| Display title | Astronomy:Synodic day |
| Default sort key | Synodic Day |
| Page length (in bytes) | 6,699 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 839073 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
| Number of redirects to this page | 0 |
| Counted as a content page | Yes |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>TextAI2 |
| Date of page creation | 14:01, 6 February 2024 |
| Latest editor | imported>TextAI2 |
| Date of latest edit | 14:01, 6 February 2024 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
| Recent number of distinct authors | 0 |
Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | A synodic day (or synodic rotation period or solar day) is the period for a celestial object to rotate once in relation to the star it is orbiting, and is the basis of solar time.
The synodic day is distinguished from the sidereal day, which is one complete rotation in relation to distant stars and is... |
