| Display title | Astronomy:Lambda Eridani variable |
| Default sort key | Lambda Eridani variable |
| Page length (in bytes) | 2,953 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375777 |
| 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>Rtextdoc |
| Date of page creation | 06:40, 2 August 2021 |
| Latest editor | imported>Rtextdoc |
| Date of latest edit | 06:40, 2 August 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. | A Lambda Eridani Variable is a class of Be stars that show small amplitude variations of a few hundredths of a magnitude. The variations are highly regular with periods between 0.5 and 2.0 days, and they were initially described as periodic Be stars. Lambda Eridani is an example and the prototype. |
