| Display title | Astronomy:V Crucis |
| Default sort key | V Crucis |
| Page length (in bytes) | 4,679 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 756195 |
| 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>LinXED |
| Date of page creation | 04:41, 27 June 2023 |
| Latest editor | imported>LinXED |
| Date of latest edit | 04:41, 27 June 2023 |
| 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 Crucis is a carbon star in the constellation Crux. A Mira variable, its apparent magnitude ranges from 8.7 to 11.1 over 376.5 days. The fact that this star's period is nearly equal to one year makes it hard to get good observational coverage over the entire cycle. Its near-infrared light curve... |
