File:Saturnoppositions (2).jpg

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Description
English: This sequence of simulated views demonstrates the 29.5-year orbital period of Saturn by opposition date, as well as the dramatic changes in the orientation of the planet's ring disk. The ring system revolves around a fixed axis, so both sides of the ring disk are visible from Earth during each period in which Saturn orbits the Sun.

(Note: If viewed with a parallel view stereo technique, this set of images provides a pretty plastic 3D effect to the viewer.)

Reference
  • Meeus, Jean (1988) Astronomical Formulae for Calculators (4th ed.), Willmann-Bell
External sources
Date (UTC)
Source Saturnoppositions.jpg
Author
  • The Saturn views were simulated with a computer program written by Tom Ruen (created here for public domain).
  • Peer (talk) removed the title.
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This file was derived from: Saturnoppositions.jpg

Derivative works of this file:  Saturnoppositions-animated.gif
This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: Title removed. The original can be viewed here: Saturnoppositions.jpg. Modifications made by Peer.

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This image is a derivative work of the following images:

  • File:Saturnoppositions.jpg licensed with Cc-by-sa-3.0-migrated, GFDL
    • 2005-06-03T08:10:11Z Mosesofmason 642x737 (100304 Bytes) These views demonstrate the 29 year period for oppositions of Saturn and the dramatic changes in the appearance of the rings. Saturn's rings stay on a fixed axis, and we see the rings from both sides over one 29 year orbit of

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current17:56, 20 December 2010Thumbnail for version as of 17:56, 20 December 2010522 × 552 (99 KB)Peer (talk | contribs){{Information |Description=These views demonstrate the 29 year period for oppositions of Saturn and the dramatic changes in the appearance of the rings. Saturn's rings stay on a fixed axis, and we see the rings from both sides over one 29 year orbit of Sa

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