集信:Lhborbits.png

集信㭲 ‎(1.360×454點影、戟𡱩集信：56kB、矯MIME：image/png)

集信尼得留於威其迷𠫾阿・古門吧伮固体得使用於各預案恪。 𠳒描寫𧵑集信在張模寫得顯示𨑜低。

Summary

Description
English: Simulation showing the outer planets and the 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.[1]
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[1]
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.[1]
Čeština: Simulace vlivu vnějších planet na vývoj Kuiperova pásu:
  • a) Kuiperův pás před tím, než se planety Jupiter a Saturn dostaly do vzájemné dráhové rezonance 2:1.
  • b) Rozptýlení těles Kuiperova pásu poté, co začal měnit svou oběžnou dráhu Neptun.
  • c) Rozptýlená tělesa se dostávala do vlivu Jupiteru, který je vymrštil pryč.

Zobrazené planety: Jupiter (zelený kruh), Saturn (oranžový kruh), Uran (bledě modrý kruh) a Neptun (tmavě modrý kruh).

Simulace byla vytvořena za použití údajů z tzv. Modelu z Nice.[1]
العربية: محاكاة تُظهر حزام كايبر والكواكب الخارجية:
  • أ) قبل أن يصل مقياس رنين زحل إلى 1:2 بالنسبة للمشتري.
  • ب) تبعثر أجرام حزام كايبر في المجموعة الشمسية بعد التحول المداري لنبتون.
  • ج) بعد قذف المُشتري لأجرام حزام كايبر
Source Own work
Author en:User:AstroMark
  1. ↑ a b c d Origin of the cataclysmic Late Heavy Bombardment period of the terrestrial planets, Gomes, Levison, Tsiganis, Morbidelli - Nature 26, May 2005.

Licensing

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歷史集信

扨𠓨𣈜／𣇞抵䀡內容集信在時點妬。

𣈜／𣇞形䀡𠓀戟櫸成員描寫
現在02:06、𣈜8𣎃2𢆥2019形䀡𠓀𧵑番版𣅶02:06、𣈜8𣎃2𢆥20191.360×454 (56kB)wikimediacommons>KesäperunaRemoved white line.

張𢖖󠄁使用集信尼：

特性形

集信尼貯通信補充、固体得添自𣛠影技術數或𣛠𢭯得使用抵造或數化𣜿。

裊集信㐌得𢯢𢷮𬧺貝狀態班頭、𠬠數枝節固体空反映𣹓𨁥集信㐌𢯢𢷮。

𥙩自「http://www.hannom-rcv.org/wi/index.php/集信:Lhborbits.png」