File:LhborbitsResonances.png: Difference between revisions

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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 Uranu...
 
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[[Category:Photos and Images - Other]]
[[:Category:Photos and Images - Other]]<br>
Simulation showing the outer planets and planetesimal belt:  
Simulation showing the outer planets and planetesimal belt:  



Latest revision as of 13:19, 14 November 2020

Category:Photos and Images - Other

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.

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'.

http://en.wikipedia.org/wiki/File:Lhborbits.png This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported, 2.5 Generic, 2.0 Generic and 1.0 Generic license.

http://en.wikipedia.org/wiki/Nice_model

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current12:01, 15 February 2014Thumbnail for version as of 12:01, 15 February 20141,360 × 454 (59 KB)Daniel Leech (talk | contribs)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 Uranu...

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