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English: Simulation showing Outer Planets and Kuiper Belt: a)Before Jupiter/Saturn 2:1 resonance b)Scattering of Kuiper Belt objects into the solar system after the orbital shift of Neptune c)After ejection of Kuiper Belt bodies by Jupiter. Planets shown: Jupiter (green circle), Saturn (orange circle), Uranus (light blue circle) and Neptune (dark blue circle). Simulation created using data from the Nice Model.
Français : Simulation montrant les planètes externes et la ceinture de Kuiper :
- a) Avant la résonance 2:1 de Jupiter et Saturne.
- b) Dispersion des objets de la ceinture de Kuiper dans le système solaire après la migration de Neptune.
- c) Après l'éjection d'objets de la ceinture de Kuiper par Jupiter.
L'orbite de Jupiter est représentée en vert, Saturne en orange, Uranus en bleu clair et Neptune en bleu foncé. Simulation créée sur la base de données du Nice Model
Deutsch: Eine Simulation, die die äußeren Planeten und den Kuipergürtel zeigt:
- a) Vor der Jupiter/Saturn 2:1 Resonanz.
- b) Zerstreuung der Objekte des Kuipergürtels in das Sonnensystem, nachdem sich die Umlaufbahn Neptuns verschoben hatte.
- c) Nach dem Ausstoß von Objekten des Kuipergürtels durch Jupiter.
Gezeigte Planeten: Jupiter (grüner Kreis), Saturn (oranger Kreis), Uranus (hellblauer Kreis) und Neptun (dunkelblauer Kreis). Die Simulation wurde mit Hilfe von Daten des Nice Models erstellt.
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self-made |
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en:User:AstroMark |
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation license, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled " GNU Free Documentation license".
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- ↑ a b c Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets, Gomes, Levison, Tsiganis, Morbidelli - Nature 26, May 2005.
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1,360×454 (59 KB) |
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