scattered outward by Uranus and Neptune onto larger orbits roughly 5, AU can have their perihelion raised by the galactic tide detaching them from the influence of the planets forming the inner Oort cloud with moderate inclinations.

Others that reach even larger orbits can be perturbed by nearby stars forming the outer Oort cloud with isotropic inclinations. Objects scattered by Jupiter and Saturn are typically ejected from the Solar System.

The Nice model has undergone a number of modifications since its initial publication. Some changes reflect a better understanding of the formation of the Solar System while others were made after significant differences between its predictions and observations were identified.

Hydrodynamical models of the early Solar System indicate that the orbits of the giant planets would converge resulting in their capture into a series of resonances.

The first could result in the orbit of Mars crossing that of the other terrestrial planets destabilizing the inner Solar System.

If the first was avoided the latter would still leave the orbits of the terrestrial planets with larger eccentricities.

The first modifications to the Nice model were the initial positions of the giant planets. Investigations of the behavior of planets orbiting in a gas disk using hydrodynamical models reveal that the giant planets would migrate toward the Sun.

If the migration continued it would have resulted in Jupiter orbiting close to the Sun like recently discovered exoplanets known as hot Jupiters.

Saturn's capture in a resonance with Jupiter prevents this, however, and the later capture of the other planets results in a quadruple resonant configuration with Jupiter and Saturn in their resonance.

Gravitational encounters with Pluto-massed objects in the outer disk would stir their orbits causing an increase in eccentricities, and through a coupling of their orbits, an inward migration of the giant planets.

During this inward migration secular resonances would be crossed that altered the eccentricities of the planets' orbits and disrupted the quadruple resonance.

A late instability similar to the original Nice model then follows. Unlike the original Nice model the timing of this instability is not sensitive to the planets initial orbits or the distance between the outer planet and the planetesimal disk.

The combination of resonant planetary orbits and the late instability triggered by these long distant interactions was referred to as the Nice 2 model.

The second modification was the requirement that one of the ice giants encounters Jupiter, causing its semi-major axis to jump.

In this jumping-Jupiter scenario , an ice giant encounters Saturn and is scattered inward onto a Jupiter-crossing orbit, causing Saturn's orbit to expand; then encounters Jupiter and is scattered outward, causing Jupiter's orbit to shrink.

This results in a step-wise separation of Jupiter's and Saturn's orbits instead of a smooth divergent migration. Most of the rocky impactors of the Late Heavy Bombardment instead originate from an inner extension that is disrupted when the giant planets reach their current positions, with a remnant remaining as the Hungaria asteroids.

This gap may be bridged by a slow dust-driven migration over several million years following an early escape from resonance.

Although this implies that the instability occurred before the formation of the terrestrial planets and could not be the source of the Late Heavy Bombardment, [47] [48] the advantage of an early instability is reduced by the sizable jumps in the semi-major axis of Jupiter and Saturn required to preserve the asteroid belt.

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