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1 Summary
- 1.1 Main graph
2 Data source
3 Licensing

[edit] Summary

Groups of irregular satellites of Jupiter.

The most distant regular satellite Callisto is shown for reference. Plotted by a program written by Eurocommuter.

[edit] Main graph

The position of a satellite (in polar co-ordinates) represents
- its orbit's semi-major axis a (horizontal axis: in Gm and as a fraction of the Hill sphere's radius)
- orbit’s inclination i in degrees
The size of the circle illustrates the satellite's size relative to others:
The eccentricity of selected orbits is shown indirectly by a segment extending from the left (pericenter) to the apocentre to the right. In other words, the segment illustrates the variations of the object's distance from the planet.

[edit] Data source

Mean Orbital Elements JPL (Aug 2006).
Size estimations: Sheppard Sheppard pages (Aug 2006)

Description	Groups of irregular satellites of Jupiter
Source	Plotted by a program written by author
Date	26 August 2006
Author	User:Eurocommuter
Permission	see Licence tag

[edit] Licensing

I, the author of this work, hereby publish it under the following licenses:

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".