| Display title | Astronomy:V Coronae Borealis |
| Default sort key | V Coronae Borealis |
| Page length (in bytes) | 3,403 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 576141 |
| 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>Steve Marsio |
| Date of page creation | 11:20, 15 November 2021 |
| Latest editor | imported>Steve Marsio |
| Date of latest edit | 11:20, 15 November 2021 |
| 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 Coronae Borealis (V CrB) is a Mira-type long period variable star and carbon star in the constellation Corona Borealis. Its apparent magnitude varies between 6.9 and 12.6 over a period of 357 days
V Coronae Borealis is too far from Earth for its parallax to be measured effectively. Basing on a period... |
