Image:TheIrregulars JUPITER GROUPS.svg

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Contents

[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
(Reusing this image)

see Licence tag

[edit] Licensing

I, the copyright holder of this work, hereby publish it under the following licenses:
GNU head 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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File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeDimensionsUserComment
current08:35, 30 August 2006400×400 (19 KB)Eurocommuter (Switched to data from JPL.)
15:15, 26 August 2006400×400 (19 KB)Eurocommuter (Groups of irregular satellites of Jupiter. By Eurocommuter. )
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