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English: Diagram of the geocentric epicyclic planetary model used in the w:en:Almagest to describe the longitudinal motion of Venus, Mars, Jupiter, and Saturn. The Earth is represented by ⊕, and the planet is represented by ☉. The direction A is fixed, and the lines labeled e, R, and r are fixed in length. The angles θ and φ increase at a constant rate with time. The direction M points towards the mean position of the planet.
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Source Own work
Author Spacepotato

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Public domain I, the copyright holder of this work, release this work into the public domain. This applies worldwide.
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28 January 2011

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00d4e5962f4ee23aad40203b5cbb85761e4a35c4

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540 pixel

620 pixel

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Date/TimeThumbnailDimensionsUserComment
current 07:36, 29 January 2011 Thumbnail for version as of 07:36, 29 January 2011620 × 540 (3 KB)AnonMoosadjusting margins, making circles more visible...
01:58, 29 January 2011 Thumbnail for version as of 01:58, 29 January 2011512 × 512 (4 KB)Spacepotato
01:44, 29 January 2011 Thumbnail for version as of 01:44, 29 January 2011512 × 512 (4 KB)SpacepotatoAdjust letter placement again
01:43, 29 January 2011 Thumbnail for version as of 01:43, 29 January 2011512 × 512 (4 KB)SpacepotatoAdjust letter placement
01:43, 29 January 2011 Thumbnail for version as of 01:43, 29 January 2011512 × 512 (4 KB)SpacepotatoAdjust letter placement
01:41, 29 January 2011 Thumbnail for version as of 01:41, 29 January 2011512 × 512 (4 KB)Spacepotato{{Information |Description ={{en|1=Diagram of geocentric planetary model used in the '' w:en:Almagest'' to describe the motion of Venus, Mars, Jupiter, and Saturn.}} |Source ={{own}} |Author = Spacepotato |Date
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