| Display title | Astronomy:W Ursae Majoris variable |
| Default sort key | W Ursae Majoris Variable |
| Page length (in bytes) | 8,885 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 607330 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
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| Counted as a content page | Yes |
| Page image |  |
| HandWiki item ID | None |
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| Page creator | imported>BotanyGa |
| Date of page creation | 21:02, 19 July 2022 |
| Latest editor | imported>BotanyGa |
| Date of latest edit | 21:02, 19 July 2022 |
| 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 W Ursae Majoris variable, also known as a low mass contact binary, is a type of eclipsing binary variable star. These stars are close binaries of spectral types F, G, or K that share a common envelope of material and are thus in contact with one another. They are termed contact binaries because the... |
