| Display title | Astronomy:Beta Cephei variable |
| Default sort key | Beta Cephei variable |
| Page length (in bytes) | 29,211 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 638385 |
| 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>Rtexter1 |
| Date of page creation | 09:44, 6 February 2024 |
| Latest editor | imported>Rtexter1 |
| Date of latest edit | 09:44, 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. | Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations of the stars' surfaces, thought due to the unusual properties of iron at temperatures of 200,000 K in their interiors. These stars are usually hot... |
