| Display title | Astronomy:V Centauri |
| Default sort key | V Centauri |
| Page length (in bytes) | 6,912 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 573122 |
| 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 |
| Page image |  |
| HandWiki item ID | None |
| Edit | Allow all users (infinite) |
| Move | Allow all users (infinite) |
| Page creator | imported>WikiEditor |
| Date of page creation | 12:47, 8 February 2024 |
| Latest editor | imported>WikiEditor |
| Date of latest edit | 12:47, 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 Centauri (V Cen) is a Classical Cepheid variable, a type of variable star, in the constellation Centaurus. It is approximately 2,350 light-years (720 parsecs) away based on parallax.
V Centauri varies regularly between visual magnitudes 4.2 and 7.2 every 5.5 days. It is classified as a Cepheid variable... |
