Back Nice-model Afrikaans نموذج نيس Arabic Model de Niça Catalan Model z Nice Czech Nizza-Modell German Μοντέλο της Νίκαιας Greek Modelo de Niza Spanish مدل نیس Persian Nizzan malli Finnish Modèle de Nice French

Nice model

The Nice (/ˈniːs/) model is a scenario for the dynamical evolution of the Solar System. It is named for the location of the Côte d'Azur Observatory—where it was initially developed in 2005—in Nice, France.[1][2][3] It proposes the migration of the giant planets from an initial compact configuration into their present positions, long after the dissipation of the initial protoplanetary disk. In this way, it differs from earlier models of the Solar System's formation. This planetary migration is used in dynamical simulations of the Solar System to explain historical events including the Late Heavy Bombardment of the inner Solar System, the formation of the Oort cloud, and the existence of populations of small Solar System bodies such as the Kuiper belt, the Neptune and Jupiter trojans, and the numerous resonant trans-Neptunian objects dominated by Neptune.

Simulation showing the outer planets and planetesimal belt: a) early configuration, before Jupiter and Saturn reach a 2:1 resonance; b) scattering of planetesimals into the inner Solar System after the orbital shift of Neptune (dark blue) and Uranus (light blue); c) after ejection of planetesimals by planets.[4]
  1. ^ "Solving solar system quandaries is simple: Just flip-flop the position of Uranus and Neptune". Press release. Arizona State University. 11 Dec 2007. Retrieved 2009-03-22.
  2. ^ Desch, S. (2007). "Mass Distribution and Planet Formation in the Solar Nebula". The Astrophysical Journal. 671 (1): 878–893. Bibcode:2007ApJ...671..878D. doi:10.1086/522825. S2CID 120903003.
  3. ^ Crida, A. (2009). "Solar System Formation". Reviews in Modern Astronomy. 21: 215–227. arXiv:0903.3008. Bibcode:2009RvMA...21..215C. doi:10.1002/9783527629190.ch12. ISBN 9783527629190. S2CID 118414100.
  4. ^ R. Gomes; H. F. Levison; K. Tsiganis; A. Morbidelli (2005). "Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets" (PDF). Nature. 435 (7041): 466–9. Bibcode:2005Natur.435..466G. doi:10.1038/nature03676. PMID 15917802. S2CID 4398337.

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