| Display title | Astronomy:Deferent and epicycle |
| Default sort key | Deferent and epicycle |
| Page length (in bytes) | 37,486 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 860636 |
| Page content language | en - English |
| Page content model | wikitext |
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| Page creator | Jworkorg (talk | contribs) |
| Date of page creation | 07:56, 6 February 2024 |
| Latest editor | Jworkorg (talk | contribs) |
| Date of latest edit | 07:56, 6 February 2024 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In the Hipparchian, Ptolemaic, and Copernican systems of astronomy, the epicycle (from grc ἐπίκυκλος (epíkuklos) 'upon the circle', meaning "circle moving on another circle") was a geometric model used to explain the variations in speed and direction of the apparent motion of the Moon, Sun, and... |
