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File:Saturnoppositions.jpg

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Original file (642 × 737 pixels, file size: 98 KB, MIME type: image/jpeg)

Summary

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
Source Originally from Saturnoppositions.png
Author The Saturn views were simulated with a computer program written by Tom Ruen (created here for public domain).
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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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Date/TimeThumbnailDimensionsUserComment
current08:10, 3 June 2005Thumbnail for version as of 08:10, 3 June 2005642 × 737 (98 KB)MosesofmasonThese 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 Saturn around the Sun. Credi
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