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Soubor:TheIrregulars JUPITER retro.png

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Obrázek + English: Retrograde irregular satellites of Jupiter. The most distant regular satellite Callisto is shown for reference.

  • Plotted by a program written by Eurocommuter.

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 of sateliites 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.
  • Date: 26 August 2006
  • Source: Plotted by a program written by the author
  • Author: User:Eurocommuter

+ pochází z Wikimedia Commons, kde má status – Creative Commons Attribution-Share Alike 3.0 Unported license.

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Datum a časNáhledRozměryUživatelKomentář
současná15. 7. 2015, 11:56Náhled verze z 15. 7. 2015, 11:561 000×1 000 (114 kB)Ivan Drago (diskuse | příspěvky) (Obrázek + English: Retrograde irregular satellites of Jupiter. The most distant regular satellite Callisto is shown for reference. * Plotted by a program written by Eurocommuter. == Main graph == * The position of a satellite (in polar co-ordinates) rep)

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