Image:TheIrregulars URANUS retro.svg

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[edit] Summary

Retrograde irregular satellites of Uranus. The most distant regular satellite Oberon 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 the orbit 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

Based on the data collected by Sheppard & Jewitt (July 2006) [1].

Description

Irregular retrograde satellites of Uranus

Source

Plotted by a program written by the User:Eurocommuter

Date

21 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
current23:41, 21 August 2006400×400 (10 KB)Eurocommuter (Clean-up)
23:17, 21 August 2006400×400 (9 KB)Eurocommuter (Showing Oberon for reference.)
16:14, 21 August 2006400×400 (9 KB)Eurocommuter (Retrograde irregulars of Uranus. By Eurocommuter.)
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