| Display title | Astronomy:V Cephei |
| Default sort key | V Cephei |
| Page length (in bytes) | 6,006 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 574677 |
| 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>Raymond Straus |
| Date of page creation | 11:53, 8 February 2024 |
| Latest editor | imported>Raymond Straus |
| Date of latest edit | 11:53, 8 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. | V Cephei is a white main sequence star in the constellation Cepheus. It only varies slightly by 0.03 of a magnitude. It was suspected of being variable by American astronomer Seth Carlo Chandler noting in 1890 that it varied by 0.7 magnitude but that it needed more confirmation. Subsequent observers... |
