File:Saturn's irregular satellites.png
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Size of this preview: 800 × 561 pixels. Other resolutions: 320 × 224 pixels | 640 × 449 pixels | 1,024 × 718 pixels | 1,280 × 898 pixels | 2,338 × 1,640 pixels.
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| Description |
English: The image shows orbital inclinations of irregular satellites of Saturn as a function of their semi-major axises. The negative inclinations correspond to retrograde moving satellites (180°–inclination). The bars parallel to the X-axis correspond to the range of their distances from Saturn. (from the periapse to apoapse) The diameters of gray circles are proportional to the moon's diameters. The names of satellites equal or larger than 15 km are shown. The three groups of irregular satellites (Inuit, Gallic and Norse) are also indicated. The information was taken from http://www.dtm.ciw.edu/users/sheppard/satellites/satsatdata.html website. |
| Date | |
| Source | Own work |
| Author | Ruslik0 |
.svg){kind=small} | This image was improved or created by the Wikigraphists of the Graphic Lab (it). You can propose images to clean up, improve, create or translate as well. |
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I, the copyright holder of this work, hereby publish it under the following licenses:
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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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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 12:12, 11 May 2013 | | 2,338 × 1,640 (29 KB) | Fulvio314 (talk | contribs) | Fix typo, "Imir" to "Ymir" & "degree" to "degrees" |
| 22:14, 7 August 2011 |  | 2,338 × 1,640 (56 KB) | JorisvS (talk | contribs) | typo fix: Iniut → Inuit | |
| 13:23, 29 April 2010 |  | 2,338 × 1,640 (39 KB) | Ruslik0 (talk | contribs) | {{Information |Description={{en|1=The image shows orbital inclinations of irregular satellites of Saturn as a function of their semi-major axises. The bars parallel to the X-axis correspond to the range of their distances from Saturn. (from the periapse t |
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