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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{{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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